J/A+A/649/A6    Gaia Catalogue of Nearby Stars - GCNS (Gaia collaboration, 2021)

Gaia Early Data Release 3: The Gaia Catalogue of Nearby Stars. Gaia collaboration, Smart R.L., Sarro L.M., Rybizki J., Reyle C., Robin A.C., Hambly N.C., Abbas U., Barstow M.A., de Bruijne J.H.J., Bucciarelli B., Carrasco J.M., Cooper W.J., Hodgkin S.T., Masana E., Michalik D., Sahlmann J., Sozzetti A., Brown A.G.A., Vallenari A., Prusti T., Babusiaux C., Biermann M., Creevey O.L., Evans D.W., Eyer L., Hutton A., Jansen F., Jordi C., Klioner S.A., Lammers U., Lindegren L., Luri X., Mignard F., Panem C., Pourbaix D., Randich S., Sartoretti P., Soubiran C., Walton N.A., Arenou F., Bailer-Jones C.A.L., Bastian U., Cropper M., Drimmel R., Katz D., Lattanzi M.G., van Leeuwen F., Bakker J., Castaneda J., De Angeli F., Ducourant C., Fabricius C., Fouesneau M., Fremat Y., Guerra R., Guerrier A., Guiraud J., Jean-Antoine Piccolo A., Messineo R., Mowlavi N., Nicolas C., Nienartowicz K., Pailler F., Panuzzo P., Riclet F., Roux W., Seabroke G.M., Sordo R., Tanga P., Thevenin F., Gracia-Abril G., Portell J., Teyssier D., Altmann M., Andrae R., Bellas-Velidis I., Benson K., Berthier J., Blomme R., Brugaletta E., Burgess P.W., Busso G., Carry B., Cellino A., Cheek N., Clementini G., Damerdji Y., Davidson M., Delchambre L., Dell'Oro A., Fernandez-Hernandez J., Galluccio L., Garcia-Lario P., Garcia-Reinaldos M., Gonzalez-Nunez J., Gosset E., Haigron R., Halbwachs J.-L., Harrison D.L., Hatzidimitriou D., Heiter U., Hernandez J., Hestroffer D., Holl B., Janssen K., Jevardat de Fombelle G., Jordan S., Krone-Martins A., Lanzafame A.C., Loeffler W., Lorca A., Manteiga M., Marchal O., Marrese P.M., Moitinho A., Mora A., Muinonen K., Osborne P., Pancino E., Pauwels T., Recio-Blanco A., Richards P.J., Riello M., Rimoldini L., Roegiers T., Siopis C., Smith M., Ulla A., Utrilla E., van Leeuwen M., van Reeven W., Abreu Aramburu A., Accart S., Aerts C., Aguado J.J., Ajaj M., Altavilla G., Alvarez M.A., Alvarez Cid-Fuentes J., Alves J., Anderson R.I., Anglada Varela E., Antoja T., Audard M., Baines D., Baker S.G., Balaguer-Nunez L., Balbinot E., Balog Z., Barache C., Barbato D., Barros M., Bartolome S., Bassilana J.-L., Bauchet N., Baudesson-Stella A., Becciani U., Bellazzini M., Bernet M., Bertone S., Bianchi L., Blanco-Cuaresma S., Boch T., Bombrun A., Bossini D., Bouquillon S., Bragaglia A., Bramante L., Breedt E., Bressan A., Brouillet N., Burlacu A., Busonero D., Butkevich A.G., Buzzi R., Caffau E., Cancelliere R., Canovas H., Cantat-Gaudin T., Carballo R., Carlucci T., Carnerero M.I,, Casamiquela L., Castellani M., Castro-Ginard A., Castro Sampol P., Chaoul L., Charlot P., Chemin L., Chiavassa A., Cioni M.-R.L., Comoretto G., Cornez T., Cowell S., Crifo F., Crosta M., Crowley C., Dafonte C., Dapergolas A., David M., David P., de Laverny P., De Luise F., De March R., De Ridder J., de Souza R., de Teodoro P., de Torres A., del Peloso E.F., del Pozo E., Delgado A., Delgado H.E., Delisle J.-B., Di Matteo P., Diakite S., Diener C., Distefano E., Dolding C., Eappachen D., Edvardsson B., Enke H., Esquej P., Fabre C., Fabrizio M., Faigler S., Fedorets G., Fernique P., Fienga A., Figueras F., Fouron C., Fragkoudi F., Fraile E., Franke F., Gai M., Garabato D., Garcia-Gutierrez A., Garcia-Torres M., Garofalo A., Gavras P., Gerlach E., Geyer R., Giacobbe P., Gilmore G., Girona S., Giuffrida G., Gomel R., Gomez A., Gonzalez-Santamaria I., Gonzalez-Vidal J.J., Granvik M., Gutierrez-Sanchez R., Guy L.P., Hauser M., Haywood M., Helmi A., Hidalgo S.L., Hilger T., Hladczuk N., Hobbs D., Holland G., Huckle H.E., Jasniewicz G., Jonker P.G., Juaristi Campillo J., Julbe F., Karbevska L., Kervella P., Khanna S., Kochoska A., Kontizas M., Kordopatis G., Korn A.J., Kostrzewa-Rutkowska Z., KruszyNska K., Lambert S., Lanza A.F., Lasne Y., Le Campion J.