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  Observations of the Crab Nebula and Pulsar with the Large-Sized Telescope Prototype of the Cherenkov Telescope Array

Project, C.-L., Abe, H., Abe, K., Abe, S., Aguasca-Cabot, A., Agudo, I., Alvarez Crespo, N., Antonelli, L., Aramo, C., Arbet-Engels, A., Arcaro, C., Artero, M., Asano, K., Aubert, P., Baktash, A., Bamba, A., Baquero Larriva, A., Baroncelli, L., Barres de Almeida, U., Barrio, J., Batkovic, I., Baxter, J., Becerra González, J., Bernardini, E., Bernardos, M., Bernete Medrano, J., Berti, A., Bhattacharjee, P., Biederbeck, N., Bigongiari, C., Bissaldi, E., Blanch, O., Bonnoli, G., Bordas, P., Borghese, A., Bulgarelli, A., Burelli, I., Buscemi, M., Cardillo, M., Caroff, S., Carosi, A., Cassol, F., Cauz, D., Ceribella, G., Chai, Y., Cheng, K., Chiavassa, A., Chikawa, M., Chytka, L., Cifuentes, A., Contreras, J., Cortina, J., Costantini, H., D'Amico, G., Dalchenko, M., De Angelis, A., de Bony de Lavergne, M., De Lotto, B., de Menezes, R., Deleglise, G., Delgado, C., Delgado Mengual, J., della Volpe, D., Dellaiera, M., Depaoli, D., Di Piano, A., Di Pierro, F., Di Tria, R., Di Venere, L., Díaz, C., Dominik, R., Dominis Prester, D., Donini, A., Dorner, D., Doro, M., Elsässer, D., Emery, G., Escudero, J., Fallah Ramazani, V., Ferrara, G., Ferrarotto, F., Fiasson, A., Freixas Coromina, L., Fröse, S., Fukami, S., Fukazawa, Y., Garcia, E., Garcia López, R., Gasbarra, C., Gasparrini, D., Geyer, F., Giesbrecht Paiva, J., Giglietto, N., Giordano, F., Giro, E., Gliwny, P., Godinovic, N., Grau, R., Green, D., Green, J., Gunji, S., Hackfeld, J., Hadasch, D., Hahn, A., Hashiyama, K., Hassan, T., Hayashi, K., Heckmann, L., Heller, M., Herrera Llorente, J., Hirotani, K., Hoffmann, D., Horns, D., Houles, J., Hrabovsky, M., Hrupec, D., Hui, D., Hütten, M., Iarlori, M., Imazawa, R., Inada, T., Inome, Y., Ioka, K., Iori, M., Ishio, K., Iwamura, Y., Jacquemont, M., Jimenez Martinez, I., Jurysek, J., Kagaya, M., Karas, V., Katagiri, H., Kataoka, J., Kerszberg, D., Kobayashi, Y., Kong, A., Kubo, H., Kushida, J., Lainez, M., Lamanna, G., Lamastra, A., Le Flour, T., Linhoff, M., Longo, F., López-Coto, R., López-Moya, M., López-Oramas, A., Loporchio, S., Lorini, A., Luque-Escamilla, P., Majumdar, P., Makariev, M., Mandat, D., Manganaro, M., Manicò, G., Mannheim, K., Mariotti, M., Marquez, P., Marsella, G., Martí, J., Martinez, O., Martínez, G., Martínez, M., Marusevec, P., Mas-Aguilar, A., Maurin, G., Mazin, D., Mestre Guillen, E., Micanovic, S., Miceli, D., Miener, T., Miranda, J., Mirzoyan, R., Mizuno, T., Molero Gonzalez, M., Molina, E., Montaruli, T., Monteiro, I., Moralejo, A., Morcuende, D., Morselli, A., Mrakovcic, K., Murase, K., Nagai, A., Nagataki, S., Nakamori, T., Nickel, L., Nievas, M., Nishijima, K., Noda, K., Nosek, D., Nozaki, S., Ohishi, M., Ohtani, Y., Oka, T., Okazaki, N., Okumura, A., Orito, R., Otero-Santos, J., Palatiello, M., Paneque, D., Pantaleo, F., Paoletti, R., Paredes, J., Pech, M., Pecimotika, M., Peresano, M., Pérez, A., Pietropaolo, E., Pirola, G., Plard, C., Podobnik, F., Poireau, V., Polo, M., Pons, E., Prandini, E., Prast, J., Principe, G., Priyadarshi, C., Prouza, M., Rando, R., Rhode, W., Ribó, M., Rizi, V., Rodriguez Fernandez, G., Ruiz, J., Saito, T., Sakurai, S., Sanchez, D., Šarić, T., Sato, Y., Saturni, F., Schleicher, B., Schmuckermaier, F., Schubert, J., Schussler, F., Schweizer, T., Seglar