- MIUR ,EC| CTA-PP ,EC| ESCAPE ,EC| PROBIST ,EC| PREBIST ,DFG ,EC| CTA-DEV ,EC| INFIERIAbe, H.; Abe, K.;
Artero, M.; Artero, M.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesArtero, M. in OpenAIRE
Hackfeld, J.; +196 AuthorsHackfeld, J.
Harvested from ORCID Public Data FileHackfeld, J. in OpenAIREAbe, H.; Abe, K.; Artero, M.; Artero, M.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesArtero, M. in OpenAIRE Hackfeld, J.; Hackfeld, J.
Harvested from ORCID Public Data FileHackfeld, J. in OpenAIRE Hadasch, D.; Hadasch, D.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesHadasch, D. in OpenAIRE Hahn, A.; Hashiyama, K.;Hahn, A.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesHahn, A. in OpenAIRE Hassan, T.; Hassan, T.
Harvested from ORCID Public Data FileHassan, T. in OpenAIRE Hayashi, K.; Hayashi, K.
Harvested from ORCID Public Data FileHayashi, K. in OpenAIRE Heckmann, L.; Heckmann, L.
Harvested from ORCID Public Data FileHeckmann, L. in OpenAIRE Heller, M.; Herrera Llorente, J.;Heller, M.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesHeller, M. in OpenAIRE Hirotani, K.; Hirotani, K.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesHirotani, K. in OpenAIRE Asano, K.; Asano, K.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesAsano, K. in OpenAIRE Hoffmann, D.; Hoffmann, D.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesHoffmann, D. in OpenAIRE Horns, D.; Horns, D.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesHorns, D. in OpenAIRE Houles, J.; Houles, J.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesHoules, J. in OpenAIRE Hrabovsky, M.; Hrabovsky, M.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesHrabovsky, M. in OpenAIRE Hrupec, D.; Hui, D.;Hrupec, D.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesHrupec, D. in OpenAIRE Hütten, M.; Hütten, M.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesHütten, M. in OpenAIRE Iarlori, M.; Iarlori, M.
Harvested from ORCID Public Data FileIarlori, M. in OpenAIRE Imazawa, R.; Imazawa, R.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesImazawa, R. in OpenAIRE Inada, T.; Aubert, P.; Inome, Y.; Ioka, K.;Inome, Y.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesInome, Y. in OpenAIRE Iori, M.; Ishio, K.; Iwamura, Y.;Iori, M.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesIori, M. in OpenAIRE Jacquemont, M.; Jacquemont, M.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesJacquemont, M. in OpenAIRE Martinez, I. Jimenez; Martinez, I. Jimenez
Harvested from ORCID Public Data FileMartinez, I. Jimenez in OpenAIRE Jurysek, J.; Kagaya, M.;Jurysek, J.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesJurysek, J. in OpenAIRE Karas, V.; Karas, V.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesKaras, V. in OpenAIRE Baktash, A.; Baktash, A.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesBaktash, A. in OpenAIRE Katagiri, H.; Katagiri, H.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesKatagiri, H. in OpenAIRE Kataoka, J.; Kataoka, J.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesKataoka, J. in OpenAIRE Kerszberg, D.; Kerszberg, D.
Harvested from ORCID Public Data FileKerszberg, D. in OpenAIRE Kobayashi, Y.; Kobayashi, Y.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesKobayashi, Y. in OpenAIRE Kong, A.; Kubo, H.; Kubo, H.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesKubo, H. in OpenAIRE Kushida, J.; Kushida, J.
Harvested from ORCID Public Data FileKushida, J. in OpenAIRE Lainez, M.; Lamanna, G.;Lainez, M.
Harvested from ORCID Public Data FileLainez, M. in OpenAIRE Lamastra, A.; Lamastra, A.
Harvested from ORCID Public Data FileLamastra, A. in OpenAIRE Bamba, A.; Le Flour, T.; Linhoff, M.; Linhoff, M.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesLinhoff, M. in OpenAIRE Longo, F.; Longo, F.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesLongo, F. in OpenAIRE López-Coto, R.; López-Coto, R.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesLópez-Coto, R. in OpenAIRE López-Moya, M.; López-Moya, M.
