FORTRAN Generation
(/./ftp/cats/J/A_A/404/223)

Conversion of standardized ReadMe file for file /./ftp/cats/J/A_A/404/223 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 2024-Apr-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/A+A/404/223       2MASS IR star clusters in the Galaxy           (Bica+, 2003)
*================================================================================
*New infrared star clusters in the Northern and Equatorial Milky Way with 2MASS.
*    Bica E., Dutra C.M., Soares J., Barbuy B.
*   <Astron. Astrophys. 404, 223 (2003)>
*   =2003A&A...404..223B
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'table1.dat'	! New objects in the area of optical nebulae

      integer*4 nr__
      parameter (nr__=103)	! Number of records
      character*140 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)

      integer*4     v_BDS2003_  ! [1/167] Object sequential number
      character*1   n__BDS2003_ ! [a-g] Individual notes (1)
      real*4        GLON        ! (deg) Galactic longitude
      real*4        GLAT        ! (deg) Galactic latitude
      integer*4     RAh         ! (h) Right ascension (J2000)
      integer*4     RAm         ! (min) Right ascension (J2000)
      integer*4     RAs         ! (s) Right ascension (J2000)
      character*1   DE_         ! Declination sign (J2000)
      integer*4     DEd         ! (deg) Declination (J2000)
      integer*4     DEm         ! (arcmin) Declination (J2000)
      integer*4     DEs         ! (arcsec) Declination (J2000)
      real*4        Dmaj        ! (arcmin) Major angular dimension
      real*4        Dmin        ! (arcmin) Minor angular dimension
      character*53  Neb         ! Related Nebulae (2)
      character*1   n_Neb       ! [a-j] Note on Neb (3)
      character*4   Class       ! Classification (4)
      character*32  Rem         ! Remarks (5)
*Note (1): Notes are coded as follows:
*     a: triplet with the NGC 6857 and K3-50B clusters (Bica et al., 2003,
*        Cat. <J/A+A/397/177>)
*     b: the present Objects 54, 55 and 56 form a quadruplet with the
*        W3-IRS5 Cluster (Bica et al., 2003, Cat. <J/A+A/397/177>),
*     c: the present Objects 71, 72 and 73 together with the Sh2-235B
*        Cluster form a quadruplet,
*     d: in Object NGC 6334V (Bica et al., 2003, Cat. <J/A+A/397/177>)
*     e: quadruplet with W49A, W49A-east and W49A-southwest clusters
*        (Bica et al., 2003, Cat. <J/A+A/397/177>)
*     f: the 2MASS images indicate stellar sources which suggest a small
*        stellar group
*     g: NGC 7538 IR Cluster in Bica et al. (2003, Cat. <J/A+A/397/177>)
*        can be divided into a large loose NW and a compact SE
*        (NGC 7538-IRS1 Cluster) components. These two clusters together
*        with the present object form a triplet,
*Note (2):
*     In Simbad, GM1-45 = GM 3-45, Gy82-13 = [G82a] 13, Gy 3-4 = [G84c] 4
*Note (3): Notes on nebulae as follows:
*     a: in Hourglass Nebula (Woodward et al., 1990ApJ...365..252W),
*        in Ced152a = IRAS 18009-2427 = G5.956-1.265,
*     b: = Gy82-2 = IRAS 02534+6029,
*     c: in Sh2-206,
*     d: in Ced61 = DG86,
*     e: in NGC 6334=RCW127 = CTB39.
*     f: in W51d = W51-IRS2 (Goldader & Wynn-Wiliams, 1994ApJ...433..164G)
*     g: in W51e = W51-IRS1-North
*        (Goldader & Wynn-Wiliams, 1994ApJ...433..164G)
*     h: in W51-IRS1-South (Goldader & Wynn-Wiliams, 1994ApJ...433..164G)
*     i: Tapia et al. (1985MNRAS.213..833T),
*     j: the 2MASS images indicate several stellar sources which suggest
*        a small cluster or stellar group around the massive YSO
*        (Marengo et al., 2000ApJ...541L..63M),
*Note (4): Object classes:
*     IRC: infrared cluster
*     IRCC: cluster candidate
*     IRGr: stellar group
*     IROC: open cluster
*Note (5): Remarks including distance (in case of kinematical ambiguity
*     the near and far distances are shown), multiplicity and linear dimension.

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

C  Declarations for 'table2.dat'	! New objects in the area of radio/infrared nebulae

      integer*4 nr__1
      parameter (nr__1=64)	! Number of records
      character*140 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)

