Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/698/1682 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/ApJ/698/1682 Most luminous dusty galaxies (Weedman+, 2009)
*================================================================================
*Evolution of the most luminous dusty galaxies.
* Weedman D.W., Houck J.R.
* <Astrophys. J., 698, 1682-1697 (2009)>
* =2009ApJ...698.1682W
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Continuum luminosities for obscured AGNs
integer*4 nr__
parameter (nr__=115) ! Number of records
character*69 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 Seq ! Running sequence number
character*16 Name ! AGN name
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)
real*4 z ! Redshift
character*1 r_z ! [efg] Flag on z (1)
real*8 F8um ! (mJy) Observed flux density in continuum at rest
* frame 8um (2)
real*4 logL8 ! ([10-7W]) Rest-frame luminosity {nu}L_{nu}(8um) (3)
real*4 logLir ! ([10-7W]) ? Infrared luminosity (only for table 2) (4)
integer*4 Ref ! Reference number (5)
*Note (1): Flag as follows:
* e = Optical redshift and classification in Lacy et al. (2007,
* Cat. J/AJ/133/186)
* f = Optical redshift and classification in Simpson et al. (2006,
* Cat. J/MNRAS/372/741, <[SMR2006] VLA JHHMMSS+DDMMm> in Simbad)
* g = Optical redshift and classification from the SDSS
*Note (2): Observed flux density measured from published spectra in references
* given, or from our own extractions, as described in Section 2.3.
* Typical uncertainties are +/-5% for sources with f_{nu}_(8um)>~5mJy
* and +/-10% for sources with f_{nu}_(8um)~1mJy. Typical uncertainties
* are +/-5% in table 2. For sources in Schweitzer et al.
* (2008ApJ...679..101S, reference 17), f_{nu}_(8um) is determined by
* scaling from published f_{nu}_(6um) using the average spectra in
* Figure 2 of Schweitzer et al. for sources without PAH (characteristic
* of the highest luminosity sources), such that
* f_{nu}_(8um)/f_{nu}_(6um)=1.12.
*Note (3): Rest-frame luminosity determined using peak f_{nu}_(8um) and
* luminosity distances D_L_ from E.L. Wright,
* http://www.astro.ucla.edu/wright/CosmoCalc.html, for H_0_=71km/s/Mpc,
* {Omega}_M_=0.27 and {Omega}_{Lambda}_=0.73.
* (log[{nu}L_{nu}_(8um)(L_{sun}_)]=log[{nu}L_{nu}_(8um)(erg/s)]-33.59.)
*Note (4): For sources in Schweitzer et al. (2008ApJ...679..101S) (reference 17),
* L_ir_ is determined as in Sanders & Mirabel (1996ARA&A..34..749S) for
* sources having measured IRAS flux densities at all IRAS wavelengths;
* L_ir_=2.14x10^36^D_L_^2^[13.5(f_{nu}_(12um))+5.2(f_{nu}_(25um))
* +2.58(f_{nu}_(60um))+(f_{nu}(100um))] for flux densities in mJy
* and luminosities in erg/s (L_{sun}_=3.83x10^33^erg/s).
*Note (5): Reference for IRS spectrum as follows:
* 1 = Farrah et al. (2007ApJ...667..149F);
* 2 = Imanishi et al. (2007ApJS..171...72I);
* 3 = Sargsyan et al. (2008, Cat. J/ApJ/683/114);
* 4 = Shi et al. (2006, Cat. J/ApJ/653/127);
* 5 = Weedman & Houck (2009, Cat. J/ApJ/693/370);
* 6 = new spectra in Figure 2 [sources 73, 111 from archival program 30447 (G.
