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001     596676
005     20250715173144.0
024 7 _ |a 10.1093/mnras/stad1576
|2 doi
024 7 _ |a CherenkovTelescopeArray:2023aqu
|2 INSPIRETeX
024 7 _ |a inspire:2663083
|2 inspire
024 7 _ |a 0035-8711
|2 ISSN
024 7 _ |a 1365-2966
|2 ISSN
024 7 _ |a 1365-8711
|2 ISSN
024 7 _ |a arXiv:2305.16707
|2 arXiv
024 7 _ |a altmetric:149068781
|2 altmetric
024 7 _ |a WOS:001023895800033
|2 WOS
024 7 _ |2 openalex
|a openalex:W4378446371
037 _ _ |a PUBDB-2023-06222
041 _ _ |a English
082 _ _ |a 520
088 _ _ |a arXiv:2305.16707
|2 arXiv
100 1 _ |a Acharyya, A.
|b 0
245 _ _ |a Sensitivity of the Cherenkov Telescope Array to TeV photon emission from the Large Magellanic Cloud
260 _ _ |a Oxford
|c 2023
|b Oxford Univ. Press
336 7 _ |a article
|2 DRIVER
336 7 _ |a Output Types/Journal article
|2 DataCite
336 7 _ |a Journal Article
|b journal
|m journal
|0 PUB:(DE-HGF)16
|s 1697547636_3725953
|2 PUB:(DE-HGF)
336 7 _ |a ARTICLE
|2 BibTeX
336 7 _ |a JOURNAL_ARTICLE
|2 ORCID
336 7 _ |a Journal Article
|0 0
|2 EndNote
500 _ _ |a Accepted for publication in MNRAS. Corresponding authors: Pierrick Martin, Maria Isabel Bernardos Martin, Fabio IoccoWaiting for fulltext
520 _ _ |a A deep survey of the Large Magellanic Cloud at ~0.1-100TeV photon energies with the Cherenkov Telescope Array is planned. We assess the detection prospects based on a model for the emission of the galaxy, comprising the four known TeV emitters, mock populations of sources, and interstellar emission on galactic scales. We also assess the detectability of 30 Doradus and SN 1987A, and the constraints that can be derived on the nature of dark matter. The survey will allow for fine spectral studies of N157B, N132D, LMC P3, and 30 Doradus C, and half a dozen other sources should be revealed, mainly pulsar-powered objects. The remnant from SN 1987A could be detected if it produces cosmic-ray nuclei with a flat power-law spectrum at high energies, or with a steeper index 2.3-2.4 pending a flux increase by a factor >3-4 over ~2015-2035. Large-scale interstellar emission remains mostly out of reach of the survey if its >10GeV spectrum has a soft photon index ~2.7, but degree-scale 0.1-10TeV pion-decay emission could be detected if the cosmic-ray spectrum hardens above >100GeV. The 30 Doradus star-forming region is detectable if acceleration efficiency is on the order of 1-10% of the mechanical luminosity and diffusion is suppressed by two orders of magnitude within <100pc. Finally, the survey could probe the canonical velocity-averaged cross section for self-annihilation of weakly interacting massive particles for cuspy Navarro-Frenk-White profiles.
536 _ _ |a 613 - Matter and Radiation from the Universe (POF4-613)
|0 G:(DE-HGF)POF4-613
|c POF4-613
|f POF IV
|x 0
588 _ _ |a Dataset connected to CrossRef, INSPIRE, Journals: bib-pubdb1.desy.de
650 _ 7 |a photon: energy
|2 INSPIRE
650 _ 7 |a acceleration: efficiency
|2 INSPIRE
650 _ 7 |a energy: high
|2 INSPIRE
650 _ 7 |a photon: emission
|2 INSPIRE
650 _ 7 |a nucleus: cosmic radiation
|2 INSPIRE
650 _ 7 |a cosmic radiation: spectrum
|2 INSPIRE
650 _ 7 |a Cherenkov Telescope Array
|2 INSPIRE
650 _ 7 |a gamma ray: emission
|2 INSPIRE
650 _ 7 |a galaxy
|2 INSPIRE
650 _ 7 |a TeV
|2 INSPIRE
650 _ 7 |a spectral
|2 INSPIRE
650 _ 7 |a diffusion
|2 INSPIRE
650 _ 7 |a dark matter: annihilation
|2 INSPIRE
650 _ 7 |a sensitivity
|2 INSPIRE
650 _ 7 |a WIMP
|2 INSPIRE
650 _ 7 |a flux
|2 INSPIRE
650 _ 7 |a suppression
|2 INSPIRE
650 _ 7 |a Navarro-Frenk-White profile
|2 INSPIRE
693 _ _ |0 EXP:(DE-H253)CTA-20150101
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700 1 _ |a Adam, R.
