Stellar noise and planet detection. I. Oscillations, granulation and sun-like spots

• Type: Article in International Conference Proceedings Book
• Date: 2011

Authors

Dumusque, X (Author) Other; N.C. Santos (Author) FCUP; Udry, S (Author) Other; Lovis, C (Author) Other; Bonfils, X (Author) Other

Conference proceedings International

Title: ASTROPHYSICS OF PLANETARY SYSTEMS: FORMATION, STRUCTURE, AND DYNAMICAL EVOLUTION

Pages: 527-529

276th Symposium of the International-Astronomical-Union on Astrophysics of Planetary Systems: Formation, Structure, and Dynamical Evolution

Torino, ITALY, OCT 10-15, 2010

Indexing

ISI Web of Knowledge - 2 Citations

Scopus - 1 Citation

Other information

Authenticus ID: P-005-70P

DOI: 10.1017/s1743921311021089

Abstract (EN): Spectrographs like HARPS can now reach a sub-ms(-1) precision in radial-velocity (RV) (Pepe & Lovis 2008). At this level of accuracy, we start to be confronted with stellar noise produced by 3 different physical phenomena: oscillations, granulation phenomena (granulation, meso- and super-granulation) and activity. On solar type stars, these 3 types of perturbation can induce ms(-1) RV variation, but on different time scales: 3 to 15 minutes for oscillations, 15 minutes to 1.5 days for granulation phenomena and 10 to 50 clays for activity. The high precision observational strategy used on HARPS, 1 measure per night of 15 minutes, on 10 consecutive clays each month, is optimized, due to a long exposure time, to average out the noise coming from oscillations (Dumusque et al. 2011a) but not to reduce the noise coining from granulation and activity (Dumusque et al. 2011a and Dumusque et al. 2011b). The smallest planets found with this strategy (Mayor et, al. 2009) seems to be at the limit of the actual observational strategy and not at the limit of the instrumental precision. To be able to find Earth mass planets in the habitable zone of solar-type stars (200 days for a K0 dwarf), new observational strategies, averaging out simultaneously all type of stellar noise, are required.

Language: English

Type (Professor's evaluation): Scientific

No. of pages: 3