Conversion of standardized ReadMe file for
file /./ftp/cats/J/AJ/131/2426 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-19
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/131/2426 Optical and radio study of Abell 2111 (Miller+, 2006)
*================================================================================
*Abell 2111: an optical and radio study of the richest Butcher-Oemler cluster.
* Miller N.A., Oegerle W.R., Hill J.M.
* <Astron. J., 131, 2426-2441 (2006)>
* =2006AJ....131.2426M
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Velocity data from optical spectroscopy
integer*4 nr__
parameter (nr__=205) ! Number of records
character*77 ar__ ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg ! (deg) Right Ascension J2000
real*8 DEdeg ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 RAh ! (h) Hour of Right Ascension (J2000)
integer*4 RAm ! (min) Minute of Right Ascension (J2000)
real*4 RAs ! (s) Second of Right Ascension (J2000)
character*1 DE_ ! Sign of the Declination (J2000)
integer*4 DEd ! (deg) Degree of Declination (J2000)
integer*4 DEm ! (arcmin) Arcminute of Declination (J2000)
real*4 DEs ! (arcsec) Arcsecond of Declination (J2000)
integer*4 cz ! (km/s) Heliocentric radial velocity
character*3 f_cz ! Flag(s) on cz (1)
integer*4 e_cz ! (km/s) Error in cz
character*39 Line ! Observed line(s) (2)
*Note (1): Flag on cz, defined as follows:
* a = A consistent velocity was found for this galaxy via cross correlation
* of absorption features with velocity standards.
* b = A velocity for this galaxy is also reported in NED.
* c = A velocity for this galaxy is also in the SDSS DR4.
*Note (2): When a velocity has been determined on the basis of emission
* lines, these lines are noted in this column. If identified lines are
* offset by parentheses, they were not used to determine the reported
* velocity but were found to be consistent with that velocity. Note that
* [OIII] usually refers to the {lambda}5007 line, but sometimes also
* includes the {lambda}4959 line. Similarly, [NII] is usually the
* {lambda}6584 line but may also include the {lambda}6548 line and [SII]
* may be either or both of {lambda}6717 and {lambda}6731.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Radio sources with optical counterparts
(separation radio/optical < 1.5arcsec)
integer*4 nr__1
parameter (nr__1=175) ! Number of records
character*60 ar__1 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_1 ! (deg) Right Ascension J2000
real*8 DEdeg_1 ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 RAh_1 ! (h) Hour of Right Ascension (J2000)
integer*4 RAm_1 ! (min) Minute of Right Ascension (J2000)
real*4 RAs_1 ! (s) Second of Right Ascension (J2000)
character*1 DE__1 ! Sign of the Declination (J2000)
integer*4 DEd_1 ! (deg) Degree of Declination (J2000)
integer*4 DEm_1 ! (arcmin) Arcminute of Declination (J2000)
real*4 DEs_1 ! (arcsec) Arcsecond of Declination (J2000)
real*4 z ! Redshift (photometric for sources without
* spectroscopy)
character*1 r_z ! Reference for z (1)
real*4 rmag ! (mag) SDSS r band magnitude
character*1 f_rmag ! [a] Classified as star in SDSS photometric data
integer*4 S1_4 ! (uJy) The 1.4GHz flux density
character*1 f_S1_4 ! [de] Note for extended sources (3)
integer*4 e_S1_4 ! (uJy) Error in S1.4GHz
integer*4 rms ! (uJy) The rms sensitivity
character*1 Res ! [RU] Resolved (R) or unresolved (U) (4)
real*4 Sep ! (arcsec) Separation
*Note (1): Reference for z, defined as follows:
* b = Redshift from SDSS DR4;
* c = Redshift from Morrison et al. (2003, Cat. J/ApJS/146/267).
*Note (3): Flag on S1.4GHz, defined as follows:
* d = Extended radio galaxy with morphology of a compact double, with flux
* calculated by TVSTAT. The separation listed is for the midpoint of the
* two radio lobes relative to the optical position. There is additional
* diffuse to the southeast, possibly associated with the galaxy.
