Zobrazeno 1 - 10
of 245
pro vyhledávání: '"Miller, G. R."'
Autor:
Hay, K. L., Collier-Cameron, A., Doyle, A. P., Hébrard, G., Skillen, I., Anderson, D. R., Barros, S. C. C., Brown, D. J. A., Bouchy, F., Busuttil, R., Delorme, P., Delrez, L., Demangeon, O., Díaz, R. F., Gillon, M., Gonzàlez, E., Hellier, C., Holmes, S., Jarvis, J. F., Jehin, E., Joshi, Y. C., Kolb, U., Lendl, M., Maxted, P. F. L., McCormac, J., Miller, G. R. M., Mortier, A., Pollacco, D., Queloz, D., Ségransan, D., Simpson, E. K., Smalley, B., Southworth, J., Triaud, A. H. M. J., Turner, O. D., Udry, S., Vanhuysse, M., West, R. G., Wilson, P. A.
We present the discovery of three new transiting giant planets, first detected with the WASP telescopes, and establish their planetary nature with follow up spectroscopy and ground-based photometric lightcurves. WASP-92 is an F7 star, with a moderate
Externí odkaz:
http://arxiv.org/abs/1607.00774
A Window on Exoplanet Dynamical Histories: Rossiter-McLaughlin Observations of WASP-13b and WASP-32b
Autor:
Brothwell, R. D., Watson, C. A., Hebrard, G., Triaud, A. H. M. J., Cegla, H. M., Santerne, A., Hebrard, E., Anderson, D. R., Pollacco, D., Simpson, E. K., Bouchy, F., Brown, D. J. A., Chew, Y. Gomez Maqueo, Cameron, A. Collier, Armstrong, D. J., Barros, S. C. C., Bento, J., Bochinski, J., Burwitz, V., Busuttil, R., Delrez, L., Doyle, A. P., Faedi, F., Fumel, A., Gillon, M., Haswell, C. A., Hellier, C., Jehin, E., Kolb, U., Lendl, M., Liebig, C., Maxted, P. F. L., McCormac, J., Miller, G. R. M., Norton, A. J., Pepe, F., Queloz, D., Rodriguez, J., Segransan, D., Skillen, I., Smalley, B., Stassun, K. G., Udry, S., West, R. G., Wheatley, P. J.
We present Rossiter-McLaughlin observations of WASP-13b and WASP-32b and determine the sky-projected angle between the normal of the planetary orbit and the stellar rotation axis ($\lambda$). WASP-13b and WASP-32b both have prograde orbits and are co
Externí odkaz:
http://arxiv.org/abs/1403.4095
Autor:
Chew, Y. Gómez Maqueo, Faedi, F., Pollacco, D., Brown, D. J. A., Doyle, A. P., Cameron, A. Collier, Gillon, M., Lendl, M., Smalley, B., Triaud, A. H. M. J., West, R. G., Wheatley, P. J., Busuttil, R., Liebig, C., Anderson, D. R., Armstrong, D. J., Barros, S. C. C., Bento, J., Bochinski, J., Burwitz, V., Delrez, L., Enoch, B., Fumel, A., Haswell, C. A., Hébrard, G., Hellier, C., Holmes, S., Jehin, E., Kolb, U., Maxted, P. F. L., McCormac, J., Miller, G. R. M., Norton, A. J., Pepe, F., Queloz, D., Rodríguez, J., Ségransan, D., Skillen, I., Stassun, K. G., Udry, S., Watson, C. A.
We report the discovery of two transiting hot Jupiters, WASP-65b (M_pl = 1.55 +/- 0.16 M_J; R_pl = 1.11 +/- 0.06 R_J), and WASP-75b (M_pl = 1.07 +/- 0.05 M_J; R_pl = 1.27 +/- 0.05 R_J). They orbit their host star every 2.311, and 2.484 days, respecti
Externí odkaz:
http://arxiv.org/abs/1307.6532
Autor:
Brown, D. J. A., Cameron, A. Collier, Díaz, R. F., Doyle, A. P., Gillon, M., Lendl, M., Smalley, B., Triaud, A. H. M. J., Anderson, D. R., Enoch, B., Hellier, C., Maxted, P. F. L., Miller, G. R. M., Pollacco, D., Queloz, D., Boisse, I., Hébrard, G.
Publikováno v:
Brown, D. J. A. et al., (2012), ApJ 760, 139
We present measurements of the spin-orbit alignment angle, lambda, for the hot Jupiter systems WASP-32, WASP-38, and HAT-P-27/WASP-40, based on data obtained using the HARPS spectrograph. We analyse the Rossiter-McLaughlin effect for all three system
Externí odkaz:
http://arxiv.org/abs/1303.5649
Autor:
Faedi, F., Pollacco, D., Barros, S. C. C., Brown, D., Cameron, A. Collier, Doyle, A. P., Enoch, R., Gillon, M., Chew, Y. Gomez Maqueo, Hebrard, G., Lendl, M., Liebig, C., Smalley, B., Triaud, A. H. M. J., West, R. G., Wheatley, P. J., Alsubai, K. A., Anderson, D. R., Armstrong, D. J., Bento, J., Bochinski, J., Bouchy, F., Busuttil, R., Fossati, L., Fumel, A., Haswell, C. A., Hellier, C., Holmes, S., Jehin, E., Kolb, U., McCormac, J., Miller, G. R. M., Moutou, C., Norton, A. J., Parley, N., Queloz, D., Santerne, A., Skillen, I., Smith, A. M. S., Udry, S., Watson, C.
