We ask for two INTEGRAL ToO observations of 600 ks each coordinated with the Imaging X-ray PolarimetryExplorer (IXPE)a recently launched NASA mission devoted to X-ray polarimetry. The aim of this prop
Identifying active galactic nuclei (AGNs) through their X-ray emission is efficient, but necessarily biased against X-ray-faint objects. We aim to characterize this bias by...
The Spiral Planetary Nebula (NGC 5189), exhibits spectacular pointsymmetricmorphology indicative of a number of collimated outflows. The WO1 central starhas lost its hydrogenrich envelope, possibly th
CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observation