FORTRAN Generation
(/./ftp/cats/J/ApJ/672/558)

Conversion of standardized ReadMe file for file /./ftp/cats/J/ApJ/672/558 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_1.5, on 2013-May-24
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__=-1.e37)     	! NULL real number
      parameter  (iNULL__=-2147483647)	! NULL int  number

C=============================================================================
Cat. J/ApJ/672/558       MIPS observations of h and {chi} Persei  (Currie+, 2008)
*================================================================================
*The rise and fall of debris disks: MIPS observations of h and {chi} Persei and
*the evolution of Mid-IR emission from planet formation.
*    Currie T., Kenyon S.J., Balog Z., Rieke G., Bragg A., Bromley B.
*   <Astrophys. J., 672, 558-574 (2008)>
*   =2008ApJ...672..558C
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'table1.dat'	! MIPS sources with 2MASS/IRAC counterparts in
                              h+{chi} Persei

      integer*4 nr__
      parameter (nr__=616)	! Number of records
      character*128 ar__   	! Full-size record

      real*8        RAdeg       ! (deg) Right Ascension in decimal degrees (J2000) (1)
      real*8        DEdeg       ! (deg) Declination in decimal degrees (J2000) (1)
      real*4        Vmag        ! (mag) ?=99.000 The V band magnitude (2)
      real*4        B_V         ! (mag) ?=99.000 The (B-V) color index (2)
      real*4        U_B         ! (mag) ?=99.000 The (U-B) color index (2)
      real*4        Jmag        ! (mag) ?=99.000 2MASS J band magnitude (2)
      real*4        Hmag        ! (mag) ?=99.000 2MASS H band magnitude (2)
      real*4        Ksmag       ! (mag) ?=99.000 2MASS K_s_ band magnitude (2)
      real*4        v3_6mag     ! (mag) ?=99.000 IRAC 3.6 micron band magnitude (2)
      real*4        v4_5mag     ! (mag) ?=99.000 IRAC 4.5 micron band magnitude (2)
      real*4        v5_8mag     ! (mag) ?=99.000 IRAC 5.8 micron band magnitude (2)
      real*4        v8_0mag     ! (mag) ?=99.000 IRAC 8 micron band magnitude (2)
      real*4        v24mag      ! (mag) ?=99.000 MIPS 24 micron band magnitude (2)
      real*4        e_3_6mag    ! (mag) ?=99.000 The 1{sigma} error in 3.6mag (2)
      real*4        e_4_5mag    ! (mag) ?=99.000 The 1{sigma} error in 4.5mag (2)
      real*4        e_5_8mag    ! (mag) ?=99.000 The 1{sigma} error in 5.8mag (2)
      real*4        e_8_0mag    ! (mag) ?=99.000 The 1{sigma} error in 8.0mag (2)
      real*4        e_24mag     ! (mag) ?=99.000 The 1{sigma} error in 24mag (2)
*Note (1): Sources identified as [CKB2008] DD.dddd+DD.dddd in Simbad.
*Note (2): Optical UBV photometry from Slesnick et al. (2002, Cat.
*     J/ApJ/576/880); errors in the 2MASS JHK_s_ filters are ~<0.05 for
*     sources except the ~21 fainter (J~14-15) sources.
*     Values of 99.000 denote sources that were not observed in the given
*     filter at the 5{sigma} level.

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

C  Declarations for 'table2.dat'	! Stars/candidates and selected evolved stars
                              with 24um excess in h and {chi} Per

      integer*4 nr__1
      parameter (nr__1=57)	! Number of records
      character*67 ar__1  	! Full-size record

