Whipple telescope observations of LS I +61 303: 2004–2006
Abstract In this paper we present the results of the past two years observations on the galactic microquasar LS I +61 303 with the Whipple 10 m gamma-ray telescope. The recent MAGIC detection of the source between 200 GeV and 4 TeV suggests that the source is periodic with very high energy (VHE) gam...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Smith, A. [verfasserIn] Atkins, R. W. [verfasserIn] Bradbury, S. [verfasserIn] Celik, O. [verfasserIn] Chow, Y. C. K. [verfasserIn] Cogan, P. [verfasserIn] Dowdall, C. [verfasserIn] Fegan, S. J. [verfasserIn] Fortin, P. [verfasserIn] Gall, D. [verfasserIn] Gillanders, G. H. [verfasserIn] Grube, J. [verfasserIn] Gutierrez, K. J. [verfasserIn] Hall, T. A. [verfasserIn] Hanna, D. [verfasserIn] Holder, J. [verfasserIn] Horan, D. [verfasserIn] Hughes, S. B. [verfasserIn] Humensky, T. B. [verfasserIn] Jung, I. [verfasserIn] Kaaret, P. [verfasserIn] Kenny, G. [verfasserIn] Kertzman, M. [verfasserIn] Kieda, D. B. [verfasserIn] Konopelko, A. [verfasserIn] Krawczynski, H. [verfasserIn] Krennrich, F. [verfasserIn] Lang, M. J. [verfasserIn] Le Bohec, S. [verfasserIn] Maier, G. [verfasserIn] Millis, J. [verfasserIn] Moriarty, P. [verfasserIn] Ong, R. A. [verfasserIn] Perkins, J. S. [verfasserIn] Ragan, K. [verfasserIn] Sembroski, G. H. [verfasserIn] Toner, J. A. [verfasserIn] Valcarcel, L. [verfasserIn] Vassiliev, V. V. [verfasserIn] Wagner, R. G. [verfasserIn] Wakely, S. P. [verfasserIn] Weekes, T. C. [verfasserIn] White, R. J. [verfasserIn] Williams, D. A. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2007 |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Dordrecht [u.a.] : Springer Science + Business Media B.V, 1968, 309(2007), 1-4 vom: 24. Apr., Seite 299-303 |
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| Übergeordnetes Werk: |
volume:309 ; year:2007 ; number:1-4 ; day:24 ; month:04 ; pages:299-303 |
| Links: |
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| DOI / URN: |
10.1007/s10509-007-9473-0 |
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| Katalog-ID: |
SPR010573216 |
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| 100 | 1 | |a Smith, A. |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Whipple telescope observations of LS I +61 303: 2004–2006 |
| 264 | 1 | |c 2007 | |
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| 337 | |a Computermedien |b c |2 rdamedia | ||
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| 520 | |a Abstract In this paper we present the results of the past two years observations on the galactic microquasar LS I +61 303 with the Whipple 10 m gamma-ray telescope. The recent MAGIC detection of the source between 200 GeV and 4 TeV suggests that the source is periodic with very high energy (VHE) gamma-ray emission linked to its orbital cycle. The entire 50-hour data set obtained with Whipple from 2004 to 2006 was analyzed with no reliable detection resulting. The upper limits obtained in the 2005–2006 season covered several of the same epochs as the MAGIC Telescope detections, albeit with lower sensitivity. Upper limits are placed on emission during the orbital phases of 0→0.1 and 0.8→1, phases which are not included in the MAGIC data set. | ||
| 650 | 4 | |a X-ray binary stars |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Gamma-ray sources |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Cherenkov detectors |7 (dpeaa)DE-He213 | |
| 700 | 1 | |a Atkins, R. W. |e verfasserin |4 aut | |
| 700 | 1 | |a Bradbury, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Celik, O. |e verfasserin |4 aut | |
| 700 | 1 | |a Chow, Y. C. K. |e verfasserin |4 aut | |
