#!/opt/gnu/bin/perl -wT use CGI ":standard"; use CGI::Carp "fatalsToBrowser"; use lib "../"; use Models; #my defined module for 2Dust models use 2dustInformation; $query = new CGI; print header; &displayPage; print end_html; #display the main page sub displayPage { #print start_html({-title=>"2Dust Model Information"}); print ""; print "Available 2Dust Models\n"; print ""; print "
"; print "
"; &dSingsHeader; #display the table of information @modelkeys =sort alphabetically keys(%sampleInfo); print "
"; print "\n"; print ""; print < HTML print ""; print ""; for ($j=0;$j<=13;$j++){ print ""; } print ""; for $i (@modelkeys) { if ($i ne "Model"){ print "\n"; print ""; for ($j=0;$j<=13;$j++){ print ""; } print "\n"; } } print "


Model Sample Information
Note that NGC4552 has been added in place of NGC1399


Model$sampleInfo{'Model'}[$j]
$i$sampleInfo{$i}[$j]
\n"; print < 

Notes:

(1) ID
(2) RC3 Type
(3) Nuclear Type: H=HII-region, SB=Starburst, L=LINER, Sy=Seyfert(1, 2)
(4) Major and minor axis diameters
(5) Heliocentric velocity
(6) Flow-corrected distance in Mpc, for Ho=70 km/s/Mpc
(7) Absolute R magnitude, when available; from the V or B bands
(8) FIR/optical luminosity ratio. The FIR luminosity is derived from the IRAS-measured 60-100 fluxes, 
	from Fullmer & Lonsdale (1989). The optical luminosity is defined as: 

	.

(9): The ratio of the 60 to 100 flux, measured by IRAS (see note above).
(10): Logarithmic gas mass, from HI and CO integrated fluxes; `H' denotes only HI data are
	available from the literature; `C' denotes only CO data available.
(11): Star formation rates derived from nebular emission, with typical A(H) = 1 mag.
(12): Oxygen abundance of the ionized gas, 12+log(O/H), at 0.4 R25.
(13): Additional data already available for a galaxy, generally from public archives. 
  	IUE=UV spectra from IUE. 
	UIT=UV images from Astro2/UIT. 
	HST= UV and/or Optical images from the HST archive. 
	ISO=data from ISO, CII=[CII] emission, at 158 micron measured by ISO. 
	CO=CO maps from the SONG collaboration; 
	HI=HI maps from the VLA or WSRT.

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HTML } sub numerically { $a <=> $b } sub alphabetically { lc $a cmp lc $b }