Zobrazeno 1 - 10
of 86
pro vyhledávání: '"Bukowiecki, Ł."'
Autor:
Maciejewski, G., Dimitrov, D., Fernández, M., Sota, A., Nowak, G., Ohlert, J., Nikolov, G., Bukowiecki, Ł., Hinse, T. C., Pallé, E., Tingley, B., Kjurkchieva, D., Lee, J. W., Lee, C. -U.
Publikováno v:
A&A 588, L6 (2016)
Most hot Jupiters are expected to spiral in towards their host stars due to transfering of the angular momentum of the orbital motion to the stellar spin. Their orbits can also precess due to planet-star interactions. Calculations show that both effe
Externí odkaz:
http://arxiv.org/abs/1602.09055
Autor:
Raetz, St., Maciejewski, G., Ginski, Ch., Mugrauer, M., Berndt, A., Eisenbeiss, T., Adam, Ch., Raetz, M., Roell, T., Seeliger, M., Marka, C., Vanko, M., Bukowiecki, L., Errmann, R., Kitze, M., Ohlert, J., Pribulla, T., Schmidt, J. G., Sebastian, D., Puchalski, D., Tetzlaff, N., Hohle, M. M., Schmidt, T. O. B., Neuhäuser, R.
Publikováno v:
Monthly Notices of the Royal Astronomical Society 2014 444 (4): 1351-1368
Homogeneous observations and careful analysis of transit light curves can lead to the identification of transit timing variations (TTVs). TrES-2 is one of few exoplanets, which offer the matchless possibility to combine long-term ground-based observa
Externí odkaz:
http://arxiv.org/abs/1408.7022
Autor:
Errmann, R., Torres, G., Schmidt, T. O. B., Seeliger, M., Howard, A. W., Maciejewski, G., Neuhäuser, R., Meibom, S., Kellerer, A., Dimitrov, D. P., Dincel, B., Marka, C., Mugrauer, M., Ginski, Ch., Adam, Ch., Raetz, St., Schmidt, J. G., Hohle, M. M., Berndt, A., Kitze, M., Trepl, L., Moualla, M., Eisenbeiß, T., Fiedler, S., Dathe, A., Graefe, Ch., Pawellek, N., Schreyer, K., Kjurkchieva, D. P., Radeva, V. S., Yotov, V., Chen, W. P., Hu, S. C. -L., Wu, Z. -Y., Zhou, X., Pribulla, T., Budaj, J., Vaňko, M., Kundra, E., Hambálek, Ľ., Krushevska, V., Bukowiecki, Ł., Nowak, G., Marschall, L., Terada, H., Tomono, D., Fernandez, M., Sota, A., Takahashi, H., Oasa, Y., Briceño, C., Chini, R., Broeg, C. H.
We report our investigation of the first transiting planet candidate from the YETI project in the young (~4 Myr old) open cluster Trumpler 37. The transit-like signal detected in the lightcurve of the F8V star 2M21385603+5711345 repeats every 1.36489
Externí odkaz:
http://arxiv.org/abs/1403.6020
Autor:
Errmann, R., Neuhäuser, R., Marschall, L., Torres, G., Mugrauer, M., Chen, W. P., Hu, S. C. -L., Briceno, C., Chini, R., Bukowiecki, Ł., Dimitrov, D. P., Kjurkchieva, D., Jensen, E. L. N., Cohen, D. H., Wu, Z. -Y., Pribulla, T., Vaňko, M., Krushevska, V., Budaj, J., Oasa, Y., Pandey, A. K., Fernandez, M., Kellerer, A., Marka, C.
With an apparent cluster diameter of 1.5{\deg} and an age of ~4 Myr, Trumpler 37 is an ideal target for photometric monitoring of young stars as well as for the search of planetary transits, eclipsing binaries and other sources of variability. The YE
Externí odkaz:
http://arxiv.org/abs/1305.4860
Autor:
Vanko, M., Maciejewski, G., Jakubik, M., Krejcova, T., Budaj, J., Pribulla, T., Ohlert, J., Raetz, St., Parimucha, S., Bukowiecki, L.