| 700 | 1 | |a Cogan, P. |e verfasserin |4 aut | |
| 700 | 1 | |a Dowdall, C. |e verfasserin |4 aut | |
| 700 | 1 | |a Fegan, S. J. |e verfasserin |4 aut | |
| 700 | 1 | |a Fortin, P. |e verfasserin |4 aut | |
| 700 | 1 | |a Gall, D. |e verfasserin |4 aut | |
| 700 | 1 | |a Gillanders, G. H. |e verfasserin |4 aut | |
| 700 | 1 | |a Grube, J. |e verfasserin |4 aut | |
| 700 | 1 | |a Gutierrez, K. J. |e verfasserin |4 aut | |
| 700 | 1 | |a Hall, T. A. |e verfasserin |4 aut | |
| 700 | 1 | |a Hanna, D. |e verfasserin |4 aut | |
| 700 | 1 | |a Holder, J. |e verfasserin |4 aut | |
| 700 | 1 | |a Horan, D. |e verfasserin |4 aut | |
| 700 | 1 | |a Hughes, S. B. |e verfasserin |4 aut | |
| 700 | 1 | |a Humensky, T. B. |e verfasserin |4 aut | |
| 700 | 1 | |a Jung, I. |e verfasserin |4 aut | |
| 700 | 1 | |a Kaaret, P. |e verfasserin |4 aut | |
| 700 | 1 | |a Kenny, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Kertzman, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Kieda, D. B. |e verfasserin |4 aut | |
| 700 | 1 | |a Konopelko, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Krawczynski, H. |e verfasserin |4 aut | |
| 700 | 1 | |a Krennrich, F. |e verfasserin |4 aut | |
| 700 | 1 | |a Lang, M. J. |e verfasserin |4 aut | |
| 700 | 1 | |a Le Bohec, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Maier, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Millis, J. |e verfasserin |4 aut | |
| 700 | 1 | |a Moriarty, P. |e verfasserin |4 aut | |
| 700 | 1 | |a Ong, R. A. |e verfasserin |4 aut | |
| 700 | 1 | |a Perkins, J. S. |e verfasserin |4 aut | |
| 700 | 1 | |a Ragan, K. |e verfasserin |4 aut | |
| 700 | 1 | |a Sembroski, G. H. |e verfasserin |4 aut | |
| 700 | 1 | |a Toner, J. A. |e verfasserin |4 aut | |
| 700 | 1 | |a Valcarcel, L. |e verfasserin |4 aut | |
| 700 | 1 | |a Vassiliev, V. V. |e verfasserin |4 aut | |
| 700 | 1 | |a Wagner, R. G. |e verfasserin |4 aut | |
| 700 | 1 | |a Wakely, S. P. |e verfasserin |4 aut | |
| 700 | 1 | |a Weekes, T. C. |e verfasserin |4 aut | |
| 700 | 1 | |a White, R. J. |e verfasserin |4 aut | |
| 700 | 1 | |a Williams, D. A. |e verfasserin |4 aut | |
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10.1007/s10509-007-9473-0 doi (DE-627)SPR010573216 (SPR)s10509-007-9473-0-e DE-627 ger DE-627 rakwb eng 520 530 620 ASE 39.00 bkl 39.22 bkl Smith, A. verfasserin aut Whipple telescope observations of LS I +61 303: 2004–2006 2007 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract In this paper we present the results of the past two years observations on the galactic microquasar LS I +61 303 with the Whipple 10 m gamma-ray telescope. The recent MAGIC detection of the source between 200 GeV and 4 TeV suggests that the source is periodic with very high energy (VHE) gamma-ray emission linked to its orbital cycle. The entire 50-hour data set obtained with Whipple from 2004 to 2006 was analyzed with no reliable detection resulting. The upper limits obtained in the 2005–2006 season covered several of the same epochs as the MAGIC Telescope detections, albeit with lower sensitivity. Upper limits are placed on emission during the orbital phases of 0→0.1 and 0.8→1, phases which are not included in the MAGIC data set. X-ray binary stars (dpeaa)DE-He213 Gamma-ray sources (dpeaa)DE-He213 Cherenkov detectors (dpeaa)DE-He213 Atkins, R. W. verfasserin aut Bradbury, S. verfasserin aut Celik, O. verfasserin aut Chow, Y. C. K. verfasserin aut Cogan, P. verfasserin aut Dowdall, C. verfasserin aut Fegan, S. J. verfasserin aut Fortin, P. verfasserin aut Gall, D. verfasserin aut Gillanders, G. H. verfasserin aut Grube, J. verfasserin aut Gutierrez, K. J. verfasserin