Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/663/960 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-20
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/ApJ/663/960 Radial velocities of Leo I stars (Sohn+, 2007)
*================================================================================
*Exploring halo substructure with giant stars.
*X. Extended dark matter or tidal disruption?:
*the case for the Leo I dwarf spheroidal galaxy.
* Sohn S.T., Majewski S.R., Munoz R.R., Kunkel W.E., Johnston K.V.,
* Ostheimer J.C., Guhathakurta P., Patterson R.J., Siegel M.H., Cooper M.C.
* <Astrophys. J., 663, 960-989 (2007)>
* =2007ApJ...663..960S
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4.dat' ! Observed Radial Velocities of Stars
integer*4 nr__
parameter (nr__=125) ! Number of records
character*81 ar__ ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg ! (deg) Right Ascension J2000
real*8 DEdeg ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
character*6 Slit ! Slit identification
integer*4 v_SMM2007_ ! Source identification number
character*1 n__SMM2007_ ! [f] 4" slit (1)
integer*4 RAh ! (h) Hour of Right Ascension (J2000)
integer*4 RAm ! (min) Minute of Right Ascension (J2000)
real*4 RAs ! (s) Second of Right Ascension (J2000)
character*1 DE_ ! Sign of the Declination (J2000)
integer*4 DEd ! (deg) Degree of Declination (J2000)
integer*4 DEm ! (arcmin) Arcminute of Declination (J2000)
real*4 DEs ! (arcsec) Arcsecond of Declination (J2000)
real*4 M0mag ! (mag) Extinction corrected M-band (Washington)
* magnitude
real*4 M_T2 ! (mag) Reddening corrected (M-T_2_) color index
real*4 M_D51 ! (mag) Reddening corrected (M-D51) color index
real*4 HRV ! (km/s) Heliocentric radial velocity (2)
real*4 Vgsr ! (km/s) Galactocentric standard of rest
* radial velocity (3)
real*4 TOff ! (km/s) Telluric offset (4)
real*4 CCP ! Cross-correlation peak
integer*4 Q ! Quality indicator (5)
*Note (1): f = Alignment stars observed with 4" wide slits. All other stars
* were observed with 1" wide slits.
*Note (2): Corrected for the Telluric offsets as described in text.
*Note (3): We convert to Galactocentric standard of rest by assuming a local
* standard of rest velocity of 220km/s and a solar peculiar velocity of
* (u,v,w)=(-9,12,7)km/s
*Note (4): The wavelength ranges on which the telluric offset determination
* is based are 6866-6912{AA} (the Fraunhofer B band), 7167-7320{AA},
* 7593-7690{AA} (the Fraunhofer A band), 8110-8320{AA}, and
* 8925-9120{AA}, but all telluric features weaker than 20% were not
* used. See text for more explanations.
*Note (5): See Majewski et al. (2004AJ....128..245M) and Kunkel et al.
* (1997A&AS..122..463K) for descriptions on how Q-values are assigned.
C=============================================================================
C Loading file 'table4.dat' ! Observed Radial Velocities of Stars
C Format for file interpretation
1 format(
+ A6,1X,I5,1X,A1,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,
+ F5.2,1X,F4.2,1X,F5.2,1X,F5.1,1X,F6.1,1X,F5.1,1X,F4.2,1X,I1)
C Effective file loading
open(unit=1,status='old',file=
+'table4.dat')
write(6,*) '....Loading file: table4.dat'
do i__=1,125
read(1,'(A81)')ar__
read(ar__,1)
+ Slit,v_SMM2007_,n__SMM2007_,RAh,RAm,RAs,DE_,DEd,DEm,DEs,M0mag,
+ M_T2,M_D51,HRV,Vgsr,TOff,CCP,Q
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(DEm .GE. 0) DEdeg=DEdeg+DEm/60.
if(DEs .GE. 0) DEdeg=DEdeg+DEs/3600.
if(DE_.EQ.'-'.AND.DEdeg.GE.0) DEdeg=-DEdeg
c ..............Just test output...........
write(6,1)
+ Slit,v_SMM2007_,n__SMM2007_,RAh,RAm,RAs,DE_,DEd,DEm,DEs,M0mag,
+ M_T2,M_D51,HRV,Vgsr,TOff,CCP,Q
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end