-F., Le Fustec Y., Lebreton Y., Lebzelter T., Leccia S., Leclerc N., Lecoeur-Taibi I., Liao S., Licata E., Lindstrom H.E.P., Lister T.A., Livanou E., Lobel A., Madrero Pardo P., Managau S., Mann R.G., Marchant J.M., Marconi M., Marcos Santos M.M.S., Marinoni S., Marocco F., Marshall D.J., Martin Polo L., Martin-Fleitas J.M., Masip A., Massari D., Mastrobuono-Battisti A., Mazeh T., McMillan P.J., Messina S., Millar N.R., Mints A., Molina D., Molinaro R., Molnar L., Montegriffo P., Mor R., Morbidelli R., Morel T., Morris D., Mulone A.F., Munoz D., Muraveva T., Murphy C.P., Musella I., Noval L., Ordenovic C., Orru G., Osinde J., Pagani C., Pagano I., Palaversa L., Palicio P.A., Panahi A., Pawlak M., Penalosa Esteller X., Penttilae A., Piersimoni A.M., Pineau F.-X., Plachy E., Plum G., Poggio E., Poretti E., Poujoulet E., Prsa A., Pulone L., Racero E., Ragaini S., Rainer M., Raiteri C.M., Rambaux N., Ramos P., Ramos-Lerate M., Re Fiorentin P., Regibo S., Ripepi V., Riva A., Rixon G., Robichon N., Robin C., Roelens M., Rohrbasser L., Romero-Gomez M., Rowell N., Royer F., Rybicki K.A., Sadowski G., Sagrista Selles A., Salgado J., Salguero E., Samaras N., Sanchez Gimenez V., Sanna N., Santovena R., Sarasso M., Schultheis M., Sciacca E., Segol M., Segovia J.C., Segransan D., Semeux D., Shahaf S., Siddiqui H.I., Siebert A., Siltala L., Slezak E., Solano E., Solitro F., Souami D., Souchay J., Spagna A., Spoto F., Steele I.A., Steidelmueller H., Stephenson C.A., Sueveges M., Szabados L., Szegedi-Elek E., Taris F., Tauran G., Taylor M.B., Teixeira R., Thuillot W., Tonello N., Torra F., Torra J., Turon C., Unger N., Vaillant M., van Dillen E., Vanel O., Vecchiato A., Viala Y., Vicente D., Voutsinas S., Weiler M., Wevers T., Wyrzykowski L., Yoldas A., Yvard P., Zhao H., Zorec J., Zucker S., Zurbach C., Zwitter T. <Astron. Astrophys. 649, A6 (2021)> =2021A&A...649A...6G 2021A&A...649A...6G (SIMBAD/NED BibCode)
ADC_Keywords: Surveys ; Stars, nearby ; Photometry ; Stars, distances ; Radial velocities Keywords: catalogs - astrometry - stars: luminosity function, mass function - Hertzsprung-Russell diagram and C-M diagrams - stars: low-mass - solar neighborhood Abstract: We produce a clean and well-characterised catalogue of objects within 100 pc of the Sun from the Gaia Early Data Release 3. We characterise the catalogue through comparisons to the full data release, external catalogues, and simulations. We carry out a first analysis of the science that is possible with this sample to demonstrate its potential and best practices for its use. The selection of objects within 100 pc from the full catalogue used selected training sets, machine-learning procedures, astrometric quantities, and solution quality indicators to determine a probability that the astrometric solution is reliable. The training set construction exploited the astrometric data, quality flags, and external photometry. For all candidates we calculated distance posterior probability densities using Bayesian procedures and mock catalogues to define priors. Any object with reliable astrometry and a non-zero probability of being within 100pc is included in the catalogue. We have produced a catalogue of 331312 objects that we estimate contains at least 92% of stars of stellar type M9 within 100pc of the Sun. We estimate that 9% of the stars in this catalogue probably lie outside 100pc, but when the distance probability function is used, a correct treatment of this contamination is possible. We produced luminosity functions with a high signal-to-noise ratio for the main-sequence stars, giants, and white dwarfs. We examined in detail the Hyades cluster, the white dwarf population, and wide-binary systems and produced candidate lists for all three samples. We detected local manifestations of several streams, superclusters, and halo objects, in which we identified 12 members of Gaia Enceladus. We present the first direct parallaxes of five objects in multiple systems within 10pc of the Sun. We provide the community with a large, well-characterised catalogue of objects in the solar neighbourhood. This is a primary benchmark for measuring and understanding fundamental parameters and descriptive functions in astronomy. Description: We produce a clean and well characterised catalogue of nearby objects within 100pc of the Sun from the Gaia early third data release. We characterise the catalogue using the full data release, and comparisons to other catalogues in literature and simulations. We started with