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M. Del Santo

Researcher at INAF

Publications -  183
Citations -  3764

M. Del Santo is an academic researcher from INAF. The author has contributed to research in topics: Neutron star & Luminosity. The author has an hindex of 33, co-authored 174 publications receiving 3375 citations. Previous affiliations of M. Del Santo include Technical University of Denmark & University of Southampton.

Papers
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MonographDOI

Science with the Cherenkov Telescope Array

B. S. Acharya, +580 more
TL;DR: The Cherenkov Telescope Array (CTA) as mentioned in this paper is the major global observatory for very high energy gamma-ray astronomy over the next decade and beyond, covering a huge range in photon energy from 20 GeV to 300 TeV.
Proceedings ArticleDOI

XIPE: the x-ray imaging polarimetry explorer

P. Soffitta, +421 more
- 01 Jan 2016 - 
TL;DR: The X-ray Imaging Polarimetry Explorer (XIPE) as discussed by the authors is a mission dedicated to Xray Astronomy which is in a competitive phase A as fourth medium size mission of ESA (M4).
Journal ArticleDOI

The First IBIS/ISGRI Soft Gamma-Ray Galactic Plane Survey Catalog*

TL;DR: The first high-energy survey catalog obtained with the IBIS gamma-ray imager on board INTEGRAL is reported in this article, which reveals the presence of ~120 sources with the unprecedented sensitivity of ~1 mcrab in the energy range 20-100 keV.
Journal ArticleDOI

Science with e-ASTROGAM (A space mission for MeV-GeV gamma-ray astrophysics)

A. De Angelis, +249 more
TL;DR: e-ASTROGAM (enhanced ASTROGAM) as mentioned in this paper is a breakthrough Observatory space mission, with a detector composed by a Silicon tracker, a calorimeter, and an anticoincidence system, dedicated to the study of the non-thermal Universe in the photon energy range from 0.3 MeV to 3 GeV.
Journal ArticleDOI

The INTEGRAL IBIS/ISGRI System Point Spread Function and source location accuracy

TL;DR: In this article, the authors used the first in-flight calibration data on strong sources for the IBIS/ISGRI system to evaluate the dependence of the calibrated location accuracy with the signal-to-noise ratio of the sources.