Conversion of standardized ReadMe file for
file /./ftp/cats/J/PASP/117/199 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. J/PASP/117/199 IRTS carbon stars (Le Bertre+, 2005)
*================================================================================
*Carbon stars in the Infrared Telescope in Space Survey.
* Le Bertre T., Tanaka M., Yamamura I., Murakami H., MacConnell D.J.
* <Publ. Astron. Soc. Pac., 117, 199-206 (2005)>
* =2005PASP..117..199L
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! IRTS carbon stars
integer*4 nr__
parameter (nr__=143) ! Number of records
character*69 ar__ ! Full-size record
C Position composed of: GLON GLAT
character*10 NIRS (nr__) ! NIRS (Near-Infrared Spectrometer) name
* ([LTY2003] NIRS HHMMm+DDMM in Simbad)
character*1 m_NIRS (nr__) ! [NS] Multiplicity flag on NIRS
real*4 GLON (nr__) ! (deg) Galactic longitude
real*4 GLAT (nr__) ! (deg) Galactic latitude
real*4 Kmag (nr__) ! (mag) K band magnitude
real*4 K_L_ (nr__) ! (mag) K-L' color index
real*4 v3_1um (nr__) ! 3.1{mu}m index (1)
character*10 IRAS (nr__) ! IRAS name
integer*4 CGCS (nr__) ! ? CGCS number (Cat. <III/227>)
character*6 Com (nr__) ! Comments (2)
*Note (1): To identify carbon stars in the NIRS PSC (Near-Infrared Spectrometer
* Point Source Catalog), we use the 3.1{mu}m index defined in Paper II
* (2003, Cat. <J/A+A/403/943>). This index gives the depth of the band
* (at 3.1{mu}m) relative to the continuum (taken at 2.9 and 3.3{mu}m);
* the maximum depth is obtained for an index value of 0.0, whereas a
* value 0.5 indicates a flat spectrum.
*Note (2): Comments, defined as follows:
* a = A 30 minute exposure plate obtained by D.J. MacConnell shows nothing at
* this position. The R DSS2 plate has a faint star 3" southeast of the
* IRAS position.
* b = A 30 minute exposure plate obtained by D.J. MacConnell shows a faint
* continuum (short and red) that has a general character of a carbon star
* but is too underexposed to be certain, although it has been tentatively
* identified as a C star by MacConnell (1979A&AS...38..335M). The R DSS2
* plate has a bright star at the IRAS position.
* c = A 60 minute exposure plate obtained by D.J. MacConnell shows nothing at
* the IRAS position.
* d = The 2.9-3.5m spectrum was also presented by Groenewegen et al.
* (1994A&A...287..163G).
* e = A 60 minute exposure plate obtained by D.J. MacConnell has a very red,
* non-C star east of the IRAS position, which probably corresponds to the
* bright star 32" away at position angle 66{deg} on the DDS2 I plate.
* f = LRS spectrum C (11{mu}m SiC emission; Kwok et al. 1997,
* Cat. <J/ApJS/112/557>); tentative identification as a C star by Chen &
* Chen (2003AJ....125.2215C)
* g = The 3.1{mu}m index is larger than 0.45 (2003, Cat. <J/A+A/403/943>).
* h = The 3.1{mu}m index is larger than 0.45 (M. Tanaka et al. 2005,
* in preparation).
C=============================================================================
C Loading file 'table1.dat' ! IRTS carbon stars
C Format for file interpretation
1 format(
+ A10,1X,A1,1X,F6.2,1X,F6.2,1X,F4.2,1X,F4.2,1X,F4.2,1X,A10,6X,
+ I4,1X,A6)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,143
read(1,'(A69)')ar__
read(ar__,1)
+ NIRS(i__),m_NIRS(i__),GLON(i__),GLAT(i__),Kmag(i__),K_L_(i__),
+ v3_1um(i__),IRAS(i__),CGCS(i__),Com(i__)
if(ar__(59:62) .EQ. '') CGCS(i__) = iNULL__
c ..............Just test output...........
write(6,1)
+ NIRS(i__),m_NIRS(i__),GLON(i__),GLAT(i__),Kmag(i__),K_L_(i__),
+ v3_1um(i__),IRAS(i__),CGCS(i__),Com(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end