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Development of the Model of Galactic Interstellar Emission for Standard Point-source Analysis of Fermi Large Area Telescope Data
DOI: 10.3847/0067-0049/223/2/26 Bibcode: 2016ApJS..223...26A

Troja, E.; Caraveo, P. A.; Mirabal, N. +131 more

Most of the celestial γ rays detected by the Large Area Telescope (LAT) on board the Fermi Gamma-ray Space Telescope originate from the interstellar medium when energetic cosmic rays interact with interstellar nucleons and photons. Conventional point-source and extended-source studies rely on the modeling of this diffuse emission for accurate char…

2016 The Astrophysical Journal Supplement Series
COS-B 364
Gamma-Ray Pulsar Studies with COMPTEL
DOI: 10.1086/192016 Bibcode: 1994ApJS...92..559H

Strong, A. W.; Grenier, I. A.; Diehl, R. +10 more

Since the launch of the Compton Gamma-Ray Observatory (CGRO) the number of detected gamma-ray pulsars increased from two to six. COMPTEL, on-board CGRO and sensitive to gamma-rays with energies between approximately 0.7 and 30 MeV, detected three of these unambiguously. The classical Crab and Vela pulsars have been observed on several occasions an…

1994 The Astrophysical Journal Supplement Series
COS-B 23
Gamma Rays from the Geminga Pulsar: Variations with Time and Phase
DOI: 10.1086/191907 Bibcode: 1994ApJS...90..813G

Grenier, I. A.; Hermsen, W.; Bennett, K. +5 more

Pulsed gamma radiation from the Geminga pulsar was recorded by the COS B satellite from 50 MeV to 5 GeV between 1975 and 1982. It has been analyzed to derive the source spectral properties as a function of time and phase. The two main peaks are separated by 0.50 +/- 0.01 in phase. Significant pulsed emission has also been detected in both phase re…

1994 The Astrophysical Journal Supplement Series
COS-B 10