Add to ORKGJournal ArticleDuring November/December 2007, we observed the region centered on the Geminga Pulsar for 10.4 hours using the VERITAS IACT Observatory. We find no evidence for either steady emission point source emission, or pulsed emission of a point source at the period of the Geminga pulsar (237 msec). The measured VHE y-ray flux limits for the impulsed search is Fy(> 300 GeV , 99% c.l) lOOGeV , 99%c.l.) < 0.8 - 1.0 x 10-8 m-2 s"1
Geminga is an enigmatic radio-quiet γ-ray pulsar located at a mere 250 pc distance from Earth. Exten...
AbstractVERITAS is a ground-based gamma-ray observatory consisting of an array of four atmospheric C...
The Very Energetic Radiation Imaging Telescope Array System (VERITAS) observes astronomical sources ...
The Geminga pulsar, one of the brighest gamma-ray sources, is a promising candidate for emission of ...
We present the results of 71.6 hr of observations of the Geminga pulsar (PSR J0633+1746) with the VE...
We present the results of 71.6 hr of observations of the Geminga pulsar (PSR J0633+1746) with the VE...
We present the results of 71.6 hr of observations of the Geminga pulsar (PSR J0633+1746) with the VE...
We present the results of 71.6 hours of observations of the Geminga pulsar (PSR J0633+1746) with the...
Highly extended gamma-ray emission around the Geminga pulsar was discovered by Milagro and verified ...
dissertationThe closest known supernova remnant and pulsar is Geminga. The Geminga pulsar is the fir...
Highly extended gamma-ray emission around the Geminga pulsar was discovered by Milagro and verified ...
The improvements in the ground-based techniques for γ-ray detection, particularly the Imaging Atmosp...
Abstract: Pulsed emission of γ-rays from Geminga pulsar were detected at the period of ∼ 237 ms by s...
Geminga is an enigmatic radio-quiet gamma-ray pulsar located at a mere 250 pc distance from Earth. E...
Per request by the author, and with approval from the advisor and graduate office, the errata was ad...
Geminga is an enigmatic radio-quiet γ-ray pulsar located at a mere 250 pc distance from Earth. Exten...
AbstractVERITAS is a ground-based gamma-ray observatory consisting of an array of four atmospheric C...
The Very Energetic Radiation Imaging Telescope Array System (VERITAS) observes astronomical sources ...
The Geminga pulsar, one of the brighest gamma-ray sources, is a promising candidate for emission of ...
We present the results of 71.6 hr of observations of the Geminga pulsar (PSR J0633+1746) with the VE...
We present the results of 71.6 hr of observations of the Geminga pulsar (PSR J0633+1746) with the VE...
We present the results of 71.6 hr of observations of the Geminga pulsar (PSR J0633+1746) with the VE...
We present the results of 71.6 hours of observations of the Geminga pulsar (PSR J0633+1746) with the...
Highly extended gamma-ray emission around the Geminga pulsar was discovered by Milagro and verified ...
dissertationThe closest known supernova remnant and pulsar is Geminga. The Geminga pulsar is the fir...
Highly extended gamma-ray emission around the Geminga pulsar was discovered by Milagro and verified ...
The improvements in the ground-based techniques for γ-ray detection, particularly the Imaging Atmosp...
Abstract: Pulsed emission of γ-rays from Geminga pulsar were detected at the period of ∼ 237 ms by s...
Geminga is an enigmatic radio-quiet gamma-ray pulsar located at a mere 250 pc distance from Earth. E...
Per request by the author, and with approval from the advisor and graduate office, the errata was ad...
Geminga is an enigmatic radio-quiet γ-ray pulsar located at a mere 250 pc distance from Earth. Exten...
AbstractVERITAS is a ground-based gamma-ray observatory consisting of an array of four atmospheric C...
The Very Energetic Radiation Imaging Telescope Array System (VERITAS) observes astronomical sources ...