Conversion of standardized ReadMe file for
file /./ftp/cats/V/32A 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-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 (nr__) ! (deg) Right Ascension B1950, Epoch=1950
real*8 DEdeg (nr__) ! (deg) Declination B1950, Epoch=1950
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 Woolley (nr__) ! *Sequence number
character*1 m_Woolley (nr__) ! Component identification
integer*4 plx (nr__) ! (mas) ?Parallax
character*2 e_plx (nr__) ! (mas) *[S0-9 ]Probable error in plx
integer*4 n_plx (nr__) ! ?Note:'8' if e_plx < 15%, '9' if e_plx < 10%
real*4 pmRA (nr__) ! (s/yr) ?Proper motion in RA
real*8 pmDE (nr__) ! (arcsec/yr) ?Proper motion in Dec
real*4 RVel (nr__) ! (km/s) ?Radial velocity
character*1 n_RVel (nr__) ! *[JV]Note on RV
integer*4 U (nr__) ! (km/s) ?U component of space velocity
* (toward galactic centre)
integer*4 V (nr__) ! (km/s) ?V component of space velocity
* (toward galactic rotation)
integer*4 W (nr__) ! (km/s) ?W component of space velocity
* (toward North galactic pole)
integer*4 GCdist (nr__) ! (10-4) *?Galactocentric distance in units of
* Sun's distance from the center
integer*4 e (nr__) ! ?Box orbit eccentricity (1)
integer*4 i (nr__) ! (10-4rad) ?Box orbit angle (highest inclination
* of the orbit) (1)
integer*4 LC_Code (nr__) ! *?Luminosity class code
character*3 SpType (nr__) ! Spectral type
character*1 r_SpType (nr__) ! *[124] Coded source of spectral type
real*4 Mag (nr__) ! (mag) [-2/19]? Magnitude m(v) or m(pg) (see n_Mag)
character*1 n_Mag (nr__) ! *[JPV]Magnitude code
real*4 B_V (nr__) ! (mag) ?B-V color
real*4 U_B (nr__) ! (mag) ?U-B color
real*4 Mv (nr__) ! (mag) *?Absolute visual magnitude
integer*4 RA1900h (nr__) ! (h) ?Hours RA, equinox B1900, epoch 1900.0
integer*4 RA1900dm (nr__) ! (0.1min) ?Minutes RA, equinox B1900, epoch 1900.0
character*1 DE1900_ (nr__) ! ?Sign Dec, equinox B1900, epoch 1900.0
integer*4 DE1900d (nr__) ! (deg) ?Degrees Dec, equinox B1900, epoch 1900.0
integer*4 DE1900m (nr__) ! (arcmin) ?Minutes Dec, equinox B1900, epoch 1900.0
integer*4 RAh (nr__) ! (h) ?Right Ascension B1950, epoch 1950 (hours)
integer*4 RAm (nr__) ! (min) ?Right Ascension B1950, epoch 1950 (minutes)
integer*4 RAs (nr__) ! (s) ?Right Ascension B1950, epoch 1950 (seconds)
character*1 DE_ (nr__) ! ?Declination B1950, epoch 1950 (sign)
integer*4 DEd (nr__) ! (deg) ?Declination B1950, epoch 1950 (degrees)
integer*4 DEdm (nr__) ! (0.1arcmin) ?Declination B1950, epoch 1950 (deci-minutes)
character*5 GCTP (nr__) ! Gen. Cat. of Trigonometric Parallaxes <I/60>
integer*4 HD (nr__) ! [1/290000]? Henry Draper Catalog (HD) number
character*10 DM (nr__) ! Durchmusterung (BD, CD, or CP)
