The EXPRES Stellar Signals Project II. State of the Field in Disentangling Photospheric Velocities
<jats:title>Abstract</jats:title> <jats:p>Measured spectral shifts due to intrinsic stellar variability (e.g., pulsations, granulation) and activity (e.g., spots, plages) are the largest source of error for extreme-precision radial-velocity (EPRV) exoplanet detectio...
Main Author: | Vanderburg, Andrew |
---|---|
Other Authors: | Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences |
Format: | Article |
Language: | English |
Published: |
American Astronomical Society
2022
|
Online Access: | https://hdl.handle.net/1721.1/142258 |
Similar Items
-
Photospheric activity, rotation, and radial velocity variations of the
planet-hosting star CoRoT-7
by: Lanza, A, et al.
Published: (2010) -
Prominence oscillations and the influence of the distant photosphere
by: Schutgens, N, et al.
Published: (1998) -
Disentangling the stellar populations in the counter-rotating disc galaxy NGC 4550
by: Johnston, E, et al.
Published: (2013) -
Computation and analysis of flow patterns in the solar photosphere.
by: Hendl, Richard Godfrey
Published: (2010) -
Prominence oscillations and stability - Communicating the distant photospheric boundary
by: Schutgens, N
Published: (1997)