      integer*4     v_CKB2008_  ! Sequential number (1)
      integer*4     Num         ! ?=99 Oosterhoff (1937AnLei..17a...1O) number
      character*7   SpType      ! MK spectral type (2)
      real*8        RAdeg_1     ! (deg) Right Ascension in decimal degrees (J2000)
      real*8        DEdeg_1     ! (deg) Declination in decimal degrees (J2000)
      real*4        Vmag_1      ! (mag) ?=99.00 The V band magnitude
      real*4        Jmag_1      ! (mag) ?=99.00 2MASS J band magnitude
      real*4        Hmag_1      ! (mag) ?=99.00 2MASS H band magnitude
      real*4        Ksmag_1     ! (mag) ?=99.00 2MASS K_s_ band magnitude
      real*4        v8_0mag_1   ! (mag) ?=99.00 IRAC 8 micron band magnitude
      real*4        v24mag_1    ! (mag) ?=99.00 MIPS 24 micron band magnitude
*Note (1): The first twenty entries are confirmed Be stars from Bragg and
*     Kenyon (2002AJ....124.3289B) and have Oosterhoff (1937AnLei..17a...1O)
*     numbers. Slesnick et al. (2002, Cat. J/ApJ/576/880) identify an
*     additional Be star in lower density regions surrounding the center of
*     h and {chi} Per (source number 23). All the other stars (referred to
*     as "candidate Be stars" in the text) are either supergiants,
*     foreground stars, or B-type cluster members from either Slesnick et
*     al. (source 21) or archived spectroscopic data from FAST (the five
*     other sources).
*Note (2):  All sources with the "e" designation in spectral type are Be stars.

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

C  Loading file 'table1.dat'	! MIPS sources with 2MASS/IRAC counterparts in
*                              h+{chi} Persei

C  Format for file interpretation

    1 format(
     +  1X,F7.4,1X,F7.4,1X,F6.3,1X,F6.3,1X,F6.3,1X,F6.3,1X,F6.3,1X,
     +  F6.3,1X,F6.3,1X,F6.3,1X,F6.3,1X,F6.3,1X,F6.3,1X,F6.3,1X,F6.3,
     +  1X,F6.3,1X,F6.3,1X,F6.3)

C  Effective file loading

      open(unit=1,file='table1.dat', status='old')
      write(6,*) '....Loading file: table1.dat'
      do i__=1,616
        read(1,'(A128)')ar__
        read(ar__,1)
     +  RAdeg,DEdeg,Vmag,B_V,U_B,Jmag,Hmag,Ksmag,v3_6mag,v4_5mag,
     +  v5_8mag,v8_0mag,v24mag,e_3_6mag,e_4_5mag,e_5_8mag,e_8_0mag,
     +  e_24mag
c    ..............Just test output...........
        write(6,1)
     +  RAdeg,DEdeg,Vmag,B_V,U_B,Jmag,Hmag,Ksmag,v3_6mag,v4_5mag,
     +  v5_8mag,v8_0mag,v24mag,e_3_6mag,e_4_5mag,e_5_8mag,e_8_0mag,
     +  e_24mag
c    .......End.of.Just test output...........
      end do
      close(1)

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

C  Loading file 'table2.dat'	! Stars/candidates and selected evolved stars
*                              with 24um excess in h and {chi} Per

C  Format for file interpretation

    2 format(
     +  I2,1X,I4,1X,A7,1X,F7.4,1X,F7.4,1X,F5.2,1X,F5.2,1X,F5.2,1X,
     +  F5.2,1X,F5.2,1X,F5.2)

C  Effective file loading

      open(unit=1,file='table2.dat', status='old')
      write(6,*) '....Loading file: table2.dat'
      do i__=1,57
        read(1,'(A67)')ar__1
        read(ar__1,2)
     +  v_CKB2008_,Num,SpType,RAdeg_1,DEdeg_1,Vmag_1,Jmag_1,Hmag_1,
     +  Ksmag_1,v8_0mag_1,v24mag_1
c    ..............Just test output...........
        write(6,2)
     +  v_CKB2008_,Num,SpType,RAdeg_1,DEdeg_1,Vmag_1,Jmag_1,Hmag_1,
     +  Ksmag_1,v8_0mag_1,v24mag_1
c    .......End.of.Just test output...........
      end do
      close(1)

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