Conversion of standardized ReadMe file for
file /./ftp/cats/III/92 into FORTRAN code for reading data files line by line.
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. III/92 A Library of Stellar Spectra (Jacoby+ 1984)
*================================================================================
*A Library of Stellar Spectra
* Jacoby G.H., Hunter D.A., Christian C.A.
* <Astrophys. J. Suppl. Ser., 56, 257 (1984)>
* =1984ApJS...56..257J
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'stars.dat' ! Information on each star
integer*4 nr__
parameter (nr__=161) ! Number of records
character*100 ar__ ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg ! (deg) Right Ascension J2000
real*8 DEdeg ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
character*1 f_Name ! [*] Name corrected from original version
character*10 Name ! *Star identification (HD, BD, SAO, misc.)
character*4 SpT ! Adopted spectral type.
character*3 Lum ! Adopted luminosity class
character*2 Sp1 ! Spectral type from lit. if different
character*3 Lum1 ! Luminosity class from literature if different
real*4 E_B_V ! (mag) *Derived color excess E(B-V)
real*4 v_U_B_s ! (mag) U-B color synthesized from the spectrum.
real*4 v_B_V_s ! (mag) B-V color synthesized from the spectrum.
real*4 v_U_B_0 ! (mag) Dereddened color derived from (U-B)s
real*4 v_B_V_0 ! Dereddened color derived from (B-V)s
real*4 U_B ! (mag) ? U-B color taken from the literature.
real*4 B_V ! (mag) ? B-V color taken from the literature.
real*8 lambda1 ! (0.1nm) [3510] Wavelength of first pixel
real*4 Dlambda ! (0.1nm) [1.40] Wavelength increment per pixel
integer*4 RAh ! (h) *Right Ascension J2000 (hours)
integer*4 RAm ! (min) *Right Ascension J2000 (minutes)
real*4 RAs ! (s) *Right Ascension J2000 (seconds)
character*1 DE_ ! *Declination J2000 (sign)
integer*4 DEd ! (deg) *Declination J2000 (degrees)
integer*4 DEm ! (arcmin) *Declination J2000 (minutes)
real*4 DEs ! (arcsec) *Declination J2000 (seconds)
*Note on E(B-V):
* Derived color excess, E(B-V), used to to deredden the spectrum.
*Note on Name, n_Name, RAh, RAm, RAs, DE-, DEd, DEm, DEs:
* Four stars (# 47, 94, 124, 128) have an asterisk (*) in the first
* byte, corresponding to the difficulties to identify them; for more
* details, see the "History" section below.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'fluxes.dat' ! The Library of Stellar Spectra, flux data
integer*4 nr__1
parameter (nr__1=64400) ! Number of records
character*80 ar__1 ! Full-size record
character*10 Name_1 ! Star identification from headers.dat
real*4 F_i (7) ! (cW/m2/nm) *? Flux values F(i) in erg/cm^2^/s/{AA}
*Note on F(i):
* Flux values F(i) in erg/cm2/s/Angstrom at wavelengths:
* lambda(i) = lambda1 + (i-1+[7*(L-1)])*Dlambda
* where L is the number of the line for the star of interest. There are
* 400 lines of fluxes for each star. Hence, L is the line number in the
* file, modulo 400.
*
* In the final record for each star, the seventh flux on the record
* appears blank.
C=============================================================================
C Loading file 'stars.dat' ! Information on each star
C Format for file interpretation
1 format(
+ A1,A10,1X,A4,A3,1X,A2,1X,A3,1X,F4.2,1X,F4.2,1X,F4.2,1X,F5.2,
+ 1X,F4.2,1X,F4.2,1X,F4.2,1X,F7.2,1X,F4.2,1X,I2,1X,I2,1X,F5.2,
+ 2X,A1,I2,1X,I2,1X,F4.1)
C Effective file loading
open(unit=1,status='old',file=
+'stars.dat')
write(6,*) '....Loading file: stars.dat'
do i__=1,161
read(1,'(A100)')ar__
read(ar__,1)
+ f_Name,Name,SpT,Lum,Sp1,Lum1,E_B_V,v_U_B_s,v_B_V_s,v_U_B_0,
+ v_B_V_0,U_B,B_V,lambda1,Dlambda,RAh,RAm,RAs,DE_,DEd,DEm,DEs
if(ar__(54:57) .EQ. '') U_B = rNULL__
if(ar__(59:62) .EQ. '') B_V = rNULL__
RAdeg = rNULL__
DEdeg = rNULL__
c Derive coordinates RAdeg and DEdeg from input data
c (RAdeg and DEdeg are set to rNULL__ when unknown)
if(RAh .GT. -180) RAdeg=RAh*15.
if(RAm .GT. -180) RAdeg=RAdeg+RAm/4.
if(RAs .GT. -180) RAdeg=RAdeg+RAs/240.
if(DEd .GE. 0) DEdeg=DEd
if(DEm .GE. 0) DEdeg=DEdeg+DEm/60.
if(DEs .GE. 0) DEdeg=DEdeg+DEs/3600.
if(DE_.EQ.'-'.AND.DEdeg.GE.0) DEdeg=-DEdeg
c ..............Just test output...........
write(6,1)
+ f_Name,Name,SpT,Lum,Sp1,Lum1,E_B_V,v_U_B_s,v_B_V_s,v_U_B_0,
+ v_B_V_0,U_B,B_V,lambda1,Dlambda,RAh,RAm,RAs,DE_,DEd,DEm,DEs
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'fluxes.dat' ! The Library of Stellar Spectra, flux data
C Format for file interpretation
2 format(A10,7E10.3)
C Effective file loading
open(unit=1,status='old',file=
+'fluxes.dat')
write(6,*) '....Loading file: fluxes.dat'
do i__=1,64400
read(1,'(A80)')ar__1
read(ar__1,2)Name_1,(F_i(j__,),j__=1,7)
if(ar__1(11:80) .EQ. '') F_i = rNULL__
c ..............Just test output...........
write(6,2)Name_1,(F_i(j__,),j__=1,7)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end