FORTRAN Generation
(/./ftp/cats/J/A_A/702/A187)

Conversion of standardized ReadMe file for file /./ftp/cats/J/A_A/702/A187 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-Jul-13
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/702/A187      GLACE survey: The mass--SFR relation    (De Daniloff+, 2025)
*================================================================================
*GLACE survey: OSIRIS/GTC multi-object spectroscopy of the rich galaxy cluster
*ZwCl 0024.0+1652 at z~0.4.
*III. The mass-SFR relation and the quenching of cluster galaxies.
*    De Daniloff S.B., Bongiovanni A., Sanchez-Portal M., Cedres B.,
*    Padilla-Torres C.P., Perez-Garcia A.M., Perez-Martinez R., Espada D.,
*    de la Casa C.C., Torres-Rios G., Gonzalez-Otero M., de Diego J.A.,
*    Rodriguez M.I., Cervino M., Lara-Lopez M.A., Cepa J., Valtchanov I.,
*    Gonzalez-Serrano J.I., Cruz-Gonzalez I., Negrete C.A., Beyoro-Amado Z.,
*    Castillo-Fraile M., Mancillas B., Povic M.
*    <Astron. Astrophys. 702, A187 (2025)>
*    =2025A&A...702A.187D        (SIMBAD/NED BibCode)
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'catalog.dat'	! Catalog of the properties of the galaxies

      integer*4 nr__
      parameter (nr__=102)	! Number of records
      character*3288 ar__   	! Full-size record

C  J2000 position composed of: RAdeg DEdeg
      character*7   ID_unique  (nr__) ! GLACE ID with pointing label,
*                                               NNNNN_a (id_unique) (1)(2)
      integer*4     ID         (nr__) ! GLACE ID without pointing label
*                                               (ID) (1)
      character*5   ID_MOS     (nr__) ! ID of the MOS spectrum after
*                                              reduction (id_MOS)
      real*8        RAdeg      (nr__) ! (deg) Right ascension (J2000) from TF
*                                               (tunable filters) calibrated data
*                                               (RA_J2000) (1)
      real*8        DEdeg      (nr__) ! (deg) Declination (J2000) from TF
*                                               calibrated data (DEC_J2000) (1)
      real*8        RAGdeg     (nr__) ! (deg) Right ascension from GAIA-DR1
*                                               (ICRS) at Ep=2015.0 (RA_GAIA) (1)
      real*8        DEGdeg     (nr__) ! (deg) Declination from GAIA- DR1 (ICRS)
*                                               at Ep=2015.0 (DEC_GAIA) (1)
      real*8        zSP15      (nr__) ! Redshift from TF calibrated data
*                                               (Sanchez-Portal et al.,
*                                               2015A&A...578A..30S,) (z_SP15)
      real*8        zHaIC      (nr__) ! Redshift of Halpha emission line
*                                               obtained from inverse convolution
*                                               method (z_Halpha_InvConv) (3)
      real*8        b_zHaIC    (nr__) ! Lower value of redshift of Halpha
*                                               emission line
*                                               (z_Halpha_InvConv_d) (3)
      real*8        B_zHaIC_1  (nr__) ! Upper value of redshift of Halpha
*                                               emission line
*                                               (z_Halpha_InvConv_u) (3)
      real*8        zOII       (nr__) ! ? Redshift of [OII] emission
*                                               line (z_OII)
      real*8        e_zOII     (nr__) ! ? Error in redshift of [OII]
*                                              emission line (e_z_OII)
      real*8        zHb        (nr__) ! ? Redshift of Hbeta emission line
*                                               (z_Hbeta)
      real*8        e_zHb      (nr__) ! ? Error in redshift of Hbeta
*                                               emission line (e_z_Hbeta)
      real*8        zOIII      (nr__) ! ? Redshift of [OIII]5007 emission
*                                               line (z_OIII)
      real*8        e_zOIII    (nr__) ! ? Error in redshift of [OIII]5007
*                                               emission line (e_z_OIII)
      real*8        zMOSavg    (nr__) ! ? Average redshift of [OII],
*                                               Hbeta, and [OIII]5007 emission
*                                               lines (z_MOS_avg)
      real*8        e_zMOSavg  (nr__) ! ? Error in average redshift of
*                                               [OII], Hbeta, and [OIII]5007
*                                               emission lines (e_z_MOS_avg)
      character*10  Structure  (nr__) ! Kinematical structure in which
*                                               the galaxy is located
*                                               (Structure) (4)
      real*8        Bmag       (nr__) ! (mag) ? B-band (CFHT/CFH12k) AUTO
*                                               magnitude (Vega system);
*                                               automatic aperture from
*                                               SExtractor; proxy for total
*                                               magnitude (B_AUTO) (1)
      real*8        e_Bmag     (nr__) ! (mag) ? Error in B-band AUTO magnitude
*                                               (e_B_AUTO) (1)
      real*8        Vmag       (nr__) ! (mag) ? V-band (CFHT/CFH12k) AUTO
*                                               magnitude V_AUTO) (1)
      real*8        e_Vmag     (nr__) ! (mag) ? Error in V-band AUTO magnitude
*                                               (e_V_AUTO) (1)
      real*8        Rmag       (nr__) ! (mag) ? R-band (CFHT/CFH12k) AUTO
*                                               magnitude (R_AUTO) (1)
      real*8        e_Rmag     (nr__) ! (mag) ? Error in R-band AUTO magnitude
*                                               (e_R_AUTO) (1)
      real*8        Imag       (nr__) ! (mag) ? I-band (CFHT/CFH12k) AUTO
*                                               magnitude (I_AUTO) (1)
      real*8        e_Imag     (nr__) ! (mag) ? Error in I-band AUTO magnitude
*                                               (e_I_AUTO) (1)
      real*8        Jmag       (nr__) ! (mag) ? J-band (Palomar200/WIRC) AUTO
*                                               magnitude (J_AUTO) (1)
      real*8        e_Jmag     (nr__) ! (mag) ? Error in J-band AUTO magnitude
*                                               (e_J_AUTO) (1)
      real*8        Ksmag      (nr__) ! (mag) ? Ks-band (Palomar200/WIRC) AUTO
*                                               magnitude (Ks_AUTO) (1)
      real*8        e_Ksmag    (nr__) ! (mag) ? Error in Ks-band AUTO magnitude
*                                               (e_Ks_AUTO) (1)
      real*8        F814Wmag   (nr__) ! (mag) ? HST/WFPC2 814nm wide band AUTO
*                                               magnitude (F814W_AUTO) (1)
      real*8        e_F814Wmag (nr__) ! (mag) ? Error in HST/WFPC2 814nm wide
*                                               band AUTO magnitude
*                                               (e_F814W_AUTO) (1)
      real*4        FHaSP15    (nr__) ! (mW/m2) Flux of Halpha emission line
*                                               (F_Halpha_SP15) (1)
      real*4        e_FHaSP15  (nr__) ! (mW/m2) Error in flux of Halpha emission
*                                               line (e_F_Halpha_SP15) (1)
      real*4        FNIISP15   (nr__) ! (mW/m2) ? Flux of [NII]6548 emission line
*                                               (F_NII_SP15) (1)
      real*4        e_FNIISP15 (nr__) ! (mW/m2) ? Error in flux of [NII]6548
*                                               emission line (e_FNII_SP15) (1)
      real*4        FHacSP15   (nr__) ! (mW/m2) Flux of Halpha adjusted and
*                                               corrected for absorptions and
*                                               extinction
*                                               (FHalpha_corrected_SP15) (1)
      real*4        e_FHacSP15 (nr__) ! (mW/m2) Error in flux of Halpha adjusted
*                                               and corrected for absorptions and
*                                               extinction
*                                               (eFHalpha_corrected_SP15) (1)
      real*4        FNIIcSP15  (nr__) ! (mW/m2) ? Flux of [NII]6548 adjusted and
*                                               corrected for absorptions and
*                                               extinction
*                                               (FNII_corrected_SP15) (1)
      real*4        e_FNIIcSP15(nr__) ! (mW/m2) ? Error in flux of [NII]6548
*                                               adjusted and corrected for
*                                               absorptions and extinction
*                                               (eFNII_corrected_SP15) (1)
      real*8        EWHaSP15   (nr__) ! (0.1nm) Equivalent width of Halpha
*                                               emission line obtained from
*                                               tunable filters
*                                               (EW_Halpha_SP15) (1)
      real*8        e_EWHaSP15 (nr__) ! (0.1nm) Error in equivalent width of
*                                               Halpha emission line obtained
*                                               from tunable filters
*                                               (e_EW_Halpha_SP15) (1)
      real*4        ContHaIC   (nr__) ! (10mW/m2/nm) Continuum level of Halpha line
