FORTRAN Generation
(/./ftp/cats/J/ApJ/687/1019)

Conversion of standardized ReadMe file for file /./ftp/cats/J/ApJ/687/1019 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 2026-May-19
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/687/1019         Chandra X-ray observations of M71         (Elsner+, 2008)
*================================================================================
*Chandra X-ray observatory observations of the globular cluster M71.
*    Elsner R.F., Heinke C.O., Cohn H.N., Lugger P.M., Maxwell J.E.,
*    Stairs I.H., Ransom S.M., Hessels J.W.T., Becker W., Huang R.H.H.,
*    Edmonds P.D., Grindlay J.E., Bogdanov S., Ghosh K., Weisskopf M.C.
*   <Astrophys. J., 687, 1019-1034 (2008)>
*   =2008ApJ...687.1019E
C=============================================================================

C  Internal variables

      integer*4 i__

c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - 

C  Declarations for 'table1.dat'	! Chandra X-ray sources detected with r_M71_<=2r_h_

      integer*4 nr__
      parameter (nr__=68)	! Number of records
      character*119 ar__   	! Full-size record

C  J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
      real*8        RAdeg      (nr__) ! (deg) Right Ascension J2000
      real*8        DEdeg      (nr__) ! (deg)     Declination J2000
C  ---------------------------------- ! (position vector(s) in degrees)

      character*3   rl         (nr__) ! Half-mass radius (r_h_) limits (1)
      character*4   ID         (nr__) ! Source identification (<[EHC2008] [s/i]sNN> in
*                               Simbad)
      character*1   f_ID       (nr__) ! [j] Flag for s55 (in table 1) (2)
      integer*4     RAh        (nr__) ! (h) Hour of right ascension (J2000)
      integer*4     RAm        (nr__) ! (min) Minute of right ascension (J2000)
      real*4        RAs        (nr__) ! (s) Second of right ascension (J2000)
      character*1   DE_        (nr__) ! Declination sign (J2000)
      integer*4     DEd        (nr__) ! (deg) Degree of declination (J2000)
      integer*4     DEm        (nr__) ! (arcmin) Arcminute of declination (J2000)
      real*4        DEs        (nr__) ! (arcsec) Arcsecond of declination (J2000)
      real*4        re         (nr__) ! (arcsec) Radius of the detect cell for collecting X-ray
*                               counts
      real*4        Cx         (nr__) ! Number of 0.3-8.0keV source counts collected
*                               in the detect cell
      real*4        SigX       (nr__) ! (arcsec) Radius enclosing the true source position
*                               with 68% confidence (3)
      character*5   Chip       (nr__) ! (arcmin) CCD on which the X-ray source appears (only
*                               for table 2) (4)
      real*4        rM71       (nr__) ! (arcmin) ? Radius from the nominal center of the
*                               cluster (J19:53:46.1+18:46:42; only for table 1)
      real*4        off        (nr__) ! (arcsec) ? Radial offset of candidate counterparts (5)
      real*4        Jmag       (nr__) ! (mag) ? J magnitude of a candidate counterpart
*                               found in the 2MASS catalog (5)
      real*4        R1mag      (nr__) ! (mag) ? R1 magnitude of a candidate counterpart
*                               found in the USNO-B1.0 catalog (5)
      real*4        R2mag      (nr__) ! (mag) ? R2 magnitude of a candidate counterpart
*                               found in the USNO-B1.0 catalog (5)
      real*4        Vmag       (nr__) ! (mag) ? VT magnitude of a candidate counterpart
*                               found in the Tycho-2 catalog (5)
      real*8        Prob       (nr__) ! (%) ? Probability of chance coincidence (5)(6)
      character*17  Com        (nr__) ! Comment (counterpart or location)
*Note (1): Limits as follows:
*    rh = sources with r_M71_<=r_h_;
*   2rh = sources with r_h_<r_M71_<=2r_h_;
*    t2 = sources with 2r_h_<=r_M71_ (table 2)
*Note (2):
*     j = This source is on the S2 front-side CCD. All other sources in this
*         table are on the S3 back-side CCD.
*Note (3): The corresponding radii for inclusion with 95% or 99% confidence are
*          found by multiplying this column by 1.62 or 2.01, respectively.
*Note (4): In a few cases, the source is dithered across the gap between CCDs.
*Note (5): Found by searching the HEASARC 2MASS (see
*          http://www.ipac.caltech.edu/2mass/; Cat. II/246), USNO-B1.0
*          (Monet et al. 2003; Cat. I/284), and Tycho-2 (Hog et al. 2000,
*          Cat. I/259) catalogs, requiring that the candidate counterpart lie
*          within the 99% confidence radius of a Chandra source.
*          There are 6414 and 3376 2MASS sources, 15324 and 9196 USNO sources,
*          and 7 and 9 Tycho sources appearing within the S2-S3-S4 and I2-I3
*          boundaries shown in Figures 3 and 4, respectively.
*          If blank, no candidate counterpart was found in these catalogs. (See
*          section 6.1 for further details).
*Note (6): The percent probability of a chance coincidence is calculated from:
*          P_coinc_=N(<m){pi}r^2^_99_/A_search_ where N(<m) is the number of
*          sources in the corresponding catalog inside the search area,
*          A_search_, with a magnitude smaller than that of the candidate
*          counterpart, and r_99_ is the radius enclosing the X-ray source
*          location with 99% confidence.

