Journal
ASTROPHYSICAL JOURNAL
Volume 888, Issue 2, Pages -Publisher
IOP Publishing Ltd
DOI: 10.3847/1538-4357/ab59d5
Keywords
Radial velocity; Solar activity; Solar faculae; Plages; Solar granulation; Sunspots; Exoplanet detection methods
Categories
Funding
- NASA [NNX16AD42G]
- Smithsonian Institution
- Smithsonian Astrophysical Observatory
- Harvard Origins of Life Initiative
- TNG
- NASA
- STFC [ST/M001296/1]
- Kepler mission under NASA Cooperative Agreement [NNX13AB58A]
- NASA Heliophysics LWS grant [NNX16AB79G]
- National Centre for Competence in Research PlanetS - Swiss National Science Foundation (SNSF)
- John Templeton Foundation
- National Aeronautics and Space Administration [NNX15AC90G, NNX17AB59G]
- European Union [313014]
- NSF-REU solar physics program at SAO [AGS-1560313]
- Prodex Program of the Swiss Space Office (SSO)
- Harvard University Origins of Life Initiative (HUOLI)
- Scottish Universities Physics Alliance (SUPA)
- University of Geneva
- Smithsonian Astrophysical Observatory (SAO)
- Italian National Astrophysical Institute (INAF)
- University of St Andrews, Queen's University Belfast
- University of Edinburgh
- NASA [476394, NNX13AB58A, 907429, NNX16AB79G] Funding Source: Federal RePORTER
Ask authors/readers for more resources
Efforts to detect low-mass exoplanets using stellar radial velocities (RVs) are currently limited by magnetic photospheric activity. Suppression of convective blueshift is the dominant magnetic contribution to RV variability in low-activity Sun-like stars. Due to convective plasma motion, the magnitude of RV contributions from the suppression of convective blueshift is related to the depth of formation of photospheric spectral lines for a given species used to compute the RV time series. Meunier et al. used this relation to demonstrate a method for spectroscopic extraction of the suppression of convective blueshift in order to isolate RV contributions, including planetary RVs, that contribute equally to the time series for each spectral line. Here, we extract disk-integrated solar RVs from observations over a 2.5 yr time span made with the solar telescope integrated with the HARPS-N spectrograph at the Telescopio Nazionale Galileo (La Palma, Canary Islands, Spain). We apply the methods outlined by Meunier et al. We are not, however, able to isolate physically meaningful contributions due to the suppression of convective blueshift from this solar data set, potentially because our data set is taken during solar minimum when the suppression of convective blueshift may not sufficiently dominate activity contributions to RVs. This result indicates that, for low-activity Sun-like stars, one must include additional RV contributions from activity sources not considered in the Meunier et al. model at different timescales, as well as instrumental variation, in order to reach the submeter per second RV sensitivity necessary to detect low-mass planets in orbit around Sun-like stars.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available