I/355 Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022)
Gaia Data Release 3 (Gaia DR3) Part 1: Main source.
Gaia collaboration
<Astron. Astrophys., in prep. (2022)>
=2022yCat.1355....0G 2022yCat.1355....0G
=doi:10.1051/0004-6361/202243940
ADC_Keywords: Surveys ; Stars, standard ; Positional data ; Proper motions ;
Photometry, photographic ; Cross identifications ;
Radial velocities ; Stars, variable ; Minor planets;
Parallaxes, trigonometric
Mission_Name: Gaia
Keywords: catalogs - astrometry - parallaxes - proper motions -
techniques: photometric - techniques: radial velocities
Abstract:
Gaia Data Release 3 (Gaia DR3) will be released on 13 June 2022.
The Gaia DR3 catalogue builds upon the Early Data Release 3 (released
on 3 December 2020) and combines, for the same stretch of time and the
same set of observations, these already-published data products with
numerous new data products such as extended objects and non-single
stars.
Description:
The set of data released as Gaia Early Data Release 3 (Gaia EDR3) on 3
December 2020 comprises:
The full astrometric solution --- positions on the sky (α,
δ), parallaxes, and proper motions --- for around 1.46 billion
(1.46*109) sources, with a limiting magnitude of about G≃21 and a
bright limit of about G≃3. The astrometric solution is accompanied
with some new quality indicators, like RUWE, and source image
descriptors. The full astrometric solution has been done as
5-parameter solution for 585 million sources and as 6-parameter
solution for 882 million sources. In the 6-parameter solution, the
additional fitted quantity is the so-called pseudo-colour that had to
be included for sources without high-quality colour information. In
addition, two-parameters solutions --- positions on the sky (α,
δ) --- for around 344 million additional sources. G magnitudes
for around 1.806 billion sources (with the known issue present in EDR3
corrected in Gaia DR3). GBP and GRP magnitudes for around 1.54 billion
and 1.55 billion sources, respectively.
In Gaia Data Release 3 (Gaia DR3), the above set of data is
complemented with new products released on 13 June 2022 (EAS
presentation A. Vallenari):
Object classifications for 1.59 billion sources and astrophysical
parameters (Teff, logg, [M/H], AG, distance, etc.) from BP/RP spectra
for 470 million objects, including MCMC samples for most sources with
astrophysical parameters (EAS presentation O.Creevey). Other
astrophysical parameters from the BP/RP spectra include:
Spectral types (217 million stars) and emission-line star
classifications (57,000 stars);
Spectroscopic parameters for 2.3 million hot stars, 94,000 ultra-cool
stars, activity index for 1.3 million cool stars, and H-alpha emission
for 235 million stars;
Evolutionary parameters (mass and age) for 128 million stars;
Astrophysical parameters for 348 million objects based on the
assumption of an unresolved binary in the BP/RP spectra;
Self-organised map (outlier) analysis based on 56 million sources with
the weakest object classifications. Astrophysical parameters (Teff,
logg, [M/H], [X/M] for 12 elements, etc.) from RVS spectra for 5.5
million objects, including diffuse interstellar bands for 472,000
objects.
All-sky total galactic extinction maps at 4 different spatial
resolutions (HEALPix levels 6, 7, 8, and 9).
Mean BP/RP spectra for 219 million sources, most of them with G < 17.6
mag (EAS Presentation F. De Angeli).
Mean RVS spectra for 1 million well-behaved objects (EAS presentation
P. Sartoretti).
Mean radial velocities for 33 million stars and mean GRVS magnitudes
for 32 million objects with GRVS≲14mag with effective temperatures
(Teff) in the range of ∼3100 to 14500K (EAS presentation P.
Sartoretti).
Rotational velocities for 3.5 million sources with GRVS≲12mag.
Variability analysis, together with the underlying epoch photometry,
for 10.5 million sources. Apart from classification into 24
variability classes, detailed variability results are provided in
separate tables for the following candidates (EAS presentation L.
Eyer):
Cepheids (15,021 objects);
Compact companions (6306 objects);
Eclipsing binaries (2,184,477 objects);
Long-period variables (1,720,588 objects);
Microlensing events (363 objects);
Planetary transits (214 objects);
RR Lyrae stars (271,779 objects);
Short-timescale variables (471,679 objects);
Solar-like rotational modulation variables (474,026 objects);
Upper-main-sequence oscillators (54,476 objects);
Active galactic nuclei (872,228 objects).
Solar-system results for 158,000 sources (including 31 planetary
satellites), with orbital solutions and individual epoch observations
for 154,000 objects and with mean BP/RP reflectance spectra for more
than 60,000 objects (EAS presentation P. Tanga). Some 813,000
non-single stars, including amongst others non-single-star models for
sources compatible with an astrometric acceleration solution,
non-single-star orbital models for spectroscopic binaries compatible
with a trend, and non-single-star orbital models for sources
compatible with a two-body solution (EAS presentation F. Arenou).
Some 6.6 million quasar candidates with redshift estimates for most of
them (EAS presentation L. Galluccio).
Some 1.1 million quasars analysed with 60,000 host galaxies detected
and 15,000 surface brightness profiles of the host galaxy.
Some 4.8 million galaxy candidates with redshift estimates for more
than 1 million objects (EAS presentation L. Galluccio).
Some 900,000 galaxies analysed with two surface brightness profiles.
The Gaia Andromeda Photometric Survey (GAPS), consisting of the
photometric time series for all 1.2 million sources located in a
5.5-degree radius field centred on the Andromeda galaxy.
Selected tables from Gaia Collaboration performance verification
papers published with Gaia DR3.
All 2612 science alerts triggered in the period underlying Gaia DR3.
The new data set neither contains new astrometry nor new photometric
calibrations such that the following elements are in common for and
apply to both Gaia EDR3 and Gaia DR3:
About 1.61 million celestial reference frame (Gaia-CRF3) sources.
Cross-matches between Gaia (E)DR3 sources on the one hand and
Hipparcos-2, Tycho-2 + TDSC merged, 2MASS PSC (merged with 2MASS XSC),
SDSS DR13, Pan-STARRS1 DR1, SkyMapper DR2, GSC 2.3, APASS DR9, RAVE
DR5, allWISE, URAT-1, and RAVE DR6 data on the other hand.
Additionally, a Gaia DR2 to Gaia (E)DR3 match table.
Full photometric passband definitions for G, GBP, GRP, and GRVS. More
information is available here. Please be aware that the photometric
system for the G, GBP, and GRP bands in Gaia (E)DR3 is different from
the photometric systems as used in Gaia DR2 and in Gaia DR1.
Simulated data from the Gaia Object Generator (GOG) and the Gaia
Universe Model Snapshot (GUMS).
The commanded scan law covering the Gaia (E)DR3 data collection
period. Also the major periods where data was not sent to the ground
or could not be processed are identified.
All of the above combined makes up the full Gaia Data Release 3.
File Summary:
--------------------------------------------------------------------------------
FileName Lrecl Records Explanations
--------------------------------------------------------------------------------
ReadMe 80 . This file
gaiadr3.sam 1781 1000 Gaia DR3 source catalog (1811709771 sources)
paramp.sam 1757 1000 1D astrophysical parameters produced by the
Apsis processing chain developed in Gaia DPAC
CU8 (1590932717 sources)
(astrophysical_parameters)
paramsup.sam 1549 1000 Additional parameters from the Apsis processing
chain, compared to the main table astrophysical
parameters, from modules that produce more than
one result for a parameter (473020612 sources)
(astrophysicalparameterssupp)
tgextmap.dat 70 4177920 Total Galactic Extinction (TGE) map for
extinction parameters A0
tgextopt.dat 49 3145728 Optimum version of the Total Galactic Extinction
Map, derived from the table tgextmap.dat
(totalgalacticextinction_map) at a
single HELPix level 9
oaninfo.dat 925 900 Content of a Self-Organized Map calculated from
a dataset composed by outliers by the Apsis
module OA (oaneuroninformation)
oaxpsp.dat 81 78300 Prototype BP/RP spectrum corresponding to each
of the neurons of the Self-Organised-Map
produced by the Apsis module OA
(oaneuronxp_spectra)
epphot.sam 325 1000 Light curves for a given object in bands
G, BP and RP (555868797 rows)
(epoch_photometry)
gcrf3xm.dat 364 1614173 Full cross-match information for the
Gaia-CRF3 sources (GaiaCrf3Xm)
rvsmean.sam 92 1000 RVS mean sampled spectrum table
(2400147645 lines) (rvsmeanspectrum)
xpsummary.sam 186 1000 Auxiliary information about the mean BP/RP
spectrum (219197643 sources) (xp_summary)
xpsample.sam 87 1000 BP/RP externally calibrated sampled mean
spectrum (11822651939 rows)
(xpsampledmean_spectrum)
xpsamp.dat 56 37730 Definition of XP spectra standard sampling
schemes (xp_sampling)
xpmerge.dat 38 343 Coefficients used to merge the BP and RP
externally calibrated sampled spectra into
the final merged product (xp_merge)
xpcont.sam 253 1000 Mean BP and RP spectra based on the continuous
representation in basis functions
(219197643 rows) (gaiadr3xpcont)
spectra.sam 51 2000 Gaia DR3 spectra view (34468373 sources)
--------------------------------------------------------------------------------
See also:
I/355 : Gaia DR3 Part 1: Main sources
I/356 : Gaia DR3 Part 2: Extra-galactic
I/357 : Gaia DR3 Part 3: Non-single stars
I/358 : Gaia DR3 Part 4: Variability
I/359 : Gaia DR3 Part 5: Solar System
I/360 : Gaia DR3 Part 6: Performance verification
Byte-by-byte Description of file: gaiadr3.sam
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 28 A28 --- DR3Name Unique source designation (unique
across all Data Releases)
(designation)
30- 44 F15.11 deg RAdeg Right ascension (ICRS) at Ep=2016.0
(ra)
46- 60 F15.11 deg DEdeg Declination (ICRS) at Ep=2016.0 (dec)
62- 80 I19 --- SolID Solution Identifier (solution_id)
82- 100 I19 --- Source Unique source identifier (unique
within a particular Data Release)
(source_id)
102- 111 I10 --- RandomI Random index for use when selecting
subsets (random_index)
113- 119 F7.4 mas e_RAdeg Standard error of right ascension
(ra_error)
121- 127 F7.4 mas e_DEdeg Standard error of declination
(dec_error)
129- 137 F9.4 mas Plx ? Parallax (parallax)
139- 144 F6.4 mas e_Plx ? Standard error of parallax
(parallax_error)
146- 155 F10.4 --- RPlx ? Parallax divided by its standard
error (parallaxovererror)
157- 165 F9.3 mas/yr PM ? Total proper motion (pm)
167- 175 F9.3 mas/yr pmRA ? Proper motion in right ascension
direction, pmRA*cosDE (pmra)
177- 181 F5.3 mas/yr e_pmRA ? Standard error of proper motion in
right ascension direction
(pmra_error)
183- 191 F9.3 mas/yr pmDE ? Proper motion in declination
direction (pmdec)
193- 197 F5.3 mas/yr e_pmDE ? Standard error of proper motion in
declination direction (pmdec_error)
199- 205 F7.4 --- RADEcor [-1/1] Correlation between right
ascension and declination
(radeccorr)
207- 213 F7.4 --- RAPlxcor [-1/1]? Correlation between right
ascension and parallax
(raparallaxcorr)
215- 221 F7.4 --- RApmRAcor [-1/1]? Correlation between right
ascension and proper motion in right
ascension (rapmracorr)
223- 229 F7.4 --- RApmDEcor [-1/1]? Correlation between right
ascension and proper motion in
declination (rapmdeccorr)
231- 237 F7.4 --- DEPlxcor [-1/1]? Correlation between
declination and parallax
(decparallaxcorr)
239- 245 F7.4 --- DEpmRAcor [-1/1]? Correlation between
declination and proper motion in
right ascension (decpmracorr)
247- 253 F7.4 --- DEpmDEcor [-1/1]? Correlation between
declination and proper motion in
declination (decpmdeccorr)
255- 261 F7.4 --- PlxpmRAcor [-1/1]? Correlation between parallax
and proper motion in right ascension
(parallaxpmracorr)
263- 269 F7.4 --- PlxpmDEcor [-1/1]? Correlation between parallax
and proper motion in declination
(parallaxpmdeccorr)
271- 277 F7.4 --- pmRApmDEcor [-1/1]? Correlation between proper
motion in right ascension and proper
motion in declination
(pmrapmdeccorr)
279- 282 I4 --- NAL Total number of observations in the
along-scan (AL) direction
(astrometricnobs_al)
284- 287 I4 --- NAC Total number of observations in the
across-scan (AC) direction
(astrometricnobs_ac)
289- 292 I4 --- NgAL Number of good observations in the
along-scan (AL) direction
(astrometricngoodobsal)
294- 296 I3 --- NbAL Number of bad observations in the
along-scan (AL) direction
(astrometricnbadobsal)
298- 307 F10.4 --- gofAL Goodness of fit statistic of model
wrt along-scan observations
(astrometricgofal)
309- 318 E10.4 --- chi2AL AL chi-square value
(astrometricchi2al)
320- 327 F8.3 mas epsi Excess noise of the source
(astrometricexcessnoise)
329- 338 E10.4 --- sepsi Significance of excess noise
(astrometricexcessnoise_sig)
340- 341 I2 --- Solved [3/95] Which parameters have been
solved for?
