Observations of the Crab Nebula and Pulsar with the Large-sized Telescope Prototype of the Cherenkov Telescope Array Article Swipe
YOU?
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· 2023
· Open Access
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· DOI: https://doi.org/10.3847/1538-4357/ace89d
The Cherenkov Telescope Array (CTA) is a next-generation ground-based observatory for gamma-ray astronomy at very high energies. The Large-Sized Telescope prototype (LST-1) is located at the CTA-North site, on the Canary Island of La Palma. LSTs are designed to provide optimal performance in the lowest part of the energy range covered by CTA, down to ≃20 GeV. LST-1 started performing astronomical observations in 2019 November, during its commissioning phase, and it has been taking data ever since. We present the first LST-1 observations of the Crab Nebula, the standard candle of very-high-energy gamma-ray astronomy, and use them, together with simulations, to assess the performance of the telescope. LST-1 has reached the expected performance during its commissioning period—only a minor adjustment of the preexisting simulations was needed to match the telescope’s behavior. The energy threshold at trigger level is around 20 GeV, rising to ≃30 GeV after data analysis. Performance parameters depend strongly on energy, and on the strength of the gamma-ray selection cuts in the analysis: angular resolution ranges from 0.°12–0.°40, and energy resolution from 15%–50%. Flux sensitivity is around 1.1% of the Crab Nebula flux above 250 GeV for a 50 hr observation (12% for 30 minutes). The spectral energy distribution (in the 0.03–30 TeV range) and the light curve obtained for the Crab Nebula agree with previous measurements, considering statistical and systematic uncertainties. A clear periodic signal is also detected from the pulsar at the center of the Nebula.
Related Topics
- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.3847/1538-4357/ace89d
- https://iopscience.iop.org/article/10.3847/1538-4357/ace89d/pdf
- OA Status
- gold
- Cited By
- 39
- References
- 54
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4381795727
Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W4381795727Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.3847/1538-4357/ace89dDigital Object Identifier
- Title
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Observations of the Crab Nebula and Pulsar with the Large-sized Telescope Prototype of the Cherenkov Telescope ArrayWork title
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articleOpenAlex work type
- Language
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enPrimary language
- Publication year
-
2023Year of publication
- Publication date
-
2023-10-01Full publication date if available
- Authors
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Hidetarô Abe, K. Abe, S. Abe, Arnau Aguasca-Cabot, I. Agudo, Nuria Álvarez Crespo, L. A. Antonelli, C. Aramo, A. Arbet Engels, C. Arcaro, Manuel Artero, Katsuaki Asano, P. Aubert, A. Baktash, A. Bamba, Andrés Baquero, L. Baroncelli, U. Barres de Almeida, J. A. Barrio, Ivana Batković, J. Baxter, J. Becerra González, E. Bernardini, M. Bernardos, J. Bernete Medrano, A. Berti, Pooja Bhattacharjee, Noah Biederbeck, C. Bigongiari, E. Bissaldi, O. Blanch, G. Bonnoli, P. Bordas, A. Borghese, A. Bulgarelli, I. Burelli, Mario Buscemi, M Cardillo, Sami Caroff, A. Carosi, F. Cassol-Brunner, D. Cauz, G. Ceribella, Yating Chai, K. S. Cheng, A. Chiavassa, M. Chikawa, L. Chytka, A. Cifuentes, J. L. Contreras, J. Cortina, H. Costantini, Giacomo D’Amico, M. Dalchenko, A. De Angelis, Mathieu de Bony de Lavergne, B. De