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Record W3099117496 · doi:10.48550/arxiv.1802.05172

Population study of Galactic supernova remnants at very high $γ$-ray energies with H.E.S.S.

2018· article· en· W3099117496 on OpenAlexaff
H. Abdalla, A. Abramowski, M. Barnard, D. Khangulyan, B. Khélifi, J. King, S. Klepser, D. Klochkov, W. Kluźniak, Nu. Komin, K. Kosack, S. Krakau, M. Kraus, Y. Becherini, P. P. Krüger, H. Laffon, G. Lamanna, J. Lau, J.-P. Lees, J. Lefaucheur, A. Lemière, M. Lemoine-Goumard, J.-P. Lenain, E. Leser, J. Becker Tjus, T. Lohse, M. Lorentz, Ruyue Liu, R. López-Coto, I. Lypova, D. Malyshev, V. Marandon, A. Marcowith, C. Mariaud, R. Marx, D. Berge, G. Maurin, Nigel Maxted, M. Mayer, P. J. Meintjes, M. Meyer, Alison Mitchell, R. Moderski, M. Mohamed, L. Mohrmann, K. Morå, S. Bernhard, E. Moulin, T. Murach, Shinya Nakashima, M. de Naurois, H. Ndiyavala, F. Niederwanger, J. Niemiec, L. Oakes, P. T. O’Brien, Hirokazu Odaka, K. Bernlöhr, S. Ohm, M. Ostrowski, R. Mirzoyan, M. Padovani, M. Panter, R. D. Parsons, N. W. Pekeur, G. Pelletier, C. Perennes, Pierre-Olivier Petrucci, R. Blackwell, B. Peyaud, Q. Piel, S. Pita, V. Poireau, H. Poon, Д. А. Прохоров, H. Prokoph, G. Pühlhofer, M. Punch, A. Quirrenbach, M. Böttcher, S. Raab, R. Rauth, A. Reimer, O. Reimer, M. Renaud, Frank Rieger, L. Rinchiuso, C. Romoli, Gavin Rowell, C. Boisson, B. Rudak, Samar Safí-Harb, V. Sahakian, Shinya Saito, D. A. Sánchez, A. Santangelo, M. Sasaki, R. Schlickeiser, F. Schüßler, J. Bolmont, U. Schwanke, S. Schwemmer, M. Seglar-Arroyo, M. Settimo, A. S. Seyffert, N. Shafi, I. Shilon, Kleopas Shiningayamwe, R. Simoni, F. Aharonian, S. Bonnefoy, H. Sol, F. Spanier, Marion Spir-Jacob, Ł. Stawarz, R. Steenkamp, C. Stegmann, C. Steppa, I. Sushch, Tadayuki Takahashi, J.-P. Tavernet, P. Bordas, T. Tavernier, Andrew M. Taylor, R. Terrier, L. Tibaldo, D. Tiziani, M. Tluczykont, C. Trichard, M. Tsirou, Naomi Tsuji, R. Tuffs, J. Bregeon, Y. Uchiyama, C. van Eldik, C. van Rensburg, G. Vasileiadis, J. Veh, C. Venter, A. Viana, P. Vincent, F. Brun, J. Vink, F. Voisin, H. J. Völk, Thomas Vuillaume, Zorawar Wadiasingh, P. Wagner, Robert Wagner, R. White, A. Wierzcholska, P. Brun, P. Willmann, A. Wörnlein, D. Wouters, Rong-Jia Yang, D. Zaborov, M. Zacharias, R. Zanin, A. A. Zdziarski, A. Zech, F. Zefi, M. Bryan, A. Ziegler, J. Zorn, Natalia Żywucka, M. Büchele, T. Bulik, M. Capasso, Sami Caroff, A. Carosi, S. Casanova, M. Cerruti, Nachiketa Chakraborty, R. C. G. Chaves, A. Chen, J. Chevalier, S. Colafrancesco, B. Condon, J. M. Conrad, E. O. Angüner, I. D. Davids, J. Decock, C. Deil, J. Devin, P. deWilt, L. Dirson, A. Djannati-Ataı̈, Axel Donath, L. O’C. Drury, K. Dutson, Masanori Arakawa, J. Dyks, T. Edwards, K. Egberts, G. Emery, J.-P. Ernenwein, S. Eschbach, C. Farnier, S. Fegan, M. V. Fernandes, D. Fernández, M. Arrieta, A. Fiasson, G. Fontaine, S. Funk, M. Füßling, S. Gabici, Y. A. Gallant, T. Garrigoux, F. Gaté, G. Giavitto, B. Giebels, P. Aubert, D. Glawion, J. F. Glicenstein, D. Gottschall, M.-H. Grondin, Joachim Hahn, M. Haupt, J. Hawkes, G. Heinzelmann, G. Henri, G. Hermann, Michael Backes, W. Hofmann, C. Hoischen, T. L. Holch, M. Holler, D. Horns, A. Ivascenko, H. Iwasaki, A. Jacholkowska, M. Jamrozy, A. Balzer, D. Jankowsky, F. Jankowsky, M. Jingo, L. Jouvin, I. Jung-Richardt, K. Katarzyński, M. Katsuragawa, U. Katz, D. Kerszberg

Bibliographic record

VenueMPG.PuRe (Max Planck Society) · 2018
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsUniversity of Manitoba
FundersInstitut National de Physique Nucléaire et de Physique des ParticulesJapan Society for the Promotion of ScienceUniversity of NamibiaNational Commission on Research, Science and TechnologyCentre National de la Recherche ScientifiqueAustrian Science FundBundesministerium für Bildung und ForschungGrantová Agentura České RepublikyUniversiteit van AmsterdamMax-Planck-GesellschaftScience and Technology Facilities CouncilNational Research FoundationDeutsche ForschungsgemeinschaftUniverzita Karlova v PrazeAlexander von Humboldt-Stiftung
KeywordsPhysicsAstrophysicsSupernovaCosmic raySupernova remnantGalaxyMilky WayPopulationGalactic planeFlux (metallurgy)PulsarAstronomy

Abstract

fetched live from OpenAlex

Shell-type supernova remnants (SNRs) are considered prime candidates for the acceleration of Galactic cosmic rays (CRs) up to the knee of the CR spectrum at $\mathrm{E} \approx \mathrm{3}\times \mathrm{10}^\mathrm{15}$ eV. Our Milky Way galaxy hosts more than 350 SNRs discovered at radio wavelengths and at high energies, of which 220 fall into the H.E.S.S. Galactic Plane Survey (HGPS) region. Of those, only 50 SNRs are coincident with a H.E.S.S source and in 8 cases the very high-energy (VHE) emission is firmly identified as an SNR. The H.E.S.S. GPS provides us with a legacy for SNR population study in VHE $γ$-rays and we use this rich data set to extract VHE flux upper limits from all undetected SNRs. Overall, the derived flux upper limits are not in contradiction with the canonical CR paradigm. Assuming this paradigm holds true, we can constrain typical ambient density values around shell-type SNRs to $n\leq 7~\textrm{cm}^\textrm{-3}$ and electron-to-proton energy fractions above 10~TeV to $ε_\textrm{ep} \leq 5\times 10^{-3}$. Furthermore, comparisons of VHE with radio luminosities in non-interacting SNRs reveal a behaviour that is in agreement with the theory of magnetic field amplification at shell-type SNRs.

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 distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.017
Threshold uncertainty score0.954

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

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 head0.007
GPT teacher head0.206
Teacher spread0.199 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one teacher head, not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
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

Citations52
Published2018
Admission routes1
Has abstractyes

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