(astrometricparamssolved) (1)
343 I1 --- APF [0/1] Primary or secondary
(astrometricprimaryflag)
345- 350 F6.3 um-1 nueff ? Effective wavenumber of the source
used in the astrometric solution
(nueffusedinastrometry)
352- 358 F7.4 um-1 pscol ? Astrometrically estimated
pseudocolour of the source
(pseudocolour)
360- 365 F6.4 um-1 e_pscol ? Standard error of the pseudocolour
of the source (pseudocolour_error)
367- 372 F6.3 --- RApscolCorr [-1/1]? Correlation between right
ascension and pseudocolour
(rapseudocolourcorr)
374- 379 F6.3 --- DEpscolCorr [-1/1]? Correlation between
declination and pseudocolour
(decpseudocolourcorr)
381- 386 F6.3 --- PlxpscolCorr [-1/1]? Correlation between parallax
and pseudocolour
(parallaxpseudocolourcorr)
388- 393 F6.3 --- pmRApscolCorr [-1/1]? Correlation between proper
motion in right ascension and
pseudocolour (pmrapseudocolourcorr)
395- 400 F6.3 --- pmDEpscolCorr [-1/1]? Correlation between proper
motion in declination and
pseudocolour
(pmdecpseudocolourcorr)
402- 404 I3 --- MatchObsA Matched FOV transits used in the AGIS
solution
(astrometricmatchedtransits)
406- 407 I2 --- Nper [1/33] Number of visibility periods
used in Astrometric solution
(visibilityperiodsused)
409- 426 F18.6 mas amax The longest semi-major axis of the
-2- -7 error ellipsoid
(astrometricsigma5dmax)
428- 430 I3 --- MatchObs The number of transits matched to this
source (matched_transits)
432- 434 I3 --- NewMatchObs The number of transits newly
incorporated into an existing source
in the current cycle
(newmatchedtransits)
436- 438 I3 --- MatchObsrm The number of transits removed from
an existing source in the current
cycle (matchedtransitsremoved)
440- 448 E9.3 --- IPDgofha Amplitude of the IPD GoF versus
position angle of scan
(ipdgofharmonic_amplitude)
450- 458 E9.3 deg IPDgofhp Phase of the IPD GoF versus position
angle of scan
(ipdgofharmonic_phase)
460- 462 I3 --- IPDfmp [0/100] Percent of successful-IPD
windows with more than one peak
(ipdfracmulti_peak)
464- 466 I3 --- IPDfow [0/100] Percent of transits with
truncated windows or multiple gate
(ipdfracodd_win)
468- 474 F7.3 --- RUWE ? Renormalised unit weight error
(ruwe)
476- 484 E9.3 --- SDSk1 ? Degree of concentration of scan
directions across the source
(scandirectionstrength_k1)
486- 494 E9.3 --- SDSk2 ? Degree of concentration of scan
directions across the source
(scandirectionstrength_k2)
496- 504 E9.3 --- SDSk3 ? Degree of concentration of scan
directions across the source
(scandirectionstrength_k3)
506- 514 E9.3 --- SDSk4 ? Degree of concentration of scan
directions across the source
(scandirectionstrength_k4)
516- 523 F8.3 --- SDMk1 ? Mean position angle of scan
directions across the source
(scandirectionmean_k1)
525- 531 F7.3 --- SDMk2 ? Mean position angle of scan
directions across the source
(scandirectionmean_k2)
533- 539 F7.3 --- SDMk3 ? Mean position angle of scan
directions across the source
(scandirectionmean_k3)
541- 547 F7.3 deg SDMk4 ? Mean position angle of scan
directions across the source
(scandirectionmean_k4)
549 I1 --- Dup [0/1] Source with multiple source
identifiers (duplicated_source)
551- 554 I4 --- o_Gmag Number of observations contributing to
G photometry (photgn_obs)
556- 571 F16.5 e-/s FG ? G-band mean flux (photgmean_flux)
573- 583 E11.5 e-/s e_FG ? Error on G-band mean flux
(photgmeanfluxerror)
585- 595 E11.5 --- RFG ? G-band mean flux divided by its
error (photgmeanfluxover_error)
597- 605 F9.6 mag Gmag ? G-band mean magnitude
(photgmean_mag)
607- 614 F8.6 mag e_Gmag ? Error on G-band mean magnitude
(added by CDS)
(photgmeanmagerror)
616- 618 I3 --- o_BPmag Number of observations contributing to
BP photometry (photbpn_obs)
620- 630 E11.5 e-/s FBP ? Integrated BP mean flux
(photbpmean_flux)
632- 642 E11.5 e-/s e_FBP ? Error on the integrated BP mean flux
(photbpmeanfluxerror)
644- 654 E11.5 --- RFBP ? Integrated BP mean flux divided by
its error
(photbpmeanfluxover_error)
656- 664 F9.6 mag BPmag ? Integrated BP mean magnitude
(photbpmean_mag)
666- 674 F9.6 mag e_BPmag ? Error on integrated BP mean
magnitude (added by CDS)
(photbpmeanmagerror)
676- 678 I3 --- o_RPmag Number of observations contributing to
RP photometry (photrpn_obs)
680- 690 E11.5 e-/s FRP ? Integrated RP mean flux
(photrpmean_flux)
692- 702 E11.5 e-/s e_FRP ? Error on the integrated RP mean flux
(photrpmeanfluxerror)
704- 714 E11.5 --- RFRP ? Integrated RP mean flux divided by
its error
(photrpmeanfluxover_error)
716- 724 F9.6 mag RPmag ? Integrated RP mean magnitude
(photrpmean_mag)
726- 734 F9.6 mag e_RPmag ? Error on integrated RP mean
magnitude (added by CDS)
(photrpmeanmagerror)
736- 744 F9.3 mag E(BP/RP) ? BP/RP excess factor
(photbprpexcessfactor)
746- 748 I3 --- NBPcont ? Number of BP contaminated transits
(photbpncontaminatedtransits)
750- 752 I3 --- NBPblend ? Number of BP blended transits
(photbpnblendedtransits)
754- 756 I3 --- NRPcont ? Number of RP contaminated transits
(photrpncontaminatedtransits)
758- 760 I3 --- NRPblend ? Number of RP contaminated transits
(photrpnblendedtransits)
762 I1 --- Mode [0/2]? Photometry processing mode
(photprocmode)
764- 772 F9.6 mag BP-RP ? BP-RP colour (bp_rp)
774- 782 F9.6 mag BP-G ? BP-G colour (bp_g)
784- 792 F9.6 mag G-RP ? G-RP colour (g_rp)
794- 800 F7.2 km/s RV ? Radial velocity (radial_velocity)
802- 806 F5.2 km/s e_RV ? Radial velocity error
(radialvelocityerror)
808 I1 --- n_RV [0/2]? Method used to obtain the
radial velocity (rvmethodused)
810- 812 I3 --- o_RV ? Number of transits used to compute
the radial velocity (rvnbtransits)
814- 816 I3 --- o_RVd ? Number of valid transits that have
undergone deblending
(rvnbdeblended_transits)
818- 819 I2 --- RVNper [0/33]? Number of visibility periods
used to estimate the radial velocity
(rvvisibilityperiods_used)
821- 830 E10.4 --- RVS/N ? Expected signal to noise ratio in
the combination of the spectra used
to obtain the radial velocity
(rvexpectedsigtonoise)
832- 842 E11.4 --- RVgof ? Radial velocity renormalised
goodness of fit (rvrenormalisedgof)
844- 851 F8.6 --- RVchi2 ? P-value for constancy based on a
chi-squared criterion
(rvchisqpvalue)
853- 860 F8.3 d RVTdur ? Time coverage of the radial velocity
time series (rvtimeduration)
862- 868 F7.2 km/s RVamp ? Total amplitude in the radial
velocity time series after outlier
removal (rvamplituderobust)
870- 876 F7.1 K RVtempTeff ? Teff of the template used to compute
the radial velocity
(rvtemplateteff)
878- 881 F4.1 [cm/s2] RVtemplogg ? Logg of the template used to compute
the radial velocity
(rvtemplatelogg)
883- 887 F5.2 [-] RVtemp[Fe/H] ? [Fe/H] of the template used to
compute the radial velocity
(rvtemplatefe_h)
889- 891 I3 --- Vatmparam ? Origin of the atmospheric parameters
associated to the template
(rvatmparam_origin)
893- 900 F8.4 km/s Vbroad ? Spectral line broadening parameter
(vbroad)
902- 909 F8.4 km/s e_Vbroad ? Uncertainty on the spectral line
broadening (vbroad_error)
911- 912 I2 --- o_Vbroad ? Number of transits used to compute
vbroad (vbroadnbtransits)
914- 922 F9.6 mag GRVSmag ? Integrated Grvs magnitude (grvs_mag)
924- 931 F8.6 mag e_GRVSmag ? Grvs magnitude uncertainty
(grvsmagerror)
933- 935 I3 --- o_GRVSmag ? Number of transits used to compute
Grvs (grvsmagnb_transits)
937- 948 E12.6 --- RVSS/N ? Signal to noise ratio in the mean
RVS spectrum (rvsspecsigtonoise)
950- 962 A13 --- VarFlag Photometric variability flag
(photvariableflag)
964- 978 F15.11 deg GLON Galactic longitude (l)
980- 994 F15.11 deg GLAT Galactic latitude (b)
996-1010 F15.11 deg ELON Ecliptic longitude (ecl_lon)
1012-1026 F15.11 deg ELAT Ecliptic latitude (ecl_lat)
1028 I1 --- QSO [0/1] Flag indicating the availability
of additional information in the QSO
candidates table (inqsocandidates)
1030 I1 --- Gal [0/1] Flag indicating the availability
of additional information in the
galaxy candidates table
(ingalaxycandidates)
1032 I1 --- NSS [0/7] Flag indicating the availability
of additional information in the
various Non-Single Star tables
(nonsinglestar)
1034 I1 --- XPcont [0/1] Flag indicating the availability
of mean BP/RP spectrum in continuous
representation for this source
(hasxpcontinuous)
1036 I1 --- XPsamp [0/1] Flag indicating the availability
of mean BP/RP spectrum in sampled
form for this source (hasxpsampled)
1038 I1 --- RVS [0/1] Flag indicating the availability
of mean RVS spectrum for this source
(has_rvs)
1040 I1 --- EpochPh [0/1] Flag indicating the availability
of epoch photometry for this source
(hasepochphotometry)
1042 I1 --- EpochRV [0/1] Flag indicating the availability
of epoch radial velocity for this
source (hasepochrv)
1044 I1 --- MCMCGSP [0/1] Flag indicating the availability
of GSP-Phot MCMC samples for this
source (hasmcmcgspphot)
1046 I1 --- MCMCMSC [0/1] Flag indicating the availability
of MSC MCMC samples for this source
(hasmcmcmsc)
1048 I1 --- And [0/1] Flag indicating that the source
is present in the Gaia Andromeda
Photometric Survey (GAPS)
(inandromedasurvey)
1050-1057 F8.6 --- PQSO ? Probability from DSC-Combmod of
being a quasar
(data used: BP/RP spectrum)
(classprobdsccombmod_quasar)
1059-1066 F8.6 --- PGal ? Probability from DSC-Combmod of
being a galaxy
(data used: BP/RP spectrum)
(classprobdsccombmod_galaxy)
1068-1075 F8.6 --- PSS ? Probability from DSC-Combmod of
being a single star (but not a
white dwarf)
(data used: BP/RP spectrum)
(classprobdsccombmod_star)
1077-1083 F7.1 K Teff ? Effective temperature from GSP-Phot
Aeneas best library using BP/RP
spectra (teff_gspphot)
1085-1091 F7.1 K b_Teff ? Lower confidence level (16%) of
effective temperature from GSP-Phot
Aeneas best library using BP/RP
spectra (teffgspphotlower)
1093-1099 F7.1 K B_Teff ? Upper confidence level (84%) of
effective temperature from GSP-Phot
Aeneas best library using BP/RP
spectra (teffgspphotupper)
1101-1107 F7.4 [cm/s2] logg ? Surface gravity from GSP-Phot Aeneas
best library using BP/RP spectra
(logg_gspphot)
1109-1115 F7.4 [cm/s2] b_logg ? Lower confidence level (16%) of
surface gravity from GSP-Phot
Aeneas best library using BP/RP
spectra (logggspphotlower)
1117-1123 F7.4 [cm/s2] B_logg ? Upper confidence level (84%) of
surface gravity from GSP-Phot Aeneas
best library using BP/RP spectra
(logggspphotupper)
1125-1131 F7.4 [-] [Fe/H] ? Iron abundance from GSP-Phot Aeneas
best library using BP/RP spectra
(mh_gspphot)
1133-1139 F7.4 [-] b_[Fe/H] ? Lower confidence level (16%) of iron
abundance from GSP-Phot Aeneas best
library using BP/RP spectra
(mhgspphotlower)
1141-1147 F7.4 [-] B_[Fe/H] ? Upper confidence level (84%) of iron
abundance from GSP-Phot Aeneas best
library using BP/RP spectra
(mhgspphotupper)
1149-1158 F10.4 pc Dist ? Distance from GSP-Phot Aeneas best
library using BP/RP spectra
(distance_gspphot)
1160-1169 F10.4 pc b_Dist ? Lower confidence level (16%) of
distance from GSP-Phot Aeneas best
library using BP/RP spectra
(distancegspphotlower)
1171-1180 F10.4 pc B_Dist ? Upper confidence level (84%) of
distance from GSP-Phot Aeneas best
library using BP/RP spectra
(distancegspphotupper)
1182-1188 F7.4 mag A0 ? Monochromatic extinction A_0 at
547.7nm from GSP-Phot Aeneas best
library using BP/RP spectra
(azero_gspphot)
1190-1195 F6.4 mag b_A0 ? Lower confidence level (16%) of
monochromatic extinction A_0 at
547.7nm from GSP-Phot Aeneas best
library using BP/RP spectra
(azerogspphotlower)
1197-1203 F7.4 mag B_A0 ? Upper confidence level (84%) of
monochromatic extinction A_0 at
547.7nm from GSP-Phot Aeneas best
library using BP/RP spectra
(azerogspphotupper)
1205-1210 F6.4 mag AG ? Extinction in G band from GSP-Phot
Aeneas best library using BP/RP
spectra (ag_gspphot)
1212-1217 F6.4 mag b_AG ? Lower confidence level (16%) of
extinction in G band from GSP-Phot
Aeneas best library using BP/RP
spectra (aggspphotlower)
1219-1224 F6.4 mag B_AG ? Upper confidence level (84%) of
extinction in G band from GSP-Phot
Aeneas best library using BP/RP
spectra (aggspphotupper)
1226-1231 F6.4 mag E(BP-RP) ? Reddening E(GBP-GRP) from
GSP-Phot Aeneas best library using
BP/RP spectra (ebpminrp_gspphot)
1233-1238 F6.4 mag b_E(BP-RP) ? Lower confidence level (16%) of
reddening E(GBP-GRP) from
GSP-Phot Aeneas best library using
BP/RP spectra
(ebpminrpgspphotlower)
1240-1245 F6.4 mag B_E(BP-RP) ? Upper confidence level (84%) of
reddening E(GBP-GRP) from
GSP-Phot Aeneas best library using
BP/RP spectra
(ebpminrpgspphotupper)
1247-1253 A7 --- Lib Name of library that achieves the
highest mean log-posterior in MCMC
samples and was used to derive
GSP-Phot parameters in this table
(libname_gspphot)
1255-1260 I6 --- HIP ? HIP cross-id number,
van Leeuwen, Cat. I/311
(hiporiginalextsourceid)
1262-1269 F8.6 arcsec dHIP ? Angular distance between the two
sources (hipangulardistance)
1271 I1 --- nHIP [0/3]? Number of neighbours in HIP
(hipnumberof_neighbours)
1273-1274 I2 --- f_HIP [0/72]? Cross-match algorithm flag
(hipxmflag)
1276-1285 I10 --- PS1coid ? PS1 cross-id original name
(cleanpanstarrs1oid)
1287-1304 I18 --- PS1 ? PS1 cross-id name,
Chambers et al., Cat. II/349
(ps1originalextsourceid)
1306-1313 F8.6 arcsec dPS1 ? Angular Distance between the two
sources (ps1angulardistance)
1315 I1 --- nPS1 [0/76]? Number of neighbours in PS1
(ps1numberof_neighbours)
1317-1318 I2 --- mPS1 ? Number of mates in Gaia Catalog
(ps1numberof_mates)
1320-1321 I2 --- f_PS1 [0/76]? Cross-match algorithm flag
(ps1xmflag)
1323-1331 I9 --- SDSS13coid ? SDSS cross-id original name
(cleansdssdr13oid)
1333-1351 I19 --- SDSS13 ? SDSS name,
Albareti et al., 2017ApJS..233...25A 2017ApJS..233...25A
(sdss13extsource_id)
1353-1360 F8.6 arcsec dSDSS13 ? Angular Distance between the two
sources (sdss13angulardistance)
1362 I1 --- nSDSS13 [0/6]? Number of neighbours in SDSS13
(sdss13numberof_neighbours)
1364 I1 --- mSDSS13 [0/6]? Number of mates in Gaia Catalog
(sdss13numberof_mates)
1366-1367 I2 --- f_SDSS13 [0/76]? Cross-match algorithm flag
(sdss13xmflag)
1369-1377 I9 --- SKYM2 ? SkyMapperDR2 cross-id name,
Onken et al., 2019PASA...36...33O 2019PASA...36...33O
(skym2originalextsourceid)
1379-1386 F8.6 arcsec dSKYM2 ? Angular Distance between the two
sources (skym2angulardistance)
1388 I1 --- nSKYM2 [0/4]? Number of neighbours in SKYM2
(skym2numberof_neighbours)
1390-1391 I2 --- mSKYM2 ? Number of mates in Gaia Catalog
(skym2numberof_mates)
1393-1394 I2 --- f_SKYM2 [0/72]? Cross-match algorithm flag
(skym2xmflag)
1396-1407 A12 --- TYC2 Tycho-2 cross-id name,
Hog et al., Cat. I/259
(tyc2originalextsourceid)
1409-1416 F8.6 arcsec dTYC2 ? Angular Distance between the two
source (tyc2angulardistance)
1418-1419 I2 --- f_TYC2 [0/72]? Cross-match algorithm flag
(tyc2xmflag)
1421-1427 I7 --- TYC2moid ? Tycho-2 cross-id original name
(tycho2tdscmergeoid)
1429 I1 --- nTYC2 [0/4]? Number of neighbours in TYC2
(tyc2numberof_neighbours)
1431-1445 A15 --- URAT1 URAT1 name,
Zacharias et al., Cat. I/329
(urat1originalextsourceid)
1447-1454 F8.6 arcsec dURAT1 ? Angular Distance between the two
sources (urat1angulardistance)
1456-1457 I2 --- f_URAT1 [0/72]? Cross-match algorithm flag
(urat1xmflag)
1459-1467 I9 --- URAT1oid ? URAT1 cross-id original name
(urat1_oid)
1469 I1 --- nURAT1 [0/4]? Number of neighbours in URAT1
(urat1numberof_neighbours)
1471 I1 --- mURAT1 [0/4]? Number of mates in Gaia Catalog
(urat1numberof_mates)
1473-1491 A19 --- AllWISE ALLWISE cross-id name,
Cutri et al., Cat. II/328
(allwiseoriginalextsourceid)
1493-1501 F9.6 arcsec dAllWISE ? Angular Distance between the two
sources (allwiseangulardistance)
1503-1504 I2 --- f_AllWISE [0/72]? Cross-match algorithm flag
(allwisexmflag)
1506-1514 I9 --- AllWISEoid ? ALLWISE identification number
(allwise_oid)
1516 I1 --- nAllWISE [0/3]? Number of neighbours in ALLWISE
catalog
(allwisenumberof_neighbours)
1518-1519 I2 --- mAllWISE ? Number of mates in Gaia Catalog
(allwisenumberof_mates)
1521-1528 I8 --- APASS9coid ? APASS9 cross-id original
identification number
(cleanapassdr9oid)
1530-1537 I8 --- APASS9 ? APASS9 identification,
Henden et al., Cat. II/336
(apass9originalextsourceid)
1539-1547 F9.6 arcsec dAPASS9 ? Angular Distance between the two
sources (apass9angulardistance)
1549-1550 I2 --- nAPASS9 ? Number of neighbours in APASS9
(apass9numberof_neighbours)
1552-1553 I2 --- mAPASS9 ? Number of mates in Gaia Catalog
(apass9numberof_mates)
1555-1556 I2 --- f_APASS9 [0/74]? Cross-match algorithm flag
(apass9xmflag)
1558-1567 A10 --- GSC23 GSC2.3 cross-id name,
Lasker et al., Cat. I/305
(gsc23originalextsourceid)
1569-1576 F8.6 arcsec dGSC23 ? Angular Distance between the two
sources (gsc23angulardistance)
1578-1579 I2 --- f_GSC23 ? Cross-match algorithm flag
(gsc23xmflag)
1581-1589 I9 --- GSC23coid ? GSC2.3 cross-id original name
(cleangsc23oid)
1591-1592 I2 --- nGSC23 [0/16]? Number of neighbours in GSC23
(gsc23numberof_neighbours)
1594-1595 I2 --- mGSC23 ? Number of mates in Gaia Catalog
(gsc23numberof_mates)
1597-1612 A16 --- RAVE5 RAVE DR5 cross-id name,
Kunder et al., Cat. III/279
(rave5originalextsourceid)
1614-1621 F8.6 arcsec dRAVE5 ? Angular Distance between the two
sources (rave5angulardistance)
1623-1624 I2 --- f_RAVE5 [0/72]? Cross-match algorithm flag
(rave5xmflag)
1626-1631 I6 --- RAVE5coid ? RAVE DR5 cross-id original name
(cleanravedr5oid)
1633 I1 --- nRAVE5 [0/3]? Number of neighbours in RAVE5
(rave5numberof_neighbours)
1635-1651 A17 --- 2MASS 2MASS cross-id name,
Cutri et al., Cat. II/246
(twomassoriginalextsourceid)
1653-1660 F8.6 arcsec d2MASS ? Angular Distance between the two
sources (twomassangulardistance)
1662-1663 I2 --- f_2MASS [0/73]? Cross-match algorithm flag
(twomassxmflag)
1665-1673 I9 --- 2MASScoid ? 2MASS cross-id original name
(cleantmasspscxscoid)
1675 I1 --- n2MASS [0/4]? Number of neighbours in 2MASS
(twomassnumberof_neighbours)
1677-1678 I2 --- m2MASS [0/13]? Number of mates in Gaia
Catalog (twomassnumberof_mates)
1680-1700 A21 --- RAVE6 RAVE DR6 cross-id name,
Steinmetz et al., Cat. III/283
(rave6originalextsourceid)
1702-1709 F8.6 arcsec dRAVE6 ? Angular Distance between the two
sources (rave6angulardistance)
1711-1712 I2 --- f_RAVE6 [0/72]? Cross-match algorithm flag
(rave6xmflag)
1714-1719 I6 --- RAVE6oid ? RAVE DR6 original name
(ravedr6_oid)
1721 I1 --- nRAVE6 [0/3]? Number of neighbours in RAVE6
(rave6numberof_neighbours)
1723-1737 F15.11 deg RAJ2000 Barycentric right ascension (ICRS) at
Ep=2000.0 (added by CDS) (ra2000)
1739-1753 F15.11 deg DEJ2000 Barycentric declination (ICRS) at
Ep=2000.0 (added by CDS) (dec2000)
1755-1763 F9.6 mas e_RAJ2000 Standard error of right ascension
(e_RA*cosDE) (added by CDS)
(ra2000_error)
1765-1773 F9.6 mas e_DEJ2000 Standard error of declination
(added by CDS) (dec2000_error)
1775-1781 F7.4 --- RADEcorJ2000 [-1/1] Correlation between right
ascension and declination at epoch
2000 (added by CDS)
(ra2000de2000corr)
--------------------------------------------------------------------------------
Note (1): The seven bits of astrometricparamssolved indicate which parameters
have been estimated in AGIS for this source. A set bit means the parameter
was updated, an unset bit means the parameter was not updated. The
leastsignificant bit corresponds to ra. The table below shows the values of
astrometric params solved for relevant combinations of the parameters.
