FORTRAN Generation
(/./ftp/cats/J/ApJ/768/172)

Conversion of standardized ReadMe file for file /./ftp/cats/J/ApJ/768/172 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 2026-Aug-16
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/768/172   Kinematic analysis of red giant in M31 dSphs   (Collins+, 2013)
*================================================================================
*A kinematic study of the Andromeda dwarf spheroidal system.
*    Collins M.L.M., Chapman S.C., Rich R.M., Ibata R.A., Martin N.F.,
*    Irwin M.J., Bate N.F., Lewis G.F., Penarrubia J., Arimoto N., Casey C.M.,
*    Ferguson A.M.N., Koch A., McConnachie A.W., Tanvir N.
*   <Astrophys. J., 768, 172 (2013)>
*   =2013ApJ...768..172C
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'table1.dat'	! *Details of the structural properties for each dwarf

      integer*4 nr__
      parameter (nr__=18)	! Number of records
      character*66 ar__   	! Full-size record

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

      character*10  Gal         ! Dwarf galaxy name
      character*1   n_Gal       ! [c] And XXX = Cas II
      integer*4     RAh         ! (h) Hour of right ascension (J2000)
      integer*4     RAm         ! (min) Minute of right ascension (J2000)
      real*4        RAs         ! (s) Second of right ascension (J2000)
      character*1   DE_         ! Sign of declination (J2000)
      integer*4     DEd         ! (deg) Degree of declination (J2000)
      integer*4     DEm         ! (arcmin) Arcminute of declination (J2000)
      real*4        DEs         ! (arcsec) Arcsecond of declination (J2000)
      real*4        VMag        ! (mag) [-10.6/-6.3] Absolute V-band magnitude
      integer*4     rh          ! (pc) [114/1481] Half-light radius
      integer*4     E_rh        ! (pc) [9/112] Positive uncertainty on rh
      integer*4     e_rh_1      ! (pc) [12/271] Negative uncertainty on rh
      integer*4     Dist        ! (kpc) [650/1255] Distance
      integer*4     E_Dist      ! (kpc) [21/218] Positive uncertainty on Dist
      integer*4     e_Dist_1    ! (kpc) [21/474] Negative uncertainty on Dist

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

C  Declarations for 'table2.dat'	! Details of spectroscopic observations

      integer*4 nr__1
      parameter (nr__1=22)	! Number of records
      character*89 ar__1  	! Full-size record

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

      character*10  Gal_1       ! Field (dwarf spheroidal) name
      character*1   m_Gal       ! [ab] Index in case of multiple observations
      character*11  Date        ! ("Y-M-D") Observation date
      character*3   n_Date      ! Observation on several days
      character*13  Inst        ! Instrument and grating
      real*4        Res         ! (0.1nm) [1.3/3.5] Resolution in {AA}
      integer*4     RAh_1       ! (h) Hour of Right Ascension (J2000)
      integer*4     RAm_1       ! (min) Minute of Right Ascension (J2000)
      real*4        RAs_1       ! (s) Second of Right Ascension (J2000)
      character*1   DE__1       ! [+] Sign of Declination (J2000)
      integer*4     DEd_1       ! (deg) Degree of Declination (J2000)
      integer*4     DEm_1       ! (arcmin) Arcminute of Declination (J2000)
      real*4        DEs_1       ! (arcsec) Arcsecond of Declination (J2000)
      integer*4     PA          ! (deg) [0/315] Slit position angle
      integer*4     Exp         ! (s) [1200/5400] Exposure time
      integer*4     Ntar        ! [33/196] Number of targets observed
      integer*4     Nmem        ! [1/43] Number of member stars observed

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

C  Declarations for 'table3.dat'	! Details of probable dSph members

      integer*4 nr__2
      parameter (nr__2=295)	! Number of records
      character*86 ar__2  	! Full-size record

C  J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
      real*8        RAdeg_2     ! (deg) Right Ascension J2000
      real*8        DEdeg_2     ! (deg)     Declination J2000
C  ---------------------------------- ! (position vector(s) in degrees)

      character*10  Gal_2       ! Field (dwarf spheroidal) name
      character*1   m_Gal_1     ! [ab] Index in case of multiple observations
      integer*4     ID          ! [1/172] Star identifier in Gal
      integer*4     RAh_2       ! (h) Hour of Right Ascension (J2000)
      integer*4     RAm_2       ! (min) Minute of Right Ascension (J2000)
      real*4        RAs_2       ! (s) Second of Right Ascension (J2000)
      character*1   DE__2       ! [+] Sign of Declination (J2000)
      integer*4     DEd_2       ! (deg) Degree of Declination (J2000)
      integer*4     DEm_2       ! (arcmin) Arcminute of Declination (J2000)
      real*4        DEs_2       ! (arcsec) Arcsecond of Declination (J2000)
      real*4        gmag        ! (mag) [21.4/25] The CFHT/MegaCam g-band magnitude
      real*4        imag        ! (mag) [20.3/24] The CFHT/MegaCam i-band magnitude
      real*8        HRV         ! (km/s) [-604.5/918.2] Heliocentric radial velocity
      real*8        e_HRV       ! (km/s) [1.2/227] Error in HRV
      real*4        S_N         ! [0.3/17] Signal-to-noise (per Angstrom)
      real*4        Pi          ! [0/1] Likelihood of membership (1)
*Note (1): Likelihood of membership as (equation 1):
*          P_i_{prop.to}P_CMD_*P_dist_*P_vel_ 
*    where P_CMD_ is the probability based on CMD position, 
*    P_dist_ is the probability based on distance, and 
*    P_vel_ is the probability based on velocity).
*    See section 3 for further details.