Harvested from ORCID Public Data FileLópez-Moya, M. in OpenAIRE López-Oramas, A.; López-Oramas, A.
Harvested from ORCID Public Data FileLópez-Oramas, A. in OpenAIRE Loporchio, S.; Lorini, A.;Loporchio, S.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesLoporchio, S. in OpenAIRE Luque-Escamilla, P. L.; Luque-Escamilla, P. L.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesLuque-Escamilla, P. L. in OpenAIRE Majumdar, P.; Majumdar, P.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesMajumdar, P. in OpenAIRE Larriva, A. Baquero; Larriva, A. Baquero
Harvested from ORCID Public Data FileLarriva, A. Baquero in OpenAIRE Makariev, M.; Makariev, M.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesMakariev, M. in OpenAIRE Mandat, D.; Mandat, D.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesMandat, D. in OpenAIRE Manganaro, M.; Manganaro, M.
Harvested from ORCID Public Data FileManganaro, M. in OpenAIRE Manicò, G.; Manicò, G.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesManicò, G. in OpenAIRE Mannheim, K.; Mannheim, K.
Harvested from ORCID Public Data FileMannheim, K. in OpenAIRE Mariotti, M.; Mariotti, M.
Harvested from ORCID Public Data FileMariotti, M. in OpenAIRE Marquez, P.; Marquez, P.
Harvested from ORCID Public Data FileMarquez, P. in OpenAIRE Marsella, G.; Marsella, G.
Harvested from ORCID Public Data FileMarsella, G. in OpenAIRE Martí, J.; Martí, J.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesMartí, J. in OpenAIRE Martinez, O.; Martinez, O.
Harvested from ORCID Public Data FileMartinez, O. in OpenAIRE Baroncelli, L.; Baroncelli, L.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesBaroncelli, L. in OpenAIRE Martínez, G.; Martínez, G.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesMartínez, G. in OpenAIRE Martínez, M.; Martínez, M.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesMartínez, M. in OpenAIRE Marusevec, P.; Marusevec, P.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesMarusevec, P. in OpenAIRE Mas-Aguilar, A.; Mas-Aguilar, A.
Harvested from ORCID Public Data FileMas-Aguilar, A. in OpenAIRE Maurin, G.; Maurin, G.
Harvested from ORCID Public Data FileMaurin, G. in OpenAIRE Mazin, D.; Guillen, E. Mestre;Mazin, D.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesMazin, D. in OpenAIRE Micanovic, S.; Micanovic, S.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesMicanovic, S. in OpenAIRE Miceli, D.; Miceli, D.
Harvested from ORCID Public Data FileMiceli, D. in OpenAIRE Miener, T.; Miener, T.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesMiener, T. in OpenAIRE de Almeida, U. Barres; de Almeida, U. Barres
Harvested from ORCID Public Data Filede Almeida, U. Barres in OpenAIRE Miranda, J. M.; Miranda, J. M.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesMiranda, J. M. in OpenAIRE Mirzoyan, R.; Mirzoyan, R.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesMirzoyan, R. in OpenAIRE Mizuno, T.; Gonzalez, M. Molero;Mizuno, T.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesMizuno, T. in OpenAIRE Molina, E.; Molina, E.
Harvested from ORCID Public Data FileMolina, E. in OpenAIRE Montaruli, T.; Monteiro, I.;Montaruli, T.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesMontaruli, T. in OpenAIRE Moralejo, A.; Moralejo, A.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesMoralejo, A. in OpenAIRE Morcuende, D.; Morcuende, D.
Harvested from ORCID Public Data FileMorcuende, D. in OpenAIRE Morselli, A.; Morselli, A.
Harvested from ORCID Public Data FileMorselli, A. in OpenAIRE Barrio, J. A.; Barrio, J. A.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesBarrio, J. A. in OpenAIRE Mrakovcic, K.; Mrakovcic, K.