*                                               obtained from inverse convolution
*                                               (Cont_Halpha_InvConv) (3)
      real*4        b_ContHaIC (nr__) ! (10mW/m2/nm) Lower value of continuum level of
*                                               Halpha line obtained from
*                                               inverse convolution
*                                               (Cont_Halpha_InvConv_d) (3)
      real*4        B_ContHaIC_1(nr__) ! (10mW/m2/nm) Upper value of continuum level of
*                                               Halpha line obtained from
*                                               inverse convolution
*                                               (Cont_Halpha_InvConv_u) (3)
      real*8        sigmaHaIC  (nr__) ! (0.1nm) Sigma of the Gaussian fit for
*                                               Halpha line obtained from
*                                               inverse convolution
*                                               (sigma_Halpha_InvConv) (3)
      real*8        b_sigmaHaIC(nr__) ! (0.1nm) Lower value of sigma of the
*                                               Gaussian fit for Halpha line
*                                               obtained from inverse convolution
*                                               (sigma_Halpha_InvConv_d) (3)
      real*8        B_sigmaHaIC_1(nr__) ! (0.1nm) Upper value of sigma of the
*                                               Gaussian fit for Halpha line
*                                               obtained from inverse convolution
*                                               (sigma_Halpha_InvConv_u) (3)
      real*4        FNII6548IC (nr__) ! (mW/m2) Flux of [NII]6548 emission line
*                                               obtained from inverse convolution
*                                               (F_NII6548_InvConv) (3)
      real*4        b_FNII6548IC(nr__) ! (mW/m2) Lower value of flux of [NII]6548
*                                               emission line obtained from
*                                               inverse convolution
*                                               (F_NII6548_InvConv_d) (3)
      real*4        B_FNII6548IC_1(nr__) ! (mW/m2) Upper value of flux of [NII]6548
*                                               emission line obtained from
*                                               inverse convolution
*                                               (F_NII6548_InvConv_u) (3)
      real*4        FHaIC      (nr__) ! (mW/m2) Flux of Halpha emission line
*                                               obtained from inverse convolution
*                                               (F_Halpha_InvConv) (3)
      real*4        b_FHaIC    (nr__) ! (mW/m2) Lower value of flux of Halpha
*                                               obtained from inverse convolution
*                                               (F_Halpha_InvConv_d) (3)
      real*4        B_FHaIC_1  (nr__) ! (mW/m2) Upper value of flux of Halpha
*                                               obtained from inverse convolution
*                                               (F_Halpha_InvConv_u) (3)
      real*4        FNII6583IC (nr__) ! (mW/m2) Flux of [NII]6583 emission line
*                                               obtained from inverse convolution
*                                               (F_NII6583_InvConv) (3)
      real*4        b_FNII6583IC(nr__) ! (mW/m2) Lower value of flux of [NII]6583
*                                               obtained from inverse convolution
*                                               (F_NII6583_InvConv_d) (3)
      real*4        B_FNII6583IC_1(nr__) ! (mW/m2) Upper value of flux of [NII]6583
*                                               obtained from inverse convolution
*                                               (F_NII6583_InvConv_u) (3)
      real*4        EWNII6548IC(nr__) ! (0.1nm) Equivalent width of [NII]6548
*                                               emission line obtained from
*                                               inverse convolution
*                                               (EW_NII6548_InvConv) (3)
      real*4        b_EWNII6548IC(nr__) ! (0.1nm) Lower value of equivalent width of
*                                               [NII]6548 emission line obtained
*                                               from inverse convolution
*                                               (EW_NII6548_InvConv_d) (3)
      real*8        B_EWNII6548IC_1(nr__) ! (0.1nm) Upper value of equivalent width of
*                                               [NII]6548 emission line
*                                               obtained from inverse convolution
*                                               (EW_NII6548_InvConv_u) (3)
      real*8        EWHaIC     (nr__) ! (0.1nm) Equivalent width of Halpha
*                                               emission line obtained from
*                                               inverse convolution
*                                               (EW_Halpha_InvConv) (3)
      real*4        b_EWHaIC   (nr__) ! (0.1nm) Lower value of equivalent width of
*                                               Halpha emission line obtained
*                                               from inverse convolution
*                                               (EW_Halpha_InvConv_d) (3)
      real*8        B_EWHaIC_1 (nr__) ! (0.1nm) Upper value of equivalent width of
*                                               Halpha emission line obtained
*                                               from inverse convolution
*                                               (EW_Halpha_InvConv_u) (3)
      real*8        EWNII6583IC(nr__) ! (0.1nm) Equivalent width of [NII]6583
*                                               emission line obtained from
*                                               inverse convolution
*                                               (EW_NII6583_InvConv) (3)
      real*4        b_EWNII6583IC(nr__) ! (0.1nm) Lower value of equivalent width of
*                                               [NII]6583 emission line obtained
*                                               from inverse convolution
*                                               (EW_NII6583_InvConv_d) (3)
      real*8        B_EWNII6583IC_1(nr__) ! (0.1nm) Upper value of equivalent width of
*                                               [NII]6583 emission line obtained
*                                               from inverse convolution
*                                               (EW_NII6583_InvConv_u) (3)
      real*8        EWOII      (nr__) ! (0.1nm) ? Equivalent width of [OII]
*                                               emission line (EW_OII)
      real*8        e_EWOII    (nr__) ! (0.1nm) ? Error in equivalent width of
*                                               [OII] emission line (e_EW_OII)
      real*8        EWHb       (nr__) ! (0.1nm) ? Equivalent width of Hbeta
*                                               emission line (EW_Hbeta)
      real*8        e_EWHb     (nr__) ! (0.1nm) ? Error in equivalent width of
*                                               Hbeta emission line (e_EW_Hbeta)
      real*8        EWOIII     (nr__) ! (0.1nm) ? Equivalent width of [OIII]5007
*                                               emission line (EW_OIII)
      real*8        e_EWOIII   (nr__) ! (0.1nm) ? Error in equivalent width of
*                                               [OIII]5007 emission line
*                                               (e_EW_OIII)
      real*8        contOII    (nr__) ! (10mW/m2/nm) ? Continuum level of [OII]
*                                               emission line (cont_OII)
      real*8        e_contOII  (nr__) ! (10mW/m2/nm) ? Error in continuum level of
*                                               [OII] emission line (e_cont_OII)
      real*8        contHb     (nr__) ! (10mW/m2/nm) ? Continuum level of Hbeta
*                                               emission line (cont_Hbeta)
      real*8        e_contHb   (nr__) ! (10mW/m2/nm) ? Error in continuum level of
*                                               Hbeta emission line
*                                               (e_cont_Hbeta)
      real*8        contOIII   (nr__) ! (10mW/m2/nm) ? Continuum level of [OIII]5007
*                                               emission line (cont_OIII)
      real*8        e_contOIII (nr__) ! (10mW/m2/nm) ? Error in continuum level of
*                                               [OIII]5007 emission line
*                                               (e_cont_OIII)
      real*8        coreOII    (nr__) ! (10mW/m2/nm) ? Core (amplitude) of [OII]
*                                               emission line (core_OII)
      real*8        e_coreOII  (nr__) ! (10mW/m2/nm) ? Error in core (amplitude) of
*                                               [OII] emission line (e_core_OII)
      real*8        coreHb     (nr__) ! (10mW/m2/nm) ? Core (amplitude) of Hbeta
*                                               emission line (core_Hbeta)
      real*8        e_coreHb   (nr__) ! (10mW/m2/nm) ? Error in core (amplitude) of
*                                               Hbeta emission line
*                                               (e_core_Hbeta)
      real*8        coreOIII   (nr__) ! (10mW/m2/nm) ? Core (amplitude) of [OIII]5007