character*5 GCRV (nr__) ! Gen. Cat. of Radial Velocities (GCRV) number
character*6 PM_Name (nr__) ! Name from other proper-motion catalog
integer*4 HR (nr__) ! ?Bright Star = Harvard Revised catalog <V.50>
character*3 Vys (nr__) ! Number in red dwarf lists of Vyssotsky
character*1 Remark1 (nr__) ! [23456789] First remark code (2)
character*1 Remark2 (nr__) ! [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(i__),m_Woolley(i__),plx(i__),e_plx(i__),n_plx(i__),
+ pmRA(i__),pmDE(i__),RVel(i__),n_RVel(i__),U(i__),V(i__),
+ W(i__),GCdist(i__),e(i__),i(i__),LC_Code(i__),SpType(i__),
+ r_SpType(i__),Mag(i__),n_Mag(i__),B_V(i__),U_B(i__),Mv(i__),
+ RA1900h(i__),RA1900dm(i__),DE1900_(i__),DE1900d(i__),
+ DE1900m(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEdm(i__),GCTP(i__),HD(i__),DM(i__),GCRV(i__),PM_Name(i__),
+ HR(i__),Vys(i__),Remark1(i__),Remark2(i__)
if(ar__(6:8) .EQ. '') plx(i__) = iNULL__
if(ar__(11:11) .EQ. '') n_plx(i__) = iNULL__
if(ar__(12:17) .EQ. '') pmRA(i__) = rNULL__
if(ar__(18:24) .EQ. '') pmDE(i__) = rNULL__
if(ar__(25:30) .EQ. '') RVel(i__) = rNULL__
if(ar__(32:35) .EQ. '') U(i__) = iNULL__
if(ar__(36:39) .EQ. '') V(i__) = iNULL__
if(ar__(40:43) .EQ. '') W(i__) = iNULL__
if(ar__(44:48) .EQ. '') GCdist(i__) = iNULL__
if(ar__(49:52) .EQ. '') e(i__) = iNULL__
if(ar__(53:56) .EQ. '') i(i__) = iNULL__
if(ar__(57:57) .EQ. '') LC_Code(i__) = iNULL__
if(ar__(62:66) .EQ. '') Mag(i__) = rNULL__
if(ar__(68:72) .EQ. '') B_V(i__) = rNULL__
if(ar__(73:77) .EQ. '') U_B(i__) = rNULL__
if(ar__(78:82) .EQ. '') Mv(i__) = rNULL__
if(ar__(83:84) .EQ. '') RA1900h(i__) = iNULL__
if(ar__(85:87) .EQ. '') RA1900dm(i__) = iNULL__
if(ar__(89:90) .EQ. '') DE1900d(i__) = iNULL__
if(ar__(91:92) .EQ. '') DE1900m(i__) = iNULL__
if(ar__(93:94) .EQ. '') RAh(i__) = iNULL__
if(ar__(95:96) .EQ. '') RAm(i__) = iNULL__
if(ar__(97:98) .EQ. '') RAs(i__) = iNULL__
if(ar__(100:101) .EQ. '') DEd(i__) = iNULL__
if(ar__(102:104) .EQ. '') DEdm(i__) = iNULL__
if(ar__(110:115) .EQ. '') HD(i__) = iNULL__
if(ar__(137:140) .EQ. '') HR(i__) = iNULL__
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(DE_(i__).EQ.'-'.AND.DEdeg(i__).GE.0) DEdeg(i__)=-DEdeg(i__)
c ..............Just test output...........
write(6,1)
+ Woolley(i__),m_Woolley(i__),plx(i__),e_plx(i__),n_plx(i__),
+ pmRA(i__),pmDE(i__),RVel(i__),n_RVel(i__),U(i__),V(i__),
+ W(i__),GCdist(i__),e(i__),i(i__),LC_Code(i__),SpType(i__),
+ r_SpType(i__),Mag(i__),n_Mag(i__),B_V(i__),U_B(i__),Mv(i__),
+ RA1900h(i__),RA1900dm(i__),DE1900_(i__),DE1900d(i__),
+ DE1900m(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEdm(i__),GCTP(i__),HD(i__),DM(i__),GCRV(i__),PM_Name(i__),
+ HR(i__),Vys(i__),Remark1(i__),Remark2(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end