FORTRAN Generation
(/./home/cats/J/ApJ/788/55)

Conversion of standardized ReadMe file for file /./home/cats/J/ApJ/788/55 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-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/788/55      HST/WFC3 SNR discoveries in M83 (NGC5236)      (Blair+, 2014)
*================================================================================
*An expanded HST/WFC3 survey of M83:
*project overview and targeted supernova remnant search.
*    Blair W.P., Chandar R., Dopita M.A., Ghavamian P., Hammer D., Kuntz K.D.,
*    Long K.S., Soria R., Whitmore B.C., Frank Winkler P.
*   <Astrophys. J., 788, 55 (2014)>
*   =2014ApJ...788...55B
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'table3.dat'	! Small diameter and new supernova remnants in M83
                               revealed by HST/WFC3

      integer*4 nr__
      parameter (nr__=63)	! Number of records
      character*123 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)

      integer*4     Seq        (nr__) ! [1/63] Running sequence number
*                                    (<[BCD2014] NN> in Simbad)
      character*7   AName      (nr__) ! Previous name (G1)
      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__) ! Sign of declination (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        Rad        (nr__) ! (arcsec) [0.07/0.8] Source radius
      real*4        Diam       (nr__) ! (pc) [3.1/34.3] Source diameter (1)
      real*4        GCD        (nr__) ! (kpc) [0.1/5.3] Galactocentric distance (1)
      integer*4     Field      (nr__) ! [1/7] WFC3 field number
      character*1   l_F657N    (nr__) ! Limit flag on F657N
      real*4        F657N      (nr__) ! (mW/m2) The F657N flux in erg/cm^2^/s (G2)
      character*1   l_F673_657 (nr__) ! Limit flag on F673/657
      real*4        F673_657   (nr__) ! [0.06/6.6]? Lower limit to the observed
*                                  F673N/F657N (F([SII])/F(H{alpha})) ratio (G3)
      character*52  Comm       (nr__) ! Comments
*Note (1): The galactocentric distances (GCDs) of each object are based on the
*          same assumptions for galactic inclination and major axis angle as
*          used in Blair et al. (2012, Cat. J/ApJS/203/8) and the assumed
*          distance of 4.61Mpc.

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

C  Declarations for 'table4.dat'	! M83 supernova remnant WFC3 image ratios and
                               supporting information

      integer*4 nr__1
      parameter (nr__1=63)	! Number of records
      character*171 ar__1  	! Full-size record

      integer*4     Seq_1      (nr__1) ! [1/63] Running sequence number
*                                    (<[BCD2014] NN> in Simbad)
      character*7   AName_1    (nr__1) ! Previous name (G1)
      character*1   l_F657N_1  (nr__1) ! Limit flag on F657N
      real*4        F657N_1    (nr__1) ! (mW/m2) The F657N flux in erg/cm^2^/s (G2)
      real*4        F164N      (nr__1) ! (mW/m2) ? The F164N flux (objects showing only [FeII]
*                                    emission) (G2)
      character*1   l_F673_657_1(nr__1) ! Limit flag on F673/657
      real*4        F673_657_1 (nr__1) ! [0.06/6.6]? Lower limit to the observed
*                                  F673N/F657N (F([SII])/F(H{alpha})) ratio (G3)
      character*1   l_F164_657 (nr__1) ! Limit flag on F164/657
      real*4        F164_657   (nr__1) ! [0.01/10]? Lower limit to the observed
*                                   F([FeII])/F(H{alpha}) ratio (G3)
      character*1   l_F164_673 (nr__1) ! Limit flag on F614/673
      real*4        F164_673   (nr__1) ! [0.01/4.86]? Lower limit to the observed
*                                   F([FeII]])/F([SII]) ratio
      character*1   l_F502_657 (nr__1) ! Limit flag on F502/657
      real*4        F502_657   (nr__1) ! ? Lower limit to the observed
*                                   F([OIII])/F(H{alpha}) ratio (G3)
      character*1   u_F502_657 (nr__1) ! Uncertainty flag on F502/657
      character*4   XID        (nr__1) ! X-Ray ID in Chandra (2)
      character*1   u_XID      (nr__1) ! Uncertainty flag on XID
*                                  (less reliable alignments)
      character*104 Comm_1     (nr__1) ! Comments
*Note (2): X-ray ID from Chandra catalog of Long et al. 2014 (J/ApJS/212/21);
*     <[LKB2014] XNNN> in Simbad.

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

C  Loading file 'table3.dat'	! Small diameter and new supernova remnants in M83
*                               revealed by HST/WFC3

C  Format for file interpretation

    1 format(
     +  I2,1X,A7,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F5.2,1X,F4.2,
     +  1X,F4.1,1X,F4.2,1X,I1,1X,A1,1X,E8.3,1X,A1,1X,F4.2,1X,A52)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table3.dat')
      write(6,*) '....Loading file: table3.dat'
      do i__=1,63
        read(1,'(A123)')ar__
        read(ar__,1)
     +  Seq(i__),AName(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
     +  DEd(i__),DEm(i__),DEs(i__),Rad(i__),Diam(i__),GCD(i__),
     +  Field(i__),l_F657N(i__),F657N(i__),l_F673_657(i__),
     +  F673_657(i__),Comm(i__)
        if(ar__(67:70) .EQ. '') F673_657(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)
     +  Seq(i__),AName(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
     +  DEd(i__),DEm(i__),DEs(i__),Rad(i__),Diam(i__),GCD(i__),
     +  Field(i__),l_F657N(i__),F657N(i__),l_F673_657(i__),
     +  F673_657(i__),Comm(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 'table4.dat'	! M83 supernova remnant WFC3 image ratios and
*                               supporting information

C  Format for file interpretation

    2 format(
     +  I2,1X,A7,1X,A1,1X,E8.3,1X,E7.2,1X,A1,1X,F4.2,1X,A1,1X,F5.2,1X,
     +  A1,1X,F4.2,1X,A1,1X,F5.2,A1,1X,A4,A1,1X,A104)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table4.dat')
      write(6,*) '....Loading file: table4.dat'
      do i__=1,63
        read(1,'(A171)')ar__1
        read(ar__1,2)
     +  Seq_1(i__),AName_1(i__),l_F657N_1(i__),F657N_1(i__),
     +  F164N(i__),l_F673_657_1(i__),F673_657_1(i__),l_F164_657(i__),
     +  F164_657(i__),l_F164_673(i__),F164_673(i__),l_F502_657(i__),
     +  F502_657(i__),u_F502_657(i__),XID(i__),u_XID(i__),Comm_1(i__)
        if(ar__1(23:29) .EQ. '') F164N(i__) = rNULL__
        if(ar__1(33:36) .EQ. '') F673_657_1(i__) = rNULL__
        if(ar__1(40:44) .EQ. '') F164_657(i__) = rNULL__
        if(ar__1(48:51) .EQ. '') F164_673(i__) = rNULL__
        if(ar__1(55:59) .EQ. '') F502_657(i__) = rNULL__
c    ..............Just test output...........
        write(6,2)
     +  Seq_1(i__),AName_1(i__),l_F657N_1(i__),F657N_1(i__),
     +  F164N(i__),l_F673_657_1(i__),F673_657_1(i__),l_F164_657(i__),
     +  F164_657(i__),l_F164_673(i__),F164_673(i__),l_F502_657(i__),
     +  F502_657(i__),u_F502_657(i__),XID(i__),u_XID(i__),Comm_1(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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