The radial proper motion (µr) is formally considered to be one of the
astrometric parameters of a source, and the sixth bit is therefore reserved
for it. It is also in principle updatable in AGIS, but in practice it will
always be computed from a spectroscopic radial velocity and the estimated
parallax, in which case the bit is not set.
C is the pseudocolour of the source, i.e. the astrometrically estimated
effective wavenumber.
astrometricparamssolved | ra | dec | parallax | pmra | pmdec | µr | C
00000112 = 3 | X | X | | | | |
00001112 = 7 | X | X | X | | | |
00110112 = 27 | X | X | | X | X | |
00111112 = 31 | X | X | X | X | X | |
01111112 = 63 | X | X | X | X | X | X |
10111112 = 95 | X | X | X | X | X | | X
In practice all the sources in DR3 have only values of 3, 31 or 95 for the
astrometric params solved, corresponding to two-parameter (position),
five-parameter (position, parallax, and proper motion) and
six-parameter (position, parallax, proper motion and astrometrically
estimated effective wavenumber) solutions.
--------------------------------------------------------------------------------
Byte-by-byte Description of file: paramp.sam
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 19 I19 --- Source Source Identifier (source_id)
21- 35 F15.11 deg RAdeg Right ascension (ICRS) at Ep=2016.0
(ra)
37- 51 F15.11 deg DEdeg Declination (ICRS) at Ep=2016.0 (dec)
53- 62 F10.8 --- PQSO ? Probability from DSC-Combmod of being
a quasar (data used: BP/RP spectrum)
(classprobdsccombmod_quasar)
64- 73 F10.8 --- PGal ? Probability from DSC-Combmod of being
a galaxy (data used: BP/RP spectrum)
(classprobdsccombmod_galaxy)
75- 84 F10.8 --- Pstar ? Probability from DSC-Combmod of being
a single star (but not a white dwarf)
(data used: BP/RP spectrum)
(classprobdsccombmod_star)
86- 95 F10.8 --- PWD ? Probability from DSC-Combmod of being
a white dwarf
(data used: BP/RP spectrum)
(classprobdsccombmod_whitedwarf)
97- 106 F10.8 --- Pbin ? Probability from DSC-Combmod of being
a binary star
(data used: BP/RP spectrum)
(classprobdsccombmod_binarystar)
108- 117 F10.8 --- PQSO-S ? Probability from DSC-Specmod of being
a quasar (data used: BP/RP spectrum)
(classprobdscspecmod_quasar)
119- 128 F10.8 --- Pgal-S ? Probability from DSC-Specmod of being
a galaxy (data used: BP/RP spectrum)
(classprobdscspecmod_galaxy)
130- 139 F10.8 --- Pstar-S ? Probability from DSC-Specmod of being
a single star (but not a white dwarf)
(data used: BP/RP spectrum)
(classprobdscspecmod_star)
141- 150 F10.8 --- PWD-S ? Probability from DSC-Specmod of being
a white dwarf
(data used: BP/RP spectrum)
(classprobdscspecmod_whitedwarf)
152- 161 F10.8 --- Pbin-S ? Probability from DSC-Specmod of being
a binary star
(data used: BP/RP spectrum)
(classprobdscspecmod_binarystar)
163- 172 F10.8 --- PQSO-A ? Probability from DSC-Allosmod of
being a quasar (data used: photometry)
(classprobdscallosmod_quasar)
174- 183 F10.8 --- PGal-A ? Probability from DSC-Allosmod of
being a galaxy (data used: photometry)
(classprobdscallosmod_galaxy)
185- 194 F10.8 --- Pstar-A ? Probability from DSC-Allosmod of
being a star (data used: photometry)
(classprobdscallosmod_star)
196- 205 F10.4 K Teff ? Effective temperature from GSP-Phot
Aeneas best library using BP/RP
spectra (teff_gspphot)
207- 216 F10.4 K b_Teff ? Lower confidence level (16%) of
effective temperature from GSP-Phot
Aeneas best library using BP/RP
spectra (teffgspphotlower)
218- 227 F10.4 K B_Teff ? Upper confidence level (84%) of
effective temperature from GSP-Phot
Aeneas best library using BP/RP
spectra (teffgspphotupper)
229- 235 F7.4 [cm/s2] logg ? Surface gravity from GSP-Phot Aeneas
best library using BP/RP spectra
(logg_gspphot)
237- 243 F7.4 [cm/s2] b_logg ? Lower confidence level (16%) of
surface gravity from GSP-Phot Aeneas
best library using BP/RP spectra
(logggspphotlower)
245- 251 F7.4 [cm/s2] B_logg ? Upper confidence level (84%) of
surface gravity from GSP-Phot Aeneas
best library using BP/RP spectra
(logggspphotupper)
253- 259 F7.4 [-] [Fe/H] ? Iron abundance from GSP-Phot Aeneas
best library using BP/RP spectra
(mh_gspphot)
261- 267 F7.4 [-] b_[Fe/H] ? Lower confidence level (16%) of iron
abundance from GSP-Phot Aeneas best
library using BP/RP spectra
(mhgspphotlower)
269- 275 F7.4 [-] B_[Fe/H] ? Upper confidence level (84%) of iron
abundance from GSP-Phot Aeneas best
library using BP/RP spectra
(mhgspphotupper)
277- 286 F10.4 pc Dist ? Distance from GSP-Phot Aeneas best
library using BP/RP spectra
(distance_gspphot)
288- 297 F10.4 pc b_Dist ? Lower confidence level (16%) of
distance from GSP-Phot Aeneas best
library using BP/RP spectra
(distancegspphotlower)
299- 308 F10.4 pc B_Dist ? Upper confidence level (84%) of
distance from GSP-Phot Aeneas best
library using BP/RP spectra
(distancegspphotupper)
310- 316 F7.4 mag A0 ? Monochromatic extinction A0 at
547.7nm from GSP-Phot Aeneas best
library using BP/RP spectra
(azero_gspphot)
318- 323 F6.4 mag b_A0 ? Lower confidence level (16%) of
monochromatic extinction A0 at 547.7nm
from GSP-Phot Aeneas best library
using BP/RP spectra
(azerogspphotlower)
325- 331 F7.4 mag B_A0 ? Upper confidence level (84%) of
monochromatic extinction A0 at 547.7nm
from GSP-Phot Aeneas best library
using BP/RP spectra
(azerogspphotupper)
333- 338 F6.4 mag AG ? Extinction in G band from GSP-Phot
Aeneas best library using BP/RP
spectra (ag_gspphot)
340- 345 F6.4 mag b_AG ? Lower confidence level (16%) of
extinction in G band from GSP-Phot
Aeneas best library using BP/RP
spectra (aggspphotlower)
347- 352 F6.4 mag B_AG ? Upper confidence level (84%) of
extinction in G band from GSP-Phot
Aeneas best library using BP/RP
spectra (aggspphotupper)
354- 359 F6.4 mag ABP ? Extinction in GBP band from
GSP-Phot Aeneas best library using
BP/RP spectra (abp_gspphot)
361- 366 F6.4 mag b_ABP ? Lower confidence level (16%) of
extinction in GBP band from
GSP-Phot Aeneas best library using
BP/RP spectra (abpgspphotlower)
368- 373 F6.4 mag B_ABP ? Upper confidence level (84%) of
extinction in GBP band from
GSP-Phot Aeneas best library using
BP/RP spectra (abpgspphotupper)
375- 380 F6.4 mag ARP ? Extinction in GRP band from
GSP-Phot Aeneas best library using
BP/RP spectra (arp_gspphot)
382- 387 F6.4 mag b_ARP ? Lower confidence level (16%) of
extinction in GRP band from GSP-Phot
Aeneas best library using BP/RP
spectra (arpgspphotlower)
389- 394 F6.4 mag B_ARP ? Upper confidence level (84%) of
extinction in GRP band from GSP-Phot
Aeneas best library using BP/RP
spectra (arpgspphotupper)
396- 401 F6.4 mag E(BP-RP) ? Reddening E(GBP-GRP) from
GSP-Phot Aeneas best library using
BP/RP spectra (ebpminrp_gspphot)
403- 408 F6.4 mag b_E(BP-RP) ? Lower confidence level (16%) of
reddening E(GBP-GRP) from
GSP-Phot Aeneas best library using
BP/RP spectra (ebpminrpgspphotlower)
410- 415 F6.4 mag B_E(BP-RP) ? Upper confidence level (84%) of
reddening E(GBP-GRP) from
GSP-Phot Aeneas best library using
BP/RP spectra (ebpminrpgspphotupper)
417- 423 F7.4 mag GMAG ? Absolute magnitude MG from GSP-Phot
Aeneas best library using BP/RP
spectra (mg_gspphot)
425- 431 F7.4 mag b_GMAG ? Lower confidence level (16%) of
absolute magnitude MG from GSP-Phot
Aeneas best library using BP/RP
spectra (mggspphotlower)
433- 439 F7.4 mag B_GMAG ? Upper confidence level (84%) of
absolute magnitude MG from GSP-Phot
Aeneas best library using BP/RP
spectra (mggspphotupper)
441- 449 F9.4 solRad Rad ? Radius from GSP-Phot Aeneas best
library using BP/RP spectra
(radius_gspphot)
451- 459 F9.4 solRad b_Rad ? Lower confidence level (16%) of
radius from GSP-Phot Aeneas best
library using BP/RP spectra
(radiusgspphotlower)
461- 469 F9.4 solRad B_Rad ? Upper confidence level (84%) of
radius from GSP-Phot Aeneas best
library using BP/RP spectra
(radiusgspphotupper)
471- 484 E14.7 --- logpost ? Goodness-of-fit score (mean
log-posterior of MCMC) of GSP-Phot
Aeneas MCMC best library
(logposterior_gspphot)
486- 496 F11.9 --- Accp ? MCMC acceptance rate of GSP-Phot
Aeneas MCMC best library
(mcmcaccept_gspphot)
498- 504 A7 --- Lib Name of library that achieves the
highest mean log-posterior in MCMC
samples and was used to derive
GSP-Phot parameters in this table
(libname_gspphot)
506- 512 F7.1 K Teff-S ? Effective temperature from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(teff_gspspec)
514- 520 F7.1 K b_Teff-S ? 16th percentile of effective
temperature from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(teffgspspeclower)
522- 528 F7.1 K B_Teff-S ? 84th percentile of effective
temperature from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(teffgspspecupper)
530- 534 F5.2 [cm/s2] logg-S ? Logarithm of the stellar surface
gravity from GSP-Spec MatisseGauguin
using RVS spectra and Monte Carlo
realisations (logg_gspspec)
536- 540 F5.2 [cm/s2] b_logg-S ? 16th percentile of the logarithm of
the stellar surface gravity from
GSP-Spec MatisseGauguin using RVS
spectra and Monte Carlo realisations
(logggspspeclower)
542- 546 F5.2 [cm/s2] B_logg-S ? 84th percentile of the logarithm of
the stellar surface gravity from
GSP-Spec MatisseGauguin using RVS
spectra and Monte Carlo realisations
(logggspspecupper)
548- 552 F5.2 [-] [M/H]-S ? Global metallicity [M/H] from
GSP-Spec MatisseGauguin using RVS
spectra and Monte Carlo realisations
(mh_gspspec)
554- 558 F5.2 [-] b_[M/H]-S ? 16th percentile of global
metallicity [M/H] from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(mhgspspeclower)
560- 564 F5.2 [-] B_[M/H]-S ? 84th percentile of global
metallicity [M/H] from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(mhgspspecupper)
566- 570 F5.2 [-] [alpha/Fe]-S ? Abundance of alpha-elements
[alpha/Fe] with respect to iron from
GSP-Spec MatisseGauguin using RVS
spectra and Monte Carlo realisations
(alphafe_gspspec)
572- 576 F5.2 [-] b_[alpha/Fe]-S ? 16th percentile of the abundance of
alpha-elements [alpha/Fe] with respect
to iron from GSP-Spec MatisseGauguin
using RVS spectra and Monte Carlo
realisations (alphafegspspeclower)
578- 582 F5.2 [-] B_[alpha/Fe]-S ? 84th percentile of the abundance of
alpha-elements [alpha/Fe] with respect
to iron from GSP-Spec MatisseGauguin
using RVS spectra and Monte Carlo
realisations (alphafegspspecupper)
584- 588 F5.2 [-] [Fe/H]-S ? Abundance of neutral iron [Fe/M] from
GSP-Spec MatisseGauguin using RVS
spectra and Monte Carlo realisations
(fem_gspspec)
590- 594 F5.2 [-] b_[Fe/H]-S ? 16th percentile of the abundance of
neutral iron [Fe/M] from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(femgspspeclower)
596- 600 F5.2 [-] B_[Fe/H]-S ? 84th percentile of the abundance of
neutral iron [Fe/M] from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(femgspspecupper)
602 I1 --- o_[Fe/H]-S [0/8]? Number of lines used for [Fe/M]
abundance estimation
(femgspspecnlines)
604- 607 F4.2 [-] s_[Fe/H]-S ? Uncertainty estimation of [Fe/M]
abundance using N lines of the element
(femgspspeclinescatter)
609- 613 F5.2 [-] [Si/Fe]-S ? Abundance of Silicon [Si/Fe] from
GSP-Spec MatisseGauguin using RVS
spectra and Monte Carlo realisations
(sife_gspspec)
615- 619 F5.2 [-] b_[Si/Fe]-S ? 16th percentile of the abundance of
silicon [Si/Fe] from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(sifegspspeclower)
621- 625 F5.2 [-] B_[Si/Fe]-S ? 84th percentile of the abundance of
silicon [Si/Fe] from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(sifegspspecupper)
627 I1 --- o_[Si/Fe]-S [0/3]? Number of lines used for [Si/Fe]
abundance estimation
(sifegspspecnlines)
629- 632 F4.2 [-] s_[Si/Fe]-S ? Uncertainty estimation of [Si/Fe]
abundance using N lines of the element
(sifegspspeclinescatter)
634- 638 F5.2 [-] [Ca/Fe]-S ? Abundance of Calcium [Ca/Fe] from
GSP-Spec MatisseGauguin using RVS
spectra and Monte Carlo realisations
(cafe_gspspec)
640- 644 F5.2 [-] b_[Ca/Fe]-S ? 16th percentile of the abundance of
Calcium [Ca/Fe] from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(cafegspspeclower)
646- 650 F5.2 [-] B_[Ca/Fe]-S ? 84th percentile of the abundance of
Calcium [Ca/Fe] from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(cafegspspecupper)
652 I1 --- o_[Ca/Fe]-S [0/7]? Number of lines used for [Ca/Fe]
abundance estimation
(cafegspspecnlines)
654- 657 F4.2 [-] s_[Ca/Fe]-S ? Uncertainty estimation of [Ca/Fe]
abundance using N lines of the element
(cafegspspeclinescatter)
659- 663 F5.2 [-] [Ti/Fe]-S ? Abundance of Titanium [Ti/Fe] from
GSP-Spec MatisseGauguin using RVS
spectra and Monte Carlo realisations
(tife_gspspec)
665- 669 F5.2 [-] b_[Ti/Fe]-S ? 16th percentile of the abundance of
Titanium [Ti/Fe] from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(tifegspspeclower)
671- 675 F5.2 [-] B_[Ti/Fe]-S ? 84th percentile of the abundance of
Titanium [Ti/Fe] from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(tifegspspecupper)
677 I1 --- o_[Ti/Fe]-S [0/3]? Number of lines used for [Ti/Fe]
abundance estimation
(tifegspspecnlines)
679- 682 F4.2 [-] s_[Ti/Fe]-S ? Uncertainty estimation of [Ti/Fe]
abundance using N lines of the element
(tifegspspeclinescatter)
684- 688 F5.2 [-] [Mg/Fe]-S ? Abundance of Magnesium [Mg/Fe] from
GSP-Spec MatisseGauguin using RVS
spectra and Monte Carlo realisations
(mgfe_gspspec)
690- 694 F5.2 [-] b_[Mg/Fe]-S ? 16th percentile of the abundance of
Magnesium [Mg/Fe] from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(mgfegspspeclower)
696- 700 F5.2 [-] B_[Mg/Fe]-S ? 84th percentile of the abundance of
Magnesium [Mg/Fe] from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(mgfegspspecupper)
702- 706 F5.2 [-] [Nd/Fe]-S ? Abundance of neodymium [Nd/Fe] from
GSP-Spec MatisseGauguin using RVS
spectra and Monte Carlo realisations
(ndfe_gspspec)
708- 712 F5.2 [-] b_[Nd/Fe]-S ? 16th percentile of the abundance of
neodymium [Nd/Fe] from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(ndfegspspeclower)
714- 718 F5.2 [-] B_[Nd/Fe]-S ? 84th percentile of the abundance of
neodymium [Nd/Fe] from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(ndfegspspecupper)
720- 724 F5.2 [-] [FeII/M]-S ? Abundance of ionised iron [FeII/M]
from GSP-Spec MatisseGauguin using RVS
spectra and Monte Carlo realisations
(feiim_gspspec)
726- 730 F5.2 [-] b_[FeII/M]-S ? 16th percentile of the abundance of
ionised iron [FeII/M] from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(feiimgspspeclower)
732- 736 F5.2 [-] B_[FeII/M]-S ? 84th percentile of the abundance of
ionised iron [FeII/M] from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(feiimgspspecupper)
738- 742 F5.2 [-] [S/Fe]-S ? Abundance of Sulphur [S/Fe] from
GSP-Spec MatisseGauguin using RVS
spectra and Monte Carlo realisations
(sfe_gspspec)
744- 748 F5.2 [-] b_[S/Fe]-S ? 16th percentile of the abundance of
Sulphur [S/Fe] from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(sfegspspeclower)
