output
19922026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

Showing 2014 · astro-ph.GAShow all

112 papers · 2 filters

astro-ph.GA2014★ 54 cited

Building gas rings and rejuvenating S0 galaxies through minor mergers

Michela Mapelli, Roberto Rampazzo, Antonietta Marino

We investigate the effects of minor mergers between an S0 galaxy and a gas-rich satellite galaxy, by means of N-body/smoothed particle hydrodynamics (SPH) simulations. The satellit…

astro-ph.GA2014★ 91 cited

The Rich Are Different: Evidence from the RAVE Survey for Stellar Radial Migration

G. Kordopatis, J. Binney, G. Gilmore +21

Using the RAdial Velocity Experiment fourth data release (RAVE DR4), and a new metallicity calibration that will be also taken into account in the future RAVE DR5, we investigate t…

astro-ph.GA2014★ 46 cited

Variability-selected Active Galactic Nuclei in the VST-SUDARE/VOICE Survey of the COSMOS Field

D. De Cicco, M. Paolillo, G. Covone +16

Optical variability has proven to be an effective way of detecting AGNs in imaging surveys, lasting from weeks to years. In the present work we test its use as a tool to identify A…

astro-ph.GA2014★ 16 cited

Combining Physical galaxy models with radio observations to constrain the SFRs of high-z dusty star forming galaxies

B. Lo Faro, L. Silva, A. Franceschini +2

We complement our previous analysis of a sample of z~1-2 luminous and ultra-luminous infrared galaxies ((U)LIRGs), by adding deep VLA radio observations at 1.4 GHz to a large data-…

astro-ph.GA2014★ 56 cited

Characterizing the High-Velocity Stars of RAVE: The Discovery of a Metal-Rich Halo Star Born in the Galactic Disk

K. Hawkins, G. Kordopatis, G. Gilmore +21

We aim to characterize high-velocity (HiVel) stars in the solar vicinity both chemically and kinematically using the fourth data release of the RAdial Velocity Experiment (RAVE). W…

astro-ph.GA2014★ 297 cited

The galaxy stellar mass function at 3.5<z<7.5 in the CANDELS/UDS, GOODS-South, and HUDF fields

A. Grazian, A. Fontana, P. Santini +38

The galaxy stellar mass function (GSMF) at high-z provides key information on star-formation history and mass assembly in the young Universe. We aimed to use the unique combination…