activity
19982024
most citedThe Transiting Exoplanet Survey Satellite

4.1k citations · 46.1k across the 313 of their papers we have counts for

collaborators
Showing 2015Show all

13 papers · 1 filter

astro-ph.EP2015★ 42 cited

The Kepler-454 System: A Small, Not-rocky Inner Planet, a Jovian World, and a Distant Companion

Sara Gettel, David Charbonneau, Courtney D. Dressing +47

Kepler-454 (KOI-273) is a relatively bright (V = 11.69 mag), Sun-like starthat hosts a transiting planet candidate in a 10.6 d orbit. From spectroscopy, we estimate the stellar tem…

astro-ph.EP2015★ 238 cited

A rocky planet transiting a nearby low-mass star

Zachory K. Berta-Thompson, Jonathan Irwin, David Charbonneau +18

M-dwarf stars -- hydrogen-burning stars that are smaller than 60 per cent of the size of the Sun -- are the most common class of star in our Galaxy and outnumber Sun-like stars by…

astro-ph.EP2015★ 120 cited

HARPS-N observes the Sun as a star

Xavier Dumusque, Alex Glenday, David F. Phillips +16

Radial velocity perturbations induced by stellar surface inhomogeneities including spots, plages and granules currently limit the detection of Earth-twins using Doppler spectroscop…

astro-ph.SR2015★ 278 cited

The rotation and Galactic kinematics of mid M dwarfs in the Solar Neighborhood

Elisabeth R. Newton, Jonathan Irwin, David Charbonneau +3

Rotation is a directly-observable stellar property, and drives magnetic field generation and activity through a magnetic dynamo. Main sequence stars with masses below approximately…

astro-ph.SR2015★ 42 cited

Calibration of the MEarth Photometric System: Optical Magnitudes and Photometric Metallicity Estimates for 1802 Nearby M-dwarfs

Jason A Dittmann, Jonathan M Irwin, David Charbonneau +1

The MEarth Project is a photometric survey systematically searching the smallest stars nearest to the Sun for transiting rocky planets. Since 2008, MEarth has taken approximately t…

astro-ph.EP2015★ 460 cited

A disintegrating minor planet transiting a white dwarf

Andrew Vanderburg, John Asher Johnson, Saul Rappaport +16

White dwarfs are the end state of most stars, including the Sun, after they exhaust their nuclear fuel. Between 1/4 and 1/2 of white dwarfs have elements heavier than helium in the…