750- 754 F5.2 [-] B_[S/Fe]-S ? 84th percentile of the abundance of
Sulphur [S/Fe] from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(sfegspspecupper)
756 I1 --- o_[S/Fe]-S [0/2]? Number of lines used for [S/Fe]
abundance estimation
(sfegspspecnlines)
758- 761 F4.2 [-] s_[S/Fe]-S ? Uncertainty estimation of [S/Fe]
abundance using N lines of the element
(sfegspspeclinescatter)
763- 767 F5.2 [-] [Zr/Fe]-S ? Abundance of Zirconium [Zr/Fe] from
GSP-Spec MatisseGauguin using RVS
spectra and Monte Carlo realisations
(zrfe_gspspec)
769- 773 F5.2 [-] b_[Zr/Fe]-S ? 16th percentile of the abundance of
Zirconium [Zr/Fe] from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(zrfegspspeclower)
775- 779 F5.2 [-] B_[Zr/Fe]-S ? 84th percentile of the abundance of
Zirconium [Zr/Fe] from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(zrfegspspecupper)
781- 785 F5.2 [-] [N/Fe]-S ? Abundance of Nitrogen [N/Fe] from
GSP-Spec MatisseGauguin using RVS
spectra and Monte Carlo realisations
(nfe_gspspec)
787- 791 F5.2 [-] b_[N/Fe]-S ? 16th percentile of the abundance of
Nitrogen [N/Fe] from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(nfegspspeclower)
793- 797 F5.2 [-] B_[N/Fe]-S ? 84th percentile of the abundance of
Nitrogen [N/Fe] from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(nfegspspecupper)
799 I1 --- o_[N/Fe]-S [0/2]? Number of lines used for [N/Fe]
abundance estimation
(nfegspspecnlines)
801- 804 F4.2 [-] s_[N/Fe]-S ? Uncertainty estimation of [N/Fe]
abundance using N lines of the element
(nfegspspeclinescatter)
806- 810 F5.2 [-] [Cr/Fe]-S ? Abundance of Chromium [Cr/Fe] from
GSP-Spec MatisseGauguin using RVS
spectra and Monte Carlo realisations
(crfe_gspspec)
812- 816 F5.2 [-] b_[Cr/Fe]-S ? 16th percentile of the abundance of
Chromium [Cr/Fe] from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(crfegspspeclower)
818- 822 F5.2 [-] B_[Cr/Fe]-S ? 84th percentile of the abundance of
Chromium [Cr/Fe] from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(crfegspspecupper)
824 I1 --- o_[Cr/Fe]-S [0/2]? Number of lines used for [Cr/Fe]
abundance estimation
(crfegspspecnlines)
826- 829 F4.2 [-] s_[Cr/Fe]-S ? Uncertainty estimation of [Cr/Fe]
abundance using N lines of the element
(crfegspspeclinescatter)
831- 835 F5.2 [-] [Ce/Fe]-S ? Abundance of Cerium [Ce/Fe] from
GSP-Spec MatisseGauguin using RVS
spectra and Monte Carlo realisations
(cefe_gspspec)
837- 841 F5.2 [-] b_[Ce/Fe]-S ? 16th percentile of the abundance of
Cerium [Ce/Fe] from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(cefegspspeclower)
843- 847 F5.2 [-] B_[Ce/Fe]-S ? 84th percentile of the abundance of
Cerium [Ce/Fe] from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(cefegspspecupper)
849- 853 F5.2 [-] [Ni/Fe]-S ? Abundance of Nickel [Ni/Fe] from
GSP-Spec MatisseGauguin using RVS
spectra and Monte Carlo realisations
(nife_gspspec)
855- 859 F5.2 [-] b_[Ni/Fe]-S ? 16th percentile of the abundance of
Nickel [Ni/Fe] from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(nifegspspeclower)
861- 865 F5.2 [-] B_[Ni/Fe]-S ? 84th percentile of the abundance of
Nickel [Ni/Fe] from GSP-Spec
MatisseGauguin using RVS spectra and
Monte Carlo realisations
(nifegspspecupper)
867- 871 F5.2 nm EWCN0 ? Equivalent width of cyoanogen line
(cn0ew_gspspec)
873- 876 F4.2 nm e_EWCN0 ? Uncertainty of equivalent width of
cyanogen absorption line
(cn0ewgspspecuncertainty)
878- 883 F6.2 nm CN0 ? Central wavelength of cyanogen line
(cn0gspspeccentralline)
885- 888 F4.2 nm CN0W ? Width of cyoanogen line
(cn0gspspecwidth)
890- 898 F9.5 nm DIB ? DIB central wavelength from GSP-Spec
MatisseGauguin using RVS spectra
(dibgspspeclambda)
900- 906 F7.5 nm e_DIB ? Uncertainty on DIB central wavelength
from GSP-Spec MatisseGauguin using RVS
spectra
(dibgspspeclambda_uncertainty)
908- 921 E14.8 0.1nm EWDIB ? Equivalent width of the DIB from
GSP-Spec MatisseGauguin using RVS
spectra (dibew_gspspec)
923- 936 E14.8 0.1nm e_EWDIB ? Global uncertainty on DIB equivalent
width value using DIB algorithm
(dibewgspspecuncertainty)
938- 945 E8.1 0.1nm s_EWDIB ? Uncertainty on DIB equivalent width
value occuring from noise part
(dibewnoisegspspecuncertainty)
947- 960 E14.7 --- DIBp0 ? Depth (p_0 parameter) of the DIB
derived from a Gaussian model fit
(dibp0_gspspec)
962- 967 F6.4 0.1nm DIBp2 ? Width (p_2 parameter) of the DIB
derived from a Gaussian model fit
(dibp2_gspspec)
969- 976 F8.4 0.1nm e_DIBp2 ? Uncertainty on the dibp2Gspspec
parameter (dibp2gspspecuncertainty)
978- 979 I2 --- q_DIB [-2/5]? Quality flag of the DIB
computation (dibqf_gspspec)
981-1021 A41 --- Flags ? Catalogue flags for GSP-Spec
MatisseGauguin (flags_gspspec) (1)
1023-1033 F11.8 --- chi2 ? Logarithm of the goodness-of-fit for
the GSP-Spec MatisseGauguin parameters
(logchisq_gspspec)
1035-1043 F9.5 nm EWHa ? Halpha pseudo-equivalent width from
ESP-ELS (ewespelshalpha)
1045-1052 F8.5 nm e_EWHa ? Uncertainty of the Halpha
pseudo-equivalent width from ESP-ELS
(ewespelshalpha_uncertainty)
1054 I1 --- f_EWHa [0/9]? Quality flag of the Halpha
pseudo-equivalent width from ESP-ELS
(ewespelshalpha_flag)
1056-1064 F9.6 nm EWHamod ? Halpha pseudo-equivalent width from
ESP-ELS measured on the synthetic
spectrum (ewespelshalpha_model)
1066-1080 A15 --- ClassELS Adopted ELS class label from ESP-ELS
(classlabel_espels)
1082-1083 I2 --- f_ClassELS ? Quality flag of the adopted ELS
class label from ESP-ELS
(classlabelespelsflag)
1085-1094 F10.8 --- PWC ? Probability from ESP-ELS of being a
Wolf-Rayet star of type WC
(classprobespelswcstar)
1096-1105 F10.8 --- PWN ? Probability from ESP-ELS of being a
Wolf-Rayet star of type WN
(classprobespelswnstar)
1107-1116 F10.8 --- PBe ? Probability from ESP-ELS of being a
Be Star (classprobespelsbestar)
1118-1127 F10.8 --- PTTau ? Probability from ESP-ELS of being a
T Tauri Star
(classprobespelsttauristar)
1129-1138 F10.8 --- PHAe/Be ? Probability from ESP-ELS of being a
Herbig Ae/Be Star
(classprobespelsherbigstar)
1140-1149 F10.8 --- PdMactive ? Probability from ESP-ELS of being an
active M dwarf Star
(classprobespelsdmestar)
1151-1160 F10.8 --- PPN ? Probability from ESP-ELS of being a
planetary nebula
(classprobespelspne)
1162-1168 F7.4 mag A0-HS ? Monochromatic interstellar extinction
(azero_esphs)
1170-1175 F6.4 mag e_A0-HS ? Uncertainty at a 68% confidence level
on A0 from ESP-HS
(azeroesphsuncertainty)
1177-1182 F6.4 mag AG-HS ? Intersterstellar extinction in G band
from ESP-HS (ag_esphs)
1184-1189 F6.4 mag e_AG-HS ? Uncertainty on AG from ESP-HS
(agesphsuncertainty)
1191-1196 F6.4 mag E(BP-RP)-HS ? Reddening E(GBP-GRP) from ESP-HS
(ebpminrp_esphs)
1198-1203 F6.4 mag e_E(BP-RP)-HS ? Uncertainty on E(GBP-GRP) from
ESP-HS (ebpminrpesphsuncertainty)
1205-1214 F10.4 K Teff-HS ? Effective temperature from ESP-HS
(teff_esphs)
1216-1225 F10.4 K e_Teff-HS ? Uncertainty at a 68% confidence level
on the effective temperature from
ESP-HS (teffesphsuncertainty)
1227-1232 F6.4 [cm/s2] logg-HS ? Surface gravity from ESP-HS
(logg_esphs)
1234-1239 F6.4 [cm/s2] e_logg-HS ? Uncertainty at a 68% confidence level
on the surface gravity from ESP-HS
(loggesphsuncertainty)
1241-1247 F7.3 km/s vsini-HS ? Projected rotational velocity from
ESP-HS (vsini_esphs)
1249-1256 F8.3 km/s e_vsini-HS ? Uncertainty on the projected
rotational velocity from ESP-HS
(vsiniesphsuncertainty)
1258-1260 I3 --- Flags-HS ? Quality flag of the ESP-HS
parametrisation (flags_esphs) (2)
1262-1268 A7 --- SpType-ELS Spectral type from ESP-ELS
(spectraltype_esphs)
1270-1277 F8.5 nm CA-CS ? Chromospheric activity index from
ESP-CS (activityindex_espcs)
1279-1285 F7.5 nm e_CA-CS ? Uncertainty in the chromospheric
activity index from ESP-CS
(activityindexespcsuncertainty)
1287-1288 A2 --- n_CA-CS [12M] Source of input stellar
parameters for the computation of the
activity index by ESP-CS
(activityindexespcsinput)
1290-1296 F7.2 K Teff-UCD ? Effective temperature estimate from
ESP-UCD based on the RP spectrum
(teff_espucd)
1298-1303 F6.2 K e_Teff-UCD ? Uncertainty of the effective
temperature estimate produced by
ESP-UCD (teffespucduncertainty)
1305-1306 I2 --- Flags-UCD [0/21]? Quality flags of the ESP-UCD
parameter estimates (flags_espucd) (3)
1308-1315 F8.4 Rsun Rad-Flame ? Radius of the star from FLAME using
teff_gspphot and lum_flame
(radius_flame)
1317-1324 F8.4 Rsun b_Rad-Flame ? Lower confidence level (16%) of
radiusFlame (radiusflamelower)
1326-1333 F8.4 Rsun B_Rad-Flame ? Upper confidence level (84%) of
radiusFlame (radiusflameupper)
1335-1344 E10.4 Lsun Lum-Flame ? Luminosity of the star from FLAME
using G band magnitude, extinction
(ag_gspphot), parallax or distance,
and a bolometric correction bc_flame
(lum_flame)
1346-1355 E10.4 Lsun b_Lum-Flame ? Lower confidence level (16%) of
lumFlame (lumflamelower)
1357-1366 E10.4 Lsun B_Lum-Flame ? Upper confidence level (84%) of
lumFlame (lumflameupper)
1368-1372 F5.3 Msun Mass-Flame ? Mass of the star from FLAME using
stellar models, lum_flame, and
teff_gspphot (mass_flame)
1374-1378 F5.3 Msun b_Mass-Flame ? Lower confidence level (16%) of
mass of the star from FLAME
(massflamelower)
1380-1384 F5.3 Msun B_Mass-Flame ? Upper confidence level (84%) of
mass of the star from FLAME
(massflameupper)
1386-1391 F6.3 Gyr Age-Flame ? Age of the star from FLAME using
stellar models (age_flame)
1393-1398 F6.3 Gyr b_Age-Flame ? Lower confidence level (84%) of
age of the star from FLAME
(ageflamelower)
1400-1405 F6.3 Gyr B_Age-Flame ? Upper confidence level (84%) of
age of the star from FLAME
(ageflameupper)
1407-1408 I2 --- Flags-Flame [0/22]? Flags indicating quality and
processing information from FLAME
(flags_flame) (4)
1410-1413 I4 --- Evol ? Evolutionary stage of the star from
FLAME using stellar models
(evolstage_flame)
1415-1424 F10.8 km/s z-Flame ? Gravitational redshift from FLAME
using radiusFlame and loggGspphot
(gravredshift_flame)
1426-1435 F10.8 km/s b_z-Flame ? Lower confidence level (16%) of
gravitational redshift from FLAME
(gravredshiftflamelower)
1437-1446 F10.8 km/s B_z-Flame ? Upper confidence level (84%) of
gravitational redshift from FLAME
(gravredshiftflameupper)
1448-1457 F10.7 mag BolCorr ? Bolometric correction used to derive
lumFlame (bc_flame)
1459-1467 F9.6 [-] [M/H]-MSC ? Metallicity of the source treated as
a binary system from MSC using BP/RP
spectra and parallax (mh_msc)
1469-1477 F9.6 [-] B_[M/H]-MSC ? Upper confidence level (84%) of the
metallicity from MSC using BP/RP
spectra and parallax (mhmscupper)
1479-1487 F9.6 [-] b_[M/H]-MSC ? Lower confidence level (16%) of the
metallicity from MSC using BP/RP
spectra and parallax (mhmsclower)
1489-1496 F8.6 mag A0-MSC ? Monochromatic extinction A0 at
541.4nm of the source treated as a
binary system from MSC using BP/RP
spectra and parallax (azero_msc)
1498-1505 F8.6 mag B_A0-MSC ? Upper confidence level (84%) of
monochromatic extinction A0 at 547.7nm
from MSC using BP/RP spectra and
parallax (azeromscupper)
1507-1514 F8.6 mag b_A0-MSC ? Lower confidence level (16%) of
monochromatic extinction A0 at 547.7nm
from MSC using BP/RP spectra and
parallax (azeromsclower)
1516-1523 F8.3 pc Dist-MSC ? Distance from MSC using BP/RP spectra
and parallax (distance_msc)
1525-1533 F9.3 pc B_Dist-MSC ? Upper confidence level (84%) of
distance from MSC using BP/RP spectra
and parallax (distancemscupper)
1535-1542 F8.3 pc b_Dist-MSC ? Lower confidence level (16%) of
distance from MSC using BP/RP spectra
and parallax (distancemsclower)
1544-1552 F9.4 K Teff1-MSC ? Effective temperature of the primary
from MSC using BP/RP spectra and
parallax (teff_msc1)
1554-1562 F9.4 K B_Teff1-MSC ? Upper confidence level (84%) of
effective temperature of the primary
from MSC using BP/RP spectra and
parallax (teffmsc1upper)
1564-1572 F9.4 K b_Teff1-MSC ? Lower confidence level (16%) of
effective temperature of the primary
from MSC using BP/RP spectra and
parallax (teffmsc1lower)
1574-1582 F9.4 K Teff2-MSC ? Effective temperature of the
secondary from MSC using BP/RP
spectra and parallax (teff_msc2)
1584-1592 F9.4 K B_Teff2-MSC ? Upper confidence level (84%) of
effective temperature of the secondary
from MSC using BP/RP spectra and
parallax (teffmsc2upper)
1594-1602 F9.4 K b_Teff2-MSC ? Lower confidence level (16%) of
effective temperature of the secondary
from MSC using BP/RP spectra and
parallax (teffmsc2lower)
1604-1609 F6.4 [cm/s2] logg1-MSC ? Surface gravity of the primary from
MSC using BP/RP spectra and parallax
(logg_msc1)
1611-1616 F6.4 [cm/s2] B_logg1-MSC ? Upper confidence level (84%) of
surface gravity of the primary from
MSC using BP/RP spectra and parallax
(loggmsc1upper)
1618-1623 F6.4 [cm/s2] b_logg1-MSC ? Lower confidence level (16%) of
surface gravity of the primary from
MSC using BP/RP spectra and parallax
(loggmsc1lower)
1625-1630 F6.4 [cm/s2] logg2-MSC ? Surface gravity of the secondary from
MSC using BP/RP spectra and parallax
(logg_msc2)
1632-1637 F6.4 [cm/s2] B_logg2-MSC ? Upper confidence level (84%) of
surface gravity of the secondary from
MSC using BP/RP spectra and parallax
(loggmsc2upper)
1639-1644 F6.4 [cm/s2] b_logg2-MSC ? Lower confidence level (16%) of
surface gravity of the secondary from
MSC using BP/RP spectra and parallax
(loggmsc2lower)
1646-1653 F8.6 mag AG-MSC ? Extinction in G band from MSC using
BP/RP spectra and parallax (ag_msc)
1655-1662 F8.6 mag B_AG-MSC ? Upper confidence level (84%) of
extinction in G band from MSC using
BP/RP spectra and parallax
(agmscupper)
1664-1671 F8.6 mag b_AG-MSC ? Lower confidence level (16%) of
extinction in G band from MSC using
BP/RP spectra and parallax
(agmsclower)
1673-1687 E15.8 --- logpost-MSC ? Goodness-of-fit score (normalised
log-posterior) of MSC MCMC
(logposterior_msc)
1689-1699 F11.9 --- Accp-MSC ? Mean MCMC acceptance rate of MSC MCMC
(mcmcaccept_msc)
1701-1713 E13.7 --- drift-MSC ? Mean drift of the MSC MCMC chain in
units of parameter standard deviation
(mcmcdrift_msc)
1715 I1 --- Flag-MSC [0/1]? Flag indicating quality
information from MSC (flags_msc) (5)
1717-1734 I18 --- NOAId ? Identifier of the OA SOM map neuron
that represents the source
(neuronoaid)
1736-1749 E14.8 --- NOADist ? Distance between the source XP
spectra and the OA neuron XP prototype
that represents the source
(neuronoadist)
1751-1752 I2 --- NOADistRank [0/95]? Percentile rank according to
the distance distribution of the OA
neuron that represents the source
(neuronoadistpercentilerank)
1754-1757 I4 --- Flags-NOA ? Flags indicating quality and
processing information from OA
(flags_oa) (6)
--------------------------------------------------------------------------------
Note (1): Definitions of each character in the GSP-Spec MatisseGauguin
(Recio-Blanco 2022, in prep.) quality flag chain.
