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2019MNRAS.490.5103D - Mon. Not. R. Astron. Soc., 490, 5103-5121 (2019/December-3)
Using HARPS-N to characterize the long-period planets in the PH-2 and Kepler-103 systems.
DUBBER S.C., MORTIER A., RICE K., NAVA C., MALAVOLTA L., GILES H., COFFINET A., CHARBONNEAU D., VANDERBURG A., BONOMO A.S., BOSCHIN W., BUCHHAVE L.A., CAMERON A.C., COSENTINO R., DUMUSQUE X., GHEDINA A., HARUTYUNYAN A., HAYWOOD R.D., LATHAM D., LOPEZ-MORALES M., MICELA G., MOLINARI E., PEPE F.A., PHILLIPS D., PIOTTO G., PORETTI E., SASSELOV D., SOZZETTI A. and UDRY S.
Abstract (from CDS):
Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): techniques: photometric - techniques: radial velocities - techniques: spectroscopic - planets and satellites: composition
Simbad objects: 17
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