c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - 

C  Declarations for 'table2.dat'	! Chandra X-ray sources detected with 2r_h_>=r_M71_

      integer*4 nr__1
      parameter (nr__1=97)	! Number of records
      character*119 ar__1  	! Full-size record

C  J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
      real*8        RAdeg_1    (nr__1) ! (deg) Right Ascension J2000
      real*8        DEdeg_1    (nr__1) ! (deg)     Declination J2000
C  ---------------------------------- ! (position vector(s) in degrees)

      character*3   rl_1       (nr__1) ! Half-mass radius (r_h_) limits (1)
      character*4   ID_1       (nr__1) ! Source identification (<[EHC2008] [s/i]sNN> in
*                               Simbad)
      character*1   f_ID_1     (nr__1) ! [j] Flag for s55 (in table 1) (2)
      integer*4     RAh_1      (nr__1) ! (h) Hour of right ascension (J2000)
      integer*4     RAm_1      (nr__1) ! (min) Minute of right ascension (J2000)
      real*4        RAs_1      (nr__1) ! (s) Second of right ascension (J2000)
      character*1   DE__1      (nr__1) ! Declination sign (J2000)
      integer*4     DEd_1      (nr__1) ! (deg) Degree of declination (J2000)
      integer*4     DEm_1      (nr__1) ! (arcmin) Arcminute of declination (J2000)
      real*4        DEs_1      (nr__1) ! (arcsec) Arcsecond of declination (J2000)
      real*4        re_1       (nr__1) ! (arcsec) Radius of the detect cell for collecting X-ray
*                               counts
      real*4        Cx_1       (nr__1) ! Number of 0.3-8.0keV source counts collected
*                               in the detect cell
      real*4        SigX_1     (nr__1) ! (arcsec) Radius enclosing the true source position
*                               with 68% confidence (3)
      character*5   Chip_1     (nr__1) ! (arcmin) CCD on which the X-ray source appears (only
*                               for table 2) (4)
      real*4        rM71_1     (nr__1) ! (arcmin) ? Radius from the nominal center of the
*                               cluster (J19:53:46.1+18:46:42; only for table 1)
      real*4        off_1      (nr__1) ! (arcsec) ? Radial offset of candidate counterparts (5)
      real*4        Jmag_1     (nr__1) ! (mag) ? J magnitude of a candidate counterpart
*                               found in the 2MASS catalog (5)
      real*4        R1mag_1    (nr__1) ! (mag) ? R1 magnitude of a candidate counterpart
*                               found in the USNO-B1.0 catalog (5)
      real*4        R2mag_1    (nr__1) ! (mag) ? R2 magnitude of a candidate counterpart
*                               found in the USNO-B1.0 catalog (5)
      real*4        Vmag_1     (nr__1) ! (mag) ? VT magnitude of a candidate counterpart
*                               found in the Tycho-2 catalog (5)
      real*8        Prob_1     (nr__1) ! (%) ? Probability of chance coincidence (5)(6)
      character*17  Com_1      (nr__1) ! Comment (counterpart or location)
*Note (1): Limits as follows:
*    rh = sources with r_M71_<=r_h_;
*   2rh = sources with r_h_<r_M71_<=2r_h_;
