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Sökning: id:"swepub:oai:DiVA.org:uu-319332" > Zodiacal exoplanets...

Zodiacal exoplanets in time (ZEIT) - II. A 'super-Earth' orbiting a young K dwarf in the Pleiades Neighbourhood

Gaidos, E. (författare)
Univ Hawaii Manoa, Dept Geol & Geophys, Honolulu, HI 96822 USA.
Mann, A. W. (författare)
Univ Texas Austin, Dept Astron, Austin, TX 78712 USA.
Rizzuto, A. (författare)
Univ Texas Austin, Dept Astron, Austin, TX 78712 USA.
visa fler...
Nofi, L. (författare)
Univ Hawaii Manoa, Inst Astron, Honolulu, HI 96822 USA.
Mace, G. (författare)
Univ Texas Austin, Dept Astron, Austin, TX 78712 USA.
Vanderburg, A. (författare)
Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA.
Feiden, Gregory (författare)
Uppsala universitet,Teoretisk astrofysik
Narita, N. (författare)
Univ Tokyo, Dept Astron, Bunkyo Ku, Tokyo 1130038, Japan.;Natl Inst Nat Sci, Astrobiol Ctr, Mitaka, Tokyo 1818588, Japan.;Natl Astron Observ Japan, Mitaka, Tokyo 1818588, Japan.;SOKENDAI Grad Univ Adv Studies, Mitaka, Tokyo 1818588, Japan.
Takeda, Y. (författare)
Natl Astron Observ Japan, Mitaka, Tokyo 1818588, Japan.
Esposito, T. M. (författare)
Univ Calif Berkeley, Dept Astron, 601 Campbell Hall, Berkeley, CA 94720 USA.
De Rosa, R. J. (författare)
Univ Calif Berkeley, Dept Astron, 601 Campbell Hall, Berkeley, CA 94720 USA.
Ansdell, M. (författare)
Univ Hawaii Manoa, Inst Astron, Honolulu, HI 96822 USA.
Hirano, T. (författare)
Tokyo Inst Technol, Dept Earth & Planetary Sci, Meguro Ku, Tokyo 1528551, Japan.
Graham, J. R. (författare)
Univ Calif Berkeley, Dept Astron, 601 Campbell Hall, Berkeley, CA 94720 USA.
Kraus, A. (författare)
Univ Texas Austin, Dept Astron, Austin, TX 78712 USA.
Jaffe, D. (författare)
Univ Texas Austin, Dept Astron, Austin, TX 78712 USA.
visa färre...
Univ Hawaii Manoa, Dept Geol & Geophys, Honolulu, HI 96822 USA Univ Texas Austin, Dept Astron, Austin, TX 78712 USA. (creator_code:org_t)
2016-09-15
2017
Engelska.
Ingår i: Monthly notices of the Royal Astronomical Society. - : Oxford University Press. - 0035-8711 .- 1365-2966. ; 464:1, s. 850-862
  • Tidskriftsartikel (refereegranskat)
Abstract Ämnesord
Stäng  
  • We describe a 'super-Earth'-size (2.30 +/- 0.16 R-circle plus)planet transiting an early K-type dwarf star in the Campaign 4 field observed by the K2 mission. The host star, EPIC 210363145, was identified as a candidate member of the approximately 120 Myr-old Pleiades cluster based on its kinematics and photometric distance. It is rotationally variable and exhibits near-ultraviolet emission consistent with a Pleiades age, but its rotational period is approximate to 20 d and its spectrum contains no H alpha emission nor the Li I absorption expected of Pleiades K dwarfs. Instead, the star is probably an interloper that is unaffiliated with the cluster, but younger (less than or similar to 1.3 Gyr) than the typical field dwarf. We ruled out a false positive transit signal produced by confusion with a background eclipsing binary by adaptive optics imaging and a statistical calculation. Doppler radial velocity measurements limit the companion mass to <2 times that of Jupiter. Screening of the light curves of 1014 potential Pleiades candidate stars uncovered no additional planets. An injection-and-recovery experiment using the K2 Pleiades light curves with simulated planets, assuming a planet population like that in the Kepler prime field, predicts only 0.8-1.8 detections (versus similar to 20 in an equivalent Kepler sample). The absence of Pleiades planet detections can be attributed to the much shorter monitoring time of K2 (80 d versus 4 yr), increased measurement noise due to spacecraft motion, and the intrinsic noisiness of the stars.

Ämnesord

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Nyckelord

planets and satellites:general
stars:low-mass
planetary systems
open clusters and associations:individual:Pleiades

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