activity
19962016
most citedThe Chandra COSMOS Legacy survey: overview and point source catalog

511 citations · 1.1k across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2016★ 511 cited

The Chandra COSMOS Legacy survey: overview and point source catalog

F. Civano, S. Marchesi, A. Comastri +39

The COSMOS-Legacy survey is a 4.6 Ms Chandra program that has imaged 2.2 deg of the COSMOS field with an effective exposure of 160 ks over the central 1.5 deg and o…

astro-ph.HE2013★ 10 cited

The XMM-Newton spectrum of a candidate recoiling supermassive black hole: an elusive inverted P-Cygni profile

G. Lanzuisi, F. Civano, S. Marchesi +12

We present a detailed spectral analysis of new XMM-Newton data of the source CXOC J100043.1+020637, also known as CID-42, detected in the COSMOS survey at z = 0.359. Previous works…

astro-ph.CO2012★ 59 cited

Chandra High resolution Observations of CID-42, a candidate recoiling SMBH

F. Civano, M. Elvis, G. Lanzuisi +15

We present Chandra High Resolution Camera observations of CID-42, a candidate recoiling supermassive black hole (SMBH) at z=0.359 in the COSMOS survey. CID-42 shows two optical com…

astro-ph.HE2009★ 294 cited

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

N. Cappelluti, M. Brusa, G. Hasinger +24

The COSMOS survey is a multiwavelength survey aimed to study the evolution of galaxies, AGN and the large scale structure. The XMM-COSMOS is a deep X-ray survey over the full 2 deg…

astro-ph2000★ 64 cited

Chandra study of an overdensity of X-ray sources around two distant (z~0.5) clusters

M. Cappi, P. Mazzotta, M. Elvis +21

We present results from a Chandra X-ray Observatory study of the field X-ray source populations in 4 different observations: two high-redshift (z~0.5) clusters of galaxies 3C295 an…

astro-ph1998★ 105 cited

The swan song: the disappearance of the nucleus of NGC 4051 and the echo of its past glory

M. Guainazzi, F. Nicastro, F. Fiore +10

BeppoSAX observed the low-luminous Seyfert 1 Galaxy NGC4051 in a ultra-dim X-ray state. The 2-10 keV flux (1.26 x 10^{-12} erg/cm^2/s) was about 20 times fainter than its historica…