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19962007
most citedGamma-ray continuum emission from the inner Galactic region as observed with INTEGRAL/SPI

127 citations · 141 across the 11 of their papers we have counts for

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astro-ph20072 cited

Imaging the Gamma-Ray Sky with SPI aboard INTEGRAL

Jürgen Knödlseder, Georg Weidenspointner, Pierre Jean +6

The spectrometer SPI on INTEGRAL allows for the first time simultaneous imaging of diffuse and point-like emission in the hard X-ray and soft gamma-ray regime. To fully exploit the…

astro-ph2007

Soft gamma-ray galactic ridge emission as unveiled by SPI aboard INTEGRAL

Jürgen Knödlseder, Vincent Lonjou, Georg Weidenspointner +6

The origin of the soft gamma-ray (200 keV - 1 MeV) galactic ridge emission is one of the long-standing mysteries in the field of high-energy astrophysics. Population studies at low…

astro-ph2005127 cited

Gamma-ray continuum emission from the inner Galactic region as observed with INTEGRAL/SPI

A. W. Strong, R. Diehl, H. Halloin +5

The diffuse continuum emission from the Galactic plane in the energy range 18-1000 keV has been studied using 16 Ms of data from the SPI instrument on INTEGRAL. With such an exposu…

astro-ph2004

Measurements of Gamma-Ray Bursts (GRBs) with Glast

G. G. Lichti, M. Briggs, R. Diehl +9

One of the scientific goals of the main instrument of GLAST is the study of Gamma-Ray Bursts (GRBs) in the energy range from ~20 MeV to ~300 GeV. In order to extend the energy meas…

astro-ph20041 cited

Search for 44Ti gamma-ray line emission from GRO J0852-4642 with INTEGRAL/SPI

A. von Kienlin, D. Attie, S. Schanne +7

The gamma-ray source GRO J0852-4642, discovered by COMPTEL, is a possible counterpart of the supernova remnant RX J0852-4622. Detection of radioactive decay from 44Ti nuclei would…

astro-ph20042 cited

SPI/INTEGRAL observation of 1809 keV gamma-ray line emission from the Cygnus X region

J. Knödlseder, M. Valsesia, M. Allain +10

We present first results on the observation of 1809 keV gamma-ray line emission from the Cygnus X region with the SPI imaging spectrometer. Our analysis is based on data from the p…