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The starburst galaxy NGC 253 revisited by H.E.S.S. and Fermi-LAT

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cris.lastimport.scopus2024-02-12T20:48:12Z
dc.abstract.enContext. NGC 253 is one of only two starburst galaxies found to emit γ-rays from hundreds of MeV to multi-TeV energies. Accurate measurements of the very-high-energy (VHE; E > 100 GeV) and high-energy (HE; E > 60 MeV) spectra are crucial to study the underlying particle accelerators, probe the dominant emission mechanism(s) and to study cosmic-ray interaction and transport. Aims: The measurement of the VHE γ-ray emission of NGC 253 published in 2012 by H.E.S.S. was limited by large systematic uncertainties. Here, the most up to date measurement of the γ-ray spectrum of NGC 253 is investigated in both HE and VHE γ-rays. Assuming a hadronic origin of the γ-ray emission, the measurement uncertainties are propagated into the interpretation of the accelerated particle population. Methods: The data of H.E.S.S. observations are reanalysed using an updated calibration and analysis chain. The improved Fermi-LAT analysis employs more than 8 yr of data processed using pass 8. The cosmic-ray particle population is evaluated from the combined HE-VHE γ-ray spectrum using NAIMA in the optically thin case. Results: The VHE γ-ray energy spectrum is best fit by a power-law distribution with a flux normalisation of (1.34 ± 0.14<SUP>stat</SUP> ± 0.27<SUP>sys</SUP>) × 10<SUP>-13</SUP> cm<SUP>-2</SUP> s<SUP>-1</SUP> TeV<SUP>1</SUP> at 1 TeV - about 40% above, but compatible with the value obtained in Abramowski et al. (2012). The spectral index Γ = 2.39 ± 0.14<SUP>stat</SUP> ± 0.25<SUP>sys</SUP> is slightly softer than but consistent with the previous measurement within systematic errors. In the Fermi energy range an integral flux of F(E > 60 MeV) = (1.56 ± 0.28<SUP>stat</SUP> ± 0.15<SUP>sys</SUP>) × 10<SUP>-8</SUP> cm<SUP>-2</SUP> s<SUP>-1</SUP> is obtained. At energies above ∼3 GeV the HE spectrum is consistent with a power-law ranging into the VHE part of the spectrum measured by H.E.S.S. with an overall spectral index Γ = 2.22 ± 0.06<SUP>stat</SUP>. Conclusions: Two scenarios for the starburst nucleus are tested, in which the gas in the starburst nucleus acts as either a thin or a thick target for hadronic cosmic rays accelerated by the individual sources in the nucleus. In these two models, the level to which NGC 253 acts as a calorimeter is estimated to a range of f<SUB>cal</SUB> = 0.1 to 1 while accounting for the measurement uncertainties. The presented spectrum is likely to remain the most accurate measurements until the Cherenkov Telescope Array (CTA) has collected a substantial set of data towards NGC 253.
dc.affiliationUniwersytet Warszawski
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dc.contributor.authorVincent, P.
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dc.contributor.authorWagner, P.
dc.contributor.authorWagner, R. M.
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dc.contributor.authorWierzcholska, A.
dc.contributor.authorWörnlein, A.
dc.contributor.authorYang, R.
dc.contributor.authorZaborov, D.
dc.contributor.authorZacharias, M.
dc.contributor.authorZanin, R.
dc.contributor.authorZdziarski, A. A.
dc.contributor.authorZech, A.
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dc.date.accessioned2024-01-26T10:48:26Z
dc.date.available2024-01-26T10:48:26Z
dc.date.copyright2018-06-11
dc.date.issued2018
dc.description.accesstimeBEFORE_PUBLICATION
dc.description.financeNie dotyczy
dc.description.versionORIGINAL_AUTHOR
dc.description.volume617
dc.identifier.doi10.1051/0004-6361/201833202
dc.identifier.issn0004-6361
dc.identifier.urihttps://repozytorium.uw.edu.pl//handle/item/123169
dc.identifier.weblinkhttp://adsabs.harvard.edu/abs/2018A&A...617A..73H
dc.languageeng
dc.pbn.affiliationastronomy
dc.relation.ispartofAstronomy and Astrophysics
dc.relation.pagesA73
dc.rightsOther
dc.sciencecloudnosend
dc.titleThe starburst galaxy NGC 253 revisited by H.E.S.S. and Fermi-LAT
dc.typeJournalArticle
dspace.entity.typePublication