HIGHLIGHTS
- who: Bourrier V. and collaborators from the (UNIVERSITY) have published the article: A CHEOPS-enhanced view of the HD 3167 systemu2605,, in the Journal: (JOURNAL) of 14/Nov/2020
- what: Following the work described in Dumusque et_al , the ESPRESSO pipeline has been optimized to work with HARPS-N data. The authors determine the radius of HD 3167 using the infrared flux method (IRFM; Blackwell and amp; Shallis 1977) in a Markov-chain Each fit was performed using the model described before (GP and transit models for planets b and c) and allocating an individual jitter . . .
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