FORTRAN Generation
(/./ftp/cats/J/A_A/532/A127)

Conversion of standardized ReadMe file for file /./ftp/cats/J/A_A/532/A127 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-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/A+A/532/A127      Inner Galaxy HII regions                 (Du+, 2011)
*================================================================================
*A H_2_CO and H110{alpha} survey of HII regions with the 25-m radio telescope of
*Nanshan Station.
*    Du Z.M., Zhou J.J., Esimbek J., Han X.H., Zhang C.P.
*   <Astron. Astrophys. 532, A127 (2011)>
*   =2011A&A...532A.127D
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'table1.dat'	! Observed sources

      integer*4 nr__
      parameter (nr__=64)	! Number of records
      character*70 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)

      character*14  Source     (nr__) ! Source name
      character*8   Name       (nr__) ! Alias name
      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        rms        (nr__) ! The rms of the spectral lines (1)
      real*4        S100um     (nr__) ! (kJy) ? Flux density at 100{mu}m
      real*4        S6cm       (nr__) ! (Jy) ? Flux density at 6cm (2)
      character*3   Note       (nr__) ! Reference (3)
*Note (1): The rms of the spectral lines were obtained during our observation.
*Note (2): The measurement results of the continuum flux densities at 6cm.
*Note (3): References as follows:
*   c = data reported by Araya et al. (2004ApJS..154..579A)
*   d = data reported by Downes et al. (1980A&AS...40..379D)
*   e = data reported by Wilson (1972A&A....19..354W)
*   f = data reported by Whiteoak & Gardner (1974A&A....37..389W)

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

C  Declarations for 'table2.dat'	! H110{alpha} line parameters of sources

      integer*4 nr__1
      parameter (nr__1=28)	! Number of records
      character*66 ar__1  	! Full-size record

      character*14  Source_1   (nr__1) ! Source name
      character*1   f_Source   (nr__1) ! [*] Changes (1)
      real*8        VLSR       (nr__1) ! (km/s) ? Local Standard of Rest Velocity
      real*4        e_VLSR     (nr__1) ! (km/s) ? The 1{sigma} error in VLSR
      real*4        FWHM       (nr__1) ! (km/s) ? Full-Width at Half-Maximum
      real*4        e_FWHM     (nr__1) ! (km/s) ? The 1{sigma} error in FWHM
      real*4        SH110a     (nr__1) ! (Jy) ? The H110{alpha} flux density at 4874.1570MHz
      real*4        e_SH110a   (nr__1) ! (Jy) ? The 1{sigma} error in SH110a
      real*8        Sint       (nr__1) ! (Jy.km/s) ? Integrated flux density at 4874.1570MHz
      real*4        e_Sint     (nr__1) ! (Jy.km/s) ? The 1{sigma} error in Sint
*Note (1):
*  * G15.032-0.687 corrected into G15.032-0.68, as in table1.
*  * G15.181-0.63  corrected into G15.181-0.62, as in table1.
*  * G81.253+1.123 corrected into G81.253+1.12, as in table1.

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

C  Declarations for 'table3.dat'	! H_2_CO line parameters

      integer*4 nr__2
      parameter (nr__2=83)	! Number of records
      character*74 ar__2  	! Full-size record

      character*14  Source_2   (nr__2) ! Source name
      integer*4     MC         (nr__2) ! [1/4]? H_2_CO molecular cloud number
*                                  within the source (G1)
      character*1   f_Source_1 (nr__2) ! [*] Changes (1)
      real*8        VLSR_1     (nr__2) ! (km/s) ? Local Standard of Rest Velocity
      real*4        e_VLSR_1   (nr__2) ! (km/s) ? The 1{sigma} error in VLSR
      real*4        FWHM_1     (nr__2) ! (km/s) ? Full-Width at Half-Maximum
      real*4        e_FWHM_1   (nr__2) ! (km/s) ? The 1{sigma} error in FWHM
      real*8        SH2CO      (nr__2) ! (Jy) ? The H_2_CO flux density at 4829.6594MHz
      real*4        e_SH2CO    (nr__2) ! (Jy) ? The 1{sigma} error in SH2CO
      real*8        Sint_1     (nr__2) ! (Jy.km/s) ? Integrated flux density at 4829.6594MHz
      real*4        e_Sint_1   (nr__2) ! (Jy.km/s) ? The 1{sigma} error in Sint
*Note (1): G15.181-0.63  corrected into G15.181-0.62, as in table1.

