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Record W2148408639 · doi:10.1051/0004-6361/201220225

Radio-to-<i>γ</i>-ray monitoring of the narrow-line Seyfert 1 galaxy PMN J0948 + 0022 from 2008 to 2011

2012· article· en· W2148408639 on OpenAlexaff
L. Foschini, E. Angelakis, L. Fuhrmann, G. Ghisellini, T. Hovatta, A. Lähteenmäki, M. L. Lister, V. Braito, Luigi Gallo, Timothy S. Hamilton, Motoki Kino, S. Komossa, A. B. Pushkarev, D. J. Thompson, O. Tibolla, A. Tramacere, A. Carramiñana, L. Carrasco, A. Falcone, M. Giroletti, D. Grupe, Y. Y. Kovalev, T. P. Krichbaum, W. Max-Moerbeck, I. Nestoras, T. J. Pearson, A. Porras, A. C. S. Readhead, E. Recillas, J. L. Richards, D. Riquelme, A. Sievers, J. Tammi, M. Tornikoski, H. Ungerechts, J. A. Zensus, A. Celotti, G. Bonnoli, Akihiro Doi, L. Maraschi, G. Tagliaferri, F. Tavecchio

Bibliographic record

VenueAstronomy and Astrophysics · 2012
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsSaint Mary's University
FundersJapan Aerospace Exploration AgencyRussian Academy of SciencesJapan Society for the Promotion of ScienceMax-Planck-Institut für AstrophysikIstituto Nazionale di Fisica NucleareInternational Max Planck Research School for Advanced Methods in Process and Systems EngineeringIstituto Nazionale di AstrofisicaCentre National de la Recherche ScientifiqueMax-Planck-GesellschaftCommissariat à l'Énergie Atomique et aux Énergies AlternativesAgenzia Spaziale ItalianaChinese Academy of SciencesMax-Planck-Institut für AstronomieAcademy of FinlandRussian Foundation for Basic ResearchInternational Max Planck Research School for Environmental, Cellular and Molecular MicrobiologyU.S. Naval ObservatoryVetenskapsrådetU.S. Department of EnergyNational Radio Astronomy ObservatoryAssociated UniversitiesNew Mexico State UniversityUniversity of PortsmouthInstitut National de Physique Nucléaire et de Physique des ParticulesDynasty FoundationUniversität BaselSwinburne University of TechnologyUniversity of PittsburghLos Alamos National LaboratoryGoddard Space Flight CenterAlfred P. Sloan FoundationUniversity of WashingtonPrinceton UniversityJohns Hopkins UniversityMinistry of Education, Culture, Sports, Science and TechnologyAspen Center for PhysicsHigh Energy Accelerator Research OrganizationOhio State UniversityFermilabCase Western Reserve UniversityNational Science FoundationDrexel UniversityNational Aeronautics and Space Administration
KeywordsPhysicsAstrophysicsLorentz factorActive galactic nucleusGalaxyLuminosityAstrophysical jetRadio galaxyFlux (metallurgy)QuasarSpectral lineLight curveEmission spectrumBL Lac objectRadiationJet (fluid)WavelengthAstronomyBlazarGamma rayLorentz transformationOptics

Abstract

fetched live from OpenAlex

We present more than three years of observations at different frequencies, from radio to high-energy -rays, of the Narrow-Line Seyfert 1 (NLS1) Galaxy PMN J0948+0022 (z = 0.585). This source is the first NLS1 detected at energies above 100 MeV and therefore can be considered the prototype of this emerging new class of -ray emitting active galactic nuclei (AGN). The observations performed from 2008 August 1 to 2011 December 31 confirmed that PMN J0948+0022 generates a powerful relativistic jet, which is able to develop an isotropic luminosity at -rays of the order of 10 48 erg s -1 , at the level of powerful quasars. The evolution of the radiation emission of this source in 2009 and 2010 followed the canonical expectations of relativistic jets with correlated multiwavelength variability (-rays followed by radio emission after a few months), but it was difficult to retrieve a similar pattern in the light curves of 2011. The comparison of -ray spectra before and including 2011 data suggested that there was a softening of the highenergy spectral slope. We selected five specific epochs to be studied by modelling the broad-band spectrum, which are characterised by an outburst at -rays or very low/high flux at other wavelengths. The observed variability can largely be explained by changes in the injected power, the bulk Lorentz factor of the jet, or the electron spectrum. The characteristic time scale of doubling/halving flux ranges from a few days to a few months, depending on the frequency and the sampling rate. The shortest doubling time scale at -rays is 2.3 0.5 days. These small values underline the need of highly sampled multiwavelength campaigns to better understand the physics of these sources.

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 categoriesMeta-epidemiology (narrow)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.409
Threshold uncertainty score1.000

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 integrity0.0000.000
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 head0.009
GPT teacher head0.205
Teacher spread0.196 · 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.

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

Citations56
Published2012
Admission routes1
Has abstractyes

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