Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/664/458 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/ApJ/664/458 Spectral fit of ULX sources (Devi+, 2007)
*================================================================================
*The dependence of the estimated luminosities of ultraluminous X-ray sources on
*spectral models.
* Devi A.S., Misra R., Agrawal V.K., Singh K.Y.
* <Astrophys. J., 664, 458-466 (2007)>
* =2007ApJ...664..458D
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Sample galaxy properties
integer*4 nr__
parameter (nr__=30) ! Number of records
character*36 ar__ ! Full-size record
character*8 Galaxy (nr__) ! Galaxy name
character*8 Gal2 (nr__) ! Associated galaxy
real*4 Dist (nr__) ! (Mpc) Distance
integer*4 ObsID (nr__) ! Chandra observation ID
real*4 Texp (nr__) ! (ks) Exposure time
integer*4 N (nr__) ! Number of point sources with total counts from
* the source >=60, as detected by wavdetect
* with fluxscale=1
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! List of sources with count rate > 0.05counts/s
integer*4 nr__1
parameter (nr__1=15) ! Number of records
character*43 ar__1 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg (nr__1) ! (deg) Right Ascension J2000
real*8 DEdeg (nr__1) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
character*8 Galaxy_1 (nr__1) ! Galaxy name
integer*4 RAh (nr__1) ! (h) Right ascension (J2000)
integer*4 RAm (nr__1) ! (min) Right ascension (J2000)
real*4 RAs (nr__1) ! (s) Right ascension (J2000)
character*1 DE_ (nr__1) ! Declination sign (J2000)
integer*4 DEd (nr__1) ! (deg) Declination (J2000)
integer*4 DEm (nr__1) ! (arcmin) Declination (J2000)
real*4 DEs (nr__1) ! (arcsec) Declination (J2000)
real*8 CR (nr__1) ! (ct/s) Count rate
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Spectral properties of point sources fitted with
the power-law model
integer*4 nr__2
parameter (nr__2=365) ! Number of records
character*89 ar__2 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_1 (nr__2) ! (deg) Right Ascension J2000
real*8 DEdeg_1 (nr__2) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
character*8 Galaxy_2 (nr__2) ! Galaxy name
integer*4 RAh_1 (nr__2) ! (h) Hour of Right Ascension (J2000)
integer*4 RAm_1 (nr__2) ! (min) Minute of Right Ascension (J2000)
real*4 RAs_1 (nr__2) ! (s) Second of Right Ascension (J2000)
character*1 DE__1 (nr__2) ! Sign of the Declination (J2000)
integer*4 DEd_1 (nr__2) ! (deg) Degree of Declination (J2000)
integer*4 DEm_1 (nr__2) ! (arcmin) Arcminute of Declination (J2000)
real*4 DEs_1 (nr__2) ! (arcsec) Arcsecond of Declination (J2000)
real*4 nHpl (nr__2) ! (10+22cm-2) Equivalent H column density (power-law)
real*4 E_nHpl (nr__2) ! (10+22cm-2) Upper limit uncertainty in nHpl
real*4 e_nHpl_1 (nr__2) ! (10+22cm-2) Lower limit uncertainty in nHpl
real*4 Gamma (nr__2) ! Photon power-law index
real*4 E_Gamma (nr__2) ! Upper limit uncertainty in Gamma
real*4 e_Gamma_1 (nr__2) ! Lower limit uncertainty in Gamma
real*4 logLpl (nr__2) ! ([10-7W]) 0.3-8keV luminosity in erg/s (power-law)
real*4 E_logLpl (nr__2) ! ([10-7W]) Upper limit uncertainty in logLpl
real*4 e_logLpl_1 (nr__2) ! ([10-7W]) Lower limit uncertainty in logLpl
real*4 Cst_pl (nr__2) ! C-statistic result in power-law model (G1)
integer*4 dof_pl (nr__2) ! Degree of freedom in power-law
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4.dat' ! Spectral properties of point sources fitted with
the disk black body model
integer*4 nr__3
parameter (nr__3=365) ! Number of records
character*90 ar__3 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_2 (nr__3) ! (deg) Right Ascension J2000
real*8 DEdeg_2 (nr__3) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
character*8 Galaxy_3 (nr__3) ! Galaxy name
integer*4 RAh_2 (nr__3) ! (h) Hour of Right Ascension (J2000)
integer*4 RAm_2 (nr__3) ! (min) Minute of Right Ascension (J2000)
real*4 RAs_2 (nr__3) ! (s) Second of Right Ascension (J2000)
character*1 DE__2 (nr__3) ! Sign of the Declination (J2000)
integer*4 DEd_2 (nr__3) ! (deg) Degree of Declination (J2000)
integer*4 DEm_2 (nr__3) ! (arcmin) Arcminute of Declination (J2000)
real*4 DEs_2 (nr__3) ! (arcsec) Arcsecond of Declination (J2000)
real*4 nHbb (nr__3) ! (10+22cm-2) Equivalent H column density (blackbody)
real*4 E_nHbb (nr__3) ! (10+22cm-2) Upper limit uncertainty in nHbb
real*4 e_nHbb_1 (nr__3) ! (10+22cm-2) Lower limit uncertainty in nHbb
real*4 kT (nr__3) ! (keV) Inner disk temperature
real*4 E_kT (nr__3) ! (keV) Upper limit uncertainty in kT
real*4 e_kT_1 (nr__3) ! (keV) Lower limit uncertainty in kT
real*4 logLbb (nr__3) ! ([10-7W]) Bolometric X-ray luminosity erg/s (blackbody)
real*4 E_logLbb (nr__3) ! ([10-7W]) Upper limit uncertainty in logL
real*4 e_logLbb_1 (nr__3) ! ([10-7W]) Lower limit uncertainty in logL
real*4 Cst_bb (nr__3) ! C-statistic result in blackbody model (G1)
integer*4 dof_bb (nr__3) ! Degree of freedom in blackbody model
C=============================================================================
C Loading file 'table1.dat' ! Sample galaxy properties
C Format for file interpretation
1 format(A8,1X,A8,1X,F4.1,1X,I4,1X,F5.2,1X,I2)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,30
read(1,'(A36)')ar__
read(ar__,1)
+ Galaxy(i__),Gal2(i__),Dist(i__),ObsID(i__),Texp(i__),N(i__)
c ..............Just test output...........
