activity
20002023
most citedFermi Large Area Telescope Second Source Catalog

1.3k citations · 32.4k across the 218 of their papers we have counts for

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Showing 2006Show all

6 papers · 1 filter

astro-ph2006★ 131 cited

A Sealed Gas Pixel Detector for X-ray Astronomy

R. Bellazzini, G. Spandre, M. Minuti +13

We report on the results of a new, sealed, Gas Pixel Detector. The very compact design and the absence of the gas flow system, make this detector substantially ready for use as foc…

astro-ph2006★ 8 cited

POLARIX: a small mission of x-ray polarimetry

Enrico Costa, Ronaldo Bellazzini, Paolo Soffitta +24

X-Ray Polarimetry can be now performed by using a Micro Pattern Gas Chamber in the focus of a telescope. It requires large area optics for most important scientific targets. But si…

astro-ph2006★ 4 cited

An X-ray polarimeter for hard X-ray optics

Fabio Muleri, Ronaldo Bellazzini, Enrico Costa +23

Development of multi-layer optics makes feasible the use of X-ray telescope at energy up to 60-80 keV: in this paper we discuss the extension of photoelectric polarimeter based on…

astro-ph2006★ 5 cited

A photoelectric polarimeter for XEUS: a new window in x-ray sky

Ronaldo Bellazzini, Luca Baldini, Francesco Bitti +18

XEUS is a large area telescope aiming to rise X-ray Astronomy to the level of Optical Astronomy in terms of collecting areas. It will be based on two satellites, locked on a format…

physics.ins-det2006★ 118 cited

Direct reading of charge multipliers with a self-triggering CMOS analog chip with 105k pixels at 50 micron pitch

R. Bellazzini, G. Spandre, M. Minuti +10

We report on a large active area (15x15mm2), high channel density (470 pixels/mm2), self-triggering CMOS analog chip that we have developed as pixelized charge collecting electrode…

astro-ph2006★ 1 cited

Opening a New Window to Fundamental Physics and Astrophysics: X-ray Polarimetry

E. Costa, R. Bellazzini, P. Soffitta +25

An extensive theoretical literature predicts that X-ray Polarimetry can directly determine relevant physical and geometrical parameters of astrophysical sources, and discriminate b…