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Article: Multiwavelength monitoring of the enigmatic narrow-line seyfert 1 PMN J0948+0022 in 2009 march-july

TitleMultiwavelength monitoring of the enigmatic narrow-line seyfert 1 PMN J0948+0022 in 2009 march-july
Authors
Abdo, AAAckermann, MAjello, MAxelsson, MBaldini, LBallet, JBarbiellini, GBastieri, DBaughman, BMBechtol, KBellazzini, RMonte, CMonzani, MEMorselli, AMoskalenko, IVNestoras, INolan, PLNorris, JPNuss, EOhsugi, TOmodei, NBerenji, BOrlando, EOrmes, JFPaneque, DParent, DPavlidou, VPelassa, VPepe, MPesceRollins, MPiron, FPorter, TABloom, EDRainò, SRando, RRazzano, MReadhead, AReimer, OReposeur, TRichards, JLRodriguez, AYRoth, MRyde, FBonamente, ESadrozinski, HFWSanchez, DSander, ASaz Parkinson, PMScargle, JDSgrò, CShaw, MSSmith, PDSpandre, GSpinelli, PBorgland, AWStrickman, MSSuson, DJTagliaferri, GTajima, HTakahashi, HTanaka, TThayer, JBThayer, JGThompson, DJTibaldo, LBregeon, JTibolla, OTorres, DFTosti, GTramacere, AUchiyama, YUsher, TLVasileiou, VVilchez, NVitale, VWaite, APBrez, AWang, PWehrle, AEWiner, BLWood, KSYlinen, TZensus, JAZiegler, MAngelakis, EBailyn, CBignall, HBrigida, MBlanchard, JBonning, EWBuxton, MCanterna, RCarramĩana, ACarrasco, LColomer, FDoi, AGhisellini, GHauser, MBruel, PHong, XIsler, JKino, MKovalev, YYKovalev, YAKrichbaum, TPKutyrev, ALahteenmaki, AVan Langevelde, HJLister, MLBurnett, THMacomb, DMaraschi, LMarchili, NNagai, HParagi, ZPhillips, CPushkarev, ABRecillas, ERoming, PSekido, MCaliandro, GAStark, MASzomoru, ATammi, JTavecchio, FTornikoski, MTzioumis, AKUrry, CMWagner, SCameron, RACaraveo, PACasandjian, JMCavazzuti, ECecchi, CÇelik, ÖCelotti, AChekhtman, AChiang, JCiprini, SClaus, RCohenTanugi, JCollmar, WConrad, JCostamante, LCutini, SDe Angelis, ADe Palma, FDo Couto E Silva, EDrell, PSDumora, DFarnier, CFavuzzi, CFegan, SJFocke, WBFortin, PFoschini, LFrailis, MFuhrmann, LFukazawa, YFunk, SFusco, PGargano, FGehrels, NGermani, SGiglietto, NGiordano, FGiroletti, MGlanzman, TGodfrey, GGrenier, IAGrove, JEGuillemot, LGuiriec, SHanabata, YHays, EHughes, REJackson, MSJóhannesson, GJohnson, ASJohnson, WNKadler, MKamae, TKatagiri, HKataoka, JKawai, NKerr, MKnödlseder, JKocian, MLKuss, MLande, JLatronico, LLongo, FLoparco, FLott, BLovellette, MNLubrano, PMadejski, GMMakeev, AMaxMoerbeck, WMazziotta, MNMcconville, WMcenery, JEMcglynn, SMeurer, CMichelson, PFMitthumsiri, WMizuno, TMoiseev, AA
KeywordsGamma Rays: Observations
Issue Date2009
PublisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/2041-8205
Citation
Astrophysical Journal Letters, 2009, v. 707 n. 1, p. 727-737 How to Cite?
AbstractFollowing the recent discovery of γ rays from the radio-loud narrow-line Seyfert 1 galaxy PMN J0948+0022 (z = 0.5846), we started a multiwavelength campaign from radio to γ rays, which was carried out between the end of 2009 March and the beginning of July. The source displayed activity at all the observed wavelengths: a general decreasing trend from optical to γ-ray frequencies was followed by an increase of radio emission after less than two months from the peak of the γ-ray emission. The largest flux change, about a factor of about 4, occurred in the X-ray band. The smallest was at ultraviolet and near-infrared frequencies, where the rate of the detected photons dropped by a factor 1.6-1.9. At optical wavelengths, where the sampling rate was the highest, it was possible to observe day scale variability, with flux variations up to a factor of about 3. The behavior of PMN J0948+0022 observed in this campaign and the calculated power carried out by its jet in the form of protons, electrons, radiation, and magnetic field are quite similar to that of blazars, specifically of flat-spectrum radio quasars. These results confirm the idea that radio-loud narrow-line Seyfert 1 galaxies host relativistic jets with power similar to that of average blazars. © 2009 The American Astronomical Society.
Persistent Identifierhttp://hdl.handle.net/10722/188373
ISSN
2015 Impact Factor: 5.487
2015 SCImago Journal Rankings: 3.369
ISI Accession Number ID
References

 

DC FieldValueLanguage
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dc.contributor.authorAckermann, Men_US
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dc.date.accessioned2013-09-03T04:04:15Z-
dc.date.available2013-09-03T04:04:15Z-
dc.date.issued2009en_US
dc.identifier.citationAstrophysical Journal Letters, 2009, v. 707 n. 1, p. 727-737en_US
dc.identifier.issn2041-8205en_US
dc.identifier.urihttp://hdl.handle.net/10722/188373-
dc.description.abstractFollowing the recent discovery of γ rays from the radio-loud narrow-line Seyfert 1 galaxy PMN J0948+0022 (z = 0.5846), we started a multiwavelength campaign from radio to γ rays, which was carried out between the end of 2009 March and the beginning of July. The source displayed activity at all the observed wavelengths: a general decreasing trend from optical to γ-ray frequencies was followed by an increase of radio emission after less than two months from the peak of the γ-ray emission. The largest flux change, about a factor of about 4, occurred in the X-ray band. The smallest was at ultraviolet and near-infrared frequencies, where the rate of the detected photons dropped by a factor 1.6-1.9. At optical wavelengths, where the sampling rate was the highest, it was possible to observe day scale variability, with flux variations up to a factor of about 3. The behavior of PMN J0948+0022 observed in this campaign and the calculated power carried out by its jet in the form of protons, electrons, radiation, and magnetic field are quite similar to that of blazars, specifically of flat-spectrum radio quasars. These results confirm the idea that radio-loud narrow-line Seyfert 1 galaxies host relativistic jets with power similar to that of average blazars. © 2009 The American Astronomical Society.en_US
dc.languageengen_US
dc.publisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/2041-8205en_US
dc.relation.ispartofAstrophysical Journal Lettersen_US
dc.subjectGamma Rays: Observationsen_US
dc.titleMultiwavelength monitoring of the enigmatic narrow-line seyfert 1 PMN J0948+0022 in 2009 march-julyen_US
dc.typeArticleen_US
dc.identifier.emailSaz Parkinson, PM: pablosp@hku.hken_US
dc.identifier.authoritySaz Parkinson, PM=rp01803en_US
dc.description.naturelink_to_subscribed_fulltexten_US
dc.identifier.doi10.1088/0004-637X/707/1/727en_US
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dc.identifier.volume707en_US
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dc.identifier.spage727en_US
dc.identifier.epage737en_US
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