In this chain, value 0 is the best, and 9 is the worst.
Note (2): The quality flag usually has 2 digits.
The first digit tells what processing mode was used to derive the effective
temperature, surface gravity, interstellar extinction and reddening, and
vsini. It takes the following values:
0: when both BP/RP and RVS spectra were used.
1: when BP/RP only was used. In this mode no v sin i is available.
The second digit is relative to the spectral type (spectraltype_esphs) that is
derived from the analysis of the BP/RP spectrum only. During the processing
a probability was assigned, and used for the quality assessment of the
spectral type tagging. Therefore, the second digit of flags esphs ranges
from 1 to 5, depending on the first (p1) and second (p2) highest probability
as follows:
p1 > 0.5 and p2 ≤ 0.1: second digit of flags_esphs = 1
p1 > 0.5 and p2 ≤ 0.2: second digit of flags_esphs = 2
p1 > 0.5 and p2 ≤ 0.3: second digit of flags_esphs = 3
p1 > 0.5 and p2 ≤ 0.4: second digit of flags_esphs = 4
p1 ≤ 0.5: second digit of flags_esphs = 5
target brighter than G=17.65, but no spectral type tag was derived:
flags_esphs = 999
Note (3): Two-digits ESP-UCD parameters quality flag.
The first digit (0, 1 or 2) is based on the goodness-of-fit estimate and
the RP spectrum signal-to-noise ratio, 0 being the best quality.
The second digit is 1 for sources with inconsistent Teff predictions given the
value of G+5log10(ϖ+5. It is 0 for all other sources.
Note (4): This field contains the quality and processing flags from FLAME and
takes the form 'AB'.
The first digit refers to the quality of the mass and age determination
(A = 0, 1, 2) and the second digit (B) informs the user if the parallax
or distance gspphot was used for deriving all FLAME stellar parameters
(lum_flame, radius_flame,...).
Concerning the quality of the mass and age (first digit, A),
the following is adopted:
A=0 nothing to report
A=1 the star is a giant and the mass and age should be considered with an
uncertainty on the order of 20%-30%
A=2 the mass and age are not available
We note that while the evolstage flame parameter is related to mass and age,
this flag is not applicable to this parameter.
For the second digit, B, the following is adopted:
B=0 parallax is used
B=1 distance gspphot is used
B=2 parallax is used due to convergence issues with distance gspphot
Note (5): Catalogue flag for MSC.
This is set to 0 if logposterior_msc≥-1000 & mcmcdrift_msc ≤1.
In all other cases it is set to 1 indicating an unreliable inference result.
Note (6): Processing flags related to the quality of the classification and
source processing performed by the OA module, which is encoded as follows:
ABCD where:
-------------------------------------------------------------------
Code | Description | Value range
-------------------------------------------------------------------
A | Number of gaps with negative fluxes in BP spectrum | [0, 2] *
B | Number of gaps with negative fluxes in RP spectrum | [0, 2] *
C | Source classification quality category | [0, 5]
D | Neuron quality category | [0, 6]
-------------------------------------------------------------------
(*) A and B flags taking value 2 means two or more gaps taking negative
flux values.
-------------------------------------------------------------------
--------------------------------------------------------------------------------
Byte-by-byte Description of file: paramsup.sam
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 19 I19 --- Source Source Identifier (source_id)
21- 35 F15.11 deg RAdeg Right ascension (ICRS) at Ep=2016.0
(ra)
37- 51 F15.11 deg DEdeg Declination (ICRS) at Ep=2016.0 (dec)
53- 71 I19 --- SolID Solution Identifier (solution_id)
73- 79 A7 --- Lib Name of library that achieves the
highest mean log-posterior in MCMC
samples from GSP-Phot Aeneas
(libnamebestgspphot)
81- 89 F9.4 K Teff ? Effective temperature from GSP-Phot
Aeneas for MARCS library using BP/RP
spectra (teffgspphotmarcs)
91- 99 F9.4 K b_Teff ? Lower confidence level (16%) of
effective temperature from GSP-Phot
Aeneas for MARCS library using BP/RP
spectra (teffgspphotmarcs_lower)
101- 109 F9.4 K B_Teff ? Upper confidence level (84%) of
effective temperature from GSP-Phot
Aeneas for MARCS library using BP/RP
spectra (teffgspphotmarcs_upper)
111- 117 F7.4 [cm/s2] logg ? Surface gravity from GSP-Phot
Aeneas for MARCS library using BP/RP
spectra (logggspphotmarcs)
119- 125 F7.4 [cm/s2] b_logg ? Lower confidence level (16%) of
surface gravity from GSP-Phot Aeneas
for MARCS library using BP/RP
spectra (logggspphotmarcs_lower)
127- 133 F7.4 [cm/s2] B_logg ? Upper confidence level (84%) of
surface gravity from GSP-Phot Aeneas
for MARCS library using BP/RP
spectra (logggspphotmarcs_upper)
135- 141 F7.4 [-] [M/H] ? Iron abundance from GSP-Phot Aeneas
for MARCS library using BP/RP
spectra (mhgspphotmarcs)
143- 149 F7.4 [-] b_[M/H] ? Lower confidence level (16%) of
iron abundance from GSP-Phot Aeneas
for MARCS library using BP/RP
spectra (mhgspphotmarcs_lower)
151- 157 F7.4 [-] B_[M/H] ? Upper confidence level (84%) of
iron abundance from GSP-Phot Aeneas
for MARCS library using BP/RP
spectra (mhgspphotmarcs_upper)
159- 168 F10.4 pc Dist ? Distance from GSP-Phot Aeneas for
MARCS library using BP/RP spectra
(distancegspphotmarcs)
170- 179 F10.4 pc b_Dist ? Lower confidence level (16%) of
distance from GSP-Phot Aeneas for
MARCS library using BP/RP spectra
(distancegspphotmarcs_lower)
181- 190 F10.4 pc B_Dist ? Upper confidence level (84%) of
distance from GSP-Phot Aeneas for
MARCS library using BP/RP spectra
(distancegspphotmarcs_upper)
192- 198 F7.4 mag A0 ? Monochromatic extinction A_0 at
547.7nm from GSP-Phot Aeneas for
MARCS library using BP/RP spectra
(azerogspphotmarcs)
200- 205 F6.4 mag b_A0 ? Lower confidence level (16%) of
monochromatic extinction A_0 at
547.7nm from GSP-Phot Aeneas for
MARCS library using BP/RP spectra
(azerogspphotmarcs_lower)
207- 213 F7.4 mag B_A0 ? Upper confidence level (84%) of
monochromatic extinction A_0 at
547.7nm from GSP-Phot Aeneas for
MARCS library using BP/RP spectra
(azerogspphotmarcs_upper)
215- 220 F6.4 mag AG ? Extinction in G band from GSP-Phot
Aeneas for MARCS library using BP/RP
spectra (aggspphotmarcs)
222- 227 F6.4 mag b_AG ? Lower confidence level (16%) of
extinction in G band from GSP-Phot
Aeneas for MARCS library using BP/RP
spectra (aggspphotmarcs_lower)
229- 234 F6.4 mag B_AG ? Upper confidence level (84%) of
extinction in G band from GSP-Phot
Aeneas for MARCS library using BP/RP
spectra (aggspphotmarcs_upper)
236- 241 F6.4 mag ABP ? Extinction in G_BP band from
GSP-Phot Aeneas for MARCS library
using BP/RP spectra
(abpgspphotmarcs)
243- 248 F6.4 mag b_ABP ? Lower confidence level (16%) of
extinction in G_BP band from
GSP-Phot Aeneas for MARCS library
using BP/RP spectra
(abpgspphotmarcs_lower)
250- 255 F6.4 mag B_ABP ? Upper confidence level (84%) of
extinction in G_BP band from
GSP-Phot Aeneas for MARCS library
using BP/RP spectra
(abpgspphotmarcs_upper)
257- 262 F6.4 mag ARP ? Extinction in G_RP band from
GSP-Phot Aeneas for MARCS library
using BP/RP spectra
(arpgspphotmarcs)
264- 269 F6.4 mag b_ARP ? Lower confidence level (16%) of
extinction in G_RP band from
GSP-Phot Aeneas for MARCS library
using BP/RP spectra
(arpgspphotmarcs_lower)
271- 276 F6.4 mag B_ARP ? Upper confidence level (84%) of
extinction in G_RP band from
GSP-Phot Aeneas for MARCS library
using BP/RP spectra
(arpgspphotmarcs_upper)
278- 283 F6.4 mag E(BP-RP) ? Reddening E(BP-RP) from GSP-Phot
Aeneas for MARCS library using BP/RP
spectra (ebpminrpgspphotmarcs)
285- 290 F6.4 mag b_E(BP-RP) ? Lower confidence level (16%) of
reddening E(BP-RP) from GSP-Phot
Aeneas for MARCS library using BP/RP
spectra
(ebpminrpgspphotmarcs_lower)
292- 297 F6.4 mag B_E(BP-RP) ? Upper confidence level (84%) of
reddening E(BP-RP) from GSP-Phot
Aeneas for MARCS library using BP/RP
spectra
(ebpminrpgspphotmarcs_upper)
299- 305 F7.4 mag GMAG ? Absolute magnitude M_G from
GSP-Phot Aeneas for MARCS library
using BP/RP spectra
(mggspphotmarcs)
307- 313 F7.4 mag b_GMAG ? Lower confidence level (16%) of
absolute magnitude M_G from
GSP-Phot Aeneas for MARCS library
using BP/RP spectra
(mggspphotmarcs_lower)
315- 321 F7.4 mag B_GMAG ? Upper confidence level (84%) of
absolute magnitude M_G from GSP-Phot
Aeneas for MARCS library using BP/RP
spectra (mggspphotmarcs_upper)
323- 331 F9.4 Rsun Rad ? Radius from GSP-Phot Aeneas for
MARCS library using BP/RP spectra
(radiusgspphotmarcs)
333- 341 F9.4 Rsun b_Rad ? Lower confidence level (16%) of
radius from GSP-Phot Aeneas for
MARCS library using BP/RP spectra
(radiusgspphotmarcs_lower)
343- 351 F9.4 Rsun B_Rad ? Upper confidence level (84%) of
radius from GSP-Phot Aeneas for
MARCS library using BP/RP spectra
(radiusgspphotmarcs_upper)
353- 366 E14.7 --- logpost ? Goodness-of-fit score (mean
log-posterior of MCMC) of GSP-Phot
Aeneas MCMC for MARCS library
(logposteriorgspphotmarcs)
368- 376 F9.7 --- Accp ? MCMC acceptance rate of GSP-Phot
Aeneas MCMC for MARCS library
(mcmcacceptgspphotmarcs)
378- 386 F9.4 K Teff-Phx ? Effective temperature from
GSP-Phot Aeneas for PHOENIX library
using BP/RP spectra
(teffgspphotphoenix)
388- 396 F9.4 K b_Teff-Phx ? Lower confidence level (16%) of
effective temperature from GSP-Phot
Aeneas for PHOENIX library using
BP/RP spectra
(teffgspphotphoenix_lower)
398- 406 F9.4 K B_Teff-Phx ? Upper confidence level (84%) of
effective temperature from GSP-Phot
Aeneas for PHOENIX library using
BP/RP spectra
(teffgspphotphoenix_upper)
408- 414 F7.4 [cm/s2] logg-Phx ? Surface gravity from GSP-Phot
Aeneas for PHOENIX library using
BP/RP spectra (logggspphotphoenix)
416- 422 F7.4 [cm/s2] b_logg-Phx ? Lower confidence level (16%) of
surface gravity from GSP-Phot Aeneas
for PHOENIX library using BP/RP
spectra (logggspphotphoenix_lower)
424- 430 F7.4 [cm/s2] B_logg-Phx ? Upper confidence level (84%) of
surface gravity from GSP-Phot Aeneas
for PHOENIX library using BP/RP
spectra (logggspphotphoenix_upper)
432- 436 F5.2 [-] [M/H]-Phx ? Iron abundance from GSP-Phot Aeneas
for PHOENIX library using BP/RP
spectra (mhgspphotphoenix)
438- 442 F5.2 [-] b_[M/H]-Phx ? Lower confidence level (16%) of
iron abundance from GSP-Phot Aeneas
for PHOENIX library using BP/RP
spectra (mhgspphotphoenix_lower)
444- 448 F5.2 [-] B_[M/H]-Phx ? Upper confidence level (84%) of
iron abundance from GSP-Phot Aeneas
for PHOENIX library using BP/RP
spectra (mhgspphotphoenix_upper)
450- 459 F10.4 pc Dist-Phx ? Distance from GSP-Phot Aeneas for
PHOENIX library using BP/RP spectra
(distancegspphotphoenix)
461- 470 F10.4 pc b_Dist-Phx ? Lower confidence level (16%) of
distance from GSP-Phot Aeneas for
PHOENIX library using BP/RP spectra
(distancegspphotphoenix_lower)
472- 481 F10.4 pc B_Dist-Phx ? Upper confidence level (84%) of
distance from GSP-Phot Aeneas for
PHOENIX library using BP/RP spectra
(distancegspphotphoenix_upper)
483- 489 F7.4 mag A0Phoenix ? Monochromatic extinction A_0 at
547.7nm from GSP-Phot Aeneas for
PHOENIX library using BP/RP
spectra (azerogspphotphoenix)
491- 496 F6.4 mag b_A0Phoenix ? Lower confidence level (16%) of
monochromatic extinction A_0 at
547.7nm from GSP-Phot Aeneas for
PHOENIX library using BP/RP spectra
(azerogspphotphoenix_lower)
498- 504 F7.4 mag B_A0Phoenix ? Upper confidence level (84%) of
monochromatic extinction A_0 at
547.7nm from GSP-Phot Aeneas for
PHOENIX library using BP/RP spectra
(azerogspphotphoenix_upper)
506- 511 F6.4 mag AG-Phx ? Extinction in G band from GSP-Phot
Aeneas for PHOENIX library using
BP/RP spectra (aggspphotphoenix)
513- 518 F6.4 mag b_AG-Phx ? Lower confidence level (16%) of
extinction in G band from GSP-Phot
Aeneas for PHOENIX library using
BP/RP spectra
(aggspphotphoenix_lower)
520- 525 F6.4 mag B_AG-Phx ? Upper confidence level (84%) of
extinction in G band from GSP-Phot
Aeneas for PHOENIX library using
BP/RP spectra
(aggspphotphoenix_upper)
527- 532 F6.4 mag ABP-Phx ? Extinction in G_BP band from
GSP-Phot Aeneas for PHOENIX library
using BP/RP spectra
(abpgspphotphoenix)
534- 539 F6.4 mag b_ABP-Phx ? Lower confidence level (16%) of
extinction in G_BP band from
GSP-Phot Aeneas for PHOENIX library
using BP/RP spectra
(abpgspphotphoenix_lower)
541- 546 F6.4 mag B_ABP-Phx ? Upper confidence level (84%) of
extinction in G_BP band from
GSP-Phot Aeneas for PHOENIX library
using BP/RP spectra
(abpgspphotphoenix_upper)
548- 553 F6.4 mag ARP-Phx ? Extinction in G_RP band from
GSP-Phot Aeneas for PHOENIX library
using BP/RP spectra
(arpgspphotphoenix)
555- 560 F6.4 mag b_ARP-Phx ? Lower confidence level (16%) of
extinction in G_RP band from
GSP-Phot Aeneas for PHOENIX library
using BP/RP spectra
(arpgspphotphoenix_lower)
562- 567 F6.4 mag B_ARP-Phx ? Upper confidence level (84%) of
extinction in G_RP band from
GSP-Phot Aeneas for PHOENIX library
using BP/RP spectra
(arpgspphotphoenix_upper)
569- 574 F6.4 mag E(BP-RP)-Phx ? Reddening E(BP-RP) from GSP-Phot
Aeneas for PHOENIX library using
BP/RP spectra
(ebpminrpgspphotphoenix)
576- 581 F6.4 mag b_E(BP-RP)-Phx ? Lower confidence level (16%) of
reddening E(BP-RP) from GSP-Phot
Aeneas for PHOENIX library using
BP/RP spectra
(ebpminrpgspphotphoenix_lower)
583- 588 F6.4 mag B_E(BP-RP)-Phx ? Upper confidence level (84%) of
reddening E(BP-RP) from GSP-Phot
Aeneas for PHOENIX library using
BP/RP spectra
(ebpminrpgspphotphoenix_upper)
590- 596 F7.4 mag GMAG-Phx ? Absolute magnitude M_G from
GSP-Phot Aeneas for PHOENIX library
using BP/RP spectra
(mggspphotphoenix)
598- 604 F7.4 mag b_GMAG-Phx ? Lower confidence level (16%) of
absolute magnitude M_G from
GSP-Phot Aeneas for PHOENIX library
using BP/RP spectra
(mggspphotphoenix_lower)
606- 612 F7.4 mag B_GMAG-Phx ? Upper confidence level (84%) of
absolute magnitude M_G from
GSP-Phot Aeneas for PHOENIX library
using BP/RP spectra
(mggspphotphoenix_upper)
614- 622 F9.4 Rsun Rad-Phx ? Radius from GSP-Phot Aeneas for
PHOENIX library using BP/RP spectra
(radiusgspphotphoenix)
624- 632 F9.4 Rsun b_Rad-Phx ? Lower confidence level (16%) of
radius from GSP-Phot Aeneas for
PHOENIX library using BP/RP spectra
(radiusgspphotphoenix_lower)
634- 642 F9.4 Rsun B_Rad-Phx ? Upper confidence level (84%) of
radius from GSP-Phot Aeneas for
PHOENIX library using BP/RP spectra
(radiusgspphotphoenix_upper)
644- 656 F13.4 --- logpost-Phx ? Goodness-of-fit score (mean
log-posterior of MCMC) of GSP-Phot
Aeneas MCMC for PHOENIX library
(logposteriorgspphotphoenix)
658- 666 F9.7 --- Accp-Phx ? MCMC acceptance rate of GSP-Phot
Aeneas MCMC for PHOENIX library