write(6,1)
+ Galaxy(i__),Gal2(i__),Dist(i__),ObsID(i__),Texp(i__),N(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! List of sources with count rate > 0.05counts/s
C Format for file interpretation
2 format(A8,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F5.2,1X,F9.7)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,15
read(1,'(A43)')ar__1
read(ar__1,2)
+ Galaxy_1(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),CR(i__)
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__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),CR(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 'table3.dat' ! Spectral properties of point sources fitted with
* the power-law model
C Format for file interpretation
3 format(
+ A8,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F5.2,1X,F4.2,1X,F4.2,
+ 1X,F4.2,1X,F4.2,1X,F4.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,F4.2,1X,
+ F6.2,1X,I2)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,365
read(1,'(A89)')ar__2
read(ar__2,3)
+ Galaxy_2(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
+ DEd_1(i__),DEm_1(i__),DEs_1(i__),nHpl(i__),E_nHpl(i__),
+ e_nHpl_1(i__),Gamma(i__),E_Gamma(i__),e_Gamma_1(i__),
+ logLpl(i__),E_logLpl(i__),e_logLpl_1(i__),Cst_pl(i__),
+ dof_pl(i__)
RAdeg_1(i__) = rNULL__
DEdeg_1(i__) = rNULL__
c Derive coordinates RAdeg_1 and DEdeg_1 from input data
c (RAdeg_1 and DEdeg_1 are set to rNULL__ when unknown)
if(RAh_1(i__) .GT. -180) RAdeg_1(i__)=RAh_1(i__)*15.
if(RAm_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAm_1(i__)/4.
if(RAs_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAs_1(i__)/240.
if(DEd_1(i__) .GE. 0) DEdeg_1(i__)=DEd_1(i__)
if(DEm_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEm_1(i__)/60.
if(DEs_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEs_1(i__)/3600.
if(DE__1(i__).EQ.'-'.AND.DEdeg_1(i__).GE.0) DEdeg_1(i__)=-DEdeg_1(i__)
c ..............Just test output...........
write(6,3)
+ Galaxy_2(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
+ DEd_1(i__),DEm_1(i__),DEs_1(i__),nHpl(i__),E_nHpl(i__),
+ e_nHpl_1(i__),Gamma(i__),E_Gamma(i__),e_Gamma_1(i__),
+ logLpl(i__),E_logLpl(i__),e_logLpl_1(i__),Cst_pl(i__),
+ dof_pl(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_1(i__),DEdeg_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table4.dat' ! Spectral properties of point sources fitted with
* the disk black body model
C Format for file interpretation
4 format(
+ A8,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F5.2,1X,F4.2,1X,F4.2,
+ 1X,F4.2,1X,F5.2,1X,F4.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,F4.2,1X,
+ F6.2,1X,I2)
C Effective file loading
open(unit=1,status='old',file=
+'table4.dat')
write(6,*) '....Loading file: table4.dat'
do i__=1,365
read(1,'(A90)')ar__3
read(ar__3,4)
+ Galaxy_3(i__),RAh_2(i__),RAm_2(i__),RAs_2(i__),DE__2(i__),
+ DEd_2(i__),DEm_2(i__),DEs_2(i__),nHbb(i__),E_nHbb(i__),
+ e_nHbb_1(i__),kT(i__),E_kT(i__),e_kT_1(i__),logLbb(i__),
+ E_logLbb(i__),e_logLbb_1(i__),Cst_bb(i__),dof_bb(i__)
RAdeg_2(i__) = rNULL__
DEdeg_2(i__) = rNULL__
c Derive coordinates RAdeg_2 and DEdeg_2 from input data
c (RAdeg_2 and DEdeg_2 are set to rNULL__ when unknown)
if(RAh_2(i__) .GT. -180) RAdeg_2(i__)=RAh_2(i__)*15.
if(RAm_2(i__) .GT. -180) RAdeg_2(i__)=RAdeg_2(i__)+RAm_2(i__)/4.
if(RAs_2(i__) .GT. -180) RAdeg_2(i__)=RAdeg_2(i__)+RAs_2(i__)/240.
if(DEd_2(i__) .GE. 0) DEdeg_2(i__)=DEd_2(i__)
if(DEm_2(i__) .GE. 0) DEdeg_2(i__)=DEdeg_2(i__)+DEm_2(i__)/60.
if(DEs_2(i__) .GE. 0) DEdeg_2(i__)=DEdeg_2(i__)+DEs_2(i__)/3600.
if(DE__2(i__).EQ.'-'.AND.DEdeg_2(i__).GE.0) DEdeg_2(i__)=-DEdeg_2(i__)
c ..............Just test output...........
write(6,4)
+ Galaxy_3(i__),RAh_2(i__),RAm_2(i__),RAs_2(i__),DE__2(i__),
+ DEd_2(i__),DEm_2(i__),DEs_2(i__),nHbb(i__),E_nHbb(i__),
+ e_nHbb_1(i__),kT(i__),E_kT(i__),e_kT_1(i__),logLbb(i__),
+ E_logLbb(i__),e_logLbb_1(i__),Cst_bb(i__),dof_bb(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_2(i__),DEdeg_2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end