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 432, Issue 2, p.944-953 (2013)
We present new observations of the transiting system TrES-3 obtained from 2009 to 2011 at several observatories. The orbital parameters of the system were re- determined and a new linear ephemeris was calculated. The best quality light curve was used
Externí odkaz:
http://arxiv.org/abs/1303.4535
Autor:
Maciejewski, G., Dimitrov, D., Seeliger, M., Raetz, St., Bukowiecki, L., Kitze, M., Errmann, R., Nowak, G., Niedzielski, A., Popov, V., Marka, C., Gozdziewski, K., Neuhaeuser, R., Ohlert, J., Hinse, T. C., Lee, J. W., Lee, C. -U., Yoon, J. -N., Berndt, A., Gilbert, H., Ginski, Ch., Hohle, M. M., Mugrauer, M., Roell, T., Schmidt, T. O. B., Tetzlaff, N., Mancini, L., Southworth, J., Dall'Ora, M., Ciceri, S., Zambelli, R., Corfini, G., Takahashi, H., Tachihara, K., Benko, J. M., Sarneczky, K., Szabo, Gy. M., Varga, T. N., Vanko, M., Joshi, Y. C., Chen, W. P.
The transiting planet WASP-12 b was identified as a potential target for transit timing studies because a departure from a linear ephemeris was reported in the literature. Such deviations could be caused by an additional planet in the system. We atte
Externí odkaz:
http://arxiv.org/abs/1301.5976
This is a continuation of our study of open clusters based on the 2--Micron All Sky Survey photometry. Here we present the results of the mass function analysis for 599 known open clusters in the Milky Way. The main goal of this project is a study of
Externí odkaz:
http://arxiv.org/abs/1209.2832
Autor:
The YETI Collaboration, Chen, W. P., Hu, S. C. -L., Errmann, R., Adam, Ch., Baar, S., Berndt, A., Bukowiecki, L., Dimitrov, D. P., Eisenbeiß, T., Fiedler, S., Ginski, Ch., Gräfe, C., Guo, J. K., Hohle, M. M., Hsiao, H. Y., Janulis, R., Kitze, M., Lin, H. C., Lin, C. S., Maciejewski, G., Marka, C., Marschall, L., Moualla, M., Mugrauer, M., Neuhäuser, R., Pribulla, T., Raetz, St., Röll, T., Schmidt, E., Schmidt, J., Schmidt, T. O. B., Seeliger, M., Trepl, L., Briceño, C., Chini, R., Jensen, E. L. N., Nikogossian, E. H., Pandey, A. K., Sperauskas, J., Takahashi, H., Walter, F. M., Wu, Z. -Y., Zhou, X.
Publikováno v:
Astrophysical Journal, 751, 118 (2012)
GM Cep in the young (~4 Myr) open cluster Trumpler 37 has been known to be an abrupt variable and to have a circumstellar disk with very active accretion. Our monitoring observations in 2009-2011 revealed the star to show sporadic flare events, each
Externí odkaz:
http://arxiv.org/abs/1203.5271
The main goal of our project is to obtain a complete picture of individual open clusters from homogeneous data and then search for correlations between their astrophysical parameters. The near-infrared JHKS photometric data from the 2-Micron All Sky
Externí odkaz:
http://arxiv.org/abs/1107.5119
Autor:
Neuhäuser, R., Errmann, R., Berndt, A., Maciejewski, G., Takahashi, H., Chen, W. P., Dimitrov, D. P., Pribulla, T., Nikogossian, E. H., Jensen, E. L. N., Marschall, L., Wu, Z. -Y., Kellerer, A., Walter, F. M., Briceño, C., Chini, R., Fernandez, M., Raetz, St., Torres, G., Latham, D. W., Quinn, S. N., Niedzielski, A., Bukowiecki, Ł., Nowak, G., Tomov, T., Tachihara, K., Hu, S. C. -L., Hung, L. W., Kjurkchieva, D. P., Radeva, V. S., Mihov, B. M., Slavcheva-Mihova, L., Bozhinova, I. N., Budaj, J., Vaňko, M., Kundra, E., Hambálek, Ľ., Krushevska, V., Movsessian, T., Harutyunyