The occurrence of potentially habitable planets orbiting M dwarfs estimated from the full Kepler dataset and an empirical measurement of the detection sensitivity
CD Dressing, D Charbonneau - The Astrophysical Journal, 2015 - iopscience.iop.org
We present an improved estimate of the occurrence rate of small planets orbiting small stars
by searching the full four-year Kepler data set for transiting planets using our own planet …
by searching the full four-year Kepler data set for transiting planets using our own planet …
How to constrain your M dwarf. II. The mass–luminosity–metallicity relation from 0.075 to 0.70 solar masses
The mass–luminosity relation for late-type stars has long been a critical tool for estimating
stellar masses. However, there is growing need for both a higher-precision relation and a …
stellar masses. However, there is growing need for both a higher-precision relation and a …
The New Generation Planetary Population Synthesis (NGPPS)-IV. Planetary systems around low-mass stars
Context. Previous theoretical works on planet formation around low-mass stars have often
been limited to large planets and individual systems. As current surveys routinely detect …
been limited to large planets and individual systems. As current surveys routinely detect …
Imaging extrasolar giant planets
BP Bowler - Publications of the Astronomical Society of the …, 2016 - iopscience.iop.org
High-contrast adaptive optics (AO) imaging is a powerful technique to probe the
architectures of planetary systems from the outside-in and survey the atmospheres of self …
architectures of planetary systems from the outside-in and survey the atmospheres of self …
The field substellar mass function based on the full-sky 20 pc census of 525 L, T, and Y dwarfs
JD Kirkpatrick, CR Gelino, JK Faherty… - The Astrophysical …, 2021 - iopscience.iop.org
We present final Spitzer trigonometric parallaxes for 361 L, T, and Y dwarfs. We combine
these with prior studies to build a list of 525 known L, T, and Y dwarfs within 20 pc of the …
these with prior studies to build a list of 525 known L, T, and Y dwarfs within 20 pc of the …
CARMENES input catalogue of M dwarfs-V. Luminosities, colours, and spectral energy distributions
C Cifuentes, JA Caballero, M Cortés-Contreras… - Astronomy & …, 2020 - aanda.org
Context. The relevance of M dwarfs in the search for potentially habitable Earth-sized
planets has grown significantly in the last years. Aims. In our on-going effort to …
planets has grown significantly in the last years. Aims. In our on-going effort to …
The stellar rotation–activity relationship in fully convective M dwarfs
NJ Wright, ER Newton, PKG Williams… - Monthly Notices of …, 2018 - academic.oup.com
The coronal activity–rotation relationship is considered to be a proxy for the underlying
stellar dynamo responsible for magnetic activity in solar and late-type stars. While this has …
stellar dynamo responsible for magnetic activity in solar and late-type stars. While this has …
The solar neighborhood. XLV. The stellar multiplicity rate of M dwarfs within 25 pc
JG Winters, TJ Henry, WC Jao… - The Astronomical …, 2019 - iopscience.iop.org
We present results of the largest, most comprehensive study ever done of the stellar
multiplicity of the most common stars in the Galaxy, the red dwarfs. We have conducted an …
multiplicity of the most common stars in the Galaxy, the red dwarfs. We have conducted an …
The solar neighborhood. xxxvii. the mass–luminosity relation for main-sequence m dwarfs
GF Benedict, TJ Henry, OG Franz… - The Astronomical …, 2016 - iopscience.iop.org
We present a mass–luminosity relation (MLR) for red dwarfs spanning a range of masses
from 0.62${{\mathcal M}} _ {\odot} $ to the end of the stellar main sequence at …
from 0.62${{\mathcal M}} _ {\odot} $ to the end of the stellar main sequence at …
TESS Discovery of an Ultra-short-period Planet around the Nearby M Dwarf LHS 3844
R Vanderspek, CX Huang, A Vanderburg… - The Astrophysical …, 2019 - iopscience.iop.org
TESS Discovery of an Ultra-short-period Planet around the Nearby M Dwarf LHS 3844 -
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