The major upgrade of the MAGIC telescopes, Part I: The hardware improvements and the commissioning of the system
The MAGIC telescopes are two Imaging Atmospheric Cherenkov Telescopes (IACTs) located on the Canary island of La Palma. The telescopes are designed to measure Cherenkov light from air showers initiated by gamma rays in the energy regime from around 50GeV to more than 50TeV. The two telescopes were b...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Aleksić, J. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2016transfer abstract |
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| Schlagwörter: |
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| Umfang: |
15 |
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| Übergeordnetes Werk: |
Enthalten in: Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells - 2012transfer abstract, Amsterdam [u.a.] |
|---|---|
| Übergeordnetes Werk: |
volume:72 ; year:2016 ; day:1 ; month:01 ; pages:61-75 ; extent:15 |
| Links: |
|---|
| DOI / URN: |
10.1016/j.astropartphys.2015.04.004 |
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| Katalog-ID: |
ELV035447966 |
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| 245 | 1 | 4 | |a The major upgrade of the MAGIC telescopes, Part I: The hardware improvements and the commissioning of the system |
| 264 | 1 | |c 2016transfer abstract | |
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| 520 | |a The MAGIC telescopes are two Imaging Atmospheric Cherenkov Telescopes (IACTs) located on the Canary island of La Palma. The telescopes are designed to measure Cherenkov light from air showers initiated by gamma rays in the energy regime from around 50GeV to more than 50TeV. The two telescopes were built in 2004 and 2009, respectively, with different cameras, triggers and readout systems. In the years 2011–2012 the MAGIC collaboration undertook a major upgrade to make the stereoscopic system uniform, improving its overall performance and easing its maintenance. In particular, the camera, the receivers and the trigger of the first telescope were replaced and the readout of the two telescopes was upgraded. This paper (Part I) describes the details of the upgrade as well as the basic performance parameters of MAGIC such as raw data treatment, linearity in the electronic chain and sources of noise. In Part II, we describe the physics performance of the upgraded system. | ||
| 520 | |a The MAGIC telescopes are two Imaging Atmospheric Cherenkov Telescopes (IACTs) located on the Canary island of La Palma. The telescopes are designed to measure Cherenkov light from air showers initiated by gamma rays in the energy regime from around 50GeV to more than 50TeV. The two telescopes were built in 2004 and 2009, respectively, with different cameras, triggers and readout systems. In the years 2011–2012 the MAGIC collaboration undertook a major upgrade to make the stereoscopic system uniform, improving its overall performance and easing its maintenance. In particular, the camera, the receivers and the trigger of the first telescope were replaced and the readout of the two telescopes was upgraded. This paper (Part I) describes the details of the upgrade as well as the basic performance parameters of MAGIC such as raw data treatment, linearity in the electronic chain and sources of noise. In Part II, we describe the physics performance of the upgraded system. | ||
| 650 | 7 | |a TeV astrophysics |2 Elsevier | |
| 650 | 7 | |a Instruments |2 Elsevier | |
| 650 | 7 | |a MAGIC |2 Elsevier | |
| 650 | 7 | |a Imaging Atmospheric Cherenkov Telescopes |2 Elsevier | |
| 650 | 7 | |a Very High Energy Gamma Rays |2 Elsevier | |
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| 700 | 1 | |a Antonelli, L.A. |4 oth | |
| 700 | 1 | |a Antoranz, P. |4 oth | |
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10.1016/j.astropartphys.2015.04.004 doi GBVA2016016000009.pica (DE-627)ELV035447966 (ELSEVIER)S0927-6505(15)00066-3 DE-627 ger DE-627 rakwb eng 540 540 DE-600 620 VZ 690 VZ 50.92 bkl Aleksić, J. verfasserin aut The major upgrade of the MAGIC telescopes, Part I: The hardware improvements and the commissioning of the system 2016transfer abstract 15 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The MAGIC telescopes are two Imaging Atmospheric Cherenkov Telescopes (IACTs) located on the Canary island of La Palma. The telescopes are designed to measure Cherenkov light from air showers initiated by gamma rays in the energy regime from around 50GeV to more than 50TeV. The two telescopes were built in 2004 and 2009, respectively, with different cameras, triggers and readout systems. In the years 2011–2012 the MAGIC collaboration undertook a major upgrade to make the stereoscopic system uniform, improving its overall performance and easing its maintenance. In particular, the camera, the receivers and the trigger of the first telescope were replaced and the readout of the two telescopes was upgraded. This paper (Part I) describes the details of the upgrade as well as the basic performance parameters of MAGIC such as raw data treatment, linearity in the electronic chain and sources of noise. In Part II, we describe the physics performance of the upgraded system. The MAGIC telescopes are two Imaging Atmospheric Cherenkov Telescopes (IACTs) located on the Canary island of La Palma. The telescopes are designed to measure Cherenkov light from air showers initiated by gamma rays in the energy regime from around 50GeV to more than 50TeV. The two telescopes were built in 2004 and 