a sample of objects with a measured parallax of 8mas. For all candidates we calculate a distance probability function using Bayesian procedures and mock catalogues for the prediction of the priors. For each entry using a random forest classifier we attempt to remove sources with spurious astrometric solutions. From this paper we provide the following data files: table1c.dat (Table1GCNScat): Any object with a non-zero probability of being within 100 pc and not indicated as a spurious astrometric solutions. We have also included external photometric and radial velocity data, the probability of reliable astrometry, probability to be a white dwarf, the distance 1st, 16th, 50th and 84th percentiles, the positions and velocities in a galactic reference frame. For questions please email richard.smart(at)inaf.it. table1r.dat (Table1GCNSreject): All other entries from the 8mas sample that were rejected as having a zero probability of being inside 100pc or indicated as a spurious astrometric solution. This table has the same format and columns as GCNS_cat.dat. progwd.dat (ProbWDlt05_ProbGFgt05): A catalogue of 45 sources with low probability of being a WD in this work (PWD<0.5), but having larger probabilities in Gentile-Fusillo et al (2019MNRAS.482.4570G 2019MNRAS.482.4570G, cat. J/MNRAS/482/4570) (PGF>0.5). For questions please email carrasco(at)fqa.ub.edu. table3.dat (Table3_ResolvedStellarSystems): Resolved binary candidates in the GCNS catalogue as discussed in the section on stellar multiplicity: resolved systems. For questions please email ummi.abbas(at)inaf.it or alessandro.sozzetti(at)inaf.it. maglim.dat (maglimhpx5percentile): The magnitude percentiles for level 5 healpixels used in the luminosity function determinations. For questions please email rybizki(at)mpia.de. distpdf.dat (distance_PDF): The full distance probability density function calculated in section 2 and used throughout the paper. For questions please email rybizki(at)mpia.de. missing.dat (missing_10mas): A list of 1258 objects with published parallaxes greater than 10mas that are not or have no parallax in EDR3. For questions please email celine.reyle(at)obs-besancon.fr. hyacomb.dat (Hyades_ComaBer): A list of 920+212 probable Hyades and ComaBer members in the GCNS sample. For questions please email daniel.michalik(at)esa.int or jos.de.bruijne(at)esa.int. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1c.dat 760 331312 Selected objects table1r.dat 760 880428 Rejected objects progwd.dat 33 45 WDs comparison to Gentile-Fusillo table3.dat 77 19176 Resolved GCNS multiple systems maglim.dat 722 12288 Healpixel 5 magnitude percentiles missing.dat 104 1259 Objects with parallax > 10mas hyacomb.dat 52 1132 Hyades and Coma cluster members distpdf.dat 923 1211740 Distance PDF all objects -------------------------------------------------------------------------------- See also: I/350 : Gaia EDR3 (Gaia Collaboration, 2020) J/MNRAS/482/4570 : Gaia DR2 white dwarf candidates (Gentile Fusillo+, 2019) J/A+A/649/A3 : Gaia EDR3 photometric passbands (Riello+, 2021) J/A+A/649/A7 : MC structure and properties (Gaia Collaboration+, 2021) Byte-by-byte Description of file: table1c.dat table1r.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 3- 21 I19 --- GaiaEDR3 Gaia EDR3 source ID (source_id) 23- 36 F14.7 deg RAdeg Right ascension (ICRS) at Ep=2016.0 (ra) 38- 44 F7.5 mas e_RAdeg Error on RAdeg (ra_error) 46- 59 F14.7 deg DEdeg Declination (ICRS) at Ep=2016.0 (dec) 61- 67 F7.5 mas e_DEdeg Error on DEdeg (dec_error) 69- 77 F9.3 mas Plx Parallax (parallax) 79- 85 F7.5 mas e_Plx Parallax error (parallax_error) 87- 95 F9.3 mas/yr pmRA Proper motion in RA, pmRA*cosDE (pmra) 97-103 F7.5 mas/yr e_pmRA RA proper motion error (pmra_error) 105-113 F9.3 mas/yr pmDE Proper motion in DE (pmdec) 115-121 F7.5 mas/yr e_pmDE DE proper motion error (pmdec_error) 123-130 F8.4 mag Gmag ? Gaia G Band magnitude (photgmean_mag) 132-140 F9.2 --- RFG ? Flux to flux error ratio in G band (photgmeanfluxover_error) 142-149 F8.4 mag BPmag ? Gaia BP Band magnitude (photbpmean_mag) 151-159 F9.2 --- RFBP ? Flux to flux error ratio in BP band (photbpmeanfluxover_error) 161-168 F8.4 mag