(mcmcacceptgspphotphoenix)
668- 677 F10.4 K Teff-OB ? Effective temperature from GSP-Phot
Aeneas for OB library using BP/RP
spectra (teffgspphotob)
679- 688 F10.4 K b_Teff-OB ? Lower confidence level (16%) of
effective temperature from GSP-Phot
Aeneas for OB library using BP/RP
spectra (teffgspphotob_lower)
690- 699 F10.4 K B_Teff-OB ? Upper confidence level (84%) of
effective temperature from GSP-Phot
Aeneas for OB library using BP/RP
spectra (teffgspphotob_upper)
701- 706 F6.4 [cm/s2] logg-OB ? Surface gravity from GSP-Phot
Aeneas for OB library using BP/RP
spectra (logggspphotob)
708- 713 F6.4 [cm/s2] b_logg-OB ? Lower confidence level (16%) of
surface gravity from GSP-Phot Aeneas
for OB library using BP/RP spectra
(logggspphotob_lower)
715- 720 F6.4 [cm/s2] B_logg-OB ? Upper confidence level (84%) of
surface gravity from GSP-Phot Aeneas
for OB library using BP/RP spectra
(logggspphotob_upper)
722- 728 F7.4 [-] [M/H]-OB ? Iron abundance from GSP-Phot Aeneas
for OB library using BP/RP spectra
(mhgspphotob)
730- 736 F7.4 [-] b_[M/H]-OB ? Lower confidence level (16%) of
iron abundance from GSP-Phot Aeneas
for OB library using BP/RP spectra
(mhgspphotob_lower)
738- 744 F7.4 [-] B_[M/H]-OB ? Upper confidence level (84%) of
iron abundance from GSP-Phot Aeneas
for OB library using BP/RP spectra
(mhgspphotob_upper)
746- 755 F10.4 pc Dist-OB ? Distance from GSP-Phot Aeneas for
OB library using BP/RP spectra
(distancegspphotob)
757- 766 F10.4 pc b_Dist-OB ? Lower confidence level (16%) of
distance from GSP-Phot Aeneas for OB
library using BP/RP spectra
(distancegspphotob_lower)
768- 777 F10.4 pc B_Dist-OB ? Upper confidence level (84%) of
distance from GSP-Phot Aeneas for OB
library using BP/RP spectra
(distancegspphotob_upper)
779- 785 F7.4 mag A0-OB ? Monochromatic extinction A_0 at
547.7nm from GSP-Phot Aeneas for OB
library using BP/RP spectra
(azerogspphotob)
787- 792 F6.4 mag b_A0-OB ? Lower confidence level (16%) of
monochromatic extinction A_0 at
547.7nm from GSP-Phot Aeneas for OB
library using BP/RP spectra
(azerogspphotob_lower)
794- 800 F7.4 mag B_A0-OB ? Upper confidence level (84%) of
monochromatic extinction A_0 at
547.7nm from GSP-Phot Aeneas for OB
library using BP/RP spectra
(azerogspphotob_upper)
802- 807 F6.4 mag AG-OB ? Extinction in G band from GSP-Phot
Aeneas for OB library using BP/RP
spectra (aggspphotob)
809- 814 F6.4 mag b_AG-OB ? Lower confidence level (16%) of
extinction in G band from GSP-Phot
Aeneas for OB library using BP/RP
spectra (aggspphotob_lower)
816- 821 F6.4 mag B_AG-OB ? Upper confidence level (84%) of
extinction in G band from GSP-Phot
Aeneas for OB library using BP/RP
spectra (aggspphotob_upper)
823- 828 F6.4 mag ABP-OB ? Extinction in G_BP band from
GSP-Phot Aeneas for OB library using
BP/RP spectra (abpgspphotob)
830- 835 F6.4 mag b_ABP-OB ? Lower confidence level (16%) of
extinction in G_BP band from
GSP-Phot Aeneas for OB library using
BP/RP spectra (abpgspphotob_lower)
837- 842 F6.4 mag B_ABP-OB ? Upper confidence level (84%) of
extinction in G_BP band from
GSP-Phot Aeneas for OB library using
BP/RP spectra (abpgspphotob_upper)
844- 849 F6.4 mag ARP-OB ? Extinction in G_RP band from
GSP-Phot Aeneas for OB library using
BP/RP spectra (arpgspphotob)
851- 856 F6.4 mag b_ARP-OB ? Lower confidence level (16%) of
extinction in G_RP band from
GSP-Phot Aeneas for OB library using
BP/RP spectra (arpgspphotob_lower)
858- 863 F6.4 mag B_ARP-OB ? Upper confidence level (84%) of
extinction in G_RP band from
GSP-Phot Aeneas for OB library using
BP/RP spectra (arpgspphotob_upper)
865- 870 F6.4 mag E(BP-RP)-OB ? Reddening E(BP-RP) from GSP-Phot
Aeneas for OB library using BP/RP
spectra (ebpminrpgspphotob)
872- 877 F6.4 mag b_E(BP-RP)-OB ? Lower confidence level (16%) of
reddening E(BP-RP) from GSP-Phot
Aeneas for OB library using BP/RP
spectra (ebpminrpgspphotob_lower)
879- 884 F6.4 mag B_E(BP-RP)-OB ? Upper confidence level (84%) of
reddening E(BP-RP) from GSP-Phot
Aeneas for OB library using BP/RP
spectra (ebpminrpgspphotob_upper)
886- 892 F7.4 mag GMAG-OB ? Absolute magnitude M_G from
GSP-Phot Aeneas for OB library using
BP/RP spectra (mggspphotob)
894- 900 F7.4 mag b_GMAG-OB ? Lower confidence level (16%) of
absolute magnitude M_G from GSP-Phot
Aeneas for OB library using BP/RP
spectra (mggspphotob_lower)
902- 908 F7.4 mag B_GMAG-OB ? Upper confidence level (84%) of
absolute magnitude M_G from GSP-Phot
Aeneas for OB library using BP/RP
spectra (mggspphotob_upper)
910- 917 F8.4 Rsun Rad-OB ? Radius from GSP-Phot Aeneas for OB
library using BP/RP spectra
(radiusgspphotob)
919- 926 F8.4 Rsun b_Rad-OB ? Lower confidence level (16%) of
radius from GSP-Phot Aeneas for OB
library using BP/RP spectra
(radiusgspphotob_lower)
928- 935 F8.4 Rsun B_Rad-OB ? Upper confidence level (84%) of
radius from GSP-Phot Aeneas for OB
library using BP/RP spectra
(radiusgspphotob_upper)
937- 950 E14.7 --- logpost-OB ? Goodness-of-fit score (mean
log-posterior of MCMC) of GSP-Phot
Aeneas MCMC for OB library
(logposteriorgspphotob)
952- 960 F9.7 --- Accp-OB ? MCMC acceptance rate of GSP-Phot
Aeneas MCMC for OB library
(mcmcacceptgspphotob)
962- 971 F10.4 K Teff-A ? Effective temperature from GSP-Phot
Aeneas for A library using BP/RP
spectra (teffgspphota)
973- 982 F10.4 K b_Teff-A ? Lower confidence level (16%) of
effective temperature from GSP-Phot
Aeneas for A library using BP/RP
spectra (teffgspphota_lower)
984- 993 F10.4 K B_Teff-A ? Upper confidence level (84%) of
effective temperature from GSP-Phot
Aeneas for A library using BP/RP
spectra (teffgspphota_upper)
995-1000 F6.4 [cm/s2] logg-A ? Surface gravity from GSP-Phot
Aeneas for A library using BP/RP
spectra (logggspphota)
1002-1007 F6.4 [cm/s2] b_logg-A ? Lower confidence level (16%) of
surface gravity from GSP-Phot Aeneas
for A library using BP/RP spectra
(logggspphota_lower)
1009-1014 F6.4 [cm/s2] B_logg-A ? Upper confidence level (84%) of
surface gravity from GSP-Phot Aeneas
for A library using BP/RP spectra
(logggspphota_upper)
1016-1022 F7.4 [-] [M/H]-A ? Iron abundance from GSP-Phot Aeneas
for A library using BP/RP spectra
(mhgspphota)
1024-1030 F7.4 [-] b_[M/H]-A ? Lower confidence level (16%) of
iron abundance from GSP-Phot Aeneas
for A library using BP/RP spectra
(mhgspphota_lower)
1032-1038 F7.4 [-] B_[M/H]-A ? Upper confidence level (84%) of
iron abundance from GSP-Phot Aeneas
for A library using BP/RP spectra
(mhgspphota_upper)
1040-1049 F10.4 pc Dist-A ? Distance from GSP-Phot Aeneas for
A library using BP/RP spectra
(distancegspphota)
1051-1060 F10.4 pc b_Dist-A ? Lower confidence level (16%) of
distance from GSP-Phot Aeneas for A
library using BP/RP spectra
(distancegspphota_lower)
1062-1071 F10.4 pc B_Dist-A ? Upper confidence level (84%) of
distance from GSP-Phot Aeneas for A
library using BP/RP spectra
(distancegspphota_upper)
1073-1079 F7.4 mag A0-A ? Monochromatic extinction A_0 at
547.7nm from GSP-Phot Aeneas for A
library using BP/RP spectra
(azerogspphota)
1081-1086 F6.4 mag b_A0-A ? Lower confidence level (16%) of
monochromatic extinction A_0 at
547.7nm from GSP-Phot Aeneas for A
library using BP/RP spectra
(azerogspphota_lower)
1088-1094 F7.4 mag B_A0-A ? Upper confidence level (84%) of
monochromatic extinction A_0 at
547.7nm from GSP-Phot Aeneas for A
library using BP/RP spectra
(azerogspphota_upper)
1096-1101 F6.4 mag AG-A ? Extinction in G band from GSP-Phot
Aeneas for A library using BP/RP
spectra (aggspphota)
1103-1108 F6.4 mag b_AG-A ? Lower confidence level (16%) of
extinction in G band from GSP-Phot
Aeneas for A library using BP/RP
spectra (aggspphota_lower)
1110-1115 F6.4 mag B_AG-A ? Upper confidence level (84%) of
extinction in G band from GSP-Phot
Aeneas for A library using BP/RP
spectra (aggspphota_upper)
1117-1122 F6.4 mag ABP-A ? Extinction in G_BP band from
GSP-Phot Aeneas for A library using
BP/RP spectra (abpgspphota)
1124-1129 F6.4 mag b_ABP-A ? Lower confidence level (16%) of
extinction in G_BP band from
GSP-Phot Aeneas for A library using
BP/RP spectra (abpgspphota_lower)
1131-1136 F6.4 mag B_ABP-A ? Upper confidence level (84%) of
extinction in G_BP band from
GSP-Phot Aeneas for A library using
BP/RP spectra (abpgspphota_upper)
1138-1143 F6.4 mag ARP-A ? Extinction in G_RP band from
GSP-Phot Aeneas for A library using
BP/RP spectra (arpgspphota)
1145-1150 F6.4 mag b_ARP-A ? Lower confidence level (16%) of
extinction in G_RP band from
GSP-Phot Aeneas for A library using
BP/RP spectra (arpgspphota_lower)
1152-1157 F6.4 mag B_ARP-A ? Upper confidence level (84%) of
extinction in G_RP band from
GSP-Phot Aeneas for A library using
BP/RP spectra (arpgspphota_upper)
1159-1164 F6.4 mag E(BP-RP)-A ? Reddening E(BP-RP) from GSP-Phot
Aeneas for A library using BP/RP
spectra (ebpminrpgspphota)
1166-1171 F6.4 mag b_E(BP-RP)-A ? Lower confidence level (16%) of
reddening E(BP-RP) from GSP-Phot
Aeneas for A library using BP/RP
spectra (ebpminrpgspphota_lower)
1173-1178 F6.4 mag B_E(BP-RP)-A ? Upper confidence level (84%) of
reddening E(BP-RP) from GSP-Phot
Aeneas for A library using BP/RP
spectra (ebpminrpgspphota_upper)
1180-1186 F7.4 mag GMAG-A ? Absolute magnitude M_G from
GSP-Phot Aeneas for A library using
BP/RP spectra (mggspphota)
1188-1194 F7.4 mag b_GMAG-A ? Lower confidence level (16%) of
absolute magnitude M_G from GSP-Phot
Aeneas for A library using BP/RP
spectra (mggspphota_lower)
1196-1202 F7.4 mag B_GMAG-A ? Upper confidence level (84%) of
absolute magnitude M_G from GSP-Phot
Aeneas for A library using BP/RP
spectra (mggspphota_upper)
1204-1210 F7.4 Rsun Rad-A ? Radius from GSP-Phot Aeneas for A
library using BP/RP spectra
(radiusgspphota)
1212-1218 F7.4 Rsun b_Rad-A ? Lower confidence level (16%) of
radius from GSP-Phot Aeneas for A
library using BP/RP spectra
(radiusgspphota_lower)
1220-1226 F7.4 Rsun B_Rad-A ? Upper confidence level (84%) of
radius from GSP-Phot Aeneas for A
library using BP/RP spectra
(radiusgspphota_upper)
1228-1241 E14.7 --- logpost-A ? Goodness-of-fit score (mean
log-posterior of MCMC) of GSP-Phot
Aeneas MCMC for A library
(logposteriorgspphota)
1243-1251 F9.7 --- Accp-A ? MCMC acceptance rate of GSP-Phot
Aeneas MCMC for A library
(mcmcacceptgspphota)
1253-1258 F6.1 K Teff-ANN ? Effective temperature from GSP-Spec
ANN using RVS spectra and Monte
Carlo realisations
(teffgspspecann)
1260-1265 F6.1 K b_Teff-ANN ? Lower confidence level (16%) of
effective temperature from GSP-Spec
ANN using RVS spectra and Monte
Carlo realisations
(teffgspspecann_lower)
1267-1272 F6.1 K B_Teff-ANN ? Upper confidence level (84%) of
effective temperature from GSP-Spec
ANN using RVS spectra and Monte
Carlo realisations
(teffgspspecann_upper)
1274-1278 F5.2 [cm/s2] logg-ANN ? Surface gravity from GSP-Spec ANN
using RVS spectra and Monte Carlo
realisations (logggspspecann)
1280-1284 F5.2 [cm/s2] b_logg-ANN ? Lower confidence level (16%) of
surface gravity from GSP-Spec ANN
using RVS spectra and Monte Carlo
realisations
(logggspspecann_lower)
1286-1290 F5.2 [cm/s2] B_logg-ANN ? Upper confidence level (84%) of
surface gravity from GSP-Spec ANN
using RVS spectra and Monte Carlo
realisations
(logggspspecann_upper)
1292-1296 F5.2 [-] [M/H]-ANN ? Global metallicity from GSP-Spec
ANN using RVS spectra and Monte
Carlo realisations (mhgspspecann)
1298-1302 F5.2 [-] b_[M/H]-ANN ? Lower confidence level (16%) of
global metallicity from GSP-Spec ANN
using RVS spectra and Monte Carlo
realisations (mhgspspecann_lower)
1304-1308 F5.2 [-] B_[M/H]-ANN ? Upper confidence level (84%) of
global metallicity from GSP-Spec ANN
using RVS spectra and Monte Carlo
realisations (mhgspspecann_upper)
1310-1314 F5.2 [-] [alpha/Fe]-ANN ? Abundance of alpha-elements with
respect to iron from GSP-Spec ANN
using RVS spectra and Monte Carlo
realisations (alphafegspspecann)
1316-1320 F5.2 [-] b_[alpha/Fe]-ANN ? Lower confidence level (16%) of
alpha-elements with respect to iron
from GSP-Spec ANN using RVS spectra
and Monte Carlo realisations
(alphafegspspecann_lower)
1322-1326 F5.2 [-] B_[alpha/Fe]-ANN ? Upper confidence level (84%) of
alpha-elements with respect to iron
from GSP-Spec ANN using RVS spectra
and Monte Carlo realisations
(alphafegspspecann_upper)
1328-1338 F11.8 --- logpost-ANN ? Logarithm of the goodness-of-fit
for the GSP-Spec ANN parameters
(logchisqgspspecann)
1340-1351 I12 --- Flags-ANN ? Catalogue flags for GSP-Spec ANN
(flagsgspspecann) (1)
1353-1365 F13.9 Rsun Rad-Flame ? Radius of the star from FLAME using
teffGspspec and lumFlameSpec
(radiusflamespec)
1367-1379 F13.9 Rsun b_Rad-Flame ? Lower confidence level (16%) of
radiusFlameSpec
(radiusflamespec_lower)
1381-1393 F13.9 Rsun B_Rad-Flame ? Upper confidence level (84%) of
radiusFlameSpec
(radiusflamespec_upper)
1395-1403 F9.4 Lsun Lum-Flame ? Luminosity of the star from FLAME
using G band magnitude
(lumflamespec)
1405-1413 F9.4 Lsun b_Lum-Flame ? Lower confidence level (16%) of
lumFlameSpec (lumflamespec_lower)
1415-1424 F10.4 Lsun B_Lum-Flame ? Upper confidence level (84%) of
lumFlameSpec (lumflamespec_upper)
1426-1435 F10.8 Msun Mass-Flame ? Mass of the star from FLAME using
stellar models (massflamespec)
1437-1446 F10.8 Msun b_Mass-Flame ? Lower confidence level (16%) of
massFlameSpec
(massflamespec_lower)
1448-1457 F10.8 Msun B_Mass-Flame ? Upper confidence level (84%) of
massFlameSpec
(massflamespec_upper)
1459-1469 F11.8 Gyr Age-Flame ? Age of the star from FLAME using
stellar models (ageflamespec)
1471-1481 F11.8 Gyr b_Age-Flame ? Lower confidence level (16%) of
ageFlameSpec (ageflamespec_lower)
1483-1493 F11.8 Gyr B_Age-Flame ? Upper confidence level (84%) of
ageFlameSpec (ageflamespec_upper)
1495 I1 --- Flag-Flame [0/2]? Flag indicating quality of
parameters from FLAME using GSP-Spec
parameters (flagsflamespec) (2)
1497-1500 I4 --- Evol ? Evolutionary stage of the star from
FLAME using stellar models
(evolstageflamespec)
1502-1512 F11.8 km/s z-Flame ? Gravitational redshift from FLAME
using GSP-Spec parameters
(gravredshiftflamespec)
1514-1524 F11.8 km/s b_z-Flame ? Lower confidence interval of
gravredshiftFlameSpec
(gravredshiftflamespec_lower)
1526-1538 F13.8 km/s B_z-Flame ? Upper confidence interval of
gravredshiftFlameSpec
(gravredshiftflamespec_upper)
1540-1549 F10.7 mag BolCorr ? Bolometric correction applied to
derive lumFlameSpec using GSP-Spec
parameters (bcflamespec)
--------------------------------------------------------------------------------
Note (1): Catalogue flags for GSP-Spec ANN (Recio-Blanco 2022, in prep.), used
to indicate the quality of the estimated parameters of this source.
