Conversion of standardized ReadMe file for
file /./ftp/cats/J/AZh/76/604 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-16
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/AZh/76/604 Spectrophotometry of S and carbon stars (Tereshchenko, 1999)
*================================================================================
*Spectrophotometry of three S stars and thirteen carbon N stars.
* Tereshchenko V.M.
* <Astron. Zh. 76, 604 (1999)>
* =1999AZh....76..604T
* =1999ARep...43..526T
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'stars.dat' ! Main photometry and spectral characteristics
integer*4 nr__
parameter (nr__=16) ! Number of records
character*114 ar__ ! Full-size record
C J2000.0 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg (nr__) ! (deg) Right Ascension J2000.0
real*8 DEdeg (nr__) ! (deg) Declination J2000.0
C ---------------------------------- ! (position vector(s) in degrees)
character*1 Type (nr__) ! [CS] C: carbon star, S: S star
integer*4 RAh (nr__) ! (h) Right ascension (J2000.0)
integer*4 RAm (nr__) ! (min) Right ascension (J2000.0)
real*4 RAs (nr__) ! (s) Right ascension (J2000.0)
character*1 DE_ (nr__) ! Declination sign (J2000.0)
integer*4 DEd (nr__) ! (deg) Declination (J2000.0)
integer*4 DEm (nr__) ! (arcmin) Declination (J2000.0)
integer*4 DEs (nr__) ! (arcsec) Declination (J2000.0)
integer*4 HR (nr__) ! HR (Cat. <V/50>) number
integer*4 HD (nr__) ! HD (Cat. <III/135>) number
character*11 Name (nr__) ! Star Name
real*4 Vmag (nr__) ! (mag) V magnitude
real*4 B_V (nr__) ! (mag) B-V colour index
real*4 U_B (nr__) ! (mag) ? U-B colour index
character*4 SpType (nr__) ! Spectral type
character*3 VarType (nr__) ! Type of variability
character*41 Obs (nr__) ! Observation dates
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Energy distributions of S and carbon stars
integer*4 nr__1
parameter (nr__1=88) ! Number of records
character*100 ar__1 ! Full-size record
integer*4 lambda (nr__1) ! (0.1nm) Spectral line wavelength
integer*4 BDCam (nr__1) ! (10nW/m2/cm) Energy distribution for BD Cam (1)
integer*4 omiOri (nr__1) ! (10nW/m2/cm) Energy distribution for omicron Ori (1)
integer*4 chiCyg (nr__1) ! (10nW/m2/cm) Energy distribution for chi Cyg (1)
integer*4 RLep (nr__1) ! (10nW/m2/cm) Energy distribution for R Lep (1)
integer*4 WOri (nr__1) ! (10nW/m2/cm) ? Energy distribution for W Ori (1)
integer*4 YTau (nr__1) ! (10nW/m2/cm) Energy distribution for Y Tau (1)
integer*4 BLOri (nr__1) ! (10nW/m2/cm) Energy distribution for BL Ori (1)
integer*4 UUAur (nr__1) ! (10nW/m2/cm) Energy distribution for UU Aur (1)
integer*4 XCnc (nr__1) ! (10nW/m2/cm) Energy distribution for X Cnc (1)
integer*4 UHya (nr__1) ! (10nW/m2/cm) Energy distribution for U Hya (1)
integer*4 VYUMa (nr__1) ! (10nW/m2/cm) Energy distribution for VY UMa (1)
integer*4 YCVn (nr__1) ! (10nW/m2/cm) Energy distribution for Y CVn (1)
integer*4 SSct (nr__1) ! (10nW/m2/cm) ? Energy distribution for S Sct (1)
integer*4 VAql (nr__1) ! (10nW/m2/cm) Energy distribution for V Aql (1)
integer*4 v460Cyg (nr__1) ! (10nW/m2/cm) Energy distribution for v460 Cyg (1)
integer*4 v19Psc (nr__1) ! (10nW/m2/cm) Energy distribution for 19 Psc (1)
*Note (1): 10nW/m2/cm=10-5.erg/(cm2.s.cm)
C=============================================================================
C Loading file 'stars.dat' ! Main photometry and spectral characteristics
C Format for file interpretation
1 format(
+ A1,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,2X,I4,2X,I6,1X,
+ A11,1X,F4.2,1X,F4.2,1X,F4.2,1X,A4,1X,A3,1X,A41)
C Effective file loading
open(unit=1,status='old',file=
+'stars.dat')
write(6,*) '....Loading file: stars.dat'
do i__=1,16
read(1,'(A114)')ar__
read(ar__,1)
+ Type(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),HR(i__),HD(i__),Name(i__),Vmag(i__),
+ B_V(i__),U_B(i__),SpType(i__),VarType(i__),Obs(i__)
if(ar__(60:63) .EQ. '') U_B(i__) = rNULL__
RAdeg(i__) = rNULL__
DEdeg(i__) = rNULL__
c Derive coordinates RAdeg and DEdeg from input data
c (RAdeg and DEdeg are set to rNULL__ when unknown)
if(RAh(i__) .GT. -180) RAdeg(i__)=RAh(i__)*15.
if(RAm(i__) .GT. -180) RAdeg(i__)=RAdeg(i__)+RAm(i__)/4.
if(RAs(i__) .GT. -180) RAdeg(i__)=RAdeg(i__)+RAs(i__)/240.
if(DEd(i__) .GE. 0) DEdeg(i__)=DEd(i__)
if(DEm(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEm(i__)/60.
if(DEs(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEs(i__)/3600.
if(DE_(i__).EQ.'-'.AND.DEdeg(i__).GE.0) DEdeg(i__)=-DEdeg(i__)
c ..............Just test output...........
write(6,1)
+ Type(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),HR(i__),HD(i__),Name(i__),Vmag(i__),
+ B_V(i__),U_B(i__),SpType(i__),VarType(i__),Obs(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3.dat' ! Energy distributions of S and carbon stars
C Format for file interpretation
2 format(
+ I4,2X,I4,2X,I4,2X,I4,2X,I4,2X,I4,2X,I4,2X,I4,2X,I4,2X,I4,2X,
+ I4,2X,I4,2X,I4,2X,I4,2X,I4,2X,I4,2X,I4)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,88
read(1,'(A100)')ar__1
read(ar__1,2)
+ lambda(i__),BDCam(i__),omiOri(i__),chiCyg(i__),RLep(i__),
+ WOri(i__),YTau(i__),BLOri(i__),UUAur(i__),XCnc(i__),UHya(i__),
+ VYUMa(i__),YCVn(i__),SSct(i__),VAql(i__),v460Cyg(i__),
+ v19Psc(i__)
if(ar__1(31:34) .EQ. '') WOri(i__) = iNULL__
if(ar__1(79:82) .EQ. '') SSct(i__) = iNULL__
c ..............Just test output...........
write(6,2)
+ lambda(i__),BDCam(i__),omiOri(i__),chiCyg(i__),RLep(i__),
+ WOri(i__),YTau(i__),BLOri(i__),UUAur(i__),XCnc(i__),UHya(i__),
+ VYUMa(i__),YCVn(i__),SSct(i__),VAql(i__),v460Cyg(i__),
+ v19Psc(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end