Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/429/1125 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-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/A+A/429/1125 Catalog of Ultraluminous X-ray sources (Liu+, 2005)
*================================================================================
*A catalogue of ultraluminous X-ray sources in external galaxies.
* Liu Q.Z., Mirabel I.R.
* <Astron. Astrophys. 429, 1125 (2005)>
* =2005A&A...429.1125L
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1a.dat' ! Host galaxies
integer*4 nr__
parameter (nr__=85) ! Number of records
character*99 ar__ ! Full-size record
character*15 Galaxy (nr__) ! Host galaxy
character*8 OName (nr__) ! Other name
character*18 MType (nr__) ! Hubble-type, from RC3 (Cat. <VII/155>)
real*4 TType (nr__) ! T-type, from RC3 (Cat. <VII/155>)
real*4 TType2 (nr__) ! ? T type of the second galaxy when pair
real*4 Dist (nr__) ! (Mpc) Distance
real*4 NH (nr__) ! (10+20cm-2) ? Galactic hydrogen column density,
* from Dickey & Lockman (1990ARA&A..28..215D)
integer*4 NH2 (nr__) ! (10+20cm-2) ? Higher Galactic hydrogen column density
* when interval
real*4 Bmag (nr__) ! (mag) ? B-band photographic magnitude, from RC3
real*4 Bmag2 (nr__) ! (mag) ? B magnitude of the second galaxy when pair
real*4 Ksmag (nr__) ! (mag) ? Ks magnitude (1)
real*4 Ksmag2 (nr__) ! (mag) ? Ksmag value of the second galaxy when pair
real*4 FIRmag (nr__) ! (mag) ? Far infrared magnitude (2)
*Note (1): The near-infrared K_s_-band magnitude is calculated from the
* 20mag/arcsec^2^ isophotal magnitude listed in the 2MASS Large Galaxy
* Atlas (Jarrett et al., 2003AJ....125..525J)
*Note (2): The far-infrared magnitude is calculated from
* FIRmag=-20.0 -2.5logFIR,
* where FIR is the far infrared continuum flux measured at 60 and
* 100microns as listed in the IRAS Point Source Catalog (1987, Cat.
* <II/125>).
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1b.dat' ! Ultraluminous X-ray sources
integer*4 nr__1
parameter (nr__1=229) ! Number of records
character*104 ar__1 ! Full-size record
C J2000.0 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg (nr__1) ! (deg) Right Ascension J2000.0
real*8 DEdeg (nr__1) ! (deg) Declination J2000.0
C ---------------------------------- ! (position vector(s) in degrees)
character*15 Galaxy_1 (nr__1) ! Host galaxy name
character*5 ULX (nr__1) ! Source Name
character*13 OName_1 (nr__1) ! Other name of the ULX source
integer*4 RAh (nr__1) ! (h) Right ascension (J2000.0)
integer*4 RAm (nr__1) ! (min) Right ascension (J2000.0)
real*4 RAs (nr__1) ! (s) Right ascension (J2000.0)
character*1 DE_ (nr__1) ! Declination sign (J2000.0)
integer*4 DEd (nr__1) ! (deg) Declination (J2000.0)
integer*4 DEm (nr__1) ! (arcmin) Declination (J2000.0)
real*4 DEs (nr__1) ! (arcsec) Declination (J2000.0)
real*4 LX (nr__1) ! (10+32W) X-ray luminosity (in 10+39erg/s)
real*4 E1 (nr__1) ! (keV) Lower limit of energy range
real*4 E2 (nr__1) ! (keV) Upper limit of energy range
real*4 Offset (nr__1) ! (arcsec) ? Nuclear offset (1)
character*6 Best_fit (nr__1) ! Best fit model of recent X-ray observation
* of ULXs (2)
real*4 Gamma1 (nr__1) ! ? Spectral index listed for a power-law fit
* inner temperature in keV for a thermal
* model fit
real*4 Gamma2 (nr__1) ! ? Results for the two-component best fit (3)
*Note (1): Radius from nucleus, assuming that the galaxy center is at
* the RC3 (Cat. <VII/155>) optical position. Only strong X-ray sources
* with enough counts have X-ray spectral fits.
