FORTRAN Generation
(/./ftp/cats/J/ApJ/675/1213)

Conversion of standardized ReadMe file for file /./ftp/cats/J/ApJ/675/1213 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_1.5, on 2013-May-19
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/675/1213      Abundances in M33 HII regions            (Rosolowsky+, 2008)
*================================================================================
*The M33 metallicity project: resolving the abundance gradient discrepancies in
*M33.
*    Rosolowsky E., Simon J.D.
*   <Astrophys. J., 675, 1213-1222 (2008)>
*   =2008ApJ...675.1213R
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'table1.dat'	! HII region line fluxes

      integer*4 nr__
      parameter (nr__=63)	! Number of records
      character*126 ar__   	! Full-size record

      real*8        RA_        (nr__) ! (deg) Right Ascension J2000.0
      real*8        Dec        (nr__) ! (deg)     Declination J2000.0
      integer*4     Seq        (nr__) ! [1/61] Sequential number
      character*1   n_Seq      (nr__) ! [d] Same object observed on multiple
*                                         slit masks
      integer*4     RAh        (nr__) ! (h) Right ascension (J2000.0) (1)
      integer*4     RAm        (nr__) ! (min) Right ascension (J2000.0) (1)
      real*4        RAs        (nr__) ! (s) Right ascension (J2000.0) (1)
      character*1   DE_        (nr__) ! Declination sign (J2000.0) (1)
      integer*4     DEd        (nr__) ! (deg) Declination (J2000.0) (1)
      integer*4     DEm        (nr__) ! (arcmin) Declination (J2000.0) (1)
      integer*4     DEs        (nr__) ! (arcsec) Declination (J2000.0) (1)
      character*6   Name       (nr__) ! Cross-identifications (2)
      real*4        Rgal       (nr__) ! (kpc) Galactocentric distance
      real*4        F_OII_     (nr__) ! Flux of [OII]{lambda}3727 line (3)
      real*4        e_F_OII_   (nr__) ! rms uncertainty on F[OII]
      real*4        F_NeIII_   (nr__) ! Flux of [NeIII]{lambda}3869 line (3)
      real*4        e_F_NeIII_ (nr__) ! rms uncertainty on F[NeIII]
      real*8        F_OIII_1   (nr__) ! Flux of [OIII]{lambda} 4363 (3)
      real*4        e_F_OIII_1 (nr__) ! rms uncertainty on F[OIII]
      real*4        F_OIII_2   (nr__) ! Flux of [OIII]{lambda} 4959 (3)
      real*4        e_F_OIII_2 (nr__) ! rms uncertainty on F[OIII]
      real*4        F_OIII_3   (nr__) ! Flux of [OIII]{lambda} 5007 (3)
      real*4        e_F_OIII_3 (nr__) ! rms uncertainty on F[OIII]
      integer*4     Te__OIII_  (nr__) ! (K) Electron temperature, from [OIII] lines
      integer*4     e_Te__OIII_(nr__) ! (K) rms uncertainty on Te([OIII])
      real*4        eps_O      (nr__) ! Oxygen abundance{epsilson}(O)=12+log(O/H)
      real*4        e_eps_O    (nr__) ! rms uncertainty on oxygen abundance
*Note (1): Actual position observed based on targets identified in the Local
*          Group Survey images of Massey et al. (2006, Cat. J/AJ/131/2478).
*Note (2): Closest matching cataloged HII region for observed coordinates.
*          Catalog abbreviations are:
*     MA = Mayall & Aller (1942ApJ....95....5M), [MA42] NNa in Simbad
*      S = Searle (1971ApJ...168..327S), [S71] M 33 NN in Simbad
*      B = Boulesteix et al. (1974A&A....37...33B), BCLMP NNNNA in Simbad
*      C = Courtes et al. (1987A&A...174...28C), CPSDP NNNA in Simbad
*    Full designations of substructure within individual HII regions
*    (indicated by the letters at the end of the catalog names) are taken
*    from Hodge et al. (2002, An Atlas of Local Group Galaxies (Dordrecht:
*    Kluwer)).
*Note (3): Extinction-corrected line fluxes relative to H{beta}=1.

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

C  Declarations for 'table2.dat'	! Balmer series line ratios and derived properties

      integer*4 nr__1
      parameter (nr__1=63)	! Number of records
      character*99 ar__1  	! Full-size record

      integer*4     Seq_1      (nr__1) ! [1/61] Running identification number
      character*1   f_EWHb     (nr__1) ! [b] b when equivalent width was poorly defined
      real*8        EWHb       (nr__1) ! (0.1nm) ? H{beta} emission line equivalent width
      real*4        e_EWHb     (nr__1) ! (0.1nm) ? Uncertainty in EWHb
      real*4        cHb        (nr__1) ! H{beta} reddening correction
      real*4        e_cHb      (nr__1) ! Uncertainty in cHb
      real*4        EW_        (nr__1) ! (0.1nm) Stellar absorption equivalent width
      real*4        e_EW_      (nr__1) ! (0.1nm) Uncertainty in EW*
      real*4        OHg        (nr__1) ! Observed H{gamma} relative to H{beta}
      real*4        OHd        (nr__1) ! Observed H{delta} relative to H{beta}
      real*8        OH7        (nr__1) ! Observed H7 relative to H{beta}
      real*8        OH9        (nr__1) ! Observed H9 relative to H{beta}
      real*4        Hgc        (nr__1) ! Extinction/Absorption corrected H{gamma}
      real*4        Hdc        (nr__1) ! Extinction/Absorption corrected H{delta}
      real*4        H7c        (nr__1) ! Extinction/Absorption corrected H7
      real*4        H9c        (nr__1) ! Extinction/Absorption corrected H9

