activity
19982009
most citedStar formation in AEGIS field galaxies since z=1.1 . Staged galaxy formation, and a model of mass-dependent gas exhaustion

434 citations · 607 across the 15 of their papers we have counts for

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57 papers · 1 filter

astro-ph200857 cited

The relationship between gas content and star formation rate in spiral galaxies. Comparing the local field with the Virgo cluster

M. Fumagalli, G. Gavazzi

Despite many studies of the star formation in spiral galaxies, a complete and coherent understanding of the physical processes that regulate the birth of stars has not yet been ach…

astro-ph20081 cited

SMC in space and time: a project to study the evolution of the prototype interacting late-type dwarf galaxy

M. Tosi, J. Gallagher, E. Sabbi +13

We introduce the SMC in space and time, a large coordinated space and ground-based program to study star formation processes and history, as well as variable stars, structure, kine…

astro-ph20083 cited

CATS: Optical to Near-Infrared Colors of the Bulge and Disk of Two z=0.7 Galaxies Using HST and Keck Laser Adaptive Optics Imaging

E. Steinbring, J. Melbourne, A. J. Metevier +5

We have employed laser guide star (LGS) adaptive optics (AO) on the Keck II telescope to obtain near-infrared (NIR) images in the Extended Groth Strip (EGS) deep galaxy survey fiel…

astro-ph2008601 cited

Galaxy Zoo: the dependence of morphology and colour on environment

Steven P. Bamford, Robert C. Nichol, Ivan K. Baldry +13

We analyse the relationships between galaxy morphology, colour, environment and stellar mass using data for over 100,000 objects from Galaxy Zoo, the largest sample of visually cla…

astro-ph2008428 cited

Galaxy Merger Morphologies and Time-Scales from Simulations of Equal-Mass Gas-Rich Disc Mergers

Jennifer M. Lotz, Patrik Jonsson, T. J. Cox +1

A key obstacle to understanding the galaxy merger rate and its role in galaxy evolution is the difficulty in constraining the merger properties and time-scales from instantaneous s…

astro-ph200818 cited

Gravitational Lensing Constraints on Dynamical and Coupled Dark Energy

G. La Vacca, L. P. L. Colombo

Upcoming Weak Lensing (WL) surveys can be used to constrain Dark Energy (DE) properties, namely if tomographic techniques are used to improve their sensitivity. In this work, we us…