Zobrazeno 1 - 10
of 315
pro vyhledávání: '"Ryans, P."'
Autor:
McCormac, James, Pollacco, Don, Wheatley, Peter, West, Richard, Walker, Simon, Bento, Joao, Skillen, Ian, Faedi, Francesca, Burleigh, Matt, Casewell, Sarah, Chazelas, Bruno, Genolet, Ludovic, Gibson, Neale, Goad, Mike, Lawrie, Katherine, Ryans, Robert, Todd, Ian, Udry, Stephan, Watson, Christopher
We present the prototype telescope for the Next Generation Transit Survey, which was built in the UK in 2008/09 and tested on La Palma in the Canary Islands in 2010. The goals for the prototype system were severalfold: to determine the level of syste
Externí odkaz:
http://arxiv.org/abs/1611.00691
Autor:
Jess, D. B., Reznikova, V. E., Ryans, R. S. I., Christian, D. J., Keys, P. H., Mathioudakis, M., Mackay, D. H., Prasad, S. Krishna, Banerjee, D., Grant, S. D. T., Yau, S., Diamond, C.
Publikováno v:
Nature Physics, 12, 179 (2016)
Sunspots on the surface of the Sun are the observational signatures of intense manifestations of tightly packed magnetic field lines, with near-vertical field strengths exceeding 6,000 G in extreme cases. It is well accepted that both the plasma dens
Externí odkaz:
http://arxiv.org/abs/1605.06112
Publikováno v:
Rehabilitation Oncology; Jul2024, Vol. 42 Issue 3, p138-145, 8p
Akademický článek
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Autor:
von Prochazka, Azrael A., Remijan, Anthony J., Balser, Dana S., Ryans, Robert S. I., Marshall, Adele H., Schwab, Fredric R., Hollis, Jan M., Jewell, Philip R., Lovas, Frank J.
We report the detection of Voigt spectral line profiles of radio recombination lines (RRLs) toward Sagittarius B2(N) with the 100-m Green Bank Telescope (GBT). At radio wavelengths, astronomical spectra are highly populated with RRLs, which serve as
Externí odkaz:
http://arxiv.org/abs/1002.3799
High resolution optical spectra of 57 Galactic B-type supergiant stars have been analyzed to determine their rotational and macroturbulent velocities. In addition, their atmospheric parameters (effective temperature, surface gravity and microturbulen
Externí odkaz:
http://arxiv.org/abs/1001.3337
Autor:
Jess, D. B., Mathioudakis, M., Christian, D. J., Keenan, F. P., Ryans, R. S. I., Crockett, P. J.
Rapid Oscillations in the Solar Atmosphere (ROSA) is a synchronized, six camera high cadence solar imaging instrument developed by Queen's University Belfast. The system is available on the Dunn Solar Telescope at the National Solar Observatory in Su
Externí odkaz:
http://arxiv.org/abs/0912.4118
Autor:
Lister, T. A., Anderson, D. R., Gillon, M., Hebb, L., Smalley, B. S., Triaud, A. H. M. J., Cameron, A. Collier, Wilson, D. M., West, R. G., Bentley, S. J., Christian, D. J., Enoch, R., Haswell, C. A., Hellier, C., Horne, K., Irwin, J., Joshi, Y. C., Kane, S. R., Mayor, M., Maxted, P. F. L., Norton, A. J., Parley, N., Pepe, F., Pollacco, D., Queloz, D., Ryans, R., Segransan, D., Skillen, I., Street, R. A., Todd, I., Udry, S., Wheatley, P. J.
We report the discovery from WASP-South of a new Jupiter-like extrasolar planet, WASP-16b, which transits its solar analog host star every 3.12 days. Analysis of the transit photometry and radial velocity spectroscopic data leads to a planet with R_p
Externí odkaz:
http://arxiv.org/abs/0908.0297
Autor:
Cameron, A. Collier, Davidson, V. A., Hebb, L., Skinner, G., Anderson, D. R., Christian, D. J., Clarkson, W. I., Enoch, B., Irwin, J., Joshi, Y., Haswell, C. A., Hellier, C., Horne, K. D., Kane, S. R., Lister, T. A., Maxted, P. F. L., Norton, A. J., Parley, N., Pollacco, D., Ryans, R., Scholz, A., Skillen, I., Smalley, B., Street, R. A., West, R. G., Wilson, D. M., Wheatley, P. J.
We present the results of a photometric survey of rotation rates in the Coma Berenices (Melotte 111) open cluster, using data obtained as part of the SuperWASP exoplanetary transit-search programme. The goal of the Coma survey was to measure precise
Externí odkaz:
http://arxiv.org/abs/0908.0189
Autor:
Skillen, I., Pollacco, D., Cameron, A. Collier, Hebb, L., Simpson, E., Bouchy, F., Christian, D. J., Gibson, N. P., Hébrard, G., Joshi, Y. C., Loeillet, B., Smalley, B., Stempels, H. C., Street, R. A., Udry, S., West, R. G., Anderson, D. R., Barros, S. C. C., Enoch, B., Haswell, C. A., Hellier, C., Horne, K., Irwin, J., Keenan, F. P., Lister, T. A., Maxted, P., Mayor, M., Moutou, C., Norton, A. J., Parley, N., Queloz, D., Ryans, R., Todd, I., Wheatley, P. J., Wilson, D. M.
We report the discovery of WASP-13b, a low-mass $ M_p = 0.46 ^{+ 0.06}_{- 0.05} M_J$ transiting exoplanet with an orbital period of $4.35298 \pm 0.00004$ days. The transit has a depth of 9 mmag, and although our follow-up photometry does not allow us
Externí odkaz:
http://arxiv.org/abs/0905.3115