FORTRAN Generation
(/./ftp/cats/J/A_A/421/623)

Conversion of standardized ReadMe file for file /./ftp/cats/J/A_A/421/623 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-Apr-20
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/A+A/421/623       ISOCAM survey of YSOs in Serpens Cloud Core    (Kaas+, 2004)
*================================================================================
*The young stellar population in the Serpens Cloud Core: An ISOCAM survey.
*     Kaas A.A., Olofsson G., Bontemps S., Andre P., Nordh L., Huldtgren M.,
*     Prusti T., Persi P., Delgado A.J., Motte F., Abergel A., Boulanger F.,
*     Burgdorf M., Casali M.M., Cesarsky C.J., Davies J., Falgarone E.,
*     Montmerle T., Perault M., Puget J.L., Sibille F.
*    <Astron. Astrophys. 421, 623 (2004)>
*    =2004A&A...421..623K
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'table2.dat'	! The 77 ISOCAM sources identified as YSOs in the
                             Serpens cluster

      integer*4 nr__
      parameter (nr__=77)	! Number of records
      character*117 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     ISO        (nr__) ! ISO number
      character*1   m_ISO      (nr__) ! [ab] Note (1)
      integer*4     RAh        (nr__) ! (h) Right ascension (J2000)
      integer*4     RAm        (nr__) ! (min) Right ascension (J2000)
      real*4        RAs        (nr__) ! (s) Right ascension (J2000)
      character*1   DE_        (nr__) ! Declination sign (J2000)
      integer*4     DEd        (nr__) ! (deg) Declination (J2000)
      integer*4     DEm        (nr__) ! (arcmin) Declination (J2000)
      integer*4     DEs        (nr__) ! (arcsec) Declination (J2000)
      real*4        Jmag       (nr__) ! (mag) ? J magnitude (3)
      character*1   n_Jmag     (nr__) ! [b] Note on Jmag (1)
      character*1   l_e_Jmag   (nr__) ! Limit flag on e_Jmag
      real*4        e_Jmag     (nr__) ! (mag) ? rms uncertainty on Jmag
      real*4        Hmag       (nr__) ! (mag) ? H magnitude (3)
      character*1   n_Hmag     (nr__) ! [ab] Note on Hmag (1)
      character*1   l_e_Hmag   (nr__) ! Limit flag on e_Hmag
      real*4        e_Hmag     (nr__) ! (mag) ? rms uncertainty on Hmag
      real*4        Kmag       (nr__) ! (mag) ? K magnitude (3)
      character*1   n_Kmag     (nr__) ! [ab] Note on Kmag (1)
      character*1   l_e_Kmag   (nr__) ! Limit flag on e_Kmag
      real*4        e_Kmag     (nr__) ! (mag) ? rms uncertainty on Kmag
      real*4        F6_7um     (nr__) ! (mJy) ? Flux density at 6.7um  (3)
      character*3   n_F6_7um   (nr__) ! Note on F6.7um (2)
      real*4        e_F6_7um   (nr__) ! (mJy) ? rms uncertainty on F6.7um
      real*4        F14_3um    (nr__) ! (mJy) ? Flux density at 14.3um  (3)
      character*3   n_F14_3um  (nr__) ! Note on F14.3um (2)
      real*4        e_F14_3um  (nr__) ! (mJy) ? rms uncertainty on F14.3um
      character*20  ID         (nr__) ! Other ID (4)
*Note (1): Notes on magnitudes:
*    a: H and K band data from the Arnica 1995 map, which is slightly
*        displaced from the 1996 map and therefore includes this object.
*    b: ISOCAM source is resolved into two sources in the near-IR, and the
*        near-IR fluxes are added.
*Note (2): Notes on fluxes:
*    c: Flux measurement affected by proximity to the dead column. If the
*        dead column cannot be avoided by any of the redundant
*        observations, this flagging. If source is located on the dead
*        column, a flux measurement is not attempted at all.
*    d: Source close to the detector edge in all redundant observations.
*    e: Extended source.
*    f: ISOCAM source is not quite resolved from a bright neighbour.
*    g: Galaxy contamination? For fluxes ~3mJy at 14.3{mu}m the "red"
*        sample is expected to contain less than two galaxies in our
*        field according to hon03.
*    m: Flux might be affected by memory effects from other sources.
*    n: Nebulous sky background.
*Note (3): Empty space means no measurement available in this work, while a
*    hyphen means no detection.
*Note (4): Identifier acronyms are related to the following references:
*    CDF: Chavarria-K et al., 1988A&A...197..151C, [CDF88] NN in Simbad
*     CK: Churchwell & Koornneef, 1986ApJ...300..729C in Simbad
*     EC: Eiroa & Casali, 1992A&A...262..468E, [EC92] NNN in Simbad
*   GCNM: Giovannetti et al., 1998A&A...330..990G
*    GEL: Gomez de Castro et al., 1988A&A...201..299G
*    GGD: Gyulbudaghian et al., 1978ApJ...224L.137G978
*     HB: Hurt & Barsony, 1996ApJ...460L..45H, [HB96] PS N in Simbad
*    HCE: Horrobin et al., 1997A&A...320L..41H, [EC92] NNN in Simbad
*    HHR: Hodapp et al., 1996ApJ...468..861H
*     HL: Hartigan & Lada, 1985ApJS...59..383H
*      K: Kaas 1999AJ....118..558K, [K99d] YSO NN in Simbad
*    MMW: McMullin et al., 1994ApJ...424..222M
*   StRS: Stephenson 1992AJ....103..263S
*    SCB: Straizys et al., 1996BaltA...5..125S, [SCB96] NNN in Simbad
*    SMM: Casali et al., 1993A&A...275..195C, [CED93] N in Simbad
*   STGM: Sogawa et al., 1997AJ....113.1057S
*         STGM3  = STGM 182709.0+010535 in Simbad
*         STGM2  = STGM 182711.4+010517 in Simbad
*         STGM14 = STGM 182721.2+011101 in Simbad
*         STGM8  = STGM 182735.3+010959 in Simbad
*    SVS: Strom et al., 1976AJ.....81..638S, [SVS76] Ser NN in Simbad

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

C  Declarations for 'table3.dat'	! *The 71 "blue" ISOCAM sources which have
                             [14.3/6.7]<-0.2.

      integer*4 nr__1
      parameter (nr__1=71)	! Number of records
      character*117 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)

      integer*4     ISO_1      (nr__1) ! ISO number
      character*1   m_ISO_1    (nr__1) ! [ab] Note (1)
      integer*4     RAh_1      (nr__1) ! (h) Right ascension (J2000)
      integer*4     RAm_1      (nr__1) ! (min) Right ascension (J2000)
      real*4        RAs_1      (nr__1) ! (s) Right ascension (J2000)
      character*1   DE__1      (nr__1) ! Declination sign (J2000)
      integer*4     DEd_1      (nr__1) ! (deg) Declination (J2000)
      integer*4     DEm_1      (nr__1) ! (arcmin) Declination (J2000)
      integer*4     DEs_1      (nr__1) ! (arcsec) Declination (J2000)
      real*4        Jmag_1     (nr__1) ! (mag) ? J magnitude (3)
      character*1   n_Jmag_1   (nr__1) ! [b] Note on Jmag (1)
      character*1   l_e_Jmag_1 (nr__1) ! Limit flag on e_Jmag
      real*4        e_Jmag_1   (nr__1) ! (mag) ? rms uncertainty on Jmag
      real*4        Hmag_1     (nr__1) ! (mag) ? H magnitude (3)
      character*1   n_Hmag_1   (nr__1) ! [ab] Note on Hmag (1)
      character*1   l_e_Hmag_1 (nr__1) ! Limit flag on e_Hmag
      real*4        e_Hmag_1   (nr__1) ! (mag) ? rms uncertainty on Hmag
      real*4        Kmag_1     (nr__1) ! (mag) ? K magnitude (3)
      character*1   n_Kmag_1   (nr__1) ! [ab] Note on Kmag (1)
      character*1   l_e_Kmag_1 (nr__1) ! Limit flag on e_Kmag
      real*4        e_Kmag_1   (nr__1) ! (mag) ? rms uncertainty on Kmag
      real*4        F6_7um_1   (nr__1) ! (mJy) ? Flux density at 6.7um  (3)
      character*3   n_F6_7um_1 (nr__1) ! Note on F6.7um (2)
      real*4        e_F6_7um_1 (nr__1) ! (mJy) ? rms uncertainty on F6.7um
      real*4        F14_3um_1  (nr__1) ! (mJy) ? Flux density at 14.3um  (3)
      character*3   n_F14_3um_1(nr__1) ! Note on F14.3um (2)
      real*4        e_F14_3um_1(nr__1) ! (mJy) ? rms uncertainty on F14.3um
      character*20  ID_1       (nr__1) ! Other ID (4)
*Note (1): Notes on magnitudes:
*    a: H and K band data from the Arnica 1995 map, which is slightly
*        displaced from the 1996 map and therefore includes this object.
*    b: ISOCAM source is resolved into two sources in the near-IR, and the
*        near-IR fluxes are added.
*Note (2): Notes on fluxes:
*    c: Flux measurement affected by proximity to the dead column. If the
*        dead column cannot be avoided by any of the redundant
*        observations, this flagging. If source is located on the dead
*        column, a flux measurement is not attempted at all.
*    d: Source close to the detector edge in all redundant observations.
*    e: Extended source.
*    f: ISOCAM source is not quite resolved from a bright neighbour.
*    g: Galaxy contamination? For fluxes ~3mJy at 14.3{mu}m the "red"
*        sample is expected to contain less than two galaxies in our
*        field according to hon03.
*    m: Flux might be affected by memory effects from other sources.
*    n: Nebulous sky background.
*Note (3): Empty space means no measurement available in this work, while a
*    hyphen means no detection.
