Conversion of standardized ReadMe file for
file /./ftp/cats/V/32A 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-18
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. V/32A Stars within 25 pc of the Sun (Woolley+ 1970)
*================================================================================
*Catalogue of Stars within 25 Parsecs of the Sun
* Woolley R.v.d.R., Epps E.A., Penston M.J., Pocock S.B.
* <Royal Obs. Ann. 5 (1970)>
* =1970ROAn....5....1W
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'catalog.dat' ! The catalogue of stars within 25pc
integer*4 nr__
parameter (nr__=2150) ! Number of records
character*145 ar__ ! Full-size record
C B1950 position composed of: RAh RAm RAs DE- DEd (Epoch=1950)
real*8 RAdeg ! (deg) Right Ascension B1950, Epoch=1950
real*8 DEdeg ! (deg) Declination B1950, Epoch=1950
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 Woolley ! *Sequence number
character*1 m_Woolley ! Component identification
integer*4 plx ! (mas) ?Parallax
character*2 e_plx ! (mas) *[S0-9 ]Probable error in plx
integer*4 n_plx ! ?Note:'8' if e_plx < 15%, '9' if e_plx < 10%
real*4 pmRA ! (s/yr) ?Proper motion in RA
real*8 pmDE ! (arcsec/yr) ?Proper motion in Dec
real*4 RVel ! (km/s) ?Radial velocity
character*1 n_RVel ! *[JV]Note on RV
integer*4 U ! (km/s) ?U component of space velocity
* (toward galactic centre)
integer*4 V ! (km/s) ?V component of space velocity
* (toward galactic rotation)
integer*4 W ! (km/s) ?W component of space velocity
* (toward North galactic pole)
integer*4 GCdist ! (10-4) *?Galactocentric distance in units of
* Sun's distance from the center
integer*4 e ! ?Box orbit eccentricity (1)
integer*4 i ! (10-4rad) ?Box orbit angle (highest inclination
* of the orbit) (1)
integer*4 LC_Code ! *?Luminosity class code
character*3 SpType ! Spectral type
character*1 r_SpType ! *[124] Coded source of spectral type
real*4 Mag ! (mag) [-2/19]? Magnitude m(v) or m(pg) (see n_Mag)
character*1 n_Mag ! *[JPV]Magnitude code
real*4 B_V ! (mag) ?B-V color
real*4 U_B ! (mag) ?U-B color
real*4 Mv ! (mag) *?Absolute visual magnitude
integer*4 RA1900h ! (h) ?Hours RA, equinox B1900, epoch 1900.0
integer*4 RA1900dm ! (0.1min) ?Minutes RA, equinox B1900, epoch 1900.0
character*1 DE1900_ ! ?Sign Dec, equinox B1900, epoch 1900.0
integer*4 DE1900d ! (deg) ?Degrees Dec, equinox B1900, epoch 1900.0
integer*4 DE1900m ! (arcmin) ?Minutes Dec, equinox B1900, epoch 1900.0
integer*4 RAh ! (h) ?Right Ascension B1950, epoch 1950 (hours)
integer*4 RAm ! (min) ?Right Ascension B1950, epoch 1950 (minutes)
integer*4 RAs ! (s) ?Right Ascension B1950, epoch 1950 (seconds)
character*1 DE_ ! ?Declination B1950, epoch 1950 (sign)
integer*4 DEd ! (deg) ?Declination B1950, epoch 1950 (degrees)
integer*4 DEdm ! (0.1arcmin) ?Declination B1950, epoch 1950 (deci-minutes)
character*5 GCTP ! Gen. Cat. of Trigonometric Parallaxes <I/60>
integer*4 HD ! [1/290000]? Henry Draper Catalog (HD) number
character*10 DM ! Durchmusterung (BD, CD, or CP)
character*5 GCRV ! Gen. Cat. of Radial Velocities (GCRV) number
character*6 PM_Name ! Name from other proper-motion catalog
integer*4 HR ! ?Bright Star = Harvard Revised catalog <V.50>
character*3 Vys ! Number in red dwarf lists of Vyssotsky
character*1 Remark1 ! [23456789] First remark code (2)
character*1 Remark2 ! [23456789] Second remark code (2)
*Note on Woolley:
* Star sequence numbers less than 1000 are from Gliese (1957);
* new stars have a number > 9000; The Sun is #0 (and therefore lacks entries
* in fields such as the RA and Dec.
*Note on e_plx:
* "S" indicates spectroscopic parallax
*Note on n_RVel:
* J = combined components of binary
* V = variable velocity
*Note on GCdist:
* i.e GCdist represents parsecs if the Sun distance is 10kpc. See
* also in file "adc.doc"
*Note on LC_Code:
* 1 = I or c; 2 = II or c;
* 3 = III or g; 4 = IV or sg;
* 5 = V or d; 6 = VI or sd;
* 7 = D or wd.
