Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/836/99 into FORTRAN code for reading data files line by line.
Note that special values are assigned to unknown or unspecified
numbers (also called NULL numbers);
when necessary, the coordinate components making up the right ascension
and declination are converted into floating-point numbers
representing these angles in degrees.
program load_ReadMe
C=============================================================================
C F77-compliant program generated by readme2f_1.81 (2015-09-23), on 2024-Apr-18
C=============================================================================
* This code was generated from the ReadMe file documenting a catalogue
* according to the "Standard for Documentation of Astronomical Catalogues"
* currently in use by the Astronomical Data Centers (CDS, ADC, A&A)
* (see full documentation at URL http://vizier.u-strasbg.fr/doc/catstd.htx)
* Please report problems or questions to
C=============================================================================
implicit none
* Unspecified or NULL values, generally corresponding to blank columns,
* are assigned one of the following special values:
* rNULL__ for unknown or NULL floating-point values
* iNULL__ for unknown or NULL integer values
real*4 rNULL__
integer*4 iNULL__
parameter (rNULL__=--2147483648.) ! NULL real number
parameter (iNULL__=(-2147483647-1)) ! NULL int number
integer idig ! testing NULL number
C=============================================================================
Cat. J/ApJ/836/99 NuSTAR serendipitous survey: the 40-month catalog (Lansbury+, 2017)
*================================================================================
*The NuSTAR serendipitous survey: the 40-month catalog and the properties of the
*distant high-energy X-ray source population.
* Lansbury G.B., Stern D., Aird J., Alexander D.M., Fuentes C.,
* Harrison F.A., Treister E., Bauer F.E., Tomsick J.A., Balokovic M.,
* Del Moro A., Gandhi P., Ajello M., Annuar A., Ballantyne D.R., Boggs S.E.,
* Brandt W.N., Brightman M., Chen C.-T.J., Christensen F.E., Civano F.,
* Comastri A., Craig W.W., Forster K., Grefenstette B.W., Hailey C.J.,
* Hickox R.C., Jiang B., Jun H.D., Koss M., Marchesi S., Melo A.D.,
* Mullaney J.R., Noirot G., Schulze S., Walton D.J., Zappacosta L.,
* Zhang W.W.
* <Astrophys. J., 836, 99-99 (2017)>
* =2017ApJ...836...99L (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Details of the individual NuSTAR observations which
make up the serendipitous survey
integer*4 nr__
parameter (nr__=591) ! Number of records
character*82 ar__ ! Full-size record
C J2000 position composed of: RAdeg DEdeg
character*4 Field ! Field identifier (1)
character*23 Target ! Primary science target identifier
integer*4 NObs ! [1/15]? Number of individual exposures in Field
integer*8 ObsID ! ? Observation identifier
character*10 Date ! ("Y/M/D") ? Field observation start UT date
real*4 RAdeg ! (deg) ? Aim point Right Ascension (J2000)
real*4 DEdeg ! (deg) ? Aim point Declination (J2000)
real*4 Exp ! (ks) [1.8/1104] Exposure time (2)
integer*4 N ! [0/12]? Number of serendipitous sources detected
integer*4 A15 ! [0/1]? Aird+ 2015ApJ...815...66A flag (3)
integer*4 H16 ! [0/1]? Harrison+ 2016ApJ...831..185H flag (3)
*Note (1): For fields with multiple NuSTAR exposures (i.e., Nobs>1), each
* individual component exposure is listed with a letter suffixed to the
* field ID (e.g., 3a and 3b).
*Note (2): For a single focal plane module (i.e., averaged over FPMA and FPMB).
*Note (3): Binary flags to highlight the serendipitous survey fields used for
* the Aird+ 2015ApJ...815...66A and Harrison+ 2016ApJ...831..185H
* studies.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table5.dat' ! The primary NuSTAR serendipitous source catalog
integer*4 nr__1
parameter (nr__1=498) ! Number of records
character*903 ar__1 ! Full-size record
C J2000 position composed of: RAdeg DEdeg
integer*4 Seq ! [1/498] Running sequence number
character*14 NuSTAR ! Unique NuSTAR source name (JHHMMSS+DDMM.m)
real*8 RAdeg_1 ! (deg) Right Ascension in decimal degrees (J2000)
real*8 DEdeg_1 ! (deg) Declination in decimal degrees (J2000)
integer*4 SFl ! [0/1] Soft (3-8keV) band detection flag (1)
integer*4 HFl ! [0/1] Hard (8-24keV) band detection flag (1)
integer*4 FFl ! [0/1] Full (3-24keV) band detection flag (1)
integer*4 SdbFl ! [0/1] Deblended soft band detection flag (2)
