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Record W2795587333 · doi:10.3847/1538-4357/aab35a

Revival of the Magnetar PSR J1622–4950: Observations with MeerKAT, Parkes, XMM-Newton, Swift, Chandra, and NuSTAR

2018· article· en· W2795587333 on OpenAlexafffund
F. Camilo, Paul Scholz, M. Serylak, S. Buchner, Marcus Merryfield, V. M. Kaspi, R. F. Archibald, M. Bailes, A. Jameson, W. van Straten, John Sarkissian, J. E. Reynolds, S. Johnston, G. Hobbs, T. D. Abbott, R. Adam, G. Adams, Thomas E. Alberts, R. Andreas, K. M. B. Asad, Daniel Baker, T. Baloyi, E. F. Bauermeister, T. Baxana, Thomas Bennett, G. Bernardi, D. Booisen, R. S. Booth, D. H. Botha, L. Boyana, L. R. S. Brederode, J. P. Burger, T. Cheetham, J. P. Conradie, David Davidson, G. De Bruin, Bonita de Swardt, Chris De Villiers, Dirk I. L. de Villiers, M. S. de Villiers, W. de Villiers, C. De Waal, M. A. Dikgale, George Du Toit, L.J. du Toit, S. W. P. Esterhuyse, B. L. Fanaroff, S. Fataar, A. Reghan Foley, Griffin Foster, D.J. Fourie, R. R. G. Gamatham, T. G. Gatsi, Riana Geschke, S. Goedhart, Trienko Grobler, S. C. Gumede, Moloko Hlakola, A. Hokwana, D. H. Hoorn, David Horn, Jasper Horrell, B.V. Hugo, A. R. Isaacson, O. Jacobs, J. P. Jansen van Rensburg, J. L. Jonas, Barney Jordaan, A. F. Joubert, Fourie Joubert, G. I. G. Józsa, Roufurd Julie, C. C. Julius, F. Kapp, A. Karastergiou, F. Karels, M. Kariseb, R. Karuppusamy, V. Kasper, Evan C. Knox-Davies, D. G. Koch, P. Kotzé, Ambroise Krebs, N. Kriek, Herman Kriel, T. W. Kusel, S. Lamoor, Robert Lehmensiek, D. H. Liebenberg, Ian Liebenberg, R. T. Lord, B. M. Lunsky, N. Mabombo, T. MacDonald, Peter S. Macfarlane, K. Madisa, L. Mafhungo, Lindsay Magnus, C. Magozore, O. Mahgoub, J. P. L. Main, Sphesihle Makhathini, J. A. Malan, P. Malgas, Jason Manley, M. Manzini, Lelanie Marais, N. Marais, S. J. Marais, M. Maree, A. Martens, S. D. Matshawule, N. Matthysen, T. Mauch, L. D. Mc Nally, Bruce Merry, Rob Millenaar, C. Mjikelo, N. Mkhabela, N. Mnyandu, I. T. Moeng, O. J. Mokone, T. E. Monama, K. Montshiwa, Vanessa A. Moss, M. C. Mphego, W. S. New, B. Ngcebetsha, K. J. Ngoasheng, Heinrich Niehaus, Pitika Ntuli, A. Nzama, F. Obies, Monika Obrocka, M. T. Ockards, C. Olyn, Nadeem Oozeer, A. J. Otto, Y. Padayachee, S. S. Passmoor, A. A. Patel, Samantha Soares de Paula, A. Peens-Hough, B. Pholoholo, P. Prozesky, S. Rakoma, A. J. T. Ramaila, I. Rammala, Z. R. Ramudzuli, M. Rasivhaga, S. Ratcliffe, H.C. Reader, R. Renil, L. Richter, A. Robyntjies, D. Rosekrans, A. Rust, S. Salie, N. Sambu, C. T. G. Schollar, L. C. Schwardt, S. Seranyane, G. Sethosa, Chris Sharpe, R. Siebrits, S. K. Sirothia, Martin Slabber, O. Smirnov, Susan Smith, L. Sofeya, N. Songqumase, R. Spann, B. W. Stappers, Dewald Steyn, T. J. Steyn, Robert Strong, Allan D. Struthers, C.G. Stuart, P. Sunnylall, Paul Swart, B. Taljaard, Cyril Tasse, G. Taylor, Isak P. Theron, Venkatasubramani L. Thondikulam, Kshitij Thorat, A. J. Tiplady, O. Toruvanda, Jason van Aardt, Tyrone van Balla, Lize Van den Heever, A. van der Byl, C. van der Merwe, Pieter van der Merwe, P. C. van Niekerk, Ruby van Rooyen, J. P. van Staden, V. Van Tonder, R. Van Wyk, I. Wait, A. L. Walker, B. Wallace, M. G. Welz, L. P. Williams, B. Xaia, Neil J. Young, Simphiwe Zitha

Bibliographic record

VenueThe Astrophysical Journal · 2018
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPulsars and Gravitational Waves Research
Canadian institutionsMcGill UniversityUniversity of VictoriaUniversity of TorontoHerzberg Institute of Astrophysics
FundersGoddard Space Flight CenterScience and Technology Facilities CouncilNatural Sciences and Engineering Research Council of CanadaNational Aeronautics and Space AdministrationCalifornia Institute of TechnologyJet Propulsion Laboratory
KeywordsMagnetarPhysicsAstrophysicsPulsarNeutron starFlux (metallurgy)MagnetosphereSwiftAstronomyMillisecond pulsarMagnetic field

Abstract

fetched live from OpenAlex

Abstract New radio (MeerKAT and Parkes) and X-ray ( XMM-Newton , Swift , Chandra , and NuSTAR ) observations of PSR J1622–4950 indicate that the magnetar, in a quiescent state since at least early 2015, reactivated between 2017 March 19 and April 5. The radio flux density, while variable, is approximately 100× larger than during its dormant state. The X-ray flux one month after reactivation was at least 800× larger than during quiescence, and has been decaying exponentially on a 111 ± 19 day timescale. This high-flux state, together with a radio-derived rotational ephemeris, enabled for the first time the detection of X-ray pulsations for this magnetar. At 5%, the 0.3–6 keV pulsed fraction is comparable to the smallest observed for magnetars. The overall pulsar geometry inferred from polarized radio emission appears to be broadly consistent with that determined 6–8 years earlier. However, rotating vector model fits suggest that we are now seeing radio emission from a different location in the magnetosphere than previously. This indicates a novel way in which radio emission from magnetars can differ from that of ordinary pulsars. The torque on the neutron star is varying rapidly and unsteadily, as is common for magnetars following outburst, having changed by a factor of 7 within six months of reactivation.

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 score0.701
Threshold uncertainty score0.419

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 studies0.0010.001
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 head0.015
GPT teacher head0.275
Teacher spread0.260 · 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

Citations160
Published2018
Admission routes2
Has abstractyes

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