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Article: Discovery of very high energy gamma rays from PKS 1424+240 and multiwavelength constraints on ITS redshift

TitleDiscovery of very high energy gamma rays from PKS 1424+240 and multiwavelength constraints on ITS redshift
Authors
Acciari, VAAliu, EArlen, TAune, TBautista, MBeilicke, MBenbow, WBöttcher, MBoltuch, DBradbury, SMBuckley, JHBregeon, JBrez, ABrigida, MBruel, PBurnett, THCaliandro, GACameron, RACaraveo, PACasandjian, JMCavazzuti, EBugaev, VCecchi, CÇelik, ÖChekhtman, ACheung, CCChiang, JCiprini, SClaus, RCohenTanugi, JConrad, JCutini, SByrum, KDermer, CDDe Angelis, ADe Palma, FDo Couto E Silva, EDrell, PSDrlicaWagner, ADubois, RDumora, DFarnier, CFavuzzi, CCannon, AFegan, SJFocke, WBFortin, PFrailis, MFukazawa, YFusco, PGargano, FGasparrini, DGehrels, NGermani, SCesarini, AGiebels, BGiglietto, NGiommi, PGiordano, FGlanzman, TGodfrey, GGrenier, IAGrove, JEGuillemot, LGuiriec, SChow, YCHanabata, YHays, EHughes, REJackson, MSJóhannesson, GJohnson, ASJohnson, WNKamae, TKatagiri, HKataoka, JCiupik, LKawai, NKerr, MKnödlseder, JKocian, MLKuss, MLande, JLatronico, LLongo, FLoparco, FLott, BCogan, PLovellette, MNLubrano, PMadejski, GMMakeev, AMazziotta, MNMcenery, JEMeurer, CMichelson, PFMitthumsiri, WMizuno, TCui, WMoiseev, AAMonte, CMonzani, MEMorselli, AMoskalenko, IVMurgia, SNolan, PLNorris, JPNuss, EOhsugi, TDuke, COmodei, NOrlando, EOrmes, JFPaneque, DParent, DPelassa, VPepe, MPesceRollins, MPiron, FPorter, TAFalcone, ARainò, SRando, RRazzano, MReimer, AReimer, OReposeur, TRodriguez, AYRoth, MRyde, FSadrozinski, HFWFinley, JPSanchez, DSander, ASaz Parkinson, PMScargle, JDSgrò, CShaw, MSSiskind, EJSmith, PDSpandre, GSpinelli, PFinnegan, GStrickman, MSSuson, DJTajima, HTakahashi, HTanaka, TThayer, JBThayer, JGThompson, DJTibaldo, LTorres, DFFortson, LTosti, GTramacere, AUchiyama, YUsher, TLVasileiou, VVilchez, NVitale, VWaite, APWang, PWiner, BLFurniss, AWood, KSYlinen, TZiegler, MBarber, SDTerndrup, DMGalante, NGall, DGillanders, GHGodambe, SGrube, JGuenette, RGyuk, GHanna, DHolder, JHui, CMHumensky, TBKaaret, PKarlsson, NKertzman, MKieda, DKonopelko, AKrawczynski, HKrennrich, FLang, MJLebohec, SMaier, GMcarthur, SMccann, AMccutcheon, MMillis, JMoriarty, PNagai, TOng, RAOtte, ANPandel, DPerkins, JSPichel, APohl, MQuinn, JRagan, KReyes, LCReynolds, PTRoache, ERose, HJSchroedter, MSembroski, GHDemet Senturk, GSmith, AWSteele, DSwordy, SPTheiling, MThibadeau, SVarlotta, AVassiliev, VVVincent, SWagner, RGWakely, SPWard, JEWeekes, TCWeinstein, AWeisgarber, TWilliams, DAWissel, SWood, MZitzer, BAbdo, AAAckermann, MAjello, MBaldini, LBallet, JBarbiellini, GBastieri, DBaughman, BMBechtol, KBellazzini, RBerenji, BBlandford, RDBloom, EDBonamente, EBorgland, AW
KeywordsBl Lacertae Objects: Individual (Pks 1424+240 = Ver J1427+237)
Gamma Rays: Observations
Issue Date2010
PublisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/2041-8205
Citation
Astrophysical Journal Letters, 2010, v. 708 n. 2 PART 2, p. L100-L106 How to Cite?
AbstractWe report the first detection of very high energy83Gamma-ray emission above 100 GeV. (VHE) gamma-ray emission above 140 GeV from PKS1424+240, a BL Lac object with an unknown redshift. The photon spectrum above 140 GeV measured by VERITAS is well described by a power law with a photon index of 3.8 0.5stat 0.3syst and a flux normalization at 200 GeV of (5.1 0.9stat 0.5syst) × 10-11 TeV -1 cm-2 s-1, where stat and syst denote the statistical and systematical uncertainties, respectively. The VHE flux is steady over the observation period between MJD 54881 and 55003 (from 2009 February 19 to June 21). Flux variability is also not observed in contemporaneous high-energy observations with the Fermi Large Area Telescope. Contemporaneous X-ray and optical data were also obtained from the Swift XRT and MDM observatory, respectively. The broadband spectral energy distribution is well described by a one-zone synchrotron self-Compton model favoring a redshift of less than 0.1. Using the photon index measured with Fermi in combination with recent extragalactic background light absorption models it can be concluded from the VERITAS data that the redshift of PKS 1424+240 is less than 0.66. © 2010. The American Astronomical Society. All rights reserved.
Persistent Identifierhttp://hdl.handle.net/10722/188389
ISSN
2015 Impact Factor: 5.487
2015 SCImago Journal Rankings: 3.369
ISI Accession Number ID
References