aut Hall, T. A. verfasserin aut Hanna, D. verfasserin aut Holder, J. verfasserin aut Horan, D. verfasserin aut Hughes, S. B. verfasserin aut Humensky, T. B. verfasserin aut Jung, I. verfasserin aut Kaaret, P. verfasserin aut Kenny, G. verfasserin aut Kertzman, M. verfasserin aut Kieda, D. B. verfasserin aut Konopelko, A. verfasserin aut Krawczynski, H. verfasserin aut Krennrich, F. verfasserin aut Lang, M. J. verfasserin aut Le Bohec, S. verfasserin aut Maier, G. verfasserin aut Millis, J. verfasserin aut Moriarty, P. verfasserin aut Ong, R. A. verfasserin aut Perkins, J. S. verfasserin aut Ragan, K. verfasserin aut Sembroski, G. H. verfasserin aut Toner, J. A. verfasserin aut Valcarcel, L. verfasserin aut Vassiliev, V. V. verfasserin aut Wagner, R. G. verfasserin aut Wakely, S. P. verfasserin aut Weekes, T. C. verfasserin aut White, R. J. verfasserin aut Williams, D. A. verfasserin aut Enthalten in Astrophysics and space science Dordrecht [u.a.] : Springer Science + Business Media B.V, 1968 309(2007), 1-4 vom: 24. Apr., Seite 299-303 (DE-627)268755868 (DE-600)1472548-4 1572-946X nnns volume:309 year:2007 number:1-4 day:24 month:04 pages:299-303 https://dx.doi.org/10.1007/s10509-007-9473-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 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_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 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_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE 39.22 ASE AR 309 2007 1-4 24 04 299-303 |
| spelling |
10.1007/s10509-007-9473-0 doi (DE-627)SPR010573216 (SPR)s10509-007-9473-0-e DE-627 ger DE-627 rakwb eng 520 530 620 ASE 39.00 bkl 39.22 bkl Smith, A. verfasserin aut Whipple telescope observations of LS I +61 303: 2004–2006 2007 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract In this paper we present the results of the past two years observations on the galactic microquasar LS I +61 303 with the Whipple 10 m gamma-ray telescope. The recent MAGIC detection of the source between 200 GeV and 4 TeV suggests that the source is periodic with very high energy (VHE) gamma-ray emission linked to its orbital cycle. The entire 50-hour data set obtained with Whipple from 2004 to 2006 was analyzed with no reliable detection resulting. The upper limits obtained in the 2005–2006 season covered several of the same epochs as the MAGIC Telescope detections, albeit with lower sensitivity. Upper limits are placed on emission during the orbital phases of 0→0.1 and 0.8→1, phases which are not included in the MAGIC data set. X-ray binary stars (dpeaa)DE-He213 Gamma-ray sources (dpeaa)DE-He213 Cherenkov detectors (dpeaa)DE-He213 Atkins, R. W. verfasserin aut Bradbury, S. verfasserin aut Celik, O. verfasserin aut Chow, Y. C. K. verfasserin aut Cogan, P. verfasserin aut Dowdall, C. verfasserin aut Fegan, S. J. verfasserin aut Fortin, P. verfasserin aut Gall, D. verfasserin aut Gillanders, G. H. verfasserin aut Grube, J. verfasserin aut Gutierrez, K. J. verfasserin aut Hall, T. A. verfasserin aut Hanna, D. verfasserin aut Holder, J. verfasserin aut Horan, D. verfasserin aut Hughes, S. B. verfasserin aut Humensky, T. B. verfasserin aut Jung, I. verfasserin aut Kaaret, P. verfasserin aut Kenny, G. verfasserin aut Kertzman, M. verfasserin aut Kieda, D. B. verfasserin aut Konopelko, A. verfasserin aut Krawczynski, H. verfasserin aut Krennrich, F. verfasserin aut Lang, M. J. verfasserin aut Le Bohec, S. verfasserin aut Maier, G. verfasserin aut Millis, J. verfasserin aut Moriarty, P. verfasserin aut Ong, R. A. verfasserin aut Perkins, J. S. verfasserin aut Ragan, K. verfasserin aut Sembroski, G. H. verfasserin aut