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

V M Rajpaul*, L A Buchhave, G Lacedelli, K Rice, A Mortier, L Malavolta, S Aigrain, L Borsato, A W Mayo, D Charbonneau, M Damasso, X Dumusque, A Ghedina, D W Latham, M López-Morales, A Magazzù, G Micela, E Molinari, F Pepe, G PiottoE Poretti, S Rowther, A Sozzetti, S Udry, C A Watson

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

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Original languageEnglish
Pages (from-to)1847-1868
Number of pages22
JournalMonthly Notices of the Royal Astronomical Society
Volume507
Issue number2
Early online date30 Jul 2021
DOIs
Publication statusPublished - Oct 2021

Keywords

  • methods: data analysis
  • techniques: radial velocities
  • techniques: spectroscopic
  • planetary systems
  • stars: activity
  • stars: individual: Kepler-37

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