activity
20062009
most citedNew constraints on the Mid-IR EBL from the HESS discovery of VHE gamma rays from 1ES 0229+200

261 citations · 1.4k across the 14 of their papers we have counts for

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11 papers · 1 filter

astro-ph200834 cited

H.E.S.S. Observations of the Prompt and Afterglow Phases of GRB 060602B

HESS Collaboration, F. Aharonian

We report on the first completely simultaneous observation of a gamma-ray burst (GRB) using an array of Imaging Atmospheric Cherenkov Telescopes which is sensitive to photons in th…

astro-ph200887 cited

A Cosmic Ray Positron Anisotropy due to Two Middle-Aged, Nearby Pulsars?

I. Buesching, O. C. de Jager, M. S. Potgieter +1

Geminga and B0656+14 are the closest pulsars with characteristic ages in the ran ge of 100 kyr to 1 Myr. They both have spindown powers of the order 3e34 erg/s at present. The wind…

astro-ph200880 cited

Exploring a SNR/Molecular Cloud Association Within HESS J1745-303

HESS Collaboration, F. Aharonian

HESS J1745-303 is an extended, unidentified VHE (very high energy) gamma-ray source discovered using HESS in the Galactic Plane Survey. Since no obvious counterpart has previously…

astro-ph200824 cited

Estimating the birth period of pulsars through GLAST/LAT observations of their wind nebulae

O. C. de Jager

In this paper we show that the high energy -ray flux in the GeV domain from mature pulsar wind nebulae (PWN) scales as the change in rotational kinetic energy s…

astro-ph200865 cited

Discovery of VHE gamma-rays from the high-frequency-peaked BL Lac object RGB J0152+017

HESS Collaboration, F. Aharonian

Aims: The BL Lac object RGB J0152+017 (z=0.080) was predicted to be a very high-energy (VHE; > 100 GeV) gamma-ray source, due to its high X-ray and radio fluxes. Our aim is to unde…

astro-ph200714 cited

Discovery of an X-ray nebula around PSR J1718-3825 and implications for the nature of the gamma-ray source HESS J1718-385

J. A. Hinton, S. Funk, S. Carrigan +5

Combined X-ray synchrotron and inverse-Compton gamma-ray observations of pulsar wind nebulae (PWN) may help to elucidate the processes of acceleration and energy loss in these syst…