Toner, J. A. verfasserin aut Valcarcel, L. verfasserin aut Vassiliev, V. V. verfasserin aut Wagner, R. G. verfasserin aut Wakely, S. P. verfasserin aut Weekes, T. C. verfasserin aut White, R. J. verfasserin aut Williams, D. A. verfasserin aut Enthalten in Astrophysics and space science Dordrecht [u.a.] : Springer Science + Business Media B.V, 1968 309(2007), 1-4 vom: 24. Apr., Seite 299-303 (DE-627)268755868 (DE-600)1472548-4 1572-946X nnns volume:309 year:2007 number:1-4 day:24 month:04 pages:299-303 https://dx.doi.org/10.1007/s10509-007-9473-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 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_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 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_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE 39.22 ASE AR 309 2007 1-4 24 04 299-303 |
| allfields_unstemmed |
10.1007/s10509-007-9473-0 doi (DE-627)SPR010573216 (SPR)s10509-007-9473-0-e DE-627 ger DE-627 rakwb eng 520 530 620 ASE 39.00 bkl 39.22 bkl Smith, A. verfasserin aut Whipple telescope observations of LS I +61 303: 2004–2006 2007 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract In this paper we present the results of the past two years observations on the galactic microquasar LS I +61 303 with the Whipple 10 m gamma-ray telescope. The recent MAGIC detection of the source between 200 GeV and 4 TeV suggests that the source is periodic with very high energy (VHE) gamma-ray emission linked to its orbital cycle. The entire 50-hour data set obtained with Whipple from 2004 to 2006 was analyzed with no reliable detection resulting. The upper limits obtained in the 2005–2006 season covered several of the same epochs as the MAGIC Telescope detections, albeit with lower sensitivity. Upper limits are placed on emission during the orbital phases of 0→0.1 and 0.8→1, phases which are not included in the MAGIC data set. X-ray binary stars (dpeaa)DE-He213 Gamma-ray sources (dpeaa)DE-He213 Cherenkov detectors (dpeaa)DE-He213 Atkins, R. W. verfasserin aut Bradbury, S. verfasserin aut Celik, O. verfasserin aut Chow, Y. C. K. verfasserin aut Cogan, P. verfasserin aut Dowdall, C. verfasserin aut Fegan, S. J. verfasserin aut Fortin, P. verfasserin aut Gall, D. verfasserin aut Gillanders, G. H. verfasserin aut Grube, J. verfasserin aut Gutierrez, K. J. verfasserin aut Hall, T. A. verfasserin aut Hanna, D. verfasserin aut Holder, J. verfasserin aut Horan, D. verfasserin aut Hughes, S. B. verfasserin aut Humensky, T. B. verfasserin aut Jung, I. verfasserin aut Kaaret, P. verfasserin aut Kenny, G. verfasserin aut Kertzman, M. verfasserin aut Kieda, D. B. verfasserin aut Konopelko, A. verfasserin aut Krawczynski, H. verfasserin aut Krennrich, F. verfasserin aut Lang, M. J. verfasserin aut Le Bohec, S. verfasserin aut Maier, G. verfasserin aut Millis, J. verfasserin aut Moriarty, P. verfasserin aut Ong, R. A. verfasserin aut Perkins, J. S. verfasserin aut Ragan, K. verfasserin aut Sembroski, G. H. verfasserin aut Toner, J. A. verfasserin aut Valcarcel, L. verfasserin aut Vassiliev, V. V. verfasserin aut Wagner, R. G. verfasserin aut Wakely, S. P. verfasserin aut Weekes, T. C. verfasserin aut White, R. J. verfasserin aut Williams, D. A. verfasserin aut Enthalten in Astrophysics and space science Dordrecht [u.a.] : Springer Science + Business Media B.V, 1968 309(2007), 1-4 vom: 24. Apr., Seite 299-303 (DE-627)268755868 (DE-600)1472548-4 1572-946X nnns volume:309 year:2007 number:1-4 day:24 month:04 pages:299-303 https://dx.doi.org/10.1007/s10509-007-9473-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 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_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 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_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE 39.22 ASE AR 309 2007 1-4 24 04 299-303 |