*                                               emission line (core_OIII)
      real*8        e_coreOIII (nr__) ! (10mW/m2/nm) ? Error in core (amplitude) of
*                                               [OIII]5007 emission line
*                                               (e_core_OIII)
      real*8        sigmaOII   (nr__) ! (0.1nm) ? sigma of the Gaussian fit for
*                                               [OII] emission line (sigma_OII)
      real*8        e_sigmaOII (nr__) ! (0.1nm) ? Error in sigma of the Gaussian
*                                               fit for [OII] emission line
*                                               (e_sigma_OII)
      real*8        sigmaHb    (nr__) ! (0.1nm) ? sigma of the Gaussian fit for
*                                               Hbeta emission line (sigma_Hbeta)
      real*8        e_sigmaHb  (nr__) ! (0.1nm) ? Error in sigma of the Gaussian
*                                               fit for Hbeta emission line
*                                               (e_sigma_Hbeta)
      real*8        sigmaOIII  (nr__) ! (0.1nm) ? sigma of the Gaussian fit for
*                                               [OIII]5007 emission line
*                                               (sigma_OIII)
      real*8        e_sigmaOIII(nr__) ! (0.1nm) ? Error in sigma of the Gaussian
*                                               fit for [OIII]5007 emission line
*                                               (e_sigma_OIII)
      real*8        FWHMOII    (nr__) ! (0.1nm) ? Full-Width at Half Maximum
*                                               (FWHM) of the Gaussian fit for
*                                               [OII] emission line (FWHM_OII)
      real*8        e_FWHMOII  (nr__) ! (0.1nm) ? Error in FWHM of the Gaussian
*                                               fit for [OII] emission line
*                                               (e_FWHM_OII)
      real*8        FWHMHb     (nr__) ! (0.1nm) ? Full-Width at Half Maximum
*                                               (FWHM) of the Gaussian fit for
*                                               Hbeta emission line (FWHM_Hbeta)
      real*8        e_FWHMHb   (nr__) ! (0.1nm) ? Error in FWHM of the Gaussian
*                                               fit for Hbeta emission line
*                                               (e_FWHM_Hbeta)
      real*8        FWHMOIII   (nr__) ! (0.1nm) ? Full-Width at Half Maximum
*                                               (FWHM) of the Gaussian fit for
*                                               [OIII]5007 emission line
*                                               (FWHM_OIII)
      real*8        e_FWHMOIII (nr__) ! (0.1nm) ? Error in FWHM of the Gaussian
*                                               fit for [OIII]5007 emission line
*                                               (e_FWHM_OIII)
      real*8        SNRlineOII (nr__) ! ? Signal-to-Noise Ratio (S/N) of
*                                               the [OII] emission line
*                                               (SNR_line_OII)
      real*8        SNRlineHb  (nr__) ! ? Signal-to-Noise Ratio (S/N) of
*                                               the Hbeta emission line
*                                               (SNR_line_Hbeta)
      real*8        SNRlineOIII(nr__) ! ? Signal-to-Noise Ratio (S/N) of
*                                               the [OIII]5007 emission line
*                                               (SNR_line_OIII)
      real*4        FOII       (nr__) ! (mW/m2) ? Flux of [OII] emission line
*                                               (F_OII)
      real*4        e_FOII     (nr__) ! (mW/m2) ? Error in flux of [OII] emission
*                                               line (e_F_OII)
      real*4        FHb        (nr__) ! (mW/m2) ? Flux of Hbeta emission line
*                                               (F_Hbeta)
      real*4        e_FHb      (nr__) ! (mW/m2) ? Error in flux of Hbeta emission
*                                               line (e_F_Hbeta)
      real*4        FHblim     (nr__) ! (mW/m2) ? Upper-limit flux of Hbeta
*                                               (if no fitting was performed)
*                                               (F_Hbeta_lim)
      real*4        FOIII      (nr__) ! (mW/m2) ? Flux of [OIII]5007 emission line
*                                               (F_OIII)
      real*4        e_FOIII    (nr__) ! (mW/m2) ? Error in flux of [OIII]5007
*                                               emission line (e_F_OIII)
      real*4        FOIIIlim   (nr__) ! (mW/m2) ? Upper-limit flux of [OIII]5007
*                                               (if no fitting was performed)
*                                               (F_OIII_lim)
      real*4        FOIIadj    (nr__) ! (mW/m2) ? Flux of [OII] emission line
*                                               adjusted for aperture effect
*                                               (F_OII_adj) (5)
      real*4        e_FOIIadj  (nr__) ! (mW/m2) ? Error in flux of [OII] emission
*                                               line adjusted for aperture effect
*                                               (e_F_OII_adj) (5)
      real*4        FHbadj     (nr__) ! (mW/m2) ? Flux of Hbeta emission line
*                                               adjusted for aperture effect
*                                               (F_Hbeta_adj) (5)
      real*4        e_FHbadj   (nr__) ! (mW/m2) ? Error in flux of Hbeta emission
*                                               line adjusted for aperture effect
*                                               (e_F_Hbeta_adj) (5)
      real*4        FHbadjlim  (nr__) ! (mW/m2) ? Upper-limit flux of Hbeta
*                                               adjusted for aperture effect
*                                               (if no fitting was performed)
*                                               (F_Hbeta_lim_adj) (4)
      real*4        FOIIIadj   (nr__) ! (mW/m2) ? Flux of [OIII]5007 emission line
*                                               adjusted for aperture effect
*                                               (F_OIII_adj) (5)
      real*4        e_FOIIIadj (nr__) ! (mW/m2) ? Error in flux of [OIII]5007
*                                               emission line adjusted for
*                                               aperture effect
*                                               (e_F_OI )5)II_adj) (5)
      real*4        FOIIIadjlim(nr__) ! (mW/m2) ? Upper-limit flux of [OIII]5007
*                                               adjusted for aperture effect
*                                               (if no fitting was performed)
*                                               (F_OIII_lim_adj) (4)
      real*4        FHaabs     (nr__) ! (mW/m2) ? Flux of Halpha emission line
*                                               adjusted and corrected for
*                                               absorption (F_Halpha_abs) (3)
      real*4        e_FHaabs   (nr__) ! (mW/m2) ? Error in flux of Halpha emission
*                                               line adjusted and corrected for
*                                               absorption (e_F_Halpha_abs) (3)
      real*4        FHbabs     (nr__) ! (mW/m2) ? Flux of Hbeta emission line
*                                               adjusted and corrected for
*                                               absorption (F_Hbeta_abs)
      real*4        e_FHbabs   (nr__) ! (mW/m2) ? Error in flux of Hbeta emission
*                                               line adjusted and corrected for
*                                               absorption (e_F_Hbeta_abs)
      real*4        FHbabslim  (nr__) ! (mW/m2) ? Upper-limit flux of Hbeta
*                                               adjusted and corrected for
*                                               absorption (if no fitting was
*                                               performed) (F_Hbeta_lim_abs)
      real*4        FNII6548ec (nr__) ! (mW/m2) ? Flux of [NII]6548 emission line
*                                               adjusted and corrected for
*                                               absorptions and extinction
*                                               (F_NII6548_extinc) (3)
      real*4        e_FNII6548ec(nr__) ! (mW/m2) ? Error in flux of [NII]6548
*                                               emission line adjusted and
*                                               corrected for absorptions and
*                                               extinction
*                                               (e_F_NII6548_extinc) (3)
      real*4        FHaec      (nr__) ! (mW/m2) ? Flux of Halpha emission line
*                                               adjusted and corrected for
*                                               absorptions and extinction
*                                               (F_Halpha_extinc)
      real*4        e_FHaec    (nr__) ! (mW/m2) ? Error in flux of Halpha emission
*                                               line adjusted and corrected for
*                                               absorptions and extinction
*                                               (e_F_Halpha_extinc) (3)
      real*4        FNII6583ec (nr__) ! (mW/m2) Flux of [NII]6583 emission line
*                                               adjusted and corrected for