In this chain, value 0 represents the best quality, and 9 the worst
Note (2): This field contains the quality flag for the data products from FLAME
derived using GSP-Spec parameters and consists of one digit A. It refers to
the quality of the mass and age determination (A = 0, 1, 2), and the
following is adopted:
A=0 nothing to report
A=1 the star is a giant and the mass and age should be considered with an
uncertainty on the order of 20% - 30%
A=2 the mass and age are not available
We note that while the evolstage flamespecparameter is related to mass and
age, this flag is not applicable to this parameter.
--------------------------------------------------------------------------------
Byte-by-byte Description of file: tgextmap.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 19 I19 --- SolID Solution Identifier (solution_id)
21- 27 I7 --- HPId Unique HEALPix index number for which the
total Galactic extinction parameters are
estimated (healpix_id)
29 I1 --- HPlevel [6/9] HEALPix level used (healpix_level) n
31- 36 F6.4 mag A0 ? Mean A0 extinction parameter (a0) (1)
38- 43 F6.4 mag e_A0 ? Uncertainty for the mean A0
(a0_uncertainty)
45- 50 F6.4 mag b_A0 ? Minimum A0 value used for the HEALPix
of interest (a0_min)
53- 59 F7.4 mag B_A0 ? Maximum A0 value used for the HEALPix
of interest (a0_max)
62- 66 I5 --- Ntracers Number of tracers used (numtracersused)
68 I1 --- foptHP [0/1] Flag to indicate whether a given HEALPix
level is the optimum (1) or not (0)
(optimumhpxflag) (2)
70 I1 --- Status [0/3] Exit status for TGE (status) (3)
--------------------------------------------------------------------------------
Note (1): median A0 of the selected extinction tracers (giants) as estimated
by GSP-Phot from BP/RP spectra, apparent G magnitude and parallax
(i.e. azeroGspphot in table gaiadr3.dat). A0 is the extinction parameter in
the adopted Fitzpatrick extinction law (Fitzpatrick, 1999PASP..111...63F 1999PASP..111...63F),
taken as the monochromatic extinction at 547.7nm.
Note (2): The Total Galactic Extinction maps are provided at four different
HEALPix levels (i.e. 4 different resolutions, levels 6 through 9). This flag
indicates whether a given HEALPix level is the optimum level (0),
or not (1).
Note (3): Exit status for TGE as follows:
0 = Nominal processing.
1 = Insufficient number of tracers, after validation of input for each
source (Step 0).
2 = Insufficient number of tracers, after (Teff, MG) selection (Step 1)
3 = Insufficient number of tracers, after check on the distance (Step 2)
4 = Insufficient number of tracers, after outlier rejection (Step 3)
5 = Insufficient number of tracers, after rejection of tracers with large A0
errors (Step 4).
99 = Unknown error flag
--------------------------------------------------------------------------------
Byte-by-byte Description of file: tgextopt.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 19 I19 --- SolID Solution Identifier (solution_id)
21- 27 I7 --- HPId Unique HEALPix index number for which the
total Galactic extinction parameters are
estimated (healpix_id)
29- 34 F6.4 mag A0 ?=- Median A0 extinction parameter (a0) (1)
36- 41 F6.4 mag e_A0 ?=- Uncertainty for the mean A0
(a0_uncertainty)
43- 45 I3 --- Ntracers Number of tracers used (numtracersused)
47 I1 --- Status [0/3] Exit status for TGE (status) (2)
49 I1 --- HPlevel [6/9] Number indicating which HEALPix level
was chosen to populate this HEALPix
(optimumhpxlevel)
--------------------------------------------------------------------------------
Note (1): median A0 of the selected extinction tracers (giants) as estimated
by GSP-Phot from BP/RP spectra, apparent G magnitude and parallax
(i.e. azeroGspphot in table gaiadr3.dat). A0 is the extinction parameter in
the adopted Fitzpatrick extinction law (Fitzpatrick, 1999PASP..111...63F 1999PASP..111...63F),
taken as the monochromatic extinction at 547.7nm.
Note (2): Exit status for TGE as follows:
0 = Nominal processing.
1 = Insufficient number of tracers, after validation of input for each
source (Step 0).
2 = Insufficient number of tracers, after (Teff, MG) selection (Step 1)
3 = Insufficient number of tracers, after check on the distance (Step 2)
--------------------------------------------------------------------------------
Byte-by-byte Description of file: oaninfo.dat
--------------------------------------------------------------------------------
Bytes Format Unit s Label Explanations
--------------------------------------------------------------------------------
1- 19 I19 --- SolID Solution Identifier (solution_id)
21- 38 I18 --- SOMID Self-Organized Map identifier (som_id)
40- 57 I18 --- NeuId Neuron identifier (neuron_id)
59- 60 I2 --- NeuRowIdx [0/29] Row index of the neuron in the
Self-Organised Map lattice
(neuronrowindex)
62- 63 I2 --- NeuColIdx [0/29] Column index of the neuron in the
Self-Organised Map lattice
(neuroncolumnindex)
65- 70 I6 --- hits Number of sources populating the neuron
(hits)
72- 82 A11 --- Class ? Astronomical class estimated for the
neuron (class_label)
84-102 I19 --- CentId Identifier of the Gaia source that minimizes
the classification distance to the neuron
(centroid_id)
104-116 E13.8 --- CentDist Squared Euclidean distance between the
centroid XP spectrum and the neuron XP
prototype (centroid_distance)
118-130 E13.8 --- TempDist ? Squared Euclidean distance between the
reference XP template and the neuron XP
prototype (template_distance)
132-140 F9.6 mag Gmag Mean G value for the sources that belong to
the neuron (gmagmean)
142-151 F10.8 mag s_Gmag Standard deviation of G values for the
sources that belong to the neuron
(gmagstd_dev)
153-163 F11.7 mag b_Gmag Minimum G value for the sources that belong
to the neuron (gmagmin)
165-173 F9.6 mag B_Gmag Maximum G value for the sources that belong
to the neuron (gmagmax)
175-183 F9.6 mag BPmag Mean GBP value for the sources that belong
to the neuron (bpmagmean)
185-194 F10.8 mag s_BPmag Standard deviation of GBP values for the
sources that belong to the neuron
(bpmagstd_dev)
196-205 F10.7 mag b_BPmag Minimum value of GBP for the sources that
belong to the neuron (bpmagmin)
207-215 F9.6 mag B_BPmag Maximum value of GBP for the sources that
belong to the neuron (bpmagmax)
217-226 F10.7 mag RPmag Mean GRP value for the sources that belong
to the neuron neuron (rpmagmean)
228-237 F10.8 mag s_RPmag Standard deviation of GRP values for the
sources that belong to the neuron
(rpmagstd_dev)
239-248 F10.7 mag b_RPmag Minimum value of GRP for the sources that
belong to the neuron (rpmagmin)
250-258 F9.6 mag B_RPmag Maximum value of GRP for the sources that
belong to the neuron (rpmagmax)
260-273 F14.10 mas/yr pmRA Mean value of the proper motion in right
ascension for the sources that belong to the
neuron (pmramean)
275-285 F11.7 mas/yr s_pmRA Standard deviation of the proper motion in
right ascension for the sources that belong
to the neuron (pmrastd_dev)
287-297 F11.5 mas/yr b_pmRA Minimum value of the proper motion in right
ascension for the sources that belong to the
neuron (pmramin)
299-308 F10.5 mas/yr B_pmRA Maximum value of the proper motion in right
ascension for the sources that belong to the
neuron (pmramax)
310-322 E13.7 mas/yr pmDE Mean value of the proper motion in
declination for the sources that belong to
the neuron (pmdecmean)
324-334 F11.7 mas/yr s_pmDE Standard deviation of the proper motion in
declination for the sources that belong to
the neuron (pmdecstd_dev)
336-346 F11.5 mas/yr b_pmDE Minimum value of the proper motion in
declination for the sources that belong to
the neuron (pmdecmin)
348-359 F12.6 mas/yr B_pmDE Maximum value of the proper motion in
declination for the sources that belong to
the neuron (pmdecmax)
361-373 E13.7 mas Plx Mean parallax value for the sources that
belong to the neuron (parallax_mean)
375-384 F10.8 mas s_Plx Standard deviation of the parallax values for
the sources that belong to the neuron
(parallaxstddev)
386-396 F11.7 mas b_Plx Minimum parallax value for the sources that
belong to the neuron (parallax_min)
398-408 F11.7 mas B_Plx Maximum parallax value for the sources that
belong to the neuron (parallax_max)
410-423 F14.10 deg GLON [] Mean galactic latitude for the sources
that belong to the neuron
(gallatitudemean)
425-434 F10.7 deg s_GLON Standard deviation of the galactic latitude
values for the sources that belong to the
neuron (gallatitudestd_dev)
436-445 F10.6 deg b_GLON Minimum galactic latitude for the sources
that belong to the neuron (gallatitudemin)
447-455 F9.6 deg B_GLON Maximum galactic latitude for the sources
that belong to the neuron (gallatitudemax)
457-468 E12.7 --- intraDist Mean value of the squared Euclidean distance
between each of the XP sources in the
neuron and the neuron prototype
(intraneurondistance_mean)
470-481 E12.7 --- s_intraDist Standard deviation of the squared Euclidean
distance between each of the XP sources in
the neuron and the neuron prototype
(intraneurondistancestddev)
483-495 E13.8 --- b_intraDist Minimum squared Euclidean distance between
each of the XP sources in the neuron and the
neuron prototype (intraneurondistance_min)
497-508 F12.10 --- B_intraDist Maximum squared Euclidean distance between
each of the XP sources in the neuron and the
neuron prototype (intraneurondistance_max)
510-522 E13.8 --- interDist Mean value of the squared Euclidean distance
between the neuron XP prototype and the XP
prototypes of its immediate neighbours
(interneurondistance_mean)
524-536 E13.8 --- s_interDist Standard deviation of the squared Euclidean
distance between the neuron XP prototype and
the XP prototypes of its immediate
neighbours (interneurondistancestddev)
538-550 E13.8 --- b_interDist Minimum value of the squared Euclidean
distance between the neuron XP prototype and
the XP prototypes of its immediate
neighbours (interneurondistance_min)
552-563 E12.7 --- B_interDist Maximum value of the squared Euclidean
distance between the neuron XP prototype and
the XP prototypes of its immediate
neighbours (interneurondistance_max)
565-578 A14 --- Template Name of the template used to describe the
neuron (template_name)
580-591 E12.7 --- dist25 25th percentile value for the intra-neuron
distance distribution
(distance_percentile25)
593-605 E13.8 --- dist50 50th percentile value for the intra-neuron
distance distribution
(distance_percentile50)
607-619 E13.8 --- dist68 68th percentile value for the intra-neuron
distance distribution
(distance_percentile68)
621-633 E13.8 --- dist75 75th percentile value for the intra-neuron
distance distribution
(distance_percentile75)
635-647 E13.8 --- dist99 95th percentile value for the intra-neuron
distance distribution
(distance_percentile95)
649-661 E13.8 --- distFWHM Full Width at Half Maximum value for the
intra-neuron distance distribution
(distance_fwhm)
663-673 F11.8 --- distSkew Skewness value for the intra-neuron distance
distribution (distance_skew)
675-690 F16.10 --- distKur Kurtosis value for the intra-neuron distance
distribution (distance_kurtosis)
692-704 E13.8 --- distiqr Inter-Quartile Range value for the
intra-neuron distance distribution
(distanceiq_r)
706-717 E12.7 --- distFWHMn Normalized FWHM value for the intra-neuron
distance distribution (distancefwhmnorm)
719 I1 --- Quality [0/6] Quality category assigned to the
neuron (quality_category)
721-730 F10.7 --- NBP Mean value of the number of BP transits for
the sources that belong to the neuron
(bptransitsmean)
732-742 F11.8 --- s_NBP Standard deviation of the number of BP
transits for the sources that belong to the
neuron (bptransitsstd_dev)
744-746 F3.1 --- b_NBP Minimum value of the number of BP transits
for the sources that belong to the neuron
(bptransitsmin)
748-752 F5.1 --- B_NBP Maximum value of the number of BP transits
for the sources that belong to the neuron
(bptransitsmax)
754-763 F10.7 --- NRP Mean value of the number of RP transits for
the sources that belong to the neuron
(rptransitsmean)
765-775 F11.8 --- s_NRP Standard deviation of the number of RP
transits for the sources that belong to the
neuron (rptransitsstd_dev)
777-779 F3.1 --- b_NRP Minimum value of the number of RP transits
for the sources that belong to the neuron
(rptransitsmin)
781-785 F5.1 --- B_NRP Maximum value of the number of RP transits
for the sources that belong to the neuron
(rptransitsmax)
787-795 F9.7 --- RUWE Mean value of the renormalised unit weight
error for the sources that belong to the
neuron (ruwe_mean)
797-807 F11.9 --- s_RUWE Standard deviation of the renormalised unit
weight error for the sources that belong to
the neuron (ruwestddev)
809-818 F10.8 --- b_RUWE Minimum value of the renormalised unit weight
error for the sources that belong to the
neuron (ruwe_min)
820-829 F10.7 --- B_RUWE Maximum value of the renormalised unit weight
error for the sources that belong to the
neuron (ruwe_max)
831-840 F10.7 --- E(BP/RP) Mean value of the BP/RP flux excess for the
sources that belong to the neuron
(bprpmeanfluxexcessmean)
842-853 F12.8 --- s_E(BP/RP) Standard deviation of the BP/RP flux excess
for the sources that belong to the neuron
(bprpmeanfluxexcessstd_dev)
855-863 F9.7 --- b_E(BP/RP) Minimum value of the BP/RP flux excess for
the sources that belong to the neuron
(bprpmeanfluxexcessmin)
865-876 F12.6 --- B_E(BP/RP) Maximum value of the BP/RP flux excess for
the sources that belong to the neuron
(bprpmeanfluxexcessmax)
878-889 F12.9 mag BP-RP Mean value of the GBP-GRP colour for the
sources that belong to the neuron
(bprpcolourmean)
891-901 F11.9 mag s_BP-RP Standard deviation of the GBP-GRP colour
for the sources that belong to the neuron
(bprpcolourstd_dev)
903-914 F12.9 mag b_BP-RP Minimum value of the GBP-GRP colour for
the sources that belong to the neuron
(bprpcolourmin)
916-925 F10.7 mag B_BP-RP Maximum value of the GBP-GRP colour for
the sources that belong to the neuron
(bprpcolourmax)
--------------------------------------------------------------------------------
Byte-by-byte Description of file: oaxpsp.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 19 I19 --- SolID Solution Identifier (solution_id)
21- 38 I18 --- NeuId Neuron identifier (neuron_id)
40- 41 I2 --- NeuRowIdx [0/29] Row index of the neuron in the
Self-Organised Map lattice
(neuronrowindex)
43- 44 I2 --- NeuColIdx [0/29] Column index of the neuron in the
Self-Organised Map lattice
(neuroncolumnindex)
46- 57 E12.7 --- XPFlux Normalised flux at wavelength XPlambda for
the preprocessed XP spectrum that best
represents the neuron (prototype)
(xpspectrumprototype_flux)
59- 67 F9.4 nm XPlambda Wavelength associated with the XP spectrum
flux values
(xpspectrumprototype_wavelength)
69- 81 E13.8 --- XPFluxTemp ? Normalised flux at wavelength XPlambda for
the preprocessed XP spectrum corresponding
to the neuron template
(xpspectrumtemplate_flux)
--------------------------------------------------------------------------------
Byte-by-byte Description of file: epphot.sam
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 19 I19 --- Source Unique source identifier (unique within a
particular Data Release) (source_id)
21- 35 F15.11 deg RAdeg Right ascension (ICRS) at Ep=2016.0 (ra)
37- 51 F15.11 deg DEdeg Declination (ICRS) at Ep=2016.0 (dec)
53- 69 I17 --- TransitID Transit unique identifier (transit_id)
71- 81 F11.6 d TimeG ? Transit averaged G band observing time
JD-2455197.5 (gtransittime)
83- 96 E14.8 e-/s FG ? Transit averaged G band flux
(gtransitflux)
98-111 E14.8 e-/s e_FG ? Transit averaged G band flux error
(gtransitflux_error)
113-131 E19.6 --- RFG ? Transit averaged G band flux divided by its
error (gtransitfluxovererror)
133-141 F9.6 mag Gmag ? Transit averaged G band Vega magnitude
(gtransitmag)
143 I1 --- NG [0-9] Number of CCD observations contributing
to transit averaged G band flux
(gtransitn_obs)
145-153 F9.4 d TimeBP ? BP CCD transit observing time JD-2455197.5
(bpobstime)
155-168 E14.8 e-/s FBP ? BP band flux (bp_flux)
170-183 E14.8 e-/s e_FBP ? BP band flux error (bpfluxerror)
185-196 E12.6 --- RFBP ? BP band flux divided by its error
(bpfluxover_error)
198-206 F9.6 mag BPmag ? BP band Vega magnitude (bp_mag)
208-216 F9.4 d TimeRP ? RP CCD transit observing time JD-2455197.5
(rpobstime)
218-231 E14.8 e-/s FRP ? RP band flux (rp_flux)
233-246 E14.8 e-/s e_FRP ? RP band flux error (rpfluxerror)
248-259 E12.6 --- RFRP ? RP band flux divided by its error
(rpfluxover_error)
261-269 F9.6 mag RPmag ? RP band Vega magnitude (rp_mag)
271 I1 --- noisyFlag [0/1] G band flux scatter larger than expected
by photometry processing (all CCDs
considered) (photometryflagnoisy_data)
