Conversion of standardized ReadMe file for
file /./ftp/cats/J/AJ/127/2455 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/AJ/127/2455 Gemini Deep Deep Survey (GDDS) (Abraham+, 2004)
*================================================================================
*The Gemini Deep Deep Survey.
*I. Introduction to the survey, catalogs, and composite spectra.
* Abraham R.G., Glazebrook K., Mccarthy P.J., Crampton D., Murowinski R.,
* Jorgensen I., Roth K., Hook I.M., Savaglio S., Chen H.-W., Marzke R.O.,
* Carlberg R.G.
* <Astron. J., 127, 2455-2483 (2004)>
* =2004AJ....127.2455A
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4.dat' ! Master data table
integer*4 nr__
parameter (nr__=309) ! Number of records
character*140 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)
character*7 GDDS (nr__) ! GDDS object identification (HH-NNNN)
real*4 z (nr__) ! ? Redshift
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 the 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)
integer*4 Conf (nr__) ! Redshift confidence (G1)
character*3 Ovlap (nr__) ! Slit geometry/collision class (1)
real*8 Weight (nr__) ! Sampling weight (2)
real*4 Bmag (nr__) ! (mag) ? B-band magnitude (3)
character*1 n_Bmag (nr__) ! [s] s for 2{sigma} detection limit in Bmag
real*4 e_Bmag (nr__) ! (mag) ? Uncertainty in Bmag (3)
real*4 Vmag (nr__) ! (mag) V-band magnitude (3)
character*1 n_Vmag (nr__) ! [s] s for 2{sigma} detection limit in Vmag
real*4 e_Vmag (nr__) ! (mag) ? Uncertainty in Vmag (3)
real*4 Rmag (nr__) ! (mag) ? Cousins R-band magnitude (3)
character*1 n_Rmag (nr__) ! [s] s for 2{sigma} detection limit in Rmag
real*4 e_Rmag (nr__) ! (mag) ? Uncertainty in Rmag (3)
real*4 Icmag (nr__) ! (mag) Cousins I-band magnitude (3)
character*1 n_Icmag (nr__) ! [s] s for 2{sigma} detection limit in Icmag
real*4 e_Icmag (nr__) ! (mag) Uncertainty in Icmag (3)
real*4 z_mag (nr__) ! (mag) z'-band magnitude (3)
character*1 n_z_mag (nr__) ! [s] s for 2{sigma} detection limit in z'mag
real*4 e_z_mag (nr__) ! (mag) ? Uncertainty in z'mag (3)
real*4 Hmag (nr__) ! (mag) ? H-band magnitude (3)
character*1 n_Hmag (nr__) ! [s] s for 2{sigma} detection limit in Hmag
real*4 e_Hmag (nr__) ! (mag) ? Uncertainty in Hmag (3)
real*4 Ksmag (nr__) ! (mag) Ks-band magnitude (3)
character*1 n_Ksmag (nr__) ! [s] s for 2{sigma} detection limit in Ksmag
real*4 e_Ksmag (nr__) ! (mag) ? Uncertainty in Ksmag (3)
*Note (1): Classification of spectrum overlaps take the following numbers:
* 0 = Both A and B channels uncontaminated (at most very minor masking
* needed).
* 1 = Single channel overlap. Offending channel not used (at most very
* minor masking needed).
* 2 = A contaminating zeroth-order line has been masked. Remaining
* continuum is trustworthy.
* 3 = Two channel collision. Major masking used in extraction.
* Continuum in blue should not be trusted.
* 4 = Two channel collision. Major masking used in extraction.
* Continuum in red should not be trusted.
* 5 = Extreme measures needed to try to recover a spectrum.
* Continuum should not be trusted.
*Note (2): The practical upshot of our general mask design strategy is
* graphically summarized in the bottom left panel of Figure 6. This
* panel is a two-dimensional histogram showing the number of independent
* slits assigned each cell of color-magnitude space. For the reasons
* just described heavy emphasis is given to the (22<I<24.5, 3<I-Ks<5)
* region of color-magnitude space. The relative number of slits as a
* function of the average population in each cell expected in a
* wide-area survey can be computed by dividing the bottom left panel of
* the figure by the top left panel. The values computed using this
* procedure are shown in the bottom right panel and correspond to
* sampling weights. These weights will prove important in the
* computation of the luminosity and mass functions in future papers in
* this series.
*Note (3): Non-detections have been placed at the formal 2{sigma} detection
* limit of the filter and magnitude error set to blank.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table5.dat' ! Spectral Features and Classifications
integer*4 nr__1
parameter (nr__1=273) ! Number of records
character*49 ar__1 ! Full-size record
character*7 GDDS_1 (nr__1) ! GDDS object identification (HH-NNNN)
integer*4 AGN (nr__1) ! [0/1] Indicative of AGN activity (1)
integer*4 v_OII_ (nr__1) ! [0/2] Is [O II] (3727 {AA}) present? (1)
integer*4 v_OIII_ (nr__1) ! [0/2] Is [O III] (5007 {AA}) present? (1)
integer*4 HiBal (nr__1) ! [0/2] Are Balmer lines bluer than H{beta}
* present? (1)
integer*4 LoBal (nr__1) ! [0/2] Is H{alpha} and/or H{beta} present? (1)
integer*4 Fe2375 (nr__1) ! [0/2] Is Fe II (2375 {AA}) present? (1)
integer*4 Fe2600 (nr__1) ! [0/2] Is Fe II (2600 {AA}) present? (1)
integer*4 Mg2800 (nr__1) ! [0/2] Is Mg II (2800 {AA}) present? (1)
integer*4 Mg2852 (nr__1) ! [0/2] Is Mg II (2852 {AA}) present? (1)
integer*4 HandK (nr__1) ! [0/2] Are Ca II H & K lines present? (1)
integer*4 Balmer (nr__1) ! [0/2] Is the Balmer decrement present? (1)
integer*4 D4000 (nr__1) ! [0/2] Is the D4000 feature present? (1)
integer*4 Temp (nr__1) ! Redshift template code (2)
integer*4 Class (nr__1) ! Spectral class (3)
integer*4 Conf_1 (nr__1) ! Confidence code (G1)
real*4 z_1 (nr__1) ! Redshift
*Note (1): Flag is: 0=No, 1=Yes
* 2=Feature did not fall within the wavelength range of our spectra
*Note (2): Redshift template code as follows:
* 1 = Comparison against a reference template was used to obtain the
* redshift
* 2 = No template needed to obtain the redshift
*Note (3): Classes use the following numbers:
* 001 = Objects showing pure, or nearly pure, signatures of an evolved
* stellar population (e.g., D4000, H&K, or template matches)
* 100 = Objects that are dominated by the flat-UV continuum and strong
* emission-lines characteristic of star- forming systems
* 010 = those showing signatures of intermediate ages (e.g., strong
* Balmer absorption).
