HST images of the Toomre sequence from Seppo:

<img alt="" src="toomre3x2aw_thumb.jpg" style="border: 0px solid ; width: 180px; height: 121px;">     <img alt="" src="toomre3x2bw_thumb.jpg" style="border: 0px solid ; width: 180px; height: 121px;">

Min's CO data (FITS files):

NGC 4676


 Comparison Images:
<table style="width: 30%; text-align: left;" border="1" cellpadding="2" cellspacing="2"> <img alt="" src="ngc4676/ngc4676_irac_composite_thumb.jpg" style="border: 0px solid ; width: 125px; height: 89px;">
<img alt="" src="ngc4676/ngc4676_irac_composite2_thumb.jpg" style="border: 0px solid ; width: 125px; height: 89px;">
<img alt="" src="ngc4676/ngc4676_composite_thumb.jpg" style="border: 0px solid ; width: 124px; height: 90px;">
<img alt="" src="ngc4676/ngc4676_14cont_9.8H2_9.jpg" style="border: 0px solid ; width: 124px; height: 90px;">
<img alt="" src="ngc4676/ngc4676_11.3_9.8H2_9.jpg" style="border: 0px solid ; width: 124px; height: 90px;">
IRAC 5.6,8 and DSS images
IRAC 5.6,8 and IRS 11.3PAH, 9.7H2 emission
IRS SL1 9.7cont, 9.7H2, 11.3 PAH, 12.8NeII
IRS SL(R=14cont, G=9.7H2, B=9.7cont)
IRS SL (R=11.3PAH, G=9.7H2, B=9.7cont)
<img alt="" src="ngc4676/ngc4676_NeII_11.3_9.jpg" style="border: 0px solid ; width: 124px; height: 90px;">
<img alt="" src="ngc4676/ngc4676_9.7cont_6.2_5.jpg" style="border: 0px solid ; width: 124px; height: 90px;">
<img alt="" src="ngc4676/ngc4676_lowres1_thumb.jpg" style="border: 0px solid ; width: 119px; height: 149px;">


IRS SL (R=12.8NeII, G=11.3PAH, B=9.7cont)
IRS SL (R=9.7cont, G=6.2PAH, B=5.5cont)
IRS SL spectra of N and S nuclei



 

IRS FITS files made from the cubes:

 SL1-11.3PAH
 SL1-14continuum
 SL1-9.7continuum
 SL1-9.7H2
 SL1-12.8NeII
 SL2-6.2PAH
 SL2-5.5continuum


IRS cube project files:

SL1
SL2
LL1
LL2



NGC 6621

Comparison Images:
<table style="width: 50%; text-align: left;" border="1" cellpadding="2" cellspacing="2"> <img alt="" src="ngc6621/ngc6621_irac_composite_thumb.jpg" style="border: 0px solid ; width: 124px; height: 95px;">
<img alt="" src="ngc6621/ngc6621_irac_composite2_thumb.jpg" style="border: 0px solid ; width: 124px; height: 101px;">
<img alt="" src="ngc6621/ngc6621_composite_thumb.jpg" style="border: 0px solid ; width: 124px; height: 90px;">
<img alt="" src="ngc6621/ngc6621_NeII_11.3_9.jpg" style="border: 0px solid ; width: 124px; height: 90px;">
IRAC 5.6, 8, and DSS images
IRAC 5.6,8 and IRS 9.7cont, 11.3PAH
IRS 9.7cont, 11.3PAH, 12.2H2, 12.8NeII
IRS SL (R= 12.8NeII, G= 11.3PAH, B= 9.7cont)
<img alt="" src="ngc6621/ngc6621_14cont_11.3_9.jpg" style="border: 0px solid ; width: 124px; height: 90px;">
<img alt="" src="ngc6621/ngc6621_H26.9_6.2_6.jpg" style="border: 0px solid ; width: 124px; height: 90px;">
<img alt="" src="ngc6621/ngc6621_lowres1_thumb.jpg" style="border: 0px solid ; width: 119px; height: 149px;">

IRS SL (R= 14cont, G= 11.3PAH, B= 9.7cont)
IRS SL (R= 6.8H2, G= 6.2PAH, B= 6.5cont)
IRS SL spectra of N and S "nuclei"
(N=18:12:55.35 +68:21:45.8;
S=18:12:58.48 +68:21:27.8)





IRS FITS files made from the cubes:

SL1-11.3PAH
SL1-14continuum
SL1-9.7continuum
SL1-12.2H2
SL1-12.8NeII
SL2-6.2PAH
SL2-6.5continuum
SL2-6.9H2


IRS cube project files:

SL1
SL2
LL1
LL2



NGC 7592

 Comparison Images:

<table style="width: 50%; text-align: left;" border="1" cellpadding="2" cellspacing="2"> <img alt="" src="ngc7592/ngc7592_irac_composite_thumb.jpg" style="border: 0px solid ; width: 124px; height: 95px;">
<img alt="" src="ngc7592/ngc7592_irac_composite2_thumb.jpg" style="border: 0px solid ; width: 124px; height: 101px;">
<img alt="" src="ngc7592/ngc7592_composite_thumb.jpg" style="border: 0px solid ; width: 124px; height: 90px;">
<img alt="" src="ngc7592/ngc7592_NeII_11.3_5.jpg" style="border: 0px solid ; width: 124px; height: 90px;">
IRAC 5.6, 8, and DSS images
IRAC 5.6,8 and IRS 12.8NeII, 11.3PAH
IRS 11.3PAH, 12.8NeII, 5.5cont
IRS SL (R= 12.8NeII, G= 11.3PAH, B= 5.5cont)
<img alt="" src="ngc7592/ngc7592_lowres1_thumb.jpg" style="border: 0px solid ; width: 115px; height: 150px;">



