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Record W2055654992 · doi:10.1088/0004-637x/780/2/168

LONG-TERM TeV AND X-RAY OBSERVATIONS OF THE GAMMA-RAY BINARY HESS J0632+057

2013· article· en· W2055654992 on OpenAlexafffund
E. Aliu, S. Archambault, T. Aune, B. Behera, M. Beilicke, W. Benbow, K. Berger, R. Bird, A. Bouvier, J. H. Buckley, V. Bugaev, K. Byrum, M. Cerruti, X. Chen, L. Ciupik, M. P. Connolly, Wei Cui, C. Duke, J. Dumm, M. Errando, A. Falcone, S. Federici, Q. Feng, J. P. Finley, P. Fortin, L. Fortson, A. Furniss, N. Galante, G. H. Gillanders, S. Griffin, S. Griffiths, J. Grube, G. Gyuk, D. Hanna, J. Holder, G. Hughes, T. B. Humensky, P. Kaaret, M. Kertzman, Y. Khassen, D. Kieda, H. Krawczynski, F. Krennrich, M. J. Lang, A. S Madhavan, G. Maier, P. Majumdar, A. McCann, P. Moriarty, R. Mukherjee, D. Nieto, A. O’Faoláin de Bhróithe, R. A. Ong, A. N. Otte, N. Park, J. S. Perkins, M. Pohl, A. Popkow, H. Prokoph, J. Quinn, K. Ragan, Jean-François Rajotte, L. C. Reyes, P. T. Reynolds, G. T. Richards, E. Roache, J. Rousselle, G. H. Sembroski, F. Sheidaei, C. Skole, A. W. Smith, D. Staszak, M. C. Stroh, I. Telezhinsky, M. Theiling, J. V. Tucci, J. Tyler, A. Varlotta, Stéphane P. Vincent, S. P. Wakely, A. J. Weinstein, R. Welsing, D. A. Williams, A. Zajczyk, B. Zitzer, A. Abramowski, F. Aharonian, F. Ait Benkhali, A. G. Akhperjanian, E. Angüner, G. Anton, S. Balenderan, A. Balzer, A. Barnacka, Y. Becherini, J. Becker Tjus, K. Bernlöhr, E. Birsin, E. Bissaldi, J. Biteau, M. Böttcher, C. Boisson, J. Bolmont, P. Bordas, J. Brucker, F. Brun, P. Brun, T. Bulik, S. Carrigan, S. Casanova, P. M. Chadwick, R. Chalmé-Calvet, R. C. G. Chaves, A. Cheesebrough, M. Chrétien, S. Colafrancesco, G. Cologna, J. M. Conrad, C. Couturier, M. Dalton, M. K. Daniel, I. D. Davids, B. Degrange, C. Deil, P. deWilt, H. J. Dickinson, A. Djannati-Ataı̈, W. Domainko, L. O’C. Drury, G. Dubus, K. Dutson, J. Dyks, M. Dyrda, T. Edwards, K. Egberts, P. Eger, P. Espigat, C. Farnier, S. Fegan, F. Feinstein, M. V. Fernandes, D. Fernández, A. Fiaßon, G. Fontaine, A. Förster, M. Füßling, M. Gajdus, Y. A. Gallant, T. Garrigoux, G. Giavitto, B. Giebels, J. F. Glicenstein, M.-H. Grondin, M. Grudzińska, S. Häffner, J. Hahn, J. Harris, G. Heinzelmann, G. Henri, G. Hermann, O. Hervet, Andreas Hillert, J. A. Hinton, W. Hofmann, P. Hofverberg, M. Holler, D. Horns, A. Jachołkowska, C. Jahn, M. Jamrozy, M. Janiak, F. Jankowsky, I. Jung, M. A. Kastendieck, K. Katarzyński, U. Katz, S. Kaufmann, B. Khélifi, M. Kieffer, S. Klepser, D. Klochkov, W. Kluźniak, T. Kneiske, D. Kolitzus, Nu. Komin, K. Kosack, S. Krakau, F. Krayzel, P. P. Krüger, H. Laffon, G. Lamanna, J. Lefaucheur, A. Lemière, M. Lemoine‐Goumard, J.-P. Lenain, D. Lennarz, T. Lohse, A. Lopatin, C. Lu, V. Marandon, R. Marx, G. Maurin, Nigel Maxted, M. Mayer, T. J. L. McComb, J. Méhault, U. Menzler, M. Meyer, R. Moderski, M. Mohamed, E. Moulin, T. Murach, C. L. Naumann, M. de Naurois, J. Niemiec, S. J. Nolan, L. Oakes, S. Ohm, E. de Oña Wilhelmi, B. Opitz, M. Ostrowski, R. Mirzoyan, M. Panter, R. D. Parsons, M. Paz Arribas, N. W. Pekeur, G. Pelletier, J. Pérez, Pierre-Olivier Petrucci, B. Peyaud, S. Pita, H. Poon, G. Pühlhofer, M. Punch, A. Quirrenbach, S. Raab, M. Raue, A. Reimer, O. Reimer, M. Renaud, R. de los Reyes, Frank Rieger, L. Rob, C. Romoli, S. Rosier-Lees, Gavin Rowell, B. Rudak, C. B. Rulten, V. Sahakian, D. A. Sánchez, A. Santangelo, R. Schlickeiser, F. Schüßler, A. Schulz, U. Schwanke, S. Schwarzburg, S. Schwemmer, H. Sol, G. Spengler, F. Spies, Ł. Stawarz, R. Steenkamp, C. Stegmann, F. Stinzing, K. Stycz, I. Sushch, A. Szostek, J.‐P. Tavernet, T. Tavernier, Andrew M. Taylor, R. Terrier, M. Tluczykont, C. Trichard, K. Valerius, C. van Eldik, G. Vasileiadis, C. Venter, A. Viana, P. Vincent, H. J. Völk, F. Volpe, M. Vorster, S. J. Wagner, P. Wagner, M. J. Ward, M. Weidinger, Q. Weitzel, R. White, A. Wierzcholska, P. Willmann, A. Wörnlein, D. Wouters, M. Zacharias, A. A. Zdziarski, A. Zech, H.-S. Zechlin

