Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/653/1004 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/653/1004 Galaxies at 1.4<~z<~3.0 in GOODS-North Field (Reddy+, 2006)
*================================================================================
*A spectroscopic survey of redshift 1.4<~z<~3.0 galaxies in the
*GOODS-North Field: survey description, catalogs, and properties.
* Reddy N.A., Steidel C.C., Erb D.K., Shapley A.E., Pettini M.
* <Astrophys. J., 653, 1004-1026 (2006)>
* =2006ApJ...653.1004R
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! GOODS-N UnGR galaxies with spectroscopic redshifts
integer*4 nr__
parameter (nr__=388) ! Number of records
character*160 ar__ ! Full-size record
C J2000.0 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg ! (deg) Right Ascension J2000.0
real*8 DEdeg ! (deg) Declination J2000.0
C ---------------------------------- ! (position vector(s) in degrees)
character*10 Name ! Name (G1)
integer*4 RAh ! (h) Right ascension (J2000.0)
integer*4 RAm ! (min) Right ascension (J2000.0)
real*4 RAs ! (s) Right ascension (J2000.0)
character*1 DE_ ! Declination sign (J2000.0)
integer*4 DEd ! (deg) Declination (J2000.0)
integer*4 DEm ! (arcmin) Declination (J2000.0)
real*4 DEs ! (arcsec) Declination (J2000.0)
character*1 u_zem ! [:] Uncertainty flag on zem
real*4 zem ! ? Emission redshift (2)
character*1 u_zabs ! [:] Uncertainty flag on zabs
real*4 zabs ! ? Absorption redshift (3)
character*4 Mcl ! Morphological class (4)
real*4 Rmag ! (mag) ? R magnitude in AB unit (G2)
real*4 G_R ! (mag) ? G-R colour index (G2)
character*1 l_Un_G ! Limit flag, upper limits given for galaxies
* undetected in Un
real*4 Un_G ! (mag) ? Un-G colour index (G2)
character*1 l_Jmag ! Limit flag on Jmag
real*4 Jmag ! (mag) ? J magnitude (5)
character*1 l_Ksmag ! Limit flag on Ksmag
real*4 Ksmag ! (mag) ? Ks magnitude (5)
real*4 m3_6 ! (mag) ? magnitude at 3.6um
real*4 e_m3_6 ! (mag) ? rms uncertainty on m3.6
real*4 m4_5 ! (mag) ? magnitude at 4.5um
real*4 e_m4_5 ! (mag) ? rms uncertainty on m4.5
real*4 m5_8 ! (mag) ? magnitude at 5.8um
real*4 e_m5_8 ! (mag) ? rms uncertainty on m5.8
real*4 m8_0 ! (mag) ? magnitude at 8.0um
real*4 e_m8_0 ! (mag) ? rms uncertainty on m8.0
real*4 F24 ! (uJy) ? flux at 24um
real*4 e_F24 ! (uJy) ? rms uncertainty on F24
character*19 Notes ! Notes (6)
*Note (2): Emission-line redshift. An entry with a colon indicates that the
* redshift is uncertain. A blank entry indicates that an emission-line
* redshift could not be measured.
*Note (3): Absorption-line redshift. An entry with a colon indicates that
* the redshift is uncertain. A blank entry indicates that an
* absorption-line redshift could not be measured.
*Note (4): Source type, either galaxy (GAL), AGN, QSO, or STAR. The
* distinction between QSO and AGN classification is based on the line
* widths, as described in Steidel et al. (2002ApJ...576..653S), where an
* object is classified as a QSO if it has any emission line with FWHM
* >2000km/s. AGNs identified using other means (X-ray or mid-IR
* emission) are discussed in Sect. 6.2.
*Note (5): A blank entry indicates that the object did not lie in the region
* with near-IR imaging.
*Note (6): Galaxies in common with the LBG survey in the HDF-N are indicated
* by their names (S03-XXX) as given in Steidel et al. (2003, Cat.
* J/ApJ/592/728). Galaxies with X-ray counterparts within are indicated
* by their names (B03-XXX) in the spectroscopic follow-up to the Chandra
* 2 Ms survey by Barger et al. (2003, Cat. <J/AJ/126/632>). Galaxies
* satisfying the distant red galaxy (DRG) criteria of Franx et al.
* (2003ApJ...587L..79F) are indicated by DRG.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Stellar Population Parameters
integer*4 nr__1
parameter (nr__1=254) ! Number of records
character*71 ar__1 ! Full-size record
character*10 Name_1 ! Name (G1) (1)
real*4 z ! Redshift
real*4 E_B_V_i ! (mag) Reddening E(B-V) calculated with
* constant formation
integer*4 Age_i ! (Myr) Age calculated with constant formation
integer*4 SFR_i ! (solMass/yr) Stellar Formation Rate calculated with
* constant formation
real*4 Mass_i ! (10+10solMass) Stellar mass calculated with constant
* formation
integer*4 tau ! (Myr) Best-fit star formation history
* decay timescale (2)
real*4 E_B_V_tau ! (mag) Reddening E(B-V) calculated with tau
integer*4 Age_tau ! (Myr) Age calculated with tau
integer*4 SFR_tau ! (solMass/yr) Stellar Formation Rate calculated
* with tau
real*4 Mass_tau ! (10+10solMass) Stellar mass calculated with tau
character*4 Note ! [IRAC Ks] Notes (3)
*Note (1): We did not fit the stellar populations of galaxies that had no
* data longward of R band, had uncertain redshifts, or are identified as
* AGN/QSO from their optical spectra. We also do not present SED
* parameters for those galaxies with optical and IRAC photometry
* inconsistent with a simple stellar population (these sources had
* large {chi}^2^>10) or those sources with 8 or 24um excesses.