Harvested from ORCID Public Data FileMrakovcic, K. in OpenAIRE Murase, K.; Nagai, A.; Nagataki, S.;Murase, K.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesMurase, K. in OpenAIRE Nakamori, T.; Nakamori, T.
Harvested from ORCID Public Data FileNakamori, T. in OpenAIRE Nickel, L.; Nickel, L.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesNickel, L. in OpenAIRE Nievas, M.; Nievas, M.
Harvested from ORCID Public Data FileNievas, M. in OpenAIRE Nishijima, K.; Nishijima, K.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesNishijima, K. in OpenAIRE Noda, K.; Noda, K.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesNoda, K. in OpenAIRE Nosek, D.; Nosek, D.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesNosek, D. in OpenAIRE Batkovic, I.; Batkovic, I.
Harvested from ORCID Public Data FileBatkovic, I. in OpenAIRE Nozaki, S.; Nozaki, S.
Harvested from ORCID Public Data FileNozaki, S. in OpenAIRE Ohishi, M.; Ohishi, M.
Harvested from ORCID Public Data FileOhishi, M. in OpenAIRE Ohtani, Y.; Ohtani, Y.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesOhtani, Y. in OpenAIRE Oka, T.; Okazaki, N.; Okumura, A.; Orito, R.;Okumura, A.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesOkumura, A. in OpenAIRE Otero-Santos, J.; Otero-Santos, J.
Harvested from ORCID Public Data FileOtero-Santos, J. in OpenAIRE Palatiello, M.; Palatiello, M.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesPalatiello, M. in OpenAIRE Paneque, D.; Abe, S.; Baxter, J.;Paneque, D.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesPaneque, D. in OpenAIRE Pantaleo, F. R.; Pantaleo, F. R.
Harvested from ORCID Public Data FilePantaleo, F. R. in OpenAIRE Paoletti, R.; Paoletti, R.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesPaoletti, R. in OpenAIRE Paredes, J. M.; Paredes, J. M.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesParedes, J. M. in OpenAIRE Pech, M.; Pech, M.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesPech, M. in OpenAIRE Pecimotika, M.; Pecimotika, M.
Harvested from ORCID Public Data FilePecimotika, M. in OpenAIRE Peresano, M.; Peresano, M.
Harvested from ORCID Public Data FilePeresano, M. in OpenAIRE Pérez, A.; Pietropaolo, E.; Pirola, G.;Pietropaolo, E.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesPietropaolo, E. in OpenAIRE Plard, C.; Becerra González, J.; Podobnik, F.; Poireau, V.; Polo, M.; Pons, E.;Poireau, V.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesPoireau, V. in OpenAIRE Prandini, E.; Prandini, E.
Harvested from ORCID Public Data FilePrandini, E. in OpenAIRE Prast, J.; Prast, J.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesPrast, J. in OpenAIRE Principe, G.; Principe, G.
Harvested from ORCID Public Data FilePrincipe, G. in OpenAIRE Priyadarshi, C.; Prouza, M.;Priyadarshi, C.
Harvested from ORCID Public Data FilePriyadarshi, C. in OpenAIRE Rando, R.; Rando, R.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesRando, R. in OpenAIRE Bernardini, E.; Bernardini, E.
Harvested from ORCID Public Data FileBernardini, E. in OpenAIRE Rhode, W.; Ribó, M.; Ribó, M.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesRibó, M. in OpenAIRE Rizi, V.; Fernandez, G. Rodriguez; Ruiz, J. E.; Ruiz, J. E.
Harvested from ORCID Public Data FileRuiz, J. E. in OpenAIRE Saito, T.; Saito, T.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesSaito, T. in OpenAIRE Sakurai, S.; Sanchez, D. A.;Sakurai, S.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesSakurai, S. in OpenAIRE Šarić, T.; Sato, Y.;Šarić, T.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesŠarić, T. in OpenAIRE Bernardos, M. I.; Bernardos, M. I.
