FORTRAN Generation
(/./ftp/cats/J/AJ/135/588)

Conversion of standardized ReadMe file for file /./ftp/cats/J/AJ/135/588 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-Sep-15
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/135/588       Arecibo legacy fast ALFA survey V.         (Saintonge+, 2008)
*================================================================================
*The Arecibo Legacy Fast Alfa Survey.
*V. The H I source catalog of the Anti-Virgo region at {delta} = +27{deg}.
*    Saintonge A., Giovanelli R., Haynes M.P., Hoffman G.L., Kent B.R.,
*    Martin A.M., Stierwalt S., Brosch N.
*   <Astron. J., 135, 588-604 (2008)>
*   =2008AJ....135..588S
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'table1.dat'	! HI Candidate Detections

      integer*4 nr__
      parameter (nr__=488)	! Number of records
      character*337 ar__   	! Full-size record

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

      integer*4     ALFALFA2   (nr__) ! Catalog entry number (2-NNN)
      integer*4     AGC        (nr__) ! Arecibo General Catalog number (1)
      integer*4     RAh        (nr__) ! (h) HI Hour of Right Ascension (J2000) (2)
      integer*4     RAm        (nr__) ! (min) HI Minute of Right Ascension (J2000) (2)
      real*4        RAs        (nr__) ! (s) HI Second of Right Ascension (J2000) (2)
      character*1   DE_        (nr__) ! HI Declination sign (J2000) (2)
      integer*4     DEd        (nr__) ! (deg) HI Degree of Declination (J2000) (2)
      integer*4     DEm        (nr__) ! (arcmin) HI Arcminute of Declination (J2000) (2)
      integer*4     DEs        (nr__) ! (arcsec) HI Arcsecond of Declination (J2000) (2)
      integer*4     RAOh       (nr__) ! (h) ? Optical Right Ascension (J2000) (3)
      integer*4     RAOm       (nr__) ! (min) ? Optical Right Ascension (J2000) (3)
      real*4        RAOs       (nr__) ! (s) ? Optical Right Ascension (J2000) (3)
      character*1   DEO_       (nr__) ! Optical Declination sign (J2000)(3)
      integer*4     DEOd       (nr__) ! (deg) ? Optical Declination (J2000) (3)
      integer*4     DEOm       (nr__) ! (arcmin) ? Optical Declination (J2000) (3)
      integer*4     DEOs       (nr__) ! (arcsec) ? Optical Declination (J2000) (3)
      integer*4     cz         (nr__) ! (km/s) Heliocentric velocity of the HI source (4)
      integer*4     W50        (nr__) ! (km/s) Velocity width at 50% level (5)
      integer*4     e_W50      (nr__) ! (km/s) Estimated error in W50
      real*4        Fc         (nr__) ! (Jy.km/s) Integrated flux density (6)
      real*4        e_Fc       (nr__) ! (Jy.km/s) Estimated error in Fc
      real*4        S_N        (nr__) ! Signal-to-noise ratio of detection (7)
      real*4        rms        (nr__) ! (mJy) Noise figure of spatially integrated
*                                   spectral profile (8)
      real*4        Dist       (nr__) ! (Mpc) ? Adopted distance (9)
      real*4        logM       (nr__) ! ([solMass]) ? Log of HI mass (10)
      integer*4     Qual       (nr__) ! Source quality code (11)
      character*231 Note       (nr__) ! Additional comments for source
