Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/510/637 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-19
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/510/637 Near IR properties of Galaxy disks (Hunt+ 1999)
*================================================================================
*The Disks of Galaxies with Seyfert and Starburst Nuclei.
*II. Near-Infrared Structural Properties
* Hunt L. K., Malkan M. A., Moriondo G., Salvati M.
* <Astrophys. J. 510, 637 (1999)>
* =1999ApJ...510..637H
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Near IR structural parameters
integer*4 nr__
parameter (nr__=24) ! Number of records
character*161 ar__ ! Full-size record
character*8 Name (nr__) ! Galaxy name
real*4 Dist (nr__) ! (Mpc) Distance (1)
integer*4 NBest (nr__) ! Best fitting bulge exponent
character*1 u_NBest (nr__) ! [:] colon signifies ill-determined
real*4 epsil (nr__) ! ? Ellipticity of the bulge
real*4 e_epsil (nr__) ! ? Uncertainty in epsil of the bulge
real*4 angBsiz (nr__) ! (arcsec) ? Angular scale length of the bulge
real*4 e_angBsiz (nr__) ! (arcsec) ? Uncertainty in angBsiz of the bulge
real*4 phyBsiz (nr__) ! (kpc) ? Physical scale length of the bulge
real*4 KmagB (nr__) ! (mag/arcsec2) ? Surface brightness in K band of
* the bulge (2)
real*4 e_KmagB (nr__) ! (mag/arcsec2) ? Uncertainty in SB of the bulge
real*4 J_K (nr__) ! (mag) ? J-K color of the bulge
real*4 H_K (nr__) ! (mag) ? H-K color of the bulge
real*4 KMagB_1 (nr__) ! (mag) ? Absolute K band magnitude of the bulge
real*4 incl (nr__) ! (deg) ? Inclination of the disk
real*4 e_incl (nr__) ! (deg) ? Uncertainty in incl
real*4 angDsiz (nr__) ! (arcsec) ? Angular scale length of the disk
real*4 e_angDsiz (nr__) ! (arcsec) ? Uncertainty in SLD
real*4 phyDsiz (nr__) ! (kpc) ? Physical scale length of the disk
real*4 SBD (nr__) ! (mag/arcsec2) ? Surface brightness in K band of
* the disk (2)
real*4 e_SBD (nr__) ! (mag/arcsec2) ? Uncertainty in SBD of the disk
real*4 v_J_K_D (nr__) ! (mag) ? J-K color of the disk
real*4 v_H_K_D (nr__) ! (mag) ? H-K color of the disk
real*4 KMagD (nr__) ! (mag) ? Absolute K band magnitude of the disk
real*4 KMagG (nr__) ! (mag) Absolute K band magnitude of the galaxy
real*4 chi2 (nr__) ! {chi}^2^ of the NBest
*Note (1): Distances are calculated according to the precepts of the RC3
* H_o_=75 km.s-1.Mpc-1
*Note (2): Surface brightness has been corrected for Galactic extinction
* and redshift as in Hunt+ 1997 (1997ApJS..108..229H), and transformed
* to face-on values assuming optical transparency (see Moriondo+ 1998a
* 1998A&AS..130...81M)
C=============================================================================
C Loading file 'table1.dat' ! Near IR structural parameters
C Format for file interpretation
1 format(
+ A8,2X,F5.1,1X,I1,A1,2X,F5.3,2X,F4.2,1X,F5.2,2X,F4.2,2X,F4.2,
+ 2X,F5.2,2X,F4.2,2X,F4.2,2X,F5.2,2X,F6.2,2X,F4.1,2X,F4.1,2X,
+ F5.2,2X,F4.2,1X,F4.2,2X,F5.2,2X,F4.2,2X,F4.2,2X,F4.2,2X,F6.2,
+ 2X,F6.2,3X,F4.1)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,24
read(1,'(A161)')ar__
read(ar__,1)
+ Name(i__),Dist(i__),NBest(i__),u_NBest(i__),epsil(i__),
+ e_epsil(i__),angBsiz(i__),e_angBsiz(i__),phyBsiz(i__),
+ KmagB(i__),e_KmagB(i__),J_K(i__),H_K(i__),KMagB_1(i__),
+ incl(i__),e_incl(i__),angDsiz(i__),e_angDsiz(i__),
+ phyDsiz(i__),SBD(i__),e_SBD(i__),v_J_K_D(i__),v_H_K_D(i__),
+ KMagD(i__),KMagG(i__),chi2(i__)
if(ar__(21:25) .EQ. '') epsil(i__) = rNULL__
if(ar__(28:31) .EQ. '') e_epsil(i__) = rNULL__
if(ar__(33:37) .EQ. '') angBsiz(i__) = rNULL__
if(ar__(40:43) .EQ. '') e_angBsiz(i__) = rNULL__
if(ar__(46:49) .EQ. '') phyBsiz(i__) = rNULL__
if(ar__(52:56) .EQ. '') KmagB(i__) = rNULL__
if(ar__(59:62) .EQ. '') e_KmagB(i__) = rNULL__
if(ar__(65:68) .EQ. '') J_K(i__) = rNULL__
if(ar__(71:75) .EQ. '') H_K(i__) = rNULL__
if(ar__(78:83) .EQ. '') KMagB_1(i__) = rNULL__
if(ar__(86:89) .EQ. '') incl(i__) = rNULL__
if(ar__(92:95) .EQ. '') e_incl(i__) = rNULL__
if(ar__(98:102) .EQ. '') angDsiz(i__) = rNULL__
if(ar__(105:108) .EQ. '') e_angDsiz(i__) = rNULL__
if(ar__(110:113) .EQ. '') phyDsiz(i__) = rNULL__
if(ar__(116:120) .EQ. '') SBD(i__) = rNULL__
if(ar__(123:126) .EQ. '') e_SBD(i__) = rNULL__
if(ar__(129:132) .EQ. '') v_J_K_D(i__) = rNULL__
if(ar__(135:138) .EQ. '') v_H_K_D(i__) = rNULL__
if(ar__(141:146) .EQ. '') KMagD(i__) = rNULL__
c ..............Just test output...........
write(6,1)
+ Name(i__),Dist(i__),NBest(i__),u_NBest(i__),epsil(i__),
+ e_epsil(i__),angBsiz(i__),e_angBsiz(i__),phyBsiz(i__),
+ KmagB(i__),e_KmagB(i__),J_K(i__),H_K(i__),KMagB_1(i__),
+ incl(i__),e_incl(i__),angDsiz(i__),e_angDsiz(i__),
+ phyDsiz(i__),SBD(i__),e_SBD(i__),v_J_K_D(i__),v_H_K_D(i__),
+ KMagD(i__),KMagG(i__),chi2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end