2 citations · 2 across the 3 of their papers we have counts for
23 papers
EXPO: a quantum leap in fast, wide-band X-ray polarimetry for astrophysics
Paolo Soffitta, Sebastien Guillot, Ian Hutchinson +137
The Enhanced X-ray Polarimetry Observatory (EXPO) is a mission concept proposed to ESA as an M8 candidate, with a prospective launch in 2041. Building on the scientific success of…
Population synthesis of Galactic middle-aged pulsar wind nebulae I. Detection prospects for current and future instruments
A. De Sarkar, D. F. Torres, B. Olmi +2
Pulsar wind nebulae (PWNe) constitute the largest population of Galactic very-high-energy (VHE; GeV) -ray sources and are key laboratories for studying particle accel…
A thick-shell formalism for pulsar wind nebulae based on energy conservation
N. Bucciantini, B. Olmi
One of the most powerful approaches to model the structural and spectral evolution of wind bubbles, and pulsar wind nebulae in particular, is based on the one-zone thin-shell forma…
Kes 75 with IXPE: Detection of Nebular X-ray Polarization and Change in Pulsar Lightcurve
Josephine Wong, Jack T. Dinsmore, Roger W. Romani +16
We present the first X-ray polarization measurements of the PSR/PWN complex within SNR Kes 75. Two IXPE observations were conducted in October/November 2024 a…
Modelling the Dynamics of Middle-Aged Pulsar Wind Nebulae in the Reverberation Phase
Yuri Batini, Niccolò Bucciantini
Pulsar Wind Nebulae (PWNe) are among the most important sources emitting in the very-high-energy gamma-ray band. Predicting their long-term evolution is crucial for forthcoming hig…
Old pulsar wind nebulae and the role of the thermal filaments
N. Bucciantini, Y. Batini, B. Olmi
Old pulsar wind nebulae are among the foremost galactic high-energy gamma-ray sources. However we still lack a robust approach to their modeling, especially in the light of forthco…