Physics
Scientific paper
Sep 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sptz.prop..108l&link_type=abstract
Spitzer Proposal ID #108
Physics
Scientific paper
Four ultraluminous galaxies will be monitored for supernova activity with oderately deep IRAC imaging at 4.5 and 8.0 microns. Arp 220, NGC 3690, NGC 7469 and NGC 1614 will be imaged with the 4.5 and 8.0 um IRAC arrays to a sensitivity of about 5 uJy, 1 sigma, approximately every 3 months for 2.5 years. A single 5.1 x 5.1 arcminute IRAC field will be used for each observation, no mapping will be done.
Gautier Nick
Lawrence Charles
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