Conversion of standardized ReadMe file for
file /./ftp/cats/J/AJ/123/2223 into FORTRAN code for loading all data files into arrays.
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-Mar-28 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/AJ/123/2223 SPICES II: CHANDRA observations of Lynx (Stern+, 2002) *================================================================================ *SPICES II: optical and near-infrared identifications of faint X-ray sources *from deep CHANDRA observations of Lynx. * Stern D., Tozzi P., Stanford S.A., Rosati P., Holden B., Eisenhardt P., * Elston R., Wu K.L., Connolly A., Spinrad H., Dawson S., Dey A., Chaffee F.H. * <Astron. J. 123, 2223 (2002)> * =2002AJ....123.2223S C============================================================================= C Internal variables integer*4 i__ c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table1.dat' ! X-ray source properties integer*4 nr__ parameter (nr__=153) ! Number of records character*85 ar__ ! Full-size record C J2000.0 position composed of: RAh RAm RAs DE- DEd DEm DEs real*8 RAdeg (nr__) ! (deg) Right Ascension J2000.0 real*8 DEdeg (nr__) ! (deg) Declination J2000.0 C ---------------------------------- ! (position vector(s) in degrees) integer*4 v_STS2002_ (nr__) ! Sequential number integer*4 RAh (nr__) ! (h) Right ascension (J2000.0) integer*4 RAm (nr__) ! (min) Right ascension (J2000.0) real*4 RAs (nr__) ! (s) Right ascension (J2000.0) character*1 DE_ (nr__) ! Declination sign (J2000.0) integer*4 DEd (nr__) ! (deg) Declination (J2000.0) integer*4 DEm (nr__) ! (arcmin) Declination (J2000.0) real*4 DEs (nr__) ! (arcsec) Declination (J2000.0) real*8 Scounts (nr__) ! (ct) ? Counts in the soft band (0.5-2keV) real*4 e_Scounts (nr__) ! (ct) ? rms uncertainty on Scounts real*4 Hcounts (nr__) ! (ct) ? Counts in the hard band (2-7keV) real*4 e_Hcounts (nr__) ! (ct) ? rms uncertainty on Hcounts real*4 HR (nr__) ! ? Hardness ratio (H-S)/(H+S) real*4 S_N (nr__) ! Signal-to-noise ratio of the X-ray detection real*4 Dist (nr__) ! (arcmin) Off-axis angle of the X-ray source (1) real*4 S0_5_2keV (nr__) ! (10-18W/m2) ? Flux in the soft band (0.5-2keV) real*4 S2_10keV (nr__) ! (10-18W/m2) ? Flux in the hard band (2-10keV) *Note (1): Offset from the nominal pointing direction. c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table2.dat' ! Optical/Near-IR Properties of X-Ray Sources integer*4 nr__1 parameter (nr__1=106) ! Number of records character*93 ar__1 ! Full-size record integer*4 v_STS2002__1(nr__1) ! Source identification number character*1 f__STS2002_(nr__1) ! [a] Flag on [STS2002] (1) real*4 oRA (nr__1) ! (arcsec) ? X-ray minus optical right ascension offset character*1 f_oRA (nr__1) ! [u] Indicates undetected source real*4 oDE (nr__1) ! (arcsec) ? X-ray minus optical declination offset character*1 f_oDE (nr__1) ! [u] Indicates undetected source real*4 Bmag (nr__1) ! (mag) ? The Harris B band magnitude (3) character*1 f_Bmag (nr__1) ! [u] Indicates undetected source real*4 Rmag (nr__1) ! (mag) ? The Harris R band magnitude (3) character*1 f_Rmag (nr__1) ! [u] Indicates undetected source character*1 u_Rmag (nr__1) ! [:] Indicates Rmag somewhat affected by nearby * stellar bleed trail real*4 Imag (nr__1) ! (mag) ? The Harris I band magnitude (3) character*1 f_Imag (nr__1) ! [u] Indicates undetected