Arroyo, M., Silvia, R., Sitarek, J., Sliusar, V., Spolon, A., Strišković, J., Strzys, M., Suda, Y., Sunada, Y., Tajima, H., Takahashi, H., Takahashi, M., Takata, J., Takeishi, R., Tam, P., Tanaka, S., Tateishi, D., Tejedor, L., Temnikov, P., Terada, Y., Terauchi, K., Terzic, T., Teshima, M., Tluczykont, M., Tokanai, F., Torres, D., Travnicek, P., Truzzi, S., Tutone, A., Uhlrich, G., Vacula, M., Vallania, P., van Scherpenberg, J., Vázquez Acosta, M., Verguilov, V., Viale, I., Vigliano, A., Vigorito, C., Vitale, V., Voutsinas, G., Vovk, I., Vuillaume, T., Walter, R., Will, M., Yamamoto, T., Yamazaki, R., Yoshida, T., Yoshikoshi, T., Zywucka, N., Bernloehr, K., Gueta, O., Kosack, K., Maier, G., Watson, J., Rijeka, U. o., Physics, D. o., Rijeka, Croatia, Physics, I. f. T., Astrophysics, Würzburg, U., Nord, C. H., Würzburg, Germany, Physik, I. f. T., IV, L., Plasma-Astroteilchenphysik, Bochum, R.-U., Bochum, Germany, Sapienza, I. S. d. R. L., Rome, Italy, ILANCE, Laboratory, C.-.-U.-o.-T.-I.-R., Kashiwa, Chiba, Japan, Program, P., Science, G. S. o. A., Engineering, University, H., Hiroshima, Japan, Vergata, I. S. d. R. T., Rome, Italy, Physics, F. o., Informatics, A., Lodz, U. o., Lodz, Poland, Split, U. o., FESB, Split, Croatia, Physics, D. o., University, Y., Yamagata, Japan, University, T., Institute, A., Aobaku, Sendai, Japan, Osijek, J. J. S. U. o., Physics, D. o., Osijek, Croatia, dell'Aquila, I.-D.-d.-S.-F.-e.-C.-.-U.-d.-S., Institute, G. S. S., L'Aquila, Italy, Oiwakecho, K., Kyoto, Japan, Astronomy, D. o., Geneva, U. o., Versoix, Switzerland, Sciences, A. I. o. t. C. A. o., Prague, Republic, C., Science, F. o., University, I., Mito, Ibaraki, Japan, Science, F. o., Engineering, University, W., Shinjuku, Tokyo, Japan, Trieste, I. S. d., Trieste, U. d. S. d., Trieste, Italy, INFN, Siena, U. d. S. d., Fisiche, D. d. S., dell'Ambiente, d. T. e., Fisica, S. d., Siena, Italy, Jaén, E. P. S. d., Jaén, U. d., Lagunillas, C. L., Jaén, Spain, Physics, S. I. o. N., Bidhannagar, Kolkata, India, Research, I. f. N., Energy, N., Sciences, B. A. o., Sofia, Bulgaria, Sciences, F.-.-I.-o.-P.-o.-t.-C.-A.-o., Praha, Republic, C., Segrè' Università degli Studi di Palermo, D. d. F. e. C. '., Scienze, v. d., Palermo, Electronica, G. d., Madrid, U. C. d., Complutense, A., Madrid, Spain, Physics, D. o. A., Zagreb, U. o., Zagreb, Croatia, Center, H. A. S., University, H., Higashi-Hiroshima, Hiroshima, Japan, RIKEN, Physical, I. o., Research, C., Wako, Saitama, Japan, University, C., Particle, I. o., Physics, N., Prague, Republic, C., Physics, D. o., Astronomy, Science, G. S. o., University, K., Sakyo-ku, Kyoto, Japan, Research, I.-f.-S.-E.-E., University, N., Chikusa-ku, Nagoya, Japan, Institute, K.-M., Particles, O. o., Universe, University, N., Chikusa-ku, Nagoya, Japan, Technology, G. S. o., Industrial, Sciences, S., University, T., Tokushima, Japan, dell'Aquila, I.-D.-d.-S.-F.-e.-C.-.-U.-d.-S., Institute, G. S. S., L'Aquila, Italy, Sciences, D. o. P., University, A. G., Fuchinobe, Sagamihara, Kanagawa, Japan, IRFU, Paris-Saclay, U., Gif-sur-Yvette, France, Science, G. S. o., Engineering, University, S., Sakura-ku, city, S., Saitama, Japan, Torino, D.-d.-F.-.-U.-d.-S.-d., Torino, Italy, Physics, D. o., University, K., Kobe, Hyogo, Japan), Heidelberg, Germany, Zeuthen, Germany, Saclay, C., Merisiers, O. d., Gif-sur-Yvette, & France), (2023). Observations of the Crab Nebula and Pulsar with the Large-Sized Telescope Prototype of the Cherenkov Telescope Array. Astrophysical Journal, 956, 80. doi:10.3847/1538-4357/ace89d.

