Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/546/694 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-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/546/694 NICMOS star formation history (Thompson +, 2001)
*================================================================================
*Star formation history in the NICMOS Northern Hubble Deep Field.
* Thompson R.I., Weymann R.J., Storrie-Lombardi L.J.
* <Astrophys. J. 546, 694 (2001)>
* =2001ApJ...546..694T
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Listing of measured quantities
integer*4 nr__
parameter (nr__=281) ! Number of records
character*104 ar__ ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg (nr__) ! (deg) Right Ascension J2000
real*8 DEdeg (nr__) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
real*8 NICMOS (nr__) ! NICMOS identification number (1)
character*8 v_WBD96_ (nr__) ! WFPC identification number from
* Williams et al., 1996, Cat. <J/AJ/112/1335>
real*4 z (nr__) ! Redshift
real*4 E_B_V (nr__) ! (mag) (B-V) color excess
real*8 SFR (nr__) ! (solMass/yr) Star formation rate determined in Section 5
real*4 Lum (nr__) ! (solLum) Bolometric luminosity (2)
real*4 Frac (nr__) ! Fraction of the luminosity removed by
* extinction and re-emitted in the
* mid & far-IR
real*4 SCUBA (nr__) ! (mJy) ? The SCUBA 850 microns flux
real*4 Temp (nr__) ! Template number of best fit between
* 1.0 (early-cold) and 6.0 (late-hot)
real*4 Chi2 (nr__) ! Modified Chi^2^ of the fit from Equ. 1 (3)
real*4 Totmag (nr__) ! (mag) ? The F160W AB magnitude (4)
real*4 Apmag (nr__) ! (mag) ? The 0.6" diameter aperture F160W magnitude
* See note (5)
integer*4 RAh (nr__) ! (h) Right Ascension (J2000)
integer*4 RAm (nr__) ! (min) Right Ascension (J2000)
real*4 RAs (nr__) ! (s) Right Ascension (J2000)
character*1 DE_ (nr__) ! Declination (J2000)
integer*4 DEd (nr__) ! (deg) Declination (J2000)
integer*4 DEm (nr__) ! (arcmin) Declination (J2000)
real*4 DEs (nr__) ! (arcsec) Declination (J2000)
*Note (1): Objects with ID numbers less than 1000 are objects that are
* identified with sources in the original KFOCAS catalog of Thompson et
* al., 1999, Cat. <J/AJ/117/17>, [TSW99] NNN.NNN in Simbad.
* Objects with catalog numbers greater than or equal to 1000 are
* SExtractor objects that did not match in position with an original
* catalog entry to within 0.3".
*Note (2): The flux of a galaxy is obtained by integrating over the
* unextincted selected template scaled by the factor A from equation 2.
* The bolometric luminosity then follows from the redshift and our
* adopted cosmology.
*Note (3): It should be noted that the distribution of the modified chi^2^
* values will not rigorously follow a true chi^2^ distribution. The
* values are provided to give a qualitative indication of the relative
* goodness of fit for the best fit values of redshift, template type and
* E(B-V) from object to object.
*Note (4): Derived from the aperture correction method described in
* Yan et al., 1998ApJ...503L..19Y.
*Note (5): If no magnitude is listed the object had a zero or negative
* measured F160W flux.
C=============================================================================
C Loading file 'table1.dat' ! Listing of measured quantities
C Format for file interpretation
1 format(
+ F10.5,1X,A8,1X,F4.2,1X,F4.2,1X,F7.3,1X,E8.2,1X,F4.2,1X,E8.2,
+ 1X,F3.1,1X,F4.1,1X,F4.1,1X,F4.1,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,
+ 1X,I2,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,281
read(1,'(A104)')ar__
read(ar__,1)
+ NICMOS(i__),v_WBD96_(i__),z(i__),E_B_V(i__),SFR(i__),Lum(i__),
+ Frac(i__),SCUBA(i__),Temp(i__),Chi2(i__),Totmag(i__),
+ Apmag(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__)
if(ar__(53:60) .EQ. '') SCUBA(i__) = rNULL__
if(ar__(71:74) .EQ. '') Totmag(i__) = rNULL__
if(ar__(76:79) .EQ. '') Apmag(i__) = rNULL__
RAdeg(i__) = rNULL__
DEdeg(i__) = rNULL__
c Derive coordinates RAdeg and DEdeg from input data
c (RAdeg and DEdeg are set to rNULL__ when unknown)
if(RAh(i__) .GT. -180) RAdeg(i__)=RAh(i__)*15.
if(RAm(i__) .GT. -180) RAdeg(i__)=RAdeg(i__)+RAm(i__)/4.
if(RAs(i__) .GT. -180) RAdeg(i__)=RAdeg(i__)+RAs(i__)/240.
if(DEd(i__) .GE. 0) DEdeg(i__)=DEd(i__)
if(DEm(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEm(i__)/60.
if(DEs(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEs(i__)/3600.
if(DE_(i__).EQ.'-'.AND.DEdeg(i__).GE.0) DEdeg(i__)=-DEdeg(i__)
c ..............Just test output...........
write(6,1)
+ NICMOS(i__),v_WBD96_(i__),z(i__),E_B_V(i__),SFR(i__),Lum(i__),
+ Frac(i__),SCUBA(i__),Temp(i__),Chi2(i__),Totmag(i__),
+ Apmag(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end