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

C  Declarations for 'table4.dat'	! Kinematic properties of Andromeda dSph galaxies as
                              derived from Keck I/LRIS, and Keck II/DEIMOS data

      integer*4 nr__3
      parameter (nr__3=18)	! Number of records
      character*90 ar__3  	! Full-size record

      character*10  Gal_3       ! Dwarf galaxy name
      character*1   n_Gal_1     ! [c] And XXX = Cas II
      real*4        eta         ! [1.5/5] Free parameter {eta} (1)
      real*4        RV          ! (km/s) [-558/-107] Radial velocity
      real*4        E_RV        ! (km/s) [0.9/6] Positive error on RV
      real*4        e_RV_1      ! (km/s) [0.9/7] Negative error on RV
      real*4        sigV        ! (km/s) [0/15] Velocity dispersion {sigma}_V_
      real*4        E_sigV      ! (km/s) Positive error on sigV
      character*1   f_sigV      ! [*] non-reliable sigV (2)
      real*4        e_sigV_1    ! (km/s) [1/8.1] Negative error on sigV
      real*4        Mh          ! (10+7Msun) [0/8.3] Mass contained within the half-light
*                                    radius
      real*4        E_Mh        ! (10+7Msun) [0.08/5] Positive error on Mh
      real*4        e_Mh_1      ! (10+7Msun) [0.06/5] Negative error on Mh
      real*4        v_M_L_      ! (Msun/Lsun) [0/1391] Dynamical central mass-to-light ratio
      real*4        E__M_L_     ! (Msun/Lsun) [4.2/1039] Positive error on [M/L]
      real*4        e__M_L__1   ! (Msun/Lsun) [3.9/1128] Negative error on [M/L]
      real*4        v_Fe_H_     ! ([Sun]) [-2.2/-1.4] Spectroscopic [Fe/H]
      real*4        e__Fe_H_    ! ([Sun]) [0.1/0.6] [Fe/H] uncertainty
*Note (1): In Section 3.3, we tested that our velocity probability criteria was
*          not overly biasing our final measurements of velocity dispersion to
*          artificially lower values with the introduction of an extra parameter,
*          {eta}, that allows us to add additional weight to stars in the tails
*          of the Gaussian velocity distribution.
*Note (2):
*  * = Velocity dispersions derived from fewer than eight members stars, and
*      require confirmation from further follow-up.

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

C  Loading file 'table1.dat'	! *Details of the structural properties for each dwarf

C  Format for file interpretation

    1 format(
     +  A10,A1,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,F4.1,1X,F5.1,1X,
     +  I4,1X,I3,1X,I3,1X,I4,1X,I3,1X,I3)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table1.dat')
      write(6,*) '....Loading file: table1.dat'
      do i__=1,18
        read(1,'(A66)')ar__
        read(ar__,1)
     +  Gal,n_Gal,RAh,RAm,RAs,DE_,DEd,DEm,DEs,VMag,rh,E_rh,e_rh_1,
     +  Dist,E_Dist,e_Dist_1
        RAdeg = rNULL__
        DEdeg = rNULL__
c  Derive coordinates RAdeg and DEdeg from input data
c  (RAdeg and DEdeg are set to rNULL__ when unknown)
        if(RAh .GT. -180) RAdeg=RAh*15.
        if(RAm .GT. -180) RAdeg=RAdeg+RAm/4.
        if(RAs .GT. -180) RAdeg=RAdeg+RAs/240.
        if(DEd .GE. 0) DEdeg=DEd
        if(DEm .GE. 0) DEdeg=DEdeg+DEm/60.
        if(DEs .GE. 0) DEdeg=DEdeg+DEs/3600.
        if(DE_.EQ.'-'.AND.DEdeg.GE.0) DEdeg=-DEdeg
c    ..............Just test output...........
        write(6,1)
     +  Gal,n_Gal,RAh,RAm,RAs,DE_,DEd,DEm,DEs,VMag,rh,E_rh,e_rh_1,
     +  Dist,E_Dist,e_Dist_1
        write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c    .......End.of.Just test output...........
      end do
      close(1)

