Search for Dark Matter Annihilation in Draco with STACEE
For some time, the Draco dwarf spheroidal galaxy has garnered interest as a possible source for the indirect detection of dark matter. Its large mass-to-light ratio and relative proximity to the Earth provide favorable conditions for the production of detectable gamma rays from dark matter self-anni...
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| creator | STACEE Collaboration Driscoll, D. D Ball, J Carson, J. E Covault, C. E Fortin, P Gingrich, D. M Hanna, D. S Jarvis, A Kildea, J Lindner, T Mueller, C Mukherjee, R Ong, R. A Ragan, K Williams, D. A Zweerink, J |
| description | For some time, the Draco dwarf spheroidal galaxy has garnered interest as a
possible source for the indirect detection of dark matter. Its large
mass-to-light ratio and relative proximity to the Earth provide favorable
conditions for the production of detectable gamma rays from dark matter
self-annihilation in its core. The Solar Tower Atmospheric Cherenkov Effect
Experiment (STACEE) is an air-shower Cherenkov telescope located in
Albuquerque, NM capable of detecting gamma rays at energies above 100 GeV. We
present the results of the STACEE observations of Draco during the 2005-2006
observing season totaling 10 hours of livetime after cuts. |
| doi_str_mv | 10.48550/arxiv.0710.3545 |
| format | Article |
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possible source for the indirect detection of dark matter. Its large
mass-to-light ratio and relative proximity to the Earth provide favorable
conditions for the production of detectable gamma rays from dark matter
self-annihilation in its core. The Solar Tower Atmospheric Cherenkov Effect
Experiment (STACEE) is an air-shower Cherenkov telescope located in
Albuquerque, NM capable of detecting gamma rays at energies above 100 GeV. We
present the results of the STACEE observations of Draco during the 2005-2006
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possible source for the indirect detection of dark matter. Its large
mass-to-light ratio and relative proximity to the Earth provide favorable
conditions for the production of detectable gamma rays from dark matter
self-annihilation in its core. The Solar Tower Atmospheric Cherenkov Effect
Experiment (STACEE) is an air-shower Cherenkov telescope located in
Albuquerque, NM capable of detecting gamma rays at energies above 100 GeV. We
present the results of the STACEE observations of Draco during the 2005-2006
observing season totaling 10 hours of livetime after cuts.</description><subject>Physics - Astrophysics of Galaxies</subject><subject>Physics - Cosmology and Nongalactic Astrophysics</subject><subject>Physics - Earth and Planetary Astrophysics</subject><subject>Physics - High Energy Astrophysical Phenomena</subject><subject>Physics - Instrumentation and Methods for Astrophysics</subject><subject>Physics - Solar and Stellar Astrophysics</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2007</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNotj71uwjAURr10qCh7J-QXCLWxja_HKKSABGIge3RxrhULSCo3auHtW36mI33D0XcYe5diqsEY8YHpEn-mwv4PymjzymBPmHzLQ5_4AtORb3EYKPG862IbTzjEvuOx44uEvue_cWj5vsqLsnxjLwFP3zR-csSqz7IqVtlmt1wX-SbDuTEZKUdSI8kGbONohtIL0s6GoPWBnJLgnfZeAmCwB-dRgRXSktXQoBKgRmzy0N6f118pnjFd61tBfStQf2XnPzQ</recordid><startdate>20071018</startdate><enddate>20071018</enddate><creator>STACEE