Zobrazeno 1 - 10
of 1 217
pro vyhledávání: '"Bentley, S"'
Publikováno v:
Patient Preference and Adherence, Vol Volume 18, Pp 1231-1242 (2024)
Sarah Bentley,1 Elizabeth Exall,1 Lucy Morgan,1 Nicolas Roche,2 Kamlesh Khunti,3 Rebecca Rossom,4 James Piercy,5 Rob Arbuckle,1 Victoria S Higgins5 1Patient-Centered Outcomes, Adelphi Values, Bollington, UK; 2Respiratory Medicine, Cochin Hospital, AP
Externí odkaz:
https://doaj.org/article/7807b917bde144a895be2962d1872aa7
Publikováno v:
Patient Preference and Adherence, Vol Volume 16, Pp 2579-2592 (2022)
Sarah Bentley,1 Lucy Morgan,1 Elizabeth Exall,1 Rob Arbuckle,1 Rebecca C Rossom,2 Nicholas Roche,3 Kamlesh Khunti,4 Victoria Higgins,5 James Piercy5 1Patient-Centered Outcomes, Adelphi Values, Bollington, Cheshire, UK; 2HealthPartners Institute, Univ
Externí odkaz:
https://doaj.org/article/9c5bee1c2902418b9525d1e6fdd26bd9
Autor:
Dixon, E., Dick, K., Ollosson, S., Jones, D., Mattock, H., Bentley, S., Saunders, C., Matthews, J., Dobra, B., King, J., Edmondson, C., Davies, J.C.
Publikováno v:
In Paediatric Respiratory Reviews June 2022 42:23-28
Akademický článek
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Publikováno v:
In Journal of Molecular Spectroscopy February 2019 356:21-27
Autor:
Geier, S., Hirsch, H., Tillich, A., Maxted, P. F. L., Bentley, S. J., Oestensen, R. H., Heber, U., Gaensicke, B. T., Marsh, T. R., Napiwotzki, R., Barlow, B. N., O'Toole, S. J.
The project Massive Unseen Companions to Hot Faint Underluminous Stars from SDSS (MUCHFUSS) aims at finding sdBs with compact companions like supermassive white dwarfs (M>1.0 Msun), neutron stars or black holes. The existence of such systems is predi
Externí odkaz:
http://arxiv.org/abs/1103.4045
Autor:
Smalley, B., Anderson, D. R., Cameron, A. Collier, Hellier, C., Lendl, M., Maxted, P. F. L., Queloz, D., Triaud, A. H. M. J., West, R. G., Bentley, S. J., Enoch, B., Gillon, M., Lister, T. A., Pepe, F., Pollacco, D., Segransan, D., Smith, A. M. S., Southworth, J., Udry, S., Wheatley, P. J., Wood, P. L., Bento, J.
We report the discovery of WASP-34b, a sub-Jupiter-mass exoplanet transiting its 10.4-magnitude solar-type host star (1SWASP J110135.89-235138.4; TYC 6636-540-1) every 4.3177 days in a slightly eccentric orbit (e = 0.038 +/- 0.012). We find a planeta
Externí odkaz:
http://arxiv.org/abs/1012.2278
Autor:
Smalley, B., Anderson, D. R., Cameron, A. Collier, Gillon, M., Hellier, C., Lister, T. A., Maxted, P. F. L., Queloz, D., Triaud, A. H. M. J., West, R. G., Bentley, S. J., Enoch, B., Pepe, F., Pollacco, D. L., Segransan, D., Smith, A. M. S., Southworth, J., Udry, S., Wheatley, P. J., Wood, P. L., Bento, J.
We report the discovery of WASP-26b, a moderately over-sized Jupiter-mass exoplanet transiting its 11.3-magnitude early-G-type host star (1SWASP J001824.70-151602.3; TYC 5839-876-1) every 2.7566 days. A simultaneous fit to transit photometry and radi
Externí odkaz:
http://arxiv.org/abs/1004.1542
Autor:
Maxted, P. F. L., Anderson, D. R., Gillon, M., Hellier, C., Queloz, D., Smalley, B., Triaud, A. H. M. J., West, R. G., Wilson, D. M., Bentley, S. J., Cegla, H., Cameron, A. Collier, Enoch, B., Hebb, L., Horne, K., Irwin, J., Lister, T. A., Mayor, M., Parley, N., Pepe, F., Pollacco, D., Segransan, D., Udry, S., Wheatley, P. J.
We report the discovery of a transiting planet orbiting the star TYC 6446-326-1. The star, WASP-22, is a moderately bright (V=12.0) solar-type star (Teff = 6000 +/- 100 K, [Fe/H] = -0.05 +/- 0.08). The lightcurve of the star obtained with the WASP-So
Externí odkaz:
http://arxiv.org/abs/1004.1514
Autor:
Hebb, Leslie, Collier-Cameron, A., Triaud, A. H. M. J., Lister, T. A., Smalley, B., Maxted, P. F. L., Hellier, C., Anderson, D. R., Pollacco, D., Gillon, M., Queloz, D., West, R. G., Bentley, S., Enoch, B., Haswell, C. A., Horne, K., Mayor, M., Pepe, F., Segransan, D., Skillen, I., Udry, S., Wheatley, P. J.
Publikováno v:
Hebb, L., et al. 2010, Astrophysical Journal, 708, 224
We report on the discovery of a new extremely short period transiting extrasolar planet, WASP-19b. The planet has mass Mpl = 1.15 \pm 0.08 MJ, radius Rpl = 1.31 \pm 0.06 RJ, and orbital period P = 0.7888399 \pm 0.0000008 days. Through spectroscopic a
Externí odkaz:
http://arxiv.org/abs/1001.0403