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

C  Loading file 'table2.dat'	! Details of spectroscopic observations

C  Format for file interpretation

    2 format(
     +  A10,A1,2X,A11,A3,2X,A13,3X,F3.1,2X,I2,1X,I2,1X,F5.2,1X,A1,I2,
     +  1X,I2,1X,F4.1,1X,I3,1X,I4,1X,I3,1X,I2)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table2.dat')
      write(6,*) '....Loading file: table2.dat'
      do i__=1,22
        read(1,'(A89)')ar__1
        read(ar__1,2)
     +  Gal_1,m_Gal,Date,n_Date,Inst,Res,RAh_1,RAm_1,RAs_1,DE__1,
     +  DEd_1,DEm_1,DEs_1,PA,Exp,Ntar,Nmem
        RAdeg_1 = rNULL__
        DEdeg_1 = 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 .GT. -180) RAdeg_1=RAh_1*15.
        if(RAm_1 .GT. -180) RAdeg_1=RAdeg_1+RAm_1/4.
        if(RAs_1 .GT. -180) RAdeg_1=RAdeg_1+RAs_1/240.
        if(DEd_1 .GE. 0) DEdeg_1=DEd_1
        if(DEm_1 .GE. 0) DEdeg_1=DEdeg_1+DEm_1/60.
        if(DEs_1 .GE. 0) DEdeg_1=DEdeg_1+DEs_1/3600.
        if(DE__1.EQ.'-'.AND.DEdeg_1.GE.0) DEdeg_1=-DEdeg_1
c    ..............Just test output...........
        write(6,2)
     +  Gal_1,m_Gal,Date,n_Date,Inst,Res,RAh_1,RAm_1,RAs_1,DE__1,
     +  DEd_1,DEm_1,DEs_1,PA,Exp,Ntar,Nmem
        write(6,'(6H Pos: 2F8.4)') RAdeg_1,DEdeg_1
c    .......End.of.Just test output...........
      end do
      close(1)

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

C  Loading file 'table3.dat'	! Details of probable dSph members

C  Format for file interpretation

    3 format(
     +  A10,A1,1X,I3,1X,I2,1X,I2,1X,F6.3,1X,A1,I2,1X,I2,1X,F6.3,1X,
     +  F6.3,1X,F6.3,1X,F8.3,1X,F7.3,1X,F6.3,1X,F5.3)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table3.dat')
      write(6,*) '....Loading file: table3.dat'
      do i__=1,295
        read(1,'(A86)')ar__2
        read(ar__2,3)
     +  Gal_2,m_Gal_1,ID,RAh_2,RAm_2,RAs_2,DE__2,DEd_2,DEm_2,DEs_2,
     +  gmag,imag,HRV,e_HRV,S_N,Pi
        RAdeg_2 = rNULL__
        DEdeg_2 = rNULL__
c  Derive coordinates RAdeg_2 and DEdeg_2 from input data
c  (RAdeg_2 and DEdeg_2 are set to rNULL__ when unknown)
        if(RAh_2 .GT. -180) RAdeg_2=RAh_2*15.
        if(RAm_2 .GT. -180) RAdeg_2=RAdeg_2+RAm_2/4.
        if(RAs_2 .GT. -180) RAdeg_2=RAdeg_2+RAs_2/240.
        if(DEd_2 .GE. 0) DEdeg_2=DEd_2
        if(DEm_2 .GE. 0) DEdeg_2=DEdeg_2+DEm_2/60.
        if(DEs_2 .GE. 0) DEdeg_2=DEdeg_2+DEs_2/3600.
        if(DE__2.EQ.'-'.AND.DEdeg_2.GE.0) DEdeg_2=-DEdeg_2
c    ..............Just test output...........
        write(6,3)
     +  Gal_2,m_Gal_1,ID,RAh_2,RAm_2,RAs_2,DE__2,DEd_2,DEm_2,DEs_2,
     +  gmag,imag,HRV,e_HRV,S_N,Pi
        write(6,'(6H Pos: 2F8.4)') RAdeg_2,DEdeg_2
c    .......End.of.Just test output...........
      end do
      close(1)

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

C  Loading file 'table4.dat'	! Kinematic properties of Andromeda dSph galaxies as
*                              derived from Keck I/LRIS, and Keck II/DEIMOS data

C  Format for file interpretation

    4 format(
     +  A10,A1,1X,F3.1,1X,F6.1,1X,F3.1,1X,F3.1,1X,F4.1,1X,F3.1,A1,1X,
     +  F3.1,1X,F4.2,1X,F4.2,1X,F4.2,1X,F6.1,1X,F6.1,1X,F6.1,1X,F4.1,
     +  1X,F4.2)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table4.dat')
      write(6,*) '....Loading file: table4.dat'
      do i__=1,18
        read(1,'(A90)')ar__3
        read(ar__3,4)
     +  Gal_3,n_Gal_1,eta,RV,E_RV,e_RV_1,sigV,E_sigV,f_sigV,e_sigV_1,
     +  Mh,E_Mh,e_Mh_1,v_M_L_,E__M_L_,e__M_L__1,v_Fe_H_,e__Fe_H_
c    ..............Just test output...........
        write(6,4)
     +  Gal_3,n_Gal_1,eta,RV,E_RV,e_RV_1,sigV,E_sigV,f_sigV,e_sigV_1,
     +  Mh,E_Mh,e_Mh_1,v_M_L_,E__M_L_,e__M_L__1,v_Fe_H_,e__Fe_H_
c    .......End.of.Just test output...........
      end do
      close(1)

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