Conversion of standardized ReadMe file for
file /./ftp/cats/VIII/3 into FORTRAN code for loading all data files into arrays.
Note that special values are assigned to unknown or unspecified
numbers (also called NULL numbers);
when necessary, the coordinate components making up the right ascension
and declination are converted into floating-point numbers
representing these angles in degrees.
program load_ReadMe
C=============================================================================
C F77-compliant program generated by readme2f_1.81 (2015-09-23), on 2024-Apr-18
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. VIII/3 An Optical Catalogue of Radio Galaxies (Burbidge+ 1979)
*================================================================================
*An Optical Catalogue of Radio Galaxies
* Burbidge G., Crowne A.H.
* <Astrophys. Journ. Suppl. 40, 583 (1979)>
* =1979ApJS...40..583B
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'catalog.dat' ! Radio sources identified with optical galaxies
integer*4 nr__
parameter (nr__=495) ! Number of records
character*272 ar__ ! Full-size record
C 1950 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg (nr__) ! (deg) Right Ascension 1950
real*8 DEdeg (nr__) ! (deg) Declination 1950
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 RAh (nr__) ! (h) Right Ascension 1950 (hours)
integer*4 RAm (nr__) ! (min) Right Ascension 1950 (minutes)
real*4 RAs (nr__) ! (s) ? Right Ascension 1950 (seconds)
integer*4 q_RAs (nr__) ! *Precision indicator of the right ascension
character*1 DE_ (nr__) ! Declination 1950 (sign)
integer*4 DEd (nr__) ! (deg) Declination 1950 (degrees)
integer*4 DEm (nr__) ! (arcmin) ? Declination 1950 (minutes)
real*4 DEs (nr__) ! (arcsec) ? Declination 1950 (seconds)
integer*4 q_DEs (nr__) ! *Precision indicator of declination
integer*4 refID (nr__) ! ?Reference identification number (file "refs")
character*1 EqPos (nr__) ! *[ R] Code for equatorial position
integer*4 FCRnum (nr__) ! ? Finder chart reference number (file "refs")
character*4 OptType (nr__) ! *Optical type code
character*2 Rdesc (nr__) ! *Radio description
real*4 Vmag (nr__) ! (mag) *? Visual magnitude.
real*4 B_V (nr__) ! (mag) ? Photoelectric colors if available
real*4 U_B (nr__) ! (mag) ? Photoelectric colors if available
integer*4 r_Vmag (nr__) ! ? Reference for photometric data (file "refs")
real*4 Z (nr__) ! *Redshift.
character*1 n_Z (nr__) ! *[CQ ] Redshift (cf. bytes 63-68) qualifier
character*2 LineType (nr__) ! *Spectral lines type
character*8 Name (nr__) ! *Coordinate designation
integer*4 r_Z (nr__) ! Redshift (z) reference number (file "refs")
real*8 S_freq (nr__) ! (Jy) ?Radio flux at frequency given in bytes 93-96.
integer*4 freq (nr__) ! (MHz) ?Frequency in MHz (408 for most entries)
integer*4 r_S_freq (nr__) ! ?Reference for radio flux (cf. bytes 85-91)
real*4 Sp_Index (nr__) ! *? Radio spectral index between 408 & 1400 MHz
integer*4 r_Sp_Index (nr__) ! ? Reference for spectral index (file "refs")
integer*4 MapRef (nr__) ! ? Primary reference for radio map number
character*1 SIcode (nr__) ! *[AB ] Code for spectral index range.
integer*4 SpNum (nr__) ! *Number of spectral lines
character*40 Lines (nr__) ! *List of 20 coded spectral lines.
integer*4 NumRef (nr__) ! Number of additional references.
character*60 Arefs (nr__) ! *Additional references
character*50 Alias (nr__) ! *Other names
integer*4 Seq (nr__) ! [1,495] Sequential counter.