*Note (1): The AGC entry (Cat. VIII/77) normally corresponds to an optical
*     counterpart except in the cases of HI sources which cannot be
*     associated with an optical object with any high degree of probability.
*     Numbers lower than 1000 are UGC number (Cat. VII/26).
*Note (2): Of the HI source, after correction for systematic telescope
*     pointing errors, which are on the order of 20". The accuracy of the 
*     HI positions depends on source strength. On average, the positional
*     accuracy is about 19".
*Note (3): Optical galaxy found to provide a reasonable optical counterpart.
*     Quality of centroids is estimated to be ~2" or better. The assessment
*     of optical identification is based on spatial proximity, optical
*     redshift (if available), morphology and color. For sources with no
*     discernible optical counterpart and those for which such assignment 
*     is ambiguous, due to the presence of more than one equally possible
*     optical counterpart, no optical position is listed.
*Note (4): Measured as the midpoint between the channels at which the flux
*     density drops to 50% of each of the two peaks (or of one, if only one
*     is present) at each side of the spectral feature.
*Note (5): This value is corrected for instrumental broadening. No
*     corrections due to turbulent motions, disk inclination or 
*     cosmological effects are applied.
*Note (6): Measured on the integrated spectrum, obtained by spatially
*     integrating the source image over a solid angle of at least 7'x7' 
*     and dividing by the sum of the survey beam values over the same 
*     set of image pixels.
*Note (7): Estimated as S/N=(1000Fc/W50)(w_smo_^1/2^/rms). Where w_smo_ is
*     either W50/(2x10) for W50<400km/s or 400/(2x10)=20 for W50{>=}400km/s
*     [w_smo_ is a smoothing width expressed as the number of spectral
*     resolution bins of 10km/s bridging half of the signal width].
*Note (8): The rms as measured over the signal- and rfi-free portions of the
*     spectrum, after Hanning smoothing to a spectral resolution of 10km/s.
*Note (9): For objects with cz>6000km/s, the distance is simply
*     cz_cmb_/H_0_; cz_cmb_ is the recession velocity measured in the Cosmic
*     Microwave Background reference frame and H_0_ is the Hubble constant,
*     for which we use a value of 70km/s/Mpc.  For objects of lower cz_cmb_,
*     we use the peculiar velocity model for the local universe of Masters
*     (Giovanelli et al., Paper II, 2005, Cat. J/AJ/130/2613), which is
*     based on data from the SFI++ catalog of galaxies (Springob et al.,
*     2007, Cat. J/ApJS/172/599).
*Note (10): Obtained by using the expression M_HI_=2.356x10^5^Dist^2^Fc.
*Note (11): Quality code as 1, 2 or 9:
*    1 = refers to sources of S/N and general qualities that make it a 
*        reliable detection.  See text for additional details.
*    2 = refers to sources of low S/N (<6.5), which would ordinarily not be
*        considered reliable detections by the criteria set for code 1.
*    9 = refers to objects assumed to be HVCs; no estimate of their
*        distances is made.