2009, respectively, with different cameras, triggers and readout systems. In the years 2011–2012 the MAGIC collaboration undertook a major upgrade to make the stereoscopic system uniform, improving its overall performance and easing its maintenance. In particular, the camera, the receivers and the trigger of the first telescope were replaced and the readout of the two telescopes was upgraded. This paper (Part I) describes the details of the upgrade as well as the basic performance parameters of MAGIC such as raw data treatment, linearity in the electronic chain and sources of noise. In Part II, we describe the physics performance of the upgraded system. TeV astrophysics Elsevier Instruments Elsevier MAGIC Elsevier Imaging Atmospheric Cherenkov Telescopes Elsevier Very High Energy Gamma Rays Elsevier Ansoldi, S. oth Antonelli, L.A. oth Antoranz, P. oth Babic, A. oth Bangale, P. oth Barceló, M. oth Barrio, J.A. oth Becerra González, J. oth Bednarek, W. oth Bernardini, E. oth Biasuzzi, B. oth Biland, A. oth Bitossi, M. oth Blanch, O. oth Bonnefoy, S. oth Bonnoli, G. oth Borracci, F. oth Bretz, T. oth Carmona, E. oth Carosi, A. oth Cecchi, R. oth Colin, P. oth Colombo, E. oth Contreras, J.L. oth Corti, D. oth Cortina, J. oth Covino, S. oth Da Vela, P. oth Dazzi, F. oth DeAngelis, A. oth De Caneva, G. oth De Lotto, B. oth de Oña Wilhelmi, E. oth Delgado Mendez, C. oth Dettlaff, A. oth Dominis Prester, D. oth Dorner, D. oth Doro, M. oth Einecke, S. oth Eisenacher, D. oth Elsaesser, D. oth Fidalgo, D. oth Fink, D. oth Fonseca, M.V. oth Font, L. oth Frantzen, K. oth Fruck, C. oth Galindo, D. oth García López, R.J. oth Garczarczyk, M. oth Garrido Terrats, D. oth Gaug, M. oth Giavitto, G. oth Godinović, N. oth González Muñoz, A. oth Gozzini, S.R. oth Haberer, W. oth Hadasch, D. oth Hanabata, Y. oth Hayashida, M. oth Herrera, J. oth Hildebrand, D. oth Hose, J. oth Hrupec, D. oth Idec, W. oth Illa, J.M. oth Kadenius, V. oth Kellermann, H. oth Knoetig, M.L. oth Kodani, K. oth Konno, Y. oth Krause, J. oth Kubo, H. oth Kushida, J. oth La Barbera, A. oth Lelas, D. oth Lemus, J.L. oth Lewandowska, N. oth Lindfors, E. oth Lombardi, S. oth Longo, F. oth López, M. oth López-Coto, R. oth López-Oramas, A. oth Lorca, A. oth Lorenz, E. oth Lozano, I. oth Makariev, M. oth Mallot, K. oth Maneva, G. oth Mankuzhiyil, N. oth Mannheim, K. oth Maraschi, L. oth Marcote, B. oth Mariotti, M. oth Martínez, M. oth Mazin, D. oth Menzel, U. oth Miranda, J.M. oth Mirzoyan, R. oth Moralejo, A. oth Munar-Adrover, P. oth Nakajima, D. oth Negrello, M. oth Neustroev, V. oth Niedzwiecki, A. oth Nilsson, K. oth Nishijima, K. oth Noda, K. oth Orito, R. oth Overkemping, A. oth Paiano, S. oth Palatiello, M. oth Paneque, D. oth Paoletti, R. oth Paredes, J.M. oth Paredes-Fortuny, X. oth Persic, M. oth Poutanen, J. oth Prada Moroni, P.G. oth Prandini, E. oth Puljak, I. oth Reinthal, R. oth Rhode, W. oth Ribó, M. oth Rico, J. oth Rodriguez Garcia, J. oth Rügamer, S. oth Saito, T. oth Saito, K. oth Satalecka, K. oth Scalzotto, V. oth Scapin, V. oth Schultz, C. oth Schlammer, J. oth Schmidl, S. oth Schweizer, T. oth Sillanpää, A. oth Sitarek, J. oth Snidaric, I. oth Sobczynska, D. oth Spanier, F. oth Stamerra, A. oth Steinbring, T. oth Storz, J. oth Strzys, M. oth Takalo, L. oth Takami, H. oth Tavecchio, F. oth Tejedor, L.A. oth Temnikov, P. oth Terzić, T. oth Tescaro, D. oth Teshima, M. oth Thaele, J. oth Tibolla, O. oth Torres, D.F. oth Toyama, T. oth Treves, A. oth Vogler, P. oth Wetteskind, H. oth Will, M. oth Zanin, R. oth Enthalten in Elsevier Science Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells 2012transfer abstract Amsterdam [u.a.] (DE-627)ELV016257995 volume:72 year:2016 day:1 month:01 pages:61-75 extent:15 https://doi.org/10.1016/j.astropartphys.2015.04.004 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_252 50.92 Meerestechnik VZ AR 72 2016 1 0101 61-75 15 045F 540 |
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10.1016/j.astropartphys.2015.04.004 doi GBVA2016016000009.pica (DE-627)ELV035447966 (ELSEVIER)S0927-6505(15)00066-3 DE-627 ger DE-627 rakwb eng 540 540 DE-600 620 VZ 690 VZ 50.92 bkl Aleksić, J. verfasserin aut The major upgrade of the MAGIC telescopes, Part I: The hardware improvements and the commissioning of the system 2016transfer abstract 15 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The MAGIC telescopes are two Imaging Atmospheric Cherenkov Telescopes (IACTs) located on the Canary island of La Palma. The telescopes are designed to measure Cherenkov light from air showers initiated by gamma rays in the energy regime from around 50GeV to more than 50TeV. The two telescopes were built in 2004 and 2009, respectively, with different cameras, triggers and readout systems. In the years 2011–2012 the MAGIC collaboration undertook a major upgrade to make the stereoscopic system uniform, improving its overall performance and easing its maintenance. In particular, the camera, the receivers and the trigger of the first telescope were replaced and the readout of the two telescopes was upgraded. This paper (Part I) describes the details of the upgrade as well as the basic performance parameters of MAGIC such as raw data treatment, linearity in the electronic chain and sources of noise. In Part II, we describe the physics performance of the upgraded system. The MAGIC telescopes are two Imaging Atmospheric Cherenkov Telescopes (IACTs) located on the Canary island of La Palma. The telescopes are designed to measure Cherenkov light from air showers initiated by gamma rays