Probing IGM With FIREBALL And CWI

Details Probing IGM With FIREBALL And CWI Probing IGM With FIREBALL And CWI

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21742602r&link_type=abstract

American Astronomical Society, AAS Meeting #217, #426.02; Bulletin of the American Astronomical Society, Vol. 43, 2011

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Scientific paper

We present overview and initial results from the balloon borne UV instrument FIREBALL and Palomar Hale Telescope instrument CWI. The FIREBALL experiment is designed to search for IGM Ly-a emission at a redshift of 0.7 and other hot gas tracers from z=0.3 to z=1.0. We report on the data and initial science results from our flight in June, 2009. CWI is an integral field spectrograph which probes the strong, redshift UV resonance lines of Lyα 1216, CIV 1550, and OVI 1033 over 3600-9000 Å to trace IGM at 1 < z < 7.

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