Dr. Jason
Melbourne
Postdoctoral Scholar in Astrophysics
California Institute of Technology
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California Institute of Technology
MS 301-17
Pasadena CA 91125
USA
(626) 395-6627

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2003
The Center for Adaptive Optics Treasury Survey (CATS)
A 3 color image combining Keck Adaptive Optics K-band (red)
with HST ACS V (blue) and z (green) in the GEMS field
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2005
CATS detects z=1.3 SN with Keck Adaptive Optics (H=24 Vega)

CATS images a gas rich merger with significant star formation (in GOODS-S)

CATS images a "dry" merger with little gas or star formation (in GOODS-S)
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