activity
20212023
most citedHandling Background in IXPE polarimetric data

137 citations · 528 across the 29 of their papers we have counts for

collaborators

15 papers

astro-ph.HE2023

Discovery of X-ray polarization angle rotation in active galaxy Mrk 421

Laura Di Gesu, Herman L. Marshall, Steven R. Ehlert +140

The magnetic field conditions in astrophysical relativistic jets can be probed by multiwavelength polarimetry, which has been recently extended to X-rays. For example, one can trac…

astro-ph.HE20235 cited

The First X-ray Polarization Observation of the Black Hole X-ray Binary 4U 1630-47 in the Steep Power Law State

Nicole Rodriguez Cavero, Lorenzo Marra, Henric Krawczynski +107

The Imaging X-ray Polarimetry Explorer (IXPE) observed the black hole X-ray binary 4U 1630-47 in the steep power law (or very high) state. The observations reveal a linear polariza…

astro-ph.HE20232 cited

The geometry of the hot corona in MCG-05-23-16 constrained by X-ray polarimetry

D. Tagliacozzo, A. Marinucci, F. Ursini +105

We report on the second observation of the radio-quiet active galactic nucleus (AGN) MCG-05-23-16 performed with the Imaging X-ray Polarimetry Explorer (IXPE). The observation star…

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.IM20233 cited

Equalizing the Pixel Response of the Imaging Photoelectric Polarimeter On-Board the IXPE Mission

John Rankin, Fabio Muleri, Alessandro Di Marco +18

The Gas Pixel Detector is a gas detector, sensitive to the polarization of X-rays, currently flying on-board IXPE - the first observatory dedicated to X-ray polarimetry. It detects…

astro-ph.HE202329 cited

IXPE observations of the quintessential wind-accreting X-ray pulsar Vela X-1

Sofia V. Forsblom, Juri Poutanen, Sergey S. Tsygankov +97

The radiation from accreting X-ray pulsars was expected to be highly polarized, with some estimates for the polarization degree of up to 80%. However, phase-resolved and energy-res…