Characterization of small planets with Kepler and HARPS-N

A. S. Bonomo; A. Sozzetti; C. Lovis; L. Malavolta; K. Rice; X. Dumusque; A. C. Cameron; D. W. Latham; E. Molinari; F. Pepe; S. Udry

Characterization of small planets with Kepler and HARPS-N

A. S. Bonomo, A. Sozzetti, C. Lovis, L. Malavolta, K. Rice, X. Dumusque, A. C. Cameron, D. W. Latham, E. Molinari, F. Pepe, S. Udry

School of Physics and Astronomy

Research output: Contribution to conference › Abstract

Abstract

The high-accuracy and high-precision HARPS-N spectrograph has been installed at the italian Telescopio Nazionale Galileo in La Palma approximately two years and a half ago. Eighty nights per year of Guaranteed Time of Observation are mostly dedicated to the radial-velocity (RV) follow up of Kepler small-size planetary candidates to establish their nature and to determine accurately their masses. We report on recent results of this ongoing RV campaign, including the recent characterization of the planetary system Kepler-101.

Original language	English
Pages	6011
Publication status	Published - 1 Sep 2015

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http://adsabs.harvard.edu/abs/2015EPJWC.10106011B

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title = "Characterization of small planets with Kepler and HARPS-N",

abstract = "The high-accuracy and high-precision HARPS-N spectrograph has been installed at the italian Telescopio Nazionale Galileo in La Palma approximately two years and a half ago. Eighty nights per year of Guaranteed Time of Observation are mostly dedicated to the radial-velocity (RV) follow up of Kepler small-size planetary candidates to establish their nature and to determine accurately their masses. We report on recent results of this ongoing RV campaign, including the recent characterization of the planetary system Kepler-101.",

author = "Bonomo, {A. S.} and A. Sozzetti and C. Lovis and L. Malavolta and K. Rice and X. Dumusque and Cameron, {A. C.} and Latham, {D. W.} and E. Molinari and F. Pepe and S. Udry",

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day = "1",

language = "English",

pages = "6011",

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TY - CONF

T1 - Characterization of small planets with Kepler and HARPS-N

AU - Bonomo, A. S.

AU - Sozzetti, A.

AU - Lovis, C.

AU - Malavolta, L.

AU - Rice, K.

AU - Dumusque, X.

AU - Cameron, A. C.

AU - Latham, D. W.

AU - Molinari, E.

AU - Pepe, F.

AU - Udry, S.

PY - 2015/9/1

Y1 - 2015/9/1

N2 - The high-accuracy and high-precision HARPS-N spectrograph has been installed at the italian Telescopio Nazionale Galileo in La Palma approximately two years and a half ago. Eighty nights per year of Guaranteed Time of Observation are mostly dedicated to the radial-velocity (RV) follow up of Kepler small-size planetary candidates to establish their nature and to determine accurately their masses. We report on recent results of this ongoing RV campaign, including the recent characterization of the planetary system Kepler-101.

AB - The high-accuracy and high-precision HARPS-N spectrograph has been installed at the italian Telescopio Nazionale Galileo in La Palma approximately two years and a half ago. Eighty nights per year of Guaranteed Time of Observation are mostly dedicated to the radial-velocity (RV) follow up of Kepler small-size planetary candidates to establish their nature and to determine accurately their masses. We report on recent results of this ongoing RV campaign, including the recent characterization of the planetary system Kepler-101.

M3 - Abstract

SP - 6011

ER -

Characterization of small planets with Kepler and HARPS-N

Abstract

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