Disentangling between stellar activity and planetary signals

By I. Boisse, F. Bouchy, G. Hébrard, X. Bonfils, Nuno C. Santos, S. Vauclair. 2010

220 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. D. Charbonneau
2. J. Southworth
3. S. Udry
4. M. Mayor
5. J. Johnson
6. C. Lovis
7. F. Pepe
8. D. Queloz

In Instrumentation

1. D. Charbonneau
2. J. Southworth
3. S. Udry
4. C. Lovis
5. Mercedes López-Morales
6. M. Mayor
7. F. Pepe
8. D. Queloz

Citations in the corpus

• THE KEPLER-10 PLANETARY SYSTEM REVISITED BY HARPS-N: A HOT ROCKY WORLD AND A SOLID NEPTUNE-MASS PLANET (2014, methodology): “In addition to this model, we also consider that Gaussian noise of stellar origin could affect the RVs.”
• The CARMENES Search for Exoplanets around M Dwarfs: A Low-mass Planet in the Temperate Zone of the Nearby K2-18 (2018, background): “The observed RV signal is often detected at the stellar rotation period (Prot) and its harmonics (Prot/2, Prot/3, ...) (Boisse et al. 2011).”