FORTRAN Generation
(/./ftp/cats/J/AJ/137/3869)

Conversion of standardized ReadMe file for file /./ftp/cats/J/AJ/137/3869 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-29
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/AJ/137/3869       Radio SNRs in 4 irregular galaxies      (Chomiuk+, 2009)
*================================================================================
*A search for radio supernova remnants in four irregular galaxies.
*    Chomiuk L., Wilcots E.M.
*   <Astron. J., 137, 3869-3883 (2009)>
*   =2009AJ....137.3869C
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'table4.dat'	! 20cm sources in NGC 1569

      integer*4 nr__
      parameter (nr__=46)	! Number of records
      character*106 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*8   v_CW2009_  (nr__) ! Source name, N1569-NN, N4214-NN, N2366-NN,
*                                   or N4449-NN
      character*1   n__CW2009_ (nr__) ! [*] Variable source (1)
      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        amaj       (nr__) ! (arcsec) Major axis
      real*4        amin       (nr__) ! (arcsec) Minor axis
      real*4        S20cm      (nr__) ! (mJy) Flux density at 20cm (1.5GHz)
      real*4        e_S20cm    (nr__) ! (mJy) rms uncertainty on S20cm
      character*1   l_S6cm     (nr__) ! Limit flag on S6cm (5GHz)
      real*4        S6cm       (nr__) ! (mJy) Flux density at 6cm
      real*4        e_S6cm     (nr__) ! (mJy) ? rms uncertainty on S6cm
      character*1   l_S3_6cm   (nr__) ! Limit flag on S3.6cm (8.3GHz)
      real*4        S3_6cm     (nr__) ! (mJy) ?=- Flux density at 3.6cm
      real*4        e_S3_6cm   (nr__) ! (mJy) ? rms uncertainty on S3.6cm
      character*1   l_alpha    (nr__) ! Limit flag on alpha
      real*4        alpha      (nr__) ! Spectral index {alpha} [S{prop.to}nu^{alpha}^]
      real*4        e_alpha    (nr__) ! ? rms uncertainty on alpha
      character*3   Ha         (nr__) ! [Yes/No ] H{alpha} emission?
      character*11  Class      (nr__) ! Classification (2)
      character*1   n_Class    (nr__) ! [ab] Note (1)
*Note (1): Notes as follows:
*   * = The flux of this source is time variable and, therefore, given
*       the different epochs of the flux measurements, the spectral
*       index is not trustworthy.
*   a = This source is actually likely an SNR based on [FeII] and Pabeta
*       emission in Labrie & Pritchet (2006ApJS..166..188L).
*   b = Additional data in the literature lend credence to this
*       characterization; see Section 6.
*Note (2): Classification as follows:
*   Bkg = no apparent H{alpha} emission associated with it
*   Bkg (>R_25) = no apparent H{alpha} emission associated with it,
*    source located beyond the galaxy's optical diameter
*   SNR = has {alpha}<=-0.2 and H{alpha} emission associated with it
*   H II = has {alpha}>-0.2 and H{alpha} emission associated with it

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

C  Declarations for 'table5.dat'	! 20cm sources in NGC 4214

      integer*4 nr__1
      parameter (nr__1=29)	! Number of records
      character*106 ar__1  	! Full-size record

C  J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
      real*8        RAdeg_1    (nr__1) ! (deg) Right Ascension J2000
      real*8        DEdeg_1    (nr__1) ! (deg)     Declination J2000
C  ---------------------------------- ! (position vector(s) in degrees)

      character*8   v_CW2009__1(nr__1) ! Source name, N1569-NN, N4214-NN, N2366-NN,
*                                   or N4449-NN
      character*1   n__CW2009__1(nr__1) ! [*] Variable source (1)
      integer*4     RAh_1      (nr__1) ! (h) Right ascension (J2000)
      integer*4     RAm_1      (nr__1) ! (min) Right ascension (J2000)
      real*4        RAs_1      (nr__1) ! (s) Right ascension (J2000)
      character*1   DE__1      (nr__1) ! Declination sign (J2000)
      integer*4     DEd_1      (nr__1) ! (deg) Declination (J2000)
      integer*4     DEm_1      (nr__1) ! (arcmin) Declination (J2000)
      real*4        DEs_1      (nr__1) ! (arcsec) Declination (J2000)
      real*4        amaj_1     (nr__1) ! (arcsec) Major axis
      real*4        amin_1     (nr__1) ! (arcsec) Minor axis
      real*4        S20cm_1    (nr__1) ! (mJy) Flux density at 20cm (1.5GHz)
      real*4        e_S20cm_1  (nr__1) ! (mJy) rms uncertainty on S20cm
      character*1   l_S6cm_1   (nr__1) ! Limit flag on S6cm (5GHz)
      real*4        S6cm_1     (nr__1) ! (mJy) Flux density at 6cm
      real*4        e_S6cm_1   (nr__1) ! (mJy) ? rms uncertainty on S6cm
      character*1   l_S3_6cm_1 (nr__1) ! Limit flag on S3.6cm (8.3GHz)
      real*4        S3_6cm_1   (nr__1) ! (mJy) ?=- Flux density at 3.6cm
      real*4        e_S3_6cm_1 (nr__1) ! (mJy) ? rms uncertainty on S3.6cm
      character*1   l_alpha_1  (nr__1) ! Limit flag on alpha
      real*4        alpha_1    (nr__1) ! Spectral index {alpha} [S{prop.to}nu^{alpha}^]
      real*4        e_alpha_1  (nr__1) ! ? rms uncertainty on alpha
      character*3   Ha_1       (nr__1) ! [Yes/No ] H{alpha} emission?
      character*11  Class_1    (nr__1) ! Classification (2)
      character*1   n_Class_1  (nr__1) ! [ab] Note (1)
*Note (1): Notes as follows:
*   * = The flux of this source is time variable and, therefore, given
*       the different epochs of the flux measurements, the spectral
*       index is not trustworthy.
*   a = This source is actually likely an SNR based on [FeII] and Pabeta
*       emission in Labrie & Pritchet (2006ApJS..166..188L).
*   b = Additional data in the literature lend credence to this
*       characterization; see Section 6.
*Note (2): Classification as follows:
*   Bkg = no apparent H{alpha} emission associated with it
*   Bkg (>R_25) = no apparent H{alpha} emission associated with it,
*    source located beyond the galaxy's optical diameter
*   SNR = has {alpha}<=-0.2 and H{alpha} emission associated with it
*   H II = has {alpha}>-0.2 and H{alpha} emission associated with it

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

C  Declarations for 'table6.dat'	! 20cm sources in NGC 2366

      integer*4 nr__2
      parameter (nr__2=24)	! Number of records
      character*106 ar__2  	! Full-size record

C  J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
      real*8        RAdeg_2    (nr__2) ! (deg) Right Ascension J2000
      real*8        DEdeg_2    (nr__2) ! (deg)     Declination J2000
C  ---------------------------------- ! (position vector(s) in degrees)

      character*8   v_CW2009__2(nr__2) ! Source name, N1569-NN, N4214-NN, N2366-NN,
*                                   or N4449-NN
      character*1   n__CW2009__2(nr__2) ! [*] Variable source (1)
      integer*4     RAh_2      (nr__2) ! (h) Right ascension (J2000)
      integer*4     RAm_2      (nr__2) ! (min) Right ascension (J2000)
      real*4        RAs_2      (nr__2) ! (s) Right ascension (J2000)
      character*1   DE__2      (nr__2) ! Declination sign (J2000)
      integer*4     DEd_2      (nr__2) ! (deg) Declination (J2000)
      integer*4     DEm_2      (nr__2) ! (arcmin) Declination (J2000)
      real*4        DEs_2      (nr__2) ! (arcsec) Declination (J2000)
      real*4        amaj_2     (nr__2) ! (arcsec) Major axis
      real*4        amin_2     (nr__2) ! (arcsec) Minor axis
      real*4        S20cm_2    (nr__2) ! (mJy) Flux density at 20cm (1.5GHz)
      real*4        e_S20cm_2  (nr__2) ! (mJy) rms uncertainty on S20cm
      character*1   l_S6cm_2   (nr__2) ! Limit flag on S6cm (5GHz)
      real*4        S6cm_2     (nr__2) ! (mJy) Flux density at 6cm
      real*4        e_S6cm_2   (nr__2) ! (mJy) ? rms uncertainty on S6cm
      character*1   l_S3_6cm_2 (nr__2) ! Limit flag on S3.6cm (8.3GHz)
      real*4        S3_6cm_2   (nr__2) ! (mJy) ?=- Flux density at 3.6cm
      real*4        e_S3_6cm_2 (nr__2) ! (mJy) ? rms uncertainty on S3.6cm
      character*1   l_alpha_2  (nr__2) ! Limit flag on alpha
      real*4        alpha_2    (nr__2) ! Spectral index {alpha} [S{prop.to}nu^{alpha}^]
      real*4        e_alpha_2  (nr__2) ! ? rms uncertainty on alpha
      character*3   Ha_2       (nr__2) ! [Yes/No ] H{alpha} emission?
      character*11  Class_2    (nr__2) ! Classification (2)
      character*1   n_Class_2  (nr__2) ! [ab] Note (1)
*Note (1): Notes as follows:
*   * = The flux of this source is time variable and, therefore, given
*       the different epochs of the flux measurements, the spectral
*       index is not trustworthy.
*   a = This source is actually likely an SNR based on [FeII] and Pabeta
*       emission in Labrie & Pritchet (2006ApJS..166..188L).
*   b = Additional data in the literature lend credence to this
*       characterization; see Section 6.
*Note (2): Classification as follows:
*   Bkg = no apparent H{alpha} emission associated with it
*   Bkg (>R_25) = no apparent H{alpha} emission associated with it,
*    source located beyond the galaxy's optical diameter
*   SNR = has {alpha}<=-0.2 and H{alpha} emission associated with it
*   H II = has {alpha}>-0.2 and H{alpha} emission associated with it

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

C  Declarations for 'table7.dat'	! 20cm sources in NGC 4449

      integer*4 nr__3
      parameter (nr__3=30)	! Number of records
      character*106 ar__3  	! Full-size record

C  J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
      real*8        RAdeg_3    (nr__3) ! (deg) Right Ascension J2000
      real*8        DEdeg_3    (nr__3) ! (deg)     Declination J2000
C  ---------------------------------- ! (position vector(s) in degrees)

      character*8   v_CW2009__3(nr__3) ! Source name, N1569-NN, N4214-NN, N2366-NN,
*                                   or N4449-NN
      character*1   n__CW2009__3(nr__3) ! [*] Variable source (1)
      integer*4     RAh_3      (nr__3) ! (h) Right ascension (J2000)
      integer*4     RAm_3      (nr__3) ! (min) Right ascension (J2000)
      real*4        RAs_3      (nr__3) ! (s) Right ascension (J2000)
      character*1   DE__3      (nr__3) ! Declination sign (J2000)
      integer*4     DEd_3      (nr__3) ! (deg) Declination (J2000)
      integer*4     DEm_3      (nr__3) ! (arcmin) Declination (J2000)
      real*4        DEs_3      (nr__3) ! (arcsec) Declination (J2000)
      real*4        amaj_3     (nr__3) ! (arcsec) Major axis
      real*4        amin_3     (nr__3) ! (arcsec) Minor axis
      real*4        S20cm_3    (nr__3) ! (mJy) Flux density at 20cm (1.5GHz)
      real*4        e_S20cm_3  (nr__3) ! (mJy) rms uncertainty on S20cm
      character*1   l_S6cm_3   (nr__3) ! Limit flag on S6cm (5GHz)
      real*4        S6cm_3     (nr__3) ! (mJy) Flux density at 6cm
      real*4        e_S6cm_3   (nr__3) ! (mJy) ? rms uncertainty on S6cm
      character*1   l_S3_6cm_3 (nr__3) ! Limit flag on S3.6cm (8.3GHz)
      real*4        S3_6cm_3   (nr__3) ! (mJy) ?=- Flux density at 3.6cm
      real*4        e_S3_6cm_3 (nr__3) ! (mJy) ? rms uncertainty on S3.6cm
      character*1   l_alpha_3  (nr__3) ! Limit flag on alpha
      real*4        alpha_3    (nr__3) ! Spectral index {alpha} [S{prop.to}nu^{alpha}^]
      real*4        e_alpha_3  (nr__3) ! ? rms uncertainty on alpha
      character*3   Ha_3       (nr__3) ! [Yes/No ] H{alpha} emission?
      character*11  Class_3    (nr__3) ! Classification (2)
      character*1   n_Class_3  (nr__3) ! [ab] Note (1)
*Note (1): Notes as follows:
*   * = The flux of this source is time variable and, therefore, given
*       the different epochs of the flux measurements, the spectral
*       index is not trustworthy.
*   a = This source is actually likely an SNR based on [FeII] and Pabeta
*       emission in Labrie & Pritchet (2006ApJS..166..188L).
*   b = Additional data in the literature lend credence to this
*       characterization; see Section 6.
*Note (2): Classification as follows:
*   Bkg = no apparent H{alpha} emission associated with it
*   Bkg (>R_25) = no apparent H{alpha} emission associated with it,
*    source located beyond the galaxy's optical diameter
*   SNR = has {alpha}<=-0.2 and H{alpha} emission associated with it
*   H II = has {alpha}>-0.2 and H{alpha} emission associated with it

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

C  Loading file 'table4.dat'	! 20cm sources in NGC 1569

C  Format for file interpretation

    1 format(
     +  A8,A1,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F4.1,1X,
     +  F4.1,1X,F5.2,1X,F4.2,1X,A1,F4.2,1X,F4.2,1X,A1,F4.2,1X,F5.3,1X,
     +  A1,F5.2,1X,F4.2,1X,A3,1X,A11,A1)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table4.dat')
      write(6,*) '....Loading file: table4.dat'
      do i__=1,46
        read(1,'(A106)')ar__
        read(ar__,1)
     +  v_CW2009_(i__),n__CW2009_(i__),RAh(i__),RAm(i__),RAs(i__),
     +  DE_(i__),DEd(i__),DEm(i__),DEs(i__),amaj(i__),amin(i__),
     +  S20cm(i__),e_S20cm(i__),l_S6cm(i__),S6cm(i__),e_S6cm(i__),
     +  l_S3_6cm(i__),S3_6cm(i__),e_S3_6cm(i__),l_alpha(i__),
     +  alpha(i__),e_alpha(i__),Ha(i__),Class(i__),n_Class(i__)
        if(ar__(62:65) .EQ. '') e_S6cm(i__) = rNULL__
        if (idig(ar__(68:71)).EQ.0) S3_6cm(i__) =  rNULL__
        if(ar__(73:77) .EQ. '') e_S3_6cm(i__) = rNULL__
        if(ar__(86:89) .EQ. '') e_alpha(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)
     +  v_CW2009_(i__),n__CW2009_(i__),RAh(i__),RAm(i__),RAs(i__),
     +  DE_(i__),DEd(i__),DEm(i__),DEs(i__),amaj(i__),amin(i__),
     +  S20cm(i__),e_S20cm(i__),l_S6cm(i__),S6cm(i__),e_S6cm(i__),
     +  l_S3_6cm(i__),S3_6cm(i__),e_S3_6cm(i__),l_alpha(i__),
     +  alpha(i__),e_alpha(i__),Ha(i__),Class(i__),n_Class(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 'table5.dat'	! 20cm sources in NGC 4214

