Extragalactic Spectral Lines with the Expanded Very Large Array

Details Extragalactic Spectral Lines with the Expanded Very Large Array Extragalactic Spectral Lines with the Expanded Very Large Array

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21532607o&link_type=abstract

American Astronomical Society, AAS Meeting #215, #326.07; Bulletin of the American Astronomical Society, Vol. 42, p.423

Astronomy and Astrophysics

Astronomy

Scientific paper

The Expanded Very Large Array (EVLA) will revolutionize the field of spectral line detection and imaging in the radio domain. Within the full 1-50GHz frequency range, many lines can be imaged simultaneously at very high spectral resolution. This new capability will be used to derive accurate redshifts of highly obscured star forming galaxies at high redshift, to obtain deep field imaging (e.g., HI deep fields out to z=0.5), to determine the distribution and state of dense molecular gas involved in actual star formation events, and to derive parameters that are crucial for the formation and stability of molecular clouds on large and small scales such as magnetic fields. We will present an overview of the EVLA capabilities and an update on the current state of the telescope as well as possible first light observations.

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