RPmag ? Gaia RP Band magnitude (photrpmean_mag) 170-178 F9.2 --- RFRP ? Flux to flux error ratio in RP band (photrpmeanfluxover_error) 180-187 F8.4 --- E(BP/RP) ? BP/RP excess factor (photbprpexcessfactor) 189-193 F5.2 --- RUWE Renormalised Error (ruwe) 195-197 I3 --- IPDfmp Double peak flag (ipdfracmulti_peak) 199-206 F8.3 km/s RV ? Adopted Radial Velocity (adoptedRV) 208-215 F8.4 km/s e_RV ? Error in adopted RV (adoptedRV_error) 218-236 A19 --- r_RV Reference bibcode for RV (adoptedRV_refname) 238 A1 --- f_RV ? T/F if eDR3 RV (radialvelocityis_valid) 240-244 F5.3 --- GCNSprob ? Good astrometry probability (GCNS_prob) 246-250 F5.3 --- WDprob ? White dwarf probability (WD_prob) 252-263 F12.5 kpc Dist1 ? 1% distance (dist_1) 265-276 F12.5 kpc Dist16 ? 16% distance (dist_16) 278-289 F12.5 kpc Dist50 ? 50% distance (dist_50) 291-302 F12.5 kpc Dist84 ? 84% distance (dist_84) 304-315 F12.5 pc xcoord50 ? x in Galactic frame (xcoord_50) 317-328 F12.5 pc xcoord16 ? x 1 sigma lower bound (xcoord_16) 330-341 F12.5 pc xcoord84 ? x 1 sigma upper bound (xcoord_84) 343-354 F12.5 pc ycoord50 ? y in Galactic frame (ycoord_50) 356-367 F12.5 pc ycoord16 ? y 1 sigma lower bound (ycoord_16) 369-380 F12.5 pc ycoord84 ? y 1 sigma upper bound (ycoord_84) 382-393 F12.5 pc zcoord50 ? z in Galactic frame (zcoord_50) 395-406 F12.5 pc zcoord16 ? z 1 sigma lower bound (zcoord_16) 408-419 F12.5 pc zcoord84 ? z 1 sigma upper bound (zcoord_84) 421-428 F8.3 km/s Uvel50 ? U in Galactic frame (uvel_50) 430-437 F8.3 km/s Uvel16 ? U 1 sigma lower bound (uvel_16) 439-446 F8.3 km/s Uvel84 ? U 1 sigma upper bound (uvel_84) 448-455 F8.3 km/s Vvel50 ? V in Galactic frame (vvel_50) 457-464 F8.3 km/s Vvel16 ? V 1 sigma lower bound (vvel_16) 466-473 F8.3 km/s Vvel84 ? V 1 sigma upper bound (vvel_84) 475-482 F8.3 km/s Wvel50 ? W in Galactic frame (wvel_50) 484-491 F8.3 km/s Wvel16 ? W 1 sigma lower bound (wvel_16) 493-500 F8.3 km/s Wvel84 ? W 1 sigma upper bound (wvel_84) 502-521 A20 --- GUNN ? Name in external catalogue, HHMMSS.ss+DDMMSS.s, PSO JHHMMSS.ss+DDMMSS.s or NNNNNNNNNNNNNNNNNNN (Gaia DR2 source_id) (NAME_GUNN) 524-542 A19 --- r_GUNN ? GUNN reference bibcode (REFNAME_GUNN) (1) 544-550 F7.3 mag gmag ? GUNN g magnitude (gmag_GUNN) 552-558 F7.3 mag e_gmag ? Error on gmag (egmagGUNN) 560-566 F7.3 mag rmag ? GUNN r magnitude (rmag_GUNN) 568-574 F7.3 mag e_rmag ? Error on rmag (ermagGUNN) 576-582 F7.3 mag imag ? GUNN i magnitude (imag_GUNN) 584-590 F7.3 mag e_imag ? Error on imag (eimagGUNN) 592-598 F7.3 mag zmag ? GUNN z magnitude (zmag_GUNN) 600-606 F7.3 mag e_zmag ? Error on zmag (ezmagGUNN) 611-627 A17 --- 2MASS ? 2MASS name, HHMMSSss+DDMMSSs (NAME_2MASS) (2) 629-635 F7.3 mag Jmag ? J magnitude (jm2MASS) 637-643 F7.3 mag e_Jmag ? Error on Jmag (jmsig2MASS) 645-651 F7.3 mag Hmag ? H magnitude (hm2MASS) 653-659 F7.3 mag e_Hmag ? Error on Hmag (hmsig2MASS) 661-667 F7.3 mag Ksmag ? Ks magnitude (km2MASS) 669-675 F7.3 mag e_Ksmag ? Error on Ksmag (kmsig2MASS) 677-696 A20 --- WISE ? CATWISE name, JHHMMSS.ss+DDMMSS.s (NAME_WISE) (3) 698-704 F7.3 mag W1mag ? CATWISE W1 magnitude (w1mpropmWISE) 706-712 F7.3 mag e_W1mag ? Error on W1mag (w1sigmpropmWISE) 714-720 F7.3 mag W2mag ? CATWISE W2 magnitude (w2mpropmWISE) 722-728 F7.3 mag e_W2mag ? Error on W2mag (w2sigmpropmWISE) 730-736 F7.3 mag W3mag ? ALLWISE W3 magnitude (w3mpro_WISE) 738-744 F7.3 mag e_W3mag ? Error on W3mag (w3sigmpro_WISE) 746-752 F7.3 mag W4mag ? ALLWISE W4 magnitude (w4mpro_WISE) 754-760 F7.3 mag e_W4mag ? Error on W4mag (w4sigmpro_WISE) -------------------------------------------------------------------------------- Note (1): GUNN reference bibcode as follows: 2016arXiv161205560C 2016arXiv161205560C = indicates data from PANSTARRS PS1 (Chambers et al., Cat. II/349) (e.g. gmag/e_gmag) 2018PASA...35...10W 2018PASA...35...10W = indicates magnitude from Skymapper DR2 (Wolf et al., DR1.1 at Cat. II/358) (e.g. g/err_g) 2017ApJS..233...25A 2017ApJS..233...25A = indicates data from SDSS DR13 (Albareti et al.) (e.g. gpsf/eg_psf) Note (2): NIR magnitudes from the 2MASS survey, Skrutskie et al., 2006AJ....131.1163S 2006AJ....131.1163S, Cat. VII/233 Note (3): WISE magnitudes from CATWISE2020 (W1/W2) Korreck et al. (2020ApJS..246...69K 2020ApJS..246...69K), or ALLWISE (W3/W4) catalogue (Cutri et al., 2013, Cat. II/328) -------------------------------------------------------------------------------- Byte-by-byte Description of file: progwd.