C  Format for file interpretation

    2 format(
     +  A8,A1,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F4.1,1X,
     +  F4.1,1X,F5.2,1X,F4.2,1X,A1,F4.2,1X,F4.2,1X,A1,F4.2,1X,F5.3,1X,
     +  A1,F5.2,1X,F4.2,1X,A3,1X,A11,A1)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table5.dat')
      write(6,*) '....Loading file: table5.dat'
      do i__=1,29
        read(1,'(A106)')ar__1
        read(ar__1,2)
     +  v_CW2009__1(i__),n__CW2009__1(i__),RAh_1(i__),RAm_1(i__),
     +  RAs_1(i__),DE__1(i__),DEd_1(i__),DEm_1(i__),DEs_1(i__),
     +  amaj_1(i__),amin_1(i__),S20cm_1(i__),e_S20cm_1(i__),
     +  l_S6cm_1(i__),S6cm_1(i__),e_S6cm_1(i__),l_S3_6cm_1(i__),
     +  S3_6cm_1(i__),e_S3_6cm_1(i__),l_alpha_1(i__),alpha_1(i__),
     +  e_alpha_1(i__),Ha_1(i__),Class_1(i__),n_Class_1(i__)
        if(ar__1(62:65) .EQ. '') e_S6cm_1(i__) = rNULL__
        if (idig(ar__1(68:71)).EQ.0) S3_6cm_1(i__) =  rNULL__
        if(ar__1(73:77) .EQ. '') e_S3_6cm_1(i__) = rNULL__
        if(ar__1(86:89) .EQ. '') e_alpha_1(i__) = rNULL__
        RAdeg_1(i__) = rNULL__
        DEdeg_1(i__) = rNULL__
c  Derive coordinates RAdeg_1 and DEdeg_1 from input data
c  (RAdeg_1 and DEdeg_1 are set to rNULL__ when unknown)
        if(RAh_1(i__) .GT. -180) RAdeg_1(i__)=RAh_1(i__)*15.
        if(RAm_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAm_1(i__)/4.
        if(RAs_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAs_1(i__)/240.
        if(DEd_1(i__) .GE. 0) DEdeg_1(i__)=DEd_1(i__)
        if(DEm_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEm_1(i__)/60.
        if(DEs_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEs_1(i__)/3600.
        if(DE__1(i__).EQ.'-'.AND.DEdeg_1(i__).GE.0) DEdeg_1(i__)=-DEdeg_1(i__)
c    ..............Just test output...........
        write(6,2)
     +  v_CW2009__1(i__),n__CW2009__1(i__),RAh_1(i__),RAm_1(i__),
     +  RAs_1(i__),DE__1(i__),DEd_1(i__),DEm_1(i__),DEs_1(i__),
     +  amaj_1(i__),amin_1(i__),S20cm_1(i__),e_S20cm_1(i__),
     +  l_S6cm_1(i__),S6cm_1(i__),e_S6cm_1(i__),l_S3_6cm_1(i__),
     +  S3_6cm_1(i__),e_S3_6cm_1(i__),l_alpha_1(i__),alpha_1(i__),
     +  e_alpha_1(i__),Ha_1(i__),Class_1(i__),n_Class_1(i__)
        write(6,'(6H Pos: 2F8.4)') RAdeg_1(i__),DEdeg_1(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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