Lotto, Raniere de Menezes, G. Deleglise, C. Delgado Mendez, J. Delgado, D. della Volpe, M. Dellaiera, Davide Depaoli, Ambra Di Piano, F. Di Pierro, R. Di Tria, L. Di Venere, C. Díaz, Rune Michael Dominik, D. Dominis Prester, Alice Donini, D. Dorner, M. Doro, Dominik Elsässer, Gabriel Emery, Juan Escudero, V. Fallah Ramazani, G. Ferrara, F. Ferrarotto, A. Fiasson, Lluís Freixas Coromina, Stefan Fröse, Satoshi Fukami, Y. Fukazawa, Enrique Alonso García, R. Garcia López, C. Gasbarra, D Gasparrini, Felix Geyer, J. Giesbrecht Paiva, N. Giglietto, F. Giordano, E. Giro, Paweł Gliwny, N. Godinović, R. Grau, D. Green, Jarred Gershon Green, Shuichi GunjiList of authors in order
- Landing page
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https://doi.org/10.3847/1538-4357/ace89dPublisher landing page
- PDF URL
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https://iopscience.iop.org/article/10.3847/1538-4357/ace89d/pdfDirect link to full text PDF
- Open access
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YesWhether a free full text is available
- OA status
-
goldOpen access status per OpenAlex
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https://iopscience.iop.org/article/10.3847/1538-4357/ace89d/pdfDirect OA link when available
- Concepts
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Crab Nebula, Physics, Cherenkov Telescope Array, Telescope, Cherenkov radiation, Pulsar, Angular resolution (graph drawing), Astrophysics, Observatory, Astronomy, Crab Pulsar, Gamma-ray astronomy, Range (aeronautics), Flux (metallurgy), Nebula, Gamma ray, Optics, Detector, Stars, Mathematics, Combinatorics, Composite material, Metallurgy, Materials scienceTop concepts (fields/topics) attached by OpenAlex
- Cited by
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39Total citation count in OpenAlex
- Citations by year (recent)
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2025: 15, 2024: 14, 2023: 10Per-year citation counts (last 5 years)
- References (count)
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54Number of works referenced by this work
- Related works (count)
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10Other works algorithmically related by OpenAlex
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| abstract_inverted_index.clear | 227 |
| abstract_inverted_index.curve | 211 |
| abstract_inverted_index.first | 81 |
| abstract_inverted_index.level | 137 |
| abstract_inverted_index.light | 210 |
| abstract_inverted_index.match | 128 |
| abstract_inverted_index.minor | 119 |
| abstract_inverted_index.range | 50 |
| abstract_inverted_index.site, | 28 |
| abstract_inverted_index.them, | 97 |
| abstract_inverted_index.≃20 | 56 |
| abstract_inverted_index.≃30 | 144 |
| abstract_inverted_index.Canary | 31 |
| abstract_inverted_index.Island | 32 |
| abstract_inverted_index.Nebula | 185, 216 |
| abstract_inverted_index.Palma. | 35 |
| abstract_inverted_index.around | 139, 180 |
| abstract_inverted_index.assess | 102 |
| abstract_inverted_index.candle | 90 |
| abstract_inverted_index.center | 238 |
| abstract_inverted_index.depend | 151 |
| abstract_inverted_index.during | 66, 114 |
| abstract_inverted_index.energy | 49, 133, 173, 201 |
| abstract_inverted_index.lowest | 45 |
| abstract_inverted_index.needed | 126 |
| abstract_inverted_index.phase, | 69 |
| abstract_inverted_index.pulsar | 235 |
| abstract_inverted_index.range) | 207 |
| abstract_inverted_index.ranges | 169 |
| abstract_inverted_index.rising | 142 |
| abstract_inverted_index.signal | 229 |
| abstract_inverted_index.since. | 77 |
| abstract_inverted_index.taking | 74 |
| abstract_inverted_index.(LST-1) | 22 |
