Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/586/814 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-18
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/586/814 NGC 4472 Chandra/HST study (Maccarone+, 2003)
*================================================================================
*The low-mass X-ray binary-globular connection.
*II. NGC 4472 X-ray source properties and source catalogs.
* Maccarone T.J., Kundu A., Zepf S.E.
* <Astrophys. J. 586, 814 (2003)>
* =2003ApJ...586..814M
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! The X-ray Source List
integer*4 nr__
parameter (nr__=147) ! Number of records
character*88 ar__ ! Full-size record
integer*4 XID (nr__) ! X-ray catalog Number, [MKZ2003] XID NNN
character*15 CXOMKZ (nr__) ! CXOMKZ Source Name (JHHMMSSs+DDMMSS)
real*4 Gamma (nr__) ! Spectral index in photon space
real*4 EGamma (nr__) ! ? 90% error in the positive direction (G1)
real*4 eGamma_1 (nr__) ! ? 90% error in the negative direction (G1)
real*4 SFlux (nr__) ! (mW/m2) The (0.5-2.0keV) X-ray model flux (G2)
real*4 HFlux (nr__) ! (mW/m2) The (2.0-8.0keV) X-ray model flux (G2)
real*4 XLum (nr__) ! (10-7W) The (0.5-8.0keV) X-ray luminosity (G2)
real*4 Chi2 (nr__) ! The chi^2^ of the model fit
integer*4 DOF (nr__) ! Degrees of freedom
character*1 GR (nr__) ! [YN] Good region flag (3)
character*1 HST (nr__) ! HST region flag (4)
integer*4 OID (nr__) ! ? The optical catalog number,
* [MKZ2003] OID NNNN (5)
*Note (3): Y indicates the source is outside the central 10" region
* associated with nuclear emission.
*Note (4): Y indicates the source is in one or more of the HST
* observation regions.
*Note (5): Refers to the catalog number in table 3.
* A blank indicates the source has no counterpart in the HST data set.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! The Optical Source List
integer*4 nr__1
parameter (nr__1=1102) ! Number of records
character*75 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)
integer*4 OID_1 (nr__1) ! Optical catalog number, [MKZ2003] OID NNNN
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 (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*4 Vmag (nr__1) ! (mag) The V band magnitude
real*4 e_Vmag (nr__1) ! (mag) Error in Vmag
real*4 Imag (nr__1) ! (mag) The I band magnitude
real*4 e_Imag (nr__1) ! (mag) Error in Imag
real*4 V_I (nr__1) ! (mag) The V-I color
real*4 e_V_I (nr__1) ! (mag) Error in V-I
real*4 HLRad (nr__1) ! (arcsec) Half-light radius
real*4 e_HLRad (nr__1) ! (arcsec) Error in HLRad
character*1 CX (nr__1) ! [YN] Chandra FOV flag (1)
character*1 GC (nr__1) ! [YN] Globular cluster color flag (2)
integer*4 XID_1 (nr__1) ! ? X-ray counterpart ID number,
* [MKZ2003] XID NNN (3)
*Note (1): Y indicates the source is in the Chandra field of view
*Note (2): Y indicates the source has colors consistent with globular
* clusters (0.8<V-I<1.2)
*Note (3): Refers to the catalog number in table 1. A blank indicates
* the source has no counterpart in the Chandra data set.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! X-Ray/HST Matches
integer*4 nr__2
parameter (nr__2=30) ! Number of records
character*144 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)
integer*4 XID_2 (nr__2) ! X-ray catalog number, [MKZ2003] XID NNN
character*15 CXOMKZ_1 (nr__2) ! CXOMKZ source name (JHHMMSSs+DDMMSS)
real*4 Gamma_1 (nr__2) ! Best-fitting power-law spectral index
real*4 EGamma_2 (nr__2) ! ? 90% error in the positive direction (G1)
real*4 eGamma_3 (nr__2) ! ? 90% error in the positive direction (G1)
character*1 n_Gamma (nr__2) ! [fb] Note on Gamma (1)
real*4 SFlux_1 (nr__2) ! (mJy) (0.5-2.0keV) X-ray model flux (G2)
real*4 HFlux_1 (nr__2) ! (mJy) (2.0-8.0keV) X-ray model flux (G2)
real*4 XLum_1 (nr__2) ! (10-7W) (0.5-8.0keV) X-ray luminosity (G2)
real*4 Chi2_1 (nr__2) ! chi2 value of the spectral fit
integer*4 DOF_1 (nr__2) ! Degree of freedom of the spectral fit
