FORTRAN Generation
(/./ftp/cats/J/MNRAS/358/149)

Conversion of standardized ReadMe file for file /./ftp/cats/J/MNRAS/358/149 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-Oct-14
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/MNRAS/358/149     HDFN SCUBA Super-map. III                (Pope+, 2005)
*================================================================================
*The Hubble Deep Field North SCUBA Super-map.
*III. Optical and near-infrared properties of submillimetre galaxies.
*    Pope A., Borys C., Scott D., Conselice C., Dickinson M., Mobasher B.
*   <Mon. Not. R. Astron. Soc., 358, 149-167 (2005)>
*   =2005MNRAS.358..149P
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'tablea1.dat'	! *Updated list of 850um sources in GOODS-N region
                             (Great Observatories Origins Deep Survey North)

      integer*4 nr__
      parameter (nr__=40)	! Number of records
      character*73 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)

      character*6   v_PBS2005_ (nr__) ! GOODS-N (prefix GN) ID number
      character*14  SMM        (nr__) ! SMM designation (JHHMMSS+DDMMSS) (G1)
      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)
      integer*4     DEs        (nr__) ! (arcsec) Declination (J2000.0)
      real*4        S850um     (nr__) ! (mJy) Flux density at 850um
      real*4        e_S850um   (nr__) ! (mJy) rms uncertainty on S850um
      real*4        S_N        (nr__) ! Signal-to-noise ratio
      character*10  Com        (nr__) ! Comments (1)
      character*1   n_Com      (nr__) ! Note on Com (2)
      character*1   OID        (nr__) ! Optical ID code (3)
*Note (1): Sources that are new since Paper II (Borys et al.,
*          2004MNRAS.355..485B) are listed as New
*Note (2): Note as follows:
*      a = See Dunlop et al. (2004MNRAS.350..769D) for detailed counterpart
*          analysis of this source. Our cleaning procedure finds a
*          companion source approximately 25 arcsec to the south-west.
*          However a simultaneous fit places it at an signal-to-noise ratio
*          of slightly less than 3.5.
*      b = There are several minor changes compared with the table 4 of
*          Paper II, which we discuss in the text. Note that GN38 is just
*          outside the GOODS-N region.
*Note (3): Status of the optical counterpart for each submillimetre (submm)
*          source as follows:
*      S = secure
*      T = tentative
*      M = multiple possible counterparts that meet our counterpart
*          selection criteria
*      N = no counterpart

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

C  Declarations for 'tablea2.dat'	! *450-um source list.

      integer*4 nr__1
      parameter (nr__1=7)	! Number of records
      character*95 ar__1  	! Full-size record

C  J2000.0 position composed of: RAh RAm RAs DE- DEd DEm DEs
      real*8        RAdeg_1    (nr__1) ! (deg) Right Ascension J2000.0
      real*8        DEdeg_1    (nr__1) ! (deg)     Declination J2000.0
C  ---------------------------------- ! (position vector(s) in degrees)

      character*14  SMM_1      (nr__1) ! SMM designation (JHHMMSS+DDMMSS) (G1)
      integer*4     RAh_1      (nr__1) ! (h) Right ascension (J2000.0)
      integer*4     RAm_1      (nr__1) ! (min) Right ascension (J2000.0)
      real*4        RAs_1      (nr__1) ! (s) Right ascension (J2000.0)
      character*1   DE__1      (nr__1) ! Declination sign (J2000.0)
      integer*4     DEd_1      (nr__1) ! (deg) Declination (J2000.0)
      integer*4     DEm_1      (nr__1) ! (arcmin) Declination (J2000.0)
      integer*4     DEs_1      (nr__1) ! (arcsec) Declination (J2000.0)
      integer*4     S450um     (nr__1) ! (mJy) Flux density at 450um
      integer*4     e_S450um   (nr__1) ! (mJy) rms uncertainty on S450um
      character*1   l_S850um   (nr__1) ! Limit flag on S850um
      real*4        S850um_1   (nr__1) ! (mJy) 3{sigma} upper limits of Flux density at 850um
      character*43  Com_1      (nr__1) ! Comment

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

C  Loading file 'tablea1.dat'	! *Updated list of 850um sources in GOODS-N region
*                             (Great Observatories Origins Deep Survey North)

C  Format for file interpretation

    1 format(
     +  A6,4X,A14,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,1X,F4.1,1X,
     +  F3.1,1X,F4.1,1X,A10,A1,1X,A1)

C  Effective file loading

      open(unit=1,status='old',file=
     +'tablea1.dat')
      write(6,*) '....Loading file: tablea1.dat'
      do i__=1,40
        read(1,'(A73)')ar__
        read(ar__,1)
     +  v_PBS2005_(i__),SMM(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
     +  DEd(i__),DEm(i__),DEs(i__),S850um(i__),e_S850um(i__),S_N(i__),
     +  Com(i__),n_Com(i__),OID(i__)
        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_PBS2005_(i__),SMM(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
     +  DEd(i__),DEm(i__),DEs(i__),S850um(i__),e_S850um(i__),S_N(i__),
     +  Com(i__),n_Com(i__),OID(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 'tablea2.dat'	! *450-um source list.

C  Format for file interpretation

    2 format(
     +  3X,A14,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,1X,I3,1X,I2,
     +  1X,A1,F4.1,1X,A43)

C  Effective file loading

      open(unit=1,status='old',file=
     +'tablea2.dat')
      write(6,*) '....Loading file: tablea2.dat'
      do i__=1,7
        read(1,'(A95)')ar__1
        read(ar__1,2)
     +  SMM_1(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
     +  DEd_1(i__),DEm_1(i__),DEs_1(i__),S450um(i__),e_S450um(i__),
     +  l_S850um(i__),S850um_1(i__),Com_1(i__)
        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)
     +  SMM_1(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
     +  DEd_1(i__),DEm_1(i__),DEs_1(i__),S450um(i__),e_S450um(i__),
     +  l_S850um(i__),S850um_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