BATSE/OSSE rapid burst response
Matz, S. M. ; Grove, J. E. ; Johnson, W. N. ; Kurfess, J. D. ; Share, G. H. ; Fishman, G. J. ; Meegan, C. A.
Springer
Published 1995
Springer
Published 1995
| ISSN: |
1572-946X
|
|---|---|
| Keywords: |
Gamma-ray bursts ; Counterparts ; Instrumentation
|
| Source: |
Springer Online Journal Archives 1860-2000
|
| Topics: |
Physics
|
| Notes: |
Abstract The BATSE and OSSE instrument teams have modified flight software to promptly (within 2 min of trigger) slew the OSSE detectors to burst locations determined on-board by BATSE. This enables OSSE to make sensitive searches for prompt and delayed post-burst line and continuum emission above 50 keV. In the best cases our sensitivity will be more than an order of magnitude better than any other search in this energy range. We expect to slew to 1–2 bursts per month, based on the OSSE FOV and BATSE event rate. Detections or limits from continued operation of this system may provide significant constraints on burst models. As an example of the observations made using this system, we present preliminary limits for post-burst emission from GRB 950223 on several time scales.
|
| Type of Medium: |
Electronic Resource
|
| URL: |
| _version_ | 1798296450358050817 |
|---|---|
| autor | Matz, S. M. Grove, J. E. Johnson, W. N. Kurfess, J. D. Share, G. H. Fishman, G. J. Meegan, C. A. |
| autorsonst | Matz, S. M. Grove, J. E. Johnson, W. N. Kurfess, J. D. Share, G. H. Fishman, G. J. Meegan, C. A. |
| book_url | http://dx.doi.org/10.1007/BF00658601 |
| datenlieferant | nat_lic_papers |
| hauptsatz | hsatz_simple |
| identnr | NLM193064197 |
| issn | 1572-946X |
| journal_name | Astrophysics and space science |
| materialart | 1 |
| notes | Abstract The BATSE and OSSE instrument teams have modified flight software to promptly (within 2 min of trigger) slew the OSSE detectors to burst locations determined on-board by BATSE. This enables OSSE to make sensitive searches for prompt and delayed post-burst line and continuum emission above 50 keV. In the best cases our sensitivity will be more than an order of magnitude better than any other search in this energy range. We expect to slew to 1–2 bursts per month, based on the OSSE FOV and BATSE event rate. Detections or limits from continued operation of this system may provide significant constraints on burst models. As an example of the observations made using this system, we present preliminary limits for post-burst emission from GRB 950223 on several time scales. |
| package_name | Springer |
| publikationsjahr_anzeige | 1995 |
| publikationsjahr_facette | 1995 |
| publikationsjahr_intervall | 8004:1995-1999 |
| publikationsjahr_sort | 1995 |
| publisher | Springer |
| reference | 231 (1995), S. 127-130 |
| schlagwort | Gamma-ray bursts Counterparts Instrumentation |
| search_space | articles |
| shingle_author_1 | Matz, S. M. Grove, J. E. Johnson, W. N. Kurfess, J. D. Share, G. H. Fishman, G. J. Meegan, C. A. |
| shingle_author_2 | Matz, S. M. Grove, J. E. Johnson, W. N. Kurfess, J. D. Share, G. H. Fishman, G. J. Meegan, C. A. |
| shingle_author_3 | Matz, S. M. Grove, J. E. Johnson, W. N. Kurfess, J. D. Share, G. H. Fishman, G. J. Meegan, C. A. |
| shingle_author_4 | Matz, S. M. Grove, J. E. Johnson, W. N. Kurfess, J. D. Share, G. H. Fishman, G. J. Meegan, C. A. |
| shingle_catch_all_1 | Matz, S. M. Grove, J. E. Johnson, W. N. Kurfess, J. D. Share, G. H. Fishman, G. J. Meegan, C. A. BATSE/OSSE rapid burst response Gamma-ray bursts Counterparts Instrumentation Gamma-ray bursts Counterparts Instrumentation Abstract The BATSE and OSSE instrument teams have modified flight software to promptly (within 2 min of trigger) slew the OSSE detectors to burst locations determined on-board by BATSE. This enables OSSE to make sensitive searches for prompt and delayed post-burst line and continuum emission above 50 keV. In the best cases our sensitivity will be more than an order of magnitude better than any other search in this energy range. We expect to slew to 1–2 bursts per month, based on the OSSE FOV and BATSE event rate. Detections or limits from continued operation of this system may provide significant constraints on burst models. As an example of the observations made using this system, we present preliminary limits for post-burst emission from GRB 950223 on several time scales. 1572-946X 1572946X Springer |