Harvested from ORCID Public Data FileBernardos, M. I. in OpenAIRE Saturni, F. G.; Saturni, F. G.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesSaturni, F. G. in OpenAIRE Schleicher, B.; Schmuckermaier, F.; Schubert, J. L.;Schleicher, B.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesSchleicher, B. in OpenAIRE Schussler, F.; Schweizer, T.; Seglar Arroyo, M.; Silvia, R.;Schussler, F.
Harvested from ORCID Public Data FileSchussler, F. in OpenAIRE Sitarek, J.; Sitarek, J.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesSitarek, J. in OpenAIRE Sliusar, V.; Medrano, J. Bernete;Sliusar, V.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesSliusar, V. in OpenAIRE Spolon, A.; Spolon, A.
Harvested from ORCID Public Data FileSpolon, A. in OpenAIRE Strišković, J.; Strišković, J.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesStrišković, J. in OpenAIRE Strzys, M.; Strzys, M.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesStrzys, M. in OpenAIRE Suda, Y.; Sunada, Y.; Sunada, Y.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesSunada, Y. in OpenAIRE Tajima, H.; Tajima, H.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesTajima, H. in OpenAIRE Takahashi, H.; Takahashi, H.
Harvested from ORCID Public Data FileTakahashi, H. in OpenAIRE Takahashi, M.; Takahashi, M.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesTakahashi, M. in OpenAIRE Takata, J.; Takata, J.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesTakata, J. in OpenAIRE Takeishi, R.; Takeishi, R.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesTakeishi, R. in OpenAIRE Berti, A.; Berti, A.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesBerti, A. in OpenAIRE Tam, P. H. T.; Tam, P. H. T.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesTam, P. H. T. in OpenAIRE Tanaka, S. J.; Tanaka, S. J.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesTanaka, S. J. in OpenAIRE Tateishi, D.; Tateishi, D.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesTateishi, D. in OpenAIRE Tejedor, L. A.; Tejedor, L. A.
Harvested from ORCID Public Data FileTejedor, L. A. in OpenAIRE Temnikov, P.; Temnikov, P.
Harvested from ORCID Public Data FileTemnikov, P. in OpenAIRE Terada, Y.; Terada, Y.
Harvested from ORCID Public Data FileTerada, Y. in OpenAIRE Terauchi, K.; Terauchi, K.
Harvested from ORCID Public Data FileTerauchi, K. in OpenAIRE Terzic, T.; Teshima, M.; Tluczykont, M.;Terzic, T.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesTerzic, T. in OpenAIRE Bhattacharjee, P.; Tokanai, F.;Bhattacharjee, P.
Harvested from ORCID Public Data FileBhattacharjee, P. in OpenAIRE Torres, D. F.; Torres, D. F.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesTorres, D. F. in OpenAIRE Travnicek, P.; Truzzi, S.;Travnicek, P.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesTravnicek, P. in OpenAIRE Tutone, A.; Uhlrich, G.;Tutone, A.
Harvested from ORCID Public Data FileTutone, A. in OpenAIRE Vacula, M.; Vallania, P.;Vacula, M.
Harvested from ORCID Public Data FileVacula, M. in OpenAIRE van Scherpenberg, J.; van Scherpenberg, J.
Harvested from ORCID Public Data Filevan Scherpenberg, J. in OpenAIRE Vázquez Acosta, M.; Vázquez Acosta, M.
Harvested from ORCID Public Data FileVázquez Acosta, M. in OpenAIRE Biederbeck, N.; Biederbeck, N.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesBiederbeck, N. in OpenAIRE Verguilov, V.; Verguilov, V.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesVerguilov, V. in OpenAIRE Viale, I.; Viale, I.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesViale, I. in OpenAIRE Vigliano, A.; Vigliano, A.
Harvested from ORCID Public Data FileVigliano, A. in OpenAIRE Vigorito, C. F.; Vigorito, C. F.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesVigorito, C. F. in OpenAIRE Vitale, V.; Voutsinas, G.;Vitale, V.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesVitale, V. in OpenAIRE Vovk, I.; Vovk, I.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesVovk, I. in OpenAIRE Vuillaume, T.; Vuillaume, T.