| allfieldsGer |
10.1007/s10509-007-9473-0 doi (DE-627)SPR010573216 (SPR)s10509-007-9473-0-e DE-627 ger DE-627 rakwb eng 520 530 620 ASE 39.00 bkl 39.22 bkl Smith, A. verfasserin aut Whipple telescope observations of LS I +61 303: 2004–2006 2007 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract In this paper we present the results of the past two years observations on the galactic microquasar LS I +61 303 with the Whipple 10 m gamma-ray telescope. The recent MAGIC detection of the source between 200 GeV and 4 TeV suggests that the source is periodic with very high energy (VHE) gamma-ray emission linked to its orbital cycle. The entire 50-hour data set obtained with Whipple from 2004 to 2006 was analyzed with no reliable detection resulting. The upper limits obtained in the 2005–2006 season covered several of the same epochs as the MAGIC Telescope detections, albeit with lower sensitivity. Upper limits are placed on emission during the orbital phases of 0→0.1 and 0.8→1, phases which are not included in the MAGIC data set. X-ray binary stars (dpeaa)DE-He213 Gamma-ray sources (dpeaa)DE-He213 Cherenkov detectors (dpeaa)DE-He213 Atkins, R. W. verfasserin aut Bradbury, S. verfasserin aut Celik, O. verfasserin aut Chow, Y. C. K. verfasserin aut Cogan, P. verfasserin aut Dowdall, C. verfasserin aut Fegan, S. J. verfasserin aut Fortin, P. verfasserin aut Gall, D. verfasserin aut Gillanders, G. H. verfasserin aut Grube, J. verfasserin aut Gutierrez, K. J. verfasserin aut Hall, T. A. verfasserin aut Hanna, D. verfasserin aut Holder, J. verfasserin aut Horan, D. verfasserin aut Hughes, S. B. verfasserin aut Humensky, T. B. verfasserin aut Jung, I. verfasserin aut Kaaret, P. verfasserin aut Kenny, G. verfasserin aut Kertzman, M. verfasserin aut Kieda, D. B. verfasserin aut Konopelko, A. verfasserin aut Krawczynski, H. verfasserin aut Krennrich, F. verfasserin aut Lang, M. J. verfasserin aut Le Bohec, S. verfasserin aut Maier, G. verfasserin aut Millis, J. verfasserin aut Moriarty, P. verfasserin aut Ong, R. A. verfasserin aut Perkins, J. S. verfasserin aut Ragan, K. verfasserin aut Sembroski, G. H. verfasserin aut Toner, J. A. verfasserin aut Valcarcel, L. verfasserin aut Vassiliev, V. V. verfasserin aut Wagner, R. G. verfasserin aut Wakely, S. P. verfasserin aut Weekes, T. C. verfasserin aut White, R. J. verfasserin aut Williams, D. A. verfasserin aut Enthalten in Astrophysics and space science Dordrecht [u.a.] : Springer Science + Business Media B.V, 1968 309(2007), 1-4 vom: 24. Apr., Seite 299-303 (DE-627)268755868 (DE-600)1472548-4 1572-946X nnns volume:309 year:2007 number:1-4 day:24 month:04 pages:299-303 https://dx.doi.org/10.1007/s10509-007-9473-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 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_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 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_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE 39.22 ASE AR 309 2007 1-4 24 04 299-303 |
| allfieldsSound |