C  Loading file 'table6.dat'	! 20cm sources in NGC 2366

C  Format for file interpretation

    3 format(
     +  A8,A1,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F4.1,1X,
     +  F4.1,1X,F5.2,1X,F4.2,1X,A1,F4.2,1X,F4.2,1X,A1,F4.2,1X,F5.3,1X,
     +  A1,F5.2,1X,F4.2,1X,A3,1X,A11,A1)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table6.dat')
      write(6,*) '....Loading file: table6.dat'
      do i__=1,24
        read(1,'(A106)')ar__2
        read(ar__2,3)
     +  v_CW2009__2(i__),n__CW2009__2(i__),RAh_2(i__),RAm_2(i__),
     +  RAs_2(i__),DE__2(i__),DEd_2(i__),DEm_2(i__),DEs_2(i__),
     +  amaj_2(i__),amin_2(i__),S20cm_2(i__),e_S20cm_2(i__),
     +  l_S6cm_2(i__),S6cm_2(i__),e_S6cm_2(i__),l_S3_6cm_2(i__),
     +  S3_6cm_2(i__),e_S3_6cm_2(i__),l_alpha_2(i__),alpha_2(i__),
     +  e_alpha_2(i__),Ha_2(i__),Class_2(i__),n_Class_2(i__)
        if(ar__2(62:65) .EQ. '') e_S6cm_2(i__) = rNULL__
        if (idig(ar__2(68:71)).EQ.0) S3_6cm_2(i__) =  rNULL__
        if(ar__2(73:77) .EQ. '') e_S3_6cm_2(i__) = rNULL__
        if(ar__2(86:89) .EQ. '') e_alpha_2(i__) = rNULL__
        RAdeg_2(i__) = rNULL__
        DEdeg_2(i__) = rNULL__
c  Derive coordinates RAdeg_2 and DEdeg_2 from input data
c  (RAdeg_2 and DEdeg_2 are set to rNULL__ when unknown)
        if(RAh_2(i__) .GT. -180) RAdeg_2(i__)=RAh_2(i__)*15.
        if(RAm_2(i__) .GT. -180) RAdeg_2(i__)=RAdeg_2(i__)+RAm_2(i__)/4.
        if(RAs_2(i__) .GT. -180) RAdeg_2(i__)=RAdeg_2(i__)+RAs_2(i__)/240.
        if(DEd_2(i__) .GE. 0) DEdeg_2(i__)=DEd_2(i__)
        if(DEm_2(i__) .GE. 0) DEdeg_2(i__)=DEdeg_2(i__)+DEm_2(i__)/60.
        if(DEs_2(i__) .GE. 0) DEdeg_2(i__)=DEdeg_2(i__)+DEs_2(i__)/3600.
        if(DE__2(i__).EQ.'-'.AND.DEdeg_2(i__).GE.0) DEdeg_2(i__)=-DEdeg_2(i__)
c    ..............Just test output...........
        write(6,3)
     +  v_CW2009__2(i__),n__CW2009__2(i__),RAh_2(i__),RAm_2(i__),
     +  RAs_2(i__),DE__2(i__),DEd_2(i__),DEm_2(i__),DEs_2(i__),
     +  amaj_2(i__),amin_2(i__),S20cm_2(i__),e_S20cm_2(i__),
     +  l_S6cm_2(i__),S6cm_2(i__),e_S6cm_2(i__),l_S3_6cm_2(i__),
     +  S3_6cm_2(i__),e_S3_6cm_2(i__),l_alpha_2(i__),alpha_2(i__),
     +  e_alpha_2(i__),Ha_2(i__),Class_2(i__),n_Class_2(i__)
        write(6,'(6H Pos: 2F8.4)') RAdeg_2(i__),DEdeg_2(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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

