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VHE gamma-ray discovery and multi-wavelength study of the blazar 1ES 2322-409

MPS-Authors
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Aharonian,  F.
Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society;

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Ait Benkhali,  Faical
Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society;

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Bernloehr,  K.
Division Prof. Dr. James A. Hinton, MPI for Nuclear Physics, Max Planck Society;

/persons/resource/persons30369

Casanova,  Sabrina
Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society;

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Deil,  C.
Division Prof. Dr. James A. Hinton, MPI for Nuclear Physics, Max Planck Society;

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Donath,  Axel
Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society;

/persons/resource/persons30555

Hahn,  Joachim
Division Prof. Dr. James A. Hinton, MPI for Nuclear Physics, Max Planck Society;

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Hermann,  German
Division Prof. Dr. James A. Hinton, MPI for Nuclear Physics, Max Planck Society;

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Hinton,  J. A.
Division Prof. Dr. James A. Hinton, MPI for Nuclear Physics, Max Planck Society;

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Hofmann,  W.
Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society;

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Marandon,  Vincent
Division Prof. Dr. James A. Hinton, MPI for Nuclear Physics, Max Planck Society;

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Marx,  Ramin
Division Prof. Dr. James A. Hinton, MPI for Nuclear Physics, Max Planck Society;

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Mitchell,  A.
Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society;

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Panter,  M.
Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society;

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Parsons,  R. D.
Division Prof. Dr. James A. Hinton, MPI for Nuclear Physics, Max Planck Society;

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Rieger,  F.
Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society;

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Ruiz Velasco,  E.
Division Prof. Dr. James A. Hinton, MPI for Nuclear Physics, Max Planck Society;

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Tuffs,  R.
Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society;

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Völk,  H.J.
Prof. Heinrich J. Völk, Emeriti, MPI for Nuclear Physics, Max Planck Society;

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White,  R.
Division Prof. Dr. James A. Hinton, MPI for Nuclear Physics, Max Planck Society;

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Yang,  Rui-zhi
Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society;

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Zanin,  R.
Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society;

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1810.04641.pdf
(Preprint), 990KB

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Citation

H.E.S.S. Collaboration, Abdalla, H., Aharonian, F., Ait Benkhali, F., Angüner, E. O., Arakawa, M., et al. (2018). VHE gamma-ray discovery and multi-wavelength study of the blazar 1ES 2322-409. Monthly Notices of the Royal Astronomical Society, 482(3), 3011-3022. doi:10.1093/mnras/sty2686.


Cite as: https://hdl.handle.net/21.11116/0000-0004-F8FA-B
Abstract
A hotspot at a position compatible with the BL Lac object 1ES 2322-409 was
serendipitously detected with H.E.S.S. during observations performed in 2004
and 2006 on the blazar PKS 2316-423. Additional data on 1ES 2322-409 were taken
in 2011 and 2012, leading to a total live-time of 22.3h. Point-like
very-high-energy (VHE; E>100GeV) $\gamma$-ray emission is detected from a
source centred on the 1ES 2322-409 position, with an excess of 116.7 events at
a significance of 6.0$\sigma$. The average VHE $\gamma$-ray spectrum is well
described with a power law with a photon index
$\Gamma=3.40\pm0.66_{\text{stat}}\pm0.20_{\text{sys}}$ and an integral flux
$\Phi(E>200GeV) = (3.11\pm0.71_{\rm stat}\pm0.62_{\rm sys})\times10^{-12}
cm^{-2} s^{-1}$, which corresponds to 1.1$\%$ of the Crab nebula flux above 200
GeV. Multi-wavelength data obtained with Fermi LAT, Swift XRT and UVOT, RXTE
PCA, ATOM, and additional data from WISE, GROND and Catalina, are also used to
characterise the broad-band non-thermal emission of 1ES 2322-409. The
multi-wavelength behaviour indicates day-scale variability. Swift UVOT and XRT
data show strong variability at longer scales. A spectral energy distribution
(SED) is built from contemporaneous observations obtained around a high state
identified in Swift data. A modelling of the SED is performed with a stationary
homogeneous one-zone synchrotron-self-Compton (SSC) leptonic model. The
redshift of the source being unknown, two plausible values were tested for the
modelling. A systematic scan of the model parameters space is performed,
resulting in a well-constrained combination of values providing a good
description of the broad-band behaviour of 1ES 2322-409.