in the energy regime from around 50GeV to more than 50TeV. The two telescopes were built in 2004 and 2009, respectively, with different cameras, triggers and readout systems. In the years 2011–2012 the MAGIC collaboration undertook a major upgrade to make the stereoscopic system uniform, improving its overall performance and easing its maintenance. In particular, the camera, the receivers and the trigger of the first telescope were replaced and the readout of the two telescopes was upgraded. This paper (Part I) describes the details of the upgrade as well as the basic performance parameters of MAGIC such as raw data treatment, linearity in the electronic chain and sources of noise. In Part II, we describe the physics performance of the upgraded system. TeV astrophysics Elsevier Instruments Elsevier MAGIC Elsevier Imaging Atmospheric Cherenkov Telescopes Elsevier Very High Energy Gamma Rays Elsevier Ansoldi, S. oth Antonelli, L.A. oth Antoranz, P. oth Babic, A. oth Bangale, P. oth Barceló, M. oth Barrio, J.A. oth Becerra González, J. oth Bednarek, W. oth Bernardini, E. oth Biasuzzi, B. oth Biland, A. oth Bitossi, M. oth Blanch, O. oth Bonnefoy, S. oth Bonnoli, G. oth Borracci, F. oth Bretz, T. oth Carmona, E. oth Carosi, A. oth Cecchi, R. oth Colin, P. oth Colombo, E. oth Contreras, J.L. oth Corti, D. oth Cortina, J. oth Covino, S. oth Da Vela, P. oth Dazzi, F. oth DeAngelis, A. oth De Caneva, G. oth De Lotto, B. oth de Oña Wilhelmi, E. oth Delgado Mendez, C. oth Dettlaff, A. oth Dominis Prester, D. oth Dorner, D. oth Doro, M. oth Einecke, S. oth Eisenacher, D. oth Elsaesser, D. oth Fidalgo, D. oth Fink, D. oth Fonseca, M.V. oth Font, L. oth Frantzen, K. oth Fruck, C. oth Galindo, D. oth García López, R.J. oth Garczarczyk, M. oth Garrido Terrats, D. oth Gaug, M. oth Giavitto, G. oth Godinović, N. oth González Muñoz, A. oth Gozzini, S.R. oth Haberer, W. oth Hadasch, D. oth Hanabata, Y. oth Hayashida, M. oth Herrera, J. oth Hildebrand, D. oth Hose, J. oth Hrupec, D. oth Idec, W. oth Illa, J.M. oth Kadenius, V. oth Kellermann, H. oth Knoetig, M.L. oth Kodani, K. oth Konno, Y. oth Krause, J. oth Kubo, H. oth Kushida, J. oth La Barbera, A. oth Lelas, D. oth Lemus, J.L. oth Lewandowska, N. oth Lindfors, E. oth Lombardi, S. oth Longo, F. oth López, M. oth López-Coto, R. oth López-Oramas, A. oth Lorca, A. oth Lorenz, E. oth Lozano, I. oth Makariev, M. oth Mallot, K. oth Maneva, G. oth Mankuzhiyil, N. oth Mannheim, K. oth Maraschi, L. oth Marcote, B. oth Mariotti, M. oth Martínez, M. oth Mazin, D. oth Menzel, U. oth Miranda, J.M. oth Mirzoyan, R. oth Moralejo, A. oth Munar-Adrover, P. oth Nakajima, D. oth Negrello, M. oth Neustroev, V. oth Niedzwiecki, A. oth Nilsson, K. oth Nishijima, K. oth Noda, K. oth Orito, R. oth Overkemping, A. oth Paiano, S. oth Palatiello, M. oth Paneque, D. oth Paoletti, R. oth Paredes, J.M. oth Paredes-Fortuny, X. oth Persic, M. oth Poutanen, J. oth Prada Moroni, P.G. oth Prandini, E. oth Puljak, I. oth Reinthal, R. oth Rhode, W. oth Ribó, M. oth Rico, J. oth Rodriguez Garcia, J. oth Rügamer, S. oth Saito, T. oth Saito, K. oth Satalecka, K. oth Scalzotto, V. oth Scapin, V. oth Schultz, C. oth Schlammer, J. oth Schmidl, S. oth Schweizer, T. oth Sillanpää, A. oth Sitarek, J. oth Snidaric, I. oth Sobczynska, D. oth Spanier, F. oth Stamerra, A. oth Steinbring, T. oth Storz, J. oth Strzys, M. oth Takalo, L. oth Takami, H. oth Tavecchio, F. oth Tejedor, L.A. oth Temnikov, P. oth Terzić, T. oth Tescaro, D. oth Teshima, M. oth Thaele, J. oth Tibolla, O. oth Torres, D.F. oth Toyama, T. oth Treves, A. oth Vogler, P. oth Wetteskind, H. oth Will, M. oth Zanin, R. oth Enthalten in Elsevier Science Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells 2012transfer abstract Amsterdam [u.a.] (DE-627)ELV016257995 volume:72 year:2016 day:1 month:01 pages:61-75 extent:15 https://doi.org/10.1016/j.astropartphys.2015.04.004 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_252 50.92 Meerestechnik VZ AR 72 2016 1 0101 61-75 15 045F 540 |
| allfields_unstemmed |
10.1016/j.astropartphys.2015.04.004 doi GBVA2016016000009.pica (DE-627)ELV035447966 (ELSEVIER)S0927-6505(15)00066-3 DE-627 ger DE-627 rakwb eng 540 540 DE-600 620 VZ 690 VZ 50.92 bkl Aleksić, J. verfasserin aut The major upgrade of the MAGIC telescopes, Part I: The hardware improvements and the commissioning of the system 2016transfer abstract 15 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The MAGIC telescopes are two Imaging Atmospheric Cherenkov Telescopes (IACTs) located on the Canary island of La Palma. The telescopes are designed to measure Cherenkov light from air showers initiated by gamma rays in the energy regime from around 50GeV to more than 50TeV. The two telescopes were built in 2004 and 2009, respectively, with different cameras, triggers and readout systems. In the years 2011–2012 the MAGIC collaboration undertook a major upgrade to make the stereoscopic system uniform, improving its overall performance and easing its maintenance. In particular, the camera, the receivers and the trigger of the first telescope were replaced and the readout of the two telescopes was upgraded. This paper (Part I) describes the details of the upgrade as well as the basic performance parameters of MAGIC such as raw data treatment, linearity in the electronic chain and sources of noise. In Part II, we describe the physics performance of the upgraded system. The MAGIC telescopes are two Imaging Atmospheric Cherenkov Telescopes (IACTs) located on the Canary island of La Palma. The telescopes are