integer*4 HdbFl ! [0/1] Deblended hard band detection flag (2)
integer*4 FdbFl ! [0/1] Deblended full band detection flag (2)
real*8 logSP ! ([-]) [-44/-0.003]?=-999 Log of soft band false
* probability; Section 2.3
real*8 logHP ! ([-]) [-42/-0.03]?=-999 Log of hard band false
* probability; Section 2.3
real*8 logFP ! ([-]) [-44/-1.7]?=-999 Log of full band false
* probability; Section 2.3
real*8 logSdbP ! ([-]) [-306/-0.003]?=-999 Log of deblended soft band
* false probability
real*8 logHdbP ! ([-]) [-231/-0.03]?=-999 Log of deblended hard band
* false probability
real*8 logFdbP ! ([-]) [-246/-1.7]?=-999 Log of deblended full band
* false probability
integer*4 dbFl ! [0/1] Source remains significant after
* deblending flag (3)
real*8 Scts ! (ct) [8/11132] Total soft (3-8keV) band counts (4)
real*8 e_Scts ! (ct) [3/107] The 84% confidence level in Scts
real*8 SBck ! (ct) [10/2568] Soft background counts scaled
* to source aperture (4)
real*8 SNet ! (ct) [5/9881] Net soft (3-8keV) band counts;
* Scts-SBck (4)
real*8 e_SNet ! (ct) [-99/107] The error in SNet (5)
real*4 Hcts ! (ct) [15/6680] Total hard (8-24keV) band counts (4)
real*4 e_Hcts ! (ct) [4/83] The 84% confidence level in Hcts
real*8 HBck ! (ct) [7/1620] Hard background counts scaled
* to source aperture (4)
real*8 HNet ! (ct) [5/5854] Net hard (8-24keV) band counts;
* Hcts-HBck (4)
real*8 e_HNet ! (ct) [-99/83] The error in HNet (5)
real*8 Fcts ! (ct) [32/17765] Total full (3-24keV) band counts (4)
real*8 e_Fcts ! (ct) [6/135] The 84% confidence level in Fcts
real*8 FBck ! (ct) [18/4178] Full background counts scaled
* to source aperture (4)
real*8 FNet ! (ct) [18/15694] Net full (3-24keV) band counts;
* Fcts-FBck (4)
real*8 e_FNet ! (ct) [-99/135] The error in FNet (5)
real*8 Sdbcts ! (ct) [8/11132] Total deblended soft band counts (4)
real*8 e_Sdbcts ! (ct) [10/2568] The 84% confidence level in Sdbcts
real*8 SdbNet ! (ct) [5/9881] Net deblended soft band
* counts; Sdbcts-SdbBck (4)
real*8 e_SdbNet ! (ct) [-99/107] The error in SdbNet (5)
real*4 Hdbcts ! (ct) [15/6680] Total deblended hard band counts (4)
real*8 e_Hdbcts ! (ct) [7/1620] The 84% confidence level in Hdbcts
real*8 HdbNet ! (ct) [5/5854] Net deblended hard band
* counts; Hdbcts-HdbBck (4)
real*8 e_HdbNet ! (ct) [-99/83] The error in HdbNet (5)
real*8 Fdbcts ! (ct) [32/17765] Total deblended full band counts (4)
real*8 e_Fdbcts ! (ct) [18/4178] The 84% confidence level in Fdbcts
real*8 FdbNet ! (ct) [18/15694] Net deblended full band
* counts; Fdbcts-FdbBck (4)
real*8 e_FdbNet ! (ct) [-99/135] The error in FdbNet (5)
real*8 Sexp ! (s) [12556/] Soft band exposure time (6)
real*8 Hexp ! (s) [10166/] Hard band exposure time (6)
real*8 Fexp ! (s) [10172/] Full band exposure time (6)
real*4 SCR ! (ct/s) [0.0004/0.06] Total soft band count rate (7)
real*4 e_SCR ! (ct/s) [/0.002] The 84% confidence level in SCR
real*4 SCRBck ! (ct/s) [0.0004/0.007] Soft background count rate (7)
real*4 SNCR ! (ct/s) [/0.06] Net soft count rate (7)
real*4 e_SNCR ! (ct/s) [-99/0.002] The error in SNCR (5)
real*4 HCR ! (ct/s) [0.0005/0.05] Total hard band count rate (7)
real*4 e_HCR ! (ct/s) [/0.001] The 84% confidence level in HCR
real*4 HCRBck ! (ct/s) [0.0006/0.005] Hard background count rate (7)
real*4 HNCR ! (ct/s) [/0.04] Net hard count rate (7)
real*4 e_HNCR ! (ct/s) [-99/0.001] The error in HNCR (5)
real*4 FCR ! (ct/s) [0.001/0.2] Total full band count rate (7)
real*4 e_FCR ! (ct/s) [/0.002] The 84% confidence level in FCR
real*4 FCRBck ! (ct/s) [0.001/0.02] Full background count rate (7)
real*4 FNCR ! (ct/s) [0.0001/0.1] Net full count rate (7)
real*4 e_FNCR ! (ct/s) [-99/0.002] The error in FNCR (5)
real*4 SdbNCR ! (ct/s) [/0.06] Deblended net soft count rate (7)
real*4 e_SdbNCR ! (ct/s) [-99/0.002] The 84% confidence level
* in SdbNCR
real*4 HdbNCR ! (ct/s) [/0.04] Deblended net hard count rate (7)
real*4 e_HdbNCR ! (ct/s) [-99/0.001] The 84% confidence level
* in HdbNCR
real*4 FdbNCR ! (ct/s) [0.0001/0.1] Deblended net full count rate (7)
real*4 e_FdbNCR ! (ct/s) [-99/0.002] The 84% confidence level
* in FdbNCR
real*4 H_S ! [/7.5]?=0 Hard to Soft band ratio
real*8 E_H_S ! [-99/1] Upper error on H/S (8)
real*8 e_H_S_1 ! [-99/1] Lower error on H/S (8)
real*4 gamma ! [-0.5/3]? Effective photon index
real*8 E_gamma ! [-99/1]? Upper error on gamma (8)
real*8 e_gamma_1 ! [-99/0.6]? Lower error on gamma (8)
