activity
19942022
most citedImproved constraints on the expansion rate of the Universe up to z~1.1 from the spectroscopic evolution of cosmic chronometers

1k citations · 6k across the 57 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

38 papers · 1 filter

astro-ph.CO2014★ 1 cited

CFHTLenS: Weak lensing calibrated scaling relations for low mass clusters of galaxies

K. Kettula, S. Giodini, E. van Uitert +24

We present weak lensing and X-ray analysis of 12 low mass clusters from the CFHTLenS and XMM-CFHTLS surveys. We combine these systems with high-mass systems from CCCP and low-mass…

astro-ph.CO2013★ 43 cited

Reversal or no reversal: the evolution of the star formation rate-density relation up to z~1.6

F. Ziparo, P. Popesso, A. Finoguenov +27

We investigate the evolution of the star formation rate (SFR)-density relation in the Extended Chandra Deep Field South (ECDFS) and the Great Observatories Origin Deep Survey (GOOD…

astro-ph.CO2013★ 12 cited

A Normal Abundance of Faint Satellites in the Fossil Group NGC 6482

S. Lieder, S. Mieske, R. Sánchez-Janssen +3

Fossil groups are considered the end product in a galaxy group's evolution -- a massive central galaxy that dominates the luminosity budget of the group, as the outcome of efficien…

astro-ph.CO2013★ 141 cited

The dependence of Galactic outflows on the properties and orientation of zCOSMOS galaxies at z ~ 1

R. Bordoloi, S. J. Lilly, E. Hardmeier +44

We present an analysis of cool outflowing gas around galaxies, traced by MgII absorption lines in the co-added spectra of a sample of 486 zCOSMOS galaxies at 1 < z < 1.5. These gal…

astro-ph.CO2013★ 102 cited

zCOSMOS 20k: Satellite galaxies are the main drivers of environmental effects in the galaxy population at least to z~0.7

K. Kovac, S. J. Lilly, C. Knobel +41

We explore the role of environment in the evolution of galaxies over 0.1<z<0.7 using the final zCOSMOS-bright data set. Using the red fraction of galaxies as a proxy for the quench…

astro-ph.CO2013★ 34 cited

The lack of star formation gradients in galaxy groups up to z~1.6

Felicia Ziparo, Paola Popesso, Andrea Biviano +28

In the local Universe, galaxy properties show a strong dependence on environment. In cluster cores, early type galaxies dominate, whereas star-forming galaxies are more and more co…

astro-ph.CO2013★ 92 cited

Larger sizes of massive quiescent early-type galaxies in clusters than in the field at 0.8 < z < 1.5

L. Delaye, M. Huertas-Company, S. Mei +13

[abridged] The mass-size relation of early-type galaxies (ETGs) has been largely studied in the last years to probe the mass assembly of the most massive objects in the Universe. I…

astro-ph.CO2013★ 73 cited

Obscured AGN at z~1 from the zCOSMOS-Bright Survey I. Selection and Optical Properties of a [Ne v]-selected sample

M. Mignoli, C. Vignali, R. Gilli +46

A sample of 94 narrow line AGN with 0.65<z<1.20 has been selected from the 20k-Bright zCOSMOS galaxy sample by detection of the high-ionization [NeV]3426 line. Taking advantage of…

astro-ph.CO2013★ 35 cited

Dust-obscured star-formation in the outskirts of XMMU J2235.3-2557, a massive galaxy cluster at z=1.4

J. S. Santos, B. Altieri, P. Popesso +17

Star-formation in the galaxy populations of local massive clusters is reduced with respect to field galaxies, and tends to be suppressed in the core region. Indications of a revers…

astro-ph.CO2013★ 92 cited

Spot the difference. Impact of different selection criteria on observed properties of passive galaxies in zCOSMOS 20-k sample

M. Moresco, L. Pozzetti, A. Cimatti +50

We present the analysis of photometric, spectroscopic, and morphological properties for differently selected samples of passive galaxies up to z=1 extracted from the zCOSMOS-20k sp…

astro-ph.CO2012★ 59 cited

The Colors of Central and Satellite Galaxies in zCOSMOS out to z ~ 0.8 and Implications for Quenching

C. Knobel, S. J. Lilly, K. Kovac +47

We examine the red fraction of central and satellite galaxies in the large zCOSMOS group catalog out to z ~ 0.8 correcting for both the incompleteness in stellar mass and for the l…

astro-ph.CO2012★ 61 cited

Proto-groups at 1.8<z<3 in the zCOSMOS-deep sample

C. Diener, S. J. Lilly, C. Knobel +48

We identify 42 candidate groups lying between 1.8<z<3.0 from a sample of 3502 galaxies with spectroscopic redshifts in the zCOSMOS-deep redshift survey within the same redshift int…

astro-ph.CO2012★ 110 cited

The cosmic evolution of oxygen and nitrogen abundances in star-forming galaxies over the past 10 Gyrs