Collaboration</creator><creator>Driscoll, D. D</creator><creator>Ball, J</creator><creator>Carson, J. E</creator><creator>Covault, C. E</creator><creator>Fortin, P</creator><creator>Gingrich, D. M</creator><creator>Hanna, D. S</creator><creator>Jarvis, A</creator><creator>Kildea, J</creator><creator>Lindner, T</creator><creator>Mueller, C</creator><creator>Mukherjee, R</creator><creator>Ong, R. A</creator><creator>Ragan, K</creator><creator>Williams, D. A</creator><creator>Zweerink, J</creator><scope>GOX</scope></search><sort><creationdate>20071018</creationdate><title>Search for Dark Matter Annihilation in Draco with STACEE</title><author>STACEE Collaboration ; Driscoll, D. D ; Ball, J ; Carson, J. E ; Covault, C. E ; Fortin, P ; Gingrich, D. M ; Hanna, D. S ; Jarvis, A ; Kildea, J ; Lindner, T ; Mueller, C ; Mukherjee, R ; Ong, R. A ; Ragan, K ; Williams, D. A ; Zweerink, J</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a655-e39e14ae1d87d9e2a1c0e497ff44be9318c94cc188af7b9ca387017e748da3083</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2007</creationdate><topic>Physics - Astrophysics of Galaxies</topic><topic>Physics - Cosmology and Nongalactic Astrophysics</topic><topic>Physics - Earth and Planetary Astrophysics</topic><topic>Physics - High Energy Astrophysical Phenomena</topic><topic>Physics - Instrumentation and Methods for Astrophysics</topic><topic>Physics - Solar and Stellar Astrophysics</topic><toplevel>online_resources</toplevel><creatorcontrib>STACEE Collaboration</creatorcontrib><creatorcontrib>Driscoll, D. D</creatorcontrib><creatorcontrib>Ball, J</creatorcontrib><creatorcontrib>Carson, J. E</creatorcontrib><creatorcontrib>Covault, C. E</creatorcontrib><creatorcontrib>Fortin, P</creatorcontrib><creatorcontrib>Gingrich, D. M</creatorcontrib><creatorcontrib>Hanna, D. S</creatorcontrib><creatorcontrib>Jarvis, A</creatorcontrib><creatorcontrib>Kildea, J</creatorcontrib><creatorcontrib>Lindner, T</creatorcontrib><creatorcontrib>Mueller, C</creatorcontrib><creatorcontrib>Mukherjee, R</creatorcontrib><creatorcontrib>Ong, R. A</creatorcontrib><creatorcontrib>Ragan, K</creatorcontrib><creatorcontrib>Williams, D. A</creatorcontrib><creatorcontrib>Zweerink, J</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>STACEE Collaboration</au><au>Driscoll, D. D</au><au>Ball, J</au><au>Carson, J. E</au><au>Covault, C. E</au><au>Fortin, P</au><au>Gingrich, D. M</au><au>Hanna, D. S</au><au>Jarvis, A</au><au>Kildea, J</au><au>Lindner, T</au><au>Mueller, C</au><au>Mukherjee, R</au><au>Ong, R. A</au><au>Ragan, K</au><au>Williams, D. A</au><au>Zweerink, J</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Search for Dark Matter Annihilation in Draco with STACEE</atitle><date>2007-10-18</date><risdate>2007</risdate><abstract>For some time, the Draco dwarf spheroidal galaxy has garnered interest as a
possible source for the indirect detection of dark matter. Its large
mass-to-light ratio and relative proximity to the Earth provide favorable
conditions for the production of detectable gamma rays from dark matter
self-annihilation in its core. The Solar Tower Atmospheric Cherenkov Effect
Experiment (STACEE) is an air-shower Cherenkov telescope located in
Albuquerque, NM capable of detecting gamma rays at energies above 100 GeV. We
present the results of the STACEE observations of Draco during the 2005-2006
observing season totaling 10 hours of livetime after cuts.</abstract><doi>10.48550/arxiv.0710.3545</doi><oa>free_for_read</oa></addata></record> |
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| subjects | Physics - Astrophysics of Galaxies Physics - Cosmology and Nongalactic Astrophysics Physics - Earth and Planetary Astrophysics Physics - High Energy Astrophysical Phenomena Physics - Instrumentation and Methods for Astrophysics Physics - Solar and Stellar Astrophysics |
| title | Search for Dark Matter Annihilation in Draco with STACEE |
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