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

C  Declarations for 'table2.dat'	! Detections in the NGC672 and NGC784 Groups

      integer*4 nr__1
      parameter (nr__1=11)	! Number of records
      character*69 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)

      integer*4     AGC_1      (nr__1) ! AGC catalog identification number
      character*6   OName      (nr__1) ! NGC, IC or [KK98a] number
      integer*4     RAh_1      (nr__1) ! (h) HI Hour of Right Ascension (J2000)
      integer*4     RAm_1      (nr__1) ! (min) HI Minute of Right Ascension (J2000)
      real*4        RAs_1      (nr__1) ! (s) HI Second of Right Ascension (J2000)
      character*1   DE__1      (nr__1) ! HI Declination sign (J2000)
      integer*4     DEd_1      (nr__1) ! (deg) HI Degree of Declination (J2000)
      integer*4     DEm_1      (nr__1) ! (arcmin) HI Arcminute of Declination (J2000)
      integer*4     DEs_1      (nr__1) ! (arcsec) HI Arcsecond of Declination (J2000)
      integer*4     cz_1       (nr__1) ! (km/s) Heliocentric recession velocity
      integer*4     W50_1      (nr__1) ! (km/s) Velocity width at 50% level
      real*4        Fc_1       (nr__1) ! (Jy.km/s) Integrated flux density
      real*4        Dist_1     (nr__1) ! (Mpc) ?=- Calculated distance using the peculiar
*                                    velocity model
      real*4        Distl      (nr__1) ! (Mpc) ? Distance from litterature (1)
      character*1   n_Distl    (nr__1) ! [a] Remark on Distance (2)
      real*4        logM_1     (nr__1) ! ([solMass]) ? Log of HI mass estimated from Dist
      real*4        logMl      (nr__1) ! ([solMass]) Log of HI mass estimated from Distl
      character*1   n_logMl    (nr__1) ! [b] means HI mass of the object, if at the
*                                    distance of NGC784 of 5.0Mpc
      character*4   Group      (nr__1) ! Group Membership
*Note (1): Distances found in the literature and assigned on the basis of
*     primary distance indicators or group membership (Huchtmeier et al.,
*     2000, Cat J/A+AS/141/469; Karachentsev et al., 2003, Cat.
*     J/A+A/398/479, Karachentsev et al., 2004, Cat. J/AJ/127/2031).
*Note (2): No association between the HI detection and an optical galaxy
*     which is part of the NGC784 group has been made. This object is likely
*     to be of Galactic origin, and therefore a distance from the peculiar
*     velocity model is not warranted.

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

C  Declarations for 'table3.dat'	! Detections of High Velocity Clouds (HVCs)
                             Previously Reported

      integer*4 nr__2
      parameter (nr__2=12)	! Number of records
      character*38 ar__2  	! Full-size record

C  J2000 position composed of: RAh RAm DE- DEd DEm
      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*6   Name       (nr__2) ! HVC catalogs identification
      character*5   Cat        (nr__2) ! Catalog reference (1)
      integer*4     RAh_2      (nr__2) ! (h) HI Hour of Right ascension (J2000)
      real*4        RAm_2      (nr__2) ! (min) HI Minute of right ascension (J2000)
      character*1   DE__2      (nr__2) ! HI Declination sign (J2000)
      integer*4     DEd_2      (nr__2) ! (deg) HI Degree of Declination (J2000)
      integer*4     DEm_2      (nr__2) ! (arcmin) HI Arcminute of declination (J2000)
      integer*4     v_LSR      (nr__2) ! (km/s) Local Standard of Rest (LSR) velocity
      integer*4     F          (nr__2) ! (Jy.km/s) ?=- Integrated flux density
      character*3   ALFALFA    (nr__2) ! Yes or No for sources in ALFALFA
*Note (1): HVC catalogs as follows:
*   WW91 = Wakker & van Woerden, 1991A&A...250..509W (WV NNN in Simbad)
*   DBB02 = de Heij et al., 2002A&A...391..159D, Cat. J/A+A/391/159 ([DBB2002]
*           NNN in Simbad)
*   L02 = Lockman et al., 2002, Cat. J/ApJS/140/331, ID=119 in table 4

