Monte Carlo performance studies for the site selection of the Cherenkov Telescope Array
The Cherenkov Telescope Array (CTA) represents the next generation of ground-based instruments for very-high-energy (VHE) gamma-ray astronomy, aimed at improving on the sensitivity of current-generation experiments by an order of magnitude and providing coverage over four decades of energy. The curr...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Hassan, T. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2017transfer abstract |
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| Umfang: |
10 |
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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:93 ; year:2017 ; pages:76-85 ; extent:10 |
| Links: |
|---|
| DOI / URN: |
10.1016/j.astropartphys.2017.05.001 |
|---|
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ELV036005045 |
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| 520 | |a The Cherenkov Telescope Array (CTA) represents the next generation of ground-based instruments for very-high-energy (VHE) gamma-ray astronomy, aimed at improving on the sensitivity of current-generation experiments by an order of magnitude and providing coverage over four decades of energy. The current CTA design consists of two arrays of tens of imaging atmospheric Cherenkov Telescopes, comprising Small, Medium and Large-Sized Telescopes, with one array located in each of the Northern and Southern Hemispheres. To study the effect of the site choice on the overall CTA performance and support the site evaluation process, detailed Monte Carlo simulations have been performed. These results show the impact of different site-related attributes such as altitude, night-sky background and local geomagnetic field on CTA performance for the observation of VHE gamma rays. | ||
| 520 | |a The Cherenkov Telescope Array (CTA) represents the next generation of ground-based instruments for very-high-energy (VHE) gamma-ray astronomy, aimed at improving on the sensitivity of current-generation experiments by an order of magnitude and providing coverage over four decades of energy. The current CTA design consists of two arrays of tens of imaging atmospheric Cherenkov Telescopes, comprising Small, Medium and Large-Sized Telescopes, with one array located in each of the Northern and Southern Hemispheres. To study the effect of the site choice on the overall CTA performance and support the site evaluation process, detailed Monte Carlo simulations have been performed. These results show the impact of different site-related attributes such as altitude, night-sky background and local geomagnetic field on CTA performance for the observation of VHE gamma rays. | ||
| 700 | 1 | |a Arrabito, L. |4 oth | |
| 700 | 1 | |a Bernlöhr, K. |4 oth | |
| 700 | 1 | |a Bregeon, J. |4 oth | |
| 700 | 1 | |a Cortina, J. |4 oth | |
| 700 | 1 | |a Cumani, P. |4 oth | |
| 700 | 1 | |a Di Pierro, F. |4 oth | |
| 700 | 1 | |a Falceta-Goncalves, D. |4 oth | |
| 700 | 1 | |a Lang, R.G. |4 oth | |
| 700 | 1 | |a Hinton, J. |4 oth | |
| 700 | 1 | |a Jogler, T. |4 oth | |
| 700 | 1 | |a Maier, G. |4 oth | |
| 700 | 1 | |a Moralejo, A. |4 oth | |
| 700 | 1 | |a Morselli, A. |4 oth | |
| 700 | 1 | |a Todero Peixoto, C.J. |4 oth | |
| 700 | 1 | |a Wood, M. |4 oth | |
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10.1016/j.astropartphys.2017.05.001 doi GBV00000000000283A.pica (DE-627)ELV036005045 (ELSEVIER)S0927-6505(17)30008-7 DE-627 ger DE-627 rakwb eng 540 540 DE-600 620 VZ 690 VZ 50.92 bkl Hassan, T. verfasserin aut Monte Carlo performance studies for the site selection of the Cherenkov Telescope Array 2017transfer abstract 10 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The Cherenkov Telescope Array (CTA) represents the next generation of ground-based instruments for very-high-energy (VHE) gamma-ray astronomy, aimed at improving on the sensitivity of current-generation experiments by an order of magnitude and providing coverage over four decades of energy. The current CTA design consists of two arrays of tens of imaging atmospheric Cherenkov Telescopes, comprising Small, Medium and Large-Sized Telescopes, with one array located in each of the Northern and Southern Hemispheres. To study the effect of the site choice on the overall CTA performance and support the site evaluation process, detailed Monte Carlo simulations have been performed. These results show the impact of different site-related attributes such as altitude, night-sky background and local geomagnetic field on CTA performance for the observation of VHE gamma rays. The Cherenkov Telescope Array (CTA) represents the next generation of ground-based instruments for very-high-energy (VHE) gamma-ray astronomy, aimed at improving on the sensitivity of current-generation experiments by an order of magnitude and providing coverage over four decades of energy. The current CTA design consists of two arrays of tens of imaging atmospheric Cherenkov Telescopes, comprising Small, Medium and Large-Sized Telescopes, with one array located in each of the Northern and Southern Hemispheres. To study the effect of the site choice on the overall CTA performance and support the site evaluation process, detailed Monte Carlo simulations have been performed. These results show the impact of different site-related attributes such as altitude, night-sky background and local geomagnetic field on CTA performance for the observation of VHE gamma rays. Arrabito, L. oth Bernlöhr, K. oth Bregeon, J. oth Cortina, J. oth Cumani, P. oth Di Pierro, F. oth Falceta-Goncalves, D. oth Lang, R.G. oth Hinton, J. oth Jogler, T. oth Maier, G. oth Moralejo, A. oth Morselli, A. oth Todero Peixoto, C.J. oth Wood, M. 