| Autor: |
Smith, M. J.S., Gandolfi, G., Celidonio, G., Coletta, A., D'Andreta, G., Di Ciolo, L., Paolino, A., Ricci, R., Tarei, G., Tesseri, A., Torroni, V., Costa, E., Feroci, M., Frontera, F., Heise, J., Muller, J. M., Piro, L., Smith, M. J.S., Gandolfi, G., Celidonio, G., Coletta, A., D'Andreta, G., Di Ciolo, L., Paolino, A., Ricci, R., Tarei, G., Tesseri, A., Torroni, V., Costa, E., Feroci, M., Frontera, F., Heise, J., Muller, J. M., Piro, L. |
| Zdroj: |
Astronomy and Astrophysics. Supplement Series; September 1999, Vol. 138 Issue: 3 p561-562, 2p |
| Abstrakt: |
Sub-second GRBs have been identified as a separate class of gamma ray transients. However, despite recent advances in the field, sub-second GRB counterparts have yet to be found successfully. In order to explore the nature of these fast transients an on-line procedure is to be implemented at the BeppoSAX Scientific Operation Centre. The main objectives are the identification of true events and rapid position determination of their X-ray counterparts. |
| Databáze: |
Supplemental Index |
| Externí odkaz: |
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