source real*4 zmag (nr__1) ! (mag) ? The RG850 long-pass z band magnitude character*1 f_zmag (nr__1) ! [u] Indicates undetected source real*4 Jmag (nr__1) ! (mag) ? The J band magnitude (4) character*1 f_Jmag (nr__1) ! [u] Indicates undetected source real*4 Ksmag (nr__1) ! (mag) ? The K_s_ band magnitude (4) character*1 f_Ksmag (nr__1) ! [u] Indicates undetected source real*4 z (nr__1) ! ? Spectroscopic redshift character*1 f_z (nr__1) ! [u] Indicates undetected source character*12 SID (nr__1) ! The SPICES identification *Note (1): Indicates host is more than 1.5" away from faint X-ray source. *Note (3): Sources with bad photometry, due either to source saturation or * contamination from the stellar bleed trail of a nearby, bright source, * are listed as 99.00. * The Harris passbands are: * B-band: {lambda}_c_ = 431.3nm D{lambda} = 106.9nm * R-band: {lambda}_c_ = 645.8nm D{lambda} = 147.2nm * I-band: {lambda}_c_ = 820.4nm D{lambda} = 182.1nm *Note (4): Only those sources contained within the near-infrared field are * tabulated under the near-infrared photometry columns. Sources with bad * photometry, due either to source saturation or contamination from the * stellar bleed trail of a nearby, bright source, are listed as 99.00. c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table3.dat' ! Luminosities of X-ray sources integer*4 nr__2 parameter (nr__2=18) ! Number of records character*67 ar__2 ! Full-size record integer*4 v_STS2002__2(nr__2) ! Sequential number real*4 z_1 (nr__2) ! Redshift real*4 BMAG_E (nr__2) ! (mag) ? EdS rest-frame absolute B magnitude (1) real*4 log_L0_5_2keV_E(nr__2) ! ([solLum]) ? EdS 0.5-2keV band luminosity (1) real*4 log_L2_10keV_E(nr__2) ! ([solLum]) ? EdS 2-10keV band luminosity (1) real*4 BMAG_L (nr__2) ! (mag) ? {Lambda} rest-frame absolute B * magnitude (1) real*4 log_L0_5_2keV_L(nr__2) ! ([solLum]) ? {Lambda} 0.5-2keV band luminosity (1) real*4 log_L2_10keV_L(nr__2) ! ([solLum]) ? {Lambda} 2-10keV band luminosity (1) character*20 Class (nr__2) ! Galaxy class or spectral type for stars *Note (1): We adopt {Gamma}=1.4 for calculation of X-ray k-corrections. * EdS: Einstein-de Sitter universe with * H_0_=50km/s/Mpc, {Omega}_M_=1, {Omega}_{Lambda}_=0 * {Lambda}: dark energy cosmology with * H_0_=65km/s/Mpc, {Omega}_M_=0.35, {Omega}_{Lambda}_=0.65 C============================================================================= C Loading file 'table1.dat' ! X-ray source properties C Format for file interpretation 1 format( + I3,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F7.2,1X,F5.2, + 1X,F6.2,1X,F5.2,1X,F5.2,1X,F4.1,1X,F5.2,1X,F6.2,1X,F6.2) C Effective file loading open(unit=1,status='old',file= +'table1.dat') write(6,*) '....Loading file: table1.dat' do i__=1,153 read(1,'(A85)')ar__ read(ar__,1) + v_STS2002_(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__), + DEm(i__),DEs(i__),Scounts(i__),e_Scounts(i__),Hcounts(i__), + e_Hcounts(i__),HR(i__),S_N(i__),Dist(i__),S0_5_2keV(i__), + S2_10keV(i__) if(ar__(29:35) .EQ. '') Scounts(i__) = rNULL__ if(ar__(37:41) .EQ. '') e_Scounts(i__) = rNULL__ if(ar__(43:48) .EQ. '') Hcounts(i__) = rNULL__ if(ar__(50:54) .EQ. '') e_Hcounts(i__) = rNULL__ if(ar__(56:60) .EQ. '') HR(i__) = rNULL__ if(ar__(73:78) .EQ. '') S0_5_2keV(i__) = rNULL__ if(ar__(80:85) .EQ. '') S2_10keV(i__) = rNULL__ RAdeg(i__) = rNULL__ DEdeg(i__) = rNULL__ c Derive coordinates RAdeg and DEdeg from input data c (RAdeg and DEdeg are set to rNULL__ when unknown) if(RAh(i__) .GT. -180) RAdeg(i__)=RAh(i__)*15. if(RAm(i__) .GT. -180) RAdeg(i__)=RAdeg(i__)+RAm(i__)/4. if(RAs(i__) .GT. -180) RAdeg(i__)=RAdeg(i__)+RAs(i__)/240. if(DEd(i__) .GE. 0) DEdeg(i__)=DEd(i__) if(DEm(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEm(i__)/60. if(DEs(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEs(i__)/3600. if(DE_(i__).EQ.'