|b 1
700 1 _ |a Aguasca-Cabot, A.
|b 2
700 1 _ |a Agudo, I.
|b 3
700 1 _ |a Aguirre-Santaella, A.
|b 4
700 1 _ |a Alfaro, J.
|b 5
700 1 _ |a Aloisio, R.
|b 6
700 1 _ |a Alves Batista, R.
|b 7
700 1 _ |a Amato, E.
|b 8
700 1 _ |a Angüner, E. O.
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700 1 _ |a Aramo, C.
|b 10
700 1 _ |a Arcaro, C.
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700 1 _ |a Asano, K.
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700 1 _ |a Aschersleben, J.
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700 1 _ |a Ashkar, H.
|b 14
700 1 _ |a Backes, M.
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700 1 _ |a Baktash, A.
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700 1 _ |a Balazs, C.
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700 1 _ |a Balbo, M.
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700 1 _ |a Ballet, J.
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700 1 _ |a Bamba, A.
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700 1 _ |a Larriva, A. Baquero
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700 1 _ |a Barbosa Martins, V.
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700 1 _ |a de Almeida, U. Barres
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700 1 _ |a Batista, P.
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700 1 _ |a Batkovic, I.
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700 1 _ |a González, J. Becerra
|b 29
700 1 _ |a Becker Tjus, J.
|b 30
700 1 _ |a Benbow, W.
|b 31
700 1 _ |a Bernardini, E.
|b 32
700 1 _ |a Martín, M. I. Bernardos
|0 P:(DE-H253)PIP1016405
|b 33
|e Corresponding author
700 1 _ |a Medrano, J. Bernete
|b 34
700 1 _ |a Berti, A.
|b 35
700 1 _ |a Bertucci, B.
|b 36
700 1 _ |a Beshley, V.
|b 37
700 1 _ |a Bhattacharjee, P.
|b 38
700 1 _ |a Bhattacharyya, S.
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700 1 _ |a Bigongiari, C.
|b 40
700 1 _ |a Biland, A.
|b 41
700 1 _ |a Bissaldi, E.
|b 42
700 1 _ |a Bocchino, F.
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700 1 _ |a Bordas, P.
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700 1 _ |a Borkowski, J.
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700 1 _ |a Bradascio, F.
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700 1 _ |a Brown, A. M.
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700 1 _ |a Burmistrov, L.
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700 1 _ |a Caroff, S.
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700 1 _ |a Carosi, A.
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700 1 _ |a Carquín, E.
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700 1 _ |a Casanova, S.
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700 1 _ |a Cassol, F.
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700 1 _ |a Cerruti, M.
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700 1 _ |a Chadwick, P.
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700 1 _ |a Chaty, S.
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700 1 _ |a Chen, A.
|b 61
700 1 _ |a Chiavassa, A.
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700 1 _ |a Chytka, L.
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700 1 _ |a De Angelis, A.
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700 1 _ |a De Caprio, V.
|b 75
700 1 _ |a de Gouveia Dal Pino, E. M.
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700 1 _ |a De Martino, D.
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700 1 _ |a de Naurois, M.
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700 1 _ |a de Souza, V.
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700 1 _ |a del Valle, M. V.
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700 1 _ |a Giler, A. G. Delgado
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700 1 _ |a Di Tria, R.
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700 1 _ |a Di Venere, L.
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700 1 _ |a Diebold, S.
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700 1 _ |a Doro, M.