E. Perez-Montero, T. Contini, F. Lamareille +35

The chemical evolution of galaxies on a cosmological timescale is still a matter of debate despite the increasing number of available data provided by spectroscopic surveys of star…

astro-ph.CO2012★ 76 cited

Occupation of X-ray selected galaxy groups by X-ray AGN

V. Allevato, A. Finoguenov, G. Hasinger +12

We present the first direct measurement of the mean Halo Occupation Distribution (HOD) of X-ray selected AGN in the COSMOS field at z < 1, based on the association of 41 XMM and 17…

astro-ph.CO2012★ 62 cited

Deep observations of CO line emission from star-forming galaxies in a cluster candidate at z=1.5

M. Aravena, C. L. Carilli, M. Salvato +20

We report results from a deep Jansky Very Large Array (JVLA) search for CO 1-0 line emission from galaxies in a candidate galaxy cluster at z~1.55 in the COSMOS field. We target 4…

astro-ph.CO2012★ 237 cited

Stellar velocity dispersions and emission line properties of SDSS-III/BOSS galaxies

D. Thomas, O. Steele, C. Maraston +24

We perform a spectroscopic analysis of 492,450 galaxy spectra from the first two years of observations of the Sloan Digital Sky Survey-III/Baryonic Oscillation Spectroscopic Survey…

astro-ph.CO2012

Environmental effects in the interaction and merging of galaxies in zCOSMOS survey

P. Kampczyk, S. J. Lilly, the zCOSMOS Collaboration

The zCOSMOS-bright 10k spectroscopic sample reveals a strong environmental dependence of close kinematic galaxy pair fractions in the redshift range 0.2 < z < 1. The fraction of cl…

astro-ph.CO2012★ 152 cited

The dominant role of mergers in the size evolution of massive early-type galaxies since z ~ 1

C. López-Sanjuan, O. Le Fèvre, O. Ilbert +60

In this paper we measure the merger fraction and rate, both minor and major, of massive early-type galaxies (M_star >= 10^11 M_Sun) in the COSMOS field, and study their role in mas…

astro-ph.CO2012★ 1k cited

Improved constraints on the expansion rate of the Universe up to z~1.1 from the spectroscopic evolution of cosmic chronometers

M. Moresco, A. Cimatti, Raul Jimenez +65

We present new improved constraints on the Hubble parameter H(z) in the redshift range 0.15 < z < 1.1, obtained from the differential spectroscopic evolution of early-type galaxies…

astro-ph.CO2011★ 45 cited

Environmental effects in the interaction and merging of galaxies in zCOSMOS

P. Kampczyk, S. J. Lilly, L. de Ravel +56

(Abridged) We analyze the environments and galactic properties (morphologies and star-formation histories) of a sample of 153 close kinematic pairs in the redshift range 0.2 < z <…

astro-ph.CO2011★ 183 cited

The impact of galaxy interactions on AGN activity in zCOSMOS

J. D. Silverman, P. Kampczyk, K. Jahnke +52

Close encounters between galaxies are expected to be a viable mechanism, as predicted by numerical simulations, by which accretion onto supermassive black holes can be initiated. T…

astro-ph.CO2011★ 54 cited

Early-type galaxies at z~1.3. IV. Scaling relations in different environments

A. Raichoor, S. Mei, S. A. Stanford +15

We present the Kormendy and mass-size relations for early-type galaxies (ETGs) as a function of environment at z~1.3. Our sample includes 76 visually classified ETGs with masses 10…

astro-ph.CO2011★ 22 cited

On the occupation of X-ray selected galaxy groups by radio AGN since z=1.3

V. Smolcic, A. Finoguenov, G. Zamorani +4

Previous clustering analysis of low-power radio AGN has indicated that they preferentially live in massive groups. The X-ray surveys of the COSMOS field have achieved a sensitivity…

astro-ph.CO2011★ 67 cited

The evolution of quiescent galaxies at high redshift (z > 1.4)

H. Domínguez Sánchez, F. Pozzi, C. Gruppioni +45

We have studied the evolution of high redshift quiescent galaxies over an effective area of ~1.7 deg^2 in the COSMOS field. Galaxies have been divided according to their star-forma…