Conversion of standardized ReadMe file for
file /./ftp/cats/J/MNRAS/388/849 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-19
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/MNRAS/388/849 NGC253 XMM observations (Barnard+, 2008)
*================================================================================
*A multi-coloured survey of NGC253 with XMM-Newton: testing the methods used for
*creating luminosity functions from low-count data.
* Barnard R., Greening L.S., Kolb U.
* <Mon. Not. R. Astron. Soc., 388, 849-862 (2008)>
* =2008MNRAS.388..849B
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'tablea1.dat' ! Positions of X-ray sources in the XMM-Newton
observations of NGC 253, along with some
observed properties
integer*4 nr__
parameter (nr__=185) ! Number of records
character*44 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 v_BGK2008_ (nr__) ! Source sequential number (G1)
integer*4 RAh (nr__) ! (h) Right ascension (J2000)
integer*4 RAm (nr__) ! (min) Right ascension (J2000)
real*4 RAs (nr__) ! (s) Right ascension (J2000)
character*1 DE_ (nr__) ! Declination sign (J2000)
integer*4 DEd (nr__) ! (deg) Declination (J2000)
integer*4 DEm (nr__) ! (arcmin) Declination (J2000)
real*4 DEs (nr__) ! (arcsec) Declination (J2000)
character*1 inD25 (nr__) ! [yn] indicates whether the source is within
* the D25 isophotal region of NGC 253
integer*4 Rs (nr__) ! (arcsec) Source extraction radius
real*4 Ab_As (nr__) ! Background-to-source area ratio
real*4 EEF (nr__) ! Encircled energy fraction (1)
*Note (1): Sources with an EEF of zero were detected, but no suitable
* spectra were obtained.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'tablea2.dat' ! Spectral properties for each source from
Observation 2
integer*4 nr__1
parameter (nr__1=185) ! Number of records
character*105 ar__1 ! Full-size record
integer*4 v_BGK2008__1(nr__1) ! Source sequential number (G1)
integer*4 CtPN (nr__1) ! (ct) pn source counts
integer*4 CtMOS (nr__1) ! (ct) MOS source counts
character*10 Mod (nr__1) ! Best fitting model (1)
real*4 NH (nr__1) ! (10+22cm-2) ? Absorption
real*4 e_NH (nr__1) ! (10+22cm-2) ? rms uncertainty on NH at
* 90% confidence level
character*1 f_NH (nr__1) ! [f] f for fixed absorption
real*4 Param (nr__1) ! ? Parameter (spectral index or
* temperature) (2)
real*4 e_Param (nr__1) ! ? rms uncertainty on Param at
* 90% confidence level
real*4 Param2 (nr__1) ! ? Second parameter value (spectral index or
* temperature) (2)
real*4 e_Param2 (nr__1) ! ? rms uncertainty on Param2 at
* 90% confidence level
real*4 chi2 (nr__1) ! ? chi^2^ value
integer*4 DOF (nr__1) ! ? Degree Of Freedom (3)
real*4 gf (nr__1) ! ? Good fit probability
real*8 LBF (nr__1) ! (10+29W) ? Best-fitting luminosity
real*8 e_LBF (nr__1) ! (10+29W) ? rms uncertainty on LBF at
* 90% confidence level
real*8 LSM (nr__1) ! (10+29W) ?=0. Standard model (Method I) luminosity
*Note (1): Best-fitting models for bright sources can be as follows:
* PO = a power law
* BB = blackbody
* BR = bremsstrahlung
* 2C = a two-component model consisting of a BB plus power law
* Faint sources are modelled using a best-fitting power law:
* -----------------------------------------------------------------------------
* Model NFnt NH/10^20^ Gamma chi2/dof [gf] Flux(pn thin) Flux (MOS med)
* -----------------------------------------------------------------------------
* IS 7 1.3 0.4 (.03) 71/54 [0.06] 12000(200) 36000(8000)
* OS 36 1.3 1.23(.13) 55/44 [0.12] 4800(400) 19000(2000)
* -----------------------------------------------------------------------------
*Note (2): Parameter (spectral index or temperature), spectral index for
* PO models, temperature for BB and BR models, spectral index and
* temperature for 2C models.
*Note (3): The quality of the spectrum may be deduced from the number of
* degrees of freedom because the spectra are grouped to a minimum number
* of counts per bin (brighter sources have more degrees of freedom).
C=============================================================================
C Loading file 'tablea1.dat' ! Positions of X-ray sources in the XMM-Newton
* observations of NGC 253, along with some
* observed properties
C Format for file interpretation
1 format(
+ I3,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F5.2,1X,A1,1X,I2,1X,
+ F5.2,1X,F4.2)
C Effective file loading
open(unit=1,status='old',file=
+'tablea1.dat')
write(6,*) '....Loading file: tablea1.dat'
do i__=1,185
read(1,'(A44)')ar__
read(ar__,1)
+ v_BGK2008_(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),inD25(i__),Rs(i__),Ab_As(i__),EEF(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(6,1)
+ v_BGK2008_(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),inD25(i__),Rs(i__),Ab_As(i__),EEF(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 'tablea2.dat' ! Spectral properties for each source from
* Observation 2
C Format for file interpretation
2 format(
+ I3,1X,I5,1X,I5,1X,A10,F5.3,F5.3,A1,2X,F5.3,1X,F5.3,1X,F4.2,
+ F4.2,2X,F5.1,1X,I3,1X,F5.3,1X,F9.2,1X,F9.2,2X,F7.2)
C Effective file loading
open(unit=1,status='old',file=
+'tablea2.dat')
write(6,*) '....Loading file: tablea2.dat'
do i__=1,185
read(1,'(A105)')ar__1
read(ar__1,2)
+ v_BGK2008__1(i__),CtPN(i__),CtMOS(i__),Mod(i__),NH(i__),
+ e_NH(i__),f_NH(i__),Param(i__),e_Param(i__),Param2(i__),
+ e_Param2(i__),chi2(i__),DOF(i__),gf(i__),LBF(i__),e_LBF(i__),
+ LSM(i__)
if(ar__1(27:31) .EQ. '') NH(i__) = rNULL__
if(ar__1(32:36) .EQ. '') e_NH(i__) = rNULL__
if(ar__1(40:44) .EQ. '') Param(i__) = rNULL__
if(ar__1(46:50) .EQ. '') e_Param(i__) = rNULL__
if(ar__1(52:55) .EQ. '') Param2(i__) = rNULL__
if(ar__1(56:59) .EQ. '') e_Param2(i__) = rNULL__
if(ar__1(62:66) .EQ. '') chi2(i__) = rNULL__
if(ar__1(68:70) .EQ. '') DOF(i__) = iNULL__
if(ar__1(72:76) .EQ. '') gf(i__) = rNULL__
if(ar__1(78:86) .EQ. '') LBF(i__) = rNULL__
if(ar__1(88:96) .EQ. '') e_LBF(i__) = rNULL__
c ..............Just test output...........
write(6,2)
+ v_BGK2008__1(i__),CtPN(i__),CtMOS(i__),Mod(i__),NH(i__),
+ e_NH(i__),f_NH(i__),Param(i__),e_Param(i__),Param2(i__),
+ e_Param2(i__),chi2(i__),DOF(i__),gf(i__),LBF(i__),e_LBF(i__),
+ LSM(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end