FORTRAN Generation
(/./ftp/cats/J/MNRAS/445/2223)

Conversion of standardized ReadMe file for file /./ftp/cats/J/MNRAS/445/2223 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-Mar-28
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/MNRAS/445/2223    Mass estimation for FGK stars            (Pinheiro+, 2014)
*================================================================================
*On the mass estimation for FGK stars: comparison of several methods.
*    Pinheiro F.J.G., Fernandes J.M., Cunha M.S., Monteiro M.J.P.F.G.,
*    Santos N.C., Sousa S.G., Marques J.P., Fang J.-J., Mortier A., Sousa J.
*   <Mon. Not. R. Astron. Soc., 445, 2223-2231 (2014)>
*   =2014MNRAS.445.2223P
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'tablea1.dat'	! Mass estimate for the targets from Sousa et al.
                            2008 (J/A+A/487/373) according to different methods

      integer*4 nr__
      parameter (nr__=451)	! Number of records
      character*98 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     Seq        (nr__) ! [1/451] Sequential number
      character*10  Name       (nr__) ! Star's identifier
      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)
      real*4        DEs        (nr__) ! (arcsec) Declination (J2000)
      real*4        M1         (nr__) ! (Msun) [0.6/1.4] Direct estimation of the stellar
*                              mass using the spectroscopic surface gravity
      real*4        e_M1       (nr__) ! (Msun) [0.04/0.12] Error in M1
      real*4        M2         (nr__) ! (Msun) [0.1/2.9] Estimation of the stellar mass using
*                              the method of Torres et al.  (2010AJ....140.1158T)
      real*4        e_M2       (nr__) ! (Msun) [0.03/2.5] Error in M2
      real*4        M3         (nr__) ! (Msun) [0.6/1.5] Estimation of the stellar mass
*                              using the method of Henry & McCarthy
*                              (1993AJ....106..773H)
      real*4        e_M3       (nr__) ! (Msun) [0.05/0.11] Error in M3
      real*4        M4         (nr__) ! (Msun) [0.5/1.4] Estimation of the stellar mass using
*                              the Padova models
      real*4        e_M4       (nr__) ! (Msun) [0.05/0.08] Error in M4
      real*4        M          (nr__) ! (Msun) [0.6/1.5] Median of the previous 4 mass estimates
      real*4        e_M        (nr__) ! (Msun) [0.03/0.08] Error in M

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

C  Declarations for 'tablea2.dat'	! Mass estimate for the targets from Sousa et al.
                            2011 (J/A+A/533/A141) according to different methods

      integer*4 nr__1
      parameter (nr__1=582)	! Number of records
      character*97 ar__1  	! Full-size record

C  J2000 position composed of: RAdeg DEdeg
      integer*4     Seq_1      (nr__1) ! [1/582] Sequential number
      character*10  Name_1     (nr__1) ! Star's identifier
      real*8        RAdeg_1    (nr__1) ! (deg) Right ascension (J2000)
      real*8        DEdeg_1    (nr__1) ! (deg) Declination (J2000)
      real*4        M1_1       (nr__1) ! (Msun) [0.6/1.5] Direct estimation of the stellar mass
*                               using the spectroscopic surface gravity
      real*4        e_M1_1     (nr__1) ! (Msun) [0.03/0.1] Error in M1
      real*4        M2_1       (nr__1) ! (Msun) [0.037/4.1] Estimation of the stellar mass using
*                               the method of Torres et al. (2010AJ....140.1158T)
      real*8        e_M2_1     (nr__1) ! (Msun) [0.03/1049] Error in M2
      real*4        M3_1       (nr__1) ! (Msun) [0.6/1.8] Estimation of the stellar mass using
*                               method of Henry & McCarthy (1993AJ....106..773H)
      real*4        e_M3_1     (nr__1) ! (Msun) [0.03/0.13] Error in M3
      real*4        M4_1       (nr__1) ! (Msun) [0.5/1.8] Estimation of the stellar mass using
*                               the Padova models
      real*4        e_M4_1     (nr__1) ! (Msun) [0.03/0.11] Error in M4
      real*4        M_1        (nr__1) ! (Msun) [0.5/1.8] Median of the previous 4 mass estimates
      real*4        e_M_1      (nr__1) ! (Msun) [0.02/0.12] Error in M

