activity
20102026
most citedWhite Dwarf Rotation as a Function of Mass and a Dichotomy of Mode Linewidths: Kepler Observations of 27 Pulsating DA White Dwarfs Through K2 Campaign 8

190 citations · 945 across the 35 of their papers we have counts for

collaborators
Showing 2018Show all

9 papers · 1 filter

astro-ph.IM2018

A Higher Cadence Subsurvey Located in the Galactic Plane

Michael B. Lund, Keivan G. Stassun, Jay Farihi +4

Presently, the Galactic plane receives relatively few observations compared to most of the LSST footprint. While this may address static science, the plane will also represent the…

astro-ph.IM2018

Continuous Cadence Acquisition of the LSST Deep Drilling Fields

Keaton J. Bell, J. J. Hermes

To extend LSST's coverage of the transient and variable sky down to minute timescales, we propose that observations of the Deep Drilling Fields are acquired in sequences of continu…

astro-ph.IM2018

A Cadence to Reduce Aliasing in LSST

Keaton J. Bell, Kelly M. Hambleton, Michael B. Lund +1

Regular sampling in the time domain results in aliasing in the frequency domain that complicates the accurate determination of the periods of astrophysical variables. We propose to…

astro-ph.SR2018

Transition from spot to faculae domination -- An alternate explanation for the dearth of intermediate \textit{Kepler} rotation periods

T. Reinhold, K. J. Bell, J. Kuszlewicz +2

The study of stellar activity cycles is crucial to understand the underlying dynamo and how it causes activity signatures such as dark spots and bright faculae. We study the appear…

astro-ph.SR2018

Coefficients of variation for detecting solar-like oscillations

Keaton J. Bell, Saskia Hekker, James S. Kuszlewicz

Detecting the presence and characteristic scale of a signal is a common problem in data analysis. We develop a fast statistical test of the null hypothesis that a Fourier-like powe…

astro-ph.SR2018

Constraining Low-Mass White Dwarf Binaries from Ellipsoidal Variations

K. J. Bell, J. J. Hermes, J. S. Kuszlewicz

Stars are stretched by tidal interactions in tight binaries, and changes to their projected areas introduce photometric variations twice per orbit. Hermes et al. (2014, ApJ, 792, 3…