SIMBAD references

2019MNRAS.488.3067H - Mon. Not. R. Astron. Soc., 488, 3067-3075 (2019/September-3)

WASP-166b: a bloated super-Neptune transiting a V = 9 star.

HELLIER C., ANDERSON D.R., TRIAUD A.H.M.J., BOUCHY F., BURDANOV A., COLLIER CAMERON A., DELREZ L., EHRENREICH D., GILLON M., JEHIN E., LENDL M., LINDER E., NIELSEN L.D., MAXTED P.F.L., PEPE F., POLLACCO D., QUELOZ D., SEGRANSAN D., SMALLEY B., SPAKE J.J., TEMPLE L.Y., UDRY S., WEST R.G. and WYTTENBACH A.

Abstract (from CDS):

We report the discovery of WASP-166b, a super-Neptune planet with a mass of 0.1 MJup (1.9 MNep) and a bloated radius of 0.63 RJup. It transits a V = 9.36, F9V star in a 5.44-d orbit that is aligned with the stellar rotation axis (sky-projected obliquity angle λ = 3 ± 5 deg). Variations in the radial-velocity measurements are likely the result of magnetic activity over a 12-d stellar rotation period. WASP-166b appears to be a rare object within the 'Neptune desert'.

Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): stars: individual: (WASP-166)

Status at CDS : Large table(s) will be appraised for possible ingestion in VizieR.

Simbad objects: 21

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2021.12.04-00:45:32

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