Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/595/A88 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-16
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+A/595/A88 G345.45+1.50 ^13^CO(3-2) clumps (Lopez-Calderon+, 2016)
*================================================================================
*G345.45+1.50: an expanding ring-like structure with massive star formation.
* Lopez-Calderon C., Bronfman L., Nyman L.-A., Garay G.,
* de Gregorio-Monsalvo I., Bergman P.
* <Astron. Astrophys., 595, A88 (2016)>
* =2016A&A...595A..88L (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'tablef1.dat' ! Physical properties of the ^13^CO clumps
integer*4 nr__
parameter (nr__=104) ! Number of records
character*62 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 Seq (nr__) ! [1/104] Sequential number
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)
real*4 DEs (nr__) ! (arcsec) Declination (J2000)
real*4 Dc (nr__) ! (pc) Clump diameter
real*4 Mc (nr__) ! (Msun) Clump mass
real*4 DVc (nr__) ! (km/s) Clump ^13^CO line velocity width
real*4 nc (nr__) ! (cm-3) Clump ^13^CO density
real*4 Nc_1 (nr__) ! (cm-2) Clump ^13^CO column density
character*1 Type (nr__) ! [ABC] Clump type (1)
character*1 B_E (nr__) ! [Y/N] indicates if clumps are candidates to be
* experimenting collapse ({xi}max>=6.5)
*Note (1): The clumps are classified into three types as follows:
* A = clumps have a counterpart seen in infrared and millimeter wavelengths
* B = clumps only have a counterpart in the 1.2mm continuum
* C = clumps are only seen in ^13^CO.
C=============================================================================
C Loading file 'tablef1.dat' ! Physical properties of the ^13^CO clumps
C Format for file interpretation
1 format(
+ I3,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F5.2,1X,F3.1,1X,E6.2,
+ 1X,F3.1,1X,E6.2,1X,E7.2,1X,A1,1X,A1)
C Effective file loading
open(unit=1,status='old',file=
+'tablef1.dat')
write(6,*) '....Loading file: tablef1.dat'
do i__=1,104
read(1,'(A62)')ar__
read(ar__,1)
+ Seq(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),Dc(i__),Mc(i__),DVc(i__),nc(i__),Nc_1(i__),
+ Type(i__),B_E(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)
+ Seq(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),Dc(i__),Mc(i__),DVc(i__),nc(i__),Nc_1(i__),
+ Type(i__),B_E(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end