FORTRAN Generation
(/./ftp/cats/J/A_A/513/A29)

Conversion of standardized ReadMe file for file /./ftp/cats/J/A_A/513/A29 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-Jun-08
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/513/A29       RACE-OC project: M11 (NGC6705)           (Messina+, 2010)
*================================================================================
*RACE-OC Project: Rotation and variability in the open cluster M11 (NGC6705).
*    Messina S., Padmakar Parihar, Koo J.R., Kim S.-L., Rey S.-C., Lee C.-U.
*   <Astron. Astrophys. 513, A29 (2010)>
*   =2010A&A...513A..29M
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'table1.dat'	! Summary of rotation period search

      integer*4 nr__
      parameter (nr__=75)	! Number of records
      character*88 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)

      integer*4     Target     (nr__) ! Target's internal ID number
      integer*4     Webda      (nr__) ! ?=- Target's Webda number (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)
      real*4        DEs        (nr__) ! (arcsec) Declination (J2000.0)
      real*8        Per        (nr__) ! (d) Period from Scargle analysis (2)
      real*8        e_Per      (nr__) ! (d) Uncertainty on the adopted period
      real*4        PN         (nr__) ! Normalized power from Scargle periodogram (2)
      real*4        v_Vmag_    (nr__) ! (mag) Mean V magnitude
      real*4        v_B_V_0    (nr__) ! (mag) Dereddened B-V color index
      real*4        Vsig       (nr__) ! (mag) V-band photometric accuracy
      real*4        Vamp       (nr__) ! (mag) V-band light curve amplitude
      character*1   Mm         (nr__) ! [abn] Membership code (1)
      character*1   Ecl        (nr__) ! [yn] detected eclipse (yes or no)
*Note (1): Membership probability flag as follows:
*      n = non members
*      b = low-probability members
*      a = high-probability members
*Note (2): The Scargle technique has been developed to search for
*     significant periodicities in unevenly sampled data, see Scargle
*     1982ApJ...263..835S), Horne & Baliunas (1986ApJ...302..757H). The
*     algorithm calculates the normalized power of each frequency PN. The
*     normalized power corresponding to a probability of a false alarm of 1%
*     (i.e. the detected frequency is due to the noise at a probability
*     level of 1%) is PN=9.2.

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

C  Declarations for 'table2.dat'	! Photometric time series of periodic variables

      integer*4 nr__1
      parameter (nr__1=8141)	! Number of records
      character*33 ar__1  	! Full-size record

      integer*4     Target_1   (nr__1) ! Target's internal ID number (G1)
      real*8        HJD        (nr__1) ! (d) Heliocentric Julian Day
      real*8        Vmag       (nr__1) ! (mag) V-band magnitude
      real*4        e_Vmag     (nr__1) ! (mag) Uncertainty on Vmag

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

C  Loading file 'table1.dat'	! Summary of rotation period search

C  Format for file interpretation

    1 format(
     +  I5,1X,I5,1X,I2,1X,I2,1X,F6.3,1X,A1,I2,1X,I2,1X,F5.2,1X,F7.4,
     +  F7.4,1X,F5.2,1X,F5.2,1X,F5.2,1X,F6.4,1X,F6.4,1X,A1,1X,A1)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table1.dat')
      write(6,*) '....Loading file: table1.dat'
      do i__=1,75
        read(1,'(A88)')ar__
        read(ar__,1)
     +  Target(i__),Webda(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
     +  DEd(i__),DEm(i__),DEs(i__),Per(i__),e_Per(i__),PN(i__),
     +  v_Vmag_(i__),v_B_V_0(i__),Vsig(i__),Vamp(i__),Mm(i__),Ecl(i__)
        if (Webda(i__) .EQ. 45) Webda(i__) =  iNULL__
        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)
     +  Target(i__),Webda(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
     +  DEd(i__),DEm(i__),DEs(i__),Per(i__),e_Per(i__),PN(i__),
     +  v_Vmag_(i__),v_B_V_0(i__),Vsig(i__),Vamp(i__),Mm(i__),Ecl(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 'table2.dat'	! Photometric time series of periodic variables

C  Format for file interpretation

    2 format(I5,1X,F12.4,1X,F7.4,1X,F6.4)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table2.dat')
      write(6,*) '....Loading file: table2.dat'
      do i__=1,8141
        read(1,'(A33)')ar__1
        read(ar__1,2)Target_1(i__),HJD(i__),Vmag(i__),e_Vmag(i__)
c    ..............Just test output...........
        write(6,2)Target_1(i__),HJD(i__),Vmag(i__),e_Vmag(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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