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Browsing by Author "Gonzalez, M."

Browsing by Author "Gonzalez, M."

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  • HARPS-N Solar RVs Are Dominated by Large, Bright Magnetic Regions 
    Milbourne, Timothy W.; Haywood, Raphaëlle D.; Phillips, David F.; Saar, Steve H.; Cegla, H. M.; Cameron, A. C.; Costes, J.; Dumusque, X.; Langellier, Nicholas; Latham, David W.; Maldonado, J.; Malavolta, L.; Mortier, A.; Palumbo, Michael L.,III; Thompson, S.; Watson, C. A.; Bouchy, F.; Buchschacher, N.; Cecconi, M.; Charbonneau, David; Cosentino, R.; Ghedina, A.; Glenday, Alexander G.; Gonzalez, M.; Li, C. -H; Lodi, M.; López-Morales, Mercedes; Lovis, C.; Mayor, M.; Micela, G.; Molinari, E.; Pepe, F.; Piotto, G.; Rice, K.; Sasselov, Dimitar; Ségransan, D.; Sozzetti, A.; Szentgyorgyi, Andrew; Udry, S.; Walsworth, Ronald L. (2019)
    State-of-the-art radial-velocity (RV) exoplanet searches are currently limited by RV signals arising from stellar magnetic activity. We analyze solar observations acquired over a 3 yr period during the decline of Carrington ...
  • A set of microsatellite markers for Heliconius melpomene and closely related species 
    Mavarez, J.; Gonzalez, M. (2006)
  • Spitzer Observations of Extended Lyman-a Clouds in the SSA22 Field 
    Webb, T. M. A.; Yamada, T.; Huang, J. -S; Ashby, Matthew L. N.; Matsuda, Y.; Egami, E.; Gonzalez, M.; Hayashimo, T. (2009)
  • Temporal evolution and correlations of optical activity indicators measured in Sun-as-a-star observations 
    Maldonado, J.; Phillips, David F.; Dumusque, X.; Collier Cameron, A.; Haywood, Raphaëlle D.; Lanza, A. F.; Micela, G.; Mortier, A.; Saar, Steven H.; Sozzetti, A.; Rice, K.; Milbourne, Timothy; Cecconi, M.; Cegla, H. M.; Cosentino, R.; Costes, J.; Ghedina, A.; Gonzalez, M.; Guerra, J.; Hernández, N.; Li, C. -H; Lodi, M.; Malavolta, L.; Molinari, E.; Pepe, F.; Piotto, G.; Poretti, E.; Sasselov, Dimitar; San Juan, J.; Thompson, S.; Udry, S.; Watson, C. (2019)
    Context. Understanding stellar activity in solar-type stars is crucial for the physics of stellar atmospheres as well as for ongoing exoplanet programmes. Aims: We aim to test how well we understand stellar activity using ...
  • Three years of Sun-as-a-star radial-velocity observations on the approach to solar minimum 
    Collier Cameron, A.; Mortier, A.; Phillips, David; Dumusque, X.; Haywood, Raphaëlle D.; Langellier, Nicholas; Watson, C. A.; Cegla, H. M.; Costes, J.; Charbonneau, David; Coffinet, A.; Latham, David W.; Lopez-Morales, Mercedes; Malavolta, L.; Maldonado, J.; Micela, G.; Milbourne, Timothy; Molinari, Emilio; Saar, S. H.; Thompson, S.; Buchschacher, Nicholas; Cecconi, M.; Cosentino, R.; Ghedina, A.; Glenday, Alexander G.; Gonzalez, M.; Li, C. -H; Lodi, M.; Lovis, C.; Pepe, F.; Poretti, E.; Rice, K.; Sasselov, Dimitar; Sozzetti, A.; Szentgyorgyi, Andrew; Udry, S.; Walsworth, Ronald L. (2019)
    The time-variable velocity fields of solar-type stars limit the precision of radial-velocity determinations of their planets' masses, obstructing detection of Earth twins. Since 2015 July, we have been monitoring ...

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