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:93 year:2017 pages:76-85 extent:10 https://doi.org/10.1016/j.astropartphys.2017.05.001 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_252 50.92 Meerestechnik VZ AR 93 2017 76-85 10 045F 540 |
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10.1016/j.astropartphys.2017.05.001 doi GBV00000000000283A.pica (DE-627)ELV036005045 (ELSEVIER)S0927-6505(17)30008-7 DE-627 ger DE-627 rakwb eng 540 540 DE-600 620 VZ 690 VZ 50.92 bkl Hassan, T. verfasserin aut Monte Carlo performance studies for the site selection of the Cherenkov Telescope Array 2017transfer abstract 10 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The Cherenkov Telescope Array (CTA) represents the next generation of ground-based instruments for very-high-energy (VHE) gamma-ray astronomy, aimed at improving on the sensitivity of current-generation experiments by an order of magnitude and providing coverage over four decades of energy. The current CTA design consists of two arrays of tens of imaging atmospheric Cherenkov Telescopes, comprising Small, Medium and Large-Sized Telescopes, with one array located in each of the Northern and Southern Hemispheres. To study the effect of the site choice on the overall CTA performance and support the site evaluation process, detailed Monte Carlo simulations have been performed. These results show the impact of different site-related attributes such as altitude, night-sky background and local geomagnetic field on CTA performance for the observation of VHE gamma rays. The Cherenkov Telescope Array (CTA) represents the next generation of ground-based instruments for very-high-energy (VHE) gamma-ray astronomy, aimed at improving on the sensitivity of current-generation experiments by an order of magnitude and providing coverage over four decades of energy. The current CTA design consists of two arrays of tens of imaging atmospheric Cherenkov Telescopes, comprising Small, Medium and Large-Sized Telescopes, with one array located in each of the Northern and Southern Hemispheres. To study the effect of the site choice on the overall CTA performance and support the site evaluation process, detailed Monte Carlo simulations have been performed. These results show the impact of different site-related attributes such as altitude, night-sky background and local geomagnetic field on CTA performance for the observation of VHE gamma rays. Arrabito, L. oth Bernlöhr, K. oth Bregeon, J. oth Cortina, J. oth Cumani, P. oth Di Pierro, F. oth Falceta-Goncalves, D. oth Lang, R.G. oth Hinton, J. oth Jogler, T. oth Maier, G. oth Moralejo, A. oth Morselli, A. oth Todero Peixoto, C.J. oth Wood, M. 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:93 year:2017 pages:76-85 extent:10 https://doi.org/10.1016/j.astropartphys.2017.05.001 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_252 50.92 Meerestechnik VZ AR 93 2017 76-85 10 045F 540 |
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10.1016/j.astropartphys.2017.05.001 doi GBV00000000000283A.pica (DE-627)ELV036005045 (ELSEVIER)S0927-6505(17)30008-7 DE-627 ger DE-627 rakwb eng 540 540 DE-600 620 VZ 690 VZ 50.92 bkl Hassan, T. verfasserin aut Monte Carlo performance studies for the site selection of the Cherenkov Telescope Array 2017transfer abstract 10 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The Cherenkov Telescope Array (CTA) represents the next generation of ground-based instruments for very-high-energy (VHE) gamma-ray astronomy, aimed at improving on the sensitivity of current-generation experiments by an order of magnitude and providing coverage over four decades of energy. The current CTA design consists of two arrays of tens of imaging atmospheric Cherenkov Telescopes, comprising Small, Medium and Large-Sized Telescopes, with one array located in each of the Northern and Southern Hemispheres. To study the effect of the site choice on the overall CTA performance and support the site evaluation process, detailed Monte Carlo simulations have been performed. These results show the impact of different site-related attributes such as altitude, night-sky background and local geomagnetic field on CTA performance for the observation of VHE gamma rays. The Cherenkov Telescope Array (CTA) represents the next generation of ground-based instruments for very-high-energy (VHE) gamma-ray astronomy, aimed at improving on the sensitivity of current-generation experiments by an order of magnitude and providing coverage over four decades of energy. The current CTA design consists of two arrays of tens of imaging atmospheric Cherenkov Telescopes, comprising Small, Medium and Large-Sized Telescopes, with one array located in each of the Northern and Southern Hemispheres. To study the effect of the site choice on the overall CTA performance and support the site evaluation process, detailed Monte Carlo simulations have been performed. These results show the impact of different site-related attributes such as altitude, night-sky background and local geomagnetic field on CTA performance for the observation of VHE gamma rays. Arrabito, L. oth Bernlöhr, K. oth Bregeon, J. oth Cortina, J. oth Cumani, P. oth Di Pierro, F. oth Falceta-Goncalves, D. oth Lang, R.G. oth Hinton, J. oth Jogler, T. oth Maier, G. oth Moralejo, A. oth Morselli, A. oth Todero Peixoto, C.J. oth Wood, M. 