*Note (4): Identifier acronyms are related to the following references:
*    CDF: Chavarria-K et al., 1988A&A...197..151C, [CDF88] NN in Simbad
*     CK: Churchwell & Koornneef, 1986ApJ...300..729C in Simbad
*     EC: Eiroa & Casali, 1992A&A...262..468E, [EC92] NNN in Simbad
*   GCNM: Giovannetti et al., 1998A&A...330..990G
*    GEL: Gomez de Castro et al., 1988A&A...201..299G
*    GGD: Gyulbudaghian et al., 1978ApJ...224L.137G978
*     HB: Hurt & Barsony, 1996ApJ...460L..45H, [HB96] PS N in Simbad
*    HCE: Horrobin et al., 1997A&A...320L..41H, [EC92] NNN in Simbad
*    HHR: Hodapp et al., 1996ApJ...468..861H
*     HL: Hartigan & Lada, 1985ApJS...59..383H
*      K: Kaas 1999AJ....118..558K, [K99d] YSO NN in Simbad
*    MMW: McMullin et al., 1994ApJ...424..222M
*   StRS: Stephenson 1992AJ....103..263S
*    SCB: Straizys et al., 1996BaltA...5..125S, [SCB96] NNN in Simbad
*    SMM: Casali et al., 1993A&A...275..195C, [CED93] N in Simbad
*   STGM: Sogawa et al., 1997AJ....113.1057S
*         STGM3  = STGM 182709.0+010535 in Simbad
*         STGM2  = STGM 182711.4+010517 in Simbad
*         STGM14 = STGM 182721.2+011101 in Simbad
*         STGM8  = STGM 182735.3+010959 in Simbad
*    SVS: Strom et al., 1976AJ.....81..638S, [SVS76] Ser NN in Simbad

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

C  Loading file 'table2.dat'	! The 77 ISOCAM sources identified as YSOs in the
*                             Serpens cluster

C  Format for file interpretation

    1 format(
     +  I3,A1,1X,I2,1X,I2,1X,F4.1,1X,A1,I1,1X,I2,1X,I2,1X,F5.2,A1,1X,
     +  A1,F5.3,1X,F5.2,A1,1X,A1,F5.3,1X,F5.2,A1,1X,A1,F5.3,1X,F6.1,
     +  A3,1X,F4.1,1X,F6.1,A3,1X,F4.1,1X,A20)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table2.dat')
      write(6,*) '....Loading file: table2.dat'
      do i__=1,77
        read(1,'(A117)')ar__
        read(ar__,1)
     +  ISO(i__),m_ISO(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
     +  DEd(i__),DEm(i__),DEs(i__),Jmag(i__),n_Jmag(i__),
     +  l_e_Jmag(i__),e_Jmag(i__),Hmag(i__),n_Hmag(i__),l_e_Hmag(i__),
     +  e_Hmag(i__),Kmag(i__),n_Kmag(i__),l_e_Kmag(i__),e_Kmag(i__),
     +  F6_7um(i__),n_F6_7um(i__),e_F6_7um(i__),F14_3um(i__),
     +  n_F14_3um(i__),e_F14_3um(i__),ID(i__)
        if(ar__(26:30) .EQ. '') Jmag(i__) = rNULL__
        if(ar__(34:38) .EQ. '') e_Jmag(i__) = rNULL__
        if(ar__(40:44) .EQ. '') Hmag(i__) = rNULL__
        if(ar__(48:52) .EQ. '') e_Hmag(i__) = rNULL__
        if(ar__(54:58) .EQ. '') Kmag(i__) = rNULL__
        if(ar__(62:66) .EQ. '') e_Kmag(i__) = rNULL__
        if(ar__(68:73) .EQ. '') F6_7um(i__) = rNULL__
        if(ar__(78:81) .EQ. '') e_F6_7um(i__) = rNULL__
        if(ar__(83:88) .EQ. '') F14_3um(i__) = rNULL__
        if(ar__(93:96) .EQ. '') e_F14_3um(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)
     +  ISO(i__),m_ISO(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
     +  DEd(i__),DEm(i__),DEs(i__),Jmag(i__),n_Jmag(i__),
     +  l_e_Jmag(i__),e_Jmag(i__),Hmag(i__),n_Hmag(i__),l_e_Hmag(i__),
     +  e_Hmag(i__),Kmag(i__),n_Kmag(i__),l_e_Kmag(i__),e_Kmag(i__),
     +  F6_7um(i__),n_F6_7um(i__),e_F6_7um(i__),F14_3um(i__),
     +  n_F14_3um(i__),e_F14_3um(i__),ID(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 'table3.dat'	! *The 71 "blue" ISOCAM sources which have
*                             [14.3/6.7]<-0.2.

