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20012026
most citedThe Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package

5k citations · 36.6k across the 347 of their papers we have counts for

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Showing 2011Show all

6 papers · 1 filter

astro-ph.HE2011★ 49 cited

Panchromatic observations of the textbook GRB 110205A: constraining physical mechanisms of prompt emission and afterglow

W. Zheng, R. F. Shen, T. Sakamoto +56

We present a comprehensive analysis of a bright, long duration (T90 ~ 257 s) GRB 110205A at redshift z= 2.22. The optical prompt emission was detected by Swift/UVOT, ROTSE-IIIb and…

astro-ph.CO2011★ 31 cited

Finding Fossil Groups: Optical Identification and X-ray Confirmation

Eric D. Miller, Eli Rykoff, Renato Dupke +6

We report the discovery of 12 new fossil groups of galaxies, systems dominated by a single giant elliptical galaxy and cluster-scale gravitational potential, but lacking the popula…

astro-ph.CO2011★ 48 cited

On the mass-to-light ratios of fossil groups. Are they simply dark clusters?

Robert N. Proctor, Claudia Mendes de Oliveira, Renato Dupke +4

Defined as X-ray bright galaxy groups with large differences between the luminosities of their brightest and second brightest galaxies, "fossil groups" are believed to be some of t…

astro-ph.CO2011★ 123 cited

Scaling Relations and Overabundance of Massive Clusters at z>~1 from Weak-Lensing Studies with HST

M. J. Jee, K. S. Dawson, H. Hoekstra +22

We present weak gravitational lensing analysis of 22 high-redshift (z >~1) clusters based on Hubble Space Telescope images. Most clusters in our sample provide significant lensing…

astro-ph.CO2011★ 40 cited

Extrinsic Sources of Scatter in the Richness-Mass Relation of Galaxy Clusters

Eduardo Rozo, Eli Rykoff, Benjamin Koester +4

Maximizing the utility of upcoming photometric cluster surveys requires a thorough understanding of the richness-mass relation of galaxy clusters. We use Monte Carlo simulations to…

astro-ph.CO2011★ 183 cited

Robust Optical Richness Estimation with Reduced Scatter

E. S. Rykoff, B. P. Koester, E. Rozo +7

Reducing the scatter between cluster mass and optical richness is a key goal for cluster cosmology from photometric catalogs. We consider various modifications to the red-sequence…