*    t2 = sources with 2r_h_<=r_M71_ (table 2)
*Note (2):
*     j = This source is on the S2 front-side CCD. All other sources in this
*         table are on the S3 back-side CCD.
*Note (3): The corresponding radii for inclusion with 95% or 99% confidence are
*          found by multiplying this column by 1.62 or 2.01, respectively.
*Note (4): In a few cases, the source is dithered across the gap between CCDs.
*Note (5): Found by searching the HEASARC 2MASS (see
*          http://www.ipac.caltech.edu/2mass/; Cat. II/246), USNO-B1.0
*          (Monet et al. 2003; Cat. I/284), and Tycho-2 (Hog et al. 2000,
*          Cat. I/259) catalogs, requiring that the candidate counterpart lie
*          within the 99% confidence radius of a Chandra source.
*          There are 6414 and 3376 2MASS sources, 15324 and 9196 USNO sources,
*          and 7 and 9 Tycho sources appearing within the S2-S3-S4 and I2-I3
*          boundaries shown in Figures 3 and 4, respectively.
*          If blank, no candidate counterpart was found in these catalogs. (See
*          section 6.1 for further details).
*Note (6): The percent probability of a chance coincidence is calculated from:
*          P_coinc_=N(<m){pi}r^2^_99_/A_search_ where N(<m) is the number of
*          sources in the corresponding catalog inside the search area,
*          A_search_, with a magnitude smaller than that of the candidate
*          counterpart, and r_99_ is the radius enclosing the X-ray source
*          location with 99% confidence.

C=============================================================================

C  Loading file 'table1.dat'	! Chandra X-ray sources detected with r_M71_<=2r_h_

C  Format for file interpretation

    1 format(
     +  A3,1X,A4,A1,1X,I2,1X,I2,1X,F6.3,1X,A1,I2,1X,I2,1X,F5.2,1X,
     +  F4.1,1X,F6.1,1X,F4.2,1X,A5,1X,F4.2,1X,F4.2,1X,F6.3,1X,F5.2,1X,
     +  F4.1,1X,F6.3,1X,F7.4,1X,A17)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table1.dat')
      write(6,*) '....Loading file: table1.dat'
      do i__=1,68
        read(1,'(A119)')ar__
        read(ar__,1)
     +  rl(i__),ID(i__),f_ID(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
     +  DEd(i__),DEm(i__),DEs(i__),re(i__),Cx(i__),SigX(i__),
     +  Chip(i__),rM71(i__),off(i__),Jmag(i__),R1mag(i__),R2mag(i__),
     +  Vmag(i__),Prob(i__),Com(i__)
        if(ar__(60:63) .EQ. '') rM71(i__) = rNULL__
        if(ar__(65:68) .EQ. '') off(i__) = rNULL__
        if(ar__(70:75) .EQ. '') Jmag(i__) = rNULL__
        if(ar__(77:81) .EQ. '') R1mag(i__) = rNULL__
        if(ar__(83:86) .EQ. '') R2mag(i__) = rNULL__
        if(ar__(88:93) .EQ. '') Vmag(i__) = rNULL__
        if(ar__(95:101) .EQ. '') Prob(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)
     +  rl(i__),ID(i__),f_ID(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
     +  DEd(i__),DEm(i__),DEs(i__),re(i__),Cx(i__),SigX(i__),
     +  Chip(i__),rM71(i__),off(i__),Jmag(i__),R1mag(i__),R2mag(i__),
     +  Vmag(i__),Prob(i__),Com(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'	! Chandra X-ray sources detected with 2r_h_>=r_M71_

