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The [OIII] emission line luminosity function of optically selected type-2 AGN from zCOSMOS
A. Bongiorno, M. Mignoli, G. Zamorani +61
We present a catalog of 213 type-2 AGN selected from the zCOSMOS survey. The selected sample covers a wide redshift range (0.15<z<0.92) and is deeper than any other previous study,…
Multi-wavelength study of XMMU J2235.3-2557: the most massive galaxy cluster at z > 1
P. Rosati, P. Tozzi, R. Gobat +14
[Abridged] XMMU J2235.3-2557 is one of the most distant X-ray selected clusters, spectroscopically confirmed at z=1.39. We characterize the galaxy populations of passive members, t…
The 10k zCOSMOS: morphological transformation of galaxies in the group environment since z~1
K. Kovac, S. J. Lilly, C. Knobel +57
We study the evolution of galaxies inside and outside of the group environment since z=1 using a large well defined set of groups and galaxies from the zCOSMOS-bright redshift surv…
K+a galaxies in the zCOSMOS Survey: Physical properties of systems in their post-starburst phase
D. Vergani, G. Zamorani, S. J. Lilly +59
The identities of the main processes triggering and quenching star-formation in galaxies remain unclear. A key stage in evolution, however, appears to be represented by post-starbu…
zCOSMOS - 10k-bright spectroscopic sample. The bimodality in the Galaxy Stellar Mass Function: exploring its evolution with redshift
L. Pozzetti, M. Bolzonella, E. Zucca +56
We present the Galaxy Stellar Mass Function (MF) up to z~1 from the zCOSMOS-bright 10k spectroscopic sample. We investigate the total MF and the contribution of ETGs and LTGs, defi…
Tracking the impact of environment on the Galaxy Stellar Mass Function up to z~1 in the 10k zCOSMOS sample
M. Bolzonella, K. Kovac, L. Pozzetti +63
We study the impact of the environment on the evolution of galaxies in the zCOSMOS 10k sample in the redshift range 0.1<z<1.0 over an area of ~1.5 deg2. The considered sample of se…
A massive star origin for an unusual helium-rich supernova in an elliptical galaxy
K. S. Kawabata, K. Maeda, K. Nomoto +6
The unusual helium-rich (type Ib) supernova SN 2005E is distinguished from any supernova hitherto observed by its faint and rapidly fading light curve, prominent calcium lines in l…