Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/733/87 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 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/733/87 Star formation efficiency in galaxies (Shi+, 2011)
*================================================================================
*Extended Schmidt law: role of existing stars in current star formation.
* Shi Y., Helou G., Yan L., Armus L., Wu Y., Papovich C., Stierwalt S.
* <Astrophys. J., 733, 87 (2011)>
* =2011ApJ...733...87S
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Samples with CO and HI data
integer*4 nr__
parameter (nr__=143) ! Number of records
character*135 ar__ ! Full-size record
character*15 Name ! Galaxy name
character*10 Type ! Galaxy type in this paper (1)
real*8 z ! [-0.0011/3.41] Redshift
real*8 Dist ! (Mpc) [0.78/29645] Distance used in this work
character*27 Ap ! Aperture definition (2)
real*8 Area ! (kpc2) De-projected area used to derive
* surface densities
real*4 logSigSFR ! ([Msun/yr/kpc2]) Log star formation rate surface density
real*4 logSigG ! ([Msun/pc2]) Log of gas surface density
character*4 Ref ! Reference(s) for SFR and gas
* surface density data (3)
real*4 logSig_ ! ([Msun/pc2]) Log of stellar mass surface density
character*27 Band ! Wavelength band used to measure
* stellar mass
character*2 Ref_ ! [2/18] Reference for stellar mass (3)
*Note (1): Type as follows:
* LSB = The subsample of low-surface-brightness (LSB) galaxies includes
* all the 19 objects from Wyder et al. (2009ApJ...696.1834W) and
* five gas-rich dwarf galaxies from Leroy et al. (2008,
* Cat. J/AJ/136/2782).
* early-type = We here included nine objects from Wei et al.
* (2010ApJ...725L..62W) and 10 objects from Crocker et al.
* (2011MNRAS.410.1197C).
* high-z-SFG = High-redshift star-forming galaxies (21 optically/near-IR
* selected star-forming galaxies (Extended Groth Strip (EGS), BzK,
* and BXMD)
* high-z-SMG = merging submillimeter galaxies (seven submillimeter objects from
* Genzel et al. (2010MNRAS.407.2091G))
* late-type = This sub-sample includes 61 and 18 objects from Kennicutt
* (1998ApJ...498..541K) and Leroy et al. (2008,
* Cat. J/AJ/136/2782), respectively.
* z=0-LIRGS = Local LIRGs
* See section 2.1 for further details.
*Note (2): Used to calculate the surface density of SFR, gas and stellar
* mass. R_25_ means the isophotal radius at 25mag/arcsec^2^ (usually in
* B band). R_max_ gives the maximum extent of the galaxy at a given
* wavelength that is indicated in square brackets. Its value relative
* to R_25_ is listed in parentheses whenever possible. R_1/2_ is the
* half light radius at a given wavelength that is indicated in square
* brackets.
*Note (3): For those with two RefSg references, the first one is for H_2_ and
* SFR data while the second is for HI data. Reference(s) as follows:
* 1 = Kennicutt (1998ApJ...498..541K);
* 2 = Leroy et al. (2008, Cat. J/AJ/136/2782);
* 3 = Wei et al. (2010ApJ...725L..62W);
* 4 = Crocker et al. (2011MNRAS.410.1197C);
* 5 = Wyder et al. (2009ApJ...696.1834W);
* 6 = Scoville et al. (1997ApJ...484..702S);
* 7 = Gracia-Carpio et al. (2007A&A...468L..67G);
* 8 = Yun & Scoville (1995ApJ...451L..45Y);
* 9 = Bryant & Scoville (1999AJ....117.2632B);
* 10 = Yun et al. (1994ApJ...430L.109Y);
* 11 = Genzel et al. (2010MNRAS.407.2091G);
* 12 = Oosterloo et al. (2010MNRAS.409..500O);
* 13 = Irwin et al. (1987ApJ...313L..91I);
* 14 = van Driel & van Woerden (1991A&A...243...71V);
* 15 = Sage & Welch (2006ApJ...644..850S);
* 16 = Knapp & Raimond (1984A&A...138...77K);
* 17 = Cox et al. (2001AJ....121..692C);
* 18 = this-work.
C=============================================================================
C Loading file 'table1.dat' ! Samples with CO and HI data
C Format for file interpretation
1 format(
+ A15,1X,A10,1X,F9.6,1X,F8.2,1X,A27,1X,F8.2,1X,F5.2,1X,F4.2,1X,
+ A4,1X,F5.2,1X,A27,1X,A2)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,143
read(1,'(A135)')ar__
read(ar__,1)
+ Name,Type,z,Dist,Ap,Area,logSigSFR,logSigG,Ref,logSig_,Band,
+ Ref_
c ..............Just test output...........
write(6,1)
+ Name,Type,z,Dist,Ap,Area,logSigSFR,logSigG,Ref,logSig_,Band,
+ Ref_
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end