We present three newly discovered sub-Jupiter mass planets from the SuperWASP survey: WASP-54b is a heavily bloated planet of mass 0.636$^{+0.025}_{-0.024}$ \mj and radius 1.653$^{+0.090}_{-0.083}$ \rj. It orbits a F9 star, evolving off the main sequ
Externí odkaz:
http://arxiv.org/abs/1210.2329
Autor:
Brown, D. J. A., Cameron, A. Collier, Anderson, D. R., Enoch, B., Hellier, C., Maxted, P. F. L., Miller, G. R. M., Pollacco, D., Queloz, D., Simpson, E., Smalley, B., Triaud, A. H. M. J., Boisse, I., Bouchy, F., Gillon, M., Hebrard, G.
We present new measurements of the Rossiter-McLaughlin (RM) effect for three WASP planetary systems, WASP-16, WASP-25 and WASP-31, from a combined analysis of their complete sets of photometric and spectroscopic data. We find a low amplitude RM effec
Externí odkaz:
http://arxiv.org/abs/1203.4971
Autor:
Enoch, B., Anderson, D. R., Barros, S. C. C., Brown, D. J. A., Cameron, A. Collier, Faedi, F., Gillon, M., Hébrard, G., Lister, T. A., Queloz, D., Santerne, A., Smalley, B., Street, R. A., Triaud, A. H. M. J., West, R. G., Bouchy, F., Bento, J., Butters, O., Fossati, L., Haswell, C. A., Hellier, C., Holmes, S., Jehen, E., Lendl, M., Maxted, P. F. L., McCormac, J., Miller, G. R. M., Moulds, V., Moutou, C., Norton, A. J., Parley, N., Pepe, F., Pollacco, D., Segransan, D., Simpson, E., Skillen, I., Smith, A. M. S., Udry, S., Wheatley, P. J.
We report the detection of WASP-35b, a planet transiting a metal-poor ([Fe/H] = -0.15) star in the Southern hemisphere, WASP-48b, an inflated planet which may have spun-up its slightly evolved host star of 1.75 R_sun in the Northern hemisphere, and t
Externí odkaz:
http://arxiv.org/abs/1104.2827
Autor:
Faedi, F., Barros, S. C. C., Anderson, D. R., Brown, D. J. A., Cameron, A. Collier, Pollacco, D., Boisse, I., Hebrard, G., Lendl, M., Lister, T. A., Smalley, B., Street, R. A., Triaud, A. H. M. J., Bento, J., Butters, O. W., Enoch, B., Bouchy, F., Haswell, C. A., Hellier, C., Keenan, F. P., Miller, G. R. M., Moulds, V., Moutou, C., Norton, A. J., Queloz, D., Santerne, A., Simpson, E. K., Skillen, I., Smith, A. M. S., Udry, S., Watson, C. A., West, R. G., Wheatley, P. J.
We present the discovery of WASP-39b, a highly inflated transiting Saturn-mass planet orbiting a late G-type dwarf star with a period of $4.055259 \pm 0.000008$\,d, Transit Epoch T$_{0}=2455342.9688\pm0.0002$\,(HJD), of duration $0.1168 \pm 0.0008$\,
Externí odkaz:
http://arxiv.org/abs/1102.1375
Autor:
Hellier, Coel, Anderson, D. R., Cameron, A. Collier, Miller, G. R. M., Queloz, D., Smalley, B., Southworth, J., Triaud, A. H. M. J.
WASP-19b has the shortest orbital period of any known exoplanet, orbiting at only 1.2 times the Roche tidal radius. By observing the Rossiter-McLaughlin effect we show that WASP-19b's orbit is aligned, with lambda = 4.6 +/- 5.2 degrees. Using, in add
Externí odkaz:
http://arxiv.org/abs/1101.3293
Autor:
Simpson, E. K., Pollacco, D., Cameron, A. Collier, Hebrard, G., Anderson, D. R., Barros, S. C. C., Boisse, I., Bouchy, F., Faedi, F., Gillon, M., Hebb, L., Keenan, F. P., Miller, G. R. M., Moutou, C., Queloz, D., Skillen, I., Sorensen, P., Stempels, H. C., Triaud, A., Watson, C. A., Wilson, P. A.
We present observations of the Rossiter-McLaughlin effect for the transiting exoplanet systems WASP-1, WASP-24, WASP-38 and HAT-P-8, and deduce the orientations of the planetary orbits with respect to the host stars' rotation axes. The planets WASP-2
Externí odkaz:
http://arxiv.org/abs/1011.5664