10.1007/s10509-007-9473-0 doi (DE-627)SPR010573216 (SPR)s10509-007-9473-0-e DE-627 ger DE-627 rakwb eng 520 530 620 ASE 39.00 bkl 39.22 bkl Smith, A. verfasserin aut Whipple telescope observations of LS I +61 303: 2004–2006 2007 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract In this paper we present the results of the past two years observations on the galactic microquasar LS I +61 303 with the Whipple 10 m gamma-ray telescope. The recent MAGIC detection of the source between 200 GeV and 4 TeV suggests that the source is periodic with very high energy (VHE) gamma-ray emission linked to its orbital cycle. The entire 50-hour data set obtained with Whipple from 2004 to 2006 was analyzed with no reliable detection resulting. The upper limits obtained in the 2005–2006 season covered several of the same epochs as the MAGIC Telescope detections, albeit with lower sensitivity. Upper limits are placed on emission during the orbital phases of 0→0.1 and 0.8→1, phases which are not included in the MAGIC data set. X-ray binary stars (dpeaa)DE-He213 Gamma-ray sources (dpeaa)DE-He213 Cherenkov detectors (dpeaa)DE-He213 Atkins, R. W. verfasserin aut Bradbury, S. verfasserin aut Celik, O. verfasserin aut Chow, Y. C. K. verfasserin aut Cogan, P. verfasserin aut Dowdall, C. verfasserin aut Fegan, S. J. verfasserin aut Fortin, P. verfasserin aut Gall, D. verfasserin aut Gillanders, G. H. verfasserin aut Grube, J. verfasserin aut Gutierrez, K. J. verfasserin aut Hall, T. A. verfasserin aut Hanna, D. verfasserin aut Holder, J. verfasserin aut Horan, D. verfasserin aut Hughes, S. B. verfasserin aut Humensky, T. B. verfasserin aut Jung, I. verfasserin aut Kaaret, P. verfasserin aut Kenny, G. verfasserin aut Kertzman, M. verfasserin aut Kieda, D. B. verfasserin aut Konopelko, A. verfasserin aut Krawczynski, H. verfasserin aut Krennrich, F. verfasserin aut Lang, M. J. verfasserin aut Le Bohec, S. verfasserin aut Maier, G. verfasserin aut Millis, J. verfasserin aut Moriarty, P. verfasserin aut Ong, R. A. verfasserin aut Perkins, J. S. verfasserin aut Ragan, K. verfasserin aut Sembroski, G. H. verfasserin aut Toner, J. A. verfasserin aut Valcarcel, L. verfasserin aut Vassiliev, V. V. verfasserin aut Wagner, R. G. verfasserin aut Wakely, S. P. verfasserin aut Weekes, T. C. verfasserin aut White, R. J. verfasserin aut Williams, D. A. verfasserin aut Enthalten in Astrophysics and space science Dordrecht [u.a.] : Springer Science + Business Media B.V, 1968 309(2007), 1-4 vom: 24. Apr., Seite 299-303 (DE-627)268755868 (DE-600)1472548-4 1572-946X nnns volume:309 year:2007 number:1-4 day:24 month:04 pages:299-303 https://dx.doi.org/10.1007/s10509-007-9473-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 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_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 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_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE 39.22 ASE AR 309 2007 1-4 24 04 299-303 |
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Enthalten in Astrophysics and space science 309(2007), 1-4 vom: 24. Apr., Seite 299-303 volume:309 year:2007 number:1-4 day:24 month:04 pages:299-303 |
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Smith, A. @@aut@@ Atkins, R. W. @@aut@@ Bradbury, S. @@aut@@ Celik, O. @@aut@@ Chow, Y. C. K. @@aut@@ Cogan, P. @@aut@@ Dowdall, C. @@aut@@ Fegan, S. J. @@aut@@ Fortin, P. @@aut@@ Gall, D. @@aut@@ Gillanders, G. H. @@aut@@ Grube, J. @@aut@@ Gutierrez, K. J. @@aut@@ Hall, T. A. @@aut@@ Hanna, D. @@aut@@ Holder, J. @@aut@@ Horan, D. @@aut@@ Hughes, S. B. @@aut@@ Humensky, T. B. @@aut@@ Jung, I. @@aut@@ Kaaret, P. @@aut@@ Kenny, G. @@aut@@ Kertzman, M. @@aut@@ Kieda, D. B. @@aut@@ Konopelko, A. @@aut@@ Krawczynski, H. @@aut@@ Krennrich, F. @@aut@@ Lang, M. J. @@aut@@ Le Bohec, S. @@aut@@ Maier, G. @@aut@@ Millis, J. @@aut@@ Moriarty, P. @@aut@@ Ong, R. A. @@aut@@ Perkins, J. S. @@aut@@ Ragan, K. @@aut@@ Sembroski, G. H. @@aut@@ Toner, J. A. @@aut@@ Valcarcel, L. @@aut@@ Vassiliev, V. V. @@aut@@ Wagner, R. G. @@aut@@ Wakely, S. P. @@aut@@ Weekes, T. C. @@aut@@ White, R. J. @@aut@@ Williams, D. A. @@aut@@ |