real*4 SFlux ! (mW/m2) Observed-frame soft flux (9)
real*4 e_SFlux ! (mW/m2) ?=-99 The 84% confidence level in SFlux
real*4 HFlux ! (mW/m2) Observed-frame hard flux (9)
real*4 e_HFlux ! (mW/m2) ?=-99 The 84% confidence level in HFlux
real*4 FFlux ! (mW/m2) Observed-frame full flux (9)
real*4 e_FFlux ! (mW/m2) ?=-99 The 84% confidence level in FFlux
character*8 XOrig ! Soft X-ray counterpart code (10)
real*8 RAXdeg ! (deg) ? Soft X-ray counterpart Right Ascension in
* decimal degrees (J2000)
real*8 DEXdeg ! (deg) ? Soft X-ray counterpart Declination in
* decimal degrees (J2000)
real*4 XOff ! (arcsec) [0.5/37]? Soft X-ray and NuSTAR position offset
real*4 XFlux ! (mW/m2) [0/2e-12]? Observed-frame 3-8 keV X-ray
* counterpart flux (11)
real*4 XTFlux ! (mW/m2) [0/2e-12]? Total combined 3-8 keV X-ray flux
* within 30" of NUSTAR
real*8 RAWdeg ! (deg) ? WISE counterpart Right Ascension in
* decimal degrees (J2000)
real*8 DEWdeg ! (deg) ? WISE counterpart Declination in
* decimal degrees (J2000)
real*4 IROff ! (arcsec) [0.05/6]? WISE and NuSTAR position offset
real*4 W1mag ! (mag) [5.6/18.8]? WISE W1 band, 3.4um, profile-fit
* Vega magnitude
real*4 e_W1mag ! (mag) [0.02/0.3]? Error in W1mag (12)
real*4 W2mag ! (mag) [3.8/17.4]? WISE W2 band, 4.6um, profile-fit
* Vega magnitude
real*4 e_W2mag ! (mag) ? Error in W2mag (12)
real*4 W3mag ! (mag) [4/14]? WISE W3 band, 12 micron, profile-fit
* Vega magnitude
real*4 e_W3mag ! (mag) ? Error in W3mag (12)
real*4 W4mag ! (mag) [1.7/10.2]? WISE W4 band, 22um, profile-fit
* Vega magnitude
real*4 e_W4mag ! (mag) ? Error in W4mag (12)
character*9 OOrig ! Adopted optical counterpart code (13)
real*8 RAOdeg ! (deg) ? Optical counterpart Right Ascension in
* decimal degrees (J2000)
real*8 DEOdeg ! (deg) ? Optical counterpart Declination in
* decimal degrees (J2000)
real*4 OOff ! (arcsec) [0.02/6]? Optical and NuSTAR position offset
real*8 Rmag ! (mag) [-99/24.3]? Optical counterpart R band Vega
* magnitude (14)
real*4 zsp ! [0/3.5]? Spectroscopic redshift (15)
real*4 XLum ! (10-7W) ? Rest-frame 10-40 keV luminosity (16)
integer*4 PFl ! [0/1] Source associated with primary science
* target (17)
integer*4 A15Fl ! [0/1] Aird+ 2015ApJ...815...66A flag (18)
*Note (1): A binary flag indicating whether the source is detected with a false
* probability lower than our threshold of log(PFalse)=-6.
*Note (2): Same as previous columns but after deblending has been performed to
* account for contamination of the source counts from very nearby
* sources (see Section 2.4 of this paper, and Section 2.3.2 of
* Mullaney+ (2015, J/ApJ/808/184). Deblending only affects a
* very small fraction of the overall sample (e.g., see Section 2.4).
*Note (3): A binary flag indicating whether the NuSTAR detected source remains
* significant after deblending, in at least one of the three standard
* energy bands.
*Note (4): Calculated at the source coordinates, and using a source aperture of
* 30" radius (see Section 2.4). The values are non-aperture-corrected;
* i.e., they correspond to the 30" values, and have not been corrected
* to the full PSF values.
*Note (5): For the net source counts, we give 90% CL upper limits for sources
* not detected in a given band. Throughout the table, upper limits are
* flagged with a -99 value in the error column.
*Note (6): The average net, vignetting-corrected exposure time at the source
* coordinates. These correspond to the A+B data, so should be divided
* by two to obtain the average exposure per FPM.
*Note (7): Non-aperture-corrected. Determined from the photometric values
* and the exposure times.
*Note (8): Upper limits, lower limits, and sources with no constraints are
* flagged with -99, -88, and -77 values, respectively, in the
* error columns.
*Note (9): After deblending has been performed. These are aperture corrected
* values (i.e., they correspond to the full NuSTAR PSF), and are
* calculated from the count rates using the conversion factors
* listed in Section 2.4.
*Note (10): An abbreviated code indicating the origin of the adopted soft (i.e.,
* low energy; <10keV) X-ray counterpart. Code as follows:
* CXO_CSC = counterparts from the Chandra Source Catalog (CSC; 82 occurrences;
* Evans+ 2010, Cat. IX/45).
* XMM_3XMM = counterparts from the third XMM-Newton serendipitous source catalog
* (3XMM; 203 occurrences; Watson+ 2009, J/A+A/493/339 ;
* Rosen+ 2016, IX/50).
