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CALSCALE:GREGORIAN
PRODID:UW-Physics-TWaP
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SEQUENCE:0
UID:UW-Physics-Event-2871
DTSTART:20121213T153000
DTEND:20121213T170000
LOCATION:4421 Sterling Hall
SUMMARY:The WISP survey: overview of recent results for galaxies in the 1<z<2 redshift range\, Astronomy Colloquium\, Claudia Scarlata\, CALTECH
DESCRIPTION:The WFC3 Infrared Spectroscopic Parallel Survey (WISP) is a large ( 750 orbits) HST program using WFC3 slitless IR spectroscopy to detect thousands of galaxies across a wide redshift range 0.3 &lt; z &lt; 2.3. I will present an overview of recent results on emission line galaxies\, including a statistical determination of their dust extinction properties and the discovery of a new population of extremely strong emission-line dwarf galaxies. I will also discuss the stellar population properties of passive galaxies at za^1/41.5 derived from the combination of the WISP IR spectra and broad-band HST optical and Spitzer photometry.
URL:http://www.physics.wisc.edu/twap/view.php?id=2871
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