activity
20072023
most citedThe Fluorescence Detector of the Pierre Auger Observatory

380 citations · 2.9k across the 66 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

22 papers · 1 filter

astro-ph.HE2023

EMU Detection of a Large and Low Surface Brightness Galactic SNR G288.8-6.3

Miroslav D. Filipović, Shi Dai, Bojan Arbutina +36

We present the serendipitous detection of a new Galactic Supernova Remnant (SNR), G288.8-6.3 using data from the Australian Square Kilometre Array Pathfinder (ASKAP)-Evolutionary M…

astro-ph.HE2022★ 13 cited

New ASKAP Radio Supernova Remnants and Candidates in the Large Magellanic Cloud

Luke M. Bozzetto, Miroslav D. Filipović, H. Sano +34

We present a new Australian Square Kilometre Array Pathfinder (ASKAP) sample of 14 radio Supernova Remnant (SNR) candidates in the Large Magellanic Cloud (LMC). This new sample is…

astro-ph.HE2022★ 36 cited

Mysterious Odd Radio Circle near the Large Magellanic Cloud -- An Intergalactic Supernova Remnant?

Miroslav D. Filipović, J. L. Payne, R. Z. E. Alsaberi +48

We report the discovery of J0624-6948, a low-surface brightness radio ring, lying between the Galactic Plane and the Large Magellanic Cloud (LMC). It was first detected at 888 MHz…

astro-ph.HE2020★ 14 cited

New high-frequency radio observations of the Cygnus Loop supernova remnant with the Italian radio telescopes

S. Loru, A. Pellizzoni, E. Egron +19

Supernova remnants (SNRs) represent a powerful laboratory to study the Cosmic-Ray acceleration processes at the shocks, and their relation to the properties of the circumstellar me…

astro-ph.HE2015★ 36 cited

Measurement of the cosmic ray spectrum above eV using inclined events detected with the Pierre Auger Observatory

The Pierre Auger Collaboration, Alexander Aab, Pedro Abreu +461

A measurement of the cosmic-ray spectrum for energies exceeding eV is presented, which is based on the analysis of showers with zenith angles greater than $60^{\…

astro-ph.HE2014★ 309 cited

Depth of Maximum of Air-Shower Profiles at the Pierre Auger Observatory: Composition Implications

Pierre Auger Collaboration

Using the data taken at the Pierre Auger Observatory between December 2004 and December 2012, we have examined the implications of the distributions of depths of atmospheric shower…