Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJS/199/27 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-Jun-10
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/ApJS/199/27 The ATLBS Extended Source Sample (Saripalli+, 2012)
*================================================================================
*ATLBS Extended Source Sample: the evolution in radio source morphology with
*flux density.
* Saripalli L., Subrahmanyan R., Thorat K., Ekers R.D., Hunstead R.W.,
* Johnston H.M., Sadler E.M.
* <Astrophys. J. Suppl. Ser., 199, 27 (2012)>
* =2012ApJS..199...27S
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! ATLBS (Australia Telescope Low Brightness Survey)
Extended Source Sample
integer*4 nr__
parameter (nr__=119) ! Number of records
character*261 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*12 ATLBS (nr__) ! Source name (JHHMM.m+DDMM)
character*3 f_ATLBS (nr__) ! [*,gf ] Flag on ATLBS (1)
integer*4 RAh (nr__) ! (h) Hour of Right Ascension (J2000)
integer*4 RAm (nr__) ! (min) Minute of Right Ascension (J2000)
real*4 RAs (nr__) ! (s) Second of Right Ascension (J2000)
character*1 DE_ (nr__) ! [-] Sign of the Declination (J2000)
integer*4 DEd (nr__) ! (deg) Degree of Declination (J2000)
integer*4 DEm (nr__) ! (arcmin) Arcminute of Declination (J2000)
real*4 DEs (nr__) ! (arcsec) Arcsecond of Declination (J2000)
integer*4 LAS (nr__) ! (arcsec) [30/1020] Angular size within 3{sigma} contours
integer*4 Size (nr__) ! (kpc) ? Linear size (from table 2)
character*5 Morph (nr__) ! Morphology (2)
integer*4 Fig (nr__) ! [1/119] Figure number
real*4 St (nr__) ! (mJy) Total flux density at 1.4GHz
real*4 Sc_St (nr__) ! ? Ratio of total and fractional core flux density
character*12 Type (nr__) ! Source classification (3)
real*4 z (nr__) ! ? Redshift
character*1 f_z (nr__) ! [r] Redshift estimated from red magnitude (4)
real*4 rmag (nr__) ! (mag) ? r-band magnitude
character*161 Comm (nr__) ! Additional comments
*Note (1): Flag as follows:
* * = Source selected from region that lies outside the effective primary
* beam attenuation of 0.5.
* g = Candidate giant radio galaxy
* f = Candidate giant radio galaxy with identifications that are too faint to
* determine reliable r magnitudes. Given their faint magnitudes they are
* expected to lie at relatively high z.
*Note (2): Morphology as follows:
* FR-I = FR-I type radio galaxy (FR-I morphology invariably manifest a pair of
* bright jets or two-sided extensions to the core and lack well-defined
* lobes; the cores are the brightest components).
* FR-II = FR-II type radio galaxy (FR-II sources are usually observed to have a
* pair of distinct edge-brightened lobes with possibly embedded hot
* spots/warm spots).
* WAT = wide angle tail structure;
* HT = head-tail type structure.
* See section 3 for further details.
*Note (3): Classification abbreviation as follows:
* RS = restarted source;
* HzFR-I = z>0.5 FR-I;
* GRG = giant radio galaxy.
*Note (4):
* r = Redshifts values estimated using the r-band magnitude-redshift relation.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4.dat' ! *Candidate halo-type radio sources in the ATLBS-ESS
integer*4 nr__1
parameter (nr__1=23) ! Number of records
character*108 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*12 ATLBS_1 (nr__1) ! Source name (JHHMM.m+DDMM)
integer*4 RAh_1 (nr__1) ! (h) Hour of right ascension (J2000) (1)
integer*4 RAm_1 (nr__1) ! (min) Minute of right ascension (J2000)
real*4 RAs_1 (nr__1) ! (s) Second of right ascension (J2000)
character*1 DE__1 (nr__1) ! Sign of declination (J2000) (1)
integer*4 DEd_1 (nr__1) ! (deg) Degree of declination (J2000) (1)
integer*4 DEm_1 (nr__1) ! (arcmin) Arcminute of declination (J2000)
real*4 DEs_1 (nr__1) ! (arcsec) Arcsecond of declination (J2000)
real*4 Fres (nr__1) ! [1.5/4]? Ratio (low/high resolution) of the
* flux densities in the 50" and 4" images
character*66 Comm_1 (nr__1) ! Comments
*Note (1): The centroid positions from the original 50" images.
C=============================================================================
C Loading file 'table1.dat' ! ATLBS (Australia Telescope Low Brightness Survey)
* Extended Source Sample
C Format for file interpretation
1 format(
+ A12,A3,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F5.2,1X,I4,1X,I4,
+ 1X,A5,1X,I3,1X,F6.2,1X,F5.3,1X,A12,1X,F5.3,A1,1X,F5.2,1X,A161)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,119
read(1,'(A261)')ar__
read(ar__,1)
+ ATLBS(i__),f_ATLBS(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
+ DEd(i__),DEm(i__),DEs(i__),LAS(i__),Size(i__),Morph(i__),
+ Fig(i__),St(i__),Sc_St(i__),Type(i__),z(i__),f_z(i__),
+ rmag(i__),Comm(i__)
if(ar__(47:50) .EQ. '') Size(i__) = iNULL__
if(ar__(69:73) .EQ. '') Sc_St(i__) = rNULL__
if(ar__(88:92) .EQ. '') z(i__) = rNULL__
if(ar__(95:99) .EQ. '') rmag(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)
+ ATLBS(i__),f_ATLBS(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
+ DEd(i__),DEm(i__),DEs(i__),LAS(i__),Size(i__),Morph(i__),
+ Fig(i__),St(i__),Sc_St(i__),Type(i__),z(i__),f_z(i__),
+ rmag(i__),Comm(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 'table4.dat' ! *Candidate halo-type radio sources in the ATLBS-ESS
C Format for file interpretation
2 format(
+ A12,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F4.2,1X,A66)
C Effective file loading
open(unit=1,status='old',file=
+'table4.dat')
write(6,*) '....Loading file: table4.dat'
do i__=1,23
read(1,'(A108)')ar__1
read(ar__1,2)
+ ATLBS_1(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
+ DEd_1(i__),DEm_1(i__),DEs_1(i__),Fres(i__),Comm_1(i__)
if(ar__1(38:41) .EQ. '') Fres(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)
+ ATLBS_1(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
+ DEd_1(i__),DEm_1(i__),DEs_1(i__),Fres(i__),Comm_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=============================================================================
stop
end