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 19 I19 --- GaiaEDR3 Gaia EDR3 source ID (sourceId) 21- 26 F6.4 --- PWD WD Probability from this work (PWD) 28- 33 F6.4 --- PGF WD Probability from Gentile-Fusillo et al. (2019, Cat. J/MNRAS/482/4570) (PGF) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 19 I19 --- SourceID1 Gaia EDR3 source ID of primary (sourceID1) 21- 39 I19 --- SourceID2 Gaia EDR3 source ID of secondary (sourceID2) 41- 49 F9.4 arcsec Sep Angular separation (separation) 51- 57 F7.4 Gmag magDiff G magnitude difference (magDiff) 59- 69 F11.4 AU projSep Projected separation (projSep) 71 I1 --- binary [0/1] binary (1) and multiple (0) flag (binary) 73 I1 --- Coma [0/1] Flag for Coma Berenices cluster members (coma) 75 I1 --- Hyades [0/1] Flag for Hyades cluster members (hyades) 77 I1 --- bound [0/1] Flag for formally bound systems (bound) -------------------------------------------------------------------------------- Byte-by-byte Description of file: maglim.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- nHEALpix HEALpix number for nested using RA and DE (nHEALpix) 8- 12 F5.1 mag mag0 Magnitude at 0 percentile (magnitude_0) 15- 19 F5.1 mag mag1 Magnitude at 1 percentile (magnitude_1) 22- 26 F5.1 mag mag2 Magnitude at 2 percentile (magnitude_2) 29- 33 F5.1 mag mag3 Magnitude at 3 percentile (magnitude_3) 36- 40 F5.1 mag mag4 Magnitude at 4 percentile (magnitude_4) 43- 47 F5.1 mag mag5 Magnitude at 5 percentile (magnitude_5) 50- 54 F5.1 mag mag6 Magnitude at 6 percentile (magnitude_6) 57- 61 F5.1 mag mag7 Magnitude at 7 percentile (magnitude_7) 64- 68 F5.1 mag mag8 Magnitude at 8 percentile (magnitude_8) 71- 75 F5.1 mag mag9 Magnitude at 9 percentile (magnitude_9) 78- 82 F5.1 mag mag10 Magnitude at 10 percentile (magnitude_10) 85- 89 F5.1 mag mag11 Magnitude at 11 percentile (magnitude_11) 92- 96 F5.1 mag mag12 Magnitude at 12 percentile (magnitude_12) 99-103 F5.1 mag mag13 Magnitude at 13 percentile (magnitude_13) 106-110 F5.1 mag mag14 Magnitude at 14 percentile (magnitude_14) 113-117 F5.1 mag mag15 Magnitude at 15 percentile (magnitude_15) 120-124 F5.1 mag mag16 Magnitude at 16 percentile (magnitude_16) 127-131 F5.1 mag mag17 Magnitude at 17 percentile (magnitude_17) 134-138 F5.1 mag mag18 Magnitude at 18 percentile (magnitude_18) 141-145 F5.1 mag mag19 Magnitude at 19 percentile (magnitude_19) 148-152 F5.1 mag mag20 Magnitude at 20 percentile (magnitude_20) 155-159 F5.1 mag mag21 Magnitude at 21 percentile (magnitude_21) 162-166 F5.1 mag mag22 Magnitude at 22 percentile (magnitude_22) 169-173 F5.1 mag mag23 Magnitude at 23 percentile (magnitude_23) 176-180 F5.1 mag mag24 Magnitude at 24 percentile (magnitude_24) 183-187 F5.1 mag mag25 Magnitude at 25 percentile (magnitude_25) 190-194 F5.1 mag mag26 Magnitude at 26 percentile (magnitude_26) 197-201 F5.1 mag mag27 Magnitude at 27 percentile (magnitude_27) 204-208 F5.1 mag mag28 Magnitude at 28 percentile (magnitude_28) 211-215 F5.1 mag mag29 Magnitude at 29 percentile (magnitude_29) 218-222 F5.1 mag mag30 Magnitude at 30 percentile (magnitude_30) 225-229 F5.1 mag mag31 Magnitude at 31 percentile (magnitude_31) 232-236 F5.1 mag mag32 Magnitude at 32 percentile (magnitude_32) 239-243 F5.1 mag mag33 Magnitude at 33 percentile (magnitude_33) 246-250 F5.1 mag mag34 Magnitude at 34 percentile (magnitude_34) 253-257 F5.1 mag mag35 Magnitude at 35 percentile (magnitude_35) 260-264 F5.1 mag mag36 Magnitude at 36 percentile (magnitude_36) 267-271 F5.1 mag mag37 Magnitude at 37 percentile (magnitude_37) 274-278 F5.1 mag mag38 Magnitude at 38 percentile (magnitude_38) 281-285 F5.1 mag mag39 Magnitude at 39 percentile (magnitude_39) 288-292 F5.1 mag mag40 Magnitude at 40 percentile (magnitude_40) 295-299 F5.1 mag mag41 Magnitude at 41 percentile (magnitude_41) 302-306 F5.1 mag mag42 Magnitude at 42 percentile (magnitude_42) 309-313 F5.1 mag mag43 Magnitude at 43 percentile (magnitude_43) 316-320 F5.1 