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Potential of the Cherenkov Telescope Array for studying the young nearby supernova remnants
Dmitry A. Prokhorov, S.-H. Lee, Shigehiro Nagataki, Jacco Vink, Donald C. Ellison, Gilles Ferrand, Daniel Patnaude, F. K. Roepke, I. R. Seitenzahl, Patrick Slane, Kazuki Abe, Shotaro Abe, A. Acharyya, Rémi Adam, Arnau Aguasca-Cabot, I. Agudo, Jorge Alfaro, Nuria Álvarez Crespo, Rafael Alves Batista, Jean-Philippe Amans, Elena Amato, Filippo Ambrosino, E. O. Angüner, L. A. Antonelli, C. Aramo, Cornelia Arcaro, Luisa Arrabito, Katsuaki Asano, J. Aschersleben, Halim Ashkar, Luiz Augusto Stuani, Dominik Baack, Michael Backes, Csaba Balázs, Matteo Balbo, Andrés Baquero, V. Barbosa Martins, U. Barres de Almeida, J. A. Barrio, D. Bastieri, Pedro Ivo Batista, Ivana Batković, R. Batzofin, Joshua Ryo Baxter, Geoffrey Beck, J. Becker Tjus, Lukas Beiske, Daniele Belardinelli, W. Benbow, E. Bernardini, Juan Bernete Medrano, K. Bernlöhr, A. Berti, Vasyl Beshley, Pooja Bhattacharjee, Saptashwa Bhattacharyya, Baiyang Bi, Noah Biederbeck, A. Biland, E. Bissaldi, O. Blanch, Jiří Blažek, C. Boisson, J. Bolmont, G. Bonnoli, P. Bordas, Ž. Bošnjak, Federica Bradascio, Catherine Braiding, E. Bronzini, Robert Brose, A. M. Brown, F. Brun, Giulia Brunelli, A. Bulgarelli, Irene Burelli, L. Burmistrov, Michael Burton, T. Bylund, P. Calisse, Anna Campoy-Ordaz, Brandon Khan Cantlay, Milvia Capalbi, Anderson Caproni, R. Capuzzo‐Dolcetta, Colin Carlile, Sami Caroff, A. Carosi, R. Carosi, Marie-Sophie Carrasco, E. Cascone, Noelia Castrejon, Fernando Catalani, Davide Cerasole, M. Cerruti, S. Chaty, A. Chen, M. Chernyakova, A. Chiavassa, J. Chudoba, Carlos H. Coimbra-Araújo, Vito Conforti, F. Conte, J. L. Contreras, Christophe Cossou, Alessandro Costa, H. Costantini, Pierre Cristofari, Omar Cuevas, Zachary Curtis-Ginsberg, Giacomo D’Amico, F. D’Ammando, M. Dadina, M. Dalchenko, Ludovic David, I. D. Davids, F. Dazzi, A. De Angelis, Mathieu de Bony de Lavergne, Vincenzo De Caprio, G. De Cesare, E. M. de Gouveia Dal Pino, B. De Lotto, Mario de Lucia, Raniere de Menezes, M. de Naurois, E. de Oña Wilhelmi, N. De Simone, L. del Peral, M. V. del Valle, E. Delagnes, Andres Gabriel Delgado Giler, Michael Dellaiera, R. Della Ceca, M. Della Valle, D. della Volpe, Davide Depaoli, A. Dettlaff, Tristano Di Girolamo, Ambra Di Piano, F. Di Pierro, Riccardo Di Tria, L. Di Venere, Christian Díaz-Bahamondes, Claudio Dib, Sebastian Diebold, R. Dima, Adithiya Dinesh, A. Djannati-Ataı̈, Julia Isabel Djuvsland, A. Domínguez, Rune Michael Dominik, Alice Donini, D. Dorner, Julien Dörner, M. Doro, R. C. dos Anjos, Jean-Laurent Dournaux, Dainis Dravins, Chaimongkol Duangchan, Coline Dubos, Vikram V. Dwarkadas, Jan Ebr, Christopher Eckner, K. Egberts, S. Einecke, Dominik Elsässer, Gabriel Emery, Miguel Escobar Godoy, Juan Escudero, P. Esposito, D. Falceta-Gonçalves, V. Fallah