A HARPS-N mass for the elusive Kepler-37d: a case study in disentangling stellar activity and planetary signals (2021)
Attributed to:
Astrophysics at Oxford 2019-2022
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2107.13900
Publication URI: https://arxiv.org/abs/2107.13900
Type: Other