Follow-Up and Validation of K2 and TESS Planetary Systems With Keck NIRC2 Adaptive Optics Imaging
High resolution imaging (HRI) is a critical part of the transiting exoplanet follow-up and validation process. HRI allows previously unresolved stellar companions and background blends to be resolved, vetting false positive signals and improving the radii measurements of true planets. Through a mult...
Main Authors: | Joshua E. Schlieder, Erica J. Gonzales, David R. Ciardi, Rahul I. Patel, Ian J. M. Crossfield, Justin R. Crepp, Courtney D. Dressing, Thomas Barclay, Andrew W. Howard |
---|---|
Format: | Article |
Language: | English |
Published: |
Frontiers Media S.A.
2021-06-01
|
Series: | Frontiers in Astronomy and Space Sciences |
Subjects: | |
Online Access: | https://www.frontiersin.org/articles/10.3389/fspas.2021.628396/full |
Similar Items
-
A Search for Exoplanets in Short-Period Binary Star Systems
by: Ronald Kaitchuck, et al.
Published: (2012-03-01) -
The NASA High-Resolution Speckle Interferometric Imaging Program: Validation and Characterization of Exoplanets and Their Stellar Hosts
by: Steve B. Howell, et al.
Published: (2021-03-01) -
Habitable Zones in Binary Star Systems: A Zoology
by: Siegfried Eggl, et al.
Published: (2020-09-01) -
Revisiting the Planet Mass and Stellar Metallicity Relation for Low-Mass Exoplanets Orbiting GKM Class Stars
by: Jonathan Jiang, et al.
Published: (2021-04-01) -
The ExoMol Atlas of Molecular Opacities
by: Jonathan Tennyson, et al.
Published: (2018-05-01)