Pith. sign in

REVIEW

EPIC211089792 b: an aligned and inflated hot jupiter in a young visual binary

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1601.07680 v1 pith:POUNNZNN submitted 2016-01-28 astro-ph.EP

EPIC211089792 b: an aligned and inflated hot jupiter in a young visual binary

A. Santerne , G. H\'ebrard , J. Lillo-Box , D. J. Armstrong , S. C. C. Barros , O. Demangeon , D. Barrado , A. Debackere
show 66 more authors
M. Deleuil E. Delgado Mena M. Montalto D. Pollacco H. P. Osborn S. G. Sousa L. Abe V. Adibekyan J.-M. Almenara P. Andr\'e G. Arlic G. Barthe P. Bendjoya R. Behrend I. Boisse F. Bouchy H. Boussier M. Bretton D. J. A. Brown B. Carry A. Cailleau E. Conseil B. Courcol B. Dauchet J.-C. Dalouzy M. Deldem P. Dubreuil J.-M. Fehrenbach S. Ferratfiat R. Girelli J. Gregorio S. Jaecques F. Kugel J. Kirk O. Labrevoir J.-C. Lachuri\'e K. W. F. Lam P. Le Guen P. Martinez L. Maurin J. McCormac J-B. Pioppa U. Quadri A. Rajpurohit J. Rey J.-P. Rivet R. Roy N. C. Santos F. Signoret L. Strabla O. Suarez D. Toublanc M. Tsantaki P. A. Wilson M. Bachschmidt F. Colas O. Gerteis P. Louis J.-C. Mario C. Marlot J. Montier V. Perroud V. Pic D. Romeuf S. Ubaud D. Verilhac
This is my paper
classification astro-ph.EP
keywords planetstellaralignedbrightcompanionepic211089792jupiternearby
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

In the present paper we report the discovery of a new hot Jupiter, EPIC211089792 b, first detected by the Super-WASP observatory and then by the K2 space mission during its campaign 4. The planet has a period of 3.25d, a mass of 0.73 +/- 0.04 Mjup, and a radius of 1.19 +/- 0.02 Rjup. The host star is a relatively bright (V=12.5) G7 dwarf with a nearby K5V companion. Based on stellar rotation and the abundance of Lithium, we find that the system might be as young as about 450 Myr. The observation of the Rossiter-McLaughlin effect shows the planet is aligned with respect to the stellar spin. Given the deep transit (20mmag), the magnitude of the star and the presence of a nearby stellar companion, the planet is a good target for both space- and ground-based transmission spectroscopy, in particular in the near-infrared where the both stars are relatively bright.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.