Ramazanı, Alice Faure, E. Fedorova, S. Fegan, Kirsty Feijen, Q. Feng, F. Ferrarotto, E. Fiandrini, A. Fiaßon, V. Fioretti, L. Foffano, Lluis Font Guiteras, G. Fontaine, Stefan Fröse, Satoshi Fukami, Y. Fukui, S. Funk, Daniele Gaggero, Giorgio Galanti, Gaspar Galaz, Yves Gallant, S. Gallozzi, V. Gammaldi, Claudio Gasbarra, M. Gaug, Arsen Ghalumyan, F. Gianotti, M. Giarrusso, N. Giglietto, F. Giordano, A. Giuliani, J. F. Glicenstein, Jonas Glombitza, P. Goldoni, José Mauricio González, M. M. González, Jaziel G. Coelho, Jonathan Granot, Dario Grasso, Roger Grau Haro, David A. Green, Jarred Gershon Green, T. Greenshaw, G. Grolleron, J. Grube, O. Gueta, S. Gunji, D. Hadasch, P. Hamal, W. Hanlon, Satoshi Hara, Violet M. Harvey, Kazuaki Hashiyama, T. Hassan, Matthieu Heller, Sergio Hernández Cadena, Jonathan Hie, Nagisa Hiroshima, B. Hnatyk, R. Hnatyk, D. Hoffmann, Werner Hofmann, Markus Holler, D. Horan, Pavel Horváth, T. Hovatta, Dario Hrupec, Saqib Hussain, Marco Iarlori, Tomohiro Inada, Federico Incardona, Yusuke Inome, Susumu Inoue, Fabio Iocco, Kazuma Ishio, M. Jamrozy, Petr Janeček, F. Jankowsky, Christian Jarnot, P. Jean, Irene Jiménez Martínez, W. Jin, L. Jocou, Claire Juramy, Jakub Jurýšek, O. Kalekin, Dimitrios Kantzas, V. Karas, S. Kaufmann, D. Kerszberg, B. Khélifi, D. Kieda, T. K. Kleiner, W. Kluźniak, Yukiho Kobayashi, Kazunori Kohri, Nu. Komin, Paula Kornecki, K. Kosack, H. Kubo, J. Kushida, A. La Barbera, N. La Palombara, María Láinez, A. Lamastra, J. Lapington, Sanja Lazarević, Jasmina Lazendic-Galloway, Steve Leach, M. Lemoine‐Goumard, J.-P. Lenain, G. Leto, Fabian Leuschner, E. Lindfors, Maximilian Linhoff, Ioannis Liodakis, Lozach Loïc, S. Lombardi, F. Longo, R. López-Coto, A. López-Oramas, S. Loporchio, J. J. Lozano Bahilo, Pedro L. Luque‐Escamilla, Oscar Macías, G. Maier, P. Majumdar, Denys Malyshev, D. Malyshev, Dušan Mandát, Giulio Manicò, Peter David Marinos, Sera Markoff, I. Márquez, Patricia Márquez, G. Marsella, J. Martı́, Pierrick Martin, Gustavo Augusto Martínez, M. Martı́nez, Oibar Martínez, Christophe Marty, Alvaro Mas-Aguilar, M. Mastropietro, G. Maurin, W. Max-Moerbeck, D. Mazin, David Melkumyan, Stefano Menchiari, Jean‐Luc Meunier, D M-A Meyer, Davide Miceli, Miltiadis Michailidis, J. Michałowski, Tjark Miener, J. M. Miranda, Alison Mitchell, Masaya Mizote, Tsunefumi Mizuno, R. Moderski, L. Mohrmann, Cesare Molfese, E. Molina, T. Montaruli, A. Moralejo, Daniel Morcuende, Katharina Morik, A. Morselli, E. Moulin, Victor Moya Zamanillo, R. Mukherjee, Kevin Munari, Adam Muraczewski, H. Muraishi, Takeshi Nakamori, Lara Nava, Amrit Nayak, Rodrigo Nemmen, Lukas Nickel, J. Niemiec, D. Nieto, M. Nievas Rosillo, M. Nikołajuk, K. Nishijima, K. Noda, Dalibor Nosek, B. Novosyadlyj, Vladimír Novotný, S. Nozaki, P. T. O’Brien, M. Ohishi, Yoshiki Ohtani, A. Okumura, J. F. Olive, Barbara Olmi, R. A. Ong, M. Orienti, Reiko