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Observations of the Crab Nebula with H.E.S.S. Phase II · Around

2015

Observations of the Crab Nebula with H.E.S.S. Phase II

Holler, M., Berge, D., van Eldik, C. et al.

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Understand

The High Energy Stereoscopic System (H.E.S.S.) phase I instrument was an array of four $100\,\mathrm{m}^2$ mirror area Imaging Atmospheric Cherenkov Telescopes (IACTs) that has very successfully mapped the sky at photon energies above $\sim 100\,$GeV.

Recently, a $600\,\mathrm{m}^2$ telescope was added to the centre of the existing array, which can be operated either in standalone mode or jointly with the four smaller telescopes.
The large telescope lowers the energy threshold for gamma-ray observations to several tens of GeV, making the array sensitive at energies where the Fermi-LAT instrument runs out of statistics.
At the same time, the new telescope makes the H.E.S.S.

Built on

S. Funk, G. Hermann, J. Hinton, D. Berge, K. Bernlöhr, W. Hofmann, P. Nayman, F. Toussenel, and P. Vincent, The trigger system of the H.E.S.S. telescope array
2004
Earlier work this paper cites.
F. Aharonian et al., Observations of the Crab nebula with HESS
2006
Earlier work this paper cites.
D. Berge et al., Background modelling in very-high-energy gamma-ray astronomy
2007
Earlier work this paper cites.
M. Holler et al., Photon reconstruction for H.E.S.S. using a semi-analytical shower model
2015
Earlier work this paper cites.

Similar

T. Murach et al., A Neural Network-Based Monoscopic Reconstruction Algorithm for H.E.S.S. II
2015
Cited alongside, same era.
D. Parsons et al., H.E.S.S. II Data Analysis with ImPACT
2015
Cited alongside, same era.
J. Aleksić et al., Measurement of the Crab Nebula spectrum over three decades in energy with the MAGIC telescopes
2015
Cited alongside, same era.

Then

K. Meagher et al., Six years of VERITAS observations of the Crab Nebula
2015
Closest in time.
D. Zaborov et al., AGN observations with a less than 100 GeV threshold using H.E.S.S. II
2015
Closest in time.
M. Gajdus et al., Pulsations from the Vela Pulsar down to 20 GeV with H.E.S.S. II
2015
Closest in time.

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