activity
20092025
most citedTrumpeting M Dwarfs with CONCH-SHELL: a Catalog of Nearby Cool Host-Stars for Habitable ExopLanets and Life

291 citations · 324 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2025

Radio and Optical Flares on the dMe Flare Star EV Lac

Rachel A. Osten, Adam F. Kowalski, Suzanne Hawley +4

We present the results of a coordinated campaign to observe radio and optical stellar flares from the nearby M dwarf flare star EV~Lac. From a total of 27 hours of radio and 29 hou…

astro-ph.SR2014★ 291 cited

Trumpeting M Dwarfs with CONCH-SHELL: a Catalog of Nearby Cool Host-Stars for Habitable ExopLanets and Life

E. Gaidos, A. W. Mann, S. Lepine +6

We present an all-sky catalog of 2970 nearby ( pc), bright () M- or late K-type dwarf stars, 86% of which have been confirmed by spectroscopy. This catalog wil…

astro-ph.SR2012★ 5 cited

M dwarf stars in the light of (future) exoplanet searches

B. Rojas-Ayala, E. J. Hilton, A. W. Mann +8

We present a brief overview of a splinter session on M dwarf stars as planet hosts that was organized as part of the Cool Stars 17 conference. The session was devoted to reviewing…

astro-ph.SR2011★ 25 cited

The Multiple Continuum Components in the White Light Flare of 16 January 2009 on the dM4.5e Star YZ CMi

Adam F. Kowalski, Suzanne L. Hawley, Jon A. Holtzman +2

The white light during M dwarf flares has long been known to exhibit the broadband shape of a T~10,000 K blackbody, and the white light in solar flares is thought to arise primaril…

astro-ph.SR2010★ 3 cited

An A star on an M star during a flare within a flare

Adam F. Kowalski, Suzanne L. Hawley, Jon A. Holtzman +2

M dwarfs produce explosive flare emission in the near-UV and optical continuum, and the mechanism responsible for this phenomenon is not well-understood. We present a near-UV/optic…

astro-ph.IM2009

Increasing the Number of Underrepresented Minorities in Astronomy at the Undergraduate, Graduate, and Postdoctoral Levels (Paper I)

Dara Norman, CSMA, NSHP +30

If the ethnic makeup of the astronomy profession is to achieve parity with the general population within one generation (~30 years), the number of underrepresented minorities earni…