designed to measure Cherenkov light from air showers initiated by gamma rays in the energy regime from around 50GeV to more than 50TeV. The two telescopes were built in 2004 and 2009, respectively, with different cameras, triggers and readout systems. In the years 2011–2012 the MAGIC collaboration undertook a major upgrade to make the stereoscopic system uniform, improving its overall performance and easing its maintenance. In particular, the camera, the receivers and the trigger of the first telescope were replaced and the readout of the two telescopes was upgraded. This paper (Part I) describes the details of the upgrade as well as the basic performance parameters of MAGIC such as raw data treatment, linearity in the electronic chain and sources of noise. In Part II, we describe the physics performance of the upgraded system. TeV astrophysics Elsevier Instruments Elsevier MAGIC Elsevier Imaging Atmospheric Cherenkov Telescopes Elsevier Very High Energy Gamma Rays Elsevier Ansoldi, S. oth Antonelli, L.A. oth Antoranz, P. oth Babic, A. oth Bangale, P. oth Barceló, M. oth Barrio, J.A. oth Becerra González, J. oth Bednarek, W. oth Bernardini, E. oth Biasuzzi, B. oth Biland, A. oth Bitossi, M. oth Blanch, O. oth Bonnefoy, S. oth Bonnoli, G. oth Borracci, F. oth Bretz, T. oth Carmona, E. oth Carosi, A. oth Cecchi, R. oth Colin, P. oth Colombo, E. oth Contreras, J.L. oth Corti, D. oth Cortina, J. oth Covino, S. oth Da Vela, P. oth Dazzi, F. oth DeAngelis, A. oth De Caneva, G. oth De Lotto, B. oth de Oña Wilhelmi, E. oth Delgado Mendez, C. oth Dettlaff, A. oth Dominis Prester, D. oth Dorner, D. oth Doro, M. oth Einecke, S. oth Eisenacher, D. oth Elsaesser, D. oth Fidalgo, D. oth Fink, D. oth Fonseca, M.V. oth Font, L. oth Frantzen, K. oth Fruck, C. oth Galindo, D. oth García López, R.J. oth Garczarczyk, M. oth Garrido Terrats, D. oth Gaug, M. oth Giavitto, G. oth Godinović, N. oth González Muñoz, A. oth Gozzini, S.R. oth Haberer, W. oth Hadasch, D. oth Hanabata, Y. oth Hayashida, M. oth Herrera, J. oth Hildebrand, D. oth Hose, J. oth Hrupec, D. oth Idec, W. oth Illa, J.M. oth Kadenius, V. oth Kellermann, H. oth Knoetig, M.L. oth Kodani, K. oth Konno, Y. oth Krause, J. oth Kubo, H. oth Kushida, J. oth La Barbera, A. oth Lelas, D. oth Lemus, J.L. oth Lewandowska, N. oth Lindfors, E. oth Lombardi, S. oth Longo, F. oth López, M. oth López-Coto, R. oth López-Oramas, A. oth Lorca, A. oth Lorenz, E. oth Lozano, I. oth Makariev, M. oth Mallot, K. oth Maneva, G. oth Mankuzhiyil, N. oth Mannheim, K. oth Maraschi, L. oth Marcote, B. oth Mariotti, M. oth Martínez, M. oth Mazin, D. oth Menzel, U. oth Miranda, J.M. oth Mirzoyan, R. oth Moralejo, A. oth Munar-Adrover, P. oth Nakajima, D. oth Negrello, M. oth Neustroev, V. oth Niedzwiecki, A. oth Nilsson, K. oth Nishijima, K. oth Noda, K. oth Orito, R. oth Overkemping, A. oth Paiano, S. oth Palatiello, M. oth Paneque, D. oth Paoletti, R. oth Paredes, J.M. oth Paredes-Fortuny, X. oth Persic, M. oth Poutanen, J. oth Prada Moroni, P.G. oth Prandini, E. oth Puljak, I. oth Reinthal, R. oth Rhode, W. oth Ribó, M. oth Rico, J. oth Rodriguez Garcia, J. oth Rügamer, S. oth Saito, T. oth Saito, K. oth Satalecka, K. oth Scalzotto, V. oth Scapin, V. oth Schultz, C. oth Schlammer, J. oth Schmidl, S. oth Schweizer, T. oth Sillanpää, A. oth Sitarek, J. oth Snidaric, I. oth Sobczynska, D. oth Spanier, F. oth Stamerra, A. oth Steinbring, T. oth Storz, J. oth Strzys, M. oth Takalo, L. oth Takami, H. oth Tavecchio, F. oth Tejedor, L.A. oth Temnikov, P. oth Terzić, T. oth Tescaro, D. oth Teshima, M. oth Thaele, J. oth Tibolla, O. oth Torres, D.F. oth Toyama, T. oth Treves, A. oth Vogler, P. oth Wetteskind, H. oth Will, M. oth Zanin, R. oth Enthalten in Elsevier Science Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells 2012transfer abstract Amsterdam [u.a.] (DE-627)ELV016257995 volume:72 year:2016 day:1 month:01 pages:61-75 extent:15 https://doi.org/10.1016/j.astropartphys.2015.04.004 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_252 50.92 Meerestechnik VZ AR 72 2016 1 0101 61-75 15 045F 540 |
| allfieldsGer |
10.1016/j.astropartphys.2015.04.004 doi GBVA2016016000009.pica (DE-627)ELV035447966 (ELSEVIER)S0927-6505(15)00066-3 DE-627 ger DE-627 rakwb eng 540 540 DE-600 620 VZ 690 VZ 50.92 bkl Aleksić, J. verfasserin aut The major upgrade of the MAGIC telescopes, Part I: The hardware improvements and the commissioning of the system 2016transfer abstract 15 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The MAGIC telescopes are two Imaging Atmospheric Cherenkov Telescopes (IACTs) located on the Canary island of La Palma. The telescopes are designed to measure Cherenkov light from air showers initiated by gamma rays in the energy regime from around 50GeV to more than 50TeV. The two telescopes were built in 2004 and 2009, respectively, with different cameras, triggers and readout systems. In the years 2011–2012 the MAGIC collaboration undertook a major upgrade to make the stereoscopic system uniform, improving its overall performance and easing its maintenance. In particular, the camera, the receivers and the trigger of the first telescope were replaced and the readout of the two telescopes was upgraded. This paper (Part I) describes the details of the upgrade as well as the basic performance parameters of MAGIC such as raw data treatment, linearity in the electronic chain and sources of noise. In Part II, we describe the physics performance of the upgraded system. The MAGIC telescopes are two Imaging Atmospheric Cherenkov Telescopes (IACTs) located on the Canary island of La Palma. The telescopes are designed to measure Cherenkov light from air showers initiated by gamma rays in the energy regime from around 50GeV to more than 50TeV. The two telescopes were built in 2004 and 2009, respectively, with different cameras, triggers and readout systems. In the years 2011–2012 the MAGIC collaboration undertook a major upgrade to make the stereoscopic system uniform, improving its overall performance and easing its maintenance. In particular, the camera, the receivers and the trigger of the first telescope were replaced and the readout of the two telescopes was upgraded. This paper (Part I) describes the details of the upgrade as well as the basic performance parameters of MAGIC such as raw data treatment, linearity in the electronic chain and sources of noise. In Part II, we describe the physics performance of the upgraded system. TeV astrophysics Elsevier Instruments Elsevier MAGIC Elsevier Imaging Atmospheric Cherenkov Telescopes Elsevier Very High Energy Gamma Rays Elsevier Ansoldi, S. oth Antonelli, L.A. oth Antoranz, P. oth Babic, A. oth Bangale, P. oth Barceló, M. oth Barrio, J.A. oth Becerra González, J. oth Bednarek, W. oth Bernardini, E. oth Biasuzzi, B. oth Biland, A. oth Bitossi, M. oth Blanch, O. oth Bonnefoy, S. oth Bonnoli, G. oth Borracci, F. oth Bretz, T. oth Carmona, E. oth Carosi, A. oth Cecchi, R. oth Colin, P. oth Colombo, E. oth Contreras, J.L. oth Corti, D. oth Cortina, J. oth Covino, S. oth Da Vela, P. oth Dazzi, F. oth DeAngelis, A. oth De Caneva, G. oth De Lotto, B. oth de Oña Wilhelmi, E. oth Delgado Mendez, C. oth Dettlaff, A. oth Dominis Prester, D. oth Dorner, D. oth Doro, M. oth Einecke, S. oth Eisenacher, D. oth Elsaesser, D. oth Fidalgo, D. oth Fink, D. oth Fonseca, M.V. oth Font, L. oth Frantzen, K. oth Fruck, C. oth Galindo, D. oth García López, R.J. oth Garczarczyk, M. oth Garrido Terrats, D. oth Gaug, M. oth Giavitto, G. oth Godinović, N. oth González Muñoz, A. oth Gozzini, S.R. oth Haberer, W. oth Hadasch, D. oth Hanabata, Y. oth Hayashida, M. oth Herrera, J. oth Hildebrand, D. oth Hose, J. oth Hrupec, D. oth Idec, W. oth Illa, J.M. oth Kadenius, V. oth Kellermann, H. oth Knoetig, M.L. oth Kodani, K. oth Konno, Y. oth Krause, J. oth Kubo, H. oth Kushida, J. oth La Barbera, A. oth Lelas, D. oth Lemus, J.L. oth Lewandowska, N. oth Lindfors, E. oth Lombardi, S. oth Longo, F. oth López, M. oth López-Coto, R. oth López-Oramas, A. oth Lorca, A. oth Lorenz, E. oth Lozano, I. oth Makariev, M. oth Mallot, K. oth Maneva, G. oth Mankuzhiyil, N. oth Mannheim, K. oth Maraschi, L. oth Marcote, B. oth Mariotti, M. oth Martínez, M. oth Mazin, D. oth Menzel, U. oth Miranda, J.M. oth Mirzoyan, R. oth Moralejo, A. oth Munar-Adrover, P. oth Nakajima, D. oth Negrello, M. oth Neustroev, V. oth Niedzwiecki, A. oth Nilsson, K. oth Nishijima, K. oth Noda, K. oth Orito, R. oth Overkemping, A. oth Paiano, S. oth Palatiello, M. oth Paneque, D. oth Paoletti, R. oth Paredes, J.M. oth Paredes-Fortuny, X. oth Persic, M. oth Poutanen, J. oth Prada Moroni, P.G. oth Prandini, E. oth Puljak, I. oth Reinthal, R. oth Rhode, W. oth Ribó, M. oth Rico, J. oth Rodriguez Garcia, J. oth Rügamer, S. oth Saito, T. oth Saito, K. oth Satalecka, K. oth Scalzotto, V. oth Scapin, V. oth Schultz, C. oth Schlammer, J. oth Schmidl, S. oth Schweizer, T. oth Sillanpää, A. oth Sitarek, J. oth Snidaric, I. oth Sobczynska, D. oth Spanier, F. oth Stamerra, A. oth Steinbring, T. oth Storz, J. oth Strzys, M. oth Takalo, L. oth Takami, H. oth Tavecchio, F. oth Tejedor, L.A. oth Temnikov, P. oth Terzić, T. oth Tescaro, D. oth Teshima, M. oth Thaele, J. oth Tibolla, O. oth Torres, D.F. oth Toyama, T. oth Treves, A. oth Vogler, P. oth Wetteskind, H. oth Will, M. oth Zanin, R. oth Enthalten in Elsevier Science Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells 2012transfer abstract Amsterdam [u.a.] (DE-627)ELV016257995 volume:72 year:2016 day:1 month:01 pages:61-75 extent:15 https://doi.org/10.1016/j.astropartphys.2015.04.004 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_252 50.92 Meerestechnik VZ AR 72 2016 1 0101 61-75 15 045F 540 |
| allfieldsSound |
10.1016/j.astropartphys.2015.04.004 doi GBVA2016016000009.pica (DE-627)ELV035447966 (ELSEVIER)S0927-6505(15)00066-3 DE-627 ger DE-627 rakwb eng 540 540 DE-600 620 VZ 690 VZ 50.92 bkl Aleksić, J. verfasserin aut The major upgrade of the MAGIC telescopes, Part I: The hardware improvements and the commissioning of the system 2016transfer abstract 15 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The MAGIC telescopes are two Imaging Atmospheric Cherenkov Telescopes (IACTs) located on the Canary island of La Palma. The telescopes are designed to measure Cherenkov light from air showers initiated by gamma rays in the energy regime from around 50GeV to more than 50TeV. The two telescopes were built in 2004 and 2009, respectively, with different cameras, triggers and readout systems. In the years 2011–2012 the MAGIC collaboration undertook a major upgrade to make the stereoscopic system uniform, improving its overall performance and easing its maintenance. In particular, the camera, the receivers and the trigger of the first telescope were replaced and the readout of the two telescopes was upgraded. This paper (Part I) describes the details of the upgrade as well as the basic performance parameters of MAGIC such as raw data treatment, linearity in the electronic chain and sources of noise. In Part II, we describe the physics performance of the upgraded system. The MAGIC