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pro vyhledávání: '"Kaye T"'
Autor:
Rappaport, S. A., Borkovits, T., Gagliano, R., Jacobs, T. L., Kostov, V. B., Powell, B. P., Terentev, I., Omohundro, M., Torres, G., Vanderburg, A., Mitnyan, T., Kristiansen, M. H., LaCourse, D., Schwengeler, H. M., Kaye, T. G., Pál, A., Pribulla, T., Bíró, I. B., Csányi, I., Garai, Z., Zasche, P., Maxted, P. F. L., Rodriguez, J. E., Stevens, D. J.
In this work we report the discovery and analysis of six new compact triply eclipsing triple star systems found with the TESS mission: TICs 37743815, 42565581, 54060695, 178010808, 242132789, and 456194776. All of these exhibit distinct third body ec
Externí odkaz:
http://arxiv.org/abs/2204.02539
Autor:
Borkovits, T., Mitnyan, T., Rappaport, S. A., Pribulla, T., Powell, B. P., Kostov, V. B., Bíró, I. B., Csányi, I., Garai, Z., Gary, B. L., Kaye, T. G., Komžík, R., Terentev, I., Omohundro, M., Gagliano, R., Jacobs, T., Kristiansen, M. H., LaCourse, D., Schwengeler, H. M., Czavalinga, D., Seli, B., Huang, C. X., Pál, A., Vanderburg, A., Rodriguez, J. E., Stevens, D. J.
In this work we report the discovery and analysis of three new triply eclipsing triple star systems found with the TESS mission during its observations of the northern skies: TICs 193993801, 388459317, and 52041148. We utilized the TESS precision pho
Externí odkaz:
http://arxiv.org/abs/2111.10074
Autor:
Borkovits, T., Rappaport, S. A., Tan, T. G., Gagliano, R., Jacobs, T., Huang, X., Mitnyan, T., Hambsch, F. -J., Kaye, T., Maxted, P. F. L., Pál, A., Schmitt, A. R.
We report the discovery in $TESS$ Sectors 3 and 4 of a compact triply eclipsing triple star system. TIC 209409435 is a previously unknown eclipsing binary with a period of 5.717 days, and the presence of a third star in an outer eccentric orbit of 12
Externí odkaz:
http://arxiv.org/abs/2006.10449
Akademický článek
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Autor:
Borkovits, T., Rappaport, S., Kaye, T., Isaacson, H., Vanderburg, A., Howard, A. W., Kristiansen, M. H., Omohundro, M. R., Schwengeler, H. M., Terentev, I. A., Shporer, A., Relles, H., Villanueva Jr., S., Tan, T. G., Colón, K. D., Blex, J., Haas, M., Cochran, W., Endl, M.
Using Campaign 15 data from the K2 mission, we have discovered a triply-eclipsing triple star system: EPIC 249432662. The inner eclipsing binary system has a period of 8.23 days, with shallow $\sim$3% eclipses. During the entire 80-day campaign, ther
Externí odkaz:
http://arxiv.org/abs/1809.04366
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
Autor:
Rappaport, S., Vanderburg, A., Nelson, L., Gary, B. L., Kaye, T. G., Kalomeni, B., Howell, S. B., Thorstensen, J. R., Lachapelle, F. -R., Lundy, M., St-Antoine, J.
Among the 28,000 targeted stars in K2 Field 10 is the white dwarf WD 1202-024 (EPIC 201283111), first noted in the SDSS survey (SDSS 120515.80-024222.7). We have found that this hot white dwarf (Teff = 22,640 K) is in a very close orbit (P = 71 min)
Externí odkaz:
http://arxiv.org/abs/1705.05863
Akademický článek
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WD 1145+017 was observed from 2015 November to 2016 July for the purpose of characterizing transit behavior of the white dwarf by dust clouds thought to be produced by fragments of an asteroid in close orbit with the star. Fortuitously, most of these
Externí odkaz:
http://arxiv.org/abs/1608.00026
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