output
20102021
most citedThe Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III

2.5k citations

Showing 2010Show all

9 papers · 1 filter

astro-ph.CO2010★ 81 cited

On the spectral resolution of the MILES stellar library

A. Beifiori, C. Maraston, D. Thomas +1

Empirical stellar libraries are extensively used to extract stellar kinematics in galaxies and to build stellar population models. An accurate knowledge of the spectral resolution…

astro-ph.CO2010★ 34 cited

Chemical abundance ratios of galactic globular clusters from modelling integrated light spectroscopy

Daniel Thomas, Jonas Johansson, Claudia Maraston

We use our new, flux-calibrated stellar population model of absorption-line indices to derive ages, metallicities, and various element abundance ratios from integrated light spectr…

astro-ph.CO2010★ 617 cited

The star formation history of mass-selected galaxies in the COSMOS field

Alexander Karim, Eva Schinnerer, Alejo Martinez-Sansigre +10

We explore the evolution of the specific star formation rate (SSFR) for 3.6um-selected galaxies of different M_* in the COSMOS field. The average SFR for sub-sets of these galaxies…

cond-mat.soft2010★ 100 cited

Transient shear banding in entangled polymers: a study using the Rolie-Poly model

J. M. Adams, S. M. Fielding, P. D. Olmsted

Spatially inhomogeneous shear flow occurs in entangled polymer solutions, both as steady state shear banding and transiently after a large step strain or during start up to a stead…

cond-mat.dis-nn2010★ 6 cited

Understanding spin glass transition as a dynamic phenomenon

Kostya Trachenko

Existing theories explain spin glass transition in terms of a phase transition and order parameters, and assume the existence of a distinct spin glass phase. In addition to problem…

astro-ph.CO2010★ 200 cited

Flux-calibrated stellar population models of Lick absorption-line indices with variable element abundance ratios

Daniel Thomas, Claudia Maraston, Jonas Johansson

We present new stellar population models of Lick absorption-line indices with variable element abundance ratios. The models are based on our new calibrations of absorption-line ind…