mag mag44 Magnitude at 44 percentile (magnitude_44) 323-327 F5.1 mag mag45 Magnitude at 45 percentile (magnitude_45) 330-334 F5.1 mag mag46 Magnitude at 46 percentile (magnitude_46) 337-341 F5.1 mag mag47 Magnitude at 47 percentile (magnitude_47) 344-348 F5.1 mag mag48 Magnitude at 48 percentile (magnitude_48) 351-355 F5.1 mag mag49 Magnitude at 49 percentile (magnitude_49) 358-362 F5.1 mag mag50 Magnitude at 50 percentile (magnitude_50) 365-369 F5.1 mag mag51 Magnitude at 51 percentile (magnitude_51) 372-376 F5.1 mag mag52 Magnitude at 52 percentile (magnitude_52) 379-383 F5.1 mag mag53 Magnitude at 53 percentile (magnitude_53) 386-390 F5.1 mag mag54 Magnitude at 54 percentile (magnitude_54) 393-397 F5.1 mag mag55 Magnitude at 55 percentile (magnitude_55) 400-404 F5.1 mag mag56 Magnitude at 56 percentile (magnitude_56) 407-411 F5.1 mag mag57 Magnitude at 57 percentile (magnitude_57) 414-418 F5.1 mag mag58 Magnitude at 58 percentile (magnitude_58) 421-425 F5.1 mag mag59 Magnitude at 59 percentile (magnitude_59) 428-432 F5.1 mag mag60 Magnitude at 60 percentile (magnitude_60) 435-439 F5.1 mag mag61 Magnitude at 61 percentile (magnitude_61) 442-446 F5.1 mag mag62 Magnitude at 62 percentile (magnitude_62) 449-453 F5.1 mag mag63 Magnitude at 63 percentile (magnitude_63) 456-460 F5.1 mag mag64 Magnitude at 64 percentile (magnitude_64) 463-467 F5.1 mag mag65 Magnitude at 65 percentile (magnitude_65) 470-474 F5.1 mag mag66 Magnitude at 66 percentile (magnitude_66) 477-481 F5.1 mag mag67 Magnitude at 67 percentile (magnitude_67) 484-488 F5.1 mag mag68 Magnitude at 68 percentile (magnitude_68) 491-495 F5.1 mag mag69 Magnitude at 69 percentile (magnitude_69) 498-502 F5.1 mag mag70 Magnitude at 70 percentile (magnitude_70) 505-509 F5.1 mag mag71 Magnitude at 71 percentile (magnitude_71) 512-516 F5.1 mag mag72 Magnitude at 72 percentile (magnitude_72) 519-523 F5.1 mag mag73 Magnitude at 73 percentile (magnitude_73) 526-530 F5.1 mag mag74 Magnitude at 74 percentile (magnitude_74) 533-537 F5.1 mag mag75 Magnitude at 75 percentile (magnitude_75) 540-544 F5.1 mag mag76 Magnitude at 76 percentile (magnitude_76) 547-551 F5.1 mag mag77 Magnitude at 77 percentile (magnitude_77) 554-558 F5.1 mag mag78 Magnitude at 78 percentile (magnitude_78) 561-565 F5.1 mag mag79 Magnitude at 79 percentile (magnitude_79) 568-572 F5.1 mag mag80 Magnitude at 80 percentile (magnitude_80) 575-579 F5.1 mag mag81 Magnitude at 81 percentile (magnitude_81) 582-586 F5.1 mag mag82 Magnitude at 82 percentile (magnitude_82) 589-593 F5.1 mag mag83 Magnitude at 83 percentile (magnitude_83) 596-600 F5.1 mag mag84 Magnitude at 84 percentile (magnitude_84) 603-607 F5.1 mag mag85 Magnitude at 85 percentile (magnitude_85) 610-614 F5.1 mag mag86 Magnitude at 86 percentile (magnitude_86) 617-621 F5.1 mag mag87 Magnitude at 87 percentile (magnitude_87) 624-628 F5.1 mag mag88 Magnitude at 88 percentile (magnitude_88) 631-635 F5.1 mag mag89 Magnitude at 89 percentile (magnitude_89) 638-642 F5.1 mag mag90 Magnitude at 90 percentile (magnitude_90) 645-649 F5.1 mag mag91 Magnitude at 91 percentile (magnitude_91) 652-656 F5.1 mag mag92 Magnitude at 92 percentile (magnitude_92) 659-663 F5.1 mag mag93 Magnitude at 93 percentile (magnitude_93) 666-670 F5.1 mag mag94 Magnitude at 94 percentile (magnitude_94) 673-677 F5.1 mag mag95 Magnitude at 95 percentile (magnitude_95) 680-684 F5.1 mag mag96 Magnitude at 96 percentile (magnitude_96) 687-691 F5.1 mag mag97 Magnitude at 97 percentile (magnitude_97) 694-698 F5.1 mag mag98 Magnitude at 98 percentile (magnitude_98) 701-705 F5.1 mag mag99 Magnitude at 99 percentile (magnitude_99) 708-712 F5.1 mag mag100 Magnitude at 100 percentile (magnitude_100) 714-722 I9 --- Count Sources per HEALpix (sourcecount) -------------------------------------------------------------------------------- Byte-by-byte Description of file: distpdf.