Conversion of standardized ReadMe file for
file /./ftp/cats/III/204/ 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-19
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. III/204 Stellar radial velocities bibliographic catalog (Malaroda+, 2000)
*================================================================================
*Bibliographic catalogue of stellar radial velocities (1991-1994)
* Malaroda S., Levato,H., Morrell, N., Garcia B., Grosso, M., Bolzicco, G.J.
* <Astron. Astrophys. Suppl. Ser. 144, 1 (2000)>
* =2000A&AS..144....1M
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'catalog.dat' ! Stellar radial velocities bibliographic catalogue
integer*4 nr__
parameter (nr__=13352) ! Number of records
character*148 ar__ ! Full-size record
C J2000.0 position composed of: RAh RAm DE- DEd DEm
real*8 RAdeg (nr__) ! (deg) Right Ascension J2000.0
real*8 DEdeg (nr__) ! (deg) Declination J2000.0
C ---------------------------------- ! (position vector(s) in degrees)
character*29 Ident (nr__) ! Identification (1)
integer*4 RAh (nr__) ! (h) ? Right ascension J2000.0 (2)
real*4 RAm (nr__) ! (min) ? Right ascension J2000.0
character*1 DE_ (nr__) ! Declination sign J2000.0
integer*4 DEd (nr__) ! (deg) ? Declination J2000.0
real*4 DEm (nr__) ! (arcmin) ? Declination J2000.0
real*4 Vmag (nr__) ! (mag) ? Visual magnitude (From Simbad)
character*15 SpType (nr__) ! Spectral type and luminosity class (3)
real*8 RV (nr__) ! (km/s) ? Radial velocity (4)
character*1 u_RV (nr__) ! Uncertainty flag on RV
integer*4 o_RV (nr__) ! ? Number of individual observations for a
* particular object
character*7 Type (nr__) ! Nature of the star (5)
character*6 R_RP_D (nr__) ! Dispersion, resolving power or resolution (6)
character*19 r_RV (nr__) ! RV bibliographic reference (bibcode)
character*28 Note (nr__) ! Complete reference when no bibcode available
*Note (1): We have preferred for identification the HD, CD or CPD numbers,
* in that order. Stars in clusters are indicated with the cluster's name
* and the number of the stars according to the primary identification
* paper for that particular cluster, found either at SIMBAD or
* Mermilliod's database (which was accessed through the web of the
* Geneva Observatory).
*Note (2): Right ascension is given to the tenth of a minute and has been
* retrieved from SIMBAD. Declination is given to the minute and has been
* retrieved from SIMBAD.
*Note (3): Spectra have been retrieved from the SIMBAD database.
* In some cases, when the number of symbols is large, the spectral type
* has been truncated.
*Note (4): For each object we have included the average radial velocity
* provided by the author. If the number of radial velocity measurements
* is more than 1, and an average has not been calculated by the author,
* we have not included any radial velocity at all. If the star is a
* spectroscopic binary, for which an orbit has been computed, then the
* systemic radial velocity is quoted in this column.
*Note (5): We have included in this column an acronym to indicate
* the nature of the star, when mentioned by the author.
* Acronyms are as follows:
* CEPH: Cepheids
* ORB: An orbit has been computed. The systemic radial velocity is listed
* SB1: Single lined binary
* SB2: Double lined binary
* EM: Emission lines. The radial velocity is derived from emission lines
* SB: Spectroscopic binary
* CV: Cataclysmic variable
* VAR: Star with variable radial velocity, according to the author
* LMC: Star belonging to the Large Magellanic Cloud
* STND: Radial velocity standard
* CONST: Star with constant radial velocity, according to the author
* SYMB: Symbiotic star
* BMP: Blue metal poor star
* VB: Visual binary
*Note (6): We have included in this column one of the above parameters.
* It is not possible to confuse the resolving power with any of the
* other two parameters because, in general, resolving power is a
* relatively large number compared with dispersion or resolution.
* As in the case of the dispersion or resolution, an ambiguity may
* arise, we have added an R to the number when it refers to the
* resolution.
* COR: radial velocity was derived through cross correlation techniques
* (like Coravel, for example)
* REL: relative velocity
* SEV: more than one resolving power or resolution have been used
* OP: objective prism observations
* IUE: radial velocities were derived from observations obtained with
* the International Ultraviolet Explorer (See cat. <VI/99>)
C=============================================================================
C Loading file 'catalog.dat' ! Stellar radial velocities bibliographic catalogue
C Format for file interpretation
1 format(
+ A29,1X,I2,1X,F4.1,1X,A1,I2,1X,F4.1,1X,F6.3,A15,1X,F8.3,A1,1X,
+ I3,2X,A7,1X,A6,2X,A19,1X,A28)
C Effective file loading
open(unit=1,status='old',file=
+'catalog.dat')
write(6,*) '....Loading file: catalog.dat'
do i__=1,13352
read(1,'(A148)')ar__
read(ar__,1)
+ Ident(i__),RAh(i__),RAm(i__),DE_(i__),DEd(i__),DEm(i__),
+ Vmag(i__),SpType(i__),RV(i__),u_RV(i__),o_RV(i__),Type(i__),
+ R_RP_D(i__),r_RV(i__),Note(i__)
if(ar__(31:32) .EQ. '') RAh(i__) = iNULL__
if(ar__(34:37) .EQ. '') RAm(i__) = rNULL__
if(ar__(40:41) .EQ. '') DEd(i__) = iNULL__
if(ar__(43:46) .EQ. '') DEm(i__) = rNULL__
if(ar__(48:53) .EQ. '') Vmag(i__) = rNULL__
if(ar__(70:77) .EQ. '') RV(i__) = rNULL__
if(ar__(80:82) .EQ. '') o_RV(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(DEd(i__) .GE. 0) DEdeg(i__)=DEd(i__)
if(DEm(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEm(i__)/60.
if(DE_(i__).EQ.'-'.AND.DEdeg(i__).GE.0) DEdeg(i__)=-DEdeg(i__)
c ..............Just test output...........
write(6,1)
+ Ident(i__),RAh(i__),RAm(i__),DE_(i__),DEd(i__),DEm(i__),
+ Vmag(i__),SpType(i__),RV(i__),u_RV(i__),o_RV(i__),Type(i__),
+ R_RP_D(i__),r_RV(i__),Note(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end