* CXO_MAN = sources manually identified using archival Chandra (27 occurrences)
* XMM_MAN = sources manually identified using archival XMM-Newton
* (24 occurrences)
* XRT_MAN = sources manually identified using archival Swift XRT data
* (60 occurrences).
* Section 3.1 details the counterpart matching.
*Note (11): For sources with counterparts in the CSC and 3XMM catalogs. For CSC
* sources we convert to the 3-8keV flux from the 2-7keV flux using a
* conversion factor of 0.83, and for the 3XMM sources we convert from
* the 4.5-12keV flux using a conversion factor of 0.92.
*Note (12): Blanks in the errors indicates the magnitude is a WISE upper limit.
*Note (13): An abbreviated code indicating the origin of the adopted optical
* counterpart to the NuSTAR source. Code as follows:
* SDSS = sources with soft X-ray counterparts and successful matches in
* the SDSS DR7 catalog (York+ 2000AJ....120.1579Y); 127 occurrences
* USNO = sources with soft X-ray counterparts and successful matches in
* the USNOB1 catalog (Monet+ 2003, I/284); 166 occurrences
* MAN = sources with a soft X-ray counterpart and a corresponding optical
* counterpart manually identified in the available optical coverage;
* 181 occurrences
* SDSS_WISE = there is no soft X-ray counterpart to the NuSTAR position, but a
* WISE AGN candidate is identified within the NuSTAR error circle
* and successfully matched to the SDSS DR7 (these are mainly used as
* candidates for spectroscopic followup); 11 occurrences.
* USNO_WISE = there is no soft X-ray counterpart to the NuSTAR position, but a
* WISE AGN candidate is identified within the NuSTAR error circle
* and successfully matched to the USNOB1 catalog (these are mainly
* used as candidates for spectroscopic followup; 6 occurrences).
* We give a detailed description of the procedure used to identify
* optical counterparts in Section 3.2.
*Note (14): For the SDSS DR7 matches, this is calculated as R=r-0.16. For
* the USNOB1 matches, this is taken as the mean of the two independent
* photographic plate measurements, R1mag and R2mag. For the manual
* identifications, the magnitude is taken from another optical catalog
* or manually determined from the imaging data.
*Note (15): The large majority of the redshifts were obtained through our own
* campaign of ground-based spectroscopic followup of NuSTAR
* serendipitous survey sources (see Section 3.3.1 and
* the "Description" section above).
*Note (16): Estimated from the observed-frame fluxes, following the procedure
* outlined in Section 2.4. Negative values indicate upper limits. The
* luminosities are observed values, uncorrected for any absorption
* along the line of sight. The intrinsic luminosities may therefore
* be higher, for highly absorbed AGNs.
*Note (17): A binary flag indicating the few sources which show evidence for
* being associated with the primary science targets of their
* respective NuSTAR observations, according to the definition in
* Section 2.3 [{Delta}(cz)<0.05cz].
*Note (18): A binary flag highlighting the sources used in the
* Aird+ (2015ApJ...815...66A) study.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table6.dat' ! Summary of the optical spectroscopy for the NuSTAR
serendipitous survey sources
integer*4 nr__2
parameter (nr__2=303) ! Number of records
character*234 ar__2 ! Full-size record
integer*4 Seq_1 ! [1/498] Unique source identification number
character*14 NuSTAR_1 ! Unique NuSTAR source name (JHHMMSS+DDMM.m)
real*4 z ! [0/3.5]? Source spectroscopic redshift
character*7 Type ! Classification (1)
character*122 Lines ! Emission/absorption lines identified (2)
character*68 Notes ! Source notes and literature spectra references
character*2 Run ! Unique observing run identification number (3)
*Note (1): Classification (for primary sources) as follows:
* BL = broad-line AGN (151 occurrences + 11 BL?)
* NL = narrow-line AGN (84 occurrences + 13 NL?)
* BL Lac? = BL Lac object candidate (1 occurrence)
* Gal = Galactic objects (z=0; 16 occurrences)
*
* See Section 3.3.2 for further details.
*Note (2): Absorption line/feature marked with "dg" footnote.
*Note (3): As defined in Table 4 ("S" and "L" mark spectra obtained from the
* SDSS and from elsewhere in the literature, respectively).