273 I1 --- SMuFlag [0/1] SM transit unavailable by photometry
processing (photometryflagsm_unavailable)
275 I1 --- AF1uFlag [0/1] AF1 transit unavailable by photometry
processing (photometryflagaf1_unavailable)
277 I1 --- AF2uFlag [0/1] AF2 transit unavailable by photometry
processing (photometryflagaf2_unavailable)
279 I1 --- AF3uFlag [0/1] AF3 transit unavailable by photometry
processing (photometryflagaf3_unavailable)
281 I1 --- AF4uFlag [0/1] AF4 transit unavailable by photometry
processing (photometryflagaf4_unavailable)
283 I1 --- AF5uFlag [0/1] AF5 transit unavailable by photometry
processing (photometryflagaf5_unavailable)
285 I1 --- AF6uFlag [0/1] AF6 transit unavailable by photometry
processing (photometryflagaf6_unavailable)
287 I1 --- AF7uFlag [0/1] AF7 transit unavailable by photometry
processing (photometryflagaf7_unavailable)
289 I1 --- AF8uFlag [0/1] AF8 transit unavailable by photometry
processing (photometryflagaf8_unavailable)
291 I1 --- AF9uFlag [0/1] AF9 transit unavailable by photometry
processing (photometryflagaf9_unavailable)
293 I1 --- BPuFlag [0/1] BP transit unavailable by photometry
processing (photometryflagbp_unavailable)
295 I1 --- RPuFlag [0/1] RP transit unavailable by photometry
processing (photometryflagrp_unavailable)
297 I1 --- SMrFlag [1] SM transit rejected by photometry
processing (photometryflagsm_reject)
299 I1 --- AF1rFlag [0/1] AF1 transit rejected by photometry
processing (photometryflagaf1_reject)
301 I1 --- AF2rFlag [0/1] AF2 transit rejected by photometry
processing (photometryflagaf2_reject)
303 I1 --- AF3rFlag [0/1] AF3 transit rejected by photometry
processing (photometryflagaf3_reject)
305 I1 --- AF4rFlag [0/1] AF4 transit rejected by photometry
processing (photometryflagaf4_reject)
307 I1 --- AF5rFlag [0/1] AF5 transit rejected by photometry
processing (photometryflagaf5_reject)
309 I1 --- AF6rFlag [0/1] AF6 transit rejected by photometry
processing (photometryflagaf6_reject)
311 I1 --- AF7rFlag [0/1] AF7 transit rejected by photometry
processing (photometryflagaf7_reject)
313 I1 --- AF8rFlag [0/1] AF8 transit rejected by photometry
processing (photometryflagaf8_reject)
315 I1 --- AF9rFlag [0/1] AF9 transit rejected by photometry
processing (photometryflagaf9_reject)
317 I1 --- BPrFlag [0/1] BP transit rejected by photometry
processing (photometryflagbp_reject)
319 I1 --- RPrFlag [0/1] RP transit rejected by photometry
processing (photometryflagrp_reject)
321 I1 --- GrVFlag [0/1] Average G transit photometry rejected by
variability processing
(variabilityflagg_reject)
323 I1 --- BPrVFlag [0/1] BP transit photometry rejected by
variability processing
(variabilityflagbp_reject)
325 I1 --- RPrVFlag [0/1] RP transit photometry rejected by
variability processing
(variabilityflagrp_reject)
--------------------------------------------------------------------------------
Byte-by-byte Description of file: gcrf3xm.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 19 I19 --- SolID Solution Identifier (solution_id)
21- 39 I19 --- Source Gaia source identifier (source_id)
41 I1 --- ICRF3sx [0/1] The flag describing if the Gaia-CRF3
source was found in ICRF3 S/X (icrf3sx)
43 I1 --- ICRF3k [0/1] The flag describing if the Gaia-CRF3
source was found in ICRF3 K (icrf3k)
45 I1 --- ICRF3xka [0/1] The flag describing if the Gaia-CRF3
source was found in ICRF3 X/Ka (icrf3xka)
47- 67 A21 --- ICRFname The ICRF name of the source (icrf_name)
69- 76 A8 --- IERSname The IERS name of the source (iers_name)
78 I1 --- OCARS [0/1] The flag describing if the Gaia-CRF3
source was found in OCARS,
www.gaoran.ru/english/as/ac_vlbi/#OCARS
(ocars)
80- 89 A10 --- OCARSname The name for this source in OCARS
(ocars_name)
91 I1 --- AW15 [0/1] The flag describing if the Gaia-CRF3
source was found in allWISE,
SECREST et al., 2015ApJS..221...12S 2015ApJS..221...12S,
Cat. J/ApJS/221/12 (aw15)
93-111 A19 --- AW15name The name for this source in allWISE
(aw15_name)
113 I1 --- R90 [0/1] The flag describing if the Gaia-CRF3
source was found in the catalogue R90,
Assef at al., 2018ApJS..234...23A 2018ApJS..234...23A,
Cat. J/ApJS/234/32 (r90)
115-133 A19 --- R90name The name for this source in R90 (r90_name)
135 I1 --- M65 [0/1] The flag describing if the Gaia-CRF3
source was found in Milliquas v6.5 (m65)
137-161 A25 --- M65name The name for this source in Milliquas v6.5,
Flesch, Cat. VII/290 (m65_name)
163 I1 --- C75 [0/1] The flag describing if the Gaia-CRF3
source was found in the catalogue C75,
Assef at al., 2018ApJS..234...23A 2018ApJS..234...23A,
Cat. J/ApJS/234/32 (c75)
166-184 A19 --- C75name The name for this source in C75 (c75_name)
186 I1 --- DR14q [0/1] The flag describing if the Gaia-CRF3
source was found in the catalogue
SDSS DR14Q, Paris et al.,
2018A&A...613A..51P 2018A&A...613A..51P, Cat. VII/286 (dr14q)
188-205 A18 --- DR14qname The name for this source in SDSS DR14Q
(dr14q_name)
207 I1 --- LQAC5 [0/1] The flag describing if the Gaia-CRF3
source was found in LQAC-5, Souchay et al.,
2019A&A...624A.145S 2019A&A...624A.145S, Cat. J/A+A/624/A145
(lqac5)
209-224 A16 --- LQAC5name The name for this source in LQAC-5
(lqac5_name)
226 I1 --- LAMOST5 [0/1] The flag describing if the Gaia-CRF3
source was found in the LAMOST QSO
catalogue (lamost5)
228-246 A19 --- LAMOST5name The name for this source in the LAMOST QSO
catalogue, Luo et al., Cat. V/164
(lamost5_name)
248 I1 --- LQRF [0/1] The flag describing if the Gaia-CRF3
source was found in LQRF, Andrei et al.,
2009A&A...505..385A 2009A&A...505..385A, Cat. I/313 (lqrf)
250-255 I6 --- LQRFname ? The name for this source in LQRF
(lqrf_name)
257 I1 --- 2QZ [0/1] The flag describing if the Gaia-CRF3
source was found in 2QZ, Croom et al.,
2004MNRAS.349.1397C 2004MNRAS.349.1397C, Cat. VII/241 (cat2qz)
259-274 A16 --- 2QZname The name for this source in 2QZ
(cat2qz_name)
276 I1 --- BZCAT5 [0/1] The flag describing if the Gaia-CRF3
source was found in Roma-BZCAT,
Massaro et al., 2015Ap&SS.357...75M 2015Ap&SS.357...75M,
Cat. VII/274 (bzcat5)
278-292 A15 --- BZCAT5name The name for this source in Roma-BZCAT
(bzcat5_name)
294 I1 --- 2WHSPJ [0/1] The flag describing if the Gaia-CRF3
source was found in 2WHSPJ (cat2whspj)
296-310 A15 --- 2WHSPJname The name for this source in 2WHSPJ,
Chang et al., 2017A&A...598A..17C 2017A&A...598A..17C,
Cat. J/A+A/598/A17 (cat2whspj_name)
312 I1 --- ALMA19 [0/1] The flag describing if the Gaia-CRF3
source was found in the ALMA calibrator
catalogue, BONATO et al.,
2019MNRAS.485.1188B 2019MNRAS.485.1188B, Cat. J/MNRAS/485/1188
(alma19)
314-323 A10 --- ALMA19name The name for this source in the ALMA
calibrator catalogue (alma19_name)
325 I1 --- GUW [0/1] The flag describing if the Gaia-CRF3
source was found in Gaia-unWISE,
Su et al., 2019MNRAS.489.4741S 2019MNRAS.489.4741S (guw)
327-342 A16 --- GUWname The name for this source in Gaia-unWISE
(guw_name)
344 I1 --- B19 [0/1] The flag describing if the Gaia-CRF3
source was found in the Gaia DR2 quasar and
galaxy classification catalogue,
Bailer-Jones et al., 2019MNRAS.490.5615B 2019MNRAS.490.5615B,
Cat VII/285 (b19)
346-364 I19 --- B19name ? The name for this source in the Gaia DR2
quasar and galaxy classification catalogue
(b19_name)
--------------------------------------------------------------------------------
Byte-by-byte Description of file: rvsmean.sam
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 19 I19 --- Source Unique source identifier (unique within a
particular Data Release) (source_id)
21- 35 F15.11 deg RAdeg Right Ascension ICRS ar Ep=2016.0 (ra)
37- 51 F15.11 deg DEdeg Declination ICRS ar Ep=2016.0 (dec)
53- 55 I3 --- NTransit Number of combined transits
(combined_transits)
57- 59 I3 --- NcCCD Number of combined CCD spectra (combined_ccds)
61- 63 I3 --- NdCDD Number of deblended CCD spectra
(deblended_ccds)
65- 70 F6.2 nm lambda [846/870] Wavelength (wavelength) (1)
72- 81 F10.7 --- Flux ? Normalized flux (flux) (1)
83- 92 F10.7 --- e_Flux ? Uncertainties in Flux (flux_error) (1)
--------------------------------------------------------------------------------
Note (1): The spectra are in the rest frame, they are normalised
and their wavelength grid ranges from 846 to 870nm in steps of 0.01nm
(2401 elements).
--------------------------------------------------------------------------------
Byte-by-byte Description of file: xpsummary.sam
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 19 I19 --- Source Unique source identifier (unique within a
particular Data Release) (source_id)
21- 35 F15.11 deg RAdeg Right ascension (ICRS) at Ep=2016.0 (ra)
37- 51 F15.11 deg DEdeg Declination (ICRS) at Ep=2016.0 (dec)
53- 71 I19 --- SolID Solution Identifier (solution_id)
73- 74 I2 --- NBPbases ? Number of bases that are relevant for the
representation of this mean BP spectrum
(bpnrelevant_bases)
76- 83 F8.6 --- BPrelsh ? Measure of the relative shrinking of the
coefficient vector when truncation is
applied for the mean BP spectrum
(bprelativeshrinking)
85- 88 I4 --- NBP ? Number of measurements used for the BP
spectrum generation (bpnmeasurements)
90- 93 I4 --- NBPrej ? Number of rejected measurements in the BP
spectrum generation
(bpnrejected_measurements)
95-104 F10.6 e-/s/pix BPstddev ? Standard deviation for the BP spectrum
representation (bpstandarddeviation)
106-117 E12.6 --- BPchi2r ? Chi squared for the BP spectrum
representation (bpchisquared)
119-121 I3 --- NTransBP ? Number of transits contributing to the
mean in BP (bpntransits)
123-124 I2 --- NcTransBP ? Number of contaminated transits in BP
(bpncontaminated_transits)
126-128 I3 --- NbTransBP ? Number of blended transits in BP
(bpnblended_transits)
130-131 I2 --- NRPbases Number of bases that are relevant for the
representation of this mean RP spectrum
(rpnrelevant_bases)
133-140 F8.6 --- NRPrelsh Measure of the relative shrinking of the
coefficient vector when truncation is
applied for the mean RP spectrum
(rprelativeshrinking)
142-146 I5 --- NRP Number of measurements used for the RP
spectrum generation (rpnmeasurements)
148-151 I4 --- NRPrej Number of rejected measurements in the RP
spectrum generation
(rpnrejected_measurements)
153-161 F9.6 e-/s/pix RPstdev Standard deviation for the RP spectrum
representation (rpstandarddeviation)
163-174 E12.6 --- RPchi2r Chi squared for the RP spectrum
representation (rpchisquared)
176-178 I3 --- NTransRP Number of transits contributing to the mean
in RP (rpntransits)
180-182 I3 --- NcTransRP Number of contaminated transits in RP
(rpncontaminated_transits)
184-186 I3 --- NbTransRP Number of blended transits in RP
(rpnblended_transits)
--------------------------------------------------------------------------------
Byte-by-byte Description of file: xpsample.sam
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 19 I19 --- Source Unique source identifier (unique within a
particular Data Release) (source_id)
21- 35 F15.11 deg RAdeg Right Ascension (ICRS) at Ep=2016.0 (ra)
37- 51 F15.11 deg DEdeg Declination (ICRS) at Ep=2016.0 (dec)
53- 56 I4 --- lambda Wavelength (wavelength) (1)
58- 72 E15.8 W/m2/nm Flux Mean BP + RP combined spectrum flux (flux)
74- 87 E14.8 W/m2/nm e_Flux Mean BP + RP combined spectrum flux error
(flux_error)
--------------------------------------------------------------------------------
Note (1): 343 values from 336 to 1020nm with a step of 2nm.
--------------------------------------------------------------------------------
Byte-by-byte Description of file: xpsamp.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 19 I19 --- SolID Solution Identifier (solution_id)
21- 22 A2 --- Band [BP RP] BP or RP photometric band (band)
24- 29 F6.1 nm lambda Wavelength (wavelength) (1)
31- 32 I2 --- Func [0/54] Basis function index
(basis_function)
34- 56 E23.16 ph/s/m2/nm SampCoeff Sampling matrix coefficient
(sampling_coefficient)
--------------------------------------------------------------------------------
Note (1): 343 values from 336 to 1020nm with a step of 2nm.
--------------------------------------------------------------------------------
Byte-by-byte Description of file: xpmerge.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 19 I19 --- SolID Solution Identifier (solution_id)
21- 26 F6.1 nm lambda Wavelength (wavelength) (1)
28- 32 F5.3 --- weightBP BP flux weight (bp_weight)
34- 38 F5.3 --- weightRP RP flux weight (rp_weight)
--------------------------------------------------------------------------------
Note (1): 343 values from 336 to 1020nm with a step of 2nm.
--------------------------------------------------------------------------------
Byte-by-byte Description of file: xpcont.sam
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 19 I19 --- Source Unique source identifier (unique within
a particular Data Release) (source_id)
21- 35 F15.11 deg RAdeg Right ascension (ICRS) at Ep=2016.0 (ra)
37- 51 F15.11 deg DEdeg Declination (ICRS) at Ep=2016.0 (dec)
53- 71 I19 --- SolID Solution Identifier (solution_id)
73- 76 I4 --- BPDOF ? Degrees of freedom for the BP spectrum
representation (bpdegreesof_freedom)
78- 81 I4 --- NBP ? Number of measurements used for the BP
spectrum generation (bpnmeasurements)
83- 86 I4 --- BPNrej ? Number of rejected measurements in the
BP spectrum generation
(bpnrejected_measurements)
88-100 F13.9 --- BPstddev ? Standard deviation for the BP spectrum
representation (bpstandarddeviation)
102-114 E13.7 --- BPchi2r ? Chi squared for the BP spectrum
representation (bpchisquared)
116-117 I2 --- NBPbases ? Number of bases that are relevant for
the representation of this mean BP
spectrum (bpnrelevant_bases)
119-129 F11.9 --- BPrelsh ? Measure of the relative shrinking of
the coefficient vector when truncation
is applied for the mean BP spectrum
(bprelativeshrinking)
131-135 I5 --- RPDOF Degrees of freedom for the RP spectrum
representation (rpdegreesof_freedom)
137-141 I5 --- NRP Number of measurements used for the RP
spectrum generation (rpnmeasurements)
143-146 I4 --- RPNrej Number of rejected measurements in the
RP spectrum generation
(rpnrejected_measurements)
148-159 F12.9 --- RPstddev Standard deviation for the RP spectrum
representation (rpstandarddeviation)
161-173 E13.7 --- RPchi2r Chi squared for the RP spectrum
representation (rpchisquared)
175-176 I2 --- NRPbases Number of bases that are relevant for the
representation of this mean RP spectrum
(rpnrelevant_bases)
178-187 F10.8 --- RPrelsh Measure of the relative shrinking of the
coefficient vector when truncation is
applied for the mean RP spectrum
(rprelativeshrinking)
189-199 I11 --- BPrecnoS Starting record number in the separated
bpcoeff/ebp_coeff file (added by CDS)
(bpstartrecno)
201-202 I2 --- BPNelem [0/55] Number of elements in the
separated bpcoeff/ebp_coeff file
(always 55 except for 1 line)
(added by CDS) (bpnelems)
204-215 I12 --- BPcorrrecnoS Starting record number in the separated
bpcoeffcorr file (added by CDS)
(bpcorrstart_recno)
217-220 I4 --- BPcorrNelem [0/1485] Number of elements in the
separated bpcoeffcorr file
(added by CDS) (always 1485 except for
1 line) (bpcorrn_elems)
222-232 I11 --- RPrecnoS Starting record number in the separated
rpcoeff/erp_coeff file (added by CDS)
(rpstartrecno)
234-235 I2 --- RPNelem Number of elements in the separated
rpcoeff/erp_coeff file (always 55)
(rpnelems)
237-248 I12 --- RPcorrrecnoS Starting record number in the separated
rpcoeffcorr file (added by CDS)
(rpcorrstart_recno)
250-253 I4 --- RPcorrNelem [1485] Number of elements in the
separated rpcoeffcorr file
(added by CDS) (rpcorrn_elems)
--------------------------------------------------------------------------------
Byte-by-byte Description of file: spectra.sam
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 15 F15.11 deg RAdeg ? Right ascension (ICRS) at Ep=2016.0 (ra)
17- 31 F15.11 deg DEdeg ? Declination (ICRS) at Ep=2016.0 (dec)
33- 51 I19 --- Source Unique source identifier (unique within a
particular Data Release) (source_id)
--------------------------------------------------------------------------------
History:
13-Jun-2022: From Gaia team
14-Oct-2022: in paramp table, E(B-V) corrected into E(BP-RP),
for the parameter and the upper and lower limits
12-Dec-2024: units of angular distances between the gaia source and the
best neighbour source in the counterpart catalogues (HIP, PS1,
SDSS13, SKYM2, TYC2, URAT1, AllWISE, APASS9, GSC23, RAVE5,
2MASS, RAVE5, and RAVE6) in gaiadr3 corrected into arcsec.
Acknowledging Gaia/esa :
Acknowledge and cite Gaia DR3:
https://www.cosmos.esa.int/web/gaia-users/credits
Acknowledgements:
Gaia team
(End) Arnaud Siebert, Francois-Xavier Pineau, Patricia Vannier [CDS] 11-May-2022