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

doi:10.1051/epjconf/201510106011

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: Chapter in Book/Report/Conference proceeding › Conference contribution

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
Title of host publication	EPJ Web of Conferences
Subtitle of host publication	CoRoT Symposium 3, Kepler KASC-7 Joint Meeting on Space Photometry Revolution; Toulouse; France; 6 July 2014 through 11 July 2014
Publisher	EDP Sciences
Number of pages	4
Volume	101
DOIs	https://doi.org/10.1051/epjconf/201510106011
Publication status	Published - 23 Sept 2015
Event	CoRoT Symposium 3, Kepler KASC-7 Joint Meeting on Space Photometry Revolution - Toulouse, France Duration: 6 Jul 2014 → 11 Jul 2014 http://corot3-kasc7.sciencesconf.org/resource/page/id/3

Conference

Conference	CoRoT Symposium 3, Kepler KASC-7 Joint Meeting on Space Photometry Revolution
Country/Territory	France
City	Toulouse
Period	6/07/14 → 11/07/14
Internet address	http://corot3-kasc7.sciencesconf.org/resource/page/id/3

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10.1051/epjconf/201510106011Licence: CC BY

Bonomo_2015_epjconf_sphr2014_06011
© Owned by the authors, published by EDP Sciences, 2015. This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Final published version, 146 KBLicence: CC BY

EU FP7 Space ETAEARTH: ETAEARTH
Cameron, A. C. (PI)
European Commission
1/01/13 → 31/12/17
Project: Standard

Cite this

Bonomo, A. S., Sozzetti, A., Lovis, C., Malavolta, L., Rice, K., Dumusque, X., Cameron, A. C., Latham, D. W., Molinari, E., Pepe, F., & Udry, S. (2015). Characterization of small planets with Kepler and HARPS-N. In EPJ Web of Conferences: CoRoT Symposium 3, Kepler KASC-7 Joint Meeting on Space Photometry Revolution; Toulouse; France; 6 July 2014 through 11 July 2014 (Vol. 101). Article 06011 EDP Sciences. https://doi.org/10.1051/epjconf/201510106011

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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",

note = "A. S. Bonomo, L. Malavolta, and X. Dumusque acknowledge fundings from the European Union Seventh Framework Programme (FP7/2007-2013) under agreement No. 313014 “Measuring ETAEARTH: characterization of terrestrial planetary systems with Kepler, HARPS-N, and Gaia” [PI: Dr. Alessandro Sozzetti].; CoRoT Symposium 3, Kepler KASC-7 Joint Meeting on Space Photometry Revolution ; Conference date: 06-07-2014 Through 11-07-2014",

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day = "23",

doi = "10.1051/epjconf/201510106011",

language = "English",

volume = "101",

booktitle = "EPJ Web of Conferences",

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Bonomo, AS, Sozzetti, A, Lovis, C, Malavolta, L, Rice, K, Dumusque, X, Cameron, AC, Latham, DW, Molinari, E, Pepe, F & Udry, S 2015, Characterization of small planets with Kepler and HARPS-N. in EPJ Web of Conferences: CoRoT Symposium 3, Kepler KASC-7 Joint Meeting on Space Photometry Revolution; Toulouse; France; 6 July 2014 through 11 July 2014. vol. 101, 06011, EDP Sciences, CoRoT Symposium 3, Kepler KASC-7 Joint Meeting on Space Photometry Revolution, Toulouse, France, 6/07/14. https://doi.org/10.1051/epjconf/201510106011

Characterization of small planets with Kepler and HARPS-N. / Bonomo, A. S.; Sozzetti, A.; Lovis, C. et al.
EPJ Web of Conferences: CoRoT Symposium 3, Kepler KASC-7 Joint Meeting on Space Photometry Revolution; Toulouse; France; 6 July 2014 through 11 July 2014. Vol. 101 EDP Sciences, 2015. 06011.

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

TY - GEN

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.

N1 - A. S. Bonomo, L. Malavolta, and X. Dumusque acknowledge fundings from the European Union Seventh Framework Programme (FP7/2007-2013) under agreement No. 313014 “Measuring ETAEARTH: characterization of terrestrial planetary systems with Kepler, HARPS-N, and Gaia” [PI: Dr. Alessandro Sozzetti].

PY - 2015/9/23

Y1 - 2015/9/23

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.

U2 - 10.1051/epjconf/201510106011

DO - 10.1051/epjconf/201510106011

M3 - Conference contribution

AN - SCOPUS:84960154298

VL - 101

BT - EPJ Web of Conferences

PB - EDP Sciences

T2 - CoRoT Symposium 3, Kepler KASC-7 Joint Meeting on Space Photometry Revolution

Y2 - 6 July 2014 through 11 July 2014

ER -

Characterization of small planets with Kepler and HARPS-N

Abstract

Conference

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Projects

EU FP7 Space ETAEARTH: ETAEARTH

Cite this