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

C  Loading file 'table1.dat'	! HII region line fluxes

C  Format for file interpretation

    1 format(
     +  I2,A1,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,1X,A6,1X,F4.2,
     +  1X,F5.3,1X,F5.3,1X,F6.4,1X,F6.4,1X,F7.5,1X,F6.4,1X,F6.4,1X,
     +  F6.4,1X,F6.4,F6.4,I5,1X,I4,1X,F5.3,1X,F5.3)

C  Effective file loading

      open(unit=1,file='table1.dat', status='old')
      write(6,*) '....Loading file: table1.dat'
      do i__=1,63
        read(1,'(A126)')ar__
        read(ar__,1)
     +  Seq(i__),n_Seq(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
     +  DEd(i__),DEm(i__),DEs(i__),Name(i__),Rgal(i__),F_OII_(i__),
     +  e_F_OII_(i__),F_NeIII_(i__),e_F_NeIII_(i__),F_OIII_1(i__),
     +  e_F_OIII_1(i__),F_OIII_2(i__),e_F_OIII_2(i__),F_OIII_3(i__),
     +  e_F_OIII_3(i__),Te__OIII_(i__),e_Te__OIII_(i__),eps_O(i__),
     +  e_eps_O(i__)
c       Derive coordinates RA_ and Dec from input data
c       (RA_ and Dec are set to rNULL_ when unknown)
        RA_(i__) = RAh(i__)
        if(RAh(i__) .GE. 0) RA_(i__)=RAh(i__)*15.
        if(RAm(i__) .GE. 0) RA_(i__)=RA_(i__)+RAm(i__)/4.
        if(RAs(i__) .GE. 0) RA_(i__)=RA_(i__)+RAs(i__)/240.
        Dec(i__) = DEd(i__)
        if(DEm(i__) .GE. 0) Dec(i__)=Dec(i__)+DEm(i__)/60.
        if(DEs(i__) .GE. 0) Dec(i__)=Dec(i__)+DEs(i__)/3600.
        if(DE_(i__).EQ.'-'.AND.Dec(i__).GE.0) Dec(i__)=-Dec(i__)
c    ..............Just test output...........
        write(6,1)
     +  Seq(i__),n_Seq(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
     +  DEd(i__),DEm(i__),DEs(i__),Name(i__),Rgal(i__),F_OII_(i__),
     +  e_F_OII_(i__),F_NeIII_(i__),e_F_NeIII_(i__),F_OIII_1(i__),
     +  e_F_OIII_1(i__),F_OIII_2(i__),e_F_OIII_2(i__),F_OIII_3(i__),
     +  e_F_OIII_3(i__),Te__OIII_(i__),e_Te__OIII_(i__),eps_O(i__),
     +  e_eps_O(i__)
        write(6,'(6H Pos: 2F8.4)') RA_(i__),Dec(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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

C  Loading file 'table2.dat'	! Balmer series line ratios and derived properties

C  Format for file interpretation

    2 format(
     +  I2,1X,A1,1X,F7.2,1X,F6.2,1X,F5.3,1X,F5.3,1X,F5.2,1X,F5.2,1X,
     +  F6.4,1X,F6.4,1X,F7.4,1X,F8.5,1X,F5.3,1X,F5.3,1X,F5.3,1X,F6.4)

C  Effective file loading

      open(unit=1,file='table2.dat', status='old')
      write(6,*) '....Loading file: table2.dat'
      do i__=1,63
        read(1,'(A99)')ar__1
        read(ar__1,2)
     +  Seq_1(i__),f_EWHb(i__),EWHb(i__),e_EWHb(i__),cHb(i__),
     +  e_cHb(i__),EW_(i__),e_EW_(i__),OHg(i__),OHd(i__),OH7(i__),
     +  OH9(i__),Hgc(i__),Hdc(i__),H7c(i__),H9c(i__)
        if(ar__1(6:12) .EQ. '') EWHb(i__) = rNULL__
        if(ar__1(14:19) .EQ. '') e_EWHb(i__) = rNULL__
c    ..............Just test output...........
        write(6,2)
     +  Seq_1(i__),f_EWHb(i__),EWHb(i__),e_EWHb(i__),cHb(i__),
     +  e_cHb(i__),EW_(i__),e_EW_(i__),OHg(i__),OHd(i__),OH7(i__),
     +  OH9(i__),Hgc(i__),Hdc(i__),H7c(i__),H9c(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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