activity
20182022
most citedRecovery of TESS Stellar Rotation Periods Using Deep Learning

48 citations · 127 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2022★ 37 cited

Rotation Distributions around the Kraft Break with TESS and Kepler: The Influences of Age, Metallicity, and Binarity

Ellis A. Avallone, Jamie N. Tayar, Jennifer L. van Saders +6

Stellar rotation is a complex function of mass, metallicity, and age and can be altered by binarity. To understand the importance of these parameters in main sequence stars, we hav…

astro-ph.SR2021

Flares Big and Small: a K2 and TESS View of ASAS-SN Superflares

Jesse Zeldes, Jason T. Hinkle, Benjamin J. Shappee +6

We investigate the flare-frequency distributions of 5 M-dwarfs that experienced superflares with energies in excess of erg detected by ASAS-SN. We use K2 and TESS short-c…

astro-ph.SR2021★ 48 cited

Recovery of TESS Stellar Rotation Periods Using Deep Learning

Zachary R. Claytor, Jennifer L. van Saders, Joe Llama +3

We used a convolutional neural network to infer stellar rotation periods from a set of synthetic light curves simulated with realistic spot evolution patterns. We convolved these s…

astro-ph.SR2020★ 30 cited

Electric Current Neutralization in Solar Active Regions and Its Relation to Eruptive Activity

Ellis A. Avallone, Xudong Sun

It is well established that magnetic free energy associated with electric currents powers solar flares and coronal mass ejections (CMEs) from solar active regions (ARs). However, t…

astro-ph.SR2018★ 12 cited

Critical magnetic field strengths for solar coronal plumes in quiet regions and coronal holes?

Ellis A. Avallone, Sanjiv K. Tiwari, Navdeep K. Panesar +2

Coronal plumes are bright magnetic funnels found in quiet regions (QRs) and coronal holes (CHs). They extend high into the solar corona and last from hours to days. The heating pro…