The magnetically quiet solar surface dominates HARPS-N solar RVs during low activity

Using images from the Helioseismic and Magnetic Imager aboard the \textit{Solar Dynamics Observatory} (SDO/HMI), we extract the radial-velocity (RV) signal arising from the suppression of convective blue-shift and from bright faculae and dark sunspots transiting the rotating solar disc. We remove th...

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Hauptverfasser: Lakeland, Ben S, Naylor, Tim, Haywood, Raphaëlle, Meunier, Nadège, Rescigno, Federica, Dalal, Shweta, Mortier, Annelies, Thompson, Samantha J, Cameron, Andrew Collier, Dumusque, Xavier, López-Morales, Mercedes, Pepe, Francesco, Rice, Ken, Sozzetti, Alessandro, Udry, Stéphane, Ford, Eric, Ghedina, Adriano, Lodi, Marcello
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Sprache:eng
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