| abstract_inverted_index.Nebula, | 87 |
| abstract_inverted_index.Nebula. | 241 |
| abstract_inverted_index.angular | 167 |
| abstract_inverted_index.covered | 51 |
| abstract_inverted_index.energy, | 154 |
| abstract_inverted_index.located | 24 |
| abstract_inverted_index.optimal | 41 |
| abstract_inverted_index.present | 79 |
| abstract_inverted_index.provide | 40 |
| abstract_inverted_index.reached | 110 |
| abstract_inverted_index.started | 59 |
| abstract_inverted_index.trigger | 136 |
| abstract_inverted_index.Abstract | 0 |
| abstract_inverted_index.designed | 38 |
| abstract_inverted_index.detected | 232 |
| abstract_inverted_index.expected | 112 |
| abstract_inverted_index.obtained | 212 |
| abstract_inverted_index.periodic | 228 |
| abstract_inverted_index.previous | 219 |
| abstract_inverted_index.spectral | 200 |
| abstract_inverted_index.standard | 89 |
| abstract_inverted_index.strength | 158 |
| abstract_inverted_index.strongly | 152 |
| abstract_inverted_index.together | 98 |
| abstract_inverted_index.0.03–30 | 205 |
| abstract_inverted_index.CTA-North | 27 |
| abstract_inverted_index.Cherenkov | 2 |
| abstract_inverted_index.November, | 65 |
| abstract_inverted_index.Telescope | 3, 20 |
| abstract_inverted_index.analysis. | 148 |
| abstract_inverted_index.analysis: | 166 |
| abstract_inverted_index.astronomy | 13 |
| abstract_inverted_index.behavior. | 131 |
| abstract_inverted_index.energies. | 17 |
| abstract_inverted_index.gamma-ray | 12, 93, 161 |
| abstract_inverted_index.minutes). | 198 |
| abstract_inverted_index.prototype | 21 |
| abstract_inverted_index.selection | 162 |
| abstract_inverted_index.threshold | 134 |
| abstract_inverted_index.15%–50%. | 176 |
| abstract_inverted_index.adjustment | 120 |
| abstract_inverted_index.astronomy, | 94 |
| abstract_inverted_index.parameters | 150 |
| abstract_inverted_index.performing | 60 |
| abstract_inverted_index.resolution | 168, 174 |
| abstract_inverted_index.systematic | 224 |
| abstract_inverted_index.telescope. | 107 |
| abstract_inverted_index.Large-Sized | 19 |
| abstract_inverted_index.Performance | 149 |
| abstract_inverted_index.considering | 221 |
| abstract_inverted_index.observation | 194 |
| abstract_inverted_index.observatory | 10 |
| abstract_inverted_index.performance | 42, 104, 113 |
| abstract_inverted_index.preexisting | 123 |
| abstract_inverted_index.sensitivity | 178 |
| abstract_inverted_index.simulations | 124 |
| abstract_inverted_index.statistical | 222 |
| abstract_inverted_index.astronomical | 61 |
| abstract_inverted_index.distribution | 202 |
| abstract_inverted_index.ground-based | 9 |
| abstract_inverted_index.observations | 62, 83 |
| abstract_inverted_index.simulations, | 100 |
| abstract_inverted_index.commissioning | 68, 116 |
| abstract_inverted_index.measurements, | 220 |
| abstract_inverted_index.period—only | 117 |
| abstract_inverted_index.telescope’s | 130 |
| abstract_inverted_index.uncertainties. | 225 |
| abstract_inverted_index.next-generation | 8 |
| abstract_inverted_index.0.°12–0.°40, | 171 |
| abstract_inverted_index.very-high-energy | 92 |
| cited_by_percentile_year.max | 100 |
| cited_by_percentile_year.min | 99 |
| countries_distinct_count | 14 |
| institutions_distinct_count | 290 |
| sustainable_development_goals[0].id | https://metadata.un.org/sdg/7 |
| sustainable_development_goals[0].score | 0.8999999761581421 |
| sustainable_development_goals[0].display_name | Affordable and clean energy |
| citation_normalized_percentile.value | 0.99613674 |
| citation_normalized_percentile.is_in_top_1_percent | False |
| citation_normalized_percentile.is_in_top_10_percent | True |