Conversion of standardized ReadMe file for
file /./ftp/cats/VII/163/ 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-19
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. VII/163 A Catalogue of Galactic Supernovae Remnants (Green 1994)
*================================================================================
*A Catalogue of Galactic Supernovae Remnants
* Green, D.A.
* <in Proc. IAU Colloq. 145, "Supernovae and Supernovae Remnants",
* held May 22-29 1993, in Xian, China,
* Eds. McCray, R., and Wang, Z., Camb. Univ. Press (1994)>
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'catalog' ! *Supernovae remnants catalog
integer*4 nr__
parameter (nr__=182) ! Number of records
character*87 ar__ ! Full-size record
C B1950 position composed of: RAh RAm RAs DE- DEd DEm
real*8 RAdeg (nr__) ! (deg) Right Ascension B1950
real*8 DEdeg (nr__) ! (deg) Declination B1950
C ---------------------------------- ! (position vector(s) in degrees)
real*4 GLON (nr__) ! (deg) *Galactic longitude l
real*4 GLAT (nr__) ! (deg) *Galactic latitude b
integer*4 RAh (nr__) ! (h) *Right Ascension B1950 hours
integer*4 RAm (nr__) ! (min) *Right Ascension B1950 minutes
integer*4 RAs (nr__) ! (s) *Right Ascension B1950 seconds
character*1 DE_ (nr__) ! *Declination sign
integer*4 DEd (nr__) ! (deg) *Declination B1950 degrees
integer*4 DEm (nr__) ! (arcmin) *Declination B1950 arcminutes
character*7 Ang_Size (nr__) ! (arcmin2) [0-9.x? ] Angular Size of remnant
character*2 type (nr__) ! *[CFS? ] Type of remnant
character*5 F_1GHz (nr__) ! (Jy) *[0-9.? ] Flux Density at 1 GHx
character*6 SpIndx (nr__) ! [0-9.?varies ] Spectral Index of
* integrated radio emission
character*26 note (nr__) ! Notes to the source
*Note on GLON, GLAT:
* Galactic Coordinates are the source centroid quoted to the nearest
* tenth of a degree.
*Note on RAh, RAm, RAs, DE-, DEd, DEm:
* The accuracy of the quoted values depends on the size of the
* remnant. For small remnants they are to the nearest few seconds of
* time and the nearest minute of arc for RA and DEC respectively. For
* the larger remnants they are rounded to coarser values. They are in
* every case sufficient to specify a point within the boundaries of the
* remnant. These coordinates are deduced from radio maps rather than
* from X-ray or optical observations, and are B1950.0.
*Note on F(1GHz):
* The flux density of the remnant at !GHz in Jansky. This is not a
* measured value, but that deduced from the observed radio frequency
* spectrum of the source. The frequency of 1GHz is chosen because flux
* density measurements at frequencies both above and below this value
* are usually available.
*Note on type:
* S remnant shows a shell
* F remnant shows a filled center
* C remnant shows a composite or combination radiostructure
* S?, C?, F? if there is some uncertainty
* ? object is conventionally considered a SNR although its nature is
* poorly known or not well understood.
C=============================================================================
C Loading file 'catalog' ! *Supernovae remnants catalog
C Format for file interpretation
1 format(
+ 1X,F5.1,2X,F5.1,1X,I2,1X,I2,1X,I2,2X,A1,I2,1X,I2,2X,A7,3X,A2,
+ 2X,A5,2X,A6,2X,A26)
C Effective file loading
open(unit=1,status='old',file=
+'catalog')
write(6,*) '....Loading file: catalog'
do i__=1,182
read(1,'(A87)')ar__
read(ar__,1)
+ GLON(i__),GLAT(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
+ DEd(i__),DEm(i__),Ang_Size(i__),type(i__),F_1GHz(i__),
+ SpIndx(i__),note(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(DE_(i__).EQ.'-'.AND.DEdeg(i__).GE.0) DEdeg(i__)=-DEdeg(i__)
c ..............Just test output...........
write(6,1)
+ GLON(i__),GLAT(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
+ DEd(i__),DEm(i__),Ang_Size(i__),type(i__),F_1GHz(i__),
+ SpIndx(i__),note(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end