* Intermediate classes have no codes, e.g. 4 is given for IV-V.
*Note on r_SpType:
* 1 if MK;
* 2 if combined MK type for multiple system;
* 4 if combined non-MK;
* blank if non-MK.
*Note on n_Mag:
* J = combined light for multiple system
* P = Mag indicates a photographic magnitude
* V = variable magnitude
*Note on Mv:
* Visual magnitude is reported to 0.01 mag if both probable error of
* parallax < 10% and V is given to 0.01 mag.
*Note (1): see details in file "adc.doc" or in the original publication.
*Note (2): the codes are
* 2 = spectroscopic binary
* 3 = spectroscopic triple
* 4 = unresolved double, unknown nature
* 5 = UV Ceti flare star
* 6 = eclipsing binary
* 7 = semi-regular variable
* 8 = astrometric binary
* 9 = planetary nebula
C=============================================================================
C Loading file 'catalog.dat' ! The catalogue of stars within 25pc
C Format for file interpretation
1 format(
+ I4,A1,I3,A2,I1,F6.4,F7.3,F6.1,A1,I4,I4,I4,I5,I4,I4,I1,A3,A1,
+ F5.2,A1,F5.2,F5.2,F5.2,I2,I3,A1,I2,I2,I2,I2,I2,A1,I2,I3,A5,I6,
+ A10,A5,A6,I4,A3,A1,A1)
C Effective file loading
open(unit=1,status='old',file=
+'catalog.dat')
write(6,*) '....Loading file: catalog.dat'
do i__=1,2150
read(1,'(A145)')ar__
read(ar__,1)
+ Woolley,m_Woolley,plx,e_plx,n_plx,pmRA,pmDE,RVel,n_RVel,U,V,W,
+ GCdist,e,i,LC_Code,SpType,r_SpType,Mag,n_Mag,B_V,U_B,Mv,
+ RA1900h,RA1900dm,DE1900_,DE1900d,DE1900m,RAh,RAm,RAs,DE_,DEd,
+ DEdm,GCTP,HD,DM,GCRV,PM_Name,HR,Vys,Remark1,Remark2
if(ar__(6:8) .EQ. '') plx = iNULL__
if(ar__(11:11) .EQ. '') n_plx = iNULL__
if(ar__(12:17) .EQ. '') pmRA = rNULL__
if(ar__(18:24) .EQ. '') pmDE = rNULL__
if(ar__(25:30) .EQ. '') RVel = rNULL__
if(ar__(32:35) .EQ. '') U = iNULL__
if(ar__(36:39) .EQ. '') V = iNULL__
if(ar__(40:43) .EQ. '') W = iNULL__
if(ar__(44:48) .EQ. '') GCdist = iNULL__
if(ar__(49:52) .EQ. '') e = iNULL__
if(ar__(53:56) .EQ. '') i = iNULL__
if(ar__(57:57) .EQ. '') LC_Code = iNULL__
if(ar__(62:66) .EQ. '') Mag = rNULL__
if(ar__(68:72) .EQ. '') B_V = rNULL__
if(ar__(73:77) .EQ. '') U_B = rNULL__
if(ar__(78:82) .EQ. '') Mv = rNULL__
if(ar__(83:84) .EQ. '') RA1900h = iNULL__
if(ar__(85:87) .EQ. '') RA1900dm = iNULL__
if(ar__(89:90) .EQ. '') DE1900d = iNULL__
if(ar__(91:92) .EQ. '') DE1900m = iNULL__
if(ar__(93:94) .EQ. '') RAh = iNULL__
if(ar__(95:96) .EQ. '') RAm = iNULL__
if(ar__(97:98) .EQ. '') RAs = iNULL__
if(ar__(100:101) .EQ. '') DEd = iNULL__
if(ar__(102:104) .EQ. '') DEdm = iNULL__
if(ar__(110:115) .EQ. '') HD = iNULL__
if(ar__(137:140) .EQ. '') HR = iNULL__
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(DE_.EQ.'-'.AND.DEdeg.GE.0) DEdeg=-DEdeg
c ..............Just test output...........
write(6,1)
+ Woolley,m_Woolley,plx,e_plx,n_plx,pmRA,pmDE,RVel,n_RVel,U,V,W,
+ GCdist,e,i,LC_Code,SpType,r_SpType,Mag,n_Mag,B_V,U_B,Mv,
+ RA1900h,RA1900dm,DE1900_,DE1900d,DE1900m,RAh,RAm,RAs,DE_,DEd,
+ DEdm,GCTP,HD,DM,GCRV,PM_Name,HR,Vys,Remark1,Remark2
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end