Orito, M. Orlandini, M. Ostrowski, A. N. Otte, I. Pagano, A. Pagliaro, M. Palatiello, Gabriele Panebianco, J. M. Paredes, N. Parmiggiani, Sonal Ramesh Patel, B. Patricelli, Dijana Pavlović, Asaf Pe’er, M. Pech, Mario Pecimotika, M. Peresano, Judit Pérez-Romero, Giada Peron, M. Persic, Pierre-Olivier Petrucci, O. Petruk, Felix Pfeifle, Fabio Pintore, Giorgio Pirola, C. Pittori, Cyann Plard, F. Podobnik, M. Pohl, Estelle Pons, E. Prandini, Julie Prast, G. Principe, Chaitanya Priyadarshi, N. Produit, E. Pueschel, G. Pühlhofer, Maria Letizia Pumo, M. Punch, A. Quirrenbach, S. Rainò, N. Randazzo, R. Rando, Thierry Ravel, S. Razzaque, Maxime Regeard, Patrick Reichherzer, A. Reimer, O. Reimer, Andreas Reisenegger, Thierry Reposeur, Brian Reville, W. Rhode, M. Ribó, T. Richtler, Frank Rieger, E. Roache, Gonzalo Rodriguez Fernandez, M. D. Rodríguez-Friás, Juan José Rodríguez‐Vázquez, P. Romano, G. Romeo, J. Rosado, Gavin Rowell, B. Rudak, Ashley J. Ruiter, C. B. Rulten, Federico Russo, I. Sadeh, L. Saha, T. Saito, Shunsuke Sakurai, Heiko Salzmann, D. A. Sánchez, M. Sánchez‐Conde, Pierluca Sangiorgi, Hidetoshi Sano, M. Santander, A. Santangelo, R. Santos-Lima, A. Sanuy, Toni Šarić, Arkadipta Sarkar, S. Sarkar, Francesco Gabriele Saturni, V. Savchenko, Andres Scherer, Pietro Schipani, Bernd Schleicher, Petr Schovánek, Jan Lukas Schubert, F. Schüßler, Ullrich Schwanke, Georg Schwefer, Salvatore Scuderi, M. Seglar-Arroyo, O. Sergijenko, V. Sguera, Ruo Yu Shang, P. Sharma, Guéréguin Der Sylvestre Sidibé, L. Sidoli, H. Siejkowski, Clarissa Siqueira, P. Sizun, Vitalii Sliusar, A. Słowikowska, Hélène Sol, Andreas Specovius, S. Spencer, Daniele Spiga, A. Stamerra, S. Stanič, Tomasz Starecki, R. L. C. Starling, Constantin Steppa, Thierry Stolarczyk, Jelena Strišković, M. Strzys, Y. Suda, Tiina Suomijärvi, D. Tak, Mitsunari Takahashi, Ryuji Takeishi, Pak-Hin Thomas Tam, Shuta Tanaka, Takaaki Tanaka, Kenta Terauchi, V. Testa, L. Tibaldo, O. Tibolla, Francesc Torradeflot, D. F. Torres, E. Torresi, N. F. H. Tothill, F. Toussenel, Victoria Touzard, A. Tramacere, P. Trávnı́ček, G. Tripodo, Stefano Truzzi, Adellain Tsiahina, Antonio Tutone, Martin Vacula, Bertrand Vallage, P. Vallania, Ramon Vallés, C. van Eldik, Juliane van Scherpenberg, J. Vandenbroucke, V. V. Vassiliev, Philippe Venault, Sofia Ventura, S. Vercellone, G. Verna, A. Viana, N. Viaux Maira, Alessandro Vigliano, Jonatan Vignatti, C. Vigorito, V. Vitale, Veronika Vodeb, Vincent Voisin, S. Vorobiov, Georgios Gerasimos Voutsinas, Ievgen Vovk, Vincent Waegebaert, S. J. Wagner, R. Walter, Martin Ward, Maneenate Wechakama, R. White, A. Wierzcholska, Martin Will, David A. Williams, Frederik Wohlleben, A. Wolter, Tokonatsu Yamamoto, Ryo Yamazaki, Lili Yang, T. Yoshida, T. Yoshikoshi, M. Zacharias, Ricardo Sánchez, D. Zavrtanik, Marko Zavrtanik, A. A. Zdziarski, Andreas Zech, В. И. Жданов, Krzysztof Ziȩtara, Miha Živec, Jaume Zuriaga-Puig