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:93 year:2017 pages:76-85 extent:10 https://doi.org/10.1016/j.astropartphys.2017.05.001 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_252 50.92 Meerestechnik VZ AR 93 2017 76-85 10 045F 540 |
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10.1016/j.astropartphys.2017.05.001 doi GBV00000000000283A.pica (DE-627)ELV036005045 (ELSEVIER)S0927-6505(17)30008-7 DE-627 ger DE-627 rakwb eng 540 540 DE-600 620 VZ 690 VZ 50.92 bkl Hassan, T. verfasserin aut Monte Carlo performance studies for the site selection of the Cherenkov Telescope Array 2017transfer abstract 10 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The Cherenkov Telescope Array (CTA) represents the next generation of ground-based instruments for very-high-energy (VHE) gamma-ray astronomy, aimed at improving on the sensitivity of current-generation experiments by an order of magnitude and providing coverage over four decades of energy. The current CTA design consists of two arrays of tens of imaging atmospheric Cherenkov Telescopes, comprising Small, Medium and Large-Sized Telescopes, with one array located in each of the Northern and Southern Hemispheres. To study the effect of the site choice on the overall CTA performance and support the site evaluation process, detailed Monte Carlo simulations have been performed. These results show the impact of different site-related attributes such as altitude, night-sky background and local geomagnetic field on CTA performance for the observation of VHE gamma rays. The Cherenkov Telescope Array (CTA) represents the next generation of ground-based instruments for very-high-energy (VHE) gamma-ray astronomy, aimed at improving on the sensitivity of current-generation experiments by an order of magnitude and providing coverage over four decades of energy. The current CTA design consists of two arrays of tens of imaging atmospheric Cherenkov Telescopes, comprising Small, Medium and Large-Sized Telescopes, with one array located in each of the Northern and Southern Hemispheres. To study the effect of the site choice on the overall CTA performance and support the site evaluation process, detailed Monte Carlo simulations have been performed. These results show the impact of different site-related attributes such as altitude, night-sky background and local geomagnetic field on CTA performance for the observation of VHE gamma rays. Arrabito, L. oth Bernlöhr, K. oth Bregeon, J. oth Cortina, J. oth Cumani, P. oth Di Pierro, F. oth Falceta-Goncalves, D. oth Lang, R.G. oth Hinton, J. oth Jogler, T. oth Maier, G. oth Moralejo, A. oth Morselli, A. oth Todero Peixoto, C.J. oth Wood, M. 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:93 year:2017 pages:76-85 extent:10 https://doi.org/10.1016/j.astropartphys.2017.05.001 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_252 50.92 Meerestechnik VZ AR 93 2017 76-85 10 045F 540 |
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10.1016/j.astropartphys.2017.05.001 doi GBV00000000000283A.pica (DE-627)ELV036005045 (ELSEVIER)S0927-6505(17)30008-7 DE-627 ger DE-627 rakwb eng 540 540 DE-600 620 VZ 690 VZ 50.92 bkl Hassan, T. verfasserin aut Monte Carlo performance studies for the site selection of the Cherenkov Telescope Array 2017transfer abstract 10 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The Cherenkov Telescope Array (CTA) represents the next generation of ground-based instruments for very-high-energy (VHE) gamma-ray astronomy, aimed at improving on the sensitivity of current-generation experiments by an order of magnitude and providing coverage over four decades of energy. The current CTA design consists of two arrays of tens of imaging atmospheric Cherenkov Telescopes, comprising Small, Medium and Large-Sized Telescopes, with one array located in each of the Northern and Southern Hemispheres. To study the effect of the site choice on the overall CTA performance and support the site evaluation process, detailed Monte Carlo simulations have been performed. These results show the impact of different site-related attributes such as altitude, night-sky background and local geomagnetic field on CTA performance for the observation of VHE gamma rays. The Cherenkov Telescope Array (CTA) represents the next generation of ground-based instruments for very-high-energy (VHE) gamma-ray astronomy, aimed at improving on the sensitivity of current-generation experiments by an order of magnitude