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700 1 _ |a Cadena, S. Hernández
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700 1 _ |a Hnatyk, B.
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700 1 _ |a Iarlori, M.
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700 1 _ |a Inada, T.
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700 1 _ |a Inoue, S.
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700 1 _ |a Iocco, F.
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|e Corresponding author
700 1 _ |a Jamrozy, M.
|b 153
700 1 _ |a Jin, W.
|b 154
700 1 _ |a Jung-Richardt, I.
|b 155
700 1 _ |a Juryšek, J.
|b 156
700 1 _ |a Kantzas, D.
|b 157
700 1 _ |a Karas, V.
|b 158
700 1 _ |a Katagiri, H.
|b 159
700 1 _ |a Kerszberg, D.
|b 160
700 1 _ |a Knödlseder, J.
|b 161
700 1 _ |a Komin, N.
|b 162
700 1 _ |a Kornecki, P.
|b 163
700 1 _ |a Kosack, K.
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700 1 _ |a Kowal, G.
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700 1 _ |a Kubo, H.
|b 166
700 1 _ |a Lamastra, A.
|b 167
700 1 _ |a Lapington, J.
|b 168
700 1 _ |a Lemoine-Goumard, M.
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700 1 _ |a Lenain, J.-P.
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700 1 _ |a Leone, F.
|b 171
700 1 _ |a Leto, G.
|b 172
700 1 _ |a Leuschner, F.
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700 1 _ |a Lindfors, E.
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700 1 _ |a Lohse, T.
|b 175
700 1 _ |a Lombardi, S.
|b 176
700 1 _ |a Longo, F.
|b 177
700 1 _ |a López-Coto, R.
|b 178
700 1 _ |a López-Oramas, A.
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700 1 _ |a Loporchio, S.
|b 180
700 1 _ |a Luque-Escamilla, P. L.
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700 1 _ |a Macias, O.
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700 1 _ |a Mandat, D.
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700 1 _ |a Mangano, S.
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700 1 _ |a Miceli, M.
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700 1 _ |a Michałowski, J.
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700 1 _ |a Mitchell, A.
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700 1 _ |a Moderski, R.
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700 1 _ |a Mohrmann, L.
|b 201
700 1 _ |a Molero, M.
|b 202
700 1 _ |a Molina, E.
|b 203
700 1 _ |a Montaruli, T.
|b 204
700 1 _ |a Moralejo, A.
|b 205
700 1 _ |a Morcuende, D.
|b 206
700 1 _ |a Morselli, A.
|b 207
700 1 _ |a Moulin, E.
|b 208
700 1 _ |a Moya, V.
|b 209
700 1 _ |a Mukherjee, R.
|b 210
700 1 _ |a Munari, K.
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700 1 _ |a Muraczewski, A.
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|b 213
700 1 _ |a Nakamori, T.
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700 1 _ |a Nayak, A.
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700 1 _ |a Niemiec, J.
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700 1 _ |a Nievas, M.
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700 1 _ |a Nikołajuk, M.
|b 218
700 1 _ |a Nishijima, K.
|b 219
700 1 _ |a Noda, K.
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700 1 _ |a Nosek, D.
|b 221
700 1 _ |a Novosyadlyj, B.
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700 1 _ |a Nozaki, S.
|b 223
700 1 _ |a Ohishi, M.
|b 224
700 1 _ |a Ohm, S.
|0 P:(DE-H253)PIP1021898
|b 225
700 1 _ |a Okumura, A.
|b 226
700 1 _ |a Olmi, B.
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700 1 _ |a Ong, R. A.
|b 228
700 1 _ |a Orienti, M.
|b 229
700 1 _ |a Orito, R.
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700 1 _ |a Orlandini, M.
|b 231
700 1 _ |a Orlando, E.
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700 1 _ |a Orlando, S.
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700 1 _ |a Ostrowski, M.
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700 1 _ |a Oya, I.
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700 1 _ |a Pagliaro, A.