*                                               absorptions and extinction
*                                               (F_NII6583_extinc) (3)
      real*4        e_FNII6583ec(nr__) ! (mW/m2) Error in flux of [NII]6583
*                                               emission line adjusted and
*                                               corrected for absorptions and
*                                               extinction
*                                               (e_F_NII6583_extinc) (3)
      real*4        FOIIec     (nr__) ! (mW/m2) ? Flux of [OII] emission line
*                                               adjusted and corrected for
*                                               absorptions and extinction
*                                               (F_OII_extinc)
      real*4        e_FOIIec   (nr__) ! (mW/m2) ? Error in flux of [OII] emission
*                                               line adjusted and corrected for
*                                               absorptions and extinction
*                                               (e_F_OII_extinc)
      real*4        FHbec      (nr__) ! (mW/m2) ? Flux of Hbeta emission line
*                                               adjusted and corrected for
*                                               absorptions and extinction
*                                               (F_Hbeta_extinc)
      real*4        e_FHbec    (nr__) ! (mW/m2) ? Error in flux of Hbeta emission
*                                               line adjusted and corrected for
*                                               absorptions and extinction
*                                               (e_F_Hbeta_extinc)
      real*4        FHbeclim   (nr__) ! (mW/m2) ? Upper-limit flux of Hbeta
*                                               adjusted and corrected for
*                                               absorptions and extinction
*                                               (if no fitting was performed)
*                                               (F_Hbeta_lim_extinc)
      real*4        FOIIIec    (nr__) ! (mW/m2) ? Flux of [OIII]5007 emission line
*                                               adjusted and corrected for
*                                               absorptions and extinction
*                                               (F_OIII_extinc)
      real*4        e_FOIIIec  (nr__) ! (mW/m2) ? Error in flux of [OIII]5007
*                                               emission line adjusted and
*                                               corrected for absorptions and
*                                               extinction (e_F_OIII_extinc)
      real*4        FOIIIeclim (nr__) ! (mW/m2) ? Upper-limit flux of [OIII]5007
*                                               adjusted and corrected for
*                                               absorptions and extinction
*                                               (if no fitting was performed)
*                                               (F_OIII_lim_extinc)
      real*8        FluxadjfacOII(nr__) ! ? Flux adjustment factor for
*                                               [OII] emission line
*                                               (flux_adj_factor_OII) (5)
      real*8        FluxadjfacHb(nr__) ! ? Flux adjustment factor for Hbeta
*                                               emission line
*                                               (flux_adj_factor_Hbeta) (5)
      real*8        FluxadjfacOIII(nr__) ! ? Flux adjustment factor for
*                                               [OIII]5007 emission line
*                                               (flux_adj_factor_OIII) (5)
      real*4        EWabsHaCSP (nr__) ! (0.1nm) ? Equivalent width of Halpha line
*                                               obtained from CSP
*                                               (EW_abs_Halpha_CSP)
      real*4        EWabsHbCSP (nr__) ! (0.1nm) ? Equivalent width of Hbeta line
*                                               obtained from CSP
*                                               (EW_abs_Hbeta_CSP)
      real*8        E_B_V_Balmer(nr__) ! ? Balmer decrement- derived color
*                                               excess of the stellar continuum
*                                               (E_B_V_Balmer)
      real*8        E_B_V_CSP  (nr__) ! ? Color excess of the stellar
*                                               continuum obtained from CSP
*                                               (E_B_V_CSP)
      real*8        E_B_V_used (nr__) ! ? Color excess of the stellar
*                                               continuum used to apply
*                                               correction of extinction
*                                               (E_B_V_used)
      character*6   FlagE_B_V  (nr__) ! Flag indicating the source of
*                                               E(B_V_used: "Balmer" for Balmer
*                                               decrement, "CSP" for CSP
*                                               (flag_EBV)
      real*8        logM_      (nr__) ! ([Msun]) ? Logarithm of the stellar mass
*                                               obtained from CSP
*                                               (logStellar_mass)
      real*8        e_logM_    (nr__) ! ([Msun]) ? Error in logarithm of the
*                                               stellar mass obtained from
*                                               CSP (e_logStellar_mass)
      real*8        D4000      (nr__) ! ? D4000 break index (D4000)
      real*8        e_D4000    (nr__) ! ? Error in D4000 break index
*                                               (e_D4000)
      real*8        MetN2IC    (nr__) ! ? N2 metallicity (12+log(O/H))
*                                               from inverse convolution
*                                               (Met_N2_InvConv) (3)
      real*8        b_MetN2IC  (nr__) ! Lower value of N2 metallicity
*                                               (12+log(O/H)) from inverse
*                                               convolution
*                                               (Met_N2_InvConv_d) (3)
      real*8        B_MetN2IC_1(nr__) ! Upper value of N2 metallicity
*                                               (12+log(O/H)) from inverse
*                                               convolution
*                                               (Met_N2_InvConv_u) (3)
      real*8        MetP05     (nr__) ! ? P05 metallicity (12+log(O/H))
*                                               (Met_P05)
      real*8        e_MetP05   (nr__) ! ? Error in P05 metallicity
*                                               (12+log(O/H)) (e_Met_P05)
      real*8        MetZ94     (nr__) ! ? Z94 metallicity (12+log(O/H))
*                                               (Met_Z94)
      real*8        e_MetZ94   (nr__) ! ? Error in Z94 metallicity
*                                               (12+log(O/H)) (e_Met_Z94)
      real*8        MetM91     (nr__) ! ? M91 metallicity (12+log(O/H))
*                                               (Met_M91)
      real*8        e_MetM91   (nr__) ! ? Error in M91 metallicity
*                                               (12+log(O/H)) (e_Met_M91)
      real*8        MetPP04    (nr__) ! ? PP04 metallicity (12+log(O/H))
*                                               (Met_PP04)
      real*8        e_MetPP04  (nr__) ! ? Error in PP04 metallicity
*                                               (12+log(O/H)) (e_Met_PP04)
      real*8        MetT04     (nr__) ! ? T04 metallicity (12+log(O/H))
*                                               (Met_T04)
      real*8        e_MetT04   (nr__) ! ? Error in T04 metallicity
*                                               (12+log(O/H)) (e_Met_T04)
      real*8        SFRHa      (nr__) ! (Msun/yr) ? Halpha star formation rate
*                                               (Kennicutt & Evans,
*                                               2012ARA&A..50..531K) (SFR_Ha)
      real*8        e_SFRHa    (nr__) ! (Msun/yr) ? Error in Halpha star formation
*                                               rate based on Halpha (Kennicutt &
*                                               Evans, 2012ARA&A..50..531K)
*                                               (e_SFR_Ha)
      real*8        SFRHb      (nr__) ! (Msun/yr) ? Hbeta star formation rate based
*                                               (Kennicutt & Evans,
*                                               2012ARA&A..50..531K) (SFR_Hbeta)
      real*8        e_SFRHb    (nr__) ! (Msun/yr) ? Error in Hbeta star formation
*                                               rate based (Kennicutt & Evans,
*                                               2012ARA&A..50..531K)
*                                               (e_SFR_Hbeta)
      real*8        SFROIIZ94  (nr__) ! (Msun/yr) ? [OII] star formation rate
*                                               corrected by Z94 (Kewley+2004)
*                                               (SFR_OII_Z94)
      real*8        e_SFROIIZ94(nr__) ! (Msun/yr) ? Error in [OII] star formation
*                                               rate corrected by Z94
*                                               (Kewley+2004) (e_SFR_OII_Z94)
      real*8        SFROIIM91  (nr__) ! (Msun/yr) ? [OII] star formation rate
*                                               corrected by M91 (Kewley et al.
