activity
20002016
most citedLSST Science Book, Version 2.0

924 citations · 4.4k across the 29 of their papers we have counts for

collaborators

29 papers

astro-ph.SR2016★ 45 cited

Kepler Flares IV: A Comprehensive Analysis of the Activity of the dM4e Star GJ 1243

Steven M. Silverberg, Adam F. Kowalski, James R. A. Davenport +3

We present a comprehensive study of the active dM4e star GJ 1243. We use previous observations and ground-based echelle spectroscopy to determine that GJ 1243 is a member of the Ar…

astro-ph.SR2016★ 76 cited

M Dwarf Flare Continuum Variations on One-Second Timescales: Calibrating and Modeling of ULTRACAM Flare Color Indices

Adam F. Kowalski, Mihalis Mathioudakis, Suzanne L. Hawley +5

We present a large dataset of high cadence dMe flare light curves obtained with custom continuum filters on the triple-beam, high-speed camera system ULTRACAM. The measurements pro…

astro-ph.SR2014★ 286 cited

Kepler Flares II: The Temporal Morphology of White-Light Flares on GJ 1243

James R. A. Davenport, Suzanne L. Hawley, Leslie Hebb +12

We present the largest sample of flares ever compiled for a single M dwarf, the active M4 star GJ 1243. Over 6100 individual flare events, with energies ranging from to $…

astro-ph.SR2014★ 384 cited

Kepler Flares I. Active and Inactive M dwarfs

Suzanne L. Hawley, James R. A. Davenport, Adam F. Kowalski +4

We analyzed Kepler short-cadence M dwarf observations. Spectra from the ARC 3.5m telescope identify magnetically active (H in emission) stars. The active stars are of mid-M spec…

astro-ph.SR2013★ 263 cited

Time-Resolved Properties and Global Trends in dMe Flares from Simultaneous Photometry and Spectra

Adam F. Kowalski, Suzanne L. Hawley, John P. Wisniewski +5

We present a homogeneous survey of line and continuum emission from near-ultraviolet (NUV) to optical wavelengths during twenty M dwarf flares with simultaneous, high cadence photo…

astro-ph.EP2013★ 58 cited

Testing the Metal of Late-Type Kepler Planet Hosts with Iron-Clad Methods

Andrew W. Mann, Eric Gaidos, Adam Kraus +1

It has been shown that F, G, and early K dwarf hosts of Neptune-sized planets are not preferentially metal-rich. However, it is less clear whether the same holds for late K and M d…