activity
20142024
most citedVela pulsar wind nebula x-rays are polarized to near the synchrotron limit

56 citations · 110 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2024

Analysis of Crab X-ray Polarization using Deeper IXPE Observations

Josephine Wong, Tsunefumi Mizuno, Niccoló Bucciantini +98

We present Crab X-ray polarization measurements using IXPE data with a total exposure of 300ks, three times more than the initial 2022 discovery paper. Polarization is detected in…

astro-ph.HE2024

Revisit the Emission Polarization of the Internal-shock for the blazars' Jet

Hao-Qiang Zhang, Da-Bin Lin, Kuan Liu +1

Recent Imaging X-ray Polarimetry Explorer (IXPE) observations of blazars tend to support the shock model for the X-ray emission, but report a low polarization degree ()…

astro-ph.HE2024

First detection of polarization in X-rays for PSR B0540-69 and its nebula

Fei Xie, Josephine Wong, Fabio La Monaca +100

We report on X-ray polarization measurements of the extra-galactic Crab-like PSR B0540-69 and its Pulsar Wind Nebula (PWN) in the Large Magellanic Cloud (LMC), using a ~850 ks Imag…

astro-ph.HE202356 cited

Vela pulsar wind nebula x-rays are polarized to near the synchrotron limit

Fei Xie, Alessandro Di Marco, Fabio La Monaca +90

Pulsar wind nebulae are formed when outflows of relativistic electrons and positrons hit the surrounding supernova remnant or interstellar medium at a shock front. The Vela pulsar…

astro-ph.IM2016

Pulsar observations with European telescopes for testing gravity and detecting gravitational waves

D. Perrodin, C. G. Bassa, G. H. Janssen +20

A background of nanohertz gravitational waves from supermassive black hole binaries could soon be detected by pulsar timing arrays, which measure the times-of-arrival of radio puls…

astro-ph.IM201454 cited

Model-based asymptotically optimal dispersion measure correction for pulsar timing

K. J. Lee, C. G. Bassa, G. H. Janssen +8

In order to reach the sensitivity required to detect gravitational waves, pulsar timing array experiments need to mitigate as much noise as possible in timing data. A dominant amou…