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2007-04-24T00:00:00Z |
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|
| author |
Smith, A. |
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Smith, A. ddc 520 bkl 39.00 bkl 39.22 misc X-ray binary stars misc Gamma-ray sources misc Cherenkov detectors Whipple telescope observations of LS I +61 303: 2004–2006 |
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Smith, A. |
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520 - Astronomy & allied sciences 530 - Physics 620 - Engineering & allied operations |
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1572-946X |
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520 530 620 ASE 39.00 bkl 39.22 bkl Whipple telescope observations of LS I +61 303: 2004–2006 X-ray binary stars (dpeaa)DE-He213 Gamma-ray sources (dpeaa)DE-He213 Cherenkov detectors (dpeaa)DE-He213 |
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ddc 520 bkl 39.00 bkl 39.22 misc X-ray binary stars misc Gamma-ray sources misc Cherenkov detectors |
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ddc 520 bkl 39.00 bkl 39.22 misc X-ray binary stars misc Gamma-ray sources misc Cherenkov detectors |
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ddc 520 bkl 39.00 bkl 39.22 misc X-ray binary stars misc Gamma-ray sources misc Cherenkov detectors |
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Elektronische Aufsätze Aufsätze Elektronische Ressource |
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Astrophysics and space science |
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Whipple telescope observations of LS I +61 303: 2004–2006 |
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Whipple telescope observations of LS I +61 303: 2004–2006 |
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Smith, A. |
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Astrophysics and space science |
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Astrophysics and space science |
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eng |
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Smith, A. Atkins, R. W. Bradbury, S. Celik, O. Chow, Y. C. K. Cogan, P. Dowdall, C. Fegan, S. J. Fortin, P. Gall, D. Gillanders, G. H. Grube, J. Gutierrez, K. J. Hall, T. A. Hanna, D. Holder, J. Horan, D. Hughes, S. B. Humensky, T. B. Jung, I. Kaaret, P. Kenny, G. Kertzman, M. Kieda, D. B. Konopelko, A. Krawczynski, H. Krennrich, F. Lang, M. J. Le Bohec, S. Maier, G. Millis, J. Moriarty, P. Ong, R. A. Perkins, J. S. Ragan, K. Sembroski, G. H. Toner, J. A. Valcarcel, L. Vassiliev, V. V. Wagner, R. G. Wakely, S. P. Weekes, T. C. White, R. J. Williams, D. A. |
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309 |
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520 530 620 ASE 39.00 bkl 39.22 bkl |
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Elektronische Aufsätze |
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Smith, A. |
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10.1007/s10509-007-9473-0 |
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520 530 620 |
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verfasserin |
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whipple telescope observations of ls i +61 303: 2004–2006 |
| title_auth |
Whipple telescope observations of LS I +61 303: 2004–2006 |
| abstract |