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

C  Declarations for 'table4.dat'	! Kinematic parameters

      integer*4 nr__3
      parameter (nr__3=45)	! Number of records
      character*83 ar__3  	! Full-size record

      character*14  Source_3   (nr__3) ! Source name
      integer*4     MC_1       (nr__3) ! [1/4]? H_2_CO molecular cloud number
*                              within the source (G1)
      character*1   f_Source_2 (nr__3) ! Changes (1)
      real*4        VLSR_2     (nr__3) ! (km/s) Local Standard of Rest Velocity
      real*4        VTP        (nr__3) ! (km/s) ? Tangent point velocity
      real*4        DTP        (nr__3) ! (kpc) ? Tangent point distance
      real*4        Dfar       (nr__3) ! (kpc) ? Far source distance
      real*4        Dnear      (nr__3) ! (kpc) ? Near source distance
      real*4        DLSR       (nr__3) ! (kpc) ? Adopted kinematic source distance
      real*4        E_DLSR     (nr__3) ! (kpc) ? Upper limit in DLSR
      real*4        e_DLSR_1   (nr__3) ! (kpc) ? Lower limit in DLSR
      real*4        Z          (nr__3) ! (pc) ? Galactic plane distance
      real*4        RGC        (nr__3) ! (kpc) ? Galactic center distance
      character*6   Code       (nr__3) ! The Near/Far code (2)
*Note (1):
*  * G15.181-0.63  corrected into G15.181-0.62, as in table1.
*  * IRAS18507+0101 was a misprint for IRAS18507+0110, corrected name
*    in the CDS table.
*Note (2): The Near/Far code is defined as follows:
*   N = a source at the near kinematic distance
*   F = a source at the far distance
*   S = a molecular cloud associated with an HII region
*  NS = a molecular cloud associated with an UC HII region
*  FS = a molecular cloud associated with an UC HII region
*   b = No classification or distance is given for this source
*   c = this source is located at the tangent point
*   d = the distance ambiguity cannot be resolved
*   e = this source is located in the outer Galaxy
*   f = Downes et al. (1980A&AS...40..379D) have reported this source' s
*       kinematic distance.

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

C  Loading file 'table1.dat'	! Observed sources

C  Format for file interpretation

    1 format(
     +  A14,1X,A8,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F5.3,
     +  1X,F5.2,1X,F6.2,1X,A3)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table1.dat')
      write(6,*) '....Loading file: table1.dat'
      do i__=1,64
        read(1,'(A70)')ar__
        read(ar__,1)
     +  Source(i__),Name(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
     +  DEd(i__),DEm(i__),DEs(i__),rms(i__),S100um(i__),S6cm(i__),
     +  Note(i__)
        if(ar__(55:59) .EQ. '') S100um(i__) = rNULL__
        if(ar__(61:66) .EQ. '') S6cm(i__) = rNULL__
        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)
     +  Source(i__),Name(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
     +  DEd(i__),DEm(i__),DEs(i__),rms(i__),S100um(i__),S6cm(i__),
     +  Note(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'	! H110{alpha} line parameters of sources

C  Format for file interpretation

    2 format(
     +  A14,A1,F7.3,1X,F5.3,1X,F5.2,1X,F5.3,1X,F5.3,1X,F5.3,1X,F7.3,
     +  1X,F5.3)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table2.dat')
      write(6,*) '....Loading file: table2.dat'
      do i__=1,28
        read(1,'(A66)')ar__1
        read(ar__1,2)
     +  Source_1(i__),f_Source(i__),VLSR(i__),e_VLSR(i__),FWHM(i__),
     +  e_FWHM(i__),SH110a(i__),e_SH110a(i__),Sint(i__),e_Sint(i__)
        if(ar__1(16:22) .EQ. '') VLSR(i__) = rNULL__
        if(ar__1(24:28) .EQ. '') e_VLSR(i__) = rNULL__
        if(ar__1(30:34) .EQ. '') FWHM(i__) = rNULL__
        if(ar__1(36:40) .EQ. '') e_FWHM(i__) = rNULL__
        if(ar__1(42:46) .EQ. '') SH110a(i__) = rNULL__
        if(ar__1(48:52) .EQ. '') e_SH110a(i__) = rNULL__
        if(ar__1(54:60) .EQ. '') Sint(i__) = rNULL__
        if(ar__1(62:66) .EQ. '') e_Sint(i__) = rNULL__
c    ..............Just test output...........
        write(6,2)
     +  Source_1(i__),f_Source(i__),VLSR(i__),e_VLSR(i__),FWHM(i__),
     +  e_FWHM(i__),SH110a(i__),e_SH110a(i__),Sint(i__),e_Sint(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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

