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1.
BOOK
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Energy spectrum and evidence for Extragalactic Origin of diffuse Gamma-Radiation in the MeV-Range (1974)
Garching bei München
Call number: SR 90.1026(95)
Location: Building A17
Branch Library: GFZ Library
Pages: 12 S.
2.
BOOK
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Call number: SR 90.1026(74)
Location: Building A17
Branch Library: GFZ Library
Pages: 24 S.
3.
BOOK
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Call number: SR 90.1026(82)
Location: Building A17
Branch Library: GFZ Library
Pages: 20 S.
4.
BOOK
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Diffuse cosmic and Atmospheric MeV gamma radiation from balloon observations (1977)
Garching bei München
Call number: SR 90.1026(133)
Location: Building A17
Branch Library: GFZ Library
Pages: 35 S.
5.
NASA TECHNICAL REPORTS
Strong gamma-ray bursts observed by COMPTEL during its second year of operation (1995)
Other Sources
Publication Date: 2011-08-19
Description: The imaging Compton telescope (COMPTEL) onboard the Compton Gamma Ray Observatory (CGRO) can localize gamma-ray bursts occurring inside its approximately 1 sr field-of-view in the energy range from 0.75 to 30 MeV with location accuracy of 1 deg. Additional time-resolved spectral measurements in the energy range 0.1 to 10 MeV are made by individual COMPTEL 'burst' detectors. During its second year of operation COMPTEL observed several gamma-ray bursts. Locations of five strong bursts (including the rapidly imaged events GRB 930131 and GRB 930309) are presented here along with the findings from preliminary spectral analysis.
Keywords: 89
Type: Advances in Space Research; 15; 5; p. (5)139-(5)142
6.
NASA TECHNICAL REPORTS
Diffuse continuum gamma rays from the Galaxy observed by COMPTEL (1994)
Other Sources
Publication Date: 2011-08-19
Description: The diffuse Galactic continuum gamma-ray emission has been studied using the full Sky Survey from COMPTEL on the Compton Observatory CGRO. The diffuse emission appears to be visible in the whole 0.75-30 MeV range covered by the instrument, although a considerable contribution from unresolved point sources cannot be excluded. A correlation analysis using HI and CO surveys of the Galaxy is used to derive the Galactic emissivity spectrum, and this is consistent with a smooth continuation to the spectrum at higher energies derived by a similar analysis of COS-B data. The apparent conversion factor from integrated CO temperature to molecular hydrogen column density can also be determined from the correlation analysis. The value obtained is consistent with results from COS-B and other non-gamma-ray methods. Calculations of the emissivity spectrum from bremsstrahlung from a cosmic-ray electron spectrum based on propagation models are compared with the observations.
Keywords: 90
Type: Astronomy and Astrophysics; 292; 1; p. 82-91
7.
PAPER
Low and medium energy gamma-ray astronomy - present status and future aspects
Amsterdam : Elsevier
Advances in Space Research 3 (1983), S. 59-69 
ISSN: 0273-1177
Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
Type of Medium: 1
8.
PAPER
ISSN: 0273-1177
Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
Type of Medium: 1
9.
PAPER
Map of the galactic center region in the 1.8 MeV ^2^6Al gamma-ray line
Amsterdam : Elsevier
Advances in Space Research 6 (1986), S. 149-152 
ISSN: 0273-1177
Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
Type of Medium: 1
10.
PAPER
The Gamma-Ray Observatory GRO in perspective
Amsterdam : Elsevier
Advances in Space Research 10 (1990), S. 243-253 
ISSN: 0273-1177
Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
Type of Medium: 1