Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJS/171/249 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. J/ApJS/171/249 Ultraviolet Spectral Atlas of VV Cephei (Bauer+, 2007)
*================================================================================
*An ultraviolet spectral atlas of VV Cephei during total eclipse.
* Bauer W.H., Bennett P.D., Brown A.
* <Astrophys. J. Suppl. Ser., 171, 249-259 (2007)>
* =2007ApJS..171..249B
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Emission lines selected from the database
integer*4 nr__
parameter (nr__=5693) ! Number of records
character*67 ar__ ! Full-size record
real*8 Wave ! (0.1nm) Wavelength in Angstroms
character*6 Ion ! Ion designation (G1)
real*4 LowE ! (eV) Lower energy level
real*4 UpE ! (eV) Upper energy level
real*4 log_gf ! ([-]) Log of the oscillator strength
real*4 LStr ! The "line strength" quantity (2)
character*1 u_LStr ! Uncertainty flag on LStr (3)
character*8 Multi ! Multiplet number (if available)
character*8 LowT ! The lower term designation
character*9 UpT ! The upper term designation
*Note (2): The difference between the line's log(gf) and the minimum log(gf)
* included for that upper level. If this quantity is negative, the
* transition was included because its log(gf) was within 1.0 of the
* minimum log(gf) for that upper level, and could explain a feature that
* would otherwise not have an identification.
*Note (3): the colon (:) indicates too few lines from that upper level for
* the strength quantity to be useful when comparing with line strengths
* from other elements or levels.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table5.dat' ! Unblended lines
integer*4 nr__1
parameter (nr__1=469) ! Number of records
character*51 ar__1 ! Full-size record
real*8 Wave_1 ! (0.1nm) Wavelength in Angstroms
character*1 f_Wave ! [b] Flag on Wave (2)
character*6 Ion_1 ! Ion designation (G1)
real*4 LowE_1 ! (eV) Lower energy level
real*4 UpE_1 ! (eV) Upper energy level
real*4 log_gf_1 ! ([-]) Log of the oscillator strength
character*8 Multi_1 ! Multiplet number (if available)
real*4 PFlux ! (10-14W/m2/nm) Peak flux (3)
character*1 f_PFlux ! [c] Possible circumstellar absorption (4)
*Note (2): 'b' indicates a line unblended for 100km/s on either side.
*Note (3): In units of 10^-12^erg/cm^2^/s/Angstrom.
* The continuum has not been subtracted.
*Note (4): 'c' indicates that the peak flux might be affected by
* circumstellar absorption.
C=============================================================================
C Loading file 'table3.dat' ! Emission lines selected from the database
C Format for file interpretation
1 format(
+ F8.3,1X,A6,1X,F4.2,1X,F5.2,1X,F5.2,1X,F5.2,A1,1X,A8,1X,A8,1X,
+ A9)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,5693
read(1,'(A67)')ar__
read(ar__,1)
+ Wave,Ion,LowE,UpE,log_gf,LStr,u_LStr,Multi,LowT,UpT
c ..............Just test output...........
write(6,1)
+ Wave,Ion,LowE,UpE,log_gf,LStr,u_LStr,Multi,LowT,UpT
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table5.dat' ! Unblended lines
C Format for file interpretation
2 format(
+ F8.3,1X,A1,1X,A6,1X,F4.2,1X,F5.2,1X,F5.2,1X,A8,1X,F5.2,1X,A1)
C Effective file loading
open(unit=1,status='old',file=
+'table5.dat')
write(6,*) '....Loading file: table5.dat'
do i__=1,469
read(1,'(A51)')ar__1
read(ar__1,2)
+ Wave_1,f_Wave,Ion_1,LowE_1,UpE_1,log_gf_1,Multi_1,PFlux,
+ f_PFlux
c ..............Just test output...........
write(6,2)
+ Wave_1,f_Wave,Ion_1,LowE_1,UpE_1,log_gf_1,Multi_1,PFlux,
+ f_PFlux
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end