*                                               2004AJ....127.2002K)
*                                               (SFR_OII_M91)
      real*8        e_SFROIIM91(nr__) ! (Msun/yr) ? Error in [OII] star formation
*                                               rate corrected by M91
*                                               (Kewley, 2004AJ....127.2002K)
*                                               (e_SFR_OII_M91)
      real*8        Dclusteras (nr__) ! (arcsec) Cluster-centric projected distance
*                                               in arcsec (D_cluster_arcsec) (6)
      real*8        DclusterMpc(nr__) ! (Mpc) Cluster-centric projected distance
*                                               in Mpc (D_cluster_Mpc) (6)
      real*8        sigma5     (nr__) ! (1/Mpc2) Local density estimated to the
*                                               5th neighbor (sigma5) (6)
      real*8        sigma10    (nr__) ! (1/Mpc2) Local density estimated to the
*                                               10th neighbor (sigma10) (6)
      real*4        isAGNSP15  (nr__) ! True/False flag for AGN activity
*                                               (isAGN_SP15) (1)
      real*4        isBLAGNSP15(nr__) ! True/False flag for broad-line AGN
*                                               (isBLAGN_SP15) (1)
      real*4        isAGNBPT   (nr__) ! [0/1]? True/False flag for AGN
*                                               activity based on BPT
*                                               (Kauffmann+2003); NaN if not
*                                               conclusive (isAGN_BPT)
      real*4        isAGNWHAN  (nr__) ! [0/1]? True/False flag for AGN
*                                               activity based on EWalphaN2
*                                               (Ho+1997); NaN if not conclusive
*                                               (isAGN_WHAN)
      real*4        isSFGMOS   (nr__) ! [0/1]True/False flag for
*                                               star-forming galaxies based on
*                                               BPT and EWalphaN2; NaN if not
*                                               conclusive (isSFG_MOS)
      real*4        isAGNMOS   (nr__) ! [0/1]True/False flag for AGN
*                                               activity based on BPT and
*                                               EWalphaN2; NaN if not conclusive
*                                               (isAGN_MOS)
      real*4        isCompMOS  (nr__) ! [0/1]? True/False flag for
*                                               composite galaxies based on BPT
*                                               and EWalphaN2; NaN if not
*                                               conclusive (isComposite_MOS)
      real*4        isOutlier  (nr__) ! [0/1] True/False flag for outlier
*                                               galaxies (TF redshift not
*                                               confident) (is_Outlier)
      integer*4     QualIC     (nr__) ! [1/6] Quality criterion of
*                                               inverse convolution
*                                               (Quality_InvConv) (3)
*Note (1): Values from Sanchez-Portal et al., 2015, Cat. J/A+A/578/A30
*Note (2): 'a' or 'b'; see Fig. 4 in Sanchez-Portal et al . 2015A&A...578A..30S,
*          'C' and 'O', respectively, in Table 5 of Sanchez-Portal et al.,
*          2015A&A...578A..30S, Cat. J/A+A/578/A30
*Note (3): Following the methodology and data described in Cedres et al.,
*           2024A&A...686A..60C
*Note (4): Based on z_avg or, if unavailable, z_Halpha_InvConv
*           (if Quality_InvConv<4) or z_SP15 (if Quality_InvConv>=4).
*           If 0.366<z<0.3876, it is "B", else if z>0.3876, it is "A";
*           if z<0.366, it is "Interloper"
*Note (5): Fluxes were adjusted due to the use of MOS slits, as described in
*           Appendix B.1.
*Note (6): Information provided by Perez-Martinez et al. (in prep.).

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

C  Loading file 'catalog.dat'	! Catalog of the properties of the galaxies

C  Format for file interpretation

    1 format(
     +  A7,1X,I5,1X,A5,1X,F9.7,1X,F10.7,1X,F8.6,1X,F8.5,1X,F8.6,1X,
     +  F8.6,1X,F8.6,1X,F8.6,1X,F19.17,1X,F22.20,1X,F19.17,1X,F22.20,
     +  1X,F19.17,1X,F22.20,1X,F19.17,1X,F22.20,1X,A10,1X,F18.15,1X,
     +  F21.19,1X,F17.14,1X,F21.19,1X,F18.15,1X,F20.18,1X,F18.15,1X,
     +  F18.16,1X,F18.15,1X,F18.16,1X,F18.15,1X,F18.16,1X,F18.15,1X,
     +  F18.16,1X,E22.17,1X,E22.17,1X,E22.17,1X,E21.16,1X,E22.17,1X,
     +  E22.17,1X,E22.17,1X,E22.17,1X,F10.6,1X,F9.6,1X,E22.17,1X,
     +  E22.17,1X,E22.17,1X,F9.6,1X,F9.6,1X,F9.6,1X,E22.17,1X,E22.17,
     +  1X,E22.17,1X,E22.17,1X,E11.6,1X,E22.17,1X,E22.17,1X,E22.17,1X,
     +  E22.17,1X,E8.6,1X,E11.6,1X,F9.6,1X,F10.6,1X,E8.6,1X,F9.5,1X,
     +  F9.6,1X,E11.9,1X,F9.6,1X,F20.15,1X,F20.16,1X,F20.16,1X,F19.16,
     +  1X,F20.16,1X,F19.16,1X,F19.16,1X,F18.16,1X,F19.16,1X,F18.16,
