Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/540/A133 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/A+A/540/A133 {eta} Car emission spectrum (1700-10400{AA}) (Zethson+, 2012)
*================================================================================
*{eta} Carinae: linelist for the emission spectrum of the Weigelt blobs in the
*1700 to 10400{AA} wavelength region.
* Zethson T., Johansson S., Hartman H., Gull T.R.
* <Astron. Astrophys. 540, A133 (2012)>
* =2012A&A...540A.133Z
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'tablec1.dat' ! Identifications of 2500 emission lines in the
wavelength region 1700-10400{AA} from the STIS
spectra of the Weigelt blobs recorded in
March 1998 and February 1999
integer*4 nr__
parameter (nr__=2537) ! Number of records
character*103 ar__ ! Full-size record
real*8 lambdaO (nr__) ! (0.1nm) ? Observed wavelength (given in vacuum) (1)
integer*4 n_lambdaO (nr__) ! ? Last 2 digits (wihtout decimals) for
* wavelength interval
character*1 u_lambdaO (nr__) ! [?]
real*8 Int (nr__) ! ? Intensity (in relative units)
character*19 Line (nr__) ! Line identification
character*32 Trans (nr__) ! Transition
real*8 lambdaL (nr__) ! (0.1nm) ? Laboratory wavelength (given in vacuum) (1)
character*20 Com (nr__) ! Comments (2)
*Note (1): The identifications for the region 2424-2706{AA} are improved using
* the line list by Nielsen et al. (2007, Cat. J/ApJS/168/289) based on high
* resolution HST/STIS spectra. The identifications and laboratory wavelengths
* are retrieved from the Kurucz database (Kurucz, 2001,
* http://cfaku5.harvard.edu/atoms.html). The laboratory wavelengths for parity
* forbidden lines are Ritz wavelengths derived from energy levels in the NIST
* Atomic Spectra Database (2006).
*Note (2): Comments used as follows:
* Not in 98 = The feature is not present in the 1998 observation
* Not in 99 = The feature is not present in the 1999 observation
* Ly{alpha} = Primary H Ly{alpha} pumped fluorescence transition
* Ly{alpha} sec. = Secondary H Ly{alpha} pumped fluorescence transition
* 4p-4s = A 4p-4s transition, discussed in section 5.5
* Si III] = Fluorescence line pumped by Si III
* (Hartman & Johansson, 2000A&A...359..627H)
* He II = Fluorescence line pumped by He II
* (Hartman & Johansson, 2000A&A...359..627H)
* N IV] = Fluorescence line pumped by N IV]
* (Hartman & Johansson, 2000A&A...359..627H)
* rd_sh = red shoulder due to extended stellar wind is noticeable out
* to +400km/s
* bl_sh = blue shoulder due to extended stellar wind is noticeable
* out to -400km/s
* ? = the feature is weak and may not be a true emission line
* ?id = The identification is regarded as uncertain
* ?Eu = the upper level has an excitation energy >10eV, and the excitation
* mechanism is questionable
* ?wl = Plausible identification, but the radial velocity differs from
* the mean, -45km/s, by >15km/s
C=============================================================================
C Loading file 'tablec1.dat' ! Identifications of 2500 emission lines in the
* wavelength region 1700-10400{AA} from the STIS
* spectra of the Weigelt blobs recorded in
* March 1998 and February 1999
C Format for file interpretation
1 format(F8.2,1X,I2,A1,1X,F7.1,1X,A19,1X,A32,1X,F8.2,1X,A20)
C Effective file loading
open(unit=1,status='old',file=
+'tablec1.dat')
write(6,*) '....Loading file: tablec1.dat'
do i__=1,2537
read(1,'(A103)')ar__
read(ar__,1)
+ lambdaO(i__),n_lambdaO(i__),u_lambdaO(i__),Int(i__),Line(i__),
+ Trans(i__),lambdaL(i__),Com(i__)
if(ar__(1:8) .EQ. '') lambdaO(i__) = rNULL__
if(ar__(10:11) .EQ. '') n_lambdaO(i__) = iNULL__
if(ar__(14:20) .EQ. '') Int(i__) = rNULL__
if(ar__(75:82) .EQ. '') lambdaL(i__) = rNULL__
c ..............Just test output...........
write(6,1)
+ lambdaO(i__),n_lambdaO(i__),u_lambdaO(i__),Int(i__),Line(i__),
+ Trans(i__),lambdaL(i__),Com(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end