C  Format for file interpretation

    2 format(
     +  A3,1X,A4,A1,1X,I2,1X,I2,1X,F6.3,1X,A1,I2,1X,I2,1X,F5.2,1X,
     +  F4.1,1X,F6.1,1X,F4.2,1X,A5,1X,F4.2,1X,F4.2,1X,F6.3,1X,F5.2,1X,
     +  F4.1,1X,F6.3,1X,F7.4,1X,A17)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table2.dat')
      write(6,*) '....Loading file: table2.dat'
      do i__=1,97
        read(1,'(A119)')ar__1
        read(ar__1,2)
     +  rl_1(i__),ID_1(i__),f_ID_1(i__),RAh_1(i__),RAm_1(i__),
     +  RAs_1(i__),DE__1(i__),DEd_1(i__),DEm_1(i__),DEs_1(i__),
     +  re_1(i__),Cx_1(i__),SigX_1(i__),Chip_1(i__),rM71_1(i__),
     +  off_1(i__),Jmag_1(i__),R1mag_1(i__),R2mag_1(i__),Vmag_1(i__),
     +  Prob_1(i__),Com_1(i__)
        if(ar__1(60:63) .EQ. '') rM71_1(i__) = rNULL__
        if(ar__1(65:68) .EQ. '') off_1(i__) = rNULL__
        if(ar__1(70:75) .EQ. '') Jmag_1(i__) = rNULL__
        if(ar__1(77:81) .EQ. '') R1mag_1(i__) = rNULL__
        if(ar__1(83:86) .EQ. '') R2mag_1(i__) = rNULL__
        if(ar__1(88:93) .EQ. '') Vmag_1(i__) = rNULL__
        if(ar__1(95:101) .EQ. '') Prob_1(i__) = rNULL__
        RAdeg_1(i__) = rNULL__
        DEdeg_1(i__) = rNULL__
c  Derive coordinates RAdeg_1 and DEdeg_1 from input data
c  (RAdeg_1 and DEdeg_1 are set to rNULL__ when unknown)
        if(RAh_1(i__) .GT. -180) RAdeg_1(i__)=RAh_1(i__)*15.
        if(RAm_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAm_1(i__)/4.
        if(RAs_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAs_1(i__)/240.
        if(DEd_1(i__) .GE. 0) DEdeg_1(i__)=DEd_1(i__)
        if(DEm_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEm_1(i__)/60.
        if(DEs_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEs_1(i__)/3600.
        if(DE__1(i__).EQ.'-'.AND.DEdeg_1(i__).GE.0) DEdeg_1(i__)=-DEdeg_1(i__)
c    ..............Just test output...........
        write(6,2)
     +  rl_1(i__),ID_1(i__),f_ID_1(i__),RAh_1(i__),RAm_1(i__),
     +  RAs_1(i__),DE__1(i__),DEd_1(i__),DEm_1(i__),DEs_1(i__),
     +  re_1(i__),Cx_1(i__),SigX_1(i__),Chip_1(i__),rM71_1(i__),
     +  off_1(i__),Jmag_1(i__),R1mag_1(i__),R2mag_1(i__),Vmag_1(i__),
     +  Prob_1(i__),Com_1(i__)
        write(6,'(6H Pos: 2F8.4)') RAdeg_1(i__),DEdeg_1(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

C=============================================================================
      stop
      end