Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/599/1006 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-18
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/599/1006 DEEP Groth Strip Survey. VII. (Kobulnicky+, 2003)
*================================================================================
*The DEEP Groth Strip Survey.
*VII. The metallicity of field galaxies at 0.26<z<0.82 and
*the evolution of the luminosity-metallicity relation.
* Kobulnicky H.A., Willmer C.N.A., Phillips A.C., Koo D.C., Faber S.M.,
* Weiner B.J., Sarajedini V.L., Simard L., Vogt N.P.
* <Astrophys. J., 599, 1006-1030 (2003); Erratum Vol. 610, p. 1234 (2004)>
* =2003ApJ...599.1006K
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! DGSS Selected Galaxies
integer*4 nr__
parameter (nr__=66) ! Number of records
character*142 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)
integer*4 Seq (nr__) ! Reference ID number for this paper
character*8 GID (nr__) ! Groth Strip survey ID
integer*4 RAh (nr__) ! (h) Hour of Right Ascension (J2000)
integer*4 RAm (nr__) ! (min) Minute of Right Ascension (J2000)
real*4 RAs (nr__) ! (s) Second of Right Ascension (J2000)
character*1 DE_ (nr__) ! Sign of Declination (J2000)
integer*4 DEd (nr__) ! (deg) Degree of Declination (J2000)
integer*4 DEm (nr__) ! (arcmin) Arcminute of Declination (J2000)
real*4 DEs (nr__) ! (arcsec) Arcsecond of Declination (J2000)
real*4 z (nr__) ! Redshift from optical emission lines
real*4 Imag (nr__) ! (mag) The I_814_ band AB magnitude
real*4 BMAG (nr__) ! (mag) Absolute rest-frame B band magnitude (1)
real*4 B_V (nr__) ! (mag) Rest-frame (B-V) color index
real*4 R_hl (nr__) ! (kpc) I_814_ image half light radius
real*4 B_T (nr__) ! I_814_ image bulge fraction
real*4 RT (nr__) ! R_T_ asymmetry index (7)
real*4 RA (nr__) ! R_A_ asymmetry index (7)
real*4 EW3727 (nr__) ! (0.1nm) The [O II] (3727{AA}) equivalent width (2)
real*4 e_EW3727 (nr__) ! (0.1nm) Uncertainty in EW3727
real*4 EW4861 (nr__) ! (0.1nm) The H{beta} equivalent width (3)
real*4 e_EW4861 (nr__) ! (0.1nm) Uncertainty in EW4861
real*4 EW4959 (nr__) ! (0.1nm) The [O III] (4959{AA}) equivalent width (2)
real*4 e_EW4959 (nr__) ! (0.1nm) Uncertainty in EW4959
real*4 EW5007 (nr__) ! (0.1nm) The [O III] (5007{AA}) equivalent width (2)
real*4 e_EW5007 (nr__) ! (0.1nm) Uncertainty in EW5007
real*4 v12_logO_H (nr__) ! ([---]) Oxygen abundance, 12+log(O/H) (4)
real*4 e_12_logO_H(nr__) ! ([---]) The 1{sigma} error in O/H (4)
real*4 SFR (nr__) ! (solMass/yr) Estimated star formation rate (5)
character*3 Note (nr__) ! Additional notes (6)
*Note (1): For H_0_=70km/s/Mpc, {Omega}_M_=0.3, {Omega}_{Lambda}_=0.7.
*Note (2): Corrected to the rest frame (divided by (1+z))
*Note (3): Corrected to the rest frame (no correction for stellar absorption).
*Note (4): From the empirical R_23_ method
* following McGaugh, 1991ApJ...380..140M as formulated in Kobulnicky
* et al. (1999ApJ...514..544K) after correction for 2{AA} of stellar
* absorption in the EW4861. An additional uncertainty of 20% has been
* added to the EW_[O II]_ as discussed in the text. An additional
* uncertainty of ~0.15dex in O/H representing uncertainties in the
* photoionization models and empirical strong-line calibration should
* be added in quadrature to the tabulated measurement errors.