telescopes are two Imaging Atmospheric Cherenkov Telescopes (IACTs) located on the Canary island of La Palma. The telescopes are designed to measure Cherenkov light from air showers initiated by gamma rays in the energy regime from around 50GeV to more than 50TeV. The two telescopes were built in 2004 and 2009, respectively, with different cameras, triggers and readout systems. In the years 2011–2012 the MAGIC collaboration undertook a major upgrade to make the stereoscopic system uniform, improving its overall performance and easing its maintenance. In particular, the camera, the receivers and the trigger of the first telescope were replaced and the readout of the two telescopes was upgraded. This paper (Part I) describes the details of the upgrade as well as the basic performance parameters of MAGIC such as raw data treatment, linearity in the electronic chain and sources of noise. In Part II, we describe the physics performance of the upgraded system. TeV astrophysics Elsevier Instruments Elsevier MAGIC Elsevier Imaging Atmospheric Cherenkov Telescopes Elsevier Very High Energy Gamma Rays Elsevier Ansoldi, S. oth Antonelli, L.A. oth Antoranz, P. oth Babic, A. oth Bangale, P. oth Barceló, M. oth Barrio, J.A. oth Becerra González, J. oth Bednarek, W. oth Bernardini, E. oth Biasuzzi, B. oth Biland, A. oth Bitossi, M. oth Blanch, O. oth Bonnefoy, S. oth Bonnoli, G. oth Borracci, F. oth Bretz, T. oth Carmona, E. oth Carosi, A. oth Cecchi, R. oth Colin, P. oth Colombo, E. oth Contreras, J.L. oth Corti, D. oth Cortina, J. oth Covino, S. oth Da Vela, P. oth Dazzi, F. oth DeAngelis, A. oth De Caneva, G. oth De Lotto, B. oth de Oña Wilhelmi, E. oth Delgado Mendez, C. oth Dettlaff, A. oth Dominis Prester, D. oth Dorner, D. oth Doro, M. oth Einecke, S. oth Eisenacher, D. oth Elsaesser, D. oth Fidalgo, D. oth Fink, D. oth Fonseca, M.V. oth Font, L. oth Frantzen, K. oth Fruck, C. oth Galindo, D. oth García López, R.J. oth Garczarczyk, M. oth Garrido Terrats, D. oth Gaug, M. oth Giavitto, G. oth Godinović, N. oth González Muñoz, A. oth Gozzini, S.R. oth Haberer, W. oth Hadasch, D. oth Hanabata, Y. oth Hayashida, M. oth Herrera, J. oth Hildebrand, D. oth Hose, J. oth Hrupec, D. oth Idec, W. oth Illa, J.M. oth Kadenius, V. oth Kellermann, H. oth Knoetig, M.L. oth Kodani, K. oth Konno, Y. oth Krause, J. oth Kubo, H. oth Kushida, J. oth La Barbera, A. oth Lelas, D. oth Lemus, J.L. oth Lewandowska, N. oth Lindfors, E. oth Lombardi, S. oth Longo, F. oth López, M. oth López-Coto, R. oth López-Oramas, A. oth Lorca, A. oth Lorenz, E. oth Lozano, I. oth Makariev, M. oth Mallot, K. oth Maneva, G. oth Mankuzhiyil, N. oth Mannheim, K. oth Maraschi, L. oth Marcote, B. oth Mariotti, M. oth Martínez, M. oth Mazin, D. oth Menzel, U. oth Miranda, J.M. oth Mirzoyan, R. oth Moralejo, A. oth Munar-Adrover, P. oth Nakajima, D. oth Negrello, M. oth Neustroev, V. oth Niedzwiecki, A. oth Nilsson, K. oth Nishijima, K. oth Noda, K. oth Orito, R. oth Overkemping, A. oth Paiano, S. oth Palatiello, M. oth Paneque, D. oth Paoletti, R. oth Paredes, J.M. oth Paredes-Fortuny, X. oth Persic, M. oth Poutanen, J. oth Prada Moroni, P.G. oth Prandini, E. oth Puljak, I. oth Reinthal, R. oth Rhode, W. oth Ribó, M. oth Rico, J. oth Rodriguez Garcia, J. oth Rügamer, S. oth Saito, T. oth Saito, K. oth Satalecka, K. oth Scalzotto, V. oth Scapin, V. oth Schultz, C. oth Schlammer, J. oth Schmidl, S. oth Schweizer, T. oth Sillanpää, A. oth Sitarek, J. oth Snidaric, I. oth Sobczynska, D. oth Spanier, F. oth Stamerra, A. oth Steinbring, T. oth Storz, J. oth Strzys, M. oth Takalo, L. oth Takami, H. oth Tavecchio, F. oth Tejedor, L.A. oth Temnikov, P. oth Terzić, T. oth Tescaro, D. oth Teshima, M. oth Thaele, J. oth Tibolla, O. oth Torres, D.F. oth Toyama, T. oth Treves, A. oth Vogler, P. oth Wetteskind, H. oth Will, M. oth Zanin, R. oth Enthalten in Elsevier Science Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells 2012transfer abstract Amsterdam [u.a.] (DE-627)ELV016257995 volume:72 year:2016 day:1 month:01 pages:61-75 extent:15 https://doi.org/10.1016/j.astropartphys.2015.04.004 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_252 50.92 Meerestechnik VZ AR 72 2016 1 0101 61-75 15 045F 540 |
| language |
English |
| source |
Enthalten in Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells Amsterdam [u.a.] volume:72 year:2016 day:1 month:01 pages:61-75 extent:15 |
| sourceStr |
Enthalten in Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells Amsterdam [u.a.] volume:72 year:2016 day:1 month:01 pages:61-75 extent:15 |
| format_phy_str_mv |
Article |
| bklname |
Meerestechnik |
| institution |
findex.gbv.de |
| topic_facet |
TeV astrophysics Instruments MAGIC Imaging Atmospheric Cherenkov Telescopes Very High Energy Gamma Rays |
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Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells |
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Aleksić, J. @@aut@@ Ansoldi, S. @@oth@@ Antonelli, L.A. @@oth@@ Antoranz, P. @@oth@@ Babic, A. @@oth@@ Bangale, P. @@oth@@ Barceló, M. @@oth@@ Barrio, J.A. @@oth@@ Becerra González, J. @@oth@@ Bednarek, W. @@oth@@ Bernardini, E. @@oth@@ Biasuzzi, B. @@oth@@ Biland, A. @@oth@@ Bitossi, M. @@oth@@ Blanch, O. @@oth@@ Bonnefoy, S. @@oth@@ Bonnoli, G. @@oth@@ Borracci, F. @@oth@@ Bretz, T. @@oth@@ Carmona, E. @@oth@@ Carosi, A. @@oth@@ Cecchi, R. @@oth@@ Colin, P. @@oth@@ Colombo, E. @@oth@@ Contreras, J.L. @@oth@@ Corti, D. @@oth@@ Cortina, J. @@oth@@ Covino, S. @@oth@@ Da Vela, P. @@oth@@ Dazzi, F. @@oth@@ DeAngelis, A. @@oth@@ De Caneva, G. @@oth@@ De Lotto, B. @@oth@@ de Oña Wilhelmi, E. @@oth@@ Delgado Mendez, C. @@oth@@ Dettlaff, A. @@oth@@ Dominis Prester, D. @@oth@@ Dorner, D. @@oth@@ Doro, M. @@oth@@ Einecke, S. @@oth@@ Eisenacher, D. @@oth@@ Elsaesser, D. @@oth@@ Fidalgo, D. @@oth@@ Fink, D. @@oth@@ Fonseca, M.V. @@oth@@ Font, L. @@oth@@ Frantzen, K. @@oth@@ Fruck, C. @@oth@@ Galindo, D. @@oth@@ García López, R.J. @@oth@@ Garczarczyk, M. @@oth@@ Garrido Terrats, D. @@oth@@ Gaug, M. @@oth@@ Giavitto, G. @@oth@@ Godinović, N. @@oth@@ González Muñoz, A. @@oth@@ Gozzini, S.R. @@oth@@ Haberer, W. @@oth@@ Hadasch, D. @@oth@@ Hanabata, Y. @@oth@@ Hayashida, M. @@oth@@ Herrera, J. @@oth@@ Hildebrand, D. @@oth@@ Hose, J. @@oth@@ Hrupec, D. @@oth@@ Idec, W. @@oth@@ Illa, J.M. @@oth@@ Kadenius, V. @@oth@@ Kellermann, H. @@oth@@ Knoetig, M.L. @@oth@@ Kodani, K. @@oth@@ Konno, Y. @@oth@@ Krause, J. @@oth@@ Kubo, H. @@oth@@ Kushida, J. @@oth@@ La Barbera, A. @@oth@@ Lelas, D. @@oth@@ Lemus, J.L. @@oth@@ Lewandowska, N. @@oth@@ Lindfors, E. @@oth@@ Lombardi, S. @@oth@@ Longo, F. @@oth@@ López, M. @@oth@@ López-Coto, R. @@oth@@ López-Oramas, A. @@oth@@ Lorca, A. @@oth@@ Lorenz, E. @@oth@@ Lozano, I. @@oth@@ Makariev, M. @@oth@@ Mallot, K. @@oth@@ Maneva, G. @@oth@@ Mankuzhiyil, N. @@oth@@ Mannheim, K. @@oth@@ Maraschi, L. @@oth@@ Marcote, B. @@oth@@ Mariotti, M. @@oth@@ Martínez, M. @@oth@@ Mazin, D. @@oth@@ Menzel, U. @@oth@@ Miranda, J.M. @@oth@@ Mirzoyan, R. @@oth@@ Moralejo, A. @@oth@@ Munar-Adrover, P. @@oth@@ Nakajima, D. @@oth@@ Negrello, M. @@oth@@ Neustroev, V. @@oth@@ Niedzwiecki, A. @@oth@@ Nilsson, K. @@oth@@ Nishijima, K. @@oth@@ Noda, K. @@oth@@ Orito, R. @@oth@@ Overkemping, A. @@oth@@ Paiano, S. @@oth@@ Palatiello, M. @@oth@@ Paneque, D. @@oth@@ Paoletti, R. @@oth@@ Paredes, J.M. @@oth@@ Paredes-Fortuny, X. @@oth@@ Persic, M. @@oth@@ Poutanen, J. @@oth@@ Prada Moroni, P.G. @@oth@@ Prandini, E. @@oth@@ Puljak, I. @@oth@@ Reinthal, R. @@oth@@ Rhode, W. @@oth@@ Ribó, M. @@oth@@ Rico, J. @@oth@@ Rodriguez Garcia, J. @@oth@@ Rügamer, S. @@oth@@ Saito, T. @@oth@@ Saito, K. @@oth@@ Satalecka, K. @@oth@@ Scalzotto, V. @@oth@@ Scapin, V. @@oth@@ Schultz, C. @@oth@@ Schlammer, J. @@oth@@ Schmidl, S. @@oth@@ Schweizer, T. @@oth@@ Sillanpää, A. @@oth@@ Sitarek, J. @@oth@@ Snidaric, I. @@oth@@ Sobczynska, D. @@oth@@ Spanier, F. @@oth@@ Stamerra, A. @@oth@@ Steinbring, T. @@oth@@ Storz, J. @@oth@@ Strzys, M. @@oth@@ Takalo, L. @@oth@@ Takami, H. @@oth@@ Tavecchio, F. @@oth@@ Tejedor, L.A. @@oth@@ Temnikov, P. @@oth@@ Terzić, T. @@oth@@ Tescaro, D. @@oth@@ Teshima, M. @@oth@@ Thaele, J. @@oth@@ Tibolla, O. @@oth@@ Torres, D.F. @@oth@@ Toyama, T. @@oth@@ Treves, A. @@oth@@ Vogler, P. @@oth@@ Wetteskind, H. @@oth@@ Will, M. @@oth@@ Zanin, R. @@oth@@ |
| publishDateDaySort_date |
2016-01-01T00:00:00Z |
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ELV016257995 |
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3540 |
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ELV035447966 |
| language_de |
englisch |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">ELV035447966</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230625204256.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">180603s2016 xx |||||o 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1016/j.astropartphys.2015.04.004</subfield><subfield code="2">doi</subfield></datafield><datafield tag="028" ind1="5" ind2="2"><subfield code="a">GBVA2016016000009.pica</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)ELV035447966</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(ELSEVIER)S0927-6505(15)00066-3</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2=" "><subfield code="a">540</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">540</subfield><subfield code="q">DE-600</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">620</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">690</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">50.92</subfield><subfield code="2">bkl</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Aleksić, J.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="4"><subfield code="a">The major upgrade of the MAGIC telescopes, Part I: The hardware improvements and the commissioning of the system</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2016transfer abstract</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">15</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zzz</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">z</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zu</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">The MAGIC telescopes are two Imaging Atmospheric Cherenkov Telescopes (IACTs) located on the Canary island of La Palma. The telescopes are designed to measure Cherenkov light from air showers initiated by gamma rays in the energy regime from around 50GeV to more than 50TeV. The two telescopes were built in 2004 and 2009, respectively, with different cameras, triggers and readout systems. In the years 2011–2012 the MAGIC collaboration undertook a major upgrade to make the stereoscopic system uniform, improving its overall performance and easing its maintenance. In particular, the camera, the receivers and the trigger of the first telescope were replaced and the readout of the two telescopes was upgraded. This paper (Part I) describes the details of the upgrade as well as the basic performance parameters of MAGIC such as raw data treatment, linearity in the electronic chain and sources of noise. In Part II, we describe the physics performance of the upgraded system.