Conversion of standardized ReadMe file for
file /./ftp/cats/J/MNRAS/360/340 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-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/MNRAS/360/340 Very Small Array. Flux density at 33GHz (Cleary+, 2005)
*================================================================================
*Source subtraction for the extended Very Small Array and 33-GHz source
*count estimates.
* Cleary K.A., Taylor A.C., Waldram E., Battye R.A., Dickinson C.,
* Davies R.D., Davis R.J., Genova-Santos R., Grainge K., Jones M.E.,
* Kneissl R., Pooley G.G., Rebolo R., Rubino-Martin J.A., Saunders R.D.E.,
* Scott P.F., Slosar A., Titterington D., Watson R.A.
* <Mon. Not. R. Astron. Soc., 360, 340-353 (2005)>
* =2005MNRAS.360..340C
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'tablea1.dat' ! 33-GHz source flux densities
integer*4 nr__
parameter (nr__=102) ! Number of records
character*43 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*9 v_CTW2005_ (nr__) ! Name, HHMM+DDMM, based on J2000 positions
character*1 m__CTW2005_(nr__) ! Multiplicity index on [CTW2005]
character*1 n__CTW2005_(nr__) ! [*] * for sources brighter than 46mJy (1)
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) Declination (J2000)
real*4 S33GHz (nr__) ! (mJy) Flux density at 33GHz
real*4 e_S33GHz (nr__) ! (mJy) rms uncertainty on S33GHz
*Note (1): The normalizing area for the source counts is 0.044sr except for
* those sources brighter than 46mJy (indicated by an asterisk), for
* which it is 0.024sr.
C=============================================================================
C Loading file 'tablea1.dat' ! 33-GHz source flux densities
C Format for file interpretation
1 format(
+ A9,A1,A1,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,1X,F5.1,1X,
+ F4.1)
C Effective file loading
open(unit=1,status='old',file=
+'tablea1.dat')
write(6,*) '....Loading file: tablea1.dat'
do i__=1,102
read(1,'(A43)')ar__
read(ar__,1)
+ v_CTW2005_(i__),m__CTW2005_(i__),n__CTW2005_(i__),RAh(i__),
+ RAm(i__),RAs(i__),DE_(i__),DEd(i__),DEm(i__),DEs(i__),
+ S33GHz(i__),e_S33GHz(i__)
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)
+ v_CTW2005_(i__),m__CTW2005_(i__),n__CTW2005_(i__),RAh(i__),
+ RAm(i__),RAs(i__),DE_(i__),DEd(i__),DEm(i__),DEs(i__),
+ S33GHz(i__),e_S33GHz(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end