Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJS/143/315 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/ApJS/143/315 IRAS 1Jy sample of ultraluminous galaxies. II. (Veilleux+, 2002)
*================================================================================
*Optical and near-infrared imaging of the IRAS 1Jy sample of ultraluminous
*galaxies. II. The analysis.
* Veilleux S., Kim D.-C., Sanders D.B.
* <Astrophys. J. Suppl. Ser. 143, 315 (2002)>
* =2002ApJS..143..315V
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Morphological Parameters
integer*4 nr__
parameter (nr__=118) ! Number of records
character*34 ar__ ! Full-size record
character*11 IRAS ! IRAS FSC name
real*4 NS ! (kpc) ? Nuclear separation
integer*4 TL ! (kpc) ? Tail length
character*4 IC ! Interaction class
character*3 MType ! Spectral type (1)
*Note (1): Spectral type:
* HII: H II region galaxy
* L: LINER
* S2: Seyfert 2
* S1: Seyfert 1
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Parameters of Surface Brightness Profiles
integer*4 nr__1
parameter (nr__1=127) ! Number of records
character*80 ar__1 ! Full-size record
character*11 IRAS_1 ! IRAS name (1)
character*2 m_IRAS ! Component (1)
integer*4 RPSF ! (%) ? Percent of R band PSF relative to the galaxy
integer*4 KPSF ! (%) ? Percent of K' band PSF relative to the galaxy
real*4 Rexp ! Reduced R band {chi}^2^ value fitted to the
* exponential profile
real*4 RdeV ! Reduced R band {chi}^2^ value fitted to the
* de Vaucouleurs's r^1/4^ law profile
real*4 Kexp ! Reduced K' band {chi}^2^ value fitted to the
* exponential profile
real*4 KdeV ! Reduced K' band {chi}^2^ value fitted to the
* de Vaucouleurs's r^1/4^ law profile
character*3 BFit ! Best fitted profile (2)
real*4 RRad ! (kpc) ? R band seeing-deconvolved half-light
* (effective) radius for E and E/D objects
real*4 KRad ! (kpc) ? K' band seeing-deconvolved half-light
* (effective) radius for E and E/D objects
real*4 RSB ! (mag/arcsec2) ? R band effective surface brightness (3)
real*4 KSB ! (mag/arcsec2) ? K' band effective surface brightness (3)
real*4 RMag ! (mag) ? Absolute R band host galaxy magnitude
real*4 KMag ! (mag) Absolute K' band host galaxy magnitude
*Note (1): See text for details. [KVS2002] HHMMm+DDMM WW in Simbad.
*Note (2): Best fitted profile code:
* A = ambiguous;
* E = elliptical-like;
* D = disk-like;
* E/D = border-line object between E and D.
*Note (3): Not corrected for cosmological dimming.
C=============================================================================
C Loading file 'table1.dat' ! Morphological Parameters
C Format for file interpretation
1 format(A11,1X,F4.1,1X,I2,1X,A4,2X,A3)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,118
read(1,'(A34)')ar__
read(ar__,1)IRAS,NS,TL,IC,MType
if(ar__(13:16) .EQ. '') NS = rNULL__
if(ar__(18:19) .EQ. '') TL = iNULL__
c ..............Just test output...........
write(6,1)IRAS,NS,TL,IC,MType
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! Parameters of Surface Brightness Profiles
C Format for file interpretation
2 format(
+ A11,1X,A2,1X,I2,1X,I2,1X,F4.1,1X,F5.1,1X,F5.1,1X,F5.1,1X,A3,
+ 1X,F3.1,1X,F3.1,1X,F4.1,1X,F4.1,1X,F6.2,1X,F6.2)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,127
read(1,'(A80)')ar__1
read(ar__1,2)
+ IRAS_1,m_IRAS,RPSF,KPSF,Rexp,RdeV,Kexp,KdeV,BFit,RRad,KRad,
+ RSB,KSB,RMag,KMag
if(ar__1(16:17) .EQ. '') RPSF = iNULL__
if(ar__1(19:20) .EQ. '') KPSF = iNULL__
if(ar__1(49:51) .EQ. '') RRad = rNULL__
if(ar__1(53:55) .EQ. '') KRad = rNULL__
if(ar__1(57:60) .EQ. '') RSB = rNULL__
if(ar__1(62:65) .EQ. '') KSB = rNULL__
if(ar__1(67:72) .EQ. '') RMag = rNULL__
c ..............Just test output...........
write(6,2)
+ IRAS_1,m_IRAS,RPSF,KPSF,Rexp,RdeV,Kexp,KdeV,BFit,RRad,KRad,
+ RSB,KSB,RMag,KMag
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end