Status of the H.E.S.S. experiment and first results

Abstract The High Energy Stereoscopic System (H.E.S.S.) consists of four 12m diameter imaging Cherenkov telescopes, and is presently under construction in the Khomas Highland region of Namibia, 1.8 km above sea level ($ 23^{∘} $16′18′′ S, $ 16^{∘} $30′00′′ E). The H.E.S.S. telescopes provide very go...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Chadwick, P.M. [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2004

Schlagwörter:	Energy Threshold Angular Resolution Astronomical Observation Highland Region Background Rejection

Übergeordnetes Werk:	Enthalten in: The European physical journal - Berlin : Springer, 1998, 33(2004), Suppl 1 vom: 03. Feb., Seite s935-s937
Übergeordnetes Werk:	volume:33 ; year:2004 ; number:Suppl 1 ; day:03 ; month:02 ; pages:s935-s937

Links:	Volltext

DOI / URN:	10.1140/epjcd/s2004-03-1629-3

Katalog-ID:	SPR008302979

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allfields	10.1140/epjcd/s2004-03-1629-3 doi (DE-627)SPR008302979 (SPR)s2004-03-1629-3-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Chadwick, P.M. verfasserin aut Status of the H.E.S.S. experiment and first results 2004 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The High Energy Stereoscopic System (H.E.S.S.) consists of four 12m diameter imaging Cherenkov telescopes, and is presently under construction in the Khomas Highland region of Namibia, 1.8 km above sea level ($ 23^{∘} $16′18′′ S, $ 16^{∘} $30′00′′ E). The H.E.S.S. telescopes provide very good angular resolution and background rejection capability resulting in a sensitivity ~ 10 mCrab with an energy threshold of around 100 GeV. The first two telescopes are currently operating, and the array will be complete in early 2004. This paper provides a description of the H.E.S.S. telescopes and reports preliminary results obtained with the first telescope. PACS: 95.55.Ka X- and gamma ray telescopes and instrumentation – 95.55.Pw Astronomical observations: gamma ray Energy Threshold (dpeaa)DE-He213 Angular Resolution (dpeaa)DE-He213 Astronomical Observation (dpeaa)DE-He213 Highland Region (dpeaa)DE-He213 Background Rejection (dpeaa)DE-He213 Enthalten in The European physical journal Berlin : Springer, 1998 33(2004), Suppl 1 vom: 03. Feb., Seite s935-s937 (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:33 year:2004 number:Suppl 1 day:03 month:02 pages:s935-s937 https://dx.doi.org/10.1140/epjcd/s2004-03-1629-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_40 GBV_ILN_63 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_206 GBV_ILN_267 GBV_ILN_293 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4305 GBV_ILN_4307 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4338 33.50 ASE AR 33 2004 Suppl 1 03 02 s935-s937
spelling	10.1140/epjcd/s2004-03-1629-3 doi (DE-627)SPR008302979 (SPR)s2004-03-1629-3-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Chadwick, P.M. verfasserin aut Status of the H.E.S.S. experiment and first results 2004 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The High Energy Stereoscopic System (H.E.S.S.) consists of four 12m diameter imaging Cherenkov telescopes, and is presently under construction in the Khomas Highland region of Namibia, 1.8 km above sea level ($ 23^{∘} $16′18′′ S, $ 16^{∘} $30′00′′ E). The H.E.S.S. telescopes provide very good angular resolution and background rejection capability resulting in a sensitivity ~ 10 mCrab with an energy threshold of around 100 GeV. The first two telescopes are currently operating, and the array will be complete in early 2004. This paper provides a description of the H.E.S.S. telescopes and reports preliminary results obtained with the first telescope. PACS: 95.55.Ka X- and gamma ray telescopes and instrumentation – 95.55.Pw Astronomical observations: gamma ray Energy Threshold (dpeaa)DE-He213 Angular Resolution (dpeaa)DE-He213 Astronomical Observation (dpeaa)DE-He213 Highland Region (dpeaa)DE-He213 Background Rejection (dpeaa)DE-He213 Enthalten in The European physical journal Berlin : Springer, 1998 33(2004), Suppl 1 vom: 03. Feb., Seite s935-s937 (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:33 year:2004 number:Suppl 1 day:03 month:02 pages:s935-s937 https://dx.doi.org/10.1140/epjcd/s2004-03-1629-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_40 GBV_ILN_63 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_206 GBV_ILN_267 GBV_ILN_293 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4305 GBV_ILN_4307 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4338 33.50 ASE AR 33 2004 Suppl 1 03 02 s935-s937
allfields_unstemmed	10.1140/epjcd/s2004-03-1629-3 doi (DE-627)SPR008302979 (SPR)s2004-03-1629-3-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Chadwick, P.M. verfasserin aut Status of the H.E.S.S. experiment and first results 2004 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The High Energy Stereoscopic System (H.E.S.S.) consists of four 12m diameter imaging Cherenkov telescopes, and is presently under construction in the Khomas Highland region of Namibia, 1.8 km above sea level ($ 23^{∘} $16′18′′ S, $ 16^{∘} $30′00′′ E). The H.E.S.S. telescopes provide very good angular resolution and background rejection capability resulting in a sensitivity ~ 10 mCrab with an energy threshold of around 100 GeV. The first two telescopes are currently operating, and the array will be complete in early 2004. This paper provides a description of the H.E.S.S. telescopes and reports preliminary results obtained with the first telescope. PACS: 95.55.Ka X- and gamma ray telescopes and instrumentation – 95.55.Pw Astronomical observations: gamma ray Energy Threshold (dpeaa)DE-He213 Angular Resolution (dpeaa)DE-He213 Astronomical Observation (dpeaa)DE-He213 Highland Region (dpeaa)DE-He213 Background Rejection (dpeaa)DE-He213 Enthalten in The European physical journal Berlin : Springer, 1998 33(2004), Suppl 1 vom: 03. Feb., Seite s935-s937 (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:33 year:2004 number:Suppl 1 day:03 month:02 pages:s935-s937 https://dx.doi.org/10.1140/epjcd/s2004-03-1629-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_40 GBV_ILN_63 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_206 GBV_ILN_267 GBV_ILN_293 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4305 GBV_ILN_4307 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4338 33.50 ASE AR 33 2004 Suppl 1 03 02 s935-s937
allfieldsGer	10.1140/epjcd/s2004-03-1629-3 doi (DE-627)SPR008302979 (SPR)s2004-03-1629-3-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Chadwick, P.M. verfasserin aut Status of the H.E.S.S. experiment and first results 2004 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The High Energy Stereoscopic System (H.E.S.S.) consists of four 12m diameter imaging Cherenkov telescopes, and is presently under construction in the Khomas Highland region of Namibia, 1.8 km above sea level ($ 23^{∘} $16′18′′ S, $ 16^{∘} $30′00′′ E). The H.E.S.S. telescopes provide very good angular resolution and background rejection capability resulting in a sensitivity ~ 10 mCrab with an energy threshold of around 100 GeV. The first two telescopes are currently operating, and the array will be complete in early 2004. This paper provides a description of the H.E.S.S. telescopes and reports preliminary results obtained with the first telescope. PACS: 95.55.Ka X- and gamma ray telescopes and instrumentation – 95.55.Pw Astronomical observations: gamma ray Energy Threshold (dpeaa)DE-He213 Angular Resolution (dpeaa)DE-He213 Astronomical Observation (dpeaa)DE-He213 Highland Region (dpeaa)DE-He213 Background Rejection (dpeaa)DE-He213 Enthalten in The European physical journal Berlin : Springer, 1998 33(2004), Suppl 1 vom: 03. Feb., Seite s935-s937 (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:33 year:2004 number:Suppl 1 day:03 month:02 pages:s935-s937 https://dx.doi.org/10.1140/epjcd/s2004-03-1629-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_40 GBV_ILN_63 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_206 GBV_ILN_267 GBV_ILN_293 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4305 GBV_ILN_4307 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4338 33.50 ASE AR 33 2004 Suppl 1 03 02 s935-s937
allfieldsSound	10.1140/epjcd/s2004-03-1629-3 doi (DE-627)SPR008302979 (SPR)s2004-03-1629-3-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Chadwick, P.M. verfasserin aut Status of the H.E.S.S. experiment and first results 2004 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The High Energy Stereoscopic System (H.E.S.S.) consists of four 12m diameter imaging Cherenkov telescopes, and is presently under construction in the Khomas Highland region of Namibia, 1.8 km above sea level ($ 23^{∘} $16′18′′ S, $ 16^{∘} $30′00′′ E). The H.E.S.S. telescopes provide very good angular resolution and background rejection capability resulting in a sensitivity ~ 10 mCrab with an energy threshold of around 100 GeV. The first two telescopes are currently operating, and the array will be complete in early 2004. This paper provides a description of the H.E.S.S. telescopes and reports preliminary results obtained with the first telescope. PACS: 95.55.Ka X- and gamma ray telescopes and instrumentation – 95.55.Pw Astronomical observations: gamma ray Energy Threshold (dpeaa)DE-He213 Angular Resolution (dpeaa)DE-He213 Astronomical Observation (dpeaa)DE-He213 Highland Region (dpeaa)DE-He213 Background Rejection (dpeaa)DE-He213 Enthalten in The European physical journal Berlin : Springer, 1998 33(2004), Suppl 1 vom: 03. Feb., Seite s935-s937 (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:33 year:2004 number:Suppl 1 day:03 month:02 pages:s935-s937 https://dx.doi.org/10.1140/epjcd/s2004-03-1629-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_40 GBV_ILN_63 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_206 GBV_ILN_267 GBV_ILN_293 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4305 GBV_ILN_4307 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4338 33.50 ASE AR 33 2004 Suppl 1 03 02 s935-s937