-'.AND.DEdeg(i__).GE.0) DEdeg(i__)=-DEdeg(i__) c ..............Just test output........... write(6,1) + v_STS2002_(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__), + DEm(i__),DEs(i__),Scounts(i__),e_Scounts(i__),Hcounts(i__), + e_Hcounts(i__),HR(i__),S_N(i__),Dist(i__),S0_5_2keV(i__), + S2_10keV(i__) write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'table2.dat' ! Optical/Near-IR Properties of X-Ray Sources C Format for file interpretation 2 format( + I3,1X,A1,2X,F5.2,1X,A1,1X,F5.2,1X,A1,1X,F5.2,1X,A1,1X,F5.2,1X, + A1,1X,A1,1X,F5.2,1X,A1,1X,F5.2,1X,A1,1X,F5.2,1X,A1,1X,F5.2,1X, + A1,1X,F5.3,1X,A1,1X,A12) C Effective file loading open(unit=1,status='old',file= +'table2.dat') write(6,*) '....Loading file: table2.dat' do i__=1,106 read(1,'(A93)')ar__1 read(ar__1,2) + v_STS2002__1(i__),f__STS2002_(i__),oRA(i__),f_oRA(i__), + oDE(i__),f_oDE(i__),Bmag(i__),f_Bmag(i__),Rmag(i__), + f_Rmag(i__),u_Rmag(i__),Imag(i__),f_Imag(i__),zmag(i__), + f_zmag(i__),Jmag(i__),f_Jmag(i__),Ksmag(i__),f_Ksmag(i__), + z(i__),f_z(i__),SID(i__) if(ar__1(8:12) .EQ. '') oRA(i__) = rNULL__ if(ar__1(16:20) .EQ. '') oDE(i__) = rNULL__ if(ar__1(24:28) .EQ. '') Bmag(i__) = rNULL__ if(ar__1(32:36) .EQ. '') Rmag(i__) = rNULL__ if(ar__1(42:46) .EQ. '') Imag(i__) = rNULL__ if(ar__1(50:54) .EQ. '') zmag(i__) = rNULL__ if(ar__1(58:62) .EQ. '') Jmag(i__) = rNULL__ if(ar__1(66:70) .EQ. '') Ksmag(i__) = rNULL__ if(ar__1(74:78) .EQ. '') z(i__) = rNULL__ c ..............Just test output........... write(6,2) + v_STS2002__1(i__),f__STS2002_(i__),oRA(i__),f_oRA(i__), + oDE(i__),f_oDE(i__),Bmag(i__),f_Bmag(i__),Rmag(i__), + f_Rmag(i__),u_Rmag(i__),Imag(i__),f_Imag(i__),zmag(i__), + f_zmag(i__),Jmag(i__),f_Jmag(i__),Ksmag(i__),f_Ksmag(i__), + z(i__),f_z(i__),SID(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'table3.dat' ! Luminosities of X-ray sources C Format for file interpretation 3 format( + I3,1X,F5.3,2X,F5.1,1X,F5.2,1X,F5.2,1X,F5.1,1X,F5.2,1X,F5.2,1X, + A20) C Effective file loading open(unit=1,status='old',file= +'table3.dat') write(6,*) '....Loading file: table3.dat' do i__=1,18 read(1,'(A67)')ar__2 read(ar__2,3) + v_STS2002__2(i__),z_1(i__),BMAG_E(i__),log_L0_5_2keV_E(i__), + log_L2_10keV_E(i__),BMAG_L(i__),log_L0_5_2keV_L(i__), + log_L2_10keV_L(i__),Class(i__) if(ar__2(12:16) .EQ. '') BMAG_E(i__) = rNULL__ if(ar__2(18:22) .EQ. '') log_L0_5_2keV_E(i__) = rNULL__ if(ar__2(24:28) .EQ. '') log_L2_10keV_E(i__) = rNULL__ if(ar__2(30:34) .EQ. '') BMAG_L(i__) = rNULL__ if(ar__2(36:40) .EQ. '') log_L0_5_2keV_L(i__) = rNULL__ if(ar__2(42:46) .EQ. '') log_L2_10keV_L(i__) = rNULL__ c ..............Just test output........... write(6,3) + v_STS2002__2(i__),z_1(i__),BMAG_E(i__),log_L0_5_2keV_E(i__), + log_L2_10keV_E(i__),BMAG_L(i__),log_L0_5_2keV_L(i__), + log_L2_10keV_L(i__),Class(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= stop end