Conversion of standardized ReadMe file for
file /./ftp/cats/J/MNRAS/437/532 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 2026-Jun-08
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/MNRAS/437/532 VY CMa molecular line spectra (Matsuura+, 2014)
*================================================================================
*Herschel SPIRE and PACS observations of the red supergiant VY CMa:
*analysis of the molecular line spectra.
* Matsuura M., Yates J.A., Barlow M.J., Swinyard B.M., Royer P.,
* Cernicharo J., Decin L., Wesson R., Polehampton E.T., Blommaert J.A.D.L.,
* Groenewegen M.A.T., Van De Steene G.C., van Hoof P.A.M.
* <Mon. Not. R. Astron. Soc., 437, 532-546 (2014)>
* =2014MNRAS.437..532M (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'tablea2.dat' ! VY CMa line fluxes and identifications (IDs) in
the SPIRE FTS SLW spectra
integer*4 nr__
parameter (nr__=170) ! Number of records
character*121 ar__ ! Full-size record
real*4 nuobs1 ! (cm-1) ? Observed wavenumber (OD123)
real*4 F1 ! (10-18W/m2) ? VY CMa line flux (OD123)
real*4 e_F1 ! (10-18W/m2) ? rms uncertainty on F1 (1)
real*4 nuobs2 ! (cm-1) ? Observed wavenumber (OD317)
character*1 u_nuobs2 ! [?] Uncertainty flag on nuobs2
real*4 e_nuobs2 ! (cm-1) ? rms uncertainty on nuobs2 (1)
real*4 F2 ! (10-18W/m2) ? VY CMa line flux (OD317)
real*4 e_F2 ! (10-18W/m2) ? rms uncertainty on F2
character*1 n_nu0 ! [+] for blend (2)
real*4 nu0 ! (cm-1) ? Vacuum wavenumber
character*1 u_nu0 ! [?] Uncertainty flag on nu0
real*8 Fnu0 ! (GHz) ? Vacuum frequency
real*4 lambda0 ! (um) ? Vacuum wavelength
character*1 u_lambda0 ! [?] Uncertainty flag on lambda0
character*10 Species ! Species
character*38 Trans ! Transition (3)
*Note (1): The listed uncertainties for the line fluxes are those from the line
* fitting.
*Note (2): An ID row beginning with a '+' indicates that the line is blended
* with that on the row above.
*Note (3): The quantum numbers are J except where stated.
* H2O transitions are given in the format J_Ka'_Kc'-J_Ka_Kc.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'tablea3.dat' ! VY CMa: Line fluxes and identifications in the
SPIRE FTS SSW spectra
integer*4 nr__1
parameter (nr__1=288) ! Number of records
character*121 ar__1 ! Full-size record
real*4 nuobs1_1 ! (cm-1) ? Observed wavenumber (OD123)
real*4 F1_1 ! (10-18W/m2) ? VY CMa line flux (OD123)
real*4 e_F1_1 ! (10-18W/m2) ? rms uncertainty on F1 (1)
real*4 nuobs2_1 ! (cm-1) ? Observed wavenumber (OD317)
character*1 u_nuobs2_1 ! [?] Uncertainty flag on nuobs2
real*4 e_nuobs2_1 ! (cm-1) ? rms uncertainty on nuobs2 (1)
real*4 F2_1 ! (10-18W/m2) ? VY CMa line flux (OD317)
real*4 e_F2_1 ! (10-18W/m2) ? rms uncertainty on F2
character*1 n_nu0_1 ! [+] for blend (2)
real*4 nu0_1 ! (cm-1) ? Vacuum wavenumber
character*1 u_nu0_1 ! [?] Uncertainty flag on nu0
real*8 Fnu0_1 ! (GHz) ? Vacuum frequency
real*4 lambda0_1 ! (um) ? Vacuum wavelength
character*1 u_lambda0_1 ! [?] Uncertainty flag on lambda0
character*10 Species_1 ! Species
character*38 Trans_1 ! Transition (3)
*Note (1): The listed uncertainties for the line fluxes are those from the line
* fitting.
*Note (2): An ID row beginning with a '+' indicates that the line is blended
* with that on the row above.