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesVuillaume, T. in OpenAIRE Walter, R.; Walter, R.
Harvested from ORCID Public Data FileWalter, R. in OpenAIREAbstract 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.
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Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesV. A. Acciari in OpenAIRE I. Agudo; +96 AuthorsI. Agudo
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesI. Agudo in OpenAIREHidetarô Abe; Shoko Abe; V. A. Acciari; V. A. Acciari
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Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesCornelia Arcaro in OpenAIRE Manuel Artero; Manuel Artero
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Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesG. Bonnoli in OpenAIRE Zeljko J. Bosnjak; Zeljko J. Bosnjak
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Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesGiovanni Ceribella in OpenAIRE Yating Chai; Yating Chai
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Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesA. Chilingarian in OpenAIRE Stefan Cikota; Stefan Cikota
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Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesGiacomo D'Amico in OpenAIRE V. D'Elia; V. D'Elia
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Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesF. Dazzi in OpenAIRE A. De Angelis; A. De Angelis
Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesA. De Angelis in OpenAIRE B. De Lotto; B. De Lotto
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Derived by OpenAIRE algorithms or harvested from 3rd party repositoriesH. Kubo in OpenAIREResumen Estudiamos la emisión de banda ancha de Mrk 501 utilizando observaciones de múltiples longitudes de onda de 2017 a 2020 realizadas con una multitud de instrumentos, que involucran, entre otros, MAGIC, Fermi 's Large Area Telescope (LAT), NuSTAR, Swift, GASP-WEBT y el Owens Valley Radio Observatory. Mrk 501 mostró una actividad de banda ancha extremadamente baja, lo que puede ayudar a desentrañar su emisión de referencia. Sin embargo, se detectan variaciones de flujo significativas en todas las bandas de onda, y las más altas ocurren en rayos X y rayos γ de muy alta energía (VHE). Se mide una correlación significativa (>3 σ ) entre los rayos X y los rayos γ de VHE, lo que respalda los escenarios leptónicos para explicar las partes variables de la emisión, también durante la baja actividad. Esto se confirma aún más cuando ampliamos nuestros datos de 2008 a 2020 e identificamos, por primera vez, correlaciones significativas entre el telescopio de rayos X Swift y Fermi-LAT. Además, encontramos correlaciones entre los rayos γ de alta energía y la radio, con un retraso de la radio de más de 100 días, lo que coloca la zona de emisión de rayos γ aguas arriba de las regiones radiobrillantes en el chorro. Además, Mrk 501 mostró una actividad históricamente baja en rayos X y rayos γ VHE desde mediados de 2017 hasta mediados de 2019 con un flujo VHE estable (>0,2 TeV) del 5% de la emisión de la Nebulosa del Cangrejo. La distribución de energía espectral de banda ancha (sed) de este estado bajo de 2 años de duración, la emisión de referencia potencial de Mrk 501, se puede caracterizar con modelos leptónicos de una zona y con modelos (lepto) -hadrónicos que cumplen con las restricciones de flujo de neutrinos de IceCube. Exploramos la evolución temporal del sed hacia el estado bajo, revelando que la emisión de referencia estable puede atribuirse a un choque permanente, y la emisión variable