Alessandra De Rosa

TL;DR: The enhanced X-ray Timing and Polarimetry mission—eXTP is a space science mission designed to study fundamental physics under extreme conditions of density, gravity and magnetism and will be a very powerful observatory for astrophysics that will provide observations of unprecedented quality on a variety of galactic and extragalactic objects.

TL;DR: The X-ray Imaging Polarimetry Explorer (XIPE) as mentioned in this paper was proposed in 2012 to the first ESA call for a small mission with a launch in 2017, but the proposal was, unfortunately, not selected.

TL;DR: In this article, a review describes the techniques used across the electromagnetic spectrum to detect dual active galactic nuclei (AGN) candidates and proposes new avenues for their search, compared with the state-of-the-art numerical simulations and models for formation of dual and binary AGN.

TL;DR: The enhanced X-ray Timing and Polarimetry (eXTP) mission as discussed by the authors is a space science mission designed to study fundamental physics under extreme conditions of density, gravity and magnetism.

TL;DR: The X-ray Imaging Polarimetry Explorer (XIPE) as mentioned in this paper is composed of two out of the three existing JET-X telescopes with two Gas Pixel Detectors (GPDs) filled with a He-DME mixture at their focus, and two additional GPDs filled with pressurized Ar DME facing the sun.