Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/420/97 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/A+A/420/97 Tully-Fisher relation at 0.1<z<1.0 (Boehm+, 2004)
*================================================================================
*The Tully-Fisher relation at intermediate redshift.
* Boehm A., Ziegler B.L., Saglia R.P., Bender R., Fricke K.J., Gabasch A.,
* Heidt J., Mehlert D., Noll S., Seitz S.
* <Astron. Astrophys. 420, 97 (2004)>
* =2004A&A...420...97B
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Photometric and kinematic data on 77 spirals
in the FORS Deep Field
integer*4 nr__
parameter (nr__=77) ! Number of records
character*80 ar__ ! Full-size record
integer*4 FDF ! FORS Deep Field photometric catalogue number
* (as in Cat. <J/A+A/398/49>)
integer*4 i ! (deg) Disk inclination angle (0 = face-on)
integer*4 delta ! (deg) Misalignment angle between disk major axis
* and slitlet
real*4 rd ! (arcsec) Exponential disk scale length (1)
real*4 z ! Spectroscopic redshift
integer*4 TType ! SED classifier in the de Vaucouleurs scheme
real*4 Xmag ! (mag) Total apparent magnitude in filter X (2)
real*4 kB ! (mag) K-correction (to rest-frame Johnson B)
real*4 AX ! (mag) Galactic absorption (in filter X)
real*4 AB ! (mag) Intrinsic absorption in rest-frame B (3)
real*4 m_M ! (mag) Distance modulus (4)
real*4 BMAG ! (mag) B-band absolute magnitude
real*4 e_BMAG ! (mag) Error on B-band absolute magnitude
integer*4 Vmax ! (km/s) Intrinsic maximum rotation velocity (5)
integer*4 e_Vmax ! (km/s) Error on intrinsic maximum rotation velocity
real*4 B_R ! (mag) Rest-frame extinction-corrected B-R color index
character*1 Qual ! Rotation curve quality (6)
*Note (1): Structural parameters were derived from 2-D surface brightness
* profile fitting on ground-based images taking into account the seeing.
* According to our simulations, the disk scale length is not a crucial
* input parameter for the determination of Vmax in the case of distant
* spirals. However, some values of rd may be affected by the limitations
* of the ground-based imaging. We therefore recommend not to use these
* scale lengths for applications like the Fundamental Plane of spiral
* galaxies.
*Note (2): Apparent magnitude is given for the filter X which best matches
* the rest-frame B-band. For objects with z<0.25, this is the B-band, in
* the range 0.25<z<0.55 the g-band was used, for 0.55<z<0.85, the R-band
* was used, and at z>0.85 the I-band.
*Note (3): Intrinsic absorption is computed following Tully & Fouque
* (1985ApJS...58...67T).
*Note (4): Adopting the concordance cosmology with {Omega}_{lambda}_=0.7,
* {Omega}_m_=0.3 and H_0_=70km/s/Mpc.
*Note (5): Derived via synthetic velocity fields assuming a linear rise
* of the rotation velocity at small galactocentric radii and a flat
* rotation curve at large radii ("rise-turnover-flat" shape).
*Note (6): Quality flags:
* "H" - High quality, symmetric rotation curves with a clearly visible
* flat part at large radii. These objects are usable for
* Tully-Fisher applications.
* "L" - Low quality rotation curves with relatively small spatial
* extent and/or asymmetric shapes.
C=============================================================================
C Loading file 'table1.dat' ! Photometric and kinematic data on 77 spirals
* in the FORS Deep Field
C Format for file interpretation
1 format(
+ I4,1X,I2,1X,I2,1X,F4.2,1X,F6.4,1X,I2,1X,F5.2,1X,F5.2,1X,F4.2,
+ 1X,F4.2,1X,F5.2,1X,F6.2,1X,F4.2,1X,I3,1X,I3,1X,F4.2,1X,A1)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,77
read(1,'(A80)')ar__
read(ar__,1)
+ FDF,i,delta,rd,z,TType,Xmag,kB,AX,AB,m_M,BMAG,e_BMAG,Vmax,
+ e_Vmax,B_R,Qual
c ..............Just test output...........
write(6,1)
+ FDF,i,delta,rd,z,TType,Xmag,kB,AX,AB,m_M,BMAG,e_BMAG,Vmax,
+ e_Vmax,B_R,Qual
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end