* Fazio, P.I.), source 90 from archival program 20629 (L. Yan, P.I.),
* source 16 from archival program 40539 (G. Helou, P.I), sources 13,20,21,
* 23,70 from our own new observations, program 50031];
* 7 = Brand et al. (2008ApJ...680..119B; <[BWD2008] SST24 JHHMMSS.s+DDMMSS> in
* Simbad);
* 8 = Farrah et al. (2009ApJ...696.2044F; <SWIRE JHHMMSS.ss+DDMMSS.s> in
* Simbad);
* 9 = Brand et al. (2008ApJ...673..119B; <[BWD2008] SST24 JHHMMSS.s+DDMMSS> in
* Simbad);
* 10 = Houck et al. (2005ApJ...622L.105H; <[HSW2005] SST24 JHHMMSS.ss+DDMMSS.s>
* in Simbad);
* 11 = Weedman et al. (2006ApJ...638..613W;
* <[WLH2006] SST24 JHHMMSS.ss+DDMMSS.s> in Simbad);
* 12 = Weedman et al. (2006ApJ...653..101W);
* 13 = Polletta et al. (2008ApJ...675..960P);
* 14 = Yan et al. (2007, Cat. J/ApJ/658/778;
* <[YSF2007] SST24 JHHMMSS.ss+DDMMSS.s> in Simbad); Sajina et
* al. (2007ApJ...664..713S);
* 15 = Martinez-Sansigre et al. (2008ApJ...674..676M);
* 16 = Hao et al. (2005ApJ...625L..75H);
* 17 = Schweitzer et al. (2008ApJ...679..101S);
* 18 = Markwick-Kemper et al. (2007ApJ...668L.107M);
* 19 = new extractions of sources in the FLS and SWIRE Lockman fields having
* f_{nu}_(24um)>5mJy and R>20mag which have optical redshifts and
* classifications cited as type 1 AGN in the NED;
* 20 = new extractions of sources available within Spitzer Legacy Program 40539
* (G. Helou, P.I.), a flux limited sample with f_{nu}_(24um)>5mJy, which
* have optical redshifts and classifications as type 1 AGN cited in the NED
* or as determined from our examination of SDSS spectra, not including 2
* sources also in reference 19.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Continuum luminosities for Silicate emission AGNs
integer*4 nr__1
parameter (nr__1=60) ! Number of records
character*69 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 Seq_1 ! Running sequence number
character*16 Name_1 ! AGN name
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_1 ! Redshift
character*1 r_z_1 ! [efg] Flag on z (1)
real*8 F8um_1 ! (mJy) Observed flux density in continuum at rest
* frame 8um (2)
real*4 logL8_1 ! ([10-7W]) Rest-frame luminosity {nu}L_{nu}(8um) (3)
real*4 logLir_1 ! ([10-7W]) ? Infrared luminosity (only for table 2) (4)
integer*4 Ref_1 ! Reference number (5)
*Note (1): Flag as follows:
* e = Optical redshift and classification in Lacy et al. (2007,
* Cat. J/AJ/133/186)
* f = Optical redshift and classification in Simpson et al. (2006,
* Cat. J/MNRAS/372/741, <[SMR2006] VLA JHHMMSS+DDMMm> in Simbad)
* g = Optical redshift and classification from the SDSS
*Note (2): Observed flux density measured from published spectra in references
* given, or from our own extractions, as described in Section 2.3.
* Typical uncertainties are +/-5% for sources with f_{nu}_(8um)>~5mJy
* and +/-10% for sources with f_{nu}_(8um)~1mJy. Typical uncertainties
* are +/-5% in table 2. For sources in Schweitzer et al.
* (2008ApJ...679..101S, reference 17), f_{nu}_(8um) is determined by
* scaling from published f_{nu}_(6um) using the average spectra in
* Figure 2 of Schweitzer et al. for sources without PAH (characteristic
* of the highest luminosity sources), such that
* f_{nu}_(8um)/f_{nu}_(6um)=1.12.
*Note (3): Rest-frame luminosity determined using peak f_{nu}_(8um) and
* luminosity distances D_L_ from E.L. Wright,
* http://www.astro.ucla.edu/wright/CosmoCalc.html, for H_0_=71km/s/Mpc,
* {Omega}_M_=0.27 and {Omega}_{Lambda}_=0.73.
* (log[{nu}L_{nu}_(8um)(L_{sun}_)]=log[{nu}L_{nu}_(8um)(erg/s)]-33.59.)
*Note (4): For sources in Schweitzer et al. (2008ApJ...679..101S) (reference 17),
* L_ir_ is determined as in Sanders & Mirabel (1996ARA&A..34..749S) for
* sources having measured IRAS flux densities at all IRAS wavelengths;
* L_ir_=2.14x10^36^D_L_^2^[13.5(f_{nu}_(12um))+5.2(f_{nu}_(25um))
* +2.58(f_{nu}_(60um))+(f_{nu}(100um))] for flux densities in mJy
* and luminosities in erg/s (L_{sun}_=3.83x10^33^erg/s).