integer*4 OID_2 (nr__2) ! Optical catalog number, [MKZ2003] OID NNNN
integer*4 RAh_1 (nr__2) ! (h) Right ascension (J2000)
integer*4 RAm_1 (nr__2) ! (min) Right ascension (J2000)
real*4 RAs_1 (nr__2) ! (s) Right ascension (J2000)
character*1 DE__1 (nr__2) ! Declination sign (J2000)
integer*4 DEd_1 (nr__2) ! (deg) Declination (J2000)
integer*4 DEm_1 (nr__2) ! (arcmin) Declination (J2000)
real*4 DEs_1 (nr__2) ! (arcsec) Declination (J2000)
real*4 Vmag_1 (nr__2) ! (mag) V magnitude
real*4 e_Vmag_1 (nr__2) ! (mag) rms uncertainty on Vmag
real*4 Imag_1 (nr__2) ! (mag) I magnitude
real*4 e_Imag_1 (nr__2) ! (mag) rms uncertainty on Imag
real*4 V_I_1 (nr__2) ! (mag) V-I colour index
real*4 e_V_I_1 (nr__2) ! (mag) rms uncertainty on V-I
real*4 HLRad_1 (nr__2) ! Half-light radius of the optical counterpart
real*4 e_HLRad_1 (nr__2) ! rms uncertainty on HLRad
*Note (1): Note on Gamma:
* f: fixed, b: bad fit
C=============================================================================
C Loading file 'table1.dat' ! The X-ray Source List
C Format for file interpretation
1 format(
+ I3,8X,A15,1X,F4.2,1X,F5.2,1X,F5.2,1X,E8.2,1X,E8.2,1X,E8.2,1X,
+ F5.1,1X,I2,1X,A1,1X,A1,1X,I4)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,147
read(1,'(A88)')ar__
read(ar__,1)
+ XID(i__),CXOMKZ(i__),Gamma(i__),EGamma(i__),eGamma_1(i__),
+ SFlux(i__),HFlux(i__),XLum(i__),Chi2(i__),DOF(i__),GR(i__),
+ HST(i__),OID(i__)
if(ar__(33:37) .EQ. '') EGamma(i__) = rNULL__
if(ar__(39:43) .EQ. '') eGamma_1(i__) = rNULL__
if(ar__(85:88) .EQ. '') OID(i__) = iNULL__
c ..............Just test output...........
write(6,1)
+ XID(i__),CXOMKZ(i__),Gamma(i__),EGamma(i__),eGamma_1(i__),
+ SFlux(i__),HFlux(i__),XLum(i__),Chi2(i__),DOF(i__),GR(i__),
+ HST(i__),OID(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! The Optical Source List
C Format for file interpretation
2 format(
+ I4,1X,I2,1X,I2,1X,F4.1,1X,A1,I1,1X,I2,1X,F4.1,1X,F5.2,1X,F4.2,
+ 1X,F5.2,1X,F4.2,1X,F4.2,1X,F4.2,1X,F4.1,1X,F3.1,1X,A1,1X,A1,
+ 1X,I3)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,1102
read(1,'(A75)')ar__1
read(ar__1,2)
+ OID_1(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),Vmag(i__),e_Vmag(i__),Imag(i__),e_Imag(i__),
+ V_I(i__),e_V_I(i__),HLRad(i__),e_HLRad(i__),CX(i__),GC(i__),
+ XID_1(i__)
if(ar__1(73:75) .EQ. '') XID_1(i__) = iNULL__
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)
+ OID_1(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),Vmag(i__),e_Vmag(i__),Imag(i__),e_Imag(i__),
+ V_I(i__),e_V_I(i__),HLRad(i__),e_HLRad(i__),CX(i__),GC(i__),
+ XID_1(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/HST Matches
C Format for file interpretation
3 format(
+ I3,8X,A15,1X,F4.2,1X,F4.2,1X,F4.2,A1,1X,E8.2,1X,E8.2,1X,E8.2,
+ 1X,F4.1,1X,I2,1X,I4,1X,I2,1X,I2,1X,F4.1,1X,A1,I1,1X,I2,1X,
+ F4.1,1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,F4.2,1X,F4.2,1X,F4.2,
+ F3.1)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,30
read(1,'(A144)')ar__2
read(ar__2,3)
+ XID_2(i__),CXOMKZ_1(i__),Gamma_1(i__),EGamma_2(i__),
+ eGamma_3(i__),n_Gamma(i__),SFlux_1(i__),HFlux_1(i__),
+ XLum_1(i__),Chi2_1(i__),DOF_1(i__),OID_2(i__),RAh_1(i__),
+ RAm_1(i__),RAs_1(i__),DE__1(i__),DEd_1(i__),DEm_1(i__),
+ DEs_1(i__),Vmag_1(i__),e_Vmag_1(i__),Imag_1(i__),
+ e_Imag_1(i__),V_I_1(i__),e_V_I_1(i__),HLRad_1(i__),
+ e_HLRad_1(i__)
if(ar__2(33:36) .EQ. '') EGamma_2(i__) = rNULL__
if(ar__2(38:41) .EQ. '') eGamma_3(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(6,3)
+ XID_2(i__),CXOMKZ_1(i__),Gamma_1(i__),EGamma_2(i__),
+ eGamma_3(i__),n_Gamma(i__),SFlux_1(i__),HFlux_1(i__),
+ XLum_1(i__),Chi2_1(i__),DOF_1(i__),OID_2(i__),RAh_1(i__),
+ RAm_1(i__),RAs_1(i__),DE__1(i__),DEd_1(i__),DEm_1(i__),
+ DEs_1(i__),Vmag_1(i__),e_Vmag_1(i__),Imag_1(i__),
+ e_Imag_1(i__),V_I_1(i__),e_V_I_1(i__),HLRad_1(i__),
+ e_HLRad_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=============================================================================
stop
end