activity
20002004
most citedThe HELLAS2XMM 1dF survey: on the nature of high X-ray to optical flux ratio sources

1 citations · 1 across the 5 of their papers we have counts for

collaborators

10 papers

astro-ph2004

The broad-band properties of the XMM-Newton Bright Serendipitous Sources

R. Della Ceca, T. Maccacaro, A. Caccianiga +2

We present here "The XMM-Newton Bright Serendipitous Survey", a survey program conducted by the XMM-Newton Survey Science Center. In particular we discuss the main goals of this pr…

astro-ph2003

The TESIS project: Are type 2 QSO hidden in X-ray emitting EROs?

P. Severgnini, R. Della Ceca, V. Braito +8

Here we present the results obtained from the analysis of 75 ksec of XMM-Newton observations of a sample of EROs selected from one MUNICS field (K'<19.5 mag). We find 6 EROs with a…

astro-ph2003

The TESIS project: revealing massive early-type galaxies at z>1

P. Saracco, M. Longhetti, P. Severgnini +8

We present the preliminary results of an on-going near-IR low resolution spectroscopic follow-up of a complete sample of 30 bright (K'<18.5) EROs selected over 360 arcmin^2 from th…

astro-ph20031 cited

The HELLAS2XMM 1dF survey: on the nature of high X-ray to optical flux ratio sources

F. Fiore, M. Brusa, F. Cocchia +12

We present results from the photometric and spectroscopic identification of 122 X-ray sources discovered by XMM-Newton in the 2-10 keV band (the HELLAS2XMM 1dF sample). One of the…

astro-ph2003

The Ultra Luminous Infrared Galaxy MKN 231: New clues from BeppoSAX and XMM-Newton

V. Braito, R. Della Ceca, E. Piconcelli +11

We present BeppoSAX and XMM-Newton observations of MKN 231. These observations and in particular the BeppoSAX PDS data allowed us to unveil, for the first time, the highly absorbed…

astro-ph2002

On the nature of X-ray Bright Optically Normal galaxies

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

Multiwavelength observations of the hard X-ray selected sources by Chandra and XMM-Newton surveys have significantly improved our knowledge of the objects responsible of the hard X…