Search for Gamma-ray Emission Coincident with Giant Radio Pulses from the Crab

Details Search for Gamma-ray Emission Coincident with Giant Radio Pulses from the Crab Search for Gamma-ray Emission Coincident with Giant Radio Pulses from the Crab

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aps..apr.c1018s&link_type=abstract

American Physical Society, APS April Meeting 2010, February 13-16, 2010, abstract #C1.018

Physics

Scientific paper

The Crab Nebula is a pulsar-powered wind nebula and supernova remnant. Non-thermal pulsed and steady emission has been measured from radio to very-high-energy (VHE, E>100 GeV) gamma-ray energies. At radio wavelengths strong bursts, called giant pulses, are observed at irregular intervals, but no counterparts have been observed at VHE energies. Observations of the Crab were carried out simultaneously with the Green Bank Radio Telescope, Fermi and VERITAS. VERITAS, besides being the most sensitive VHE instrument is also sensitive to bursts of high energy (HE, >100 MeV) gamma rays with good sensitivity. We present the results of a search for HE and VHE gamma-ray emission in coincidence with radio giant pulses. )

Affiliated with

Also associated with

No associations

Rating

Search for Gamma-ray Emission Coincident with Giant Radio Pulses from the Crab does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Search for Gamma-ray Emission Coincident with Giant Radio Pulses from the Crab, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Search for Gamma-ray Emission Coincident with Giant Radio Pulses from the Crab will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1309876