SIGLETIB: RN 5906(554) / FIZ - Fachinformationszzentrum Karlsruhe / TIB - Technische InformationsbibliothekDEGerman

Abe, L.

Adibekyan, V.

Almenara, J. -M.

André, P.

Arlic, G.

Armstrong, D. J.

Bachschmidt, M.

Barrado, D.

Barros, S. C. C.

Barthe, G.

Behrend, R.

Bendjoya, P.

Boisse, I.

Bouchy, F.

Boussier, H.

Bretton, M.

Brown, D. J. A.

Cailleau, A.

Carry, B.

Colas, Florent

Conseil, E.

Coulon, G.

Courcol, B.

Dalouzy, J. -C.

Dauchet, B.

Debackere, A.

Deldem, M.

Deleuil, M.

Delgado Mena, E.

Demangeon, O.

Desormieres, O.

Dubreuil, P.

Fehrenbach, J. -M.

Ferratfiat, S.

Gerteis, O.

Girelli, R.

Gregorio, J.

Hébrard, G.

Jaecques, S.

Kirk, J.

Kugel, F.

Labrevoir, O.

Lachurie, J. -C.

Lam, K. W. F.

Le Guen, P.

Lillo-Box, J.

Louis, P.

Mario, J. -C.

Marlot, C.

Martinez, P.

Maurin, L. P. A.

McCormac, J.

Montalto, M.

Montier, J.

Osborn, H. P.

Perroud, V.

Pic, V.

Pioppa, J-B.

Pollacco, D.

Quadri, U.

Rajpurohit, A.

Rey, J.

Rivet, J. -P.

Romeuf, D.

Roy, R.

Santerne, A.

Santos, N. C.

Signoret, F.

Sousa, S. G.

Strabla, L.

Suarez, O.

Toublanc, D.

Tsantaki, M.

Ubaud, S.

Verilhac, D.

Vienney, J. -M.

Wilson, P. A.

The Astrophysical Journal

arXiv

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 MX, and a radius of 1.19±0.02RX. 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

Armstrong, David J.

Barros, S. C. C

Pollacco, Don

Osborn, Hugh P.

Fehrenbach, S.

Kirk, James

Lachurié, J. -C.

Lam, K. W. F

Maurin, L.

McCormac, J. J.

Pioppa, J. -B.

Bachschmidt, F.

Warwick Research Archives Portal Repository

K2-29 b/WASP-152 b : an aligned and inflated hot jupiter in a young visual binary

International audienceIn the present paper we report the discovery of a new hot Jupiter, K2-29 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 3.25 days, a mass of 0.73 +/- 0.04M(sic), and a radius of 1.19 +/- 0.02 R(sic). 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 similar to 450 Myr. The observation of the Rossiter-McLaughlin effect shows that the planet is aligned with respect to the stellar spin. Given the deep transit (20 mmag), 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 both stars are relatively bright

Martinez, Pedro

Mccormac, J.

HAL: Hyper Article en Ligne

K2-29 b/WASP-152 b: AN ALIGNED AND INFLATED HOT JUPITER IN A YOUNG VISUAL BINARY

A. Santerne

G. Hébrard

J. Lillo-Box

D. J. Armstrong

S. C. C. Barros

O. Demangeon

D. Barrado

A. Debackere

M. Deleuil

E. Delgado Mena

M. Montalto

D. Pollacco

H. P. Osborn

S. G. Sousa

L. Abe

V. Adibekyan

J.-M. Almenara

P. André

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

G. Coulon

B. Courcol

B. Dauchet

J.-C. Dalouzy

M. Deldem

O. Desormières

P. Dubreuil

J.-M. Fehrenbach

S. Ferratfiat

R. Girelli

J. Gregorio

S. Jaecques

F. Kugel

J. Kirk

O. Labrevoir

J.-C. Lachurié

K. W. F. Lam

P. Le Guen

P. Martinez

L. P. A. 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

J.-M. Vienney

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

Crossref

Lauppe, W.D.

Richter, B.

Stein, G.

Kernforschungsanlage Juelich G.m.b.H. (KFA) (Germany). Programmgruppe Technik und Gesellschaft.

Bundesministerium fuer Forschung und Technologie (BMFT), Bonn (Germany)

OpenGrey Repository