     +  1X,F19.16,1X,F18.16,1X,F19.16,1X,F18.16,1X,F19.16,1X,F18.16,
     +  1X,F20.16,1X,F18.16,1X,F18.16,1X,F18.16,1X,F18.16,1X,F19.16,
     +  1X,F18.16,1X,F18.16,1X,F18.15,1X,F18.16,1X,F18.15,1X,F19.16,
     +  1X,F18.15,1X,F18.16,1X,F19.15,1X,F20.16,1X,F19.16,1X,E22.17,
     +  1X,E22.17,1X,E22.17,1X,E22.17,1X,E22.17,1X,E22.17,1X,E22.17,
     +  1X,E22.17,1X,E22.17,1X,E22.17,1X,E22.17,1X,E22.17,1X,E22.17,
     +  1X,E22.17,1X,E22.17,1X,E22.17,1X,E22.17,1X,E22.17,1X,E22.17,
     +  1X,E22.17,1X,E21.16,1X,E22.17,1X,E22.17,1X,E22.17,1X,E22.17,
     +  1X,E22.17,1X,E22.17,1X,E22.17,1X,E22.17,1X,E22.17,1X,E22.17,
     +  1X,E22.17,1X,E22.17,1X,E22.17,1X,E22.17,1X,F18.16,1X,F18.16,
     +  1X,F18.16,1X,F4.2,1X,F4.2,1X,F19.16,1X,F18.16,1X,F18.16,1X,A6,
     +  1X,F18.15,1X,F20.18,1X,F18.16,1X,F18.16,1X,F7.5,1X,F7.5,1X,
     +  F7.5,1X,F18.16,1X,F22.10,1X,F17.15,1X,F18.16,1X,F17.15,1X,
     +  F18.16,1X,F17.15,1X,F18.16,1X,F17.15,1X,F18.16,1X,F19.16,1X,
     +  F18.16,1X,F19.16,1X,F18.16,1X,F19.16,1X,F18.16,1X,F18.16,1X,
     +  F18.16,1X,F18.14,1X,F18.16,1X,F20.16,1X,F19.16,1X,F3.1,1X,
     +  F3.1,1X,F3.1,1X,F3.1,1X,F3.1,1X,F3.1,1X,F3.1,1X,F3.1,1X,I1)

C  Effective file loading

      open(unit=1,status='old',file=
     +'catalog.dat')
      write(6,*) '....Loading file: catalog.dat'
      do i__=1,102
        read(1,'(A3288)')ar__
        read(ar__,1)
     +  ID_unique(i__),ID(i__),ID_MOS(i__),RAdeg(i__),DEdeg(i__),
     +  RAGdeg(i__),DEGdeg(i__),zSP15(i__),zHaIC(i__),b_zHaIC(i__),
     +  B_zHaIC_1(i__),zOII(i__),e_zOII(i__),zHb(i__),e_zHb(i__),
     +  zOIII(i__),e_zOIII(i__),zMOSavg(i__),e_zMOSavg(i__),
     +  Structure(i__),Bmag(i__),e_Bmag(i__),Vmag(i__),e_Vmag(i__),
     +  Rmag(i__),e_Rmag(i__),Imag(i__),e_Imag(i__),Jmag(i__),
     +  e_Jmag(i__),Ksmag(i__),e_Ksmag(i__),F814Wmag(i__),
     +  e_F814Wmag(i__),FHaSP15(i__),e_FHaSP15(i__),FNIISP15(i__),
     +  e_FNIISP15(i__),FHacSP15(i__),e_FHacSP15(i__),FNIIcSP15(i__),
     +  e_FNIIcSP15(i__),EWHaSP15(i__),e_EWHaSP15(i__),ContHaIC(i__),
     +  b_ContHaIC(i__),B_ContHaIC_1(i__),sigmaHaIC(i__),
     +  b_sigmaHaIC(i__),B_sigmaHaIC_1(i__),FNII6548IC(i__),
     +  b_FNII6548IC(i__),B_FNII6548IC_1(i__),FHaIC(i__),b_FHaIC(i__),
     +  B_FHaIC_1(i__),FNII6583IC(i__),b_FNII6583IC(i__),
     +  B_FNII6583IC_1(i__),EWNII6548IC(i__),b_EWNII6548IC(i__),
     +  B_EWNII6548IC_1(i__),EWHaIC(i__),b_EWHaIC(i__),
     +  B_EWHaIC_1(i__),EWNII6583IC(i__),b_EWNII6583IC(i__),
     +  B_EWNII6583IC_1(i__),EWOII(i__),e_EWOII(i__),EWHb(i__),
     +  e_EWHb(i__),EWOIII(i__),e_EWOIII(i__),contOII(i__),
     +  e_contOII(i__),contHb(i__),e_contHb(i__),contOIII(i__),
     +  e_contOIII(i__),coreOII(i__),e_coreOII(i__),coreHb(i__),
     +  e_coreHb(i__),coreOIII(i__),e_coreOIII(i__),sigmaOII(i__),
     +  e_sigmaOII(i__),sigmaHb(i__),e_sigmaHb(i__),sigmaOIII(i__),
     +  e_sigmaOIII(i__),FWHMOII(i__),e_FWHMOII(i__),FWHMHb(i__),
     +  e_FWHMHb(i__),FWHMOIII(i__),e_FWHMOIII(i__),SNRlineOII(i__),
     +  SNRlineHb(i__),SNRlineOIII(i__),FOII(i__),e_FOII(i__),
     +  FHb(i__),e_FHb(i__),FHblim(i__),FOIII(i__),e_FOIII(i__),
     +  FOIIIlim(i__),FOIIadj(i__),e_FOIIadj(i__),FHbadj(i__),
     +  e_FHbadj(i__),FHbadjlim(i__),FOIIIadj(i__),e_FOIIIadj(i__),
     +  FOIIIadjlim(i__),FHaabs(i__),e_FHaabs(i__),FHbabs(i__),
     +  e_FHbabs(i__),FHbabslim(i__),FNII6548ec(i__),
     +  e_FNII6548ec(i__),FHaec(i__),e_FHaec(i__),FNII6583ec(i__),
     +  e_FNII6583ec(i__),FOIIec(i__),e_FOIIec(i__),FHbec(i__),
     +  e_FHbec(i__),FHbeclim(i__),FOIIIec(i__),e_FOIIIec(i__),
     +  FOIIIeclim(i__),FluxadjfacOII(i__),FluxadjfacHb(i__),
     +  FluxadjfacOIII(i__),EWabsHaCSP(i__),EWabsHbCSP(i__),
     +  E_B_V_Balmer(i__),E_B_V_CSP(i__),E_B_V_used(i__),
     +  FlagE_B_V(i__),logM_(i__),e_logM_(i__),D4000(i__),
     +  e_D4000(i__),MetN2IC(i__),b_MetN2IC(i__),B_MetN2IC_1(i__),
     +  MetP05(i__),e_MetP05(i__),MetZ94(i__),e_MetZ94(i__),
     +  MetM91(i__),e_MetM91(i__),MetPP04(i__),e_MetPP04(i__),
     +  MetT04(i__),e_MetT04(i__),SFRHa(i__),e_SFRHa(i__),SFRHb(i__),
     +  e_SFRHb(i__),SFROIIZ94(i__),e_SFROIIZ94(i__),SFROIIM91(i__),
     +  e_SFROIIM91(i__),Dclusteras(i__),DclusterMpc(i__),sigma5(i__),
     +  sigma10(i__),isAGNSP15(i__),isBLAGNSP15(i__),isAGNBPT(i__),
     +  isAGNWHAN(i__),isSFGMOS(i__),isAGNMOS(i__),isCompMOS(i__),
     +  isOutlier(i__),QualIC(i__)
        if(ar__(96:114) .EQ. '') zOII(i__) = rNULL__
        if(ar__(116:137) .EQ. '') e_zOII(i__) = rNULL__
        if(ar__(139:157) .EQ. '') zHb(i__) = rNULL__
        if(ar__(159:180) .EQ. '') e_zHb(i__) = rNULL__
        if(ar__(182:200) .EQ. '') zOIII(i__) = rNULL__
        if(ar__(202:223) .EQ. '') e_zOIII(i__) = rNULL__
        if(ar__(225:243) .EQ. '') zMOSavg(i__) = rNULL__
        if(ar__(245:266) .EQ. '') e_zMOSavg(i__) = rNULL__
        if(ar__(279:296) .EQ. '') Bmag(i__) = rNULL__
        if(ar__(298:318) .EQ. '') e_Bmag(i__) = rNULL__
        if(ar__(320:336) .EQ. '') Vmag(i__) = rNULL__
