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  • Speaker: Claudia Scarlata (U. Minnesota)
  • Host Department: Astronomy
  • Date: 04/18/2013
  • Time: 4:00 PM - 5:00 PM

  • Location: Dennison 807

  • Description:

    The WFC3 Infrared Spectroscopic Parallel Survey (WISP) is a large ( ~1000 orbits) HST program that uses WFC3 slitless spectroscopy to detect thousands of galaxies across a wide redshift range 0.3 < z < 2.3. I will present an overview of recent results on emission line galaxies, including a statistical determination of their dust extinction properties, the discovery of a new population of extremely strong emission-line dwarf galaxies, and the implication of the observed number counts for the EUCLID mission. I will also discuss the properties of passive galaxies at z~1.5 derived from the combination of the WISP spectra with broad-band photometry from HST-UVIS and Spitzer images.

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