177 citations · 416 across the 8 of their papers we have counts for
8 papers
The Art of Measuring Physical Parameters in Galaxies: A Critical Assessment of Spectral Energy Distribution Fitting Techniques
Camilla Pacifici, Kartheik G. Iyer, Bahram Mobasher +52
The study of galaxy evolution hinges on our ability to interpret multi-wavelength galaxy observations in terms of their physical properties. To do this, we rely on spectral energy…
Morphology & Environment's Role on the Star Formation Rate -- Stellar Mass Relation in COSMOS from 0 < z < 3.5
Kevin C. Cooke, Jeyhan S. Kartaltepe, Caitlin Rose +6
We investigate the relationship between environment, morphology, and the star formation rate -- stellar mass relation derived from a sample of star-forming galaxies (commonly refer…
Stellar Mass Growth of Brightest Cluster Galaxy Progenitors in COSMOS Since z ~ 3
Kevin C. Cooke, Jeyhan S. Kartaltepe, K. D. Tyler +5
We examine the role of environment on the in situ star formation (SF) hosted by the progenitors of the most massive galaxies in the present-day universe, the brightest cluster gala…
The Nature of Star Formation at 24 microns in the Group Environment at 0.3 < z < 0.55
K. Tyler, G. H. Rieke, D. J. Wilman +7
Galaxy star formation rates (SFRs) are sensitive to the local environment; for example, the high-density regions at the cores of dense clusters are known to suppress star formation…
Unveiling the Important Role of Groups in the Evolution of Massive Galaxies: Insights from an Infrared Passive Sequence at Intermediate Redshift
D. J. Wilman, D. Pierini, K. Tyler +6
The most massive galaxies in the Universe are also the oldest. To overturn this apparent contradiction with hierarchical growth models, we focus on the group scale haloes which hos…
Lyman Break Galaxies at z~1 and the evolution of the dust attenuation in star-forming galaxies with the redshift
D. Burgarella, E. Le Floc'h, T. T. Takeuchi +4
Ultraviolet (UV) galaxies have been selected from GALEX. The presence of a FUV-dropout in their spectral energy distributions proved to be a very complete (83.3%) but not very effi…