*Note on q_RAs:
* Precision indicator of the right ascension; the right ascension is
* given as HH MM SS.ss with eight possible significant digits. The
* precision indicator identifies how many of these eight digits are
* given as blank (i.e. not known) and so may vary between zero and
* eight.
*Note on q_DEs:
* Precision indicator of declination: the declination is given as DD MM
* SS.S with seven possible significant digits. The precision indicator
* identifies how many of these seven digits are given as blank (i.e. not
* known) and so may vary between zero and seven.
*Note on EqPos:
* Code for equatorial position:
* blank = optical position given taken primarily from papers reporting
* the redshift and identification papers.
* R = radio position given ("*" in published catalogue).
*Note on OptType:
* Optical type code - left justified in field. The type codes and their
* statistics are given in "Table A-2" section below. All types and
* cluster information (cf. bytes 38-39) is drawn from either the
* identification reference (cf. bytes 25-27) or the redshift reference
* (cf. bytes 81-83).
*Note on Rdesc:
* Radio description which is no longer used. If these bytes are not
* blank then given object is in a cluster. The radio description codes
* and their statistics are given in "Table A-3" section below.
*Note on Vmag:
* Visual magnitude. These values are very uncertain since very few
* photometric measurements have been made.
*Note on Z:
* Redshift. Most of the redshifts listed are uncorrected for galactic
* rotation.
*Note on n_Z:
* Redshift (cf. bytes 63-68) qualifier:
* blank - if the value of the redshift (z) is not corrected for galactic
* rotation.
* "C" - if z is corrected ("*" in published catalogue)
* "Q" - if unknown if z has been corrected ("?" in published catalogue).
*Note on LineType:
* Spectral lines type:
* "A" - if absorption lines.
* "E" - if emission lines.
* "AE"- if absorption and emission.
* Where no spectral-line lists have been published but mention has been
* made of the appearance of absorption or emission, it is noted with an "A"
* or "E" in these bytes.
*Note on Name:
* Coordinate designation given as HHMMSDDX based on equatorial coordinates
* at epoch B1950.0 where:
* HH = hours of right ascension
* MM = minutes of right ascension
* S = sign of the declination
* DDX= declination (unit=0.1deg)
*Note on Sp-Index:
* Radio spectral index between 408 and 1400 MHz. The spectral index
* alpha is defined by
* S(nu) = K. nu**(-alpha)
* In the published catalogue the symbol ">" following the value of the
* spectral index indicates a range between 408 and 5000 MHz and the
* symbol "<" indicates a range between 178 and 408 MHz. No attempt has
* been made to extrapolate where fluxes have been given at other
* frequencies (cf. byte 115).
*Note on SIcode:
* Code for spectral index range. This code is for the symbols ">" and
* "<" as defined above in bytes 102-106. The ">" is coded as an "A" and
* the "<" is coded as a "B". This byte is blank if other than these two
* spectral indices. See the file "refs".
*Note on SpNum:
* Number of spectral lines used in the computation of the value of the
* redshift. This number ranges from 0 to 20.
*Note on Lines:
* List of 20 coded spectral lines.
* The coded values range from 01 to OR and are defined in
* "Table A-4" section below. The N (cf. bytes 116-117) coded values are
* at the beginning of this field and the remaining bytes are blank.
*Note on Arefs:
* Additional references are five characters each where the first three
* represent the reference number (file "refs") and the two letter code
* for the type of reference as follows:
* ID - identification
* FC - finder chart
* Z - redshift
* S - radio flux (S)
* SI - radio spectral index (SI)
* M - radio map
*Note on Alias:
* Other names - maximum of seven names separated by commas with no
* embedded blanks. "Table A-1" section below gives the codes used in
* these fields along with their full reference to the published
* literature.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'refs.dat' ! References in numeric order
integer*4 nr__1
parameter (nr__1=412) ! Number of records
character*130 ar__1 ! Full-size record
integer*4 RefNum (nr__1) ! *Reference number
character*125 Text (nr__1) ! *Text of References
*Note on RefNum:
* Reference number which ranges from 1-414 but only 412 references.
