Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/696/924 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/696/924 UV and X-Ray radio-quiet QSOs (Gibson+, 2009)
*================================================================================
*X-ray insights into the physics of mini-BAL quasar outflows.
* Gibson R.R., Brandt W.N., Gallagher S.C., Schneider D.P.
* <Astrophys. J., 696, 924-940 (2009)>
* =2009ApJ...696..924G
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! UV and X-Ray radio-quiet source properties
integer*4 nr__
parameter (nr__=256) ! Number of records
character*146 ar__ ! Full-size record
character*19 SDSS (nr__) ! SDSS-DR5 name (JHHMMSS.ss+DDMMSS.s)
real*4 z (nr__) ! SDSS-DR5 redshift
character*10 ObsID (nr__) ! Chandra (four-digit) or XMM (ten-digit)
* observation number
real*4 ExpT (nr__) ! (ks) Exposure time
real*4 AI (nr__) ! (km/s) Absorption index for CIV{lambda}1549
real*4 BI (nr__) ! (km/s) Extended balnicity index, BI_0_, for CIV1549
integer*4 V_min (nr__) ! (km/s) ? Outflow velocity corresponding to the
* longest CIV wavelength (1)
integer*4 V_max (nr__) ! (km/s) ? Outflow velocity corresponding to the
* shortest CIV wavelength (1)
real*4 logLuv (nr__) ! ([10-7W/Hz]) Log monochromatic luminosity at 2500{AA}
real*4 SN1700 (nr__) ! Signal to noise ratio (2)
character*1 l_logLx (nr__) ! Limit flag on logLx
real*4 logLx (nr__) ! ([10-7W/Hz]) Log monochromatic luminosity at 2keV
real*4 e_logLx (nr__) ! ([10-7W/Hz]) ? logLx uncertainty (3)
real*4 HR (nr__) ! ? Hardness ratio (4)
real*4 e_HR (nr__) ! ? Error on HR computed formally
real*4 Gamma (nr__) ! ? Power-law photon index {Gamma}
real*4 e_Gamma (nr__) ! ? Gamma uncertainty
character*1 l_Aox (nr__) ! Limit flag on Aox
real*4 Aox (nr__) ! Optical-to-X-ray spectral index
real*4 e_Aox (nr__) ! ? Aox uncertainty
character*1 l_DAox (nr__) ! Limit flag on DAox
real*4 DAox (nr__) ! Difference between measured and predicted
* {alpha}_ox_
real*4 e_DAox (nr__) ! ? DAox uncertainty
*Note (1): We define {nu}_max_ as the outflow velocity corresponding to the
* shortest wavelength which is identified as part of a CIV mini-BAL or
* BAL trough. Similarly, {nu}_min_ is the outflow velocity associated
* with the longest wavelength in a trough. See section 3.3 for further
* details.
*Note (2): SN_1700_ is defined as the median of the flux divided by the
* noise (as reported by the SDSS pipeline) for all spectral bins in
* the 1650-1700{AA} region.
*Note (3): Errors are estimated using the method in Section 2.2
*Note (4): The hardness ratio, HR=(H-S)/(H+S) is calculated from H, the
* number of X-ray counts with observed-frame energies of 2-8keV, and S,
* the number of counts with observed-frame energies in the 0.5-2keV
* range. See section 3.2 for further details.
C=============================================================================
C Loading file 'table2.dat' ! UV and X-Ray radio-quiet source properties
C Format for file interpretation
1 format(
+ A19,1X,F5.3,1X,A10,1X,F5.1,1X,F6.1,1X,F6.1,1X,I6,1X,I6,1X,
+ F6.3,1X,F4.1,1X,A1,F6.3,1X,F5.3,1X,F5.2,1X,F4.2,1X,F5.2,1X,
+ F4.2,1X,A1,F6.3,1X,F5.3,1X,A1,F6.3,1X,F5.3)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,256
read(1,'(A146)')ar__
read(ar__,1)
+ SDSS(i__),z(i__),ObsID(i__),ExpT(i__),AI(i__),BI(i__),
+ V_min(i__),V_max(i__),logLuv(i__),SN1700(i__),l_logLx(i__),
+ logLx(i__),e_logLx(i__),HR(i__),e_HR(i__),Gamma(i__),
+ e_Gamma(i__),l_Aox(i__),Aox(i__),e_Aox(i__),l_DAox(i__),
+ DAox(i__),e_DAox(i__)
if(ar__(58:63) .EQ. '') V_min(i__) = iNULL__
if(ar__(65:70) .EQ. '') V_max(i__) = iNULL__
if(ar__(92:96) .EQ. '') e_logLx(i__) = rNULL__
if(ar__(98:102) .EQ. '') HR(i__) = rNULL__
if(ar__(104:107) .EQ. '') e_HR(i__) = rNULL__
if(ar__(109:113) .EQ. '') Gamma(i__) = rNULL__
if(ar__(115:118) .EQ. '') e_Gamma(i__) = rNULL__
if(ar__(128:132) .EQ. '') e_Aox(i__) = rNULL__
if(ar__(142:146) .EQ. '') e_DAox(i__) = rNULL__
c ..............Just test output...........
write(6,1)
+ SDSS(i__),z(i__),ObsID(i__),ExpT(i__),AI(i__),BI(i__),
+ V_min(i__),V_max(i__),logLuv(i__),SN1700(i__),l_logLx(i__),
+ logLx(i__),e_logLx(i__),HR(i__),e_HR(i__),Gamma(i__),
+ e_Gamma(i__),l_Aox(i__),Aox(i__),e_Aox(i__),l_DAox(i__),
+ DAox(i__),e_DAox(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end