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20102021
most citedSearch for photon line-like signatures from Dark Matter annihilations with H.E.S.S

251 citations · 952 across the 23 of their papers we have counts for

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Showing 2019Show all

11 papers · 1 filter

astro-ph.GA201932 cited

Radio Observations of Supernova Remnant G1.9+0.3

Kieran J. Luken, Miroslav D. Filipović, Nigel I. Maxted +18

We present 1 to 10GHz radio continuum flux density, spectral index, polarisation and Rotation Measure (RM) images of the youngest known Galactic Supernova Remnant (SNR) G1.9+0.3, u…

astro-ph.HE201912 cited

Radio Emission from Interstellar Shocks: Young Type Ia Supernova Remnants and the Case of N 103B in the Large Magellanic Cloud

R. Z. E. Alsaberi, L. A. Barnes, M. D. Filipovic +19

Here we present a radio continuum study based on new and archival data from the Australia Telescope Compact Array towards N 103B, a young (<=1000 yrs) spectroscopically confirmed t…

astro-ph.GA201929 cited

The ASKAP-EMU Early Science Project:Radio Continuum Survey of the Small Magellanic Cloud

T. D. Joseph, M. D. Filipović, E. J. Crawford +53

We present two new radio continuum images from the Australian Square Kilometre Array Pathfinder (ASKAP) survey in the direction of the Small Magellanic Cloud (SMC). These images ar…

astro-ph.HE2019

A Supernova Remnant Counterpart for HESS J1832-085

Nigel I. Maxted, M. D. Filipovic, N. Hurley-Walker +18

We examine the new Galactic supernova remnant (SNR) candidate, G23.11+0.18, as seen by the Murchison Widefield Array (MWA) radio telescope. We describe the morphology of the candid…

astro-ph.GA2019

ALMA CO Observations of a Giant Molecular Cloud in M33: Evidence for High-Mass Star Formation Triggered by Cloud-Cloud Collisions

Hidetoshi Sano, Kisetsu Tsuge, Kazuki Tokuda +14

We report the first evidence for high-mass star formation triggered by collisions of molecular clouds in M33. Using the Atacama Large Millimeter/submillimeter Array, we spatially r…

astro-ph.HE2019

Connecting the ISM to TeV PWNe and PWNe candidates

F. J. Voisin, G. P. Rowell, M. G. Burton +7

We investigate the interstellar medium (ISM) towards seven TeV gamma-ray sources thought to be pulsar wind nebulae (PWNe) using Mopra molecular line observations at 7mm [CS(1-0), S…