*Note (2): In some cases, a model with constant star formation (infinity)
* provided the best fit.
*Note (3): Objects with large Ks band residuals are indicated (i.e., those
* sources whose Ks band measurement lies more than 3{sigma} away from
* the best-fit stellar population). MD31 is the only directly detected
* X-ray source that shows no optical signatures of an AGN, has a
* relatively faint 24um flux, and has photometry that is consistent with
* a stellar population. The IRAC photometry for BX1267 may suffer from a
* deblending problem, and these (IRAC) data were not used in the SED fit.
C=============================================================================
C Loading file 'table2.dat' ! GOODS-N UnGR galaxies with spectroscopic redshifts
C Format for file interpretation
1 format(
+ A10,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,A1,F5.3,1X,
+ A1,F5.3,1X,A4,1X,F5.2,1X,F5.2,A1,F5.2,1X,A1,F5.2,1X,A1,F5.2,
+ 1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,
+ F4.2,1X,F5.1,1X,F4.1,1X,A19)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,388
read(1,'(A160)')ar__
read(ar__,1)
+ Name,RAh,RAm,RAs,DE_,DEd,DEm,DEs,u_zem,zem,u_zabs,zabs,Mcl,
+ Rmag,G_R,l_Un_G,Un_G,l_Jmag,Jmag,l_Ksmag,Ksmag,m3_6,e_m3_6,
+ m4_5,e_m4_5,m5_8,e_m5_8,m8_0,e_m8_0,F24,e_F24,Notes
if(ar__(37:41) .EQ. '') zem = rNULL__
if(ar__(44:48) .EQ. '') zabs = rNULL__
if(ar__(55:59) .EQ. '') Rmag = rNULL__
if(ar__(61:65) .EQ. '') G_R = rNULL__
if(ar__(67:71) .EQ. '') Un_G = rNULL__
if(ar__(74:78) .EQ. '') Jmag = rNULL__
if(ar__(81:85) .EQ. '') Ksmag = rNULL__
if(ar__(87:91) .EQ. '') m3_6 = rNULL__
if(ar__(93:96) .EQ. '') e_m3_6 = rNULL__
if(ar__(98:102) .EQ. '') m4_5 = rNULL__
if(ar__(104:107) .EQ. '') e_m4_5 = rNULL__
if(ar__(109:113) .EQ. '') m5_8 = rNULL__
if(ar__(115:118) .EQ. '') e_m5_8 = rNULL__
if(ar__(120:124) .EQ. '') m8_0 = rNULL__
if(ar__(126:129) .EQ. '') e_m8_0 = rNULL__
if(ar__(131:135) .EQ. '') F24 = rNULL__
if(ar__(137:140) .EQ. '') e_F24 = rNULL__
RAdeg = rNULL__
DEdeg = rNULL__
c Derive coordinates RAdeg and DEdeg from input data
c (RAdeg and DEdeg are set to rNULL__ when unknown)
if(RAh .GT. -180) RAdeg=RAh*15.
if(RAm .GT. -180) RAdeg=RAdeg+RAm/4.
if(RAs .GT. -180) RAdeg=RAdeg+RAs/240.
if(DEd .GE. 0) DEdeg=DEd
if(DEm .GE. 0) DEdeg=DEdeg+DEm/60.
if(DEs .GE. 0) DEdeg=DEdeg+DEs/3600.
if(DE_.EQ.'-'.AND.DEdeg.GE.0) DEdeg=-DEdeg
c ..............Just test output...........
write(6,1)
+ Name,RAh,RAm,RAs,DE_,DEd,DEm,DEs,u_zem,zem,u_zabs,zabs,Mcl,
+ Rmag,G_R,l_Un_G,Un_G,l_Jmag,Jmag,l_Ksmag,Ksmag,m3_6,e_m3_6,
+ m4_5,e_m4_5,m5_8,e_m5_8,m8_0,e_m8_0,F24,e_F24,Notes
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3.dat' ! Stellar Population Parameters
C Format for file interpretation
2 format(
+ A10,1X,F5.3,1X,F4.2,1X,I4,1X,I4,1X,F6.3,1X,I4,1X,F5.2,1X,I4,
+ 1X,I4,1X,F6.3,1X,A4)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,254
read(1,'(A71)')ar__1
read(ar__1,2)
+ Name_1,z,E_B_V_i,Age_i,SFR_i,Mass_i,tau,E_B_V_tau,Age_tau,
+ SFR_tau,Mass_tau,Note
c ..............Just test output...........
write(6,2)
+ Name_1,z,E_B_V_i,Age_i,SFR_i,Mass_i,tau,E_B_V_tau,Age_tau,
+ SFR_tau,Mass_tau,Note
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end