* Many objects show characteristics of more than one type and so are
* assigned classes that are the sum of old (001), intermediates (010),
* and young (100) populations. Example:
* Objects listed as "101" may show strong H&K absorption and 4000{AA}
* breaks and yet have a flat-UV continuum tail indicative of a low level
* of ongoing star formation.
C=============================================================================
C Loading file 'table4.dat' ! Master data table
C Format for file interpretation
1 format(
+ 2X,A7,1X,F6.4,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F5.2,1X,
+ I2,1X,A3,1X,F7.5,1X,F5.2,A1,F5.2,1X,F5.2,A1,F5.2,1X,F5.2,A1,
+ F5.2,1X,F5.2,A1,F4.2,1X,F5.2,A1,F5.2,1X,F5.2,A1,F5.2,1X,F5.2,
+ A1,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table4.dat')
write(6,*) '....Loading file: table4.dat'
do i__=1,309
read(1,'(A140)')ar__
read(ar__,1)
+ GDDS(i__),z(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),Conf(i__),Ovlap(i__),Weight(i__),Bmag(i__),
+ n_Bmag(i__),e_Bmag(i__),Vmag(i__),n_Vmag(i__),e_Vmag(i__),
+ Rmag(i__),n_Rmag(i__),e_Rmag(i__),Icmag(i__),n_Icmag(i__),
+ e_Icmag(i__),z_mag(i__),n_z_mag(i__),e_z_mag(i__),Hmag(i__),
+ n_Hmag(i__),e_Hmag(i__),Ksmag(i__),n_Ksmag(i__),e_Ksmag(i__)
if(ar__(11:16) .EQ. '') z(i__) = rNULL__
if(ar__(58:62) .EQ. '') Bmag(i__) = rNULL__
if(ar__(64:68) .EQ. '') e_Bmag(i__) = rNULL__
if(ar__(76:80) .EQ. '') e_Vmag(i__) = rNULL__
if(ar__(82:86) .EQ. '') Rmag(i__) = rNULL__
if(ar__(88:92) .EQ. '') e_Rmag(i__) = rNULL__
if(ar__(111:115) .EQ. '') e_z_mag(i__) = rNULL__
if(ar__(117:121) .EQ. '') Hmag(i__) = rNULL__
if(ar__(123:127) .EQ. '') e_Hmag(i__) = rNULL__
if(ar__(135:139) .EQ. '') e_Ksmag(i__) = rNULL__
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)
+ GDDS(i__),z(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),Conf(i__),Ovlap(i__),Weight(i__),Bmag(i__),
+ n_Bmag(i__),e_Bmag(i__),Vmag(i__),n_Vmag(i__),e_Vmag(i__),
+ Rmag(i__),n_Rmag(i__),e_Rmag(i__),Icmag(i__),n_Icmag(i__),
+ e_Icmag(i__),z_mag(i__),n_z_mag(i__),e_z_mag(i__),Hmag(i__),
+ n_Hmag(i__),e_Hmag(i__),Ksmag(i__),n_Ksmag(i__),e_Ksmag(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table5.dat' ! Spectral Features and Classifications
C Format for file interpretation
2 format(
+ 2X,A7,1X,I1,1X,I1,1X,I1,1X,I1,1X,I1,1X,I1,1X,I1,1X,I1,1X,I1,
+ 1X,I1,1X,I1,1X,I1,1X,I1,1X,I3,1X,I2,1X,F5.3)
C Effective file loading
open(unit=1,status='old',file=
+'table5.dat')
write(6,*) '....Loading file: table5.dat'
do i__=1,273
read(1,'(A49)')ar__1
read(ar__1,2)
+ GDDS_1(i__),AGN(i__),v_OII_(i__),v_OIII_(i__),HiBal(i__),
+ LoBal(i__),Fe2375(i__),Fe2600(i__),Mg2800(i__),Mg2852(i__),
+ HandK(i__),Balmer(i__),D4000(i__),Temp(i__),Class(i__),
+ Conf_1(i__),z_1(i__)
c ..............Just test output...........
write(6,2)
+ GDDS_1(i__),AGN(i__),v_OII_(i__),v_OIII_(i__),HiBal(i__),
+ LoBal(i__),Fe2375(i__),Fe2600(i__),Mg2800(i__),Mg2852(i__),
+ HandK(i__),Balmer(i__),D4000(i__),Temp(i__),Class(i__),
+ Conf_1(i__),z_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end