activity
20042007
most citedThe sky distribution of 511 keV positron annihilation line emission as measured with INTEGRAL/SPI

10 citations · 31 across the 15 of their papers we have counts for

collaborators
Showing 2004Show all

8 papers · 1 filter

astro-ph2004

Hypernovae and light dark matter as possible Galactic positron sources

S. Schanne, M. Casse, J. Paul +1

The electron-positron annihilation source in the Galactic center region has recently been observed with INTEGRAL/SPI, which shows that this 511 keV source is strong and its extensi…

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-ph20045 cited

The INTEGRAL/SPI response and the Crab observations

P. Sizun, C. R. Shrader, D. Attie +8

The Crab region was observed several times by INTEGRAL for calibration purposes. This paper aims at underlining the systematic interactions between (i) observations of this referen…

astro-ph2004

Al(26) Studies with INTEGRAL's Spectrometer SPI

R. Diehl, K. Kretschmer, G. Lichti +13

Al(26) radioactivity traces recent nucleosynthesis throughout the Galaxy, and is known to be produced in massive stars and novae. The map from its decay gamma-ray line suggests mas…

astro-ph20044 cited

Search for a light dark matter annihilation signal in the Sagittarius Dwarf Galaxy

B. Cordier, D. Attie, M. Casse +6

The 511 keV emission from the Galactic Bulge observed by INTEGRAL/SPI could be the product of light (1-100 MeV) annihilating dark matter particles. In order to distinguish between…

astro-ph20042 cited

Integral and Light Dark Matter

M. Casse, P. Fayet, S. Schanne +2

The nature of Dark Matter remains one of the outstanding questions of modern astrophysics. The success of the Cold Dark Matter cosmological model argues strongly in favor of a majo…