language	English
source	Enthalten in The European physical journal 33(2004), Suppl 1 vom: 03. Feb., Seite s935-s937 volume:33 year:2004 number:Suppl 1 day:03 month:02 pages:s935-s937
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author	Chadwick, P.M.
spellingShingle	Chadwick, P.M. ddc 530 bkl 33.50 misc Energy Threshold misc Angular Resolution misc Astronomical Observation misc Highland Region misc Background Rejection Status of the H.E.S.S. experiment and first results
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topic_title	530 ASE 33.50 bkl Status of the H.E.S.S. experiment and first results Energy Threshold (dpeaa)DE-He213 Angular Resolution (dpeaa)DE-He213 Astronomical Observation (dpeaa)DE-He213 Highland Region (dpeaa)DE-He213 Background Rejection (dpeaa)DE-He213
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title	Status of the H.E.S.S. experiment and first results
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title_sort	status of the h.e.s.s. experiment and first results
title_auth	Status of the H.E.S.S. experiment and first results
abstract	Abstract The High Energy Stereoscopic System (H.E.S.S.) consists of four 12m diameter imaging Cherenkov telescopes, and is presently under construction in the Khomas Highland region of Namibia, 1.8 km above sea level ($ 23^{∘} $16′18′′ S, $ 16^{∘} $30′00′′ E). The H.E.S.S. telescopes provide very good angular resolution and background rejection capability resulting in a sensitivity ~ 10 mCrab with an energy threshold of around 100 GeV. The first two telescopes are currently operating, and the array will be complete in early 2004. This paper provides a description of the H.E.S.S. telescopes and reports preliminary results obtained with the first telescope. PACS: 95.55.Ka X- and gamma ray telescopes and instrumentation – 95.55.Pw Astronomical observations: gamma ray
abstractGer	Abstract The High Energy Stereoscopic System (H.E.S.S.) consists of four 12m diameter imaging Cherenkov telescopes, and is presently under construction in the Khomas Highland region of Namibia, 1.8 km above sea level ($ 23^{∘} $16′18′′ S, $ 16^{∘} $30′00′′ E). The H.E.S.S. telescopes provide very good angular resolution and background rejection capability resulting in a sensitivity ~ 10 mCrab with an energy threshold of around 100 GeV. The first two telescopes are currently operating, and the array will be complete in early 2004. This paper provides a description of the H.E.S.S. telescopes and reports preliminary results obtained with the first telescope. PACS: 95.55.Ka X- and gamma ray telescopes and instrumentation – 95.55.Pw Astronomical observations: gamma ray
abstract_unstemmed	Abstract The High Energy Stereoscopic System (H.E.S.S.) consists of four 12m diameter imaging Cherenkov telescopes, and is presently under construction in the Khomas Highland region of Namibia, 1.8 km above sea level ($ 23^{∘} $16′18′′ S, $ 16^{∘} $30′00′′ E). The H.E.S.S. telescopes provide very good angular resolution and background rejection capability resulting in a sensitivity ~ 10 mCrab with an energy threshold of around 100 GeV. The first two telescopes are currently operating, and the array will be complete in early 2004. This paper provides a description of the H.E.S.S. telescopes and reports preliminary results obtained with the first telescope. PACS: 95.55.Ka X- and gamma ray telescopes and instrumentation – 95.55.Pw Astronomical observations: gamma ray
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title_short	Status of the H.E.S.S. experiment and first results
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The H.E.S.S. telescopes provide very good angular resolution and background rejection capability resulting in a sensitivity ~ 10 mCrab with an energy threshold of around 100 GeV. The first two telescopes are currently operating, and the array will be complete in early 2004. This paper provides a description of the H.E.S.S. telescopes and reports preliminary results obtained with the first telescope. 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