A HARPS-N mass for the elusive Kepler-37d: a case study in disentangling stellar activity and planetary signals (2021)

First Author: Rajpaul V
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