and providing coverage over four decades of energy. The current CTA design consists of two arrays of tens of imaging atmospheric Cherenkov Telescopes, comprising Small, Medium and Large-Sized Telescopes, with one array located in each of the Northern and Southern Hemispheres. To study the effect of the site choice on the overall CTA performance and support the site evaluation process, detailed Monte Carlo simulations have been performed. These results show the impact of different site-related attributes such as altitude, night-sky background and local geomagnetic field on CTA performance for the observation of VHE gamma rays. Arrabito, L. oth Bernlöhr, K. oth Bregeon, J. oth Cortina, J. oth Cumani, P. oth Di Pierro, F. oth Falceta-Goncalves, D. oth Lang, R.G. oth Hinton, J. oth Jogler, T. oth Maier, G. oth Moralejo, A. oth Morselli, A. oth Todero Peixoto, C.J. oth Wood, M. 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:93 year:2017 pages:76-85 extent:10 https://doi.org/10.1016/j.astropartphys.2017.05.001 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_252 50.92 Meerestechnik VZ AR 93 2017 76-85 10 045F 540 |
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English |
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Enthalten in Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells Amsterdam [u.a.] volume:93 year:2017 pages:76-85 extent:10 |
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Enthalten in Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells Amsterdam [u.a.] volume:93 year:2017 pages:76-85 extent:10 |
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Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells |
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Hassan, T. @@aut@@ Arrabito, L. @@oth@@ Bernlöhr, K. @@oth@@ Bregeon, J. @@oth@@ Cortina, J. @@oth@@ Cumani, P. @@oth@@ Di Pierro, F. @@oth@@ Falceta-Goncalves, D. @@oth@@ Lang, R.G. @@oth@@ Hinton, J. @@oth@@ Jogler, T. @@oth@@ Maier, G. @@oth@@ Moralejo, A. @@oth@@ Morselli, A. @@oth@@ Todero Peixoto, C.J. @@oth@@ Wood, M. @@oth@@ |
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Monte Carlo performance studies for the site selection of the Cherenkov Telescope Array |
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The Cherenkov Telescope Array (CTA) represents the next generation of ground-based instruments for very-high-energy (VHE) gamma-ray astronomy, aimed at improving on the sensitivity of current-generation experiments by an order of magnitude and providing coverage over four decades of energy. The current CTA design consists of two arrays of tens of imaging atmospheric Cherenkov Telescopes, comprising Small, Medium and Large-Sized Telescopes, with one array located in each of the Northern and Southern Hemispheres. To study the effect of the site choice on the overall CTA performance and support the site evaluation process, detailed Monte Carlo simulations have been performed. These results show the impact of different site-related attributes such as altitude, night-sky background and local geomagnetic field on CTA performance for the observation of VHE gamma rays. |
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The Cherenkov Telescope Array (CTA) represents the next generation of ground-based instruments for very-high-energy (VHE) gamma-ray astronomy, aimed at improving on the sensitivity of current-generation experiments by an order of magnitude and providing coverage over four decades of energy. The current CTA design consists of two arrays of tens of imaging atmospheric Cherenkov Telescopes, comprising Small, Medium and Large-Sized Telescopes, with one array located in each of the Northern and Southern Hemispheres. To study the effect of the site choice on the overall CTA performance and support the site evaluation process, detailed Monte Carlo simulations have been performed. These results show the impact of different site-related attributes such as altitude, night-sky background and local geomagnetic field on CTA performance for the observation of VHE gamma rays. |
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The Cherenkov Telescope Array (CTA) represents the next generation of ground-based instruments for very-high-energy (VHE) gamma-ray astronomy, aimed at improving on the sensitivity of current-generation experiments by an order of magnitude and providing coverage over four decades of energy. The current CTA design consists of two arrays of tens of imaging atmospheric Cherenkov Telescopes, comprising Small, Medium and Large-Sized Telescopes, with one array located in each of the Northern and Southern Hemispheres. To study the effect of the site choice on the overall CTA performance and support the site evaluation process, detailed Monte Carlo simulations have been performed. These results show the impact of different site-related attributes such as altitude, night-sky background and local geomagnetic field on CTA performance for the observation of VHE gamma rays. |
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Monte Carlo performance studies for the site selection of the Cherenkov Telescope Array |
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