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

C  Loading file 'table1.dat'	! HI Candidate Detections

C  Format for file interpretation

    1 format(
     +  2X,I3,1X,I6,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,1X,I2,1X,
     +  I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,1X,I5,1X,I3,1X,I3,1X,F6.2,1X,
     +  F4.2,1X,F5.1,1X,F4.2,1X,F5.1,1X,F5.2,1X,I1,1X,A231)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table1.dat')
      write(6,*) '....Loading file: table1.dat'
      do i__=1,488
        read(1,'(A337)')ar__
        read(ar__,1)
     +  ALFALFA2(i__),AGC(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
     +  DEd(i__),DEm(i__),DEs(i__),RAOh(i__),RAOm(i__),RAOs(i__),
     +  DEO_(i__),DEOd(i__),DEOm(i__),DEOs(i__),cz(i__),W50(i__),
     +  e_W50(i__),Fc(i__),e_Fc(i__),S_N(i__),rms(i__),Dist(i__),
     +  logM(i__),Qual(i__),Note(i__)
        if(ar__(35:36) .EQ. '') RAOh(i__) = iNULL__
        if(ar__(38:39) .EQ. '') RAOm(i__) = iNULL__
        if(ar__(41:44) .EQ. '') RAOs(i__) = rNULL__
        if(ar__(47:48) .EQ. '') DEOd(i__) = iNULL__
        if(ar__(50:51) .EQ. '') DEOm(i__) = iNULL__
        if(ar__(53:54) .EQ. '') DEOs(i__) = iNULL__
        if(ar__(93:97) .EQ. '') Dist(i__) = rNULL__
        if(ar__(99:103) .EQ. '') logM(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)
     +  ALFALFA2(i__),AGC(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
     +  DEd(i__),DEm(i__),DEs(i__),RAOh(i__),RAOm(i__),RAOs(i__),
     +  DEO_(i__),DEOd(i__),DEOm(i__),DEOs(i__),cz(i__),W50(i__),
     +  e_W50(i__),Fc(i__),e_Fc(i__),S_N(i__),rms(i__),Dist(i__),
     +  logM(i__),Qual(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'	! Detections in the NGC672 and NGC784 Groups

C  Format for file interpretation

    2 format(
     +  I6,1X,A6,1X,I2,I2,F4.1,A1,I2,I2,I2,1X,I3,1X,I3,1X,F6.2,1X,
     +  F3.1,1X,F3.1,A1,1X,F4.2,1X,F4.2,A1,1X,A4)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table2.dat')
      write(6,*) '....Loading file: table2.dat'
      do i__=1,11
        read(1,'(A69)')ar__1
        read(ar__1,2)
     +  AGC_1(i__),OName(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),
     +  DE__1(i__),DEd_1(i__),DEm_1(i__),DEs_1(i__),cz_1(i__),
     +  W50_1(i__),Fc_1(i__),Dist_1(i__),Distl(i__),n_Distl(i__),
     +  logM_1(i__),logMl(i__),n_logMl(i__),Group(i__)
        if (idig(ar__1(46:48)).EQ.0) Dist_1(i__) =  rNULL__
        if(ar__1(50:52) .EQ. '') Distl(i__) = rNULL__
        if(ar__1(55:58) .EQ. '') logM_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)
     +  AGC_1(i__),OName(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),
     +  DE__1(i__),DEd_1(i__),DEm_1(i__),DEs_1(i__),cz_1(i__),
     +  W50_1(i__),Fc_1(i__),Dist_1(i__),Distl(i__),n_Distl(i__),
     +  logM_1(i__),logMl(i__),n_logMl(i__),Group(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 'table3.dat'	! Detections of High Velocity Clouds (HVCs)
*                             Previously Reported

C  Format for file interpretation

    3 format(A6,1X,A5,1X,I2,F4.1,A1,I2,I2,1X,I4,1X,I4,1X,A3)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table3.dat')
      write(6,*) '....Loading file: table3.dat'
      do i__=1,12
        read(1,'(A38)')ar__2
        read(ar__2,3)
     +  Name(i__),Cat(i__),RAh_2(i__),RAm_2(i__),DE__2(i__),
     +  DEd_2(i__),DEm_2(i__),v_LSR(i__),F(i__),ALFALFA(i__)
        if (F(i__) .EQ. 45) F(i__) =  iNULL__
        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(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(DE__2(i__).EQ.'-'.AND.DEdeg_2(i__).GE.0) DEdeg_2(i__)=-DEdeg_2(i__)
c    ..............Just test output...........
        write(6,3)
     +  Name(i__),Cat(i__),RAh_2(i__),RAm_2(i__),DE__2(i__),
     +  DEd_2(i__),DEm_2(i__),v_LSR(i__),F(i__),ALFALFA(i__)
        write(6,'(6H Pos: 2F8.4)') RAdeg_2(i__),DEdeg_2(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