*Note (3): The quantum numbers are J except where stated.
* H2O transitions are given in the format J_Ka'_Kc'-J_Ka_Kc.
C=============================================================================
C Loading file 'tablea2.dat' ! VY CMa line fluxes and identifications (IDs) in
* the SPIRE FTS SLW spectra
C Format for file interpretation
1 format(
+ F6.3,1X,F6.1,1X,F5.1,1X,F6.3,A1,1X,F5.3,1X,F6.1,1X,F5.1,1X,A1,
+ F6.3,A1,1X,F7.2,1X,F6.2,A1,1X,A10,1X,A38)
C Effective file loading
open(unit=1,status='old',file=
+'tablea2.dat')
write(6,*) '....Loading file: tablea2.dat'
do i__=1,170
read(1,'(A121)')ar__
read(ar__,1)
+ nuobs1,F1,e_F1,nuobs2,u_nuobs2,e_nuobs2,F2,e_F2,n_nu0,nu0,
+ u_nu0,Fnu0,lambda0,u_lambda0,Species,Trans
if(ar__(1:6) .EQ. '') nuobs1 = rNULL__
if(ar__(8:13) .EQ. '') F1 = rNULL__
if(ar__(15:19) .EQ. '') e_F1 = rNULL__
if(ar__(21:26) .EQ. '') nuobs2 = rNULL__
if(ar__(29:33) .EQ. '') e_nuobs2 = rNULL__
if(ar__(35:40) .EQ. '') F2 = rNULL__
if(ar__(42:46) .EQ. '') e_F2 = rNULL__
if(ar__(49:54) .EQ. '') nu0 = rNULL__
if(ar__(57:63) .EQ. '') Fnu0 = rNULL__
if(ar__(65:70) .EQ. '') lambda0 = rNULL__
c ..............Just test output...........
write(6,1)
+ nuobs1,F1,e_F1,nuobs2,u_nuobs2,e_nuobs2,F2,e_F2,n_nu0,nu0,
+ u_nu0,Fnu0,lambda0,u_lambda0,Species,Trans
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'tablea3.dat' ! VY CMa: Line fluxes and identifications in the
* SPIRE FTS SSW spectra
C Format for file interpretation
2 format(
+ F6.3,1X,F6.1,1X,F5.1,1X,F6.3,A1,1X,F5.3,1X,F6.1,1X,F5.1,1X,A1,
+ F6.3,A1,1X,F7.2,1X,F6.2,A1,1X,A10,1X,A38)
C Effective file loading
open(unit=1,status='old',file=
+'tablea3.dat')
write(6,*) '....Loading file: tablea3.dat'
do i__=1,288
read(1,'(A121)')ar__1
read(ar__1,2)
+ nuobs1_1,F1_1,e_F1_1,nuobs2_1,u_nuobs2_1,e_nuobs2_1,F2_1,
+ e_F2_1,n_nu0_1,nu0_1,u_nu0_1,Fnu0_1,lambda0_1,u_lambda0_1,
+ Species_1,Trans_1
if(ar__1(1:6) .EQ. '') nuobs1_1 = rNULL__
if(ar__1(8:13) .EQ. '') F1_1 = rNULL__
if(ar__1(15:19) .EQ. '') e_F1_1 = rNULL__
if(ar__1(21:26) .EQ. '') nuobs2_1 = rNULL__
if(ar__1(29:33) .EQ. '') e_nuobs2_1 = rNULL__
if(ar__1(35:40) .EQ. '') F2_1 = rNULL__
if(ar__1(42:46) .EQ. '') e_F2_1 = rNULL__
if(ar__1(49:54) .EQ. '') nu0_1 = rNULL__
if(ar__1(57:63) .EQ. '') Fnu0_1 = rNULL__
if(ar__1(65:70) .EQ. '') lambda0_1 = rNULL__
c ..............Just test output...........
write(6,2)
+ nuobs1_1,F1_1,e_F1_1,nuobs2_1,u_nuobs2_1,e_nuobs2_1,F2_1,
+ e_F2_1,n_nu0_1,nu0_1,u_nu0_1,Fnu0_1,lambda0_1,u_lambda0_1,
+ Species_1,Trans_1
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end