2k citations · 9.3k across the 65 of their papers we have counts for
15 papers · 1 filter
The relation between stellar populations, structure and environment for dwarf elliptical galaxies from the MAGPOP-ITP
D. Michielsen, A. Boselli, C. J. Conselice +9
Dwarf galaxies, as the most numerous type of galaxy, offer the potential to study galaxy formation and evolution in detail in the nearby Universe. Although they seem to be simple s…
Hierarchical Disk Galaxy Assembly as the Origin of Scatter in the z~1 Stellar Mass Tully-Fisher Relation
Nicola Atkinson, Christopher J. Conselice, Nicole Fox
Recent observations of distant disk galaxies show that there is little to no evolution in the relation between maximum rotation speed and stellar mass at z < 1.2. There is however…
The Structures of Distant Galaxies I: Galaxy Structures and the Merger Rate to z~3 in the Hubble Ultra-Deep Field
Christopher J. Conselice, Sheena Rajgor, Robert Myers
This paper begins a series in which we examine the structures of distant galaxies to directly determine the history of their formation modes. We start this series by examining the…
The Faint and Extremely Red K-band Selected Galaxy Population in the DEEP2/Palomar Fields
C. J. Conselice, K. Bundy, Vivian U +3
We present in this paper an analysis of the faint and red near-infrared selected galaxy population found in near-infrared imaging from the Palomar Observatory Wide-Field Infrared S…
AEGIS: New Evidence Linking Active Galactic Nuclei to the Quenching of Star Formation
Kevin Bundy, Antonis Georgakakis, Kirpal Nandra +10
Utilizing Chandra X-ray observations in the All-wavelength Extended Groth Strip International Survey (AEGIS) we identify 241 X-ray selected Active Galactic Nuclei (AGNs, L > 10^{42…
Keck spectroscopy of the faint dwarf elliptical galaxy population in the Perseus Cluster core: mixed stellar populations and a flat luminosity function
Samantha J. Penny, Christopher J. Conselice
We present the result of a photometric and Keck-LRIS spectroscopic study of dwarf galaxies in the core of the Perseus Cluster, down to a magnitude of M_B = -12.5. Spectra were obta…