Follow-up Observations of Gamma-ray Bursts with STACEE
STACEE is an atmospheric Cherenkov telescope using the large mirror area of a solar research facility to obtain a low energy threshold. The telescope has a peak in the detected signal of a power-law gamma-ray spectrum near 100 GeV. The low energy threshold of STACEE allows detection of gamma rays fr...
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| creator | Williams, D A Alabiso, A Boone, L M Bramel, D Carson, J Covault, C E tin, P Gingrich, D M Hanna, D Jarvis, A Kildea, J Lindner, T Muellerr, C Mukherjee, R Ong, R A Ragan, K Scalzo, R A Zweerink, J |
| description | STACEE is an atmospheric Cherenkov telescope using the large mirror area of a solar research facility to obtain a low energy threshold. The telescope has a peak in the detected signal of a power-law gamma-ray spectrum near 100 GeV. The low energy threshold of STACEE allows detection of gamma rays from higher redshifts than most other ground-based experiments. The STACEE instrument can be re-targeted to the position of a GRB within a few minutes of an alert to search for emission above 50 GeV. So far, data have been acquired within a few hours of the burst for five GRB. We discuss the STACEE sensitivity to high energy gamma-ray emission from GRB and preliminary results of the observations. |
| doi_str_mv | 10.1063/1.1878470 |
| format | Conference Proceeding |
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The telescope has a peak in the detected signal of a power-law gamma-ray spectrum near 100 GeV. The low energy threshold of STACEE allows detection of gamma rays from higher redshifts than most other ground-based experiments. The STACEE instrument can be re-targeted to the position of a GRB within a few minutes of an alert to search for emission above 50 GeV. So far, data have been acquired within a few hours of the burst for five GRB. 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We discuss the STACEE sensitivity to high energy gamma-ray emission from GRB and preliminary results of the observations.</description><subject>CHERENKOV COUNTERS</subject><subject>COSMIC GAMMA BURSTS</subject><subject>COSMIC GAMMA SOURCES</subject><subject>COSMIC PHOTONS</subject><subject>COSMIC RAY DETECTION</subject><subject>GAMMA ASTRONOMY</subject><subject>GAMMA RADIATION</subject><subject>GAMMA SPECTRA</subject><subject>GEV RANGE</subject><subject>PHOTON EMISSION</subject><subject>PHYSICS OF ELEMENTARY PARTICLES AND FIELDS</subject><subject>SENSITIVITY</subject><subject>TELESCOPE COUNTERS</subject><issn>0094-243X</issn><issn>1551-7616</issn><isbn>0735402299</isbn><isbn>9780735402294</isbn><fulltext>true</fulltext><rsrctype>conference_proceeding</rsrctype><creationdate>2005</creationdate><recordtype>conference_proceeding</recordtype><recordid>eNotj8tKAzEYRoMXsK0ufIMBwV3qn8vksqxDW4VCF1ZwNyRpQkemkzrJWHx7K3V1NofD9yF0T2BKQLAnMiVKKi7hAo1IWRIsBRGXaAySlRwo1foKjQA0x5Szjxs0TukTgGop1QiJRWzbeMTDoVjb5Ptvk5vYpSKGYmn2e4N781M8D33KqTg2eVe8bWbVfH6LroNpk7_75wS9L-ab6gWv1svXarbCkRKecZBUeU8ccEFkYI5z54SyuqQkgLTUOeK5EcwGA5wLW-qtBRGY1X7riFVsgh7O3ZhyUyfXZO92Lnadd7mmp_dQsj_r8Wwd-vg1-JTrfZOcb1vT-TikmmoFpwGK_QJrElVA</recordid><startdate>20050101</startdate><enddate>20050101</enddate><creator>Williams, D A</creator><creator>Alabiso, A</creator><creator>Boone, L M</creator><creator>Bramel, D</creator><creator>Carson, J</creator><creator>Covault, C E</creator><creator>tin, P</creator><creator>Gingrich, D M</creator><creator>Hanna, D</creator><creator>Jarvis, A</creator><creator>Kildea, J</creator><creator>Lindner, T</creator><creator>Muellerr, C</creator><creator>Mukherjee, R</creator><creator>Ong, R A</creator><creator>Ragan, K</creator><creator>Scalzo, R A</creator><creator>Zweerink, J</creator><scope>7U5</scope><scope>8FD</scope><scope>L7M</scope><scope>OTOTI</scope></search><sort><creationdate>20050101</creationdate><title>Follow-up Observations of Gamma-ray Bursts with STACEE</title><author>Williams, D A ; 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The telescope has a peak in the detected signal of a power-law gamma-ray spectrum near 100 GeV. The low energy threshold of STACEE allows detection of gamma rays from higher redshifts than most other ground-based experiments. The STACEE instrument can be re-targeted to the position of a GRB within a few minutes of an alert to search for emission above 50 GeV. So far, data have been acquired within a few hours of the burst for five GRB. We discuss the STACEE sensitivity to high energy gamma-ray emission from GRB and preliminary results of the observations.</abstract><cop>United States</cop><doi>10.1063/1.1878470</doi><tpages>5</tpages></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0094-243X |
| ispartof | AIP conference proceedings, 2005, Vol.745 (1), p.603-607 |
| issn | 0094-243X 1551-7616 |
| language | eng |
| recordid | cdi_osti_scitechconnect_20630538 |
| source | AIP Journals Complete |
| subjects | CHERENKOV COUNTERS COSMIC GAMMA BURSTS COSMIC GAMMA SOURCES COSMIC PHOTONS COSMIC RAY DETECTION GAMMA ASTRONOMY GAMMA RADIATION GAMMA SPECTRA GEV RANGE PHOTON EMISSION PHYSICS OF ELEMENTARY PARTICLES AND FIELDS SENSITIVITY TELESCOPE COUNTERS |
| title | Follow-up Observations of Gamma-ray Bursts with STACEE |
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