C  Loading file 'table7.dat'	! 20cm sources in NGC 4449

C  Format for file interpretation

    4 format(
     +  A8,A1,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F4.1,1X,
     +  F4.1,1X,F5.2,1X,F4.2,1X,A1,F4.2,1X,F4.2,1X,A1,F4.2,1X,F5.3,1X,
     +  A1,F5.2,1X,F4.2,1X,A3,1X,A11,A1)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table7.dat')
      write(6,*) '....Loading file: table7.dat'
      do i__=1,30
        read(1,'(A106)')ar__3
        read(ar__3,4)
     +  v_CW2009__3(i__),n__CW2009__3(i__),RAh_3(i__),RAm_3(i__),
     +  RAs_3(i__),DE__3(i__),DEd_3(i__),DEm_3(i__),DEs_3(i__),
     +  amaj_3(i__),amin_3(i__),S20cm_3(i__),e_S20cm_3(i__),
     +  l_S6cm_3(i__),S6cm_3(i__),e_S6cm_3(i__),l_S3_6cm_3(i__),
     +  S3_6cm_3(i__),e_S3_6cm_3(i__),l_alpha_3(i__),alpha_3(i__),
     +  e_alpha_3(i__),Ha_3(i__),Class_3(i__),n_Class_3(i__)
        if(ar__3(62:65) .EQ. '') e_S6cm_3(i__) = rNULL__
        if (idig(ar__3(68:71)).EQ.0) S3_6cm_3(i__) =  rNULL__
        if(ar__3(73:77) .EQ. '') e_S3_6cm_3(i__) = rNULL__
        if(ar__3(86:89) .EQ. '') e_alpha_3(i__) = rNULL__
        RAdeg_3(i__) = rNULL__
        DEdeg_3(i__) = rNULL__
c  Derive coordinates RAdeg_3 and DEdeg_3 from input data
c  (RAdeg_3 and DEdeg_3 are set to rNULL__ when unknown)
        if(RAh_3(i__) .GT. -180) RAdeg_3(i__)=RAh_3(i__)*15.
        if(RAm_3(i__) .GT. -180) RAdeg_3(i__)=RAdeg_3(i__)+RAm_3(i__)/4.
        if(RAs_3(i__) .GT. -180) RAdeg_3(i__)=RAdeg_3(i__)+RAs_3(i__)/240.
        if(DEd_3(i__) .GE. 0) DEdeg_3(i__)=DEd_3(i__)
        if(DEm_3(i__) .GE. 0) DEdeg_3(i__)=DEdeg_3(i__)+DEm_3(i__)/60.
        if(DEs_3(i__) .GE. 0) DEdeg_3(i__)=DEdeg_3(i__)+DEs_3(i__)/3600.
        if(DE__3(i__).EQ.'-'.AND.DEdeg_3(i__).GE.0) DEdeg_3(i__)=-DEdeg_3(i__)
c    ..............Just test output...........
        write(6,4)
     +  v_CW2009__3(i__),n__CW2009__3(i__),RAh_3(i__),RAm_3(i__),
     +  RAs_3(i__),DE__3(i__),DEd_3(i__),DEm_3(i__),DEs_3(i__),
     +  amaj_3(i__),amin_3(i__),S20cm_3(i__),e_S20cm_3(i__),
     +  l_S6cm_3(i__),S6cm_3(i__),e_S6cm_3(i__),l_S3_6cm_3(i__),
     +  S3_6cm_3(i__),e_S3_6cm_3(i__),l_alpha_3(i__),alpha_3(i__),
     +  e_alpha_3(i__),Ha_3(i__),Class_3(i__),n_Class_3(i__)
        write(6,'(6H Pos: 2F8.4)') RAdeg_3(i__),DEdeg_3(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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

C Locate position of first digit in string; or return 0
      integer function idig(c)
      character*(*) c
      character*1 c1
      integer lc,i
      lc=len(c)
      idig=0
      do i=1,lc
         if(c(i:i).ne.' ') go to 1
      end do
    1 if(i.gt.lc) return
      c1=c(i:i)
      if(c1.eq.'.'.or.c1.eq.'-'.or.c1.eq.'+') i=i+1
      if(i.gt.lc) return
      c1=c(i:i)
      if(c1.ge.'0'.and.c1.le.'9') idig=i
      return
      end