M. Perri

TL;DR: Swift_deepsky as discussed by the authors is a data analysis pipeline based on the Swift XRTDAS software and the XIMAGE package, encapsulated into a Docker container, which downloads and reads low-level data, generates higher-level products, detects X-ray sources and estimates several intensity and spectral parameters for each detection.

TL;DR: In this article, the authors investigate whether there is any correlation between the X-ray afterglow luminosity and the prompt emission properties of a carefully selected sub-sample of bright Swift long Gamma-Ray Bursts nearly complete in redshift (~90%).

TL;DR: In this article, a homogeneous analysis of all 318 Gamma Ray Bursts detected by the X-ray Telescope on the Swift satellite up to 2008 July 23 is presented, and the results of their analysis of GRBs, including probability distribution functions of the temporal and spectral properties of the sample.

TL;DR: In this paper, the authors analyse the light curve in the R band of the blazar OJ287, gathered during the 2015/2016 observing season, and search for quasi-periodic oscillations (QPOs) using several methods over a wide range of timescales.

TL;DR: In this article , a polarimetric observation of the X-ray binary Cygnus X-1 using the Imaging Xray Polarimetry Explorer (IXPEL) was performed, showing that hot x-ray emitting plasma is spatially extended in a plane perpendicular to, not parallel to, the jet axis.