IRS SL spectra of E,W,S, and total components





IRS FITS files made from the cubes:

SL1-11.3PAH
SL1-IRAC8
SL1-12.8NeII
SL2-6.2PAH
SL2-5.5continuum
SL2-IRAC5.8


IRS cube project files:

SL1
SL2
LL1
LL2



NGC 2623

Comparison Images:
<table style="width: 50%; text-align: left;" border="1" cellpadding="2" cellspacing="2"> <img alt="" src="ngc2623/ngc2623_irac_composite2_thumb.jpg" style="border: 0px solid ; width: 124px; height: 95px;">
<img alt="" src="ngc2623/ngc2623_irac_composite3_thumb.jpg" style="border: 0px solid ; width: 124px; height: 101px;">
<img alt="" src="ngc2623/ngc2623_composite_thumb.jpg" style="border: 0px solid ; width: 124px; height: 90px;">
<img alt="" src="ngc2623/ngc2623_lowres1_thumb.jpg" style="border: 0px solid ; width: 124px; height: 90px;">
IRAC 5.6, 8, DSS, and HST F814W images
IRAC 5.6,8 and IRS 11.3PAH, 12.8NeII
IRS 9.7cont, 11.3PAH, 12.2H2, 12.8NeII
IRS SL spectrum











IRS FITS files made from the cubes:

SL1-11.3PAH
SL1-13continuum
SL1-9.7continuum
SL1-9.7H2
SL1-12.8NeII
SL2-6.2PAH
SL2-6.8continuum


IRS cube project files:

SL1
SL2
LL1
LL2



NGC 520

Comparison Images:
<table style="width: 50%; text-align: left;" border="1" cellpadding="2" cellspacing="2"> <img alt="" src="ngc520/ngc520_irac_composite2_thumb.jpg" style="border: 0px solid ; width: 124px; height: 101px;">
<img alt="" src="ngc520/ngc520_composite_thumb.jpg" style="border: 0px solid ; width: 124px; height: 90px;">
<img alt="" src="ngc520/ngc520_lowres1_thumb.jpg" style="border: 0px solid ; width: 124px; height: 90px;">
IRAC 5.6,8 DSS, and IRS 11.3PAH
IRS 9.7cont, 11.3PAH, 9.7H2, and 12.8NeII
IRS SL spectra of East and West nuclei









IRS FITS files made from the cubes:

SL1-11.3PAH
SL1-14continuum
SL1-9.7continuum
SL1-9.7H2
SL1-12.8NeII
SL2-6.2PAH
SL2-5.8continuum
SL2-6.9H2


IRS cube project files:

SL1
SL2
LL1
LL2




NGC 3921

Comparison Images:
<table style="width: 50%; text-align: left;" border="1" cellpadding="2" cellspacing="2"> <img alt="" src="ngc3921/ngc3921_irac_composite_thumb.jpg" style="border: 0px solid ; width: 124px; height: 95px;">
<img alt="" src="ngc3921/ngc3921_irac_composite2_thumb.jpg" style="border: 0px solid ; width: 124px; height: 101px;">
<img alt="" src="ngc3921/ngc3921_composite_thumb.jpg" style="border: 0px solid ; width: 124px; height: 90px;">
<img alt="" src="ngc3921/ngc3921_lowres1_thumb.jpg" style="border: 0px solid ; width: 124px; height: 90px;">
IRAC 5.6, 8, and DSS images
IRAC 5.6,8 and IRS 9.7H2, 11.3PAH
IRS 6.2PAH, 11.3PAH, 9.7H2, 12.8NeII
IRS SL spectrum











IRS FITS files made from the cubes:

SL1-11.3PAH
SL1-14continuum
SL1-9.7continuum
SL1-9.7H2
SL1-12.8NeII
SL2-6.2PAH
SL2-5.8continuum
SL1-IRAC8
SL2-IRAC5.6


IRS cube project files:

SL1
SL2
LL1
LL2




NGC 7252

Comparison Images:
<table style="width: 50%; text-align: left;" border="1" cellpadding="2" cellspacing="2"> <img alt="" src="ngc7252/ngc7252_irac_composite_thumb.jpg" style="border: 0px solid ; width: 124px; height: 95px;">
<img alt="" src="ngc7252/ngc7252_irac_composite2_thumb.jpg" style="border: 0px solid ; width: 124px; height: 101px;">
<img alt="" src="ngc7252/ngc7252_composite_thumb.jpg" style="border: 0px solid ; width: 124px; height: 90px;">
<img alt="" src="ngc7252/ngc7252_lowres1_thumb.jpg" style="border: 0px solid ; width: 124px; height: 90px;">
IRAC 5.6, 8, and DSS images
IRAC 5.6,8 and IRS 11.3PAH
IRS 9.7H2, 11.3PAH, 12.8NeII, 14cont
IRS SL spectrum











IRS FITS files made from the cubes:

SL1-11.3PAH
SL1-14continuum
SL1-9.7H2
SL1-IRAC8
SL1-12.8NeII
SL2-6.2PAH
SL2-6.0continuum
SL2-IRAC5.6


IRS cube project files:

SL1
SL2
LL1
LL2


-- JohnHibbard - 05 Feb 2007
Topic revision: r1 - 2007-02-05, JohnHibbard
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