| shingle_catch_all_2 | Matz, S. M. Grove, J. E. Johnson, W. N. Kurfess, J. D. Share, G. H. Fishman, G. J. Meegan, C. A. BATSE/OSSE rapid burst response Gamma-ray bursts Counterparts Instrumentation Gamma-ray bursts Counterparts Instrumentation Abstract The BATSE and OSSE instrument teams have modified flight software to promptly (within 2 min of trigger) slew the OSSE detectors to burst locations determined on-board by BATSE. This enables OSSE to make sensitive searches for prompt and delayed post-burst line and continuum emission above 50 keV. In the best cases our sensitivity will be more than an order of magnitude better than any other search in this energy range. We expect to slew to 1–2 bursts per month, based on the OSSE FOV and BATSE event rate. Detections or limits from continued operation of this system may provide significant constraints on burst models. As an example of the observations made using this system, we present preliminary limits for post-burst emission from GRB 950223 on several time scales. 1572-946X 1572946X Springer |
| shingle_catch_all_3 | Matz, S. M. Grove, J. E. Johnson, W. N. Kurfess, J. D. Share, G. H. Fishman, G. J. Meegan, C. A. BATSE/OSSE rapid burst response Gamma-ray bursts Counterparts Instrumentation Gamma-ray bursts Counterparts Instrumentation Abstract The BATSE and OSSE instrument teams have modified flight software to promptly (within 2 min of trigger) slew the OSSE detectors to burst locations determined on-board by BATSE. This enables OSSE to make sensitive searches for prompt and delayed post-burst line and continuum emission above 50 keV. In the best cases our sensitivity will be more than an order of magnitude better than any other search in this energy range. We expect to slew to 1–2 bursts per month, based on the OSSE FOV and BATSE event rate. Detections or limits from continued operation of this system may provide significant constraints on burst models. As an example of the observations made using this system, we present preliminary limits for post-burst emission from GRB 950223 on several time scales. 1572-946X 1572946X Springer |
| shingle_catch_all_4 | Matz, S. M. Grove, J. E. Johnson, W. N. Kurfess, J. D. Share, G. H. Fishman, G. J. Meegan, C. A. BATSE/OSSE rapid burst response Gamma-ray bursts Counterparts Instrumentation Gamma-ray bursts Counterparts Instrumentation Abstract The BATSE and OSSE instrument teams have modified flight software to promptly (within 2 min of trigger) slew the OSSE detectors to burst locations determined on-board by BATSE. This enables OSSE to make sensitive searches for prompt and delayed post-burst line and continuum emission above 50 keV. In the best cases our sensitivity will be more than an order of magnitude better than any other search in this energy range. We expect to slew to 1–2 bursts per month, based on the OSSE FOV and BATSE event rate. Detections or limits from continued operation of this system may provide significant constraints on burst models. As an example of the observations made using this system, we present preliminary limits for post-burst emission from GRB 950223 on several time scales. 1572-946X 1572946X Springer |
| shingle_title_1 | BATSE/OSSE rapid burst response |
| shingle_title_2 | BATSE/OSSE rapid burst response |
| shingle_title_3 | BATSE/OSSE rapid burst response |
| shingle_title_4 | BATSE/OSSE rapid burst response |
| sigel_instance_filter | dkfz geomar wilbert ipn albert fhp |
| source_archive | Springer Online Journal Archives 1860-2000 |
| timestamp | 2024-05-06T09:52:17.473Z |
| titel | BATSE/OSSE rapid burst response |
| titel_suche | BATSE/OSSE rapid burst response |
| topic | U |
| uid | nat_lic_papers_NLM193064197 |