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 3- 21 I19 --- GaiaEDR3 Gaia EDR3 source ID (source_id) 23- 30 F8.6 kpc Dist1 1 percentile of the distance PDF (dist_1) 32- 39 F8.6 kpc Dist2 2 percentile of the distance PDF (dist_2) 41- 48 F8.6 kpc Dist3 3 percentile of the distance PDF (dist_3) 50- 57 F8.6 kpc Dist4 4 percentile of the distance PDF (dist_4) 59- 66 F8.6 kpc Dist5 5 percentile of the distance PDF (dist_5) 68- 75 F8.6 kpc Dist6 6 percentile of the distance PDF (dist_6) 77- 84 F8.6 kpc Dist7 7 percentile of the distance PDF (dist_7) 86- 93 F8.6 kpc Dist8 8 percentile of the distance PDF (dist_8) 95-102 F8.6 kpc Dist9 9 percentile of the distance PDF (dist_9) 104-111 F8.6 kpc Dist10 10 percentile of the distance PDF (dist_10) 113-120 F8.6 kpc Dist11 11 percentile of the distance PDF (dist_11) 122-129 F8.6 kpc Dist12 12 percentile of the distance PDF (dist_12) 131-138 F8.6 kpc Dist13 13 percentile of the distance PDF (dist_13) 140-147 F8.6 kpc Dist14 14 percentile of the distance PDF (dist_14) 149-156 F8.6 kpc Dist15 15 percentile of the distance PDF (dist_15) 158-165 F8.6 kpc Dist16 16 percentile of the distance PDF (dist_16) 167-174 F8.6 kpc Dist17 17 percentile of the distance PDF (dist_17) 176-183 F8.6 kpc Dist18 18 percentile of the distance PDF (dist_18) 185-192 F8.6 kpc Dist19 19 percentile of the distance PDF (dist_19) 194-201 F8.6 kpc Dist20 20 percentile of the distance PDF (dist_20) 203-210 F8.6 kpc Dist21 21 percentile of the distance PDF (dist_21) 212-219 F8.6 kpc Dist22 22 percentile of the distance PDF (dist_22) 221-228 F8.6 kpc Dist23 23 percentile of the distance PDF (dist_23) 230-237 F8.6 kpc Dist24 24 percentile of the distance PDF (dist_24) 239-246 F8.6 kpc Dist25 25 percentile of the distance PDF (dist_25) 248-255 F8.6 kpc Dist26 26 percentile of the distance PDF (dist_26) 257-264 F8.6 kpc Dist27 27 percentile of the distance PDF (dist_27) 266-273 F8.6 kpc Dist28 28 percentile of the distance PDF (dist_28) 275-282 F8.6 kpc Dist29 29 percentile of the distance PDF (dist_29) 284-291 F8.6 kpc Dist30 30 percentile of the distance PDF (dist_30) 293-300 F8.6 kpc Dist31 31 percentile of the distance PDF (dist_31) 302-309 F8.6 kpc Dist32 32 percentile of the distance PDF (dist_32) 311-318 F8.6 kpc Dist33 33 percentile of the distance PDF (dist_33) 320-327 F8.6 kpc Dist34 34 percentile of the distance PDF (dist_34) 329-336 F8.6 kpc Dist35 35 percentile of the distance PDF (dist_35) 338-345 F8.6 kpc Dist36 36 percentile of the distance PDF (dist_36) 347-354 F8.6 kpc Dist37 37 percentile of the distance PDF (dist_37) 356-363 F8.6 kpc Dist38 38 percentile of the distance PDF (dist_38) 365-372 F8.6 kpc Dist39 39 percentile of the distance PDF (dist_39) 374-381 F8.6 kpc Dist40 40 percentile of the distance PDF (dist_40) 383-390 F8.6 kpc Dist41 41 percentile of the distance PDF (dist_41) 392-399 F8.6 kpc Dist42 42 percentile of the distance PDF (dist_42) 401-408 F8.6 kpc Dist43 43 percentile of the distance PDF (dist_43) 410-417 F8.6 kpc Dist44 44 percentile of the distance PDF (dist_44) 419-426 F8.6 kpc Dist45 45 percentile of the distance PDF (dist_45) 428-435 F8.6 kpc Dist46 46 percentile of the distance PDF (dist_46) 437-444 F8.6 kpc Dist47 47 percentile of the distance PDF (dist_47) 446-453 F8.6 kpc Dist48 48 percentile of the distance PDF (dist_48) 455-462 F8.6 kpc Dist49 49 percentile of the distance PDF (dist_49) 464-471 F8.6 kpc Dist50 50 percentile of the distance PDF (dist_50) 473-480 F8.6 kpc Dist51 51 percentile of the distance PDF (dist_51) 482-489 F8.6 kpc Dist52 52 percentile of the distance PDF (dist_52) 491-498 F8.6 kpc Dist53 53 percentile of the distance PDF (dist_53) 500-507 F8.6 kpc Dist54 54 percentile of the distance PDF (dist_54) 509-516 F8.6 kpc Dist55 55 percentile of the distance PDF (dist_55) 518-525 F8.6 kpc Dist56 56 percentile of the distance PDF (dist_56) 527-534 F8.6 kpc Dist57 57 percentile of the distance PDF (dist_57) 536-543 F8.6 kpc Dist58 58 percentile of the distance PDF (dist_58) 545-552 F8.6 kpc Dist59 59 percentile of the distance PDF (dist_59) 554-561 F8.6 kpc Dist60 60 percentile of the distance PDF (dist_60) 563-570 F8.6 kpc Dist61 61 percentile of the distance PDF (dist_61) 572-579 F8.6 kpc Dist62 62 percentile of the distance PDF (dist_62) 581-588 F8.6 kpc Dist63 63 percentile of the distance PDF (dist_63) 590-597 F8.6 kpc Dist64 64 percentile of the distance PDF (dist_64) 599-606 F8.6 kpc Dist65 65 percentile of the distance PDF (dist_65) 608-615 