C  Loading file 'table3.dat'	! H_2_CO line parameters

C  Format for file interpretation

    3 format(
     +  A14,2X,I1,A1,F8.3,1X,F5.3,1X,F6.3,1X,F5.3,1X,F7.3,1X,F5.3,1X,
     +  F8.3,1X,F5.3)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table3.dat')
      write(6,*) '....Loading file: table3.dat'
      do i__=1,83
        read(1,'(A74)')ar__2
        read(ar__2,3)
     +  Source_2(i__),MC(i__),f_Source_1(i__),VLSR_1(i__),
     +  e_VLSR_1(i__),FWHM_1(i__),e_FWHM_1(i__),SH2CO(i__),
     +  e_SH2CO(i__),Sint_1(i__),e_Sint_1(i__)
        if(ar__2(17:17) .EQ. '') MC(i__) = iNULL__
        if(ar__2(19:26) .EQ. '') VLSR_1(i__) = rNULL__
        if(ar__2(28:32) .EQ. '') e_VLSR_1(i__) = rNULL__
        if(ar__2(34:39) .EQ. '') FWHM_1(i__) = rNULL__
        if(ar__2(41:45) .EQ. '') e_FWHM_1(i__) = rNULL__
        if(ar__2(47:53) .EQ. '') SH2CO(i__) = rNULL__
        if(ar__2(55:59) .EQ. '') e_SH2CO(i__) = rNULL__
        if(ar__2(61:68) .EQ. '') Sint_1(i__) = rNULL__
        if(ar__2(70:74) .EQ. '') e_Sint_1(i__) = rNULL__
c    ..............Just test output...........
        write(6,3)
     +  Source_2(i__),MC(i__),f_Source_1(i__),VLSR_1(i__),
     +  e_VLSR_1(i__),FWHM_1(i__),e_FWHM_1(i__),SH2CO(i__),
     +  e_SH2CO(i__),Sint_1(i__),e_Sint_1(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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

C  Loading file 'table4.dat'	! Kinematic parameters

C  Format for file interpretation

    4 format(
     +  A14,2X,I1,A1,F5.1,1X,F5.1,1X,F4.2,1X,F5.2,1X,F4.2,1X,F5.2,2X,
     +  F4.2,2X,F4.2,1X,F6.1,1X,F5.2,1X,A6)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table4.dat')
      write(6,*) '....Loading file: table4.dat'
      do i__=1,45
        read(1,'(A83)')ar__3
        read(ar__3,4)
     +  Source_3(i__),MC_1(i__),f_Source_2(i__),VLSR_2(i__),VTP(i__),
     +  DTP(i__),Dfar(i__),Dnear(i__),DLSR(i__),E_DLSR(i__),
     +  e_DLSR_1(i__),Z(i__),RGC(i__),Code(i__)
        if(ar__3(17:17) .EQ. '') MC_1(i__) = iNULL__
        if(ar__3(25:29) .EQ. '') VTP(i__) = rNULL__
        if(ar__3(31:34) .EQ. '') DTP(i__) = rNULL__
        if(ar__3(36:40) .EQ. '') Dfar(i__) = rNULL__
        if(ar__3(42:45) .EQ. '') Dnear(i__) = rNULL__
        if(ar__3(47:51) .EQ. '') DLSR(i__) = rNULL__
        if(ar__3(54:57) .EQ. '') E_DLSR(i__) = rNULL__
        if(ar__3(60:63) .EQ. '') e_DLSR_1(i__) = rNULL__
        if(ar__3(65:70) .EQ. '') Z(i__) = rNULL__
        if(ar__3(72:76) .EQ. '') RGC(i__) = rNULL__
c    ..............Just test output...........
        write(6,4)
     +  Source_3(i__),MC_1(i__),f_Source_2(i__),VLSR_2(i__),VTP(i__),
     +  DTP(i__),Dfar(i__),Dnear(i__),DLSR(i__),E_DLSR(i__),
     +  e_DLSR_1(i__),Z(i__),RGC(i__),Code(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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