Conversion of standardized ReadMe file for
file /./ftp/cats/J/AZh/77/619 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_1.5, on 2013-May-20
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__
ter (rNULL__=-1.e37) ! NULL real number
parameter (iNULL__=-2147483647) ! NULL int number
C=============================================================================
Cat. J/AZh/77/619 Energy distributions in giants and supergiants (Knyazeva+, 2000)
*================================================================================
*The normal energy distributions in stellar spectra: giants and supergiants.
* Knyazeva L.N., Kharitonov A.V.
* <Astron. Zh. 77, 619 (2000)>
* =2000AZh....77..619K
* =2000ARep...44..548K
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Giants used to derive the normal energy distributions
integer*4 nr__
parameter (nr__=56) ! Number of records
character*72 ar__ ! Full-size record
real*8 RA_ ! (deg) Right Ascension J2000
real*8 Dec ! (deg) Declination J2000
character*5 SpType ! MK Spectral type
character*9 Name ! Name of the star
character*1 n_Name ! [*] *: star is considered as unreddened
integer*4 RAh ! (h) Right ascension (J2000)
integer*4 RAm ! (min) Right ascension (J2000)
real*8 RAs ! (s) Right ascension (J2000)
character*1 DE_ ! Declination sign (J2000)
integer*4 DEd ! (deg) Declination (J2000)
integer*4 DEm ! (arcmin) Declination (J2000)
real*4 DEs ! (arcsec) Declination (J2000)
real*4 Vmag ! (mag) V magnitude
real*4 B_V ! (mag) B-V color index
real*4 Plx ! (arcsec) ? Trigonometric parallax
integer*4 GLAT ! (deg) Galactic latitude
character*5 Ref ! References to spectrophotometric data (G1)
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Supergiants used to derive the normal energy
distributions
integer*4 nr__1
parameter (nr__1=22) ! Number of records
character*78 ar__1 ! Full-size record
real*8 RA__1 ! (deg) Right Ascension J2000
real*8 Dec_1 ! (deg) Declination J2000
character*7 SpType_1 ! MK Spectral type
character*9 Name_1 ! Name of the star
character*1 n_Name_1 ! [*] *: star is considered as unreddened
integer*4 RAh_1 ! (h) Right ascension (J2000)
integer*4 RAm_1 ! (min) Right ascension (J2000)
real*8 RAs_1 ! (s) Right ascension (J2000)
character*1 DE__1 ! Declination sign (J2000)
integer*4 DEd_1 ! (deg) Declination (J2000)
integer*4 DEm_1 ! (arcmin) Declination (J2000)
real*4 DEs_1 ! (arcsec) Declination (J2000)
real*4 Vmag_1 ! (mag) V magnitude
real*4 B_V_1 ! (mag) B-V color index
real*4 Plx_1 ! (arcsec) ? Trigonometric parallax
integer*4 GLAT_1 ! (deg) Galactic latitude
real*4 E_B_V ! (mag) ? Color excess
character*5 Ref_1 ! References to spectrophotometric data (G1)
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table5.dat' ! Normal color indices of stars in the WBVR
(Kornilov et al., 1991, Tr. Gos. Astron. Inst.
Shternberga 63) system
integer*4 nr__2
parameter (nr__2=81) ! Number of records
character*27 ar__2 ! Full-size record
character*8 SpType_2 ! MK Spectral type
real*4 v_B_V_0 ! (mag) (B-V)0 color index
real*4 v_W_B_0 ! (mag) (W-B)0 color index
C=============================================================================
C Loading file 'table1.dat' ! Giants used to derive the normal energy distributions
C Format for file interpretation
1 format(
+ A5,1X,A9,A1,1X,I2,1X,I2,1X,F7.4,1X,A1,I2,1X,I2,1X,F6.3,1X,
+ F4.2,1X,F5.2,1X,F5.3,2X,I3,1X,A5)
C Effective file loading
open(unit=1,file='table1.dat', status='old')
write(6,*) '....Loading file: table1.dat'
do i__=1,56
read(1,'(A72)')ar__
read(ar__,1)
+ SpType,Name,n_Name,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Vmag,B_V,Plx,
+ GLAT,Ref
if(ar__(57:61) .EQ. '') Plx = rNULL__
c Derive coordinates RA_ and Dec from input data
c (RA_ and Dec are set to rNULL_ when unknown)
RA_ = RAh
if(RAh .GE. 0) RA_=RAh*15.
if(RAm .GE. 0) RA_=RA_+RAm/4.
if(RAs .GE. 0) RA_=RA_+RAs/240.
Dec = DEd
if(DEm .GE. 0) Dec=Dec+DEm/60.
if(DEs .GE. 0) Dec=Dec+DEs/3600.
if(DE_.EQ.'-'.AND.Dec.GE.0) Dec=-Dec
c ..............Just test output...........
write(6,1)
+ SpType,Name,n_Name,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Vmag,B_V,Plx,
+ GLAT,Ref
write(6,'(6H Pos: 2F8.4)') RA_,Dec
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! Supergiants used to derive the normal energy
* distributions
C Format for file interpretation
2 format(
+ A7,1X,A9,A1,I2,1X,I2,1X,F7.4,1X,A1,I2,1X,I2,1X,F6.3,1X,F4.2,
+ 1X,F5.2,1X,F5.3,1X,I3,1X,F4.2,2X,A5)
C Effective file loading
open(unit=1,file='table2.dat', status='old')
write(6,*) '....Loading file: table2.dat'
do i__=1,22
read(1,'(A78)')ar__1
read(ar__1,2)
+ SpType_1,Name_1,n_Name_1,RAh_1,RAm_1,RAs_1,DE__1,DEd_1,DEm_1,
+ DEs_1,Vmag_1,B_V_1,Plx_1,GLAT_1,E_B_V,Ref_1
if(ar__1(58:62) .EQ. '') Plx_1 = rNULL__
if(ar__1(68:71) .EQ. '') E_B_V = rNULL__
c Derive coordinates RA__1 and Dec_1 from input data
c (RA__1 and Dec_1 are set to rNULL_ when unknown)
RA__1 = RAh_1
if(RAh_1 .GE. 0) RA__1=RAh_1*15.
if(RAm_1 .GE. 0) RA__1=RA__1+RAm_1/4.
if(RAs_1 .GE. 0) RA__1=RA__1+RAs_1/240.
Dec_1 = DEd_1
if(DEm_1 .GE. 0) Dec_1=Dec_1+DEm_1/60.
if(DEs_1 .GE. 0) Dec_1=Dec_1+DEs_1/3600.
if(DE__1.EQ.'-'.AND.Dec_1.GE.0) Dec_1=-Dec_1
c ..............Just test output...........
write(6,2)
+ SpType_1,Name_1,n_Name_1,RAh_1,RAm_1,RAs_1,DE__1,DEd_1,DEm_1,
+ DEs_1,Vmag_1,B_V_1,Plx_1,GLAT_1,E_B_V,Ref_1
write(6,'(6H Pos: 2F8.4)') RA__1,Dec_1
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table5.dat' ! Normal color indices of stars in the WBVR
* (Kornilov et al., 1991, Tr. Gos. Astron. Inst.
* Shternberga 63) system
C Format for file interpretation
3 format(A8,1X,F6.3,2X,F6.3)
C Effective file loading
open(unit=1,file='table5.dat', status='old')
write(6,*) '....Loading file: table5.dat'
do i__=1,81
read(1,'(A27)')ar__2
read(ar__2,3)SpType_2,v_B_V_0,v_W_B_0
c ..............Just test output...........
write(6,3)SpType_2,v_B_V_0,v_W_B_0
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end