</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">The MAGIC telescopes are two Imaging Atmospheric Cherenkov Telescopes (IACTs) located on the Canary island of La Palma. The telescopes are designed to measure Cherenkov light from air showers initiated by gamma rays in the energy regime from around 50GeV to more than 50TeV. The two telescopes were built in 2004 and 2009, respectively, with different cameras, triggers and readout systems. In the years 2011–2012 the MAGIC collaboration undertook a major upgrade to make the stereoscopic system uniform, improving its overall performance and easing its maintenance. In particular, the camera, the receivers and the trigger of the first telescope were replaced and the readout of the two telescopes was upgraded. This paper (Part I) describes the details of the upgrade as well as the basic performance parameters of MAGIC such as raw data treatment, linearity in the electronic chain and sources of noise. In Part II, we describe the physics performance of the upgraded system.</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">TeV astrophysics</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Instruments</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">MAGIC</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Imaging Atmospheric Cherenkov Telescopes</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Very High Energy Gamma Rays</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ansoldi, S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Antonelli, 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Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells |
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major upgrade of the magic telescopes, part i: the hardware improvements and the commissioning of the system |
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The major upgrade of the MAGIC telescopes, Part I: The hardware improvements and the commissioning of the system |
| abstract |
The MAGIC telescopes are two Imaging Atmospheric Cherenkov Telescopes (IACTs) located on the Canary island of La Palma. The telescopes are designed to measure Cherenkov light from air showers initiated by gamma rays in the energy regime from around 50GeV to more than 50TeV. The two telescopes were built in 2004 and 2009, respectively, with different cameras, triggers and readout systems. In the years 2011–2012 the MAGIC collaboration undertook a major upgrade to make the stereoscopic system uniform, improving its overall performance and easing its maintenance. In particular, the camera, the receivers and the trigger of the first telescope were replaced and the readout of the two telescopes was upgraded. This paper (Part I) describes the details of the upgrade as well as the basic performance parameters of MAGIC such as raw data treatment, linearity in the electronic chain and sources of noise. In Part II, we describe the physics performance of the upgraded system. |
| abstractGer |
The MAGIC telescopes are two Imaging Atmospheric Cherenkov Telescopes (IACTs) located on the Canary island of La Palma. The telescopes are designed to measure Cherenkov light from air showers initiated by gamma rays in the energy regime from around 50GeV to more than 50TeV. The two telescopes were built in 2004 and 2009, respectively, with different cameras, triggers and readout systems. In the years 2011–2012 the MAGIC collaboration undertook a major upgrade to make the stereoscopic system uniform, improving its overall performance and easing its maintenance. In particular, the camera, the receivers and the trigger of the first telescope were replaced and the readout of the two telescopes was upgraded. This paper (Part I) describes the details of the upgrade as well as the basic performance parameters of MAGIC such as raw data treatment, linearity in the electronic chain and sources of noise. In Part II, we describe the physics performance of the upgraded system. |
| abstract_unstemmed |
The MAGIC telescopes are two Imaging Atmospheric Cherenkov Telescopes (IACTs) located on the Canary island of La Palma. The telescopes are designed to measure Cherenkov light from air showers initiated by gamma rays in the energy regime from around 50GeV to more than 50TeV. The two telescopes were built in 2004 and 2009, respectively, with different cameras, triggers and readout systems. In the years 2011–2012 the MAGIC collaboration undertook a major upgrade to make the stereoscopic system uniform, improving its overall performance and easing its maintenance. In particular, the camera, the receivers and the trigger of the first telescope were replaced and the readout of the two telescopes was upgraded. This paper (Part I) describes the details of the upgrade as well as the basic performance parameters of MAGIC such as raw data treatment, linearity in the electronic chain and sources of noise. In Part II, we describe the physics performance of the upgraded system. |
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The major upgrade of the MAGIC telescopes, Part I: The hardware improvements and the commissioning of the system |
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https://doi.org/10.1016/j.astropartphys.2015.04.004 |
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| doi_str |
10.1016/j.astropartphys.2015.04.004 |
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2024-07-06T17:34:48.241Z |
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