Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/713/L11 into FORTRAN code for reading data files line by line.
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/713/L11 X-ray properties of Seyfert 1 galaxies (Zhou+, 2010)
*================================================================================
*A comparison of hard X-ray photon indices and iron k{alpha} emission lines in
*X-ray luminous narrow- and broad-line Seyfert 1 galaxies.
* Zhou X.-L., Zhang S.-N.
* <Astrophys. J., 713, L11-L15 (2010)>
* =2010ApJ...713L..11Z
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! XMM-Newton flux-limited sample of Seyfert 1 galaxies
integer*4 nr__
parameter (nr__=114) ! Number of records
character*71 ar__ ! Full-size record
character*15 Name ! Source name
character*4 Type ! Source type (1)
real*4 Flux ! (fW/m2) Absorption-corrected 2-10keV flux in
* units of 10^-12^erg/s/cm^2^
real*4 Gamma ! The 2-10keV photon index {Gamma}
real*4 e_Gamma ! Uncertainty in Gamma
character*2 l_EW ! [<~] Limit flag on EW
integer*4 EW ! (eV) ? Equivalent width of 6.4keV narrow Fe
* K{alpha} line (2)
integer*4 b_EW ! (eV) ? Lower limit value on EW
integer*4 B_EW_1 ! (eV) ? Upper limit value on EW
real*4 logLX ! ([10-7W]) Log of 2-10keV luminosity calculated from
* the 2-10keV flux
integer*4 W_Hb ! (km/s) ? FWHM of broad H{beta} line
character*1 f_W_Hb ! [a] W(Hb) derived from H{alpha} line (3)
real*4 logER ! ([-]) ? Log of Eddington ratio (4)
*Note (1): Source type as follows:
* NELG = Narrow-emission-line galaxy,
* NLS1 = Narrow line Seyfert 1 galaxy,
* BLS1 = Broad line Seyfert 1 galaxy.
* NELGs are intermediate Seyfert galaxies whose broad line regions are
* lightly obscured. We take NELGs with {Gamma}>2.0 as NLS1s in our
* analysis.
*Note (2): The intrinsic width is fixed at 10eV for the EW measurements.
*Note (3):
* a = Object with the FWHMH{beta} calculated from the FWHMH{alpha} using the
* relation FWHMH{beta}=1070*(FWHMH{alpha}/1000)^1.03^km/s given in
* Greene & Ho (2005ApJ...630..122G). This object has the FWHMH{alpha}
* measurement but lacks the FWHMH{beta} measurement. FWHMH{alpha} of
* these objects are taken from Pietsch et al. (1998A&A...333...48P),
* Rodriguez-Ardila et al. (2000ApJS..126...63R) and Piconcelli et al.
* (2006A&A...453..839P), respectively.
*Note (4): Calculated from the data available in Bianchi et al. (2009,
* Cat. J/A+A/495/421).
C=============================================================================
C Loading file 'table1.dat' ! XMM-Newton flux-limited sample of Seyfert 1 galaxies
C Format for file interpretation
1 format(
+ A15,1X,A4,1X,F6.2,1X,F4.2,1X,F4.2,1X,A2,1X,I3,1X,I3,1X,I3,1X,
+ F5.2,1X,I4,1X,A1,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,114
read(1,'(A71)')ar__
read(ar__,1)
+ Name,Type,Flux,Gamma,e_Gamma,l_EW,EW,b_EW,B_EW_1,logLX,W_Hb,
+ f_W_Hb,logER
if(ar__(42:44) .EQ. '') EW = iNULL__
if(ar__(46:48) .EQ. '') b_EW = iNULL__
if(ar__(50:52) .EQ. '') B_EW_1 = iNULL__
if(ar__(60:63) .EQ. '') W_Hb = iNULL__
if(ar__(67:71) .EQ. '') logER = rNULL__
c ..............Just test output...........
write(6,1)
+ Name,Type,Flux,Gamma,e_Gamma,l_EW,EW,b_EW,B_EW_1,logLX,W_Hb,
+ f_W_Hb,logER
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end