Zobrazeno 1 - 10
of 127
pro vyhledávání: '"Croll, B."'
Autor:
Xu, S., Rappaport, S., van Lieshout, R., Vanderburg, A., Gary, B., Hallakoun, N., Ivanov, V. D., Wyatt, M. C., DeVore, J., Bayliss, D., Bento, J., Bieryla, A., Cameron, A., Cann, J. M., Croll, B., Collins, K. A., Dalba, P. A., Debes, J., Doyle, D., Dufour, P., Ely, J., Espinoza, N., Joner, M. D., Jura, M., Kaye, T., McClain, J. L., Muirhead, P., Palle, E., Panka, P. A., Provencal, J., Randall, S., Rodriguez, J. E., Scarborough, J., Sefako, R., Shporer, A., Strickland, W., Zhou, G., Zuckerman, B.
White dwarf WD 1145+017 is orbited by several clouds of dust, possibly emanating from actively disintegrating bodies. These dust clouds reveal themselves through deep, broad, and evolving transits in the star's light curve. Here, we report two epochs
Externí odkaz:
http://arxiv.org/abs/1711.06960
We have obtained extensive photometric observations of the polluted white dwarf WD 1145+017 which has been reported to be transited by at least one, and perhaps several, large asteroids (or, planetesimals) with dust emission. We have carried out 53 o
Externí odkaz:
http://arxiv.org/abs/1602.00740
Autor:
Cowan, N. B., Machalek, P., Croll, B., Shekhtman, L. M., Burrows, A., Deming, D., Greene, T., Hora, J. L.
[Abridged] We report Warm Spitzer full-orbit phase observations of WASP-12b at 3.6 and 4.5 micron. We are able to measure the transit depths, eclipse depths, thermal and ellipsoidal phase variations at both wavelengths. The large amplitude phase vari
Externí odkaz:
http://arxiv.org/abs/1112.0574
Autor:
Steinbring, E., Carlberg, R., Croll, B., Fahlman, G., Hickson, P., Ivanescu, L., Leckie, B., Pfrommer, T., Schoeck, M.
Ellesmere Island, at the most northerly tip of Canada, possesses the highest mountain peaks within 10 degrees of the pole. The highest is 2616 m, with many summits over 1000 m, high enough to place them above a stable low-elevation thermal inversion
Externí odkaz:
http://arxiv.org/abs/1007.1680
Autor:
Huber, D., Matthews, J. M., Croll, B., Obbrugger, M., Gruberbauer, M., Guenther, D. B., Weiss, W. W., Rowe, J. F., Kallinger, T., Kuschnig, R., Scholtz, A. L., Moffat, A. F. J., Rucinski, S., Sasselov, D., Walker, G. A. H.
Context: Asteroseismology has great potential for the study of metal-poor stars due to its sensitivity to determine stellar ages. Aims: Our goal was to detect p-mode oscillations in the metal-poor sub-dwarf 85 Peg A and to search for other variabilit
Externí odkaz:
http://arxiv.org/abs/0907.1929
Autor:
Boisse, I., Moutou, C., Vidal-Madjar, A., Bouchy, F., Pont, F., Hébrard, G., Bonfils, X., Croll, B., Delfosse, X., Desort, M., Forveille, T., Lagrange, A. -M., Loeillet, B., Lovis, C., Matthews, J. M., Mayor, M., Pepe, F., Perrier, C., Queloz, D., Rowe, J. F., Santos, N. C., Ségransan, D., Udry, S.
Extra-solar planet search programs require high-precision velocity measurements. They need to study how to disentangle radial-velocity variations due to Doppler motion from the noise induced by stellar activity. We monitored the active K2V star HD 18
Externí odkaz:
http://arxiv.org/abs/0811.3923
Autor:
Miller-Ricci, E., Rowe, J. F., Sasselov, D., Matthews, J. M., Kuschnig, R., Croll, B., Guenther, D. B., Moffat, A. F. J, Rucinski, S. M., Walker, G. A. H., Weiss, W. W.
We have measured transit times for HD 189733b passing in front of its bright (V = 7.67) chromospherically active and spotted parent star. Nearly continuous broadband optical photometry of this system was obtained with the MOST (Microvariability & Osc
Externí odkaz:
http://arxiv.org/abs/0802.2722
Akademický článek
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Autor:
Xu, S, Rappaport, S, Van Lieshout, R, Vanderburg, A, Gary, B, Hallakoun, N, Ivanov, VD, Wyatt, MC, DeVore, J, Bayliss, D, Bento, J, Bieryla, A, Cameron, A, Cann, JM, Croll, B, Collins, KA, Dalba, PA, Debes, J, Doyle, D, Dufour, P, Ely, J, Espinoza, N, Joner, MD, Jura, M, Kaye, T, McClain, JL, Muirhead, P, Palle, E, Panka, PA, Provencal, J, Randall, S, Rodriguez, JE, Scarborough, J, Sefako, R, Shporer, A, Strickland, W, Zhou, G, Zuckerman, B
White dwarf WD 1145+017 is orbited by several clouds of dust, possibly emanating from actively disintegrating bodies. These dust clouds reveal themselves through deep, broad, and evolving transits in the star's light curve. Here, we report two epochs
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::890e4048d93aa0d1c71245232942de58
https://www.repository.cam.ac.uk/handle/1810/273196
https://www.repository.cam.ac.uk/handle/1810/273196
Akademický článek
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