Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_AS/141/123 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-May-20
C=============================================================================
* This code was generated from the ReadMe file documenting a catalogue
* according to the "Standard for Documentation of Astronomical Catalogues"
* currently in use by the Astronomical Data Centers (CDS, ADC, A&A)
* (see full documentation at URL http://vizier.u-strasbg.fr/doc/catstd.htx)
* Please report problems or questions to
C=============================================================================
implicit none
* Unspecified or NULL values, generally corresponding to blank columns,
* are assigned one of the following special values:
* rNULL__ for unknown or NULL floating-point values
* iNULL__ for unknown or NULL integer values
real*4 rNULL__
integer*4 iNULL__
parameter (rNULL__=--2147483648.) ! NULL real number
parameter (iNULL__=(-2147483647-1)) ! NULL int number
integer idig ! testing NULL number
C=============================================================================
Cat. J/A+AS/141/123 Galaxies behind Southern Milky Way (Kraan-Korteweg 2000)
*================================================================================
*A catalog of galaxies behind the Southern Milky Way.
*I. The Hydra/Antlia extension (l=~266{deg}-296{deg}).
* Kraan-Korteweg R.
* <Astron. Astrophys. Suppl. 141, 123 (2000)>
* =2000A&AS..141..123K
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Galaxies behind the Southern Milky Way
integer*4 nr__
parameter (nr__=3279) ! Number of records
character*154 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 RKK (nr__) ! Running number of identified galaxy
character*8 Name (nr__) ! Other optical identification
character*2 IRAS (nr__) ! Code for cross-identification in IRAS PSC (G1)
integer*4 RA1h (nr__) ! (h) Right ascension B1950
integer*4 RA1m (nr__) ! (min) Right ascension B1950
real*4 RA1s (nr__) ! (s) Right ascension B1950
character*1 DE1_ (nr__) ! Declination sign B1950
integer*4 DE1d (nr__) ! (deg) Declination B1950
integer*4 DE1m (nr__) ! (arcmin) Declination B1950
integer*4 DE1s (nr__) ! (arcsec) Declination B1950
character*1 q_DE1s (nr__) ! [:] Positional accuracy for B1950 positions
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
integer*4 DEs (nr__) ! (arcsec) [0,60]? Declination J2000
character*1 q_DEs (nr__) ! [:] Positional accuracy for J2000 positions
real*4 GLON (nr__) ! (deg) Galactic longitude
real*4 GLAT (nr__) ! (deg) Galactic latitude
character*3 ESO_SRC (nr__) ! ESO/SRC Field number
real*4 Xpos (nr__) ! (mm) X coordinate from center of field
real*4 Ypos (nr__) ! (mm) Y coordinate from center of field
integer*4 amaj (nr__) ! (arcsec) Major axis (arcsec)
integer*4 amin (nr__) ! (arcsec) Minor axis (arcsec)
real*4 Bmag (nr__) ! (mag) Estimated B magnitude
real*4 E_B_V (nr__) ! (mag) Extinction E(B-V) according to
* Schlegel et al., 1998ApJ...500..525S
character*11 MType (nr__) ! Morphological type (G2)
character*28 Rem (nr__) ! Remarks (1)
*Note (1): Abbreviations used in Remarks:
* * or **: star or stars
* asym.: asymmetric
* blg: bulge
* br.: bright; to indicate bright bulges, nearby or superimposed
* bright stars or bright bulges
* cl.to br. *: close to bright star
* dbl: double
* diff.: diffuse
* dist.: distinct
* HSB: extremely high surface brightness
* i.a.w.: interacting with; close pair of galaxies which display
* disturbances in the image or light bridges between the
* galaxies.
* LSB: low surface brightness galaxy. Also vLSB for very low surface
* brightness, and vvLSB for galaxies just barely visible
* against the sky background
* neb?: nebula?