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table7.dat' ! The secondary NuSTAR serendipitous source catalog
integer*4 nr__3
parameter (nr__3=64) ! Number of records
character*377 ar__3 ! Full-size record
C J2000 position composed of: RAdeg DEdeg
integer*4 Seq_2 ! [1/64] Unique source identification number
character*14 NuSTAR_2 ! Unique NuSTAR source name (JHHMMSS+DDMM.m)
real*8 RAdeg_2 ! (deg) Right Ascension in decimal degrees (J2000)
real*8 DEdeg_2 ! (deg) Declination in decimal degrees (J2000)
real*8 Scts_1 ! (ct) [36/7049]? Total soft band (3-8keV) counts (1)
real*8 SBck_1 ! (ct) ? Soft background counts (1)
real*8 SNet_1 ! (ct) [16/6633]? Net soft band counts (1)
real*8 e_SNet_1 ! (ct) [-99/85]? The error in SNet (2)
real*8 Hcts_1 ! (ct) ? Total hard band (8-24 keV) counts (1)
real*8 HBck_1 ! (ct) ? Hard background counts (1)
real*8 HNet_1 ! (ct) [13/4306]? Net hard band counts (1)
real*8 e_HNet_1 ! (ct) [-99/69]? The error in HNet (2)
real*8 Fcts_1 ! (ct) [85/11617]? Total full band (3-24keV) counts (1)
real*8 FBck_1 ! (ct) ? Full background counts (1)
real*8 FNet_1 ! (ct) [22/10900]? Net full band counts (1)
real*8 e_FNet_1 ! (ct) [-99/109]? The error in FNet (2)
real*8 Sexp_1 ! (s) [14375/643091]? Soft band exposure time (3)
real*8 Hexp_1 ! (s) ? Hard band exposure time (3)
real*8 Fexp_1 ! (s) ? Full band exposure time (3)
real*4 SNCR_1 ! (ct/s) [0.0003/0.5]? Net soft count rate,
* aperture-corrected (4)
real*4 e_SNCR_1 ! (ct/s) [-99/0.006]? The error in SNCR (2)
real*4 HNCR_1 ! (ct/s) [0.0003/0.4]? Net hard count rate,
* aperture-corrected (4)
real*4 e_HNCR_1 ! (ct/s) [-99/0.006]? The error in HNCR (2)
real*4 FNCR_1 ! (ct/s) [0.0005/1]? Net full count rate,
* aperture-corrected (4)
real*4 e_FNCR_1 ! (ct/s) [-99/0.01]? The error in FNCR (2)
real*4 SFlux_1 ! (mW/m2) ? Observed-frame soft flux (5)
real*4 e_SFlux_1 ! (mW/m2) [-99/]? The 84% confidence level in SFlux
real*4 HFlux_1 ! (mW/m2) ? Observed-frame hard flux (5)
real*4 e_HFlux_1 ! (mW/m2) [-99/]? The 84% confidence level in HFlux
real*4 FFlux_1 ! (mW/m2) ? Observed-frame full flux (5)
real*4 e_FFlux_1 ! (mW/m2) [-99/]? The 84% confidence level in FFlux
character*3 XName ! Lower energy X-ray counterpart observatory name
real*8 RAXdeg_1 ! (deg) ? Lower energy X-ray counterpart Right Ascension
* in decimal degrees (J2000)
real*8 DEXdeg_1 ! (deg) ? Lower energy X-ray counterpart Declination
* in decimal degrees (J2000)
character*4 OName ! Other, optical or WISE, counterpart
* observatory name
real*8 RAOdeg_1 ! (deg) ? Other counterpart Right Ascension in
* decimal degrees (J2000)
real*8 DEOdeg_1 ! (deg) ? Other counterpart Declination in
* decimal degrees (J2000)
real*4 zsp_1 ! [0/1.9]? Spectroscopic redshift (6)
real*4 XLum_1 ! (10-7W) ? Non-absorption-corrected, rest-frame
* 10-40keV luminosity (7)
character*1 Fl ! Primary catalog code (8)
*Note (1): Calculated at the source coordinates. The values are
* non-aperture-corrected.
*Note (2): For the net source counts, we give 90% CL upper limits for sources
* not detected in a given band. Throughout the table, upper limits are
* flagged with a -99 value in the error column. The photometric columns
* are blank where the A+B data prohibit reliable photometric
* constraints.
*Note (3): The average net, vignetting-corrected exposure time at the source
* coordinates. These correspond to the A+B data, so should be divided
* by two to obtain the average exposure per FPM.
*Note (4): Determined from the photometric values and the exposure times.
*Note (5): After deblending has been performed. These are aperture corrected
* values (i.e., they correspond to the full NuSTAR PSF), and are
* calculated from the count rates using the conversion factors
* listed in Section 2.4.
*Note (6): The large majority of the redshifts were obtained through our own
* campaign of ground-based spectroscopic followup of NuSTAR
* serendipitous survey sources (see Section 3.3.1 and
* the "Description" section above).
*Note (7): Estimated from the observed-frame fluxes, following the procedure
* outlined in Section 2.4. Negative values indicate upper limits. The
* luminosities are observed values, uncorrected for any absorption
* along the line of sight. The intrinsic luminosities may therefore
* be higher, for highly absorbed AGNs.
*Note (8): A character indicating the reason for not being included in the
* primary catalog. These are categorised into four groups as follows:
* E = the source is within or very close to the peripheral region of the NuSTAR
* mosaic, which is excluded from the primary source detection (33% of
* cases);
* T = the source is narrowly offset from the central science target position
* for the NuSTAR observation (and thus automatically excluded;
* see Section 2.3), or from another bright source in the field (11%);
* X = the source lies in a region which is masked out, or in a NuSTAR field
* which is excluded, from the primary source detection (44%; e.g., due to
* highly contaminating stray light or a bright science target); or
* L = the source has a comparatively low detection significance (12%).
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table8.dat' ! Summary of the optical spectroscopy for
the secondary catalog sources
integer*4 nr__4
parameter (nr__4=46) ! Number of records
character*234 ar__4 ! Full-size record
integer*4 Seq_3 ! [1/498] Unique source identification number
character*14 NuSTAR_3 ! Unique NuSTAR source name (JHHMMSS+DDMM.m)
real*4 z_1 ! [0/3.5]? Source spectroscopic redshift
character*7 Type_1 ! Classification (1)
character*122 Lines_1 ! Emission/absorption lines identified (2)
character*68 Notes_1 ! Source notes and literature spectra references
character*2 Run_1 ! Unique observing run identification number (3)
*Note (1): Classification (for primary sources) as follows:
* BL = broad-line AGN (151 occurrences + 11 BL?)
