Conversion of standardized ReadMe file for
file /./ftp/cats/III/216/ 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-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/216 Stellar Radial Velocities 1991-1998 (Malaroda+ 2001)
*================================================================================
*Bibliographic catalogue of stellar radial velocities, 1991-1998
* Malaroda S., Levato H., Galliani S.
* <Complejo Astronomico El Leoncito (CASLEO), San Juan, Argentina (2001)>
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'cat91-98.dat' ! Stellar radial velocities bibliographic catalogue
integer*4 nr__
parameter (nr__=33471) ! Number of records
character*181 ar__ ! Full-size record
C J2000.0 position composed of: RAh RAm DE- DEd DEm
real*8 RAdeg ! (deg) Right Ascension J2000.0
real*8 DEdeg ! (deg) Declination J2000.0
C ---------------------------------- ! (position vector(s) in degrees)
character*29 Ident ! Identification (1)
integer*4 RAh ! (h) ? Right ascension J2000.0 (2)
real*4 RAm ! (min) [0,60]? Right ascension J2000.0
character*1 DE_ ! Declination sign J2000.0
integer*4 DEd ! (deg) ? Declination J2000.0
real*4 DEm ! (arcmin) [0,60]? Declination J2000.0
real*4 Vmag ! (mag) ? Visual magnitude (From Simbad)
character*1 u_Vmag ! [:?] Uncertainty flag on Vmag
character*2 n_Vmag ! [abV?R ]
character*9 SpType ! Spectral type and luminosity class (3)
character*1 l_RV ! [~]
real*8 RV ! (km/s) ? Heliocentric Radial velocity (4)
character*1 u_RV ! [:v?] Uncertainty flag on RV
character*1 l_o_RV ! Limit flag on o_RV
integer*4 o_RV ! ? Number of individual observations for a
* particular object
character*1 u_o_RV ! [?#]
character*8 Type ! Nature of the star (5)
character*6 R_RP_D ! Dispersion, resolving power or resolution (6)
character*19 r_RV ! Reference (BibCode)
character*57 Note ! 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 'cat91-98.dat' ! Stellar radial velocities bibliographic catalogue
C Format for file interpretation
1 format(
+ A29,1X,I2,1X,F5.2,1X,A1,I2,1X,F4.1,1X,F6.3,A1,A2,1X,A9,1X,A1,
+ F8.3,A1,1X,A1,I5,A1,1X,A8,1X,A6,2X,A19,1X,A57)
C Effective file loading
open(unit=1,status='old',file=
+'cat91-98.dat')
write(6,*) '....Loading file: cat91-98.dat'
do i__=1,33471
read(1,'(A181)')ar__
read(ar__,1)
+ Ident,RAh,RAm,DE_,DEd,DEm,Vmag,u_Vmag,n_Vmag,SpType,l_RV,RV,
+ u_RV,l_o_RV,o_RV,u_o_RV,Type,R_RP_D,r_RV,Note
if(ar__(31:32) .EQ. '') RAh = iNULL__
if(ar__(34:38) .EQ. '') RAm = rNULL__
if(ar__(41:42) .EQ. '') DEd = iNULL__
if(ar__(44:47) .EQ. '') DEm = rNULL__
if(ar__(49:54) .EQ. '') Vmag = rNULL__
if(ar__(70:77) .EQ. '') RV = rNULL__
if(ar__(81:85) .EQ. '') o_RV = 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(DEd .GE. 0) DEdeg=DEd
if(DEm .GE. 0) DEdeg=DEdeg+DEm/60.
if(DE_.EQ.'-'.AND.DEdeg.GE.0) DEdeg=-DEdeg
c ..............Just test output...........
write(6,1)
+ Ident,RAh,RAm,DE_,DEd,DEm,Vmag,u_Vmag,n_Vmag,SpType,l_RV,RV,
+ u_RV,l_o_RV,o_RV,u_o_RV,Type,R_RP_D,r_RV,Note
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end