STACEE Observations of 1ES 1218+304
We present the analysis and results of recent high-energy gamma-ray observations of the high energy-peaked BL Lac (HBL) object 1ES 1218+304 with the Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE). 1ES 1218+304 is an X-ray bright HBL at a redshift z=0.182. It has been predicted to be a...
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| creator | STACEE Collaboration Mukherjee, R Akhter, N Ball, J Carson, J. E Covault, C. E Driscoll, D. D Fortin, P Gingrich, D. M Hanna, D. S Jarvis, A Kildea, J Lindner, T Mueller, C Ong, R. A Ragan, K Williams, D. A Zweerink, J |
| description | We present the analysis and results of recent high-energy gamma-ray
observations of the high energy-peaked BL Lac (HBL) object 1ES 1218+304 with
the Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE). 1ES 1218+304
is an X-ray bright HBL at a redshift z=0.182. It has been predicted to be a
gamma-ray emitter above 100 GeV, detectable by ground-based Cherenkov
telescopes. Recently this source has been detected by MAGIC and VERITAS,
confirming these predictions. STACEE's sensitivity to astrophysical sources at
energies above 100 GeV allows it to explore high energy sources such as X-ray
bright active galaxies and gamma-ray bursts. We present results from STACEE
observations of 1ES 1218+304 in the 2006 and 2007 observing seasons. |
| doi_str_mv | 10.48550/arxiv.0710.4170 |
| format | Article |
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observations of the high energy-peaked BL Lac (HBL) object 1ES 1218+304 with
the Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE). 1ES 1218+304
is an X-ray bright HBL at a redshift z=0.182. It has been predicted to be a
gamma-ray emitter above 100 GeV, detectable by ground-based Cherenkov
telescopes. Recently this source has been detected by MAGIC and VERITAS,
confirming these predictions. STACEE's sensitivity to astrophysical sources at
energies above 100 GeV allows it to explore high energy sources such as X-ray
bright active galaxies and gamma-ray bursts. We present results from STACEE
observations of 1ES 1218+304 in the 2006 and 2007 observing seasons.</description><identifier>DOI: 10.48550/arxiv.0710.4170</identifier><language>eng</language><subject>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</subject><creationdate>2007-10</creationdate><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,776,881</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/0710.4170$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.0710.4170$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>STACEE Collaboration</creatorcontrib><creatorcontrib>Mukherjee, R</creatorcontrib><creatorcontrib>Akhter, N</creatorcontrib><creatorcontrib>Ball, J</creatorcontrib><creatorcontrib>Carson, J. E</creatorcontrib><creatorcontrib>Covault, C. E</creatorcontrib><creatorcontrib>Driscoll, D. D</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>Ong, R. A</creatorcontrib><creatorcontrib>Ragan, K</creatorcontrib><creatorcontrib>Williams, D. A</creatorcontrib><creatorcontrib>Zweerink, J</creatorcontrib><title>STACEE Observations of 1ES 1218+304</title><description>We present the analysis and results of recent high-energy gamma-ray
observations of the high energy-peaked BL Lac (HBL) object 1ES 1218+304 with
the Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE). 1ES 1218+304
is an X-ray bright HBL at a redshift z=0.182. It has been predicted to be a
gamma-ray emitter above 100 GeV, detectable by ground-based Cherenkov
telescopes. Recently this source has been detected by MAGIC and VERITAS,
confirming these predictions. STACEE's sensitivity to astrophysical sources at
energies above 100 GeV allows it to explore high energy sources such as X-ray
bright active galaxies and gamma-ray bursts. We present results from STACEE
observations of 1ES 1218+304 in the 2006 and 2007 observing seasons.</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>eNotzjsLwjAUhuEsDqLuTlJwlNaTpCdJRyn1AoUOdi9JmwMFb7RS9N9L1emDd_h4GFtyiGKDCFvbvdohAj0GrmHK1udyl2ZZULjed4N9tvdbH9wp4Nk54IKbjYR4ziZkL71f_HfGyn1WpscwLw6ndJeHViGEPmk0xEjOoAJALchr4TgZElQnyngZg5MaXW0ISVlfN0kjyHohEKlWcsZWv9svsnp07dV272rEViNWfgBy1DY2</recordid><startdate>20071022</startdate><enddate>20071022</enddate><creator>STACEE Collaboration</creator><creator>Mukherjee, R</creator><creator>Akhter, N</creator><creator>Ball, J</creator><creator>Carson, J. E</creator><creator>Covault, C. E</creator><creator>Driscoll, D. D</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>Ong, R. A</creator><creator>Ragan, K</creator><creator>Williams, D. A</creator><creator>Zweerink, J</creator><scope>GOX</scope></search><sort><creationdate>20071022</creationdate><title>STACEE Observations of 1ES 1218+304</title><author>STACEE Collaboration ; Mukherjee, R ; Akhter, N ; Ball, J ; Carson, J. E ; Covault, C. E ; Driscoll, D. D ; Fortin, P ; Gingrich, D. M ; Hanna, D. S ; Jarvis, A ; Kildea, J ; Lindner, T ; Mueller, C ; Ong, R. A ; Ragan, K ; Williams, D. A ; Zweerink, J</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a650-e9d7045fb85600572fe72b1f8f2fc968e340b375bc8f5f6aecd9d2fae2255fc63</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>Mukherjee, R</creatorcontrib><creatorcontrib>Akhter, N</creatorcontrib><creatorcontrib>Ball, J</creatorcontrib><creatorcontrib>Carson, J. E</creatorcontrib><creatorcontrib>Covault, C. E</creatorcontrib><creatorcontrib>Driscoll, D. D</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>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>Mukherjee, R</au><au>Akhter, N</au><au>Ball, J</au><au>Carson, J. E</au><au>Covault, C. E</au><au>Driscoll, D. D</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>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>STACEE Observations of 1ES 1218+304</atitle><date>2007-10-22</date><risdate>2007</risdate><abstract>We present the analysis and results of recent high-energy gamma-ray
observations of the high energy-peaked BL Lac (HBL) object 1ES 1218+304 with
the Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE). 1ES 1218+304
is an X-ray bright HBL at a redshift z=0.182. It has been predicted to be a
gamma-ray emitter above 100 GeV, detectable by ground-based Cherenkov
telescopes. Recently this source has been detected by MAGIC and VERITAS,
confirming these predictions. STACEE's sensitivity to astrophysical sources at
energies above 100 GeV allows it to explore high energy sources such as X-ray
bright active galaxies and gamma-ray bursts. We present results from STACEE
observations of 1ES 1218+304 in the 2006 and 2007 observing seasons.</abstract><doi>10.48550/arxiv.0710.4170</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 | STACEE Observations of 1ES 1218+304 |
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