Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/682/1020 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/682/1020 X-ray sources in NGC 4194 and NGC 7541 (Kaaret+, 2008)
*================================================================================
*X-ray sources in the star-forming galaxies NGC 4194 and NGC 7541.
* Kaaret P., Alonso-Herrero A.
* <Astrophys. J., 682, 1020-1028 (2008)>
* =2008ApJ...682.1020K
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! X-ray sources within the field of NGC 4194
integer*4 nr__
parameter (nr__=6) ! Number of records
character*74 ar__ ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg (nr__) ! (deg) Right Ascension J2000
real*8 DEdeg (nr__) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 Seq (nr__) ! Running sequence number (G1)
integer*4 RAh (nr__) ! (h) Hour of right ascension (J2000)
integer*4 RAm (nr__) ! (min) Minute of right ascension (J2000)
real*4 RAs (nr__) ! (s) Second of right ascension (J2000)
character*1 DE_ (nr__) ! Declination sign (J2000)
integer*4 DEd (nr__) ! (deg) Degree of declination (J2000)
integer*4 DEm (nr__) ! (arcmin) Arcminute of declination (J2000)
real*4 DEs (nr__) ! (arcsec) Arcsecond of declination (J2000)
real*4 S_N (nr__) ! Significance of the source detection as
* calculated by wavdetect
integer*4 Cts (nr__) ! (ct) Counts in the 0.3-8keV band
real*4 Flux (nr__) ! (aW/m2) Source flux in the 0.3-8keV band
* (in units of 10^-15^ergs/cm^2^/s) (1)
real*4 e_Flux (nr__) ! (aW/m2) Uncertainty in Flux
real*4 Lx (nr__) ! (10+31W) Source luminosity in units of 10^38^ergs/s in
* the 2-10keV band using the same spectral model
real*4 HR (nr__) ! ? Hardness ratio (2)
character*12 xid (nr__) ! Optical counterpart (3)
*Note (1): Calculated assuming a power-law spectrum with photon index of 1.7
* and corrected for the Galactic absorption column density along the
* line of sight.
*Note (2): Defined as the ratio of counts in the 1-8keV band to counts in
* the 0.3-8keV band.
*Note (3): In table 5, the counterparts C1-C6 indicate sources from Kaaret
* (2001ApJ...560..715K, <[K2001] AN> in Simbad).
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! X-ray sources within the field of NGC 7541
integer*4 nr__1
parameter (nr__1=15) ! Number of records
character*74 ar__1 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_1 (nr__1) ! (deg) Right Ascension J2000
real*8 DEdeg_1 (nr__1) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 Seq_1 (nr__1) ! Running sequence number (G1)
integer*4 RAh_1 (nr__1) ! (h) Hour of right ascension (J2000)
integer*4 RAm_1 (nr__1) ! (min) Minute of right ascension (J2000)
real*4 RAs_1 (nr__1) ! (s) Second of right ascension (J2000)
character*1 DE__1 (nr__1) ! Declination sign (J2000)
integer*4 DEd_1 (nr__1) ! (deg) Degree of declination (J2000)
integer*4 DEm_1 (nr__1) ! (arcmin) Arcminute of declination (J2000)
real*4 DEs_1 (nr__1) ! (arcsec) Arcsecond of declination (J2000)
real*4 S_N_1 (nr__1) ! Significance of the source detection as
* calculated by wavdetect
integer*4 Cts_1 (nr__1) ! (ct) Counts in the 0.3-8keV band
real*4 Flux_1 (nr__1) ! (aW/m2) Source flux in the 0.3-8keV band
* (in units of 10^-15^ergs/cm^2^/s) (1)
real*4 e_Flux_1 (nr__1) ! (aW/m2) Uncertainty in Flux
real*4 Lx_1 (nr__1) ! (10+31W) Source luminosity in units of 10^38^ergs/s in
* the 2-10keV band using the same spectral model
real*4 HR_1 (nr__1) ! ? Hardness ratio (2)
character*12 xid_1 (nr__1) ! Optical counterpart (3)
*Note (1): Calculated assuming a power-law spectrum with photon index of 1.7
* and corrected for the Galactic absorption column density along the
* line of sight.
*Note (2): Defined as the ratio of counts in the 1-8keV band to counts in
* the 0.3-8keV band.
*Note (3): In table 5, the counterparts C1-C6 indicate sources from Kaaret
* (2001ApJ...560..715K, <[K2001] AN> in Simbad).