Bibliographic record
Venuenot available
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsUniversity of Manitoba
Fundersnot available
KeywordsCherenkov Telescope ArrayCherenkov radiationCassiopeia APhysicsSupernovaTelescopeAstronomyGamma rayHigh energyAstrophysicsSupernova remnantOpticsDetectorEngineering physics
Abstract
Modern imaging atmospheric Cherenkov telescopes have extensively observed young nearby supernova remnants (SNRs), with ages of about 1000 years or less, in the very-high-energy (VHE) gamma-ray band. These efforts resulted in the detection of VHE emission from three young SNRs - Cassiopeia A, Tycho, and SN 1006 - and provided significant evidence for emission from the more distant Kepler's SNR. However, many questions on the production of VHE gamma rays in these remnants remain unanswered. Using detailed physical models for Tycho's SNR based on the CR-hydro-NEI code and physically motivated models for the other young nearby remnants, we simulated observations with the Cherenkov Telescope Array (CTA) of these gamma-ray sources. We highlight properties of these remnants accessible for investigation with future CTA observations and discuss which questions are expected to be answered.
Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.
How this classification was reachedexpand
Full frame machine prediction
Teacher imitationNot calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.
metaresearch head score (Codex)0.001
metaresearch head score (Gemma)0.002
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: Simulation or modeling
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.014
Threshold uncertainty score0.027
Distilled classifier scores by category (both heads)
| Category | Codex | Gemma |
|---|---|---|
| Metaresearch | 0.001 | 0.002 |
| Meta-epidemiology (narrow) | 0.000 | 0.000 |
| Meta-epidemiology (broad) | 0.000 | 0.001 |
| Bibliometrics | 0.000 | 0.000 |
| Science and technology studies | 0.000 | 0.000 |
| Scholarly communication | 0.001 | 0.001 |
| Open science | 0.001 | 0.001 |
| Research integrity | 0.000 | 0.000 |
| Insufficient payload (model declined to judge) | 0.001 | 0.000 |
Machine scores (provisional)
The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.
Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.
Opus teacher head0.017
GPT teacher head0.238
Teacher spread0.222 · how far apart the two teachers sit on this one work
Validation status
score_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from itClassification
machine, unvalidatedMachine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.
The models applied no category: nothing in the taxonomy fit this work.
Study designSimulation or modeling
Domainnot available
GenreEmpirical
How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".
Quick stats
Citations0
Published2023
Admission routes1
Has abstractyes