activity
19962009
most citedThe Chandra COSMOS Survey, I: Overview and Point Source Catalog

445 citations · 2.6k across the 37 of their papers we have counts for

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Showing 2005Show all

9 papers · 1 filter

astro-ph2005

UBVRI Light Curves of 44 Type Ia Supernovae

Saurabh Jha, Robert P. Kirshner, Peter Challis +2

We present UBVRI photometry of 44 type-Ia supernovae (SN Ia) observed from 1997 to 2001 as part of a continuing monitoring campaign at the Fred Lawrence Whipple Observatory of the…

astro-ph2005

The HELLAS2XMM survey. VII. The hard X-ray luminosity function of AGN up to z=4: more absorbed AGN at low luminosities and high redshifts

F. La Franca, F. Fiore, A. Comastri +14

We have determined the cosmological evolution of the density of AGN and of their Nh distribution as a function of the un-absorbed 2-10 keV luminosity up to redshift 4. We used the…

astro-ph2005

Active and passive shielding design optimization and technical solutions for deep sensitivity hard X-ray focusing telescopes

G. Malaguti, G. Pareschi, P. Ferrando +12

The 10-100 keV region of the electromagnetic spectrum contains the potential for a dramatic improvement in our understanding of a number of key problems in high energy astrophysics…

astro-ph2005

SIMBOL-X, a formation flying-mission for hard X-ray astrophysics

P. Ferrando, A. Goldwurm, P. Laurent +13

SIMBOL-X is a hard X-ray mission, operating in the ~ 0.5-70 keV range, which is proposed by a consortium of European laboratories in response to the 2004 call for ideas of CNES for…

astro-ph2005

Extinction properties of the X-ray bright/optically faint afterglow of GRB 020405

G. Stratta, R. Perna, D. Lazzati +3

We present an optical-to-X-ray spectral analysis of the afterglow of GRB 020405. The optical spectral energy distribution not corrected for the extragalactic extinction is signific…

astro-ph2005

Probing the Local Group Medium Toward Mkn 421 with Chandra and FUSE

Rik J. Williams, Smita Mathur, Fabrizio Nicastro +7

We report the detection of highly-ionized gas at z~0 seen in resonant UV and X-ray absorption lines toward the z=0.03 blazar Mkn 421. A total of 13 X-ray and 3 UV lines were measur…