Zobrazeno 1 - 10
of 1 786
pro vyhledávání: '"Doyle L"'
Publikováno v:
Open Access Journal of Sports Medicine, Vol Volume 10, Pp 171-183 (2019)
Fionn T McSwiney,1,2 Lorna Doyle,3 Daniel J Plews,4 Caryn Zinn4 1School of Health and Human Performance, Dublin City University, Dublin, Ireland; 2Setanta College, Thurlus, Tipperary, Ireland; 3Department of Sport and Exercise Science, Waterford Inst
Externí odkaz:
https://doaj.org/article/0cf493d67fdc464faa12d2391dd93483
Autor:
Ahrer, E., Seidel, J. V., Doyle, L., Gandhi, S., Prinoth, B., Cegla, H. M., McDonald, C. H., Astudillo-Defru, N., Ayache, E., Nealon, R., Veras, Dimitri, Wheatley, P. J., Ehrenreich, D.
We present high spectral resolution observations of the hot Jupiter WASP-94 A b using the HARPS instrument on ESO's 3.6m telescope in La Silla, Chile. We probed for Na absorption in its atmosphere as well as constrained the previously reported misali
Externí odkaz:
http://arxiv.org/abs/2404.06550
Autor:
Doyle, L., Cegla, H. M., Anderson, D. R., Lendl, M., Bourrier, V., Bryant, E., Vines, J., Allart, R., Bayliss, D., Burleigh, M. R., Buchschacher, N., Casewell, S. L., Hawthorn, F., Jenkins, J. S., Lafarga, M., Moyano, M., Psaridi, A., Roguet-Kern, N., Sosnowska, D., Wheatley, P.
In this paper, we present observations of two high-resolution transit datasets obtained with ESPRESSO of the bloated sub-Saturn planet WASP-131~b. We have simultaneous photometric observations with NGTS and EulerCam. In addition, we utilised photomet
Externí odkaz:
http://arxiv.org/abs/2304.12163
Autor:
Weiße, N., Esslinger, J., Howard, S., Foerster, F. M., Haberstroh, F., Doyle, L., Norreys, P., Schreiber, J., Karsch, S., Doepp, A.
Knowledge of spatio-temporal couplings such as pulse-front tilt or curvature is important to determine the focused intensity of high-power lasers. Common techniques to diagnose these couplings are either qualitative or require hundreds of measurement
Externí odkaz:
http://arxiv.org/abs/2303.01360
Autor:
Lafarga, M., Brogi, M., Gandhi, S., Cegla, H. M., Seidel, J. V., Doyle, L., Allart, R., Buchschacher, N., Lendl, M., Lovis, C., Sosnowska, D.
With high-resolution spectroscopy we can study exoplanet atmospheres and learn about their chemical composition, temperature profiles, and presence of clouds and winds, mainly in hot, giant planets. State-of-the-art instrumentation is pushing these s
Externí odkaz:
http://arxiv.org/abs/2302.04794
Autor:
Doyle, L., Cegla, H. M., Bryant, E., Bayliss, D., Lafarga, M., Anderson, D. R., Allart, R., Bourrier, V., Brogi, M., Buchschacher, N., Kunovac, V., Lendl, M., Lovis, C., Moyano, M., Roguet-Kern, N., Seidel, J. V., Sosnowska, D., Wheatley, P. J., Acton, J. S., Burleigh, M. R., Casewell, S. L., Gill, S., Goad, M. R., Henderson, B. A., Jenkins, J. S., Tilbrook, R. H., West, R. G.
In this paper, we present high-resolution spectroscopic transit observations from ESPRESSO of the super-Neptune WASP-166~b. In addition to spectroscopic ESPRESSO data, we analyse photometric data from {\sl TESS} of six WASP-166~b transits along with
Externí odkaz:
http://arxiv.org/abs/2207.10127
Autor:
Seidel, J. V., Cegla, H. M., Doyle, L., Lafarga, M., Brogi, M., Gandhi, S., Anderson, D. R., Allart, R., Buchschacher, N., Lovis, C., Sosnowska, D.
The hot Neptune desert, a distinct lack of highly irradiated planets in the size range of Neptune, remains one of the most intriguing results of exoplanet population studies. A deeper understanding of the atmosphere of exoplanets sitting at the edge
Externí odkaz:
http://arxiv.org/abs/2203.04494
In our previous study of low mass stars using TESS, we found a handful which show a periodic modulation on a period <1 d but also displayed no flaring activity. Here we present the results of a systematic search for Ultra Fast Rotators (UFRs) in the
Externí odkaz:
http://arxiv.org/abs/2007.04071
Detailed studies of the Sun have shown that sunspots and solar flares are closely correlated. Photometric data from Kepler/K2 has allowed similar studies to be carried out on other stars. Here, we utilise TESS photometric 2-min cadence of 167 low mas
Externí odkaz:
http://arxiv.org/abs/1908.02698
We present an analysis of K2 short cadence data of 34 M dwarfs which have spectral types in the range M0 - L1. Of these stars, 31 showed flares with a duration between $\sim$10-90 min. Using distances obtained from Gaia DR2 parallaxes, we determined
Externí odkaz:
http://arxiv.org/abs/1807.08592