* neighb. of: neighbor of a listed galaxy. In general, these galaxies are
* below the diameter limit of D=13" but close to a catalogued
* galaxy and possibly associated with the named neighbor
* PN: Planetary Nebula
* p.cov.by *: partly covered by star
* poss.larger: possibly larger
* s.p.: superimposed (generally used to note superimposed star or
* stars on the galaxy image
* sp.: spiral (e.g. spiral arm)
* struct.: structure
* in st.diff.pat.: galaxy lies within a stellar diffraction pattern, i.e.,
* generally on darkened background
* trpl syst: triple system, generally followed by the identification of
* the other members
* v.: very
* v.obs.: very obscured
* vLSB: see LSB
* vvLSB: see LSB
* w.: with
* w.comp.: with companion: a small galaxy, below the diameter limit of
* the catalog in the vicinity of the galaxy. The companion was
* not entered into the catalog (contrarily to neighbors,
* cf. above)
* w.sev.comp.: with several companions. Same as w.comp., two or more nearby
* small galaxies were seen.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! IRAS galaxies behind the Southern Milky Way
integer*4 nr__1
parameter (nr__1=197) ! Number of records
character*162 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*10 IRAS_1 (nr__1) ! Identification in IRAS PSC (Cat. <II/125>)
character*1 Yamada (nr__1) ! [Y] Crossidentification in Yamada et al.,
* 1993, Cat. <J/ApJS/89/57>
character*3 q_IRAS (nr__1) ! Quality of IRAS PSC cross-identification (G1)
integer*4 RKK_1 (nr__1) ! Running number of identified galaxy
* (from Table 1)
character*1 Lauberts (nr__1) ! [L] Identification in Lauberts catalog
* (1982, Cat. <VII/34>)
integer*4 RA1h_1 (nr__1) ! (h) Right ascension B1950
integer*4 RA1m_1 (nr__1) ! (min) Right ascension B1950
real*4 RA1s_1 (nr__1) ! (s) Right ascension B1950
character*1 DE1__1 (nr__1) ! Declination sign B1950
integer*4 DE1d_1 (nr__1) ! (deg) Declination B1950
integer*4 DE1m_1 (nr__1) ! (arcmin) Declination B1950
integer*4 DE1s_1 (nr__1) ! (arcsec) Declination B1950
character*1 q_DE1s_1 (nr__1) ! [:] Positional accuracy on B1950 positions
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
integer*4 DEs_1 (nr__1) ! (arcsec) Declination J2000
character*1 u_DEs (nr__1) ! [:] Positional accuracy on J2000 positions
real*4 GLON_1 (nr__1) ! (deg) Galactic longitude
real*4 GLAT_1 (nr__1) ! (deg) Galactic latitude
integer*4 amaj_1 (nr__1) ! (arcsec) Major axis
integer*4 amin_1 (nr__1) ! (arcsec) Minor axis
real*4 Bmag_1 (nr__1) ! (mag) Estimated B magnitude
character*4 MType_1 (nr__1) ! Morphological type (G2)
integer*4 Oir_opt (nr__1) ! (arcsec) ? Positional offset (IRAS - optical)
real*4 S12um (nr__1) ! (Jy) Flux density at 12 micron
real*4 S25um (nr__1) ! (Jy) Flux density at 25 micron
real*4 S60um (nr__1) ! (Jy) Flux density at 60 micron
real*4 S100um (nr__1) ! (Jy) Flux density at 100 micron
integer*4 q_S12um (nr__1) ! [1,3] Flux quality at 12 micron (2)
integer*4 q_S25um (nr__1) ! [1,3] Flux quality at 25 micron (2)
integer*4 q_S60um (nr__1) ! [1,3] Flux quality at 60 micron (2)
integer*4 q_S100um (nr__1) ! [1,3] Flux quality at 100 micron (2)