C  Format for file interpretation

    2 format(
     +  I3,A1,1X,I2,1X,I2,1X,F4.1,1X,A1,I1,1X,I2,1X,I2,1X,F5.2,A1,1X,
     +  A1,F5.3,1X,F5.2,A1,1X,A1,F5.3,1X,F5.2,A1,1X,A1,F5.3,1X,F6.1,
     +  A3,1X,F4.1,1X,F6.1,A3,1X,F4.1,1X,A20)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table3.dat')
      write(6,*) '....Loading file: table3.dat'
      do i__=1,71
        read(1,'(A117)')ar__1
        read(ar__1,2)
     +  ISO_1(i__),m_ISO_1(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),
     +  DE__1(i__),DEd_1(i__),DEm_1(i__),DEs_1(i__),Jmag_1(i__),
     +  n_Jmag_1(i__),l_e_Jmag_1(i__),e_Jmag_1(i__),Hmag_1(i__),
     +  n_Hmag_1(i__),l_e_Hmag_1(i__),e_Hmag_1(i__),Kmag_1(i__),
     +  n_Kmag_1(i__),l_e_Kmag_1(i__),e_Kmag_1(i__),F6_7um_1(i__),
     +  n_F6_7um_1(i__),e_F6_7um_1(i__),F14_3um_1(i__),
     +  n_F14_3um_1(i__),e_F14_3um_1(i__),ID_1(i__)
        if(ar__1(26:30) .EQ. '') Jmag_1(i__) = rNULL__
        if(ar__1(34:38) .EQ. '') e_Jmag_1(i__) = rNULL__
        if(ar__1(40:44) .EQ. '') Hmag_1(i__) = rNULL__
        if(ar__1(48:52) .EQ. '') e_Hmag_1(i__) = rNULL__
        if(ar__1(54:58) .EQ. '') Kmag_1(i__) = rNULL__
        if(ar__1(62:66) .EQ. '') e_Kmag_1(i__) = rNULL__
        if(ar__1(68:73) .EQ. '') F6_7um_1(i__) = rNULL__
        if(ar__1(78:81) .EQ. '') e_F6_7um_1(i__) = rNULL__
        if(ar__1(83:88) .EQ. '') F14_3um_1(i__) = rNULL__
        if(ar__1(93:96) .EQ. '') e_F14_3um_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)
     +  ISO_1(i__),m_ISO_1(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),
     +  DE__1(i__),DEd_1(i__),DEm_1(i__),DEs_1(i__),Jmag_1(i__),
     +  n_Jmag_1(i__),l_e_Jmag_1(i__),e_Jmag_1(i__),Hmag_1(i__),
     +  n_Hmag_1(i__),l_e_Hmag_1(i__),e_Hmag_1(i__),Kmag_1(i__),
     +  n_Kmag_1(i__),l_e_Kmag_1(i__),e_Kmag_1(i__),F6_7um_1(i__),
     +  n_F6_7um_1(i__),e_F6_7um_1(i__),F14_3um_1(i__),
     +  n_F14_3um_1(i__),e_F14_3um_1(i__),ID_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