activity
19952020
most citedThe XMM-Newton wide-field survey in the COSMOS field. The point-like X-ray source catalogue

294 citations · 1.3k across the 44 of their papers we have counts for

collaborators
Showing astro-phShow all

13 papers · 1 filter

astro-ph2008★ 75 cited

SPACE: the SPectroscopic All-sky Cosmic Explorer

A. Cimatti, M. Robberto, C. M. Baugh +18

We describe the scientific motivations, the mission concept and the instrumentation of SPACE, a class-M mission proposed for concept study at the first call of the ESA Cosmic-Visio…

astro-ph2006★ 10 cited

Rolling down from the 30 keV peak: modelling the hard X-ray and gamma-ray backgrounds

Andrea Comastri, Roberto Gilli, Guenther Hasinger

We will briefly discuss the importance of sensitive X-ray observations above a few tens of keV for a better understanding of the physical mechanisms associated to the Supermassive…

astro-ph2002★ 16 cited

BeppoSAX observations of LINER-2 galaxies

I. Georgantopoulos, F. Panessa, A. Akylas +3

We present BeppoSAX observations of 6 ``type-2'' LINER and ``transition'' galaxies (NGC3379, NGC3627, NGC4125, NGC4374, NGC5195 and NGC5879)from the Ho et al. (1997) spectroscopic…

astro-ph2001★ 36 cited

Disclosing the true nature of the Sy 2 galaxy NGC 3281: one more Compton-thick source

C. Vignali, A. Comastri

We present the BeppoSAX broad-band X-ray spectrum of the Seyfert 2 galaxy NGC 3281. The source high-energy spectrum is characterized by the nuclear transmitted component, with an a…

astro-ph2001

X-ray bright optically quiet galaxies: the case of P3

A. Comastri, M. Brusa, P. Ciliegi +10

Recent X-ray surveys have clearly demonstrated that a population of optically dull, X-ray bright galaxies is emerging at X-ray fluxes of the order of 10-14 erg cm-2 s-1. The nature…

astro-ph2001★ 139 cited

The HELLAS2XMM survey: I. The X-ray data and the Log(N)-Log(S)

A. Baldi, S. Molendi, A. Comastri +3

We present the first results from an XMM-Newton serendipitous medium-deep survey, which covers nearly three square degrees. We detect a total of 1022, 495 and 100 sources, down to…