real*4 IRAS1 (nr__1) ! IRAS color 1: (f12xf25)/(f60xf60)
real*4 IRAS2 (nr__1) ! IRAS color 2: f100/f60
*Note (2): The IRAS flags are coded as:
* 1 = lower limit
* 2 = uncertain flux
* 3 = good flux quality
C=============================================================================
C Loading file 'table1.dat' ! Galaxies behind the Southern Milky Way
C Format for file interpretation
1 format(
+ 1X,I4,1X,A8,1X,A2,2X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,A1,
+ 1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,A1,1X,F6.2,1X,F6.2,
+ 2X,A3,1X,F6.1,1X,F6.1,1X,I3,1X,I3,1X,F4.1,1X,F4.2,1X,A11,1X,
+ A28)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,3279
read(1,'(A154)')ar__
read(ar__,1)
+ RKK(i__),Name(i__),IRAS(i__),RA1h(i__),RA1m(i__),RA1s(i__),
+ DE1_(i__),DE1d(i__),DE1m(i__),DE1s(i__),q_DE1s(i__),RAh(i__),
+ RAm(i__),RAs(i__),DE_(i__),DEd(i__),DEm(i__),DEs(i__),
+ q_DEs(i__),GLON(i__),GLAT(i__),ESO_SRC(i__),Xpos(i__),
+ Ypos(i__),amaj(i__),amin(i__),Bmag(i__),E_B_V(i__),MType(i__),
+ Rem(i__)
if(ar__(60:61) .EQ. '') DEs(i__) = iNULL__
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)
+ RKK(i__),Name(i__),IRAS(i__),RA1h(i__),RA1m(i__),RA1s(i__),
+ DE1_(i__),DE1d(i__),DE1m(i__),DE1s(i__),q_DE1s(i__),RAh(i__),
+ RAm(i__),RAs(i__),DE_(i__),DEd(i__),DEm(i__),DEs(i__),
+ q_DEs(i__),GLON(i__),GLAT(i__),ESO_SRC(i__),Xpos(i__),
+ Ypos(i__),amaj(i__),amin(i__),Bmag(i__),E_B_V(i__),MType(i__),
+ Rem(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' ! IRAS galaxies behind the Southern Milky Way
C Format for file interpretation
2 format(
+ 1X,A10,2X,A1,1X,A3,1X,I4,1X,A1,2X,I2,1X,I2,1X,F4.1,1X,A1,I2,
+ 1X,I2,1X,I2,A1,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,A1,1X,
+ F6.2,1X,F6.2,1X,I3,1X,I3,1X,F4.1,3X,A4,1X,I4,2X,F5.2,2X,F5.2,
+ 2X,F5.2,1X,F6.2,2X,I1,1X,I1,1X,I1,1X,I1,2X,F6.2,1X,F6.2)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,197
read(1,'(A162)')ar__1
read(ar__1,2)
+ IRAS_1(i__),Yamada(i__),q_IRAS(i__),RKK_1(i__),Lauberts(i__),
+ RA1h_1(i__),RA1m_1(i__),RA1s_1(i__),DE1__1(i__),DE1d_1(i__),
+ DE1m_1(i__),DE1s_1(i__),q_DE1s_1(i__),RAh_1(i__),RAm_1(i__),
+ RAs_1(i__),DE__1(i__),DEd_1(i__),DEm_1(i__),DEs_1(i__),
+ u_DEs(i__),GLON_1(i__),GLAT_1(i__),amaj_1(i__),amin_1(i__),
+ Bmag_1(i__),MType_1(i__),Oir_opt(i__),S12um(i__),S25um(i__),
+ S60um(i__),S100um(i__),q_S12um(i__),q_S25um(i__),q_S60um(i__),
+ q_S100um(i__),IRAS1(i__),IRAS2(i__)
if(ar__1(106:109) .EQ. '') Oir_opt(i__) = iNULL__
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)
+ IRAS_1(i__),Yamada(i__),q_IRAS(i__),RKK_1(i__),Lauberts(i__),
+ RA1h_1(i__),RA1m_1(i__),RA1s_1(i__),DE1__1(i__),DE1d_1(i__),
+ DE1m_1(i__),DE1s_1(i__),q_DE1s_1(i__),RAh_1(i__),RAm_1(i__),
+ RAs_1(i__),DE__1(i__),DEd_1(i__),DEm_1(i__),DEs_1(i__),
+ u_DEs(i__),GLON_1(i__),GLAT_1(i__),amaj_1(i__),amin_1(i__),
+ Bmag_1(i__),MType_1(i__),Oir_opt(i__),S12um(i__),S25um(i__),
+ S60um(i__),S100um(i__),q_S12um(i__),q_S25um(i__),q_S60um(i__),
+ q_S100um(i__),IRAS1(i__),IRAS2(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_1(i__),DEdeg_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end