*Note (5): Based on H{beta} flux (not corrected for stellar absorption),
* derived from the EW4861 and V-band absolute magnitude. We estimate the
* H{beta} luminosity as L_H{beta}_(erg/s)=5.49E31*2.5^-M_V_^*EW4861. The
* SFR then is computed by SFR(solMass/yr)=2.8*L_H{beta}_/1.12E41 which
* assumes the Kennicutt (1983ApJ...272...54K) calibration of SFR in
* terms of H{alpha} luminosity. This estimate is a lower limit since
* extinction and stellar Balmer absorption are not taken into account.
*Note (6): Additional notes as follows:
* A = Probable star-forming galaxy (non-AGN or minimal AGN
* contribution), as defined in text.
* B = [O II] EW is particularly uncertain due to low continuum levels.
* C = Low-luminosity object with line ratios in the "turn-around"
* region of the strong-line abundance diagram, so the oxygen
* abundance is highly uncertain, in the range 7.8<12+log(O/H)<8.4.
* Object removed from remaining analysis.
* D = Object is a probable AGN on basis of [NeIII]/[OII]>0.4.
*Note (7): Asymmetry indices as defined in paper II:
* The asymmetry parameter R_A_ + R_T_ was found to be a good estimate
* of the total asymmetric flux present in large, bright galaxies.
* R_T_ = (R_T_)raw - (R_T_)bkg
* = [{Sum}i,j(1/2)|Rij+Rij^180^|-{Sum}i,j(1/2)|Bij+Bij^180^|]/[{sum}i,jIij]
* R_A_ = (R_A_)raw - (R_A_)bkg
* = [{Sum}i,j(1/2)|Rij-Rij^180^|-{Sum}i,j(1/2)|Bij-Bij^180^|]/[{sum}i,jIij]
* where the Rij are pixel values in the residual image, and the
* Rij^180^ are pixel values in the residual image rotated by 180{deg}
* Bij are background pixel values in the residual image, and the
* Bij^180^ are background pixel values in the residual image rotated
* by 180{deg}. Iij is the image.
C=============================================================================
C Loading file 'table1.dat' ! DGSS Selected Galaxies
C Format for file interpretation
1 format(
+ I2,1X,A8,1X,I2,1X,I2,1X,F6.3,A1,I2,1X,I2,1X,F5.2,1X,F6.4,1X,
+ F5.2,1X,F5.1,1X,F4.2,1X,F4.2,1X,F4.2,1X,F4.2,1X,F4.2,1X,F5.1,
+ 1X,F4.1,1X,F5.1,1X,F3.1,1X,F5.1,1X,F4.1,1X,F5.1,1X,F4.1,1X,
+ F4.2,1X,F4.2,1X,F4.1,1X,A3)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,66
read(1,'(A142)')ar__
read(ar__,1)
+ Seq(i__),GID(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
+ DEd(i__),DEm(i__),DEs(i__),z(i__),Imag(i__),BMAG(i__),
+ B_V(i__),R_hl(i__),B_T(i__),RT(i__),RA(i__),EW3727(i__),
+ e_EW3727(i__),EW4861(i__),e_EW4861(i__),EW4959(i__),
+ e_EW4959(i__),EW5007(i__),e_EW5007(i__),v12_logO_H(i__),
+ e_12_logO_H(i__),SFR(i__),Note(i__)
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)
+ Seq(i__),GID(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
+ DEd(i__),DEm(i__),DEs(i__),z(i__),Imag(i__),BMAG(i__),
+ B_V(i__),R_hl(i__),B_T(i__),RT(i__),RA(i__),EW3727(i__),
+ e_EW3727(i__),EW4861(i__),e_EW4861(i__),EW4959(i__),
+ e_EW4959(i__),EW5007(i__),e_EW5007(i__),v12_logO_H(i__),
+ e_12_logO_H(i__),SFR(i__),Note(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end