 

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dc.date.accessioned2013-09-03T04:04:55Z-
dc.date.available2013-09-03T04:04:55Z-
dc.date.issued2010en_US
dc.identifier.citationAstrophysical Journal Letters, 2010, v. 708 n. 2 PART 2, p. L100-L106en_US
dc.identifier.issn2041-8205en_US
dc.identifier.urihttp://hdl.handle.net/10722/188389-
dc.description.abstractWe report the first detection of very high energy83Gamma-ray emission above 100 GeV. (VHE) gamma-ray emission above 140 GeV from PKS1424+240, a BL Lac object with an unknown redshift. The photon spectrum above 140 GeV measured by VERITAS is well described by a power law with a photon index of 3.8 0.5stat 0.3syst and a flux normalization at 200 GeV of (5.1 0.9stat 0.5syst) × 10-11 TeV -1 cm-2 s-1, where stat and syst denote the statistical and systematical uncertainties, respectively. The VHE flux is steady over the observation period between MJD 54881 and 55003 (from 2009 February 19 to June 21). Flux variability is also not observed in contemporaneous high-energy observations with the Fermi Large Area Telescope. Contemporaneous X-ray and optical data were also obtained from the Swift XRT and MDM observatory, respectively. The broadband spectral energy distribution is well described by a one-zone synchrotron self-Compton model favoring a redshift of less than 0.1. Using the photon index measured with Fermi in combination with recent extragalactic background light absorption models it can be concluded from the VERITAS data that the redshift of PKS 1424+240 is less than 0.66. © 2010. The American Astronomical Society. All rights reserved.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.subjectBl Lacertae Objects: Individual (Pks 1424+240 = Ver J1427+237)en_US
dc.subjectGamma Rays: Observationsen_US
dc.titleDiscovery of very high energy gamma rays from PKS 1424+240 and multiwavelength constraints on ITS redshiften_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.doi10.1088/2041-8205/708/2/L100en_US
dc.identifier.scopuseid_2-s2.0-77949547554en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-77949547554&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume708en_US
dc.identifier.issue2 PART 2en_US
dc.identifier.spageL100en_US
dc.identifier.epageL106en_US
dc.identifier.isiWOS:000273308000007-
dc.publisher.placeUnited Kingdomen_US
dc.identifier.scopusauthoridAcciari, VA=23479136200en_US
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