* NL = narrow-line AGN (84 occurrences + 13 NL?)
* BL Lac? = BL Lac object candidate (1 occurrence)
* Gal = Galactic objects (z=0; 16 occurrences)
*
* See Section 3.3.2 for further details.
*Note (2): Absorption line/feature marked with "dg" footnote.
*Note (3): As defined in Table 4 ("S" and "L" mark spectra obtained from the
* SDSS and from elsewhere in the literature, respectively).
C=============================================================================
C Loading file 'table1.dat' ! Details of the individual NuSTAR observations which
* make up the serendipitous survey
C Format for file interpretation
1 format(
+ A4,1X,A23,1X,I2,1X,I11,1X,A10,1X,F6.2,1X,F6.2,1X,F6.1,1X,I2,
+ 1X,I1,1X,I1)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,591
read(1,'(A82)')ar__
read(ar__,1)
+ Field,Target,NObs,ObsID,Date,RAdeg,DEdeg,Exp,N,A15,H16
if(ar__(30:31) .EQ. '') NObs = iNULL__
if(ar__(33:43) .EQ. '') ObsID = iNULL__
if(ar__(56:61) .EQ. '') RAdeg = rNULL__
if(ar__(63:68) .EQ. '') DEdeg = rNULL__
if(ar__(77:78) .EQ. '') N = iNULL__
if(ar__(80:80) .EQ. '') A15 = iNULL__
if(ar__(82:82) .EQ. '') H16 = iNULL__
c ..............Just test output...........
write(6,1)
+ Field,Target,NObs,ObsID,Date,RAdeg,DEdeg,Exp,N,A15,H16
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table5.dat' ! The primary NuSTAR serendipitous source catalog
C Format for file interpretation
2 format(
+ I3,7X,A14,1X,F10.6,1X,F10.6,1X,I1,1X,I1,1X,I1,1X,I1,1X,I1,1X,
+ I1,1X,F8.3,1X,F8.3,1X,F8.3,1X,F8.3,1X,F8.3,1X,F8.3,1X,I1,1X,
+ F7.1,1X,F7.3,1X,F8.3,1X,F8.3,1X,F7.3,1X,F6.1,1X,F6.3,1X,F8.3,
+ 1X,F8.3,1X,F7.3,1X,F7.1,1X,F7.3,1X,F8.3,1X,F9.3,1X,F7.3,1X,
+ F7.1,1X,F8.3,1X,F8.3,1X,F7.3,1X,F6.1,1X,F8.3,1X,F8.3,1X,F7.3,
+ 1X,F7.1,1X,F8.3,1X,F9.3,1X,F7.3,1X,F9.1,1X,F9.1,1X,F9.1,1X,
+ E9.3,1X,E9.3,1X,E9.3,1X,E9.3,1X,E10.3,1X,E9.3,1X,E9.3,1X,E9.3,
+ 1X,E9.3,1X,E10.3,1X,E9.3,1X,E9.3,1X,E9.3,1X,E9.3,1X,E10.3,1X,
+ E9.3,1X,E10.3,1X,E9.3,1X,E10.3,1X,E9.3,1X,E10.3,1X,F5.3,1X,
+ F7.3,1X,F7.3,1X,F6.3,1X,F7.3,1X,F7.3,1X,E9.3,1X,E10.3,1X,E9.3,
+ 1X,E10.3,1X,E9.3,1X,E10.3,1X,A8,1X,F10.6,1X,F10.6,1X,F5.2,1X,
+ E9.3,1X,E9.3,1X,F10.6,1X,F10.6,1X,F5.3,1X,F6.3,1X,F5.3,1X,
+ F6.3,1X,F5.3,1X,F6.3,1X,F5.3,1X,F6.3,1X,F5.3,1X,A9,1X,F12.8,
+ 1X,F12.8,1X,F5.3,1X,F7.3,1X,F5.3,1X,E10.3,1X,I1,1X,I1)
C Effective file loading
open(unit=1,status='old',file=
+'table5.dat')
write(6,*) '....Loading file: table5.dat'
do i__=1,498
read(1,'(A903)')ar__1
read(ar__1,2)
+ Seq,NuSTAR,RAdeg_1,DEdeg_1,SFl,HFl,FFl,SdbFl,HdbFl,FdbFl,
+ logSP,logHP,logFP,logSdbP,logHdbP,logFdbP,dbFl,Scts,e_Scts,
+ SBck,SNet,e_SNet,Hcts,e_Hcts,HBck,HNet,e_HNet,Fcts,e_Fcts,
+ FBck,FNet,e_FNet,Sdbcts,e_Sdbcts,SdbNet,e_SdbNet,Hdbcts,
+ e_Hdbcts,HdbNet,e_HdbNet,Fdbcts,e_Fdbcts,FdbNet,e_FdbNet,Sexp,