*Note (2): The following abbreviations have been used for the fit model:
* PL: power-law model
* BB: blackbody
* MCD: multicolor disk (Mitsuda et al., 1984PASJ...36..741M)
* MKL: MEKAL
* BR: bremsstrahlung
* RS: Raymond-Smith thermal model (Raymond & Smith 1977ApJS...35..419R)
*Note (3): If a two-component fit is needed, we use the symbol '+'
* between the two fit models and fit results for the two-component best fit.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'notes.dat' ! Notes
integer*4 nr__2
parameter (nr__2=740) ! Number of records
character*80 ar__2 ! Full-size record
character*15 Galaxy_2 (nr__2) ! Galaxy name
character*65 Note (nr__2) ! Text of the note
C=============================================================================
C Loading file 'table1a.dat' ! Host galaxies
C Format for file interpretation
1 format(
+ A15,1X,A8,2X,A18,1X,F5.1,1X,F5.1,1X,F6.3,1X,F5.2,1X,I2,1X,
+ F5.2,1X,F5.2,1X,F5.2,1X,F3.1,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table1a.dat')
write(6,*) '....Loading file: table1a.dat'
do i__=1,85
read(1,'(A99)')ar__
read(ar__,1)
+ Galaxy(i__),OName(i__),MType(i__),TType(i__),TType2(i__),
+ Dist(i__),NH(i__),NH2(i__),Bmag(i__),Bmag2(i__),Ksmag(i__),
+ Ksmag2(i__),FIRmag(i__)
if(ar__(52:56) .EQ. '') TType2(i__) = rNULL__
if(ar__(65:69) .EQ. '') NH(i__) = rNULL__
if(ar__(71:72) .EQ. '') NH2(i__) = iNULL__
if(ar__(74:78) .EQ. '') Bmag(i__) = rNULL__
if(ar__(80:84) .EQ. '') Bmag2(i__) = rNULL__
if(ar__(86:90) .EQ. '') Ksmag(i__) = rNULL__
if(ar__(92:94) .EQ. '') Ksmag2(i__) = rNULL__
if(ar__(95:99) .EQ. '') FIRmag(i__) = rNULL__
c ..............Just test output...........
write(6,1)
+ Galaxy(i__),OName(i__),MType(i__),TType(i__),TType2(i__),
+ Dist(i__),NH(i__),NH2(i__),Bmag(i__),Bmag2(i__),Ksmag(i__),
+ Ksmag2(i__),FIRmag(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table1b.dat' ! Ultraluminous X-ray sources
C Format for file interpretation
2 format(
+ A15,1X,A5,1X,A13,2X,I2,1X,I2,1X,F6.3,2X,A1,I2,1X,I2,1X,F5.2,
+ 1X,F5.2,2X,F3.1,1X,F4.1,1X,F6.2,1X,A6,1X,F5.3,1X,F4.2)
C Effective file loading
open(unit=1,status='old',file=
+'table1b.dat')
write(6,*) '....Loading file: table1b.dat'
do i__=1,229
read(1,'(A104)')ar__1
read(ar__1,2)
+ Galaxy_1(i__),ULX(i__),OName_1(i__),RAh(i__),RAm(i__),
+ RAs(i__),DE_(i__),DEd(i__),DEm(i__),DEs(i__),LX(i__),E1(i__),
+ E2(i__),Offset(i__),Best_fit(i__),Gamma1(i__),Gamma2(i__)
if(ar__1(81:86) .EQ. '') Offset(i__) = rNULL__
if(ar__1(95:99) .EQ. '') Gamma1(i__) = rNULL__
if(ar__1(101:104) .EQ. '') Gamma2(i__) = rNULL__
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(DEm(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEm(i__)/60.
if(DEs(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEs(i__)/3600.
if(DE_(i__).EQ.'-'.AND.DEdeg(i__).GE.0) DEdeg(i__)=-DEdeg(i__)
c ..............Just test output...........
write(6,2)
+ Galaxy_1(i__),ULX(i__),OName_1(i__),RAh(i__),RAm(i__),
+ RAs(i__),DE_(i__),DEd(i__),DEm(i__),DEs(i__),LX(i__),E1(i__),
+ E2(i__),Offset(i__),Best_fit(i__),Gamma1(i__),Gamma2(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'notes.dat' ! Notes
C Format for file interpretation
3 format(A15,A65)
C Effective file loading
open(unit=1,status='old',file=
+'notes.dat')
write(6,*) '....Loading file: notes.dat'
do i__=1,740
read(1,'(A80)')ar__2
read(ar__2,3)Galaxy_2(i__),Note(i__)
c ..............Just test output...........
write(6,3)Galaxy_2(i__),Note(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end