F8.6 kpc Dist66 66 percentile of the distance PDF (dist_66) 617-624 F8.6 kpc Dist67 67 percentile of the distance PDF (dist_67) 626-633 F8.6 kpc Dist68 68 percentile of the distance PDF (dist_68) 635-642 F8.6 kpc Dist69 69 percentile of the distance PDF (dist_69) 644-651 F8.6 kpc Dist70 70 percentile of the distance PDF (dist_70) 653-660 F8.6 kpc Dist71 71 percentile of the distance PDF (dist_71) 662-669 F8.6 kpc Dist72 72 percentile of the distance PDF (dist_72) 671-678 F8.6 kpc Dist73 73 percentile of the distance PDF (dist_73) 680-687 F8.6 kpc Dist74 74 percentile of the distance PDF (dist_74) 689-696 F8.6 kpc Dist75 75 percentile of the distance PDF (dist_75) 698-705 F8.6 kpc Dist76 76 percentile of the distance PDF (dist_76) 707-714 F8.6 kpc Dist77 77 percentile of the distance PDF (dist_77) 716-723 F8.6 kpc Dist78 78 percentile of the distance PDF (dist_78) 725-732 F8.6 kpc Dist79 79 percentile of the distance PDF (dist_79) 734-741 F8.6 kpc Dist80 80 percentile of the distance PDF (dist_80) 743-750 F8.6 kpc Dist81 81 percentile of the distance PDF (dist_81) 752-759 F8.6 kpc Dist82 82 percentile of the distance PDF (dist_82) 761-768 F8.6 kpc Dist83 83 percentile of the distance PDF (dist_83) 770-777 F8.6 kpc Dist84 84 percentile of the distance PDF (dist_84) 779-786 F8.6 kpc Dist85 85 percentile of the distance PDF (dist_85) 788-795 F8.6 kpc Dist86 86 percentile of the distance PDF (dist_86) 797-804 F8.6 kpc Dist87 87 percentile of the distance PDF (dist_87) 806-813 F8.6 kpc Dist88 88 percentile of the distance PDF (dist_88) 815-822 F8.6 kpc Dist89 89 percentile of the distance PDF (dist_89) 824-831 F8.6 kpc Dist90 90 percentile of the distance PDF (dist_90) 833-840 F8.6 kpc Dist91 91 percentile of the distance PDF (dist_91) 842-849 F8.6 kpc Dist92 92 percentile of the distance PDF (dist_92) 851-858 F8.6 kpc Dist93 93 percentile of the distance PDF (dist_93) 860-867 F8.6 kpc Dist94 94 percentile of the distance PDF (dist_94) 869-876 F8.6 kpc Dist95 95 percentile of the distance PDF (dist_95) 878-885 F8.6 kpc Dist96 96 percentile of the distance PDF (dist_96) 887-894 F8.6 kpc Dist97 97 percentile of the distance PDF (dist_97) 896-903 F8.6 kpc Dist98 98 percentile of the distance PDF (dist_98) 905-912 F8.6 kpc Dist99 99 percentile of the distance PDF (dist_99) 914-918 F5.3 --- mnacc-frac Mean acceptance fraction of MCMC chains (mnaccfrac) 920-923 F4.1 --- mncor-time ? Mean autocorrelation time of MCMC chains (mncortime) -------------------------------------------------------------------------------- Byte-by-byte Description of file: missing.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 26 A26 --- Name Simbad source name (main_id) 29- 38 F10.6 deg RAdeg Right ascension (ICRS, epoch 2000.0) (ra) 43- 52 F10.6 deg DEdeg Declination (ICRS, epoch 2000.0) (dec) 57- 63 F7.3 mas plx Parallax (plx_value) 74- 92 A19 --- r_plx Reference bibcode for parallax (plx_bibcode) 101-104 A4 --- Type Simbad object type (otype_txt) -------------------------------------------------------------------------------- Byte-by-byte Description of file: hyacomb.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 3- 21 I19 --- GaiaEDR3 Gaia EDR3 source ID (source_id) 25- 31 A7 --- Cluster Cluster name (name) 34- 39 F6.3 --- MembCluster Membership value (c_cluster) (1) 46- 52 F7.3 pc DistCluster Barycentre distance (dist_cluster) (2) -------------------------------------------------------------------------------- Note (1): Dimensionless chi-square test statistic. Small values indicate highly probable members. See Reino et al. 2018MNRAS.477.3197R 2018MNRAS.477.3197R, Eq. (4). Note (2): Distance of each star from the cluster barycentre, using (XCOORD_50, YCOORD_50, ZCOORD_50) from GCNS_cat.dat. The cluster barycentre is computed as the average (X, Y, Z) coordinate of all stars in the central region of the cluster (two tidal radii), assuming equal masses for all stars. -------------------------------------------------------------------------------- Acknowledgements: Richard Smart, richard.smart(at)rinaf.it
(End) Richard L. Smart [OATo-INAF], Patricia Vannier [CDS] 17-Nov-2020
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line