FORTRAN Generation
(/./ftp/cats/J/ApJS/112/245)

Conversion of standardized ReadMe file for file /./ftp/cats/J/ApJS/112/245 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-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/ApJS/112/245      Redshift survey for IRAS galaxies (Nakanishi+ 1997)
*================================================================================
*Search and redshift survey for IRAS galaxies behind the Milky Way and
*structure of the Local Void
*       Nakanishi K., Takata T., Yamada T., Takeuchi T.T., Shiroya R.,
*       Miyazawa M., Watanabe S., Saito M.
*      <Astrophys. J. Suppl. Ser. 112, 245 (1997)>
*      =1997ApJS..112..245N      (SIMBAD/NED BibCode)
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'table5.dat'	! The catalog of IRAS galaxies with F60>=0.6Jy

      integer*4 nr__
      parameter (nr__=950)	! Number of records
      character*106 ar__   	! Full-size record

C  Position composed of: GLON GLAT
      character*10  IRAS        ! IRAS (Cat. <II/125>) point source name
      character*1   m_IRAS      ! Multiplicity index in IRAS
      real*8        GLON        ! (deg) Galactic longitude
      real*8        GLAT        ! (deg) Galactic latitude
      real*4        F60um       ! (Jy) Flux density at 60{mu}m
      real*4        F100um      ! (Jy) Flux density at 100{mu}m
      character*2   Gal_        ! [G? ] G: galaxy; G?: possible galaxy
      character*3   MType       ! Morphological type (1)
      real*4        Dmaj        ! (mm) ? Major axis diameter (1mm = 67")
      real*4        Dmin        ! (mm) ? Minor axis diameter (1mm = 67")
      character*1   Note        ! [IJ] Emulsion (2)
      character*9   Com         ! Comment on multiplicity (3)
      integer*4     cz          ! (km/s) ? Heliocentric radial velocity
      character*2   r_cz        ! Reference for cz (4)
      character*25  Ident       ! Cross-identification
*Note (1): E: elliptical galaxy
*          S: spiral galaxy
*          I: Irregular galaxy
*        E/S: galaxy we could not classified
*Note (2): I: UK Schmidt I film copy
*          J: ESO/SRC J film copy
*      blank: POSS E paper prints
*Note (3): For multiplicity:
*             pair: two galaxies are located within a separation as wide as the
*                    galaxy sizes
*              tri: triplet
*            group: group of galaxies
*              int: two galaxies appear to be interacting
*          For image appearance:
*             PN?: possible planetary nebula
*             LSB: low surface brightness
*             HSB: high surface brightness
*              ND: nuclear dominated
*             pec: peculiar.
*Note (4): A: Measurement at OAO by us
*          1: RC3, de Vaucouleurs et al. (1991, Cat. <VII/155>)
*          2:  General Catalog of H I Observations of Galaxies (Huchtmeier &
*               Richter, 1989, New York: Springer)
*          3: "1.936 Jy sample" by Strauss et al. (1992, Cat. <II/174>)
*          4: Lu et al. (1990ApJ...357..388L)
*          5: Seeberger, Huchtmeier, & Weinberger (1994, Cat. <J/A+A/286/17>)
*          6: Bottinelli et al. (1994, ASP Conf. Ser. 67, 225)
*          7:  "1.2 Jy sample" by Fisher et al. (1995, Cat. <VII/185>)
*          8: Kraan-Korteweg et al. (1994Natur.372...77K)
*          9: Weinberger, Saurer & Seeberger (1995, Cat. <J/A+AS/110/269>)
*         10: Marzke, Huchra, & Geller (1996, Cat. <J/AJ/112/1803>)
*         11: The IRAS PSC Redshift Survey (PSCz)" and the extension to low
*              latitude BTP survey by Saunders et al. (1997, Priv. Comm.)

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

C  Declarations for 'table6.dat'	! Radial velocities of IRAS galaxies with
                                 F60>=0.6Jy at 150<l<225 and |b|<=15

      integer*4 nr__1
      parameter (nr__1=27)	! Number of records
      character*56 ar__1  	! Full-size record

C  Position composed of: GLON GLAT
      character*10  IRAS_1      ! IRAS point source name
      real*8        GLON_1      ! (deg) Galactic longitude
      real*8        GLAT_1      ! (deg) Galactic latitude
      real*4        F60um_1     ! (Jy) Flux density at 60{mu}m
      real*4        F100um_1    ! (Jy) Flux density at 100{mu}m
      integer*4     cz_1        ! (km/s) Heliocentric radial velocity (this paper)
      character*12  Ident_1     ! Cross-identification

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

C  Loading file 'table5.dat'	! The catalog of IRAS galaxies with F60>=0.6Jy

C  Format for file interpretation

    1 format(
     +  A10,A1,1X,F7.3,1X,F7.3,1X,F5.2,1X,F6.2,2X,A2,1X,A3,1X,F4.1,1X,
     +  F4.1,1X,A1,1X,A9,1X,I5,1X,A2,1X,A25)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table5.dat')
      write(6,*) '....Loading file: table5.dat'
      do i__=1,950
        read(1,'(A106)')ar__
        read(ar__,1)
     +  IRAS,m_IRAS,GLON,GLAT,F60um,F100um,Gal_,MType,Dmaj,Dmin,Note,
     +  Com,cz,r_cz,Ident
        if(ar__(50:53) .EQ. '') Dmaj = rNULL__
        if(ar__(55:58) .EQ. '') Dmin = rNULL__
        if(ar__(72:76) .EQ. '') cz = iNULL__
c    ..............Just test output...........
        write(6,1)
     +  IRAS,m_IRAS,GLON,GLAT,F60um,F100um,Gal_,MType,Dmaj,Dmin,Note,
     +  Com,cz,r_cz,Ident
c    .......End.of.Just test output...........
      end do
      close(1)

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

C  Loading file 'table6.dat'	! Radial velocities of IRAS galaxies with
*                                 F60>=0.6Jy at 150<l<225 and |b|<=15

C  Format for file interpretation

    2 format(A10,1X,F7.3,1X,F7.3,1X,F4.2,1X,F5.2,1X,I5,1X,A12)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table6.dat')
      write(6,*) '....Loading file: table6.dat'
      do i__=1,27
        read(1,'(A56)')ar__1
        read(ar__1,2)
     +  IRAS_1,GLON_1,GLAT_1,F60um_1,F100um_1,cz_1,Ident_1
c    ..............Just test output...........
        write(6,2)
     +  IRAS_1,GLON_1,GLAT_1,F60um_1,F100um_1,cz_1,Ident_1
c    .......End.of.Just test output...........
      end do
      close(1)

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