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アイテムのパーマリンク: https://hdl.handle.net/21.11116/0000-000F-125E-4 版のパーマリンク: https://hdl.handle.net/21.11116/0000-000F-125F-3
資料種別: 学術論文

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 作成者:
Project, CTA-LST1, 著者
Abe, H.1, 著者
Abe, K.1, 著者
Abe, S.1, 著者
Aguasca-Cabot, A.1, 著者
Agudo, I.1, 著者
Alvarez Crespo, N.1, 著者
Antonelli, L.A.1, 著者
Aramo, C.1, 著者
Arbet-Engels, A.1, 著者
Arcaro, C.1, 著者
Artero, M.1, 著者
Asano, K.1, 著者
Aubert, P.1, 著者
Baktash, A.1, 著者
Bamba, A.1, 著者
Baquero Larriva, A.1, 著者
Baroncelli, L.1, 著者
Barres de Almeida, U.1, 著者
Barrio, J.A.1, 著者
Batkovic, I.1, 著者Baxter, J.1, 著者Becerra González, J.1, 著者Bernardini, E.1, 著者Bernardos, M.I.1, 著者Bernete Medrano, J.1, 著者Berti, A.1, 著者Bhattacharjee, P.1, 著者Biederbeck, N.1, 著者Bigongiari, C.1, 著者Bissaldi, E.1, 著者Blanch, O.1, 著者Bonnoli, G.1, 著者Bordas, P.1, 著者Borghese, A.1, 著者Bulgarelli, A.1, 著者Burelli, I.1, 著者Buscemi, M.1, 著者Cardillo, M.1, 著者Caroff, S.1, 著者Carosi, A.1, 著者Cassol, F.1, 著者Cauz, D.1, 著者Ceribella, G.1, 著者Chai, Y.1, 著者Cheng, K.1, 著者Chiavassa, A.1, 著者Chikawa, M.1, 著者Chytka, L.1, 著者Cifuentes, A.1, 著者Contreras, J.L.1, 著者Cortina, J.1, 著者Costantini, H.1, 著者D'Amico, G.1, 著者Dalchenko, M.1, 著者De Angelis, A.1, 著者de Bony de Lavergne, M.1, 著者De Lotto, B.1, 著者de Menezes, R.1, 著者Deleglise, G.1, 著者Delgado, C.1, 著者Delgado Mengual, J.1, 著者della Volpe, D.1, 著者Dellaiera, M.1, 著者Depaoli, D.1, 著者Di Piano, A.1, 著者Di Pierro, F.1, 著者Di Tria, R.1, 著者Di Venere, L.1, 著者Díaz, C.1, 著者Dominik, R.M.1, 著者Dominis Prester, D.1, 著者Donini, A.1, 著者Dorner, D.1, 著者Doro, M.1, 著者Elsässer, D.1, 著者Emery, G.1, 著者Escudero, J.1, 著者Fallah Ramazani, V.1, 著者Ferrara, G.1, 著者Ferrarotto, F.1, 著者Fiasson, A.1, 著者Freixas Coromina, L.1, 著者Fröse, S.1, 著者Fukami, S.1, 著者Fukazawa, Y.1, 著者Garcia, E.1, 著者Garcia López, R.1, 著者Gasbarra, C.1, 著者Gasparrini, D.1, 著者Geyer, F.1, 著者Giesbrecht Paiva, J.1, 著者Giglietto, N.1, 著者Giordano, F.1, 著者Giro, E.1, 著者Gliwny, P.1, 著者Godinovic, N.1, 著者Grau, R.1, 著者Green, D.1, 著者Green, J.1, 著者Gunji, S.1, 著者Hackfeld, J.1, 著者Hadasch, D.1, 著者Hahn, A.1, 著者Hashiyama, K.1, 著者Hassan, T.1, 著者Hayashi, K.1, 著者Heckmann, L.1, 著者Heller, M.1, 著者Herrera Llorente, J.1, 著者Hirotani, K.1, 著者Hoffmann, D.1, 著者Horns, D.1, 著者Houles, J.1, 著者Hrabovsky, M.1, 著者Hrupec, D.1, 著者Hui, D.1, 著者Hütten, M.1, 著者Iarlori, M.1, 著者Imazawa, R.1, 著者Inada, T.1, 著者Inome, Y.1, 著者Ioka, K.1, 著者Iori, M.1, 著者Ishio, K.1, 著者Iwamura, Y.1, 著者Jacquemont, M.1, 著者Jimenez Martinez, I.1, 著者Jurysek, J.1, 著者Kagaya, M.1, 著者Karas, V.1, 著者Katagiri, H.1, 著者Kataoka, J.1, 著者Kerszberg, D.1, 著者Kobayashi, Y.1, 著者Kong, A.1, 著者Kubo, H.1, 著者Kushida, J.1, 著者Lainez, M.1, 著者Lamanna, G.1, 著者Lamastra, A.1, 著者Le Flour, T.1, 著者Linhoff, M.1, 著者Longo, F.1, 著者López-Coto, R.1, 著者López-Moya, M.1, 著者López-Oramas, A.1, 著者Loporchio, S.1, 著者Lorini, A.1, 著者Luque-Escamilla, P.L.1, 著者Majumdar, P.1, 著者Makariev, M.1, 著者Mandat, D.1, 著者Manganaro, M.1, 著者Manicò, G.1, 著者Mannheim, K.1, 著者Mariotti, M.1, 著者Marquez, P.1, 著者Marsella, G.1, 著者Martí, J.1, 著者Martinez, O.1, 著者Martínez, G.1, 著者Martínez, M.1, 著者Marusevec, P.1, 著者Mas-Aguilar, A.1, 著者Maurin, G.1, 著者Mazin, D.1, 著者Mestre Guillen, E.1, 著者Micanovic, S.1, 著者Miceli, D.1, 著者Miener, T.1, 著者Miranda, J.M.1, 著者Mirzoyan, R.1, 著者Mizuno, T.1, 著者Molero Gonzalez, M.1, 