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

C  Declarations for 'tablea3.dat'	! Mass estimate for the targets from Bruntt et al.
                            (2010MNRAS.405.1907B) according to different methods

      integer*4 nr__2
      parameter (nr__2=22)	! Number of records
      character*75 ar__2  	! Full-size record

      integer*4     Seq_2      (nr__2) ! [1/22] Sequential number
      character*11  Name_2     (nr__2) ! Star's identifier
      real*4        M1_2       (nr__2) ! (Msun) [0.7/2.2] Direct estimation of the stellar mass
*                               using the spectroscopic surface gravity
      real*4        e_M1_2     (nr__2) ! (Msun) [0.05/0.3] Error in M1
      real*4        M2_2       (nr__2) ! (Msun) [0.9/2.9] Estimation of the stellar mass using
*                               the method of Torres et al. (2010AJ....140.1158T)
      real*4        e_M2_2     (nr__2) ! (Msun) [0.4/1.4] Error in M2
      real*4        M3_2       (nr__2) ! (Msun) [0.9/2.5] Estimation of the stellar mass using
*                               method of Henry & McCarthy (1993AJ....106..773H)
      real*4        e_M3_2     (nr__2) ! (Msun) [0.06/0.2] Error in M3
      real*4        M4_2       (nr__2) ! (Msun) [0.7/2.9] Estimation of the stellar mass using
*                               the Padova models
      real*4        e_M4_2     (nr__2) ! (Msun) [0.05/0.2] Error in M4
      real*4        M_2        (nr__2) ! (Msun) [0.8/2.7] Median of the previous 4 mass estimates
      real*4        e_M_2      (nr__2) ! (Msun) [0.05/0.24] Error in M

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

C  Loading file 'tablea1.dat'	! Mass estimate for the targets from Sousa et al.
*                            2008 (J/A+A/487/373) according to different methods

C  Format for file interpretation

    1 format(
     +  I3,1X,A10,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F5.3,
     +  1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,
     +  F5.3,1X,F5.3)

C  Effective file loading

      open(unit=1,status='old',file=
     +'tablea1.dat')
      write(6,*) '....Loading file: tablea1.dat'
      do i__=1,451
        read(1,'(A98)')ar__
        read(ar__,1)
     +  Seq(i__),Name(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
     +  DEd(i__),DEm(i__),DEs(i__),M1(i__),e_M1(i__),M2(i__),
     +  e_M2(i__),M3(i__),e_M3(i__),M4(i__),e_M4(i__),M(i__),e_M(i__)
        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)
     +  Seq(i__),Name(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
     +  DEd(i__),DEm(i__),DEs(i__),M1(i__),e_M1(i__),M2(i__),
     +  e_M2(i__),M3(i__),e_M3(i__),M4(i__),e_M4(i__),M(i__),e_M(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 'tablea2.dat'	! Mass estimate for the targets from Sousa et al.
*                            2011 (J/A+A/533/A141) according to different methods

C  Format for file interpretation

    2 format(
     +  I3,1X,A10,1X,F9.5,1X,F9.5,1X,F5.3,1X,F5.3,1X,F5.3,1X,F8.3,1X,
     +  F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3)

C  Effective file loading

      open(unit=1,status='old',file=
     +'tablea2.dat')
      write(6,*) '....Loading file: tablea2.dat'
      do i__=1,582
        read(1,'(A97)')ar__1
        read(ar__1,2)
     +  Seq_1(i__),Name_1(i__),RAdeg_1(i__),DEdeg_1(i__),M1_1(i__),
     +  e_M1_1(i__),M2_1(i__),e_M2_1(i__),M3_1(i__),e_M3_1(i__),
     +  M4_1(i__),e_M4_1(i__),M_1(i__),e_M_1(i__)
c    ..............Just test output...........
        write(6,2)
     +  Seq_1(i__),Name_1(i__),RAdeg_1(i__),DEdeg_1(i__),M1_1(i__),
     +  e_M1_1(i__),M2_1(i__),e_M2_1(i__),M3_1(i__),e_M3_1(i__),
     +  M4_1(i__),e_M4_1(i__),M_1(i__),e_M_1(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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

C  Loading file 'tablea3.dat'	! Mass estimate for the targets from Bruntt et al.
*                            (2010MNRAS.405.1907B) according to different methods

C  Format for file interpretation

    3 format(
     +  I3,1X,A11,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,
     +  F5.3,1X,F5.3,1X,F5.3,1X,F5.3)

C  Effective file loading

      open(unit=1,status='old',file=
     +'tablea3.dat')
      write(6,*) '....Loading file: tablea3.dat'
      do i__=1,22
        read(1,'(A75)')ar__2
        read(ar__2,3)
     +  Seq_2(i__),Name_2(i__),M1_2(i__),e_M1_2(i__),M2_2(i__),
     +  e_M2_2(i__),M3_2(i__),e_M3_2(i__),M4_2(i__),e_M4_2(i__),
     +  M_2(i__),e_M_2(i__)
c    ..............Just test output...........
        write(6,3)
     +  Seq_2(i__),Name_2(i__),M1_2(i__),e_M1_2(i__),M2_2(i__),
     +  e_M2_2(i__),M3_2(i__),e_M3_2(i__),M4_2(i__),e_M4_2(i__),
     +  M_2(i__),e_M_2(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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