Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/706/A261 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-May-17
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/706/A261 EELG phys. prop. and ion. efficiency (Gimenez-Alcazar+, 2026)
*================================================================================
*J-PAS: First identification, physical properties and ionization efficiency of
*extreme emission line galaxies.
* Gimenez-Alcazar A., Amorin R., Vilchez J.M., Hernan-Caballero A.,
* Gonzalez-Otero M., Arroyo-Polonio A., Iglesias-Paramo J.,
* Lumbreras-Calle A., Fernandez-Ontiveros J.A., Bonatto L.,
* Gonzalez Delgado R.M., Kehrig C., Torralba A., Rahna P.T., Jimenez-Teja Y.,
* Marquez I., Breda I., Alvarez-Candal A., Abramo R., Alcaniz J., Benitez N.,
* Bonoli S., Carneiro S., Cenarro J., Cristobal-Hornillos D., Dupke R.,
* Ederoclite A., Hernandez-Monteagudo C., Marin-Franch A.,
* Mendes de Oliveira C., Moles M., Sodre L.Jr, Taylor K., Varela J.,
* Vazquez Ramio.H.
* <Astron. Astrophys. 706, A261 (2026)>
* =2026A&A...706A.261G (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Derived SED Parameters
integer*4 nr__
parameter (nr__=917) ! Number of records
character*198 ar__ ! Full-size record
C J2000 position composed of: RAdeg DEdeg
integer*4 TileID ! J-PAS tile identifier
integer*4 Number ! Source number within the tile
real*8 RAdeg ! (deg) Right Ascension (J2000)
real*8 DEdeg ! (deg) Declination (J2000)
real*8 z ! Spectroscopic or photometric redshift
real*8 Reff ! (arcsec) Effective radius enclosing specified
* fraction of flux
real*8 logMstar ! ([Msun]) Stellar mass from SED fitting (1)
real*8 e_logMstar ! ([Msun]) 1-sigma uncertainty from Bayesian
* analysis on logMstar (1)
real*8 logSFR10 ! ([Msun/yr]) Star formation rate averaged over
* last 10Myr (1)
real*8 e_logSFR10 ! ([Msun/yr]) 1-sigma uncertainty from Bayesian
* analysis on logSFR10 (1)
real*8 E_B_V ! (mag) Dust attenuation
real*4 e_E_B_V ! (mag) 1-sigma uncertainty from Bayesian
* analysis on E(B-V)
*Note (1): Stellar mass and SFR are derived using CIGALE with parametric SFHs,
* Charlot & Bruzal (2019, see 2003MNRAS.344.1000B) stellar populations,
* Chabrier (2003PASP..115..763C) IMF, and Dale et al. (2014ApJ...784...83D)
* dust models.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Emission line quantities
integer*4 nr__1
parameter (nr__1=917) ! Number of records
character*323 ar__1 ! Full-size record
integer*4 TileID_1 ! J-PAS tile identifier
integer*4 Number_1 ! Source number within the tile
real*8 z_1 ! Spectroscopic or photometric redshift
real*8 xiHalpha ! (10+7Hz/J) ? Ionizing photon production
* efficiency from H-alpha (in Hz/erg
* unit) (1)
real*8 e_xiHalpha ! (10+7Hz/J) ? 1-sigma uncertainty on xi_Halpha
real*8 xiHbeta ! (10+7Hz/J) ? Ionizing photon production
* efficiency from H-beta (in Hz/erg
* unit) (1)
real*8 e_xiHbeta ! (10+7Hz/J) ? 1-sigma uncertainty on xi_Hbeta
real*8 FHalpha ! (10-20W/m2/nm) ? H-alpha line flux
* (in 10^-19^erg/s/cm^2/{AA} unit)
real*8 e_FHalpha ! (10-20W/m2/nm) ? 1-sigma uncertainty on FHalpha
* (in 10^-19^erg/s/cm^2/{AA} unit)
real*8 FHbeta ! (10-20W/m2/nm) ? H-beta line flux
* (in 10^-19^erg/s/cm^2/{AA} unit)
real*8 e_FHbeta ! (10-20W/m2/nm) ? 1-sigma uncertainty on FHbetaa
* (in 10^-19^erg/s/cm^2/{AA} unit)
real*8 EWHalpha ! (0.1nm) ? H-alpha equivalent width
* (in {AA} unit)
real*8 e_EWHalpha ! (0.1nm) ? 1-sigma uncertainty on EWHalpha
* (in {AA} unit)
real*8 EWHbeta ! (0.1nm) ? H-beta equivalent width
* (in {AA} unit)
real*8 e_EWHbeta ! (0.1nm) ? 1-sigma uncertainty on EWHbeta
* (in {AA} unit)
real*8 EWOIII5007 ! (0.1nm) ? Line [O III] 5007 A equivalent width
* (in {AA} unit)
real*8 e_EWOIII5007 ! (0.1nm) ? 1-sigma uncertainty on EWOIII5007
* (in {AA} unit)
*Note (1): xi values assume f_esc_ = 0, i.e., all Lyman continuum photons are
* reprocessed into Balmer lines.