a un choque adicional en expansión o en movimiento. Résumé Nous étudions l'émission à large bande de Mrk 501 à l'aide d'observations multi-longueurs d'onde de 2017 à 2020 effectuées avec une multitude d'instruments, impliquant, entre autres, MAGIC, le Large Area Telescope (LAT) de Fermi, NuSTAR, Swift, GASP-WEBT et l'Owens Valley Radio Observatory. Mrk 501 a montré une activité à large bande extrêmement faible, ce qui peut aider à démêler son émission de base. Néanmoins, des variations de flux significatives sont détectées à toutes les bandes d'ondes, les plus élevées se produisant aux rayons X et aux rayons γ de très haute énergie (VHE). Une corrélation significative (>3 σ ) entre les rayons X et les rayons γ VHE est mesurée, soutenant des scénarios leptoniques pour expliquer les parties variables de l'émission, également en cas de faible activité. Cela est également confirmé lorsque nous étendons nos données de 2008 à 2020 et identifions, pour la première fois, des corrélations significatives entre le télescope à rayons X Swift et Fermi-LAT. Nous trouvons en outre des corrélations entre les rayons γ de haute énergie et la radio, la radio étant en retard de plus de 100 jours, plaçant la zone d'émission des rayons γ en amont des régions radio-brillantes dans le jet. En outre, Mrk 501 a montré une activité historiquement faible dans les rayons X et les rayons γ VHE de mi-2017 à mi-2019 avec un flux VHE stable (>0,2 TeV) de 5% de l'émission de la nébuleuse du Crabe. La distribution d'énergie spectrale à large bande (SED) de cet état bas de 2 ans de long, l'émission de base potentielle de Mrk 501, peut être caractérisée avec des modèles leptoniques à une zone et avec des modèles (lepto)-hadroniques satisfaisant aux contraintes de flux de neutrinos de IceCube. Nous explorons l'évolution temporelle du SED vers l'état bas, révélant que l'émission de base stable peut être attribuée à un choc permanent et l'émission variable à un choc supplémentaire en expansion ou en déplacement. Abstract We study the broadband emission of Mrk 501 using multiwavelength observations from 2017 to 2020 performed with a multitude of instruments, involving, among others, MAGIC, Fermi's Large Area Telescope (LAT), NuSTAR, Swift, GASP-WEBT, and the Owens Valley Radio Observatory. Mrk 501 showed an extremely low broadband activity, which may help to unravel its baseline emission. Nonetheless, significant flux variations are detected at all wave bands, with the highest occurring at X-rays and very-high-energy (VHE) γ -rays. A significant correlation (>3 σ ) between X-rays and VHE γ -rays is measured, supporting leptonic scenarios to explain the variable parts of the emission, also during low activity. This is further supported when we extend our data from 2008 to 2020, and identify, for the first time, significant correlations between the Swift X-Ray Telescope and Fermi-LAT. We additionally find correlations between high-energy γ -rays and radio, with the radio lagging by more than 100 days, placing the γ -ray emission zone upstream of the radio-bright regions in the jet. Furthermore, Mrk 501 showed a historically low activity in X-rays and VHE γ -rays from mid-2017 to mid-2019 with a stable VHE flux (>0.2 TeV) of 5% the emission of the Crab Nebula. The broadband spectral energy distribution (SED) of this 2 yr long low state, the potential baseline emission of Mrk 501, can be characterized with one-zone leptonic models, and with (lepto)-hadronic models fulfilling neutrino flux constraints from IceCube. We explore the time evolution of the SED toward the low state, revealing that the stable baseline emission may be ascribed to a