activity
20072023
most citedemcee: The MCMC Hammer

12.4k citations · 27.9k across the 95 of their papers we have counts for

collaborators
Showing 2014Show all

8 papers · 1 filter

astro-ph.CO2014★ 167 cited

GREAT3 results I: systematic errors in shear estimation and the impact of real galaxy morphology

Rachel Mandelbaum, Barnaby Rowe, Robert Armstrong +40

We present first results from the third GRavitational lEnsing Accuracy Testing (GREAT3) challenge, the third in a sequence of challenges for testing methods of inferring weak gravi…

astro-ph.CO2014★ 29 cited

Hierarchical probabilistic inference of cosmic shear

Michael D. Schneider, David W. Hogg, Philip J. Marshall +4

Point estimators for the shearing of galaxy images induced by gravitational lensing involve a complex inverse problem in the presence of noise, pixelization, and model uncertaintie…

astro-ph.IM2014★ 205 cited

WISE photometry for 400 million SDSS sources

Dustin Lang, David W. Hogg, David J. Schlegel

We present photometry of images from the Wide-Field Infrared Survey Explorer (WISE; Wright et al. 2010) of over 400 million sources detected by the Sloan Digital Sky Survey (SDSS;…

astro-ph.GA2014★ 228 cited

The Panchromatic Hubble Andromeda Treasury X. Ultraviolet to Infrared Photometry of 117 Million Equidistant Stars

Benjamin F. Williams, Dustin Lang, Julianne J. Dalcanton +16

We have measured stellar photometry with the Hubble Space Telescope (HST) Wide Field Camera 3 (WFC3) and Advanced Camera for Surveys (ACS) in near ultraviolet (F275W, F336W), optic…

astro-ph.GA2014★ 4 cited

The Panchromatic Hubble Andromeda Treasury. Progression of Large-Scale Star Formation across Space and Time in M31

Dimitrios A. Gouliermis, Lori C. Beerman, Luciana Bianchi +11

We investigate the clustering of early-type stars younger than 300 Myr on galactic scales in M31. Based on the stellar photometric catalogs of the Panchromatic Hubble Andromeda Tre…

cs.CV2014★ 1 cited

Towards building a Crowd-Sourced Sky Map

Dustin Lang, David W. Hogg, Bernhard Scholkopf

We describe a system that builds a high dynamic-range and wide-angle image of the night sky by combining a large set of input images. The method makes use of pixel-rank information…