著者Molina, E.1, 著者Montaruli, T.1, 著者Monteiro, I.1, 著者Moralejo, A.1, 著者Morcuende, D.1, 著者Morselli, A.1, 著者Mrakovcic, K.1, 著者Murase, K.1, 著者Nagai, A.1, 著者Nagataki, S.1, 著者Nakamori, T.1, 著者Nickel, L.1, 著者Nievas, M.1, 著者Nishijima, K.1, 著者Noda, K.1, 著者Nosek, D.1, 著者Nozaki, S.1, 著者Ohishi, M.1, 著者Ohtani, Y.1, 著者Oka, T.1, 著者Okazaki, N.1, 著者Okumura, A.1, 著者Orito, R.1, 著者Otero-Santos, J.1, 著者Palatiello, M.1, 著者Paneque, D.1, 著者Pantaleo, F.R.1, 著者Paoletti, R.1, 著者Paredes, J.M.1, 著者Pech, M.1, 著者Pecimotika, M.1, 著者Peresano, M.1, 著者Pérez, A.1, 著者Pietropaolo, E.1, 著者Pirola, G.1, 著者Plard, C.1, 著者Podobnik, F.1, 著者Poireau, V.1, 著者Polo, M.1, 著者Pons, E.1, 著者Prandini, E.1, 著者Prast, J.1, 著者Principe, G.1, 著者Priyadarshi, C.1, 著者Prouza, M.1, 著者Rando, R.1, 著者Rhode, W.1, 著者Ribó, M.1, 著者Rizi, V.1, 著者Rodriguez Fernandez, G.1, 著者Ruiz, J.E.1, 著者Saito, T.1, 著者Sakurai, S.1, 著者Sanchez, D.A.1, 著者Šarić, T.1, 著者Sato, Y.1, 著者Saturni, F.G.1, 著者Schleicher, B.1, 著者Schmuckermaier, F.1, 著者Schubert, J.L.1, 著者Schussler, F.1, 著者Schweizer, T.1, 著者Seglar Arroyo, M.1, 著者Silvia, R.1, 著者Sitarek, J.1, 著者Sliusar, V.1, 著者Spolon, A.1, 著者Strišković, J.1, 著者Strzys, M.1, 著者Suda, Y.1, 著者Sunada, Y.1, 著者Tajima, H.1, 著者Takahashi, H.1, 著者Takahashi, M.1, 著者Takata, J.1, 著者Takeishi, R.1, 著者Tam, P.H.T.1, 著者Tanaka, S.J.1, 著者Tateishi, D.1, 著者Tejedor, L.A.1, 著者Temnikov, P.1, 著者Terada, Y.1, 著者Terauchi, K.1, 著者Terzic, T.1, 著者Teshima, M.1, 著者Tluczykont, M.1, 著者Tokanai, F.1, 著者Torres, D.F.1, 著者Travnicek, P.1, 著者Truzzi, S.1, 著者Tutone, A.1, 著者Uhlrich, G.1, 著者Vacula, M.1, 著者Vallania, P.1, 著者van Scherpenberg, J.1, 著者Vázquez Acosta, M.1, 著者Verguilov, V.1, 著者Viale, I.1, 著者Vigliano, A.1, 著者Vigorito, C.F.1, 著者Vitale, V.1, 著者Voutsinas, G.1, 著者Vovk, I.1, 著者Vuillaume, T.1, 著者Walter, R.1, 著者Will, M.1, 著者Yamamoto, T.1, 著者Yamazaki, R.1, 著者Yoshida, T.1, 著者Yoshikoshi, T.1, 著者Zywucka, N.1, 著者Bernloehr, K.1, 著者Gueta, O.1, 著者Kosack, K.1, 著者Maier, G.1, 著者Watson, J.1, 著者Rijeka, University of1, 著者Physics, Department of1, 著者Rijeka1, 著者Croatia1, 著者Physics, Institute for Theoretical1, 著者Astrophysics1, 著者Würzburg, Universität1, 著者Nord, Campus Hubland1, 著者Würzburg1, 著者Germany1, 著者Physik, Institut für Theoretische1, 著者IV, Lehrstuhl1, 著者Plasma-Astroteilchenphysik1, 著者Bochum, Ruhr-Universität1, 著者Bochum1, 著者Germany1, 著者Sapienza, INFN Sezione di Roma La1, 著者Rome1, 著者Italy1, 著者ILANCE1, 著者Laboratory, CNRS - 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Università degli Studi1, 著者Institute, Gran Sasso Science1, 著者L'Aquila1, 著者Italy1, 著者Sciences, Department of Physical1, 著者University, Aoyama Gakuin1, 著者Fuchinobe1, 著者Sagamihara1, 著者Kanagawa1, 著者Japan1, 著者IRFU1, 著者Paris-Saclay, Université1, 著者Gif-sur-Yvette1, 著者France1, 著者Science, Graduate School of1, 著者Engineering1, 著者University, Saitama1, 著者Sakura-ku1, 著者city, Saitama1, 著者Saitama1, 著者Japan1, 著者Torino, Dipartimento di Fisica - Universitá degli Studi di1, 著者Torino1, 著者Italy1, 著者Physics, Department of1, 著者University, Konan1, 著者Kobe1, 著者Hyogo1, 著者Japan)1, 著者Heidelberg1, 著者Germany1, 著者Zeuthen1, 著者Germany1, 著者Saclay, CEA1, 著者Merisiers, Orme des1, 著者Gif-sur-Yvette1, 著者France)1, 著者 全て表示
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1Max Planck Institute for Physics, Max Planck Society and Cooperation Partners, ou_2253650              