standing shock, and the variable emission to an additional expanding or traveling shock. ندرس انبعاث النطاق العريض لـ MRK 501 باستخدام ملاحظات متعددة الأطوال الموجية من 2017 إلى 2020 التي يتم إجراؤها باستخدام العديد من الأدوات، والتي تشمل، من بين أمور أخرى، MAGIC، وتلسكوب فيرمي واسع النطاق (LAT)، و NuSTAR، و SWIFT، و GASP - WEBT، ومرصد أوينز فالي الراديوي. أظهر MRK 501 نشاطًا منخفضًا للغاية للنطاق العريض، مما قد يساعد في كشف انبعاثه الأساسي. ومع ذلك، يتم الكشف عن اختلافات كبيرة في التدفق في جميع نطاقات الموجة، مع حدوث أعلىها في الأشعة السينية وأشعة γ عالية الطاقة للغاية (VHE). يتم قياس ارتباط كبير (>3 σ ) بين الأشعة السينية وأشعة VHE γ، مما يدعم السيناريوهات اللبتونية لشرح الأجزاء المتغيرة من الانبعاث، أيضًا أثناء النشاط المنخفض. يتم دعم ذلك بشكل أكبر عندما نوسع بياناتنا من 2008 إلى 2020، ونحدد، لأول مرة، الارتباطات المهمة بين تلسكوب Swift X - Ray و Fermi - LAT. بالإضافة إلى ذلك، نجد ارتباطات بين أشعة جاما عالية الطاقة والراديو، حيث يتخلف الراديو بأكثر من 100 يوم، مما يضع منطقة انبعاث أشعة جاما في المنبع لمناطق الإشعاع الراديوي في الطائرة. علاوة على ذلك، أظهر Mrk 501 نشاطًا منخفضًا تاريخيًا في الأشعة السينية وأشعة VHE γ من منتصف عام 2017 إلى منتصف عام 2019 مع تدفق ثابت لـ VHE (>0.2 TeV) بنسبة 5 ٪ من انبعاث سديم السرطان. يمكن تمييز توزيع الطاقة الطيفية عريضة النطاق (SED) لهذه الحالة المنخفضة لمدة عامين، وهو الانبعاث الأساسي المحتمل لـ Mrk 501، بنماذج لبتونية من منطقة واحدة، وبنماذج (لبتو) - متناظرية تفي بقيود تدفق النيوترينو من IceCube. نستكشف التطور الزمني لـ SED نحو الحالة المنخفضة، مما يكشف عن أن انبعاث خط الأساس المستقر قد يعزى إلى صدمة دائمة، والانبعاث المتغير إلى صدمة إضافية متوسعة أو متنقلة.
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Powered by BIP!add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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You have already added works in your ORCID record related to the merged Research product.<script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.60692/gcryz-5j603&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.eu - EC| CTA-PP ,EC| CTA-DEV ,EC| ESCAPE ,EC| INFIERIAbe, Kazuki; Abe, Shotaro; Asano, Katsuaki; Grau Haro, Roger; Green, Jarred Gershon; Green, David; Gunji, Shuichi; Günther, Patrick; Hackfeld, Jonas; Hadasch, Daniela; Hahn, Alexander; Hashiyama, Kazuaki; Hassan, Tarek; Aubert, Pierre; Hayashi, Kohei; Heckmann, Lea; Heller, Matthieu; Herrera Llorente, Javier; Hirotani, Kouichi; Hoffmann, Dirk; Horns, Dieter; Houles, Julien; Hrabovsky, Miroslav; Hrupec, Dario; Baktash, Ali; Hui, David; Hütten, Moritz;
Hassan, Tarek
Harvested from ORCID Public Data FileHassan, Tarek in OpenAIRE Iarlori, Marco; Imazawa, Ryo; Inada, Tomohiro; Inome, Yusuke; Ioka, Kunihito; Iori, Maurizio; Ishio, Kazuma; Jiménez Martínez, Irene; Bamba, Aya; Jurysek, Jakub; Kagaya, Mika; Karas, Vladimir; Katagiri, Hideaki; Kataoka, Jun; Kerszberg, Daniel; Kobayashi, Yukiho; Kohri, Kazunori; Kong, Albert; Kubo, Hidetoshi;Iarlori, Marco
Harvested from ORCID Public Data FileIarlori, Marco in OpenAIRE Baquero Larriva, Andres; Kushida, Junko;Baquero Larriva, Andres
Harvested from ORCID Public Data FileBaquero Larriva, Andres in OpenAIRE Lainez, Maria; Lamanna, Giovanni; Lamastra, Alessandra; Le Flour, Thierry; Linhoff, Maximilian; Longo, Francesco; López-Coto, Rubén; López-Oramas, Alicia; Loporchio, Serena; Baroncelli, Leonardo; Lorini, Andrea; Lozano Bahilo, Julio; Luque-Escamilla, Pedro L.; Majumdar, Pratik; MAKARIEV, Martin; Mandat, Dusan;Lainez, Maria
Harvested from ORCID Public Data FileLainez, Maria in OpenAIRE Manganaro, Marina; Manicò, Giulio; Mannheim, Karl; Mariotti, Mosè; Barres de Almeida, Ulisses; Marquez, Patricia;Manganaro, Marina