      integer*4     v_BDS2003__1 ! [1/167] Object sequential number
      character*1   n__BDS2003__1 ! [a-g] Individual notes (1)
      real*4        GLON_1      ! (deg) Galactic longitude
      real*4        GLAT_1      ! (deg) Galactic latitude
      integer*4     RAh_1       ! (h) Right ascension (J2000)
      integer*4     RAm_1       ! (min) Right ascension (J2000)
      integer*4     RAs_1       ! (s) Right ascension (J2000)
      character*1   DE__1       ! Declination sign (J2000)
      integer*4     DEd_1       ! (deg) Declination (J2000)
      integer*4     DEm_1       ! (arcmin) Declination (J2000)
      integer*4     DEs_1       ! (arcsec) Declination (J2000)
      real*4        Dmaj_1      ! (arcmin) Major angular dimension
      real*4        Dmin_1      ! (arcmin) Minor angular dimension
      character*53  Neb_1       ! Related Nebulae (2)
      character*1   n_Neb_1     ! [a-j] Note on Neb (3)
      character*4   Class_1     ! Classification (4)
      character*32  Rem_1       ! Remarks (5)
*Note (1): Notes are coded as follows:
*     a: triplet with the NGC 6857 and K3-50B clusters (Bica et al., 2003,
*        Cat. <J/A+A/397/177>)
*     b: the present Objects 54, 55 and 56 form a quadruplet with the
*        W3-IRS5 Cluster (Bica et al., 2003, Cat. <J/A+A/397/177>),
*     c: the present Objects 71, 72 and 73 together with the Sh2-235B
*        Cluster form a quadruplet,
*     d: in Object NGC 6334V (Bica et al., 2003, Cat. <J/A+A/397/177>)
*     e: quadruplet with W49A, W49A-east and W49A-southwest clusters
*        (Bica et al., 2003, Cat. <J/A+A/397/177>)
*     f: the 2MASS images indicate stellar sources which suggest a small
*        stellar group
*     g: NGC 7538 IR Cluster in Bica et al. (2003, Cat. <J/A+A/397/177>)
*        can be divided into a large loose NW and a compact SE
*        (NGC 7538-IRS1 Cluster) components. These two clusters together
*        with the present object form a triplet,
*Note (2):
*     In Simbad, GM1-45 = GM 3-45, Gy82-13 = [G82a] 13, Gy 3-4 = [G84c] 4
*Note (3): Notes on nebulae as follows:
*     a: in Hourglass Nebula (Woodward et al., 1990ApJ...365..252W),
*        in Ced152a = IRAS 18009-2427 = G5.956-1.265,
*     b: = Gy82-2 = IRAS 02534+6029,
*     c: in Sh2-206,
*     d: in Ced61 = DG86,
*     e: in NGC 6334=RCW127 = CTB39.
*     f: in W51d = W51-IRS2 (Goldader & Wynn-Wiliams, 1994ApJ...433..164G)
*     g: in W51e = W51-IRS1-North
*        (Goldader & Wynn-Wiliams, 1994ApJ...433..164G)
*     h: in W51-IRS1-South (Goldader & Wynn-Wiliams, 1994ApJ...433..164G)
*     i: Tapia et al. (1985MNRAS.213..833T),
*     j: the 2MASS images indicate several stellar sources which suggest
*        a small cluster or stellar group around the massive YSO
*        (Marengo et al., 2000ApJ...541L..63M),
*Note (4): Object classes:
*     IRC: infrared cluster
*     IRCC: cluster candidate
*     IRGr: stellar group
*     IROC: open cluster
*Note (5): Remarks including distance (in case of kinematical ambiguity
*     the near and far distances are shown), multiplicity and linear dimension.

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

C  Loading file 'table1.dat'	! New objects in the area of optical nebulae

C  Format for file interpretation

    1 format(
     +  I3,A1,1X,F6.2,1X,F6.2,1X,I2,1X,I2,1X,I2,1X,A1,I2,1X,I2,1X,I2,
     +  1X,F4.2,1X,F4.2,1X,A53,A1,1X,A4,1X,A32)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table1.dat')
      write(6,*) '....Loading file: table1.dat'
      do i__=1,103
        read(1,'(A140)')ar__
        read(ar__,1)
     +  v_BDS2003_,n__BDS2003_,GLON,GLAT,RAh,RAm,RAs,DE_,DEd,DEm,DEs,
     +  Dmaj,Dmin,Neb,n_Neb,Class,Rem
        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)
     +  v_BDS2003_,n__BDS2003_,GLON,GLAT,RAh,RAm,RAs,DE_,DEd,DEm,DEs,
     +  Dmaj,Dmin,Neb,n_Neb,Class,Rem
        write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c    .......End.of.Just test output...........
      end do
      close(1)

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

C  Loading file 'table2.dat'	! New objects in the area of radio/infrared nebulae

C  Format for file interpretation

    2 format(
     +  I3,A1,1X,F6.2,1X,F6.2,1X,I2,1X,I2,1X,I2,1X,A1,I2,1X,I2,1X,I2,
     +  1X,F4.2,1X,F4.2,1X,A53,A1,1X,A4,1X,A32)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table2.dat')
      write(6,*) '....Loading file: table2.dat'
      do i__=1,64
        read(1,'(A140)')ar__1
        read(ar__1,2)
     +  v_BDS2003__1,n__BDS2003__1,GLON_1,GLAT_1,RAh_1,RAm_1,RAs_1,
     +  DE__1,DEd_1,DEm_1,DEs_1,Dmaj_1,Dmin_1,Neb_1,n_Neb_1,Class_1,
     +  Rem_1
        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)
     +  v_BDS2003__1,n__BDS2003__1,GLON_1,GLAT_1,RAh_1,RAm_1,RAs_1,
     +  DE__1,DEd_1,DEm_1,DEs_1,Dmaj_1,Dmin_1,Neb_1,n_Neb_1,Class_1,
     +  Rem_1
        write(6,'(6H Pos: 2F8.4)') RAdeg_1,DEdeg_1
c    .......End.of.Just test output...........
      end do
      close(1)

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