        if(ar__(338:358) .EQ. '') e_Vmag(i__) = rNULL__
        if(ar__(360:377) .EQ. '') Rmag(i__) = rNULL__
        if(ar__(379:398) .EQ. '') e_Rmag(i__) = rNULL__
        if(ar__(400:417) .EQ. '') Imag(i__) = rNULL__
        if(ar__(419:436) .EQ. '') e_Imag(i__) = rNULL__
        if(ar__(438:455) .EQ. '') Jmag(i__) = rNULL__
        if(ar__(457:474) .EQ. '') e_Jmag(i__) = rNULL__
        if(ar__(476:493) .EQ. '') Ksmag(i__) = rNULL__
        if(ar__(495:512) .EQ. '') e_Ksmag(i__) = rNULL__
        if(ar__(514:531) .EQ. '') F814Wmag(i__) = rNULL__
        if(ar__(533:550) .EQ. '') e_F814Wmag(i__) = rNULL__
        if(ar__(598:619) .EQ. '') FNIISP15(i__) = rNULL__
        if(ar__(621:641) .EQ. '') e_FNIISP15(i__) = rNULL__
        if(ar__(689:710) .EQ. '') FNIIcSP15(i__) = rNULL__
        if(ar__(712:733) .EQ. '') e_FNIIcSP15(i__) = rNULL__
        if(ar__(1144:1163) .EQ. '') EWOII(i__) = rNULL__
        if(ar__(1165:1184) .EQ. '') e_EWOII(i__) = rNULL__
        if(ar__(1186:1205) .EQ. '') EWHb(i__) = rNULL__
        if(ar__(1207:1225) .EQ. '') e_EWHb(i__) = rNULL__
        if(ar__(1227:1246) .EQ. '') EWOIII(i__) = rNULL__
        if(ar__(1248:1266) .EQ. '') e_EWOIII(i__) = rNULL__
        if(ar__(1268:1286) .EQ. '') contOII(i__) = rNULL__
        if(ar__(1288:1305) .EQ. '') e_contOII(i__) = rNULL__
        if(ar__(1307:1325) .EQ. '') contHb(i__) = rNULL__
        if(ar__(1327:1344) .EQ. '') e_contHb(i__) = rNULL__
        if(ar__(1346:1364) .EQ. '') contOIII(i__) = rNULL__
        if(ar__(1366:1383) .EQ. '') e_contOIII(i__) = rNULL__
        if(ar__(1385:1403) .EQ. '') coreOII(i__) = rNULL__
        if(ar__(1405:1422) .EQ. '') e_coreOII(i__) = rNULL__
        if(ar__(1424:1442) .EQ. '') coreHb(i__) = rNULL__
        if(ar__(1444:1461) .EQ. '') e_coreHb(i__) = rNULL__
        if(ar__(1463:1482) .EQ. '') coreOIII(i__) = rNULL__
        if(ar__(1484:1501) .EQ. '') e_coreOIII(i__) = rNULL__
        if(ar__(1503:1520) .EQ. '') sigmaOII(i__) = rNULL__
        if(ar__(1522:1539) .EQ. '') e_sigmaOII(i__) = rNULL__
        if(ar__(1541:1558) .EQ. '') sigmaHb(i__) = rNULL__
        if(ar__(1560:1578) .EQ. '') e_sigmaHb(i__) = rNULL__
        if(ar__(1580:1597) .EQ. '') sigmaOIII(i__) = rNULL__
        if(ar__(1599:1616) .EQ. '') e_sigmaOIII(i__) = rNULL__
        if(ar__(1618:1635) .EQ. '') FWHMOII(i__) = rNULL__
        if(ar__(1637:1654) .EQ. '') e_FWHMOII(i__) = rNULL__
        if(ar__(1656:1673) .EQ. '') FWHMHb(i__) = rNULL__
        if(ar__(1675:1693) .EQ. '') e_FWHMHb(i__) = rNULL__
        if(ar__(1695:1712) .EQ. '') FWHMOIII(i__) = rNULL__
        if(ar__(1714:1731) .EQ. '') e_FWHMOIII(i__) = rNULL__
        if(ar__(1733:1751) .EQ. '') SNRlineOII(i__) = rNULL__
        if(ar__(1753:1772) .EQ. '') SNRlineHb(i__) = rNULL__
        if(ar__(1774:1792) .EQ. '') SNRlineOIII(i__) = rNULL__
        if(ar__(1794:1815) .EQ. '') FOII(i__) = rNULL__
        if(ar__(1817:1838) .EQ. '') e_FOII(i__) = rNULL__
        if(ar__(1840:1861) .EQ. '') FHb(i__) = rNULL__
        if(ar__(1863:1884) .EQ. '') e_FHb(i__) = rNULL__
        if(ar__(1886:1907) .EQ. '') FHblim(i__) = rNULL__
        if(ar__(1909:1930) .EQ. '') FOIII(i__) = rNULL__
        if(ar__(1932:1953) .EQ. '') e_FOIII(i__) = rNULL__
        if(ar__(1955:1976) .EQ. '') FOIIIlim(i__) = rNULL__
        if(ar__(1978:1999) .EQ. '') FOIIadj(i__) = rNULL__
        if(ar__(2001:2022) .EQ. '') e_FOIIadj(i__) = rNULL__
        if(ar__(2024:2045) .EQ. '') FHbadj(i__) = rNULL__
        if(ar__(2047:2068) .EQ. '') e_FHbadj(i__) = rNULL__
        if(ar__(2070:2091) .EQ. '') FHbadjlim(i__) = rNULL__
        if(ar__(2093:2114) .EQ. '') FOIIIadj(i__) = rNULL__
        if(ar__(2116:2137) .EQ. '') e_FOIIIadj(i__) = rNULL__
        if(ar__(2139:2160) .EQ. '') FOIIIadjlim(i__) = rNULL__
        if(ar__(2162:2183) .EQ. '') FHaabs(i__) = rNULL__
        if(ar__(2185:2206) .EQ. '') e_FHaabs(i__) = rNULL__
        if(ar__(2208:2229) .EQ. '') FHbabs(i__) = rNULL__
        if(ar__(2231:2252) .EQ. '') e_FHbabs(i__) = rNULL__
        if(ar__(2254:2274) .EQ. '') FHbabslim(i__) = rNULL__
        if(ar__(2276:2297) .EQ. '') FNII6548ec(i__) = rNULL__
        if(ar__(2299:2320) .EQ. '') e_FNII6548ec(i__) = rNULL__
        if(ar__(2322:2343) .EQ. '') FHaec(i__) = rNULL__
        if(ar__(2345:2366) .EQ. '') e_FHaec(i__) = rNULL__
        if(ar__(2414:2435) .EQ. '') FOIIec(i__) = rNULL__
        if(ar__(2437:2458) .EQ. '') e_FOIIec(i__) = rNULL__
        if(ar__(2460:2481) .EQ. '') FHbec(i__) = rNULL__
        if(ar__(2483:2504) .EQ. '') e_FHbec(i__) = rNULL__
        if(ar__(2506:2527) .EQ. '') FHbeclim(i__) = rNULL__
        if(ar__(2529:2550) .EQ. '') FOIIIec(i__) = rNULL__
        if(ar__(2552:2573) .EQ. '') e_FOIIIec(i__) = rNULL__
        if(ar__(2575:2596) .EQ. '') FOIIIeclim(i__) = rNULL__
        if(ar__(2598:2615) .EQ. '') FluxadjfacOII(i__) = rNULL__
        if(ar__(2617:2634) .EQ. '') FluxadjfacHb(i__) = rNULL__
        if(ar__(2636:2653) .EQ. '') FluxadjfacOIII(i__) = rNULL__