Harvested from ORCID Public Data FileManganaro, Marina in OpenAIRE Marsella, Giovanni; Martí, Josep;Marsella, Giovanni
Harvested from ORCID Public Data FileMarsella, Giovanni in OpenAIRE Martinez, Oibar; Martínez, Gustavo; Martínez, Manel; Mas-Aguilar, Alvaro; Maurin, Gilles; Mazin, Daniel; Mestre Guillen, Enrique; Barrio, Juan Abel; Mićanović, Saša;Martinez, Oibar
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Harvested from ORCID Public Data FileNozaki, Seiya in OpenAIRE Bernardini, Elisa; Pietropaolo, Ermanno; Pirola, Giorgio; Plard, Cyann; Podobnik, Franjo; Poireau, Vincent; Polo, Miguel; Pons, Estelle; Prandini, Elisa; Prast, Julie; Principe, Giacomo; Bernardos, Mabel;Bernardini, Elisa
Harvested from ORCID Public Data FileBernardini, Elisa in OpenAIRE Priyadarshi, Chaitanya; Prouza, Michael; Rando, Riccardo; Rhode, Wolgang; Ribó, Marc; Righi, Chiara;Priyadarshi, Chaitanya
Harvested from ORCID Public Data FilePriyadarshi, Chaitanya in OpenAIRE Rizi, Vincenzo; Rodriguez Fernandez, Gonzalo; Rodríguez Frías, Maria Dolores; Saito, Takayuki; Bernete Medrano, Juan; Sakurai, Shunsuke; Sanchez, David; Šarić, Toni; Sato, Yuri; Saturni, Francesco Gabriele; Savchenko, Volodymyr; Schleicher, Bernd; Schmuckermaier, Felix; Schubert, Jan Lukas; Schüssler, Fabian; Berti, Alessio; Schweizer, Thomas; Seglar Arroyo, Monica; Siegert, Thomas; Silvia, Rainò; Sitarek, Julian; Sliusar, Vitalii; Spolon, Alessia;Rizi, Vincenzo
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Harvested from ORCID Public Data FileBhattacharjee, Pooja in OpenAIRE Terauchi, Kenta; Terzić, Tomislav; Teshima, Masahiro; Tluczykont, Martin; Tokanai, Fuyuki; Torres, Diego F.; Travnicek, Petr; Truzzi, Stefano; Tutone, Antonio;Terauchi, Kenta
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Harvested from ORCID Public Data Filevan Scherpenberg, Juliane in OpenAIRE Vigliano, Alessandro; Vigorito, Carlo francesco; Vitale, Vincenzo; Voutsinas, Georgios Gerasimos; Vovk, Ievgen;Vigliano, Alessandro
Harvested from ORCID Public Data FileVigliano, Alessandro in OpenAIREThe next-generation ground-based gamma-ray Cherenkov Telescope Array Observatory (CTAO) will consist of imaging atmospheric Cherenkov telescopes (IACTs) of three different sizes distributed in two sites. The Large-Sized Telescopes will cover the low-energy end of the CTA energy range, starting at about 20 GeV. After its first years of operation at the CTA northern site, the Large-Sized Telescope prototype (LST-1) is in the final stage of its commissioning phase, having collected a significant amount of scientific data to date. In this contribution, we present the physics performance of the telescope using low-zenith Crab Nebula observations and Monte Carlo simulations fine-tuned accordingly. We show performance figures of merit such as the energy threshold, effective area, energy and angular resolution, and sensitivity based on the standard Hillas-parameters approach and following the source-independent and dependent analysis methods. The analysis threshold is estimated at 30 GeV. The energy resolution is around 30%, and the angular resolution is 0.3 degrees at 100 GeV. The best integral sensitivity of LST-1 is about 1.1% of the Crab Nebula flux above 250 GeV for 50 hours of observations. We also show the spectral energy distribution and light curve from Crab Nebula observations, which agree with results from other IACTs and link smoothly with Fermi-LAT when considering statistical and systematic uncertainties near the energy threshold. Presented at the 38th International Cosmic Ray Conference (ICRC 2023), 2023 (arXiv:2309.08219)
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