6 citations · 14 across the 9 of their papers we have counts for
10 papers
Joint X-ray and gamma-ray analysis at the photon level: Application to MSH 15-52
Katharina Egg, Alison M. W. Mitchell
Joint analysis of multi-wavelength (MWL) data at the level of photon events is challenging, but it provides a statistically preferable method of fitting the data, in contrast to fi…
Towards a joint X-ray and gamma-ray analysis of Pulsar Wind Nebulae with Gammapy
Katharina Egg, Alison M. W. Mitchell
For detailed studies of Pulsar Wind Nebulae (PWNe), objects that show photon emission across the entire electromagnetic spectrum, multiwavelength analyses are crucial. The comparis…
A catalogue of TeV pulsar environments
Tina Wach, Tim Linden, Alison M. W. Mitchell +1
Pulsars and their environments represent a major class of Galactic gamma-ray sources. Their complex evolution, shaped by the interactions of the pulsar outflow with the supernova r…
Joint eROSITA and H.E.S.S. analysis of MSH 15-52 using Gammapy
Katharina Egg, Alison M. W. Mitchell
Pulsar wind nebulae (PWNe) are prominent sources in the very-high energy (VHE) gamma-ray sky, constituting the most numerous identified source class in the H.E.S.S. Galactic Plane…
Analysis of the Supernova Remnant IC 443 using H.E.S.S. Data
Alison M. W. Mitchell, Lukas Grosspietsch, Tina Wach
IC 443 is a well-known supernova remnant that stands out due to its interaction with a dense molecular cloud, creating a complex environment where shocks can efficiently accelerate…
TeV Emission from PSR B1055-52 with HESS: Evidence for a Pulsar Halo
Tina Wach, Alison M. W. Mitchell
Pulsar halos are a recently identified class of TeV -ray sources, offering valuable insights into the evolution of pulsar systems at the highest energies. However, only a handfu…
A background-estimation technique for the detection of extended gamma-ray structures with IACTs
Tina Wach, Alison Mitchell, Lars Mohrmann
Estimation of the amount of cosmic-ray induced background events is a challenging task for Imaging Atmospheric Cherenkov Telescopes (IACTs). Most approaches rely on a model of the…
Pulsar Wind Nebulae
A. M. W. Mitchell, J. Gelfand
Pulsar Wind Nebulae (PWNe), structures powered by energetic pulsars, are known for their detection across the entire electromagnetic spectrum, with diverse morphologies and spectra…
Galactic Science with the Southern Wide-field Gamma-ray Observatory
R. López-Coto, A. Mitchell, E. O. Angüner +1
The Southern Wide-field Gamma-ray Observatory (SWGO) is a proposed ground-based gamma-ray detector that will be located in the Southern Hemisphere and is currently in its design ph…
Observations of the Pulsar Wind Nebula HESS J1825-137 with H.E.S.S. II
A. M. W. Mitchell, S. Caroff, R. D. Parsons +3
We present a new and deep analysis of the pulsar wind nebula (PWN) HESS\,J1825--137 with a comprehensive data set of almost 400 hours taken with the H.E.S.S. array between 2004 and…