        if(ar__(2655:2658) .EQ. '') EWabsHaCSP(i__) = rNULL__
        if(ar__(2660:2663) .EQ. '') EWabsHbCSP(i__) = rNULL__
        if(ar__(2665:2683) .EQ. '') E_B_V_Balmer(i__) = rNULL__
        if(ar__(2685:2702) .EQ. '') E_B_V_CSP(i__) = rNULL__
        if(ar__(2704:2721) .EQ. '') E_B_V_used(i__) = rNULL__
        if(ar__(2730:2747) .EQ. '') logM_(i__) = rNULL__
        if(ar__(2749:2768) .EQ. '') e_logM_(i__) = rNULL__
        if(ar__(2770:2787) .EQ. '') D4000(i__) = rNULL__
        if(ar__(2789:2806) .EQ. '') e_D4000(i__) = rNULL__
        if(ar__(2808:2814) .EQ. '') MetN2IC(i__) = rNULL__
        if(ar__(2832:2849) .EQ. '') MetP05(i__) = rNULL__
        if(ar__(2851:2872) .EQ. '') e_MetP05(i__) = rNULL__
        if(ar__(2874:2890) .EQ. '') MetZ94(i__) = rNULL__
        if(ar__(2892:2909) .EQ. '') e_MetZ94(i__) = rNULL__
        if(ar__(2911:2927) .EQ. '') MetM91(i__) = rNULL__
        if(ar__(2929:2946) .EQ. '') e_MetM91(i__) = rNULL__
        if(ar__(2948:2964) .EQ. '') MetPP04(i__) = rNULL__
        if(ar__(2966:2983) .EQ. '') e_MetPP04(i__) = rNULL__
        if(ar__(2985:3001) .EQ. '') MetT04(i__) = rNULL__
        if(ar__(3003:3020) .EQ. '') e_MetT04(i__) = rNULL__
        if(ar__(3022:3040) .EQ. '') SFRHa(i__) = rNULL__
        if(ar__(3042:3059) .EQ. '') e_SFRHa(i__) = rNULL__
        if(ar__(3061:3079) .EQ. '') SFRHb(i__) = rNULL__
        if(ar__(3081:3098) .EQ. '') e_SFRHb(i__) = rNULL__
        if(ar__(3100:3118) .EQ. '') SFROIIZ94(i__) = rNULL__
        if(ar__(3120:3137) .EQ. '') e_SFROIIZ94(i__) = rNULL__
        if(ar__(3139:3156) .EQ. '') SFROIIM91(i__) = rNULL__
        if(ar__(3158:3175) .EQ. '') e_SFROIIM91(i__) = rNULL__
        if(ar__(3264:3266) .EQ. '') isAGNBPT(i__) = rNULL__
        if(ar__(3268:3270) .EQ. '') isAGNWHAN(i__) = rNULL__
        if(ar__(3280:3282) .EQ. '') isCompMOS(i__) = rNULL__
c    ..............Just test output...........
        write(6,1)
     +  ID_unique(i__),ID(i__),ID_MOS(i__),RAdeg(i__),DEdeg(i__),
     +  RAGdeg(i__),DEGdeg(i__),zSP15(i__),zHaIC(i__),b_zHaIC(i__),
     +  B_zHaIC_1(i__),zOII(i__),e_zOII(i__),zHb(i__),e_zHb(i__),
     +  zOIII(i__),e_zOIII(i__),zMOSavg(i__),e_zMOSavg(i__),
     +  Structure(i__),Bmag(i__),e_Bmag(i__),Vmag(i__),e_Vmag(i__),
     +  Rmag(i__),e_Rmag(i__),Imag(i__),e_Imag(i__),Jmag(i__),
     +  e_Jmag(i__),Ksmag(i__),e_Ksmag(i__),F814Wmag(i__),
     +  e_F814Wmag(i__),FHaSP15(i__),e_FHaSP15(i__),FNIISP15(i__),
     +  e_FNIISP15(i__),FHacSP15(i__),e_FHacSP15(i__),FNIIcSP15(i__),
     +  e_FNIIcSP15(i__),EWHaSP15(i__),e_EWHaSP15(i__),ContHaIC(i__),
     +  b_ContHaIC(i__),B_ContHaIC_1(i__),sigmaHaIC(i__),
     +  b_sigmaHaIC(i__),B_sigmaHaIC_1(i__),FNII6548IC(i__),
     +  b_FNII6548IC(i__),B_FNII6548IC_1(i__),FHaIC(i__),b_FHaIC(i__),
     +  B_FHaIC_1(i__),FNII6583IC(i__),b_FNII6583IC(i__),
     +  B_FNII6583IC_1(i__),EWNII6548IC(i__),b_EWNII6548IC(i__),
     +  B_EWNII6548IC_1(i__),EWHaIC(i__),b_EWHaIC(i__),
     +  B_EWHaIC_1(i__),EWNII6583IC(i__),b_EWNII6583IC(i__),
     +  B_EWNII6583IC_1(i__),EWOII(i__),e_EWOII(i__),EWHb(i__),
     +  e_EWHb(i__),EWOIII(i__),e_EWOIII(i__),contOII(i__),
     +  e_contOII(i__),contHb(i__),e_contHb(i__),contOIII(i__),
     +  e_contOIII(i__),coreOII(i__),e_coreOII(i__),coreHb(i__),
     +  e_coreHb(i__),coreOIII(i__),e_coreOIII(i__),sigmaOII(i__),
     +  e_sigmaOII(i__),sigmaHb(i__),e_sigmaHb(i__),sigmaOIII(i__),
     +  e_sigmaOIII(i__),FWHMOII(i__),e_FWHMOII(i__),FWHMHb(i__),
     +  e_FWHMHb(i__),FWHMOIII(i__),e_FWHMOIII(i__),SNRlineOII(i__),
     +  SNRlineHb(i__),SNRlineOIII(i__),FOII(i__),e_FOII(i__),
     +  FHb(i__),e_FHb(i__),FHblim(i__),FOIII(i__),e_FOIII(i__),
     +  FOIIIlim(i__),FOIIadj(i__),e_FOIIadj(i__),FHbadj(i__),
     +  e_FHbadj(i__),FHbadjlim(i__),FOIIIadj(i__),e_FOIIIadj(i__),
     +  FOIIIadjlim(i__),FHaabs(i__),e_FHaabs(i__),FHbabs(i__),
     +  e_FHbabs(i__),FHbabslim(i__),FNII6548ec(i__),
     +  e_FNII6548ec(i__),FHaec(i__),e_FHaec(i__),FNII6583ec(i__),
     +  e_FNII6583ec(i__),FOIIec(i__),e_FOIIec(i__),FHbec(i__),
     +  e_FHbec(i__),FHbeclim(i__),FOIIIec(i__),e_FOIIIec(i__),
     +  FOIIIeclim(i__),FluxadjfacOII(i__),FluxadjfacHb(i__),
     +  FluxadjfacOIII(i__),EWabsHaCSP(i__),EWabsHbCSP(i__),
     +  E_B_V_Balmer(i__),E_B_V_CSP(i__),E_B_V_used(i__),
     +  FlagE_B_V(i__),logM_(i__),e_logM_(i__),D4000(i__),
     +  e_D4000(i__),MetN2IC(i__),b_MetN2IC(i__),B_MetN2IC_1(i__),
     +  MetP05(i__),e_MetP05(i__),MetZ94(i__),e_MetZ94(i__),
     +  MetM91(i__),e_MetM91(i__),MetPP04(i__),e_MetPP04(i__),
     +  MetT04(i__),e_MetT04(i__),SFRHa(i__),e_SFRHa(i__),SFRHb(i__),
     +  e_SFRHb(i__),SFROIIZ94(i__),e_SFROIIZ94(i__),SFROIIM91(i__),
     +  e_SFROIIM91(i__),Dclusteras(i__),DclusterMpc(i__),sigma5(i__),
     +  sigma10(i__),isAGNSP15(i__),isBLAGNSP15(i__),isAGNBPT(i__),
     +  isAGNWHAN(i__),isSFGMOS(i__),isAGNMOS(i__),isCompMOS(i__),
     +  isOutlier(i__),QualIC(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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