*Note (5): Reference for IRS spectrum as follows:
* 1 = Farrah et al. (2007ApJ...667..149F);
* 2 = Imanishi et al. (2007ApJS..171...72I);
* 3 = Sargsyan et al. (2008, Cat. J/ApJ/683/114);
* 4 = Shi et al. (2006, Cat. J/ApJ/653/127);
* 5 = Weedman & Houck (2009, Cat. J/ApJ/693/370);
* 6 = new spectra in Figure 2 [sources 73, 111 from archival program 30447 (G.
* Fazio, P.I.), source 90 from archival program 20629 (L. Yan, P.I.),
* source 16 from archival program 40539 (G. Helou, P.I), sources 13,20,21,
* 23,70 from our own new observations, program 50031];
* 7 = Brand et al. (2008ApJ...680..119B; <[BWD2008] SST24 JHHMMSS.s+DDMMSS> in
* Simbad);
* 8 = Farrah et al. (2009ApJ...696.2044F; <SWIRE JHHMMSS.ss+DDMMSS.s> in
* Simbad);
* 9 = Brand et al. (2008ApJ...673..119B; <[BWD2008] SST24 JHHMMSS.s+DDMMSS> in
* Simbad);
* 10 = Houck et al. (2005ApJ...622L.105H; <[HSW2005] SST24 JHHMMSS.ss+DDMMSS.s>
* in Simbad);
* 11 = Weedman et al. (2006ApJ...638..613W;
* <[WLH2006] SST24 JHHMMSS.ss+DDMMSS.s> in Simbad);
* 12 = Weedman et al. (2006ApJ...653..101W);
* 13 = Polletta et al. (2008ApJ...675..960P);
* 14 = Yan et al. (2007, Cat. J/ApJ/658/778;
* <[YSF2007] SST24 JHHMMSS.ss+DDMMSS.s> in Simbad); Sajina et
* al. (2007ApJ...664..713S);
* 15 = Martinez-Sansigre et al. (2008ApJ...674..676M);
* 16 = Hao et al. (2005ApJ...625L..75H);
* 17 = Schweitzer et al. (2008ApJ...679..101S);
* 18 = Markwick-Kemper et al. (2007ApJ...668L.107M);
* 19 = new extractions of sources in the FLS and SWIRE Lockman fields having
* f_{nu}_(24um)>5mJy and R>20mag which have optical redshifts and
* classifications cited as type 1 AGN in the NED;
* 20 = new extractions of sources available within Spitzer Legacy Program 40539
* (G. Helou, P.I.), a flux limited sample with f_{nu}_(24um)>5mJy, which
* have optical redshifts and classifications as type 1 AGN cited in the NED
* or as determined from our examination of SDSS spectra, not including 2
* sources also in reference 19.
C=============================================================================
C Loading file 'table1.dat' ! Continuum luminosities for obscured AGNs
C Format for file interpretation
1 format(
+ I3,1X,A16,I2,I2,F5.2,A1,I2,I2,F4.1,1X,F6.4,A1,1X,F7.2,1X,F5.2,
+ 1X,F5.2,1X,I2)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,115
read(1,'(A69)')ar__
read(ar__,1)
+ Seq,Name,RAh,RAm,RAs,DE_,DEd,DEm,DEs,z,r_z,F8um,logL8,logLir,
+ Ref
if(ar__(62:66) .EQ. '') logLir = 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)
+ Seq,Name,RAh,RAm,RAs,DE_,DEd,DEm,DEs,z,r_z,F8um,logL8,logLir,
+ Ref
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! Continuum luminosities for Silicate emission AGNs
C Format for file interpretation
2 format(
+ I3,1X,A16,I2,I2,F5.2,A1,I2,I2,F4.1,1X,F6.4,A1,1X,F7.2,1X,F5.2,
+ 1X,F5.2,1X,I2)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,60
read(1,'(A69)')ar__1
read(ar__1,2)
+ Seq_1,Name_1,RAh_1,RAm_1,RAs_1,DE__1,DEd_1,DEm_1,DEs_1,z_1,
+ r_z_1,F8um_1,logL8_1,logLir_1,Ref_1
if(ar__1(62:66) .EQ. '') logLir_1 = rNULL__
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)
+ Seq_1,Name_1,RAh_1,RAm_1,RAs_1,DE__1,DEd_1,DEm_1,DEs_1,z_1,
+ r_z_1,F8um_1,logL8_1,logLir_1,Ref_1
write(6,'(6H Pos: 2F8.4)') RAdeg_1,DEdeg_1
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end