(WFRF:(Almeida J)) pers:(Petrucci P. O)
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| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 09311naa a2202425 4500 | |
| 001 | oai:DiVA.org:lnu-30254 | |
| 003 | SwePub | |
| 008 | 131108s2010 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:lnu:diva-302542 URI |
| 024 | 7 | a https://doi.org/10.1051/0004-6361/2009130732 DOI |
| 040 | a (SwePub)lnu | |
| 041 | a engb eng | |
| 042 | 9 SwePub | |
| 072 | 7 | a ref2 swepub-contenttype |
| 072 | 7 | a art2 swepub-publicationtype |
| 100 | 1 | a Acero, F.4 aut |
| 245 | 1 0 | a PKS2005-489 at VHE :b four years of monitoring with HESS and simultaneous multi-wavelength observations |
| 264 | c 2010-03-30 | |
| 264 | 1 | b EDP Sciences,c 2010 |
| 338 | a print2 rdacarrier | |
| 520 | a Aims. Our aim is to study the very high energy (VHE; E > 100 GeV) gamma-ray emission from BL Lac objects and the evolution in time of their broad-band spectral energy distribution (SED). Methods. VHE observations of the high-frequency peaked BL Lac object PKS 2005-489 were made with the High Energy Stereoscopic System (HESS) from 2004 through 2007. Three simultaneous multi-wavelength campaigns at lower energies were performed during the HESS data taking, consisting of several individual pointings with the XMM-Newton and RXTE satellites. Results. A strong VHE signal, similar to 17 sigma total, from PKS 2005-489 was detected during the four years of HESS observations (90.3 h live time). The integral flux above the average analysis threshold of 400 GeV is similar to 3% of the flux observed from the Crab Nebula and varies weakly on time scales from days to years. The average VHE spectrum measured from similar to 300 GeV to similar to 5 TeV is characterized by a power law with a photon index, Gamma = 3.20 +/- 0.16(stat) +/- 0.10(syst). At X-ray energies the flux is observed to vary by more than an order of magnitude between 2004 and 2005. Strong changes in the X-ray spectrum (Delta Gamma(X) approximate to 0.7) are also observed, which appear to be mirrored in the VHE band. Conclusions. The SED of PKS 2005-489, constructed for the first time with contemporaneous data on both humps, shows significant evolution. The large flux variations in the X-ray band, coupled with weak or no variations in the VHE band and a similar spectral behavior, suggest the emergence of a new, separate, harder emission component in September 2005. | |
| 650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
| 653 | a galaxies: active | |
| 653 | a BL Lacertae objects: individual: PKS 2005-489 | |
| 653 | a gamma rays: galaxies | |
| 653 | a X-rays: individuals: PKS 2005-489 | |
| 653 | a Astropartikelfysik | |
| 653 | a Astroparticle Physics | |
| 700 | 1 | a Aharonian, F.4 aut |
| 700 | 1 | a Akhperjanian, A. G.4 aut |
| 700 | 1 | a Anton, G.4 aut |
| 700 | 1 | a de Almeida, U. Barres4 aut |
| 700 | 1 | a Bazer-Bachi, A. R.4 aut |
| 700 | 1 | a Becherini, Yvonne4 aut |
| 700 | 1 | a Behera, B.4 aut |
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| 700 | 1 | a Glueck, B.4 aut |
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| 700 | 1 | a Mehault, J.4 aut |
| 700 | 1 | a Moderski, R.4 aut |
| 700 | 1 | a Moulin, E.4 aut |
| 700 | 1 | a Naumann-Godo, M.4 aut |
| 700 | 1 | a de Naurois, M.4 aut |
| 700 | 1 | a Nedbal, D.4 aut |
| 700 | 1 | a Nekrassov, D.4 aut |
| 700 | 1 | a Nicholas, B.4 aut |
| 700 | 1 | a Niemiec, J.4 aut |
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| 700 | 1 | a Ohm, S.4 aut |
| 700 | 1 | a Olive, J. -F4 aut |
| 700 | 1 | a Wilhelmi, E. de Ona4 aut |
| 700 | 1 | a Orford, K. J.4 aut |
| 700 | 1 | a Ostrowski, M.4 aut |
| 700 | 1 | a Panter, M.4 aut |
| 700 | 1 | a Arribas, M. Paz4 aut |
| 700 | 1 | a Pedaletti, G.4 aut |
| 700 | 1 | a Pelletier, G.4 aut |
| 700 | 1 | a Petrucci, P. -O4 aut |
| 700 | 1 | a Pita, S.4 aut |
| 700 | 1 | a Puehlhofer, G.4 aut |
| 700 | 1 | a Punch, M.u Univ Paris Diderot, APC, AstroParticule & Cosmology, CNRS,IN2P3,CEA,Irfu, Observ Paris,Sorbonne Paris C, 10 Rue Alice Domon & Leonie Duquet, F-75205 Paris 13, France4 aut0 (Swepub:lnu)mipuaa |
| 700 | 1 | a Quirrenbach, A.4 aut |
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| 700 | 1 | a Renaud, M.4 aut |
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| 700 | 1 | a Rowell, G.4 aut |
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| 700 | 1 | a Rulten, C. B.4 aut |
| 700 | 1 | a Ruppel, J.4 aut |
| 700 | 1 | a Sahakian, V.4 aut |
| 700 | 1 | a Santangelo, A.4 aut |
| 700 | 1 | a Schlickeiser, R.4 aut |
| 700 | 1 | a Schoeck, F. M.4 aut |
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| 700 | 1 | a Steenkamp, R.4 aut |
| 700 | 1 | a Stegmann, C.4 aut |
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| 700 | 1 | a Superina, G.4 aut |
| 700 | 1 | a Szostek, A.4 aut |
| 700 | 1 | a Tam, P. H.4 aut |
| 700 | 1 | a Tavernet, J. -P4 aut |
| 700 | 1 | a Terrier, R.4 aut |
| 700 | 1 | a Tibolla, O.4 aut |
| 700 | 1 | a Tluczykont, M.4 aut |
| 700 | 1 | a van Eldik, C.4 aut |
| 700 | 1 | a Vasileiadis, G.4 aut |
| 700 | 1 | a Venter, C.4 aut |
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| 700 | 1 | a Vialle, J. P.4 aut |
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| 700 | 1 | a Volpe, F.4 aut |
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| 700 | 1 | a Ward, M.4 aut |
| 700 | 1 | a Zdziarski, A. A.4 aut |
| 700 | 1 | a Zech, A.4 aut |
| 710 | 2 | a Univ Paris Diderot, APC, AstroParticule & Cosmology, CNRS,IN2P3,CEA,Irfu, Observ Paris,Sorbonne Paris C, 10 Rue Alice Domon & Leonie Duquet, F-75205 Paris 13, France4 org |
| 773 | 0 | t Astronomy and Astrophysicsd : EDP Sciencesg 511, s. A52-q 511<A52-x 0004-6361x 1432-0746 |
| 856 | 4 | u https://www.aanda.org/articles/aa/pdf/2010/03/aa13073-09.pdf |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:lnu:diva-30254 |
| 856 | 4 8 | u https://doi.org/10.1051/0004-6361/200913073 |
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