+ Hexp,Fexp,SCR,e_SCR,SCRBck,SNCR,e_SNCR,HCR,e_HCR,HCRBck,HNCR,
+ e_HNCR,FCR,e_FCR,FCRBck,FNCR,e_FNCR,SdbNCR,e_SdbNCR,HdbNCR,
+ e_HdbNCR,FdbNCR,e_FdbNCR,H_S,E_H_S,e_H_S_1,gamma,E_gamma,
+ e_gamma_1,SFlux,e_SFlux,HFlux,e_HFlux,FFlux,e_FFlux,XOrig,
+ RAXdeg,DEXdeg,XOff,XFlux,XTFlux,RAWdeg,DEWdeg,IROff,W1mag,
+ e_W1mag,W2mag,e_W2mag,W3mag,e_W3mag,W4mag,e_W4mag,OOrig,
+ RAOdeg,DEOdeg,OOff,Rmag,zsp,XLum,PFl,A15Fl
if(ar__1(611:616) .EQ. '') gamma = rNULL__
if(ar__1(618:624) .EQ. '') E_gamma = rNULL__
if(ar__1(626:632) .EQ. '') e_gamma_1 = rNULL__
if(ar__1(706:715) .EQ. '') RAXdeg = rNULL__
if(ar__1(717:726) .EQ. '') DEXdeg = rNULL__
if(ar__1(728:732) .EQ. '') XOff = rNULL__
if(ar__1(734:742) .EQ. '') XFlux = rNULL__
if(ar__1(744:752) .EQ. '') XTFlux = rNULL__
if(ar__1(754:763) .EQ. '') RAWdeg = rNULL__
if(ar__1(765:774) .EQ. '') DEWdeg = rNULL__
if(ar__1(776:780) .EQ. '') IROff = rNULL__
if(ar__1(782:787) .EQ. '') W1mag = rNULL__
if(ar__1(789:793) .EQ. '') e_W1mag = rNULL__
if(ar__1(795:800) .EQ. '') W2mag = rNULL__
if(ar__1(802:806) .EQ. '') e_W2mag = rNULL__
if(ar__1(808:813) .EQ. '') W3mag = rNULL__
if(ar__1(815:819) .EQ. '') e_W3mag = rNULL__
if(ar__1(821:826) .EQ. '') W4mag = rNULL__
if(ar__1(828:832) .EQ. '') e_W4mag = rNULL__
if(ar__1(844:855) .EQ. '') RAOdeg = rNULL__
if(ar__1(857:868) .EQ. '') DEOdeg = rNULL__
if(ar__1(870:874) .EQ. '') OOff = rNULL__
if(ar__1(876:882) .EQ. '') Rmag = rNULL__
if(ar__1(884:888) .EQ. '') zsp = rNULL__
if(ar__1(890:899) .EQ. '') XLum = rNULL__
c ..............Just test output...........
write(6,2)
+ Seq,NuSTAR,RAdeg_1,DEdeg_1,SFl,HFl,FFl,SdbFl,HdbFl,FdbFl,
+ logSP,logHP,logFP,logSdbP,logHdbP,logFdbP,dbFl,Scts,e_Scts,
+ SBck,SNet,e_SNet,Hcts,e_Hcts,HBck,HNet,e_HNet,Fcts,e_Fcts,
+ FBck,FNet,e_FNet,Sdbcts,e_Sdbcts,SdbNet,e_SdbNet,Hdbcts,
+ e_Hdbcts,HdbNet,e_HdbNet,Fdbcts,e_Fdbcts,FdbNet,e_FdbNet,Sexp,
+ Hexp,Fexp,SCR,e_SCR,SCRBck,SNCR,e_SNCR,HCR,e_HCR,HCRBck,HNCR,
+ e_HNCR,FCR,e_FCR,FCRBck,FNCR,e_FNCR,SdbNCR,e_SdbNCR,HdbNCR,
+ e_HdbNCR,FdbNCR,e_FdbNCR,H_S,E_H_S,e_H_S_1,gamma,E_gamma,
+ e_gamma_1,SFlux,e_SFlux,HFlux,e_HFlux,FFlux,e_FFlux,XOrig,
+ RAXdeg,DEXdeg,XOff,XFlux,XTFlux,RAWdeg,DEWdeg,IROff,W1mag,
+ e_W1mag,W2mag,e_W2mag,W3mag,e_W3mag,W4mag,e_W4mag,OOrig,
+ RAOdeg,DEOdeg,OOff,Rmag,zsp,XLum,PFl,A15Fl
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table6.dat' ! Summary of the optical spectroscopy for the NuSTAR
* serendipitous survey sources
C Format for file interpretation
3 format(I3,7X,A14,1X,F5.3,1X,A7,2X,A122,1X,A68,1X,A2)
C Effective file loading
open(unit=1,status='old',file=
+'table6.dat')
write(6,*) '....Loading file: table6.dat'
do i__=1,303
read(1,'(A234)')ar__2
read(ar__2,3)Seq_1,NuSTAR_1,z,Type,Lines,Notes,Run
if(ar__2(26:30) .EQ. '') z = rNULL__
c ..............Just test output...........
