activity
19972009
most citedThe Kormendy relation of massive elliptical galaxies at z~1.5. Evidence for size evolution ?

151 citations · 685 across the 24 of their papers we have counts for

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Showing 2004 · astro-phShow all

9 papers · 2 filters

astro-ph2004

The density of very massive evolved galaxies to z~1.7

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

We spectroscopically identified 7 massive evolved galaxies with magnitudes 17.8<K<18.4 at 1.3<z<1.7 over an area of ~160 arcmin^2 of the MUNICS survey. Their rest-frame K-band abso…

astro-ph2004

Looking for obscured QSOs in the X-ray emitting ERO population

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

We present XMM-Newton data centered on one of the MUNICS Near Infrared Cluster Survey fields (S2F1) and we discuss the X-ray properties of the 6 X-ray emitting EROs found. For one…

astro-ph2004

XMM-Newton spectroscopy of an X-ray selected sample of RL AGNs

E. Galbiati, A. Caccianiga, T. Maccacaro +6

This paper presents the X-ray spectroscopy of an X-ray selected sample of 25 radio-loud (RL) AGNs extracted from the XBSS sample. The main goal is to study the origin of the X-ray…

astro-ph2004

First XMM-Newton study of two Narrow-Line Seyfert 1 galaxies discovered in the Sloan Digital Sky Survey

L. Foschini, V. Braito, G. G. C. Palumbo +6

The Early Data Release of the Sloan Digital Sky Survey (SDSS) contains 150 Narrow-Line Seyfert 1 (NLS1) galaxies, most of them previously unknown. We present here the study of the…

astro-ph2004

X-ray properties of the "Composite" Seyfert/Star-forming galaxies

A. Wolter, G. Trinchieri, R. Della Ceca +7

An enigmatic, small class of IR and X-ray luminous sources, named ``Composite'' starburst/Seyfert galaxies, has been defined from IRAS and RASS data. The objects have optical spect…

astro-ph2004

Exploring the X-ray Sky with the XMM-Newton Bright Serendipitous Survey

R. Della Ceca, T. Maccacaro, A. Caccianiga +11

ABRIDGED. We present "The XMM-Newton Bright Serendipitous Survey", two flux-limited samples with flux limit fx ~7E-14 cgs in the 0.5-4.5 keV (BSS) and 4.5-7.5 keV (HBSS) energy ban…