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table5.dat' ! X-ray sources within the field of M100
integer*4 nr__2
parameter (nr__2=50) ! Number of records
character*74 ar__2 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_2 (nr__2) ! (deg) Right Ascension J2000
real*8 DEdeg_2 (nr__2) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 Seq_2 (nr__2) ! Running sequence number (G1)
integer*4 RAh_2 (nr__2) ! (h) Hour of right ascension (J2000)
integer*4 RAm_2 (nr__2) ! (min) Minute of right ascension (J2000)
real*4 RAs_2 (nr__2) ! (s) Second of right ascension (J2000)
character*1 DE__2 (nr__2) ! Declination sign (J2000)
integer*4 DEd_2 (nr__2) ! (deg) Degree of declination (J2000)
integer*4 DEm_2 (nr__2) ! (arcmin) Arcminute of declination (J2000)
real*4 DEs_2 (nr__2) ! (arcsec) Arcsecond of declination (J2000)
real*4 S_N_2 (nr__2) ! Significance of the source detection as
* calculated by wavdetect
integer*4 Cts_2 (nr__2) ! (ct) Counts in the 0.3-8keV band
real*4 Flux_2 (nr__2) ! (aW/m2) Source flux in the 0.3-8keV band
* (in units of 10^-15^ergs/cm^2^/s) (1)
real*4 e_Flux_2 (nr__2) ! (aW/m2) Uncertainty in Flux
real*4 Lx_2 (nr__2) ! (10+31W) Source luminosity in units of 10^38^ergs/s in
* the 2-10keV band using the same spectral model
real*4 HR_2 (nr__2) ! ? Hardness ratio (2)
character*12 xid_2 (nr__2) ! Optical counterpart (3)
*Note (1): Calculated assuming a power-law spectrum with photon index of 1.7
* and corrected for the Galactic absorption column density along the
* line of sight.
*Note (2): Defined as the ratio of counts in the 1-8keV band to counts in
* the 0.3-8keV band.
*Note (3): In table 5, the counterparts C1-C6 indicate sources from Kaaret
* (2001ApJ...560..715K, <[K2001] AN> in Simbad).
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table6.dat' ! X-ray sources within the field of NGC 4945
integer*4 nr__3
parameter (nr__3=48) ! Number of records
character*74 ar__3 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_3 (nr__3) ! (deg) Right Ascension J2000
real*8 DEdeg_3 (nr__3) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 Seq_3 (nr__3) ! Running sequence number (G1)
integer*4 RAh_3 (nr__3) ! (h) Hour of right ascension (J2000)
integer*4 RAm_3 (nr__3) ! (min) Minute of right ascension (J2000)
real*4 RAs_3 (nr__3) ! (s) Second of right ascension (J2000)
character*1 DE__3 (nr__3) ! Declination sign (J2000)
integer*4 DEd_3 (nr__3) ! (deg) Degree of declination (J2000)
integer*4 DEm_3 (nr__3) ! (arcmin) Arcminute of declination (J2000)
real*4 DEs_3 (nr__3) ! (arcsec) Arcsecond of declination (J2000)
real*4 S_N_3 (nr__3) ! Significance of the source detection as
* calculated by wavdetect
integer*4 Cts_3 (nr__3) ! (ct) Counts in the 0.3-8keV band
real*4 Flux_3 (nr__3) ! (aW/m2) Source flux in the 0.3-8keV band
* (in units of 10^-15^ergs/cm^2^/s) (1)
real*4 e_Flux_3 (nr__3) ! (aW/m2) Uncertainty in Flux
real*4 Lx_3 (nr__3) ! (10+31W) Source luminosity in units of 10^38^ergs/s in
* the 2-10keV band using the same spectral model
real*4 HR_3 (nr__3) ! ? Hardness ratio (2)
character*12 xid_3 (nr__3) ! Optical counterpart (3)
*Note (1): Calculated assuming a power-law spectrum with photon index of 1.7
* and corrected for the Galactic absorption column density along the
* line of sight.
*Note (2): Defined as the ratio of counts in the 1-8keV band to counts in
* the 0.3-8keV band.
*Note (3): In table 5, the counterparts C1-C6 indicate sources from Kaaret
* (2001ApJ...560..715K, <[K2001] AN> in Simbad).