write(6,3)Seq_1,NuSTAR_1,z,Type,Lines,Notes,Run
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table7.dat' ! The secondary NuSTAR serendipitous source catalog
C Format for file interpretation
4 format(
+ I2,7X,A14,1X,F10.6,1X,F10.6,1X,F8.3,1X,F8.3,1X,F8.3,1X,F7.3,
+ 1X,F8.3,1X,F8.3,1X,F8.3,1X,F7.3,1X,F9.3,1X,F8.3,1X,F9.3,1X,
+ F7.3,1X,F8.1,1X,F8.1,1X,F8.1,1X,E9.3,1X,E10.3,1X,E9.3,1X,
+ E10.3,1X,E9.3,1X,E10.3,1X,E9.3,1X,E10.3,1X,E9.3,1X,E10.3,1X,
+ E9.3,1X,E10.3,1X,A3,1X,F10.6,1X,F10.6,1X,A4,1X,F10.6,1X,F10.6,
+ 1X,F5.3,1X,E10.3,1X,A1)
C Effective file loading
open(unit=1,status='old',file=
+'table7.dat')
write(6,*) '....Loading file: table7.dat'
do i__=1,64
read(1,'(A377)')ar__3
read(ar__3,4)
+ Seq_2,NuSTAR_2,RAdeg_2,DEdeg_2,Scts_1,SBck_1,SNet_1,e_SNet_1,
+ Hcts_1,HBck_1,HNet_1,e_HNet_1,Fcts_1,FBck_1,FNet_1,e_FNet_1,
+ Sexp_1,Hexp_1,Fexp_1,SNCR_1,e_SNCR_1,HNCR_1,e_HNCR_1,FNCR_1,
+ e_FNCR_1,SFlux_1,e_SFlux_1,HFlux_1,e_HFlux_1,FFlux_1,
+ e_FFlux_1,XName,RAXdeg_1,DEXdeg_1,OName,RAOdeg_1,DEOdeg_1,
+ zsp_1,XLum_1,Fl
if(ar__3(47:54) .EQ. '') Scts_1 = rNULL__
if(ar__3(56:63) .EQ. '') SBck_1 = rNULL__
if(ar__3(65:72) .EQ. '') SNet_1 = rNULL__
if(ar__3(74:80) .EQ. '') e_SNet_1 = rNULL__
if(ar__3(82:89) .EQ. '') Hcts_1 = rNULL__
if(ar__3(91:98) .EQ. '') HBck_1 = rNULL__
if(ar__3(100:107) .EQ. '') HNet_1 = rNULL__
if(ar__3(109:115) .EQ. '') e_HNet_1 = rNULL__
if(ar__3(117:125) .EQ. '') Fcts_1 = rNULL__
if(ar__3(127:134) .EQ. '') FBck_1 = rNULL__
if(ar__3(136:144) .EQ. '') FNet_1 = rNULL__
if(ar__3(146:152) .EQ. '') e_FNet_1 = rNULL__
if(ar__3(154:161) .EQ. '') Sexp_1 = rNULL__
if(ar__3(163:170) .EQ. '') Hexp_1 = rNULL__
if(ar__3(172:179) .EQ. '') Fexp_1 = rNULL__
if(ar__3(181:189) .EQ. '') SNCR_1 = rNULL__
if(ar__3(191:200) .EQ. '') e_SNCR_1 = rNULL__
if(ar__3(202:210) .EQ. '') HNCR_1 = rNULL__
if(ar__3(212:221) .EQ. '') e_HNCR_1 = rNULL__
if(ar__3(223:231) .EQ. '') FNCR_1 = rNULL__
if(ar__3(233:242) .EQ. '') e_FNCR_1 = rNULL__
if(ar__3(244:252) .EQ. '') SFlux_1 = rNULL__
if(ar__3(254:263) .EQ. '') e_SFlux_1 = rNULL__
if(ar__3(265:273) .EQ. '') HFlux_1 = rNULL__
if(ar__3(275:284) .EQ. '') e_HFlux_1 = rNULL__
if(ar__3(286:294) .EQ. '') FFlux_1 = rNULL__
if(ar__3(296:305) .EQ. '') e_FFlux_1 = rNULL__
if(ar__3(311:320) .EQ. '') RAXdeg_1 = rNULL__
if(ar__3(322:331) .EQ. '') DEXdeg_1 = rNULL__
if(ar__3(338:347) .EQ. '') RAOdeg_1 = rNULL__
if(ar__3(349:358) .EQ. '') DEOdeg_1 = rNULL__
if(ar__3(360:364) .EQ. '') zsp_1 = rNULL__
if(ar__3(366:375) .EQ. '') XLum_1 = rNULL__
c ..............Just test output...........
write(6,4)
+ Seq_2,NuSTAR_2,RAdeg_2,DEdeg_2,Scts_1,SBck_1,SNet_1,e_SNet_1,
+ Hcts_1,HBck_1,HNet_1,e_HNet_1,Fcts_1,FBck_1,FNet_1,e_FNet_1,
+ Sexp_1,Hexp_1,Fexp_1,SNCR_1,e_SNCR_1,HNCR_1,e_HNCR_1,FNCR_1,
+ e_FNCR_1,SFlux_1,e_SFlux_1,HFlux_1,e_HFlux_1,FFlux_1,
+ e_FFlux_1,XName,RAXdeg_1,DEXdeg_1,OName,RAOdeg_1,DEOdeg_1,
+ zsp_1,XLum_1,Fl
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table8.dat' ! Summary of the optical spectroscopy for
* the secondary catalog sources
C Format for file interpretation
5 format(I3,7X,A14,1X,F5.3,1X,A7,2X,A122,1X,A68,1X,A2)
C Effective file loading
open(unit=1,status='old',file=
+'table8.dat')
write(6,*) '....Loading file: table8.dat'
do i__=1,46
read(1,'(A234)')ar__4
read(ar__4,5)Seq_3,NuSTAR_3,z_1,Type_1,Lines_1,Notes_1,Run_1
if(ar__4(26:30) .EQ. '') z_1 = rNULL__
c ..............Just test output...........
write(6,5)Seq_3,NuSTAR_3,z_1,Type_1,Lines_1,Notes_1,Run_1
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end