Abstract In this paper we present the results of the past two years observations on the galactic microquasar LS I +61 303 with the Whipple 10 m gamma-ray telescope. The recent MAGIC detection of the source between 200 GeV and 4 TeV suggests that the source is periodic with very high energy (VHE) gamma-ray emission linked to its orbital cycle. The entire 50-hour data set obtained with Whipple from 2004 to 2006 was analyzed with no reliable detection resulting. The upper limits obtained in the 2005–2006 season covered several of the same epochs as the MAGIC Telescope detections, albeit with lower sensitivity. Upper limits are placed on emission during the orbital phases of 0→0.1 and 0.8→1, phases which are not included in the MAGIC data set. |
| abstractGer |
Abstract In this paper we present the results of the past two years observations on the galactic microquasar LS I +61 303 with the Whipple 10 m gamma-ray telescope. The recent MAGIC detection of the source between 200 GeV and 4 TeV suggests that the source is periodic with very high energy (VHE) gamma-ray emission linked to its orbital cycle. The entire 50-hour data set obtained with Whipple from 2004 to 2006 was analyzed with no reliable detection resulting. The upper limits obtained in the 2005–2006 season covered several of the same epochs as the MAGIC Telescope detections, albeit with lower sensitivity. Upper limits are placed on emission during the orbital phases of 0→0.1 and 0.8→1, phases which are not included in the MAGIC data set. |
| abstract_unstemmed |
Abstract In this paper we present the results of the past two years observations on the galactic microquasar LS I +61 303 with the Whipple 10 m gamma-ray telescope. The recent MAGIC detection of the source between 200 GeV and 4 TeV suggests that the source is periodic with very high energy (VHE) gamma-ray emission linked to its orbital cycle. The entire 50-hour data set obtained with Whipple from 2004 to 2006 was analyzed with no reliable detection resulting. The upper limits obtained in the 2005–2006 season covered several of the same epochs as the MAGIC Telescope detections, albeit with lower sensitivity. Upper limits are placed on emission during the orbital phases of 0→0.1 and 0.8→1, phases which are not included in the MAGIC data set. |
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| container_issue |
1-4 |
| title_short |
Whipple telescope observations of LS I +61 303: 2004–2006 |
| url |
https://dx.doi.org/10.1007/s10509-007-9473-0 |
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true |
| author2 |
Atkins, R. W. Bradbury, S. Celik, O. Chow, Y. C. K. Cogan, P. Dowdall, C. Fegan, S. J. Fortin, P. Gall, D. Gillanders, G. H. Grube, J. Gutierrez, K. J. Hall, T. A. Hanna, D. Holder, J. Horan, D. Hughes, S. B. Humensky, T. B. Jung, I. Kaaret, P. Kenny, G. Kertzman, M. Kieda, D. B. Konopelko, A. Krawczynski, H. Krennrich, F. Lang, M. J. Le Bohec, S. Maier, G. Millis, J. Moriarty, P. Ong, R. A. Perkins, J. S. Ragan, K. Sembroski, G. H. Toner, J. A. Valcarcel, L. Vassiliev, V. V. Wagner, R. G. Wakely, S. P. Weekes, T. C. White, R. J. Williams, D. A. |
| author2Str |
Atkins, R. W. Bradbury, S. Celik, O. Chow, Y. C. K. Cogan, P. Dowdall, C. Fegan, S. J. Fortin, P. Gall, D. Gillanders, G. H. Grube, J. Gutierrez, K. J. Hall, T. A. Hanna, D. Holder, J. Horan, D. Hughes, S. B. Humensky, T. B. Jung, I. Kaaret, P. Kenny, G. Kertzman, M. Kieda, D. B. Konopelko, A. Krawczynski, H. Krennrich, F. Lang, M. J. Le Bohec, S. Maier, G. Millis, J. Moriarty, P. Ong, R. A. Perkins, J. S. Ragan, K. Sembroski, G. H. Toner, J. A. Valcarcel, L. Vassiliev, V. V. Wagner, R. G. Wakely, S. P. Weekes, T. C. White, R. J. Williams, D. A. |
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| doi_str |
10.1007/s10509-007-9473-0 |
| up_date |
2024-07-03T16:59:12.696Z |
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| score |
7.3982067 |