C=============================================================================
C Loading file 'table1.dat' ! Derived SED Parameters
C Format for file interpretation
1 format(
+ I4,1X,I5,1X,F18.14,1X,F18.15,1X,F11.9,1X,F10.8,2X,F19.16,1X,
+ F20.18,1X,F21.18,1X,F19.17,1X,F19.17,1X,E22.19)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,917
read(1,'(A198)')ar__
read(ar__,1)
+ TileID,Number,RAdeg,DEdeg,z,Reff,logMstar,e_logMstar,logSFR10,
+ e_logSFR10,E_B_V,e_E_B_V
c ..............Just test output...........
write(6,1)
+ TileID,Number,RAdeg,DEdeg,z,Reff,logMstar,e_logMstar,logSFR10,
+ e_logSFR10,E_B_V,e_E_B_V
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! Emission line quantities
C Format for file interpretation
2 format(
+ I4,1X,I5,1X,F11.9,1X,F18.15,1X,F20.18,1X,F18.15,1X,F20.18,1X,
+ F21.16,1X,F19.16,1X,F24.18,1X,F20.16,1X,F21.16,1X,F20.16,1X,
+ F23.17,1X,F21.16,1X,F23.16,1X,F19.15)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,917
read(1,'(A323)')ar__1
read(ar__1,2)
+ TileID_1,Number_1,z_1,xiHalpha,e_xiHalpha,xiHbeta,e_xiHbeta,
+ FHalpha,e_FHalpha,FHbeta,e_FHbeta,EWHalpha,e_EWHalpha,EWHbeta,
+ e_EWHbeta,EWOIII5007,e_EWOIII5007
if(ar__1(24:41) .EQ. '') xiHalpha = rNULL__
if(ar__1(43:62) .EQ. '') e_xiHalpha = rNULL__
if(ar__1(64:81) .EQ. '') xiHbeta = rNULL__
if(ar__1(83:102) .EQ. '') e_xiHbeta = rNULL__
if(ar__1(104:124) .EQ. '') FHalpha = rNULL__
if(ar__1(126:144) .EQ. '') e_FHalpha = rNULL__
if(ar__1(146:169) .EQ. '') FHbeta = rNULL__
if(ar__1(171:190) .EQ. '') e_FHbeta = rNULL__
if(ar__1(192:212) .EQ. '') EWHalpha = rNULL__
if(ar__1(214:233) .EQ. '') e_EWHalpha = rNULL__
if(ar__1(235:257) .EQ. '') EWHbeta = rNULL__
if(ar__1(259:279) .EQ. '') e_EWHbeta = rNULL__
if(ar__1(281:303) .EQ. '') EWOIII5007 = rNULL__
if(ar__1(305:323) .EQ. '') e_EWOIII5007 = rNULL__
c ..............Just test output...........
write(6,2)
+ TileID_1,Number_1,z_1,xiHalpha,e_xiHalpha,xiHbeta,e_xiHbeta,
+ FHalpha,e_FHalpha,FHbeta,e_FHbeta,EWHalpha,e_EWHalpha,EWHbeta,
+ e_EWHbeta,EWOIII5007,e_EWOIII5007
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end