Conversion of standardized ReadMe file for
file /./ftp/cats/J/MNRAS/468/4735 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/MNRAS/468/4735 Spectral evolution of 4U 1543-47 in 2002 (Lipunova+, 2017)
*================================================================================
*Determination of the turbulent parameter in accretion discs:
*effects of self-irradiation in 4U 1543-47 during the 2002 outburst.
* Lipunova G.V., Malanchev K.L.
* <Mon. Not. R. Astron. Soc., 468, 4735-4747 (2017)>
* =2017MNRAS.468.4735L (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'figure1.dat' ! Evolution of spectral parameters of
4U 1543-47 during the 2002 outburst
integer*4 nr__
parameter (nr__=58) ! Number of records
character*302 ar__ ! Full-size record
character*15 ObsID (nr__) ! Observation ID (1)
real*8 tbegin (nr__) ! (s) Observation start (Julian date)
real*8 tend (nr__) ! (s) Observation end (Julian date)
real*8 chi2 (nr__) ! Chi-square of the spectral fit (2)
integer*4 dof (nr__) ! Number of degrees of freedom of the
* spectral fit (3)
real*4 FDisc_min (nr__) ! (mW/m2) Lower boundary of 1-sigma confidence
* interval on the disc flux (4)
real*4 FDisc_max (nr__) ! (mW/m2) Upper boundary of 1-sigma confidence
* interval on the disc flux (4)
real*4 FTot_min (nr__) ! (mW/m2) Lower boundary of 1-sigma confidence
* interval on the total flux (5)
real*4 FTot_max (nr__) ! (mW/m2) Upper boundary of 1-sigma confidence
* interval on the total flux (5)
real*8 Gamma (nr__) ! Best-fit value of the photon power law index
* in the spectral component simpl
real*8 b_Gamma (nr__) ! Lower boundary of 1-sigma confidence
* interval for Gamma
real*8 B_Gamma_1 (nr__) ! Upper boundary of 1-sigma confidence
* interval for Gamma
real*8 FracSctr (nr__) ! Best-fit value of the scattered fraction in
* the spectral component simpl
real*8 b_FracSctr (nr__) ! Lower boundary of 1-sigma confidence
* interval for FracSctr
real*8 B_FracSctr_1(nr__) ! Upper boundary of 1-sigma confidence
* interval for FracSctr
real*8 dotM (nr__) ! (10+18g/s) Best-fit value of the mass accretion rate of
* the disc in the spectral component kerrbb
real*8 b_dotM (nr__) ! (10+18g/s) Lower boundary of 1-sigma confidence
* interval for dotM
real*8 B_dotM_1 (nr__) ! (10+18g/s) Upper boundary of 1-sigma confidence
* interval for dotM
real*8 dist (nr__) ! (kpc) Best-fit value of the distance in the
* spectral component kerrbb (6)
real*8 b_dist (nr__) ! (kpc) ?=99.99 Lower boundary of 1-sigma confidence
* interval for dist (6)
real*8 B_dist_1 (nr__) ! (kpc) ?=99.99 Upper boundary of 1-sigma confidence
* interval for dist (6)
real*8 LineE (nr__) ! (keV) Best-fit value of the line energy in the
* spectral component laor
real*8 b_LineE (nr__) ! (keV) ?=0 Lower boundary of 1-sigma confidence
* interval for LineE
real*8 B_LineE_1 (nr__) ! (keV) ?=0 Upper boundary of 1-sigma confidence
* interval for LineE
real*8 norm (nr__) ! (ph/cm2/s) Best-fit value of the photon flux in the
* spectral component laor
real*8 b_norm (nr__) ! (ph/cm2/s) ?=99.99 Lower boundary of 1-sigma confidence
* interval for norm
real*8 B_norm_1 (nr__) ! (ph/cm2/s) Upper boundary of 1-sigma confidence
* interval for norm
real*8 edgeE (nr__) ! (keV) Best-fit value of the threshold energy in
* the spectral component smedge
real*8 b_edgeE (nr__) ! (keV) ?=99.99 Lower boundary of 1-sigma confidence
* interval for edgeE
real*8 B_edgeE_1 (nr__) ! (keV) Upper boundary of 1-sigma confidence
* interval for edgeE
real*8 MaxTau (nr__) ! Best-fit value of the maximum absorption
* factor at threshold in the spectral
* component smedge
real*8 b_MaxTau (nr__) ! ?=99.99 Lower boundary of 1-sigma confidence
* interval for MaxTau
real*8 B_MaxTau_1 (nr__) ! Upper boundary of 1-sigma confidence
* interval for MaxTau
*Note (1): Some rows have the same ObsID because an original observation
* was divided in two parts.
