activity
20062020
most citedA Reverberation-Based Mass for the Central Black Hole in NGC 4151

211 citations · 1.2k across the 30 of their papers we have counts for

collaborators
Showing 2013Show all

8 papers · 1 filter

astro-ph.SR2013★ 1 cited

RR Lyrae in the LMC: Insights Into the Oosterhoff Phenomenon

Charles A Kuehn, Horace A. Smith, Marcio Catelan +8

Although more than eight decades have passed since P. Th. Oosterhoff drew attention to differences in the properties of RR Lyrae variables in globular clusters, the origin and sign…

astro-ph.SR2013★ 3 cited

40 Years of Variable Stars: A Celebration of Contributions by Horace A. Smith

Karen Kinemuchi, Charles A. Kuehn, Nathan De Lee +1

This online book contains the proceedings of a meeting held at Michigan State University to celebrate the career and contributions of Horace A Smith. The meeting focused on the are…

astro-ph.SR2013

Photometry Using Kepler "Superstamps" of Open Clusters NGC 6791 & NGC 6819

Charles A. Kuehn, Jason Drury, Dennis Stello +1

The Kepler space telescope has proven to be a gold mine for the study of variable stars. Unfortunately, Kepler only returns a handful of pixels surrounding each star on the target…

astro-ph.SR2013★ 1 cited

The Kepler-SEP Mission: Harvesting the South Ecliptic Pole large-amplitude variables with Kepler

R. Szabó, L. Molnár, Z. Kołaczkowski +28

As a response to the white paper call, we propose to turn Kepler to the South Ecliptic Pole (SEP) and observe thousands of large amplitude variables for years with high cadence in…

astro-ph.SR2013★ 19 cited

Variable Stars in Large Magellanic Cloud Globular Clusters III: Reticulum

Charles A. Kuehn, Kyra Dame, Horace A. Smith +8

This is the third in a series of papers studying the variable stars in old globular clusters in the Large Magellanic Cloud. The primary goal of this series is to look at how the ch…

astro-ph.SR2013★ 56 cited

Properties of oscillation modes in subgiant stars observed by Kepler

O. Benomar, T. R. Bedding, B. Mosser +7

Mixed modes seen in evolved stars carry information on their deeper layers that can place stringent constraints on their physics and on their global properties (mass, age, etc...).…