C=============================================================================
C Loading file 'table2.dat' ! X-ray sources within the field of NGC 4194
C Format for file interpretation
1 format(
+ I2,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F5.1,1X,I4,
+ 1X,F5.1,1X,F5.2,1X,F6.2,1X,F4.2,1X,A12)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,6
read(1,'(A74)')ar__
read(ar__,1)
+ Seq(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),S_N(i__),Cts(i__),Flux(i__),e_Flux(i__),
+ Lx(i__),HR(i__),xid(i__)
if(ar__(58:61) .EQ. '') HR(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(6,1)
+ Seq(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),S_N(i__),Cts(i__),Flux(i__),e_Flux(i__),
+ Lx(i__),HR(i__),xid(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' ! X-ray sources within the field of NGC 7541
C Format for file interpretation
2 format(
+ I2,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F5.1,1X,I4,
+ 1X,F5.1,1X,F5.2,1X,F6.2,1X,F4.2,1X,A12)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,15
read(1,'(A74)')ar__1
read(ar__1,2)
+ Seq_1(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
+ DEd_1(i__),DEm_1(i__),DEs_1(i__),S_N_1(i__),Cts_1(i__),
+ Flux_1(i__),e_Flux_1(i__),Lx_1(i__),HR_1(i__),xid_1(i__)
if(ar__1(58:61) .EQ. '') HR_1(i__) = rNULL__
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(6,2)
+ Seq_1(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
+ DEd_1(i__),DEm_1(i__),DEs_1(i__),S_N_1(i__),Cts_1(i__),
+ Flux_1(i__),e_Flux_1(i__),Lx_1(i__),HR_1(i__),xid_1(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 'table5.dat' ! X-ray sources within the field of M100
C Format for file interpretation
3 format(
+ I2,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F5.1,1X,I4,
+ 1X,F5.1,1X,F5.2,1X,F6.2,1X,F4.2,1X,A12)
C Effective file loading
open(unit=1,status='old',file=
+'table5.dat')
write(6,*) '....Loading file: table5.dat'
do i__=1,50
read(1,'(A74)')ar__2
read(ar__2,3)
+ Seq_2(i__),RAh_2(i__),RAm_2(i__),RAs_2(i__),DE__2(i__),
+ DEd_2(i__),DEm_2(i__),DEs_2(i__),S_N_2(i__),Cts_2(i__),
+ Flux_2(i__),e_Flux_2(i__),Lx_2(i__),HR_2(i__),xid_2(i__)
if(ar__2(58:61) .EQ. '') HR_2(i__) = rNULL__
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(6,3)
+ Seq_2(i__),RAh_2(i__),RAm_2(i__),RAs_2(i__),DE__2(i__),
+ DEd_2(i__),DEm_2(i__),DEs_2(i__),S_N_2(i__),Cts_2(i__),
+ Flux_2(i__),e_Flux_2(i__),Lx_2(i__),HR_2(i__),xid_2(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_2(i__),DEdeg_2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table6.dat' ! X-ray sources within the field of NGC 4945
C Format for file interpretation
4 format(
+ I2,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F5.1,1X,I4,
+ 1X,F5.1,1X,F5.2,1X,F6.2,1X,F4.2,1X,A12)
C Effective file loading
open(unit=1,status='old',file=
+'table6.dat')
write(6,*) '....Loading file: table6.dat'
do i__=1,48
read(1,'(A74)')ar__3
read(ar__3,4)
+ Seq_3(i__),RAh_3(i__),RAm_3(i__),RAs_3(i__),DE__3(i__),
+ DEd_3(i__),DEm_3(i__),DEs_3(i__),S_N_3(i__),Cts_3(i__),
+ Flux_3(i__),e_Flux_3(i__),Lx_3(i__),HR_3(i__),xid_3(i__)
if(ar__3(58:61) .EQ. '') HR_3(i__) = rNULL__
RAdeg_3(i__) = rNULL__
DEdeg_3(i__) = rNULL__
c Derive coordinates RAdeg_3 and DEdeg_3 from input data
c (RAdeg_3 and DEdeg_3 are set to rNULL__ when unknown)
if(RAh_3(i__) .GT. -180) RAdeg_3(i__)=RAh_3(i__)*15.
if(RAm_3(i__) .GT. -180) RAdeg_3(i__)=RAdeg_3(i__)+RAm_3(i__)/4.
if(RAs_3(i__) .GT. -180) RAdeg_3(i__)=RAdeg_3(i__)+RAs_3(i__)/240.
if(DEd_3(i__) .GE. 0) DEdeg_3(i__)=DEd_3(i__)
if(DEm_3(i__) .GE. 0) DEdeg_3(i__)=DEdeg_3(i__)+DEm_3(i__)/60.
if(DEs_3(i__) .GE. 0) DEdeg_3(i__)=DEdeg_3(i__)+DEs_3(i__)/3600.
if(DE__3(i__).EQ.'-'.AND.DEdeg_3(i__).GE.0) DEdeg_3(i__)=-DEdeg_3(i__)
c ..............Just test output...........
write(6,4)
+ Seq_3(i__),RAh_3(i__),RAm_3(i__),RAs_3(i__),DE__3(i__),
+ DEd_3(i__),DEm_3(i__),DEs_3(i__),S_N_3(i__),Cts_3(i__),
+ Flux_3(i__),e_Flux_3(i__),Lx_3(i__),HR_3(i__),xid_3(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_3(i__),DEdeg_3(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end