Observed Properties of Lyman Alpha Emitters from the Virus-p Survey at 2<z<4

Details Observed Properties of Lyman Alpha Emitters from the Virus-p Survey at 2<z<4 Observed Properties of Lyman Alpha Emitters from the Virus-p Survey at 2<z<4

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...211.5213f&link_type=abstract

American Astronomical Society, AAS Meeting #211, #52.13; Bulletin of the American Astronomical Society, Vol. 39, p.822

Astronomy and Astrophysics

Astronomy

Scientific paper

We study the spectroscopic and photometric properties of Lyman Alpha Emitter galaxies detected with the VIRUS-P spectrograph on the McDonald 2.7m telescope. VIRUS-P is an integral-field spectrograph composed of 247 fibers, each one 13.5 square arcseconds on sky. This blind redshift survey is a precursor to the Hobby-Eberly Telescope Dark Energy Experiment. From the data reduced to date, we find dozens of LAEs and twice as many [OII] emitters to a flux limit of 5e-17 ergs/s/cm^2. We sample a uniquely large redshift range of 1.9

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