内容説明

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キーワード: CTA
 要旨: CTA (Cherenkov Telescope Array) is the next generation ground-based observatory for gamma-ray astronomy at very-high energies. The Large-Sized Telescope prototype (LST-1) is located at the Northern site of CTA, 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 $\simeq 20$ GeV. LST-1 started performing astronomical observations in November 2019, during its commissioning phase, and it has been taking data since then. 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 basic performance parameters of the telescope. The data sample consists of around 36 hours of observations at low zenith angles collected between November 2020 and March 2022. 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 behavior. The energy threshold at trigger level is estimated to be around 20 GeV, rising to $\simeq 30$ 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 to 0.40 degrees, and energy resolution from 15 to 50%. Flux sensitivity is around 1.1% of the Crab Nebula flux above 250 GeV for a 50-h 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.

資料詳細

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 日付: 2023
 出版の状態: 出版
 ページ: -
 出版情報: -
 目次: -
 査読: -
 識別子（DOI, ISBNなど）: その他: MPP-2023-372
URI: https://publications.mppmu.mpg.de/?action=search&mpi=MPP-2023-372
arXiv: arxiv:2306.12960
DOI: 10.3847/1538-4357/ace89d
URI: https://inspirehep.net/arxiv/2306.12960
 学位: -

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出版物 1

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出版物名: Astrophysical Journal
  省略形 : Astrophys.J.
種別: 学術雑誌
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ページ: - 巻号: 956 通巻号: - 開始・終了ページ: 80 識別子（ISBN, ISSN, DOIなど）: -