Zobrazeno 1 - 10
of 1 151
pro vyhledávání: '"Busuttil, R"'
Autor:
Staab, D., Haswell, C. A., Smith, Gareth D., Fossati, L., Barnes, J. R., Busuttil, R., Jenkins, J. S.
We measured the chromospheric activity of the four hot Jupiter hosts WASP-43, WASP-51/HAT-P-30, WASP-72 & WASP-103 to search for anomalous values caused by the close-in companions. The Mount Wilson Ca II H&K S-index was calculated for each star using
Externí odkaz:
http://arxiv.org/abs/1612.01739
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
Autor:
Campbell, H. C., Marsh, T. R., Fraser, M., Hodgkin, S. T., de Miguel, E., Gänsicke, B. T., Steeghs, D., Hourihane, A., Breedt, E., Littlefair, S. P., Koposov, S. E., Wyrzykowski, L., Altavilla, G., Blagorodnova, N., Clementini, G., Damljanovic, G., Delgado, A., Dennefeld, M., Drake, A. J., Fernández-Hernández, J., Gilmore, G., Gualandi, R., Hamanowicz, A., Handzlik, B., Hardy, L. K., Harrison, D. L., Ilkiewicz, K., Jonker, P. G., Kochanek, C. S., Kolaczkowski, Z., Kostrzewa-Rutkowska, Z., Kotak, R., van Leeuwen, G., Leto, G., Ochner, P., Pawlak, M., Palaversa, L., Rixon, G., Rybicki, K., Shappee, B. J., Smartt, S. J., Torres, M. A. P., Tomasella, L., Turatto, M., Ulaczyk, K., van Velzen, S., Vince, O., Walton, N. A., Wielgórski, P., Wevers, T., Whitelock, P., Yoldas, A., De Angeli, F., Burgess, P., Busso, G., Busuttil, R., Butterley, T., Chambers, K. C., Copperwheat, C., Danilet, A. B., Dhillon, V. S., Evans, D. W., Eyer, L., Froebrich, D., Gomboc, A., Holland, G., Holoien, T. W. -S., Jarvis, J. F., Kaiser, N., Kann, D. A., Koester, D., Kolb, U., Komossa, S., Magnier, E. A., Mahabal, A., Polshaw, J., Prieto, J. L., Prusti, T., Riello, M., Scholz, A., Simonian, G., Stanek, K. Z., Szabados, L., Waters, C., Wilson, R. W.
We report the discovery and characterisation of a deeply eclipsing AM CVn-system, Gaia14aae (= ASSASN-14cn). Gaia14aae was identified independently by the All-Sky Automated Survey for Supernovae (ASAS-SN; Shappee et al. 2014) and by the Gaia Science
Externí odkaz:
http://arxiv.org/abs/1507.04663
Autor:
Lohr, M. E., Norton, A. J., Gillen, E., Busuttil, R., Kolb, U. C., Aigrain, S., McQuillan, A., Hodgkin, S. T., González, E.
Publikováno v:
A&A 578, A103 (2015)
Our discovery of 1SWASP J093010.78+533859.5 as a probable doubly eclipsing quadruple system containing a contact binary with P~0.23 d and a detached binary with P~1.31 d was announced in 2013. Subsequently Koo et al. confirmed the detached binary spe
Externí odkaz:
http://arxiv.org/abs/1504.07065
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:
Maxted, P. F. L., Bloemen, S., Heber, U., Geier, S., Wheatley, P. J., Marsh, T. R., Breedt, E., Sebastian, D., Faillace, G., Owen, C., Pulley, D., Smith, D., Kolb, U., Haswell, C. A., Southworth, J., Anderson, D. R., Smalley, B., Cameron, A. Collier, Hebb, L., Simpson, E. K., West, R. G., Bochinski, J., Busuttil, R., Hadigal, S.
The star 1SWASP J024743.37-251549.2 was recently discovered to be a binary star in which an A-type dwarf star eclipses the remnant of a disrupted red giant star (WASP0247-25B). The remnant is in a rarely-observed state evolving to higher effective te
Externí odkaz:
http://arxiv.org/abs/1310.4863
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:
Haswell, C. A., Fossati, L., Ayres, T., France, K., Froning, C. S., Holmes, S., Kolb, U. C., Busuttil, R., Street, R. A., Hebb, L., Cameron, A. Collier, Enoch, B., Burwitz, V., Rodriguez, J., West, R. G., Pollacco, D., Wheatley, P. J., Carter, A.
Publikováno v:
2012, The Astrophysical Journal, 760, 79
We observed the extreme close-in hot Jupiter system WASP-12 with HST. Near-UV transits up to three times deeper than the optical transit of WASP-12b reveal extensive diffuse gas, extending well beyond the Roche lobe. The distribution of absorbing gas
Externí odkaz:
http://arxiv.org/abs/1301.1860
Autor:
Sosa, R.A., Bhat, A., Yin, Y., Naini, B., Zheng, Y., Gjertson, D., Busuttil, R., Kupiec-Weglinski, J., Kaldas, F.M., Reed, E.F.
Publikováno v:
In Human Immunology September 2024 85 Supplement
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