Bibliographic record

VenueThe Astrophysical Journal · 2013
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsMcGill University
FundersInstitut National de Physique Nucléaire et de Physique des ParticulesOffice of ScienceU.S. Department of EnergyUniversity of NamibiaCentre National de la Recherche ScientifiqueBundesministerium für Bildung und ForschungMax-Planck-GesellschaftScience and Technology Facilities CouncilNational Research FoundationUniverzita Karlova v PrazeNatural Sciences and Engineering Research Council of CanadaSmithsonian InstitutionScience Foundation IrelandNational Science Foundation
KeywordsPhysicsAstrophysicsLight curveEphemerisOrbital periodAstronomyCherenkov radiationGamma rayTelescopeSkyPulsarContext (archaeology)Orbit (dynamics)SatelliteStarsDetectorOptics

Abstract

fetched live from OpenAlex

HESS J0632+057 is the only gamma-ray binary known so far whose position in the sky allows observations
\nwith ground-based observatories in both the northern and southern hemispheres. Here we report on long-term
\nobservations of HESS J0632+057 conducted with the Very Energetic Radiation Imaging Telescope Array System
\nand High Energy Stereoscopic System Cherenkov telescopes and the X-ray satellite Swift, spanning a time range
\nfrom 2004 to 2012 and covering most of the system’s orbit. The very-high-energy (VHE) emission is found to be
\nvariable and is correlated with that at X-ray energies. An orbital period of 315+6
\n−4 days is derived from the X-ray
\ndata set, which is compatible with previous results, P = (321 ± 5) days. The VHE light curve shows a distinct
\nmaximum at orbital phases close to 0.3, or about 100 days after periastron passage, which coincides with the
\nperiodic enhancement of the X-ray emission. Furthermore, the analysis of the TeV data shows for the first time a
\nstatistically significant (>6.5σ) detection at orbital phases 0.6–0.9. The obtained gamma-ray and X-ray light curves
\nand the correlation of the source emission at these two energy bands are discussed in the context of the recent
\nephemeris obtained for the system. Our results are compared to those reported for other gamma-ray binaries

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: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.785
Threshold uncertainty score0.490

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 science0.0010.000
Research integrity0.0000.001
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 head0.014
GPT teacher head0.218
Teacher spread0.204 · 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

Citations51
Published2013
Admission routes2
Has abstractyes

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