Home > Publications database > Discovery of TeV γ -ray emission from PKS 0447-439 and derivation of an upper limit on its redshift > print

001     165671
005     20250717142930.0
024 7 _ |a 10.1051/0004-6361/201321108
|2 doi
024 7 _ |a 0004-6361
|2 ISSN
024 7 _ |a 1432-0746
|2 ISSN
024 7 _ |a arXiv:1303.1628
|2 arXiv
024 7 _ |a 10.3204/DESY-2014-00637
|2 datacite_doi
024 7 _ |a WOS:000317912000117
|2 WOS
024 7 _ |a inspire:1222812
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024 7 _ |a altmetric:1288491
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024 7 _ |a openalex:W2002034199
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037 _ _ |a DESY-2014-00637
082 _ _ |a 520
088 1 _ |a arXiv:1303.1628
088 _ _ |a arXiv:1303.1628
|2 arXiv
100 1 _ |a H.E.S.S. Collaboration
|0 P:(DE-HGF)0
|b 0
|e Collaboration author
245 _ _ |a Discovery of TeV γ -ray emission from PKS 0447-439 and derivation of an upper limit on its redshift
260 _ _ |a Les Ulis
|c 2013
|b EDP Sciences
336 7 _ |a article
|2 DRIVER
336 7 _ |a Output Types/Journal article
|2 DataCite
336 7 _ |a Report
|0 PUB:(DE-HGF)29
|2 PUB:(DE-HGF)
|m report
336 7 _ |a Journal Article
|b journal
|m journal
|0 PUB:(DE-HGF)16
|s 1423723761_23076
|2 PUB:(DE-HGF)
336 7 _ |a ARTICLE
|2 BibTeX
336 7 _ |a JOURNAL_ARTICLE
|2 ORCID
336 7 _ |a Journal Article
|0 0
|2 EndNote
500 _ _ |a 14 pages, 10 figures, accepted for publication in A&A
520 _ _ |a Very high-energy γ-ray emission from PKS 0447−439 was detected with the H.E.S.S. Cherenkov telescope array in December 2009. This blazar is one of the brightest extragalactic objects in the Fermi bright source list and has a hard spectrum in the MeV to GeV range. In the TeV range, a photon index of 3.89 ± 0.37 (stat) ±0.22 (sys) and a flux normalisation at 1 TeV, Φ1 TeV = (3.5 ± 1.1(stat) ± 0.9(sys)) × 10-13 cm-2   s-1   TeV-1 were found. The detection with H.E.S.S. triggered observations in the X-ray band with the Swift and RXTE telescopes. Simultaneous UV and optical data from Swift UVOT and data from the optical telescopes ATOM and ROTSE are also available. The spectrum and light curve measured with H.E.S.S. are presented and compared to the multi-wavelength data at lower energies. A rapid flare is seen in the Swift XRT and RXTE data, together with a flux variation in the UV band, at a time scale of the order of one day. A firm upper limit of z < 0.59 on the redshift of PKS 0447−439 is derived from the combined Fermi-LAT and H.E.S.S. data, given the assumptions that there is no upturn in the intrinsic spectrum above the Fermi-LAT energy range and that absorption on the extragalactic background light (EBL) is not weaker than the lower limit provided by current models. The spectral energy distribution is well described by a simple one-zone synchrotron self-Compton scenario, if the redshift of the source is less than z ≲ 0.4.
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773 _ _ |a 10.1051/0004-6361/201321108
|g Vol. 552, p. A118 -
|0 PERI:(DE-600)1458466-9
|n 118
|p 1-14
|t Astronomy and astrophysics
|v 552
|y 2013
|x 1432-0746
787 0 _ |a H. E. S. S. Collaboration et.al.
|d 2013
|i IsParent
|0 DESY-2014-00632
|r arXiv:1303.1628
|t Discovery of TeV gamma-ray emission from PKS 0447-439 and derivation of an upper limit on its redshift
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Marc 21