activity
20032013
most citedNearly 5000 Distant Early-Type Galaxies in COMBO-17: a Red Sequence and its Evolution since z~1

1.2k citations · 5.6k across the 31 of their papers we have counts for

collaborators

31 papers

astro-ph.CO2013★ 121 cited

MegaMorph -- multi-wavelength measurement of galaxy structure: Sérsic profile fits to galaxies near and far

Marina Vika, Steven P. Bamford, Boris Haeussler +3

We demonstrate a new multi-wavelength technique for two-dimensional parametric modelling of galaxy surface-brightness profiles, which we have incorporated into the widely used soft…

astro-ph.CO2009★ 239 cited

History of Galaxy Interactions and their Impact on Star Formation over the Last 7 Gyr from GEMS

Shardha Jogee, Sarah H. Miller, Kyle Penner +22

We perform a comprehensive estimate of the frequency of galaxy mergers and their impact on star formation over z~0.24--0.80 (lookback time T_b~3--7 Gyr) using 3698 (M*>=1e9 Msun) g…

astro-ph2008

Exploring the Impact of Galaxy Interactions over Seven Billion Years with CAS

Sarah H. Miller, S. Jogee, C. Conselice +22

We explore galaxy assembly over the last seven billion years by characterizing "normal" galaxies along the Hubble sequence, against strongly disturbed merging/interacting galaxies…

astro-ph2008★ 8 cited

Frequency and Impact of Galaxy Mergers and Interactions over the last 7 Gyr

S. Jogee, S. Miller, K. Penner +21

We explore the history and impact of galaxy mergers and interactions over z~0.24 to 0.80, based on HST ACS, Combo-17, and Spitzer 24 mu data of ~4500 galaxies in the GEMS survey. U…

astro-ph2007★ 292 cited

GEMS: Galaxy fitting catalogues and testing parametric galaxy fitting codes

Boris Häußler, Daniel H. McIntosh, Marco Barden +14

In the context of measuring structure and morphology of intermediate redshift galaxies with recent HST/ACS surveys, we tune, test, and compare two widely used fitting codes (GALFIT…

astro-ph2007

NBODY meets stellar population - The HYDE-PARC Project

Andrea Borch, Rainer Spurzem, Jarrod Hurley

N-body simulations give us a rough idea of how the shape of a simulated object appears in three-dimensional space. From an observational point of view this may give us a misleading…