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<title>30th International Cosmic Ray Conference</title>
<description>The 30th International Cosmic Ray Conference will be held from July 3, 2007 to July 11, 2007 in Merida, Yucatan, Mexico.</description>
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<startDate>2007-07-03T08:00:00</startDate>
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 <title>Search for pulsed emission of TeV gamma rays from Geminga Pulsar</title>
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  <name>Merida, Mexico</name>
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  <room>Regency (Hyatt)</room>
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 <startDate>2007-07-06T14:45:00</startDate>
 <endDate>2007-07-06T14:45:00</endDate>
 <abstract>Pulsed emission of gamma/X rays from Geminga pulsar were detected earlier at the
period of ~237 msec using EGRET/ROSAT  instruments. However, there are conflicting
reports about emission of pulsed gamma rays from this pulsar at very high energies.
We have observed this source for about 56 hours using the PACT setup  during the last
6 years spanning c. 2000 to 2006. This pulsar was found to undergo a glitch during
1996-97 from X-ray observations as reported by Jackson et al. We have analysed our
data by extrapolaing the post-glitch pulsar elements to our epoch of observation and
using the "TEMPO" package for calculating the pulsar phase of each event. In this
paper we describe our data, analysis procedure and the results.</abstract>
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