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Oxford University Press, Monthly Notices of the Royal Astronomical Society, 3(486), p. 3886-3891, 2019

DOI: 10.1093/mnras/stz1031

arXiv, 2019

DOI: 10.48550/arxiv.1904.05139

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H.E.S.S. observations of the flaring gravitationally lensed galaxy PKS 1830-211

Journal article published in 2019 by N. Żywucka, P. deWilt, M. de Naurois, D. J. van der Walt, C. van Rensburg, C. van Eldik, B. van Soelen, N. Zywucka, F. Ait Benkhali, :., E. O. Anguener, F. Aharonian ORCID, J. Becker Tjus, H. Abdalla, M. Arakawa and other authors.
This paper is made freely available by the publisher.
This paper is made freely available by the publisher.

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Data provided by SHERPA/RoMEO

Abstract

PKS 1830-211 is a known macrolensed quasar located at a redshift of z=2.5. Its high-energy gamma-ray emission has been detected with the Fermi-LAT instrument and evidence for lensing was obtained by several authors from its high-energy data. Observations of PKS 1830-211 were taken with the H.E.S.S. array of Imaging Atmospheric Cherenkov Telescopes in August 2014, following a flare alert by the Fermi- LAT collaboration. The H.E.S.S observations were aimed at detecting a gamma-ray flare delayed by 20-27 days from the alert flare, as expected from observations at other wavelengths. More than twelve hours of good quality data were taken with an analysis threshold of $∼67$ GeV. The significance of a potential signal is computed as a function of the date as well as the average significance over the whole period. Data are compared to simultaneous observations by Fermi-LAT. No photon excess or significant signal is detected. An upper limit on PKS 1830-211 flux above 67 GeV is computed and compared to the extrapolation of the Fermi-LAT flare spectrum.