*Note on Text:
* References in format usually found in the astronomical literature.
C=============================================================================
C Loading file 'catalog.dat' ! Radio sources identified with optical galaxies
C Format for file interpretation
1 format(
+ I2,1X,I2,1X,F5.2,I1,A1,I2,1X,I2,1X,F4.1,I1,I3,A1,I3,1X,A4,1X,
+ A2,1X,F5.2,1X,F5.2,1X,F5.2,1X,I3,1X,F6.4,A1,A2,1X,A8,I3,1X,
+ F7.2,1X,I4,1X,I3,1X,F5.2,1X,I3,1X,I3,A1,I2,A40,I2,A60,A50,I3)
C Effective file loading
open(unit=1,status='old',file=
+'catalog.dat')
write(6,*) '....Loading file: catalog.dat'
do i__=1,495
read(1,'(A272)')ar__
read(ar__,1)
+ RAh(i__),RAm(i__),RAs(i__),q_RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),q_DEs(i__),refID(i__),EqPos(i__),
+ FCRnum(i__),OptType(i__),Rdesc(i__),Vmag(i__),B_V(i__),
+ U_B(i__),r_Vmag(i__),Z(i__),n_Z(i__),LineType(i__),Name(i__),
+ r_Z(i__),S_freq(i__),freq(i__),r_S_freq(i__),Sp_Index(i__),
+ r_Sp_Index(i__),MapRef(i__),SIcode(i__),SpNum(i__),Lines(i__),
+ NumRef(i__),Arefs(i__),Alias(i__),Seq(i__)
if(ar__(7:11) .EQ. '') RAs(i__) = rNULL__
if(ar__(17:18) .EQ. '') DEm(i__) = iNULL__
if(ar__(20:23) .EQ. '') DEs(i__) = rNULL__
if(ar__(25:27) .EQ. '') refID(i__) = iNULL__
if(ar__(29:31) .EQ. '') FCRnum(i__) = iNULL__
if(ar__(41:45) .EQ. '') Vmag(i__) = rNULL__
if(ar__(47:51) .EQ. '') B_V(i__) = rNULL__
if(ar__(53:57) .EQ. '') U_B(i__) = rNULL__
if(ar__(59:61) .EQ. '') r_Vmag(i__) = iNULL__
if(ar__(85:91) .EQ. '') S_freq(i__) = rNULL__
if(ar__(93:96) .EQ. '') freq(i__) = iNULL__
if(ar__(98:100) .EQ. '') r_S_freq(i__) = iNULL__
if(ar__(102:106) .EQ. '') Sp_Index(i__) = rNULL__
if(ar__(108:110) .EQ. '') r_Sp_Index(i__) = iNULL__
if(ar__(112:114) .EQ. '') MapRef(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)
+ RAh(i__),RAm(i__),RAs(i__),q_RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),q_DEs(i__),refID(i__),EqPos(i__),
+ FCRnum(i__),OptType(i__),Rdesc(i__),Vmag(i__),B_V(i__),
+ U_B(i__),r_Vmag(i__),Z(i__),n_Z(i__),LineType(i__),Name(i__),
+ r_Z(i__),S_freq(i__),freq(i__),r_S_freq(i__),Sp_Index(i__),
+ r_Sp_Index(i__),MapRef(i__),SIcode(i__),SpNum(i__),Lines(i__),
+ NumRef(i__),Arefs(i__),Alias(i__),Seq(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 'refs.dat' ! References in numeric order
C Format for file interpretation
2 format(I3,2X,A125)
C Effective file loading
open(unit=1,status='old',file=
+'refs.dat')
write(6,*) '....Loading file: refs.dat'
do i__=1,412
read(1,'(A130)')ar__1
read(ar__1,2)RefNum(i__),Text(i__)
c ..............Just test output...........
write(6,2)RefNum(i__),Text(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end