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Veritas: Status c. 2009

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arxiv 1001.5305 v1 pith:TOXZPA2O submitted 2010-01-29 astro-ph.HE

Veritas: Status c. 2009

classification astro-ph.HE
keywords veritasarrayatmosphericbeencherenkovgamma-rayimagingobservatory
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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VERITAS is a ground-based gamma-ray observatory that uses the imaging atmospheric Cherenkov technique and operates in the very high-energy (VHE) region of the gamma- ray spectrum from 100 GeV to 50 TeV. The observatory consists of an array of four 12m-diameter imaging atmospheric Cherenkov telescopes located in southern Arizona, USA. The four-telescope array has been fully operational since September 2007, and over the last two years, VERITAS has been operating with high reliability and sensitivity. It is currently one of the most sensitive VHE observatories. This paper summarizes the status of VERITAS as of October, 2009, and describes the detection of several new VHE gamma-ray sources.

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