Search Results - "Maxted, P FL"

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    WASP-South transiting exoplanets: WASP-130b, WASP-131b, WASP-132b, WASP-139b, WASP-140b, WASP-141b and WASP-142b by Hellier, C, Anderson, D R, Cameron, A Collier, Delrez, L, Gillon, M, Jehin, E, Lendl, M, Maxted, P FL, Neveu-VanMalle, M, Pepe, F, Pollacco, D, Queloz, D, Segransan, D, Smalley, B, Southworth, J, Triaud, A HMJ, Udry, S, Wagg, T, West, R G

    “…We describe seven exoplanets transiting stars of brightness V = 10.1-12.4. WASP-130b is a 'warm Jupiter' having an orbital period of 11.6 d around a metal-rich…”
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    Pulsation versus metallicism in Am stars as revealed by LAMOST and WASP by Smalley, B, Antoci, V, Holdsworth, D L, Kurtz, D W, Murphy, S J, DeCat, P, Anderson, D R, Catanzaro, G, Cameron, A Collier, Hellier, C, Maxted, P FL, Norton, A J, Pollacco, D, Ripepi, V, West, R G, Wheatley, P J

    “…Abstract We present the results of a study of a large sample of A and Am stars with spectral types from LAMOST and light curves from WASP. We find that, unlike…”
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    A kinematically unbiased search for nearby young stars in the Northern hemisphere selected using SuperWASP rotation periods by Binks, A. S., Jeffries, R. D., Maxted, P. F. L.

    “…We present a kinematically-unbiased search to identify young, nearby low-mass members of kinematic moving groups (MGs). Objects with both rotation periods…”
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    Multiwaveband photometry of the irradiated brown dwarf WD0137−349B by Casewell, S L, Lawrie, K A, Maxted, P FL, Marley, M S, tney, J J, Rimmer, P B, Littlefair, S P, Wynn, G, Burleigh, M R, Helling, Ch

    “…WD0137-349 is a white dwarf-brown dwarf binary system in a 116 min orbit. We present radial velocity observations and multiwaveband photometry from V, R and I…”
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    Thermal emission at 3.6-8 [mu]m from WASP-19b: a hot Jupiter without a stratosphere orbiting an active star by Anderson, D R, Smith, A MS, Madhusudhan, N, Wheatley, P J, Cameron, A Collier, Hellier, C, Campo, C, Gillon, M, Harrington, J, Maxted, P FL, Pollacco, D, Queloz, D, Smalley, B, Triaud, A HMJ, West, R G

    “…We report detection of thermal emission from the exoplanet WASP-19b at 3.6, 4.5, 5.8 and 8.0 μm. We used the InfraRed Array Camera on the Spitzer Space…”
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