* Including this emission the total flux is 19.8mJy with an error of
* 0.5mJy. The galaxy and its radio emission are depicted in Figure 9.
* e = Extended radio source, TVSTAT.
*Note (4): Sources for which the fitted major axis had a minimum size of
* zero were considered unresolved, and their peak flux measurements
* were adopted as their flux; otherwise, the fitted integral flux
* was adopted.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Spectroscopic classifications of cluster members
(Tables 3 and 4 of the paper)
integer*4 nr__2
parameter (nr__2=95) ! Number of records
character*74 ar__2 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_2 ! (deg) Right Ascension J2000
real*8 DEdeg_2 ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 RAh_2 ! (h) Hour of Right Ascension (J2000)
integer*4 RAm_2 ! (min) Minute of Right Ascension (J2000)
real*4 RAs_2 ! (s) Second of Right Ascension (J2000)
character*1 DE__2 ! Sign of the Declination (J2000)
integer*4 DEd_2 ! (deg) Degree of Declination (J2000)
integer*4 DEm_2 ! (arcmin) Arcminute of Declination (J2000)
real*4 DEs_2 ! (arcsec) Arcsecond of Declination (J2000)
character*4 Class ! Source class (1)
real*4 S_N ! Signal-to-noise per resolution element
* near H{delta}
character*1 Color ! [BR] Color type (2)
real*4 Dist ! (Mpc) Distance from cluster center
character*1 Radio ! [DNO] Radio detection (3)
real*4 z_1 ! ? Redshift
real*4 RMAG_1 ! (mag) ? Absolute R magnitude (4)
real*4 D_g_r ! (mag) ? Color relative to the cluster
* color-magnitude relation (4)
real*4 log_L1_4 ! ([W/Hz]) ? Log of the 1.4GHz luminosity (4)
real*4 SFR ! (solMass/yr) ? Star formation rate (4)
character*1 f_SFR ! [a] AGN likelihood (4) (5)
*Note (1): Source class, defined as follows:
* e(a) = star-forming galaxies with strong H{delta} absorption
* e(c) = galaxies with spectra representative of continuous star formation
* histories evidenced by moderate [OII] emission and at most slight
* H{delta} absorption
* e(n) = galaxies with line widths and other lines such as [OIII]
* indicating an AGN
* k = passive galaxies, lacking emission lines
* k+a = strong H{delta} absorption caused by a large population of
* young A stars
*Note (2): Color type, defined as follows:
* R = consistent with red sequence;
* B = blue in Butcher & Oemler (1984ApJ...285..426B) sense
* (i.e., {Delta}(g-r)<=-0.2).
*Note (3): Radio detection, defined as follows:
* N = non-detected;
* D = detected;
* O = outside surveyed area.
*Note (4): Additional data from Table 4.
*Note (5): Based on the color and/or optical spectrum, this galaxy is likely
* to have an AGN, and hence the SFR is an upper limit due to inclusion
* of radio emission associated with the active nucleus.
C=============================================================================
C Loading file 'table1.dat' ! Velocity data from optical spectroscopy
C Format for file interpretation
1 format(
+ I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,I6,1X,A3,1X,I2,1X,
+ A39)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,205
read(1,'(A77)')ar__
read(ar__,1)RAh,RAm,RAs,DE_,DEd,DEm,DEs,cz,f_cz,e_cz,Line
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)RAh,RAm,RAs,DE_,DEd,DEm,DEs,cz,f_cz,e_cz,Line
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! Radio sources with optical counterparts
* (separation radio/optical < 1.5arcsec)
C Format for file interpretation
2 format(
+ I2,1X,I2,1X,F5.2,A1,I2,1X,I2,1X,F4.1,1X,F6.4,1X,A1,1X,F5.2,1X,
+ A1,1X,I5,1X,A1,1X,I3,1X,I2,1X,A1,1X,F3.1)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,175
read(1,'(A60)')ar__1
read(ar__1,2)
+ RAh_1,RAm_1,RAs_1,DE__1,DEd_1,DEm_1,DEs_1,z,r_z,rmag,f_rmag,
+ S1_4,f_S1_4,e_S1_4,rms,Res,Sep
RAdeg_1 = rNULL__
DEdeg_1 = rNULL__
c Derive coordinates RAdeg_1 and DEdeg_1 from input data
c (RAdeg_1 and DEdeg_1 are set to rNULL__ when unknown)
if(RAh_1 .GT. -180) RAdeg_1=RAh_1*15.
