Characterization of small planets with Kepler and HARPS-N
Journal
Date Issued
2015
Author(s)
•
•
Lovis, C.
•
•
Rice, K.
•
Dumusque, X.
•
Cameron, A. C.
•
Latham, D. W.
•
•
Pepe, F.
•
Udry, S.
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.
Coverage
The Space Photometry Revolution – CoRoT Symposium 3, Kepler KASC-7 Joint Meeting
All editors
García. R.A.; Ballot, J.
Volume
101
Start page
06011
Conferenece
The Space Photometry Revolution – CoRoT Symposium 3, Kepler KASC-7 Joint Meeting
Conferenece place
Toulouse, France
Conferenece date
July 6-11, 2014
Issn Identifier
2101-6275
Ads BibCode
2015EPJWC.10106011B
Rights
open.access
File(s)![Thumbnail Image]()
Loading...
Name
Bonomoetal.2015.pdf
Size
145.95 KB
Format
Adobe PDF
Checksum (MD5)
06eaa8ec856799aa69cab4d32d0756df