Conversion of standardized ReadMe file for
file /./ftp/cats/J/AJ/132/271 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/AJ/132/271 SFR of M31 from resolved stars in near-IR (Olsen+, 2006)
*================================================================================
*The star formation histories of the bulge and disk of M31 from resolved stars
*in the near-infrared.
* Olsen K.A.G., Blum R.D., Stephens A.W., Davidge T.J., Massey P.,
* Strom S.E., Rigaut F.
* <Astron. J., 132, 271-289 (2006)>
* =2006AJ....132..271O
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Summary of Luminosity Function Fits
integer*4 nr__
parameter (nr__=480) ! Number of records
character*115 ar__ ! Full-size record
character*9 ID (nr__) ! Solution identifier
real*4 AK (nr__) ! The K band dust extinction used in model
integer*4 Age (nr__) ! (Gyr) Model age
real*4 Z1e_4 (nr__) ! (solMass/yr) ? Best fit star formation rate for Z=0.0001
real*4 e_Z1e_4 (nr__) ! (solMass/yr) ? Error in Z1e-4
real*4 Z4e_4 (nr__) ! (solMass/yr) ? Best fit star formation rate for Z=0.0004
real*4 e_Z4e_4 (nr__) ! (solMass/yr) ? Error in Z4e-4
real*4 Z1e_3 (nr__) ! (solMass/yr) ? Best fit star formation rate for Z=0.001
real*4 e_Z1e_3 (nr__) ! (solMass/yr) ? Error in Z1e-3
real*4 Z8e_3 (nr__) ! (solMass/yr) ? Best fit star formation rate for Z=0.008
real*4 e_Z8e_3 (nr__) ! (solMass/yr) ? Error in Z8e-3
real*4 Z1_9e_2 (nr__) ! (solMass/yr) ? Best fit star formation rate for Z=0.019
real*4 e_Z1_9e_2 (nr__) ! (solMass/yr) ? Error in Z1.9e-2
real*4 Z3e_2 (nr__) ! (solMass/yr) ? Best fit star formation rate for Z=0.03
real*4 e_Z3e_2 (nr__) ! (solMass/yr) ? Error in Z3e-2
real*8 chi2 (nr__) ! ? Best fit model {chi}^2^ value (1)
real*4 sigma (nr__) ! ? Extent that chi2 deviates from model
* expectation (2)
real*4 Prob (nr__) ! (%) ? Probability that chi2 arose by chance (3)
*Note (1): Where {chi}^2^=2*Sum_i(m_i-n_i+n_i*ln(n_i/m_i)), see text.
*Note (2): Calculated as ({chi}^2^-<{chi}^2^>)/{sigma}, where the bracketed
* quantities are the expected mean and variance of {chi}^2^ for
* each model.
*Note (3): If the LFs were truly drawn from the given models, then we expect
* Prob~50%; low values of Prob are indicative that the models are not
* good fits.
C=============================================================================
C Loading file 'table3.dat' ! Summary of Luminosity Function Fits
C Format for file interpretation
1 format(
+ A9,1X,F3.1,1X,I2,1X,F6.2,1X,F4.2,2X,F6.2,1X,F4.2,2X,F6.2,1X,
+ F4.2,2X,F5.2,1X,F4.2,2X,F5.2,1X,F5.2,2X,F5.2,1X,F5.2,2X,F7.2,
+ 1X,F6.2,1X,F6.3)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,480
read(1,'(A115)')ar__
read(ar__,1)
+ ID(i__),AK(i__),Age(i__),Z1e_4(i__),e_Z1e_4(i__),Z4e_4(i__),
+ e_Z4e_4(i__),Z1e_3(i__),e_Z1e_3(i__),Z8e_3(i__),e_Z8e_3(i__),
+ Z1_9e_2(i__),e_Z1_9e_2(i__),Z3e_2(i__),e_Z3e_2(i__),chi2(i__),
+ sigma(i__),Prob(i__)
if(ar__(18:23) .EQ. '') Z1e_4(i__) = rNULL__
if(ar__(25:28) .EQ. '') e_Z1e_4(i__) = rNULL__
if(ar__(31:36) .EQ. '') Z4e_4(i__) = rNULL__
if(ar__(38:41) .EQ. '') e_Z4e_4(i__) = rNULL__
if(ar__(44:49) .EQ. '') Z1e_3(i__) = rNULL__
if(ar__(51:54) .EQ. '') e_Z1e_3(i__) = rNULL__
if(ar__(57:61) .EQ. '') Z8e_3(i__) = rNULL__
if(ar__(63:66) .EQ. '') e_Z8e_3(i__) = rNULL__
if(ar__(69:73) .EQ. '') Z1_9e_2(i__) = rNULL__
if(ar__(75:79) .EQ. '') e_Z1_9e_2(i__) = rNULL__
if(ar__(82:86) .EQ. '') Z3e_2(i__) = rNULL__
if(ar__(88:92) .EQ. '') e_Z3e_2(i__) = rNULL__
if(ar__(95:101) .EQ. '') chi2(i__) = rNULL__
if(ar__(103:108) .EQ. '') sigma(i__) = rNULL__
if(ar__(110:115) .EQ. '') Prob(i__) = rNULL__
c ..............Just test output...........
write(6,1)
+ ID(i__),AK(i__),Age(i__),Z1e_4(i__),e_Z1e_4(i__),Z4e_4(i__),
+ e_Z4e_4(i__),Z1e_3(i__),e_Z1e_3(i__),Z8e_3(i__),e_Z8e_3(i__),
+ Z1_9e_2(i__),e_Z1_9e_2(i__),Z3e_2(i__),e_Z3e_2(i__),chi2(i__),
+ sigma(i__),Prob(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end