if(RAm_1 .GT. -180) RAdeg_1=RAdeg_1+RAm_1/4.
if(RAs_1 .GT. -180) RAdeg_1=RAdeg_1+RAs_1/240.
if(DEd_1 .GE. 0) DEdeg_1=DEd_1
if(DEm_1 .GE. 0) DEdeg_1=DEdeg_1+DEm_1/60.
if(DEs_1 .GE. 0) DEdeg_1=DEdeg_1+DEs_1/3600.
if(DE__1.EQ.'-'.AND.DEdeg_1.GE.0) DEdeg_1=-DEdeg_1
c ..............Just test output...........
write(6,2)
+ RAh_1,RAm_1,RAs_1,DE__1,DEd_1,DEm_1,DEs_1,z,r_z,rmag,f_rmag,
+ S1_4,f_S1_4,e_S1_4,rms,Res,Sep
write(6,'(6H Pos: 2F8.4)') RAdeg_1,DEdeg_1
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3.dat' ! Spectroscopic classifications of cluster members
* (Tables 3 and 4 of the paper)
C Format for file interpretation
3 format(
+ I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,A4,1X,F4.1,1X,A1,
+ 1X,F4.2,1X,A1,1X,F6.4,1X,F6.2,1X,F5.2,1X,F5.2,1X,F4.1,A1)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,95
read(1,'(A74)')ar__2
read(ar__2,3)
+ RAh_2,RAm_2,RAs_2,DE__2,DEd_2,DEm_2,DEs_2,Class,S_N,Color,
+ Dist,Radio,z_1,RMAG_1,D_g_r,log_L1_4,SFR,f_SFR
if(ar__2(44:49) .EQ. '') z_1 = rNULL__
if(ar__2(51:56) .EQ. '') RMAG_1 = rNULL__
if(ar__2(58:62) .EQ. '') D_g_r = rNULL__
if(ar__2(64:68) .EQ. '') log_L1_4 = rNULL__
if(ar__2(70:73) .EQ. '') SFR = rNULL__
RAdeg_2 = rNULL__
DEdeg_2 = rNULL__
c Derive coordinates RAdeg_2 and DEdeg_2 from input data
c (RAdeg_2 and DEdeg_2 are set to rNULL__ when unknown)
if(RAh_2 .GT. -180) RAdeg_2=RAh_2*15.
if(RAm_2 .GT. -180) RAdeg_2=RAdeg_2+RAm_2/4.
if(RAs_2 .GT. -180) RAdeg_2=RAdeg_2+RAs_2/240.
if(DEd_2 .GE. 0) DEdeg_2=DEd_2
if(DEm_2 .GE. 0) DEdeg_2=DEdeg_2+DEm_2/60.
if(DEs_2 .GE. 0) DEdeg_2=DEdeg_2+DEs_2/3600.
if(DE__2.EQ.'-'.AND.DEdeg_2.GE.0) DEdeg_2=-DEdeg_2
c ..............Just test output...........
write(6,3)
+ RAh_2,RAm_2,RAs_2,DE__2,DEd_2,DEm_2,DEs_2,Class,S_N,Color,
+ Dist,Radio,z_1,RMAG_1,D_g_r,log_L1_4,SFR,f_SFR
write(6,'(6H Pos: 2F8.4)') RAdeg_2,DEdeg_2
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end