Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/920/122 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 2026-Oct-11
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/920/122 Candidate Ly{alpha}-emitting galaxies spectra (Davis+, 2021)
*================================================================================
*Detection of Lyman Continuum from 3.0<z<3.5 galaxies in the HETDEX survey.
* Davis D., Gebhardt K., Mentuch Cooper E., Chisholm J., Ciardullo R.,
* Farrow D.J., Finkelstein S.L., Gronwall C., Gawiser E., Hill G.J.,
* Hopp U., Jeong D., Landriau M., Liu C., Lujan Niemeyer M., Schneider D.P.,
* Snigula J., Tuttle S.
* <Astrophys. J., 920, 122 (2021)>
* =2021ApJ...920..122D
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Candidate LAE galaxies for this work
integer*4 nr__
parameter (nr__=214) ! Number of records
character*73 ar__ ! Full-size record
C Position composed of: RAdeg DEdeg
integer*8 ID ! Detection ID
character*26 Name ! HETDEX Detection Name, JHHMMSS.ss+DDMMSS.s
real*8 RAdeg ! (deg) [165/230] Right Ascension (ICRS)
real*8 DEdeg ! (deg) [48/57] Declination, decimal degrees (ICRS)
real*4 zspec ! [2.99/3.5] Spectroscopic redshift
real*4 rmag ! (mag) [23.5/26.5] r-band magnitude
real*4 e_rmag ! (mag) [0.04/2]?=0.000 Uncertainty in rmag (1)
*Note (1): Entries with no result are fainter than the imaging
* magnitude limit of 26.5.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Sub-sample Stacked Spectra
integer*4 nr__1
parameter (nr__1=123) ! Number of records
character*97 ar__1 ! Full-size record
real*8 lambda1 ! (0.1nm) [780/1378] Full sample, wavelength
real*8 flux1 ! (10-17mW/m2) [-8.6/60]? Full sample, flux (1)
real*4 e_flux1 ! (10-17mW/m2) [0.4/8]? Full sample, flux uncertainty (1)
real*8 lambda2 ! (0.1nm) [782/1379]? Brightest 1/3, wavelength
real*8 flux2 ! (10-17mW/m2) [-12/68]? Brightest 1/3, flux (1)
real*8 e_flux2 ! (10-17mW/m2) [0.7/13]? Brightest 1/3, flux uncertainty
* (1)
real*8 lambda3 ! (0.1nm) [780/1378] Faintest 2/3, wavelength
real*8 flux3 ! (10-17mW/m2) [-39/56]? Faintest 2/3, flux (1)
real*8 e_flux3 ! (10-17mW/m2) [0.4/13]? Faintest 2/3, flux uncertainty
* (1)
real*8 lambda4 ! (0.1nm) [779/1378]? Faintest 1/3, wavelength
real*8 flux4 ! (10-17mW/m2) [-18/54]? Faintest 1/3, flux (1)
real*8 e_flux4 ! (10-17mW/m2) [0.6/21]? Faintest 1/3 flux uncertainty (1)
*Note (1): Null entries for the flux# and e_flux# are present only for alignment
* across the four samples.
C=============================================================================
C Loading file 'table1.dat' ! Candidate LAE galaxies for this work
C Format for file interpretation
1 format(I10,1X,A26,1X,F8.4,1X,F7.4,1X,F6.4,1X,F5.2,1X,F5.3)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,214
read(1,'(A73)')ar__
read(ar__,1)ID,Name,RAdeg,DEdeg,zspec,rmag,e_rmag
c ..............Just test output...........
write(6,1)ID,Name,RAdeg,DEdeg,zspec,rmag,e_rmag
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! Sub-sample Stacked Spectra
C Format for file interpretation
2 format(
+ F7.2,1X,F7.4,1X,F6.4,1X,F7.2,1X,F8.4,1X,F7.4,1X,F7.2,1X,F8.4,
+ 1X,F7.4,1X,F7.2,1X,F8.4,1X,F7.4)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,123
read(1,'(A97)')ar__1
read(ar__1,2)
+ lambda1,flux1,e_flux1,lambda2,flux2,e_flux2,lambda3,flux3,
+ e_flux3,lambda4,flux4,e_flux4
if(ar__1(9:15) .EQ. '') flux1 = rNULL__
if(ar__1(17:22) .EQ. '') e_flux1 = rNULL__
if(ar__1(24:30) .EQ. '') lambda2 = rNULL__
if(ar__1(32:39) .EQ. '') flux2 = rNULL__
if(ar__1(41:47) .EQ. '') e_flux2 = rNULL__
if(ar__1(57:64) .EQ. '') flux3 = rNULL__
if(ar__1(66:72) .EQ. '') e_flux3 = rNULL__
if(ar__1(74:80) .EQ. '') lambda4 = rNULL__
if(ar__1(82:89) .EQ. '') flux4 = rNULL__
if(ar__1(91:97) .EQ. '') e_flux4 = rNULL__
c ..............Just test output...........
write(6,2)
+ lambda1,flux1,e_flux1,lambda2,flux2,e_flux2,lambda3,flux3,
+ e_flux3,lambda4,flux4,e_flux4
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end