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700 1 _ |a Palatka, M.
|b 237
700 1 _ |a Pantaleo, F. R.
|b 238
700 1 _ |a Paoletti, R.
|b 239
700 1 _ |a Paredes, J. M.
|b 240
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|b 241
700 1 _ |a Patricelli, B.
|b 242
700 1 _ |a Pech, M.
|b 243
700 1 _ |a Pecimotika, M.
|b 244
700 1 _ |a Persic, M.
|b 245
700 1 _ |a Petruk, O.
|b 246
700 1 _ |a Pierre, E.
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700 1 _ |a Pietropaolo, E.
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700 1 _ |a Pirola, G.
|b 249
700 1 _ |a Pohl, M.
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700 1 _ |a Prandini, E.
|b 251
700 1 _ |a Priyadarshi, C.
|b 252
700 1 _ |a Pühlhofer, G.
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|b 257
700 1 _ |a Rainò, S.
|b 258
700 1 _ |a Rando, R.
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700 1 _ |a Razzaque, S.
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700 1 _ |a Reimer, O.
|b 262
700 1 _ |a Reposeur, T.
|b 263
700 1 _ |a Ribó, M.
|b 264
700 1 _ |a Richtler, T.
|b 265
700 1 _ |a Rico, J.
|b 266
700 1 _ |a Rieger, F.
|b 267
700 1 _ |a Rigoselli, M.
|b 268
700 1 _ |a Rizi, V.
|b 269
700 1 _ |a Roache, E.
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700 1 _ |a Fernandez, G. Rodriguez
|b 271
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|b 272
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|b 273
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700 1 _ |a de Leon, A. Rosales
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700 1 _ |a Rulten, C.
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700 1 _ |a Sadeh, I.
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700 1 _ |a Santangelo, A.
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700 1 _ |a Santos-Lima, R.
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700 1 _ |a Sarkar, S.
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700 1 _ |a Saturni, F. G.
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700 1 _ |a Schwanke, U.
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700 1 _ |a Servillat, M.
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700 1 _ |a Siejkowski, H.
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|b 295
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|b 296
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|b 297
700 1 _ |a Stolarczyk, T.
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700 1 _ |a Suda, Y.
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700 1 _ |a Tavernier, T.
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|b 306
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|b 307
700 1 _ |a van Eldik, C.
|b 308
700 1 _ |a Vázquez Acosta, M.
|b 309
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|b 310
700 1 _ |a Ventura, S.
|b 311
700 1 _ |a Vercellone, S.
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700 1 _ |a Viana, A.
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700 1 _ |a Vink, J.
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700 1 _ |a Vitale, V.
|b 316
700 1 _ |a Vodeb, V.
|b 317
700 1 _ |a Vorobiov, S.
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700 1 _ |a Vuillaume, T.
|b 319
700 1 _ |a Wagner, S. J.
|b 320
700 1 _ |a Walter, R.
|b 321
700 1 _ |a White, M.
|b 322
700 1 _ |a Wierzcholska, A.
|b 323
700 1 _ |a Will, M.
|b 324
700 1 _ |a Yamazaki, R.
|b 325
700 1 _ |a Yang, L.
|b 326
700 1 _ |a Yoshikoshi, T.
|b 327
700 1 _ |a Zacharias, M.
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700 1 _ |a Zaharijas, G.
|b 329
700 1 _ |a Zavrtanik, D.
|b 330
700 1 _ |a Zavrtanik, M.
|b 331
773 _ _ |a 10.1093/mnras/stad1576
|g Vol. 523, no. 4, p. 5353 - 5387
|0 PERI:(DE-600)2016084-7
|n 4
|p 5353 - 5387
|t Monthly notices of the Royal Astronomical Society
|v 523
|y 2023
|x 0035-8711
787 0 _ |a Acharyya, A. et.al.
|d 2023
|i IsParent
|0 PUBDB-2023-03711
|r arXiv:2305.16707
|t Sensitivity of the Cherenkov Telescope Array to TeV photon emission from the Large Magellanic Cloud
856 4 _ |u https://bib-pubdb1.desy.de/record/596676/files/MNRAS523%282023%295353.pdf
|y Restricted
856 4 _ |u https://bib-pubdb1.desy.de/record/596676/files/MNRAS523%282023%295353.pdf?subformat=pdfa
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Marc 21