activity
20142024
most citedThe Factory and The Beehive II. Activity and Rotation in Praesepe and the Hyades

151 citations · 236 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.EP20241 cited

The occurrence of small, short-period planets younger than 200 Myr with TESS

Sydney Vach, George Zhou, Chelsea X. Huang +10

Within the first few hundreds of millions of years, many physical processes sculpt the eventual properties of young planets. NASA's TESS mission has surveyed young stellar associat…

astro-ph.SR20233 cited

A Novel Application of Conditional Normalizing Flows: Stellar Age Inference with Gyrochronology

Phil Van-Lane, Joshua S. Speagle, Stephanie Douglas

Stellar ages are critical building blocks of evolutionary models, but challenging to measure for low mass main sequence stars. An unexplored solution in this regime is the applicat…

astro-ph.EP202313 cited

Hyades Member K2-136c: The Smallest Planet in an Open Cluster with a Precisely Measured Mass

Andrew W. Mayo, Courtney D. Dressing, Andrew Vanderburg +39

K2-136 is a late-K dwarf ( M) in the Hyades open cluster with three known, transiting planets and an age of Myr. Analyzing K2 photometry, we found…

astro-ph.SR20237 cited

Contemporaneous Observations of Luminosities and Photometric Amplitudes for M Dwarfs

Aylin García Soto, Elisabeth R. Newton, Stephanie T. Douglas +2

While many M dwarfs are known to have strong magnetic fields and high levels of magnetic activity, we are still unsure about the properties of their starspots and the origin of the…

astro-ph.IM20165 cited

The Astropy Problem

Demitri Muna, Michael Alexander, Alice Allen +151

The Astropy Project (http://astropy.org) is, in its own words, "a community effort to develop a single core package for Astronomy in Python and foster interoperability between Pyth…

astro-ph.SR201656 cited

Exploring the Role of Sub-micron Sized Dust Grains in the Atmospheres of Red L0 - L6 Dwarfs

Kay Hiranaka, Kelle L. Cruz, Stephanie T. Douglas +2

We examine the hypothesis that the red near-infrared colors of some L dwarfs could be explained by a "dust haze" of small particles in their upper atmospheres. This dust haze would…