*Note (2): The XSPEC spectral model consists of the following spectral
* components: TBabs((simpl*kerrbb+laor)smedge). Full description of the
* spectral parameters can be found in Table A1 and Appendix A of the paper.
*Note (3): The number of the degrees of freedom depends on whether the parameter
* dist of the spectral component kerrbb is fixed or not (see also the caption
* of Figure 1 in the paper).
* dof=40 if the distance to the source was estimated during fitting,
* dof=41 if the distance was fixed. The number of the spectral channels
* is 49 for all observations. The total number of the spectral model
* parameters, free and frozen, is 24.
*Note (4): The model flux before absorption in the energy band 0.05-50 keV
* of the following spectral model components: (kerrbb+laor)smedge.
*Note (5): The model flux before absorption in the energy band 0.05-50 keV
* of the following spectral model components:
* (simpl*kerrbb+laor)smedge.
*Note (6): If the lower and upper boundaries of parameter dist are
* unspecified, this means that the distance was fixed during fitting.
C=============================================================================
C Loading file 'figure1.dat' ! Evolution of spectral parameters of
* 4U 1543-47 during the 2002 outburst
C Format for file interpretation
1 format(
+ A15,1X,F16.8,1X,F16.8,1X,F7.4,1X,I2,1X,E10.5,1X,E10.5,1X,
+ E10.5,1X,E10.5,1X,F7.5,1X,F7.5,1X,F7.5,1X,F7.5,1X,F7.5,1X,
+ F7.5,1X,F8.5,1X,F8.5,1X,F8.5,1X,F8.5,1X,F8.5,1X,F8.5,1X,F7.5,
+ 1X,F7.5,1X,F7.5,1X,F7.5,1X,F7.5,1X,F7.5,1X,F7.5,1X,F7.5,1X,
+ F7.5,1X,F7.5,1X,F7.5,1X,F7.5)
C Effective file loading
open(unit=1,status='old',file=
+'figure1.dat')
write(6,*) '....Loading file: figure1.dat'
do i__=1,58
read(1,'(A302)')ar__
read(ar__,1)
+ ObsID(i__),tbegin(i__),tend(i__),chi2(i__),dof(i__),
+ FDisc_min(i__),FDisc_max(i__),FTot_min(i__),FTot_max(i__),
+ Gamma(i__),b_Gamma(i__),B_Gamma_1(i__),FracSctr(i__),
+ b_FracSctr(i__),B_FracSctr_1(i__),dotM(i__),b_dotM(i__),
+ B_dotM_1(i__),dist(i__),b_dist(i__),B_dist_1(i__),LineE(i__),
+ b_LineE(i__),B_LineE_1(i__),norm(i__),b_norm(i__),
+ B_norm_1(i__),edgeE(i__),b_edgeE(i__),B_edgeE_1(i__),
+ MaxTau(i__),b_MaxTau(i__),B_MaxTau_1(i__)
c ..............Just test output...........
write(6,1)
+ ObsID(i__),tbegin(i__),tend(i__),chi2(i__),dof(i__),
+ FDisc_min(i__),FDisc_max(i__),FTot_min(i__),FTot_max(i__),
+ Gamma(i__),b_Gamma(i__),B_Gamma_1(i__),FracSctr(i__),
+ b_FracSctr(i__),B_FracSctr_1(i__),dotM(i__),b_dotM(i__),
+ B_dotM_1(i__),dist(i__),b_dist(i__),B_dist_1(i__),LineE(i__),
+ b_LineE(i__),B_LineE_1(i__),norm(i__),b_norm(i__),
+ B_norm_1(i__),edgeE(i__),b_edgeE(i__),B_edgeE_1(i__),
+ MaxTau(i__),b_MaxTau(i__),B_MaxTau_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end