|
Experiment: LILAS-2
RESEARCH OF THE COSMIC AND SOLAR GAMMA-RAY BURSTS
Main scientific objectives:
the localisation of the GRB sources with high precision ~10 arc sec (using the data of ULYSSES and BATSE-CGRO);
the analysis of the low energy absorption features in the spectra;
the studying of the thermal radiation at the damping stage of the GRB.
Physical and technical characteristics:
|
| |
Two Detectors NaI(Tl), | d x h = 72 x 16 mm |
Energy range | 5 KeV - 600 KeV |
Energy resolution | 8% at the line 5,9 keV; 40% - at 662 keV |
Sensitivity | 5·10-7 erg/cm2 |
Time resolution 1 ms for the research of the time structure, | 0.25 s for the spectrum analysis |
Power | 3 W |
Mass | 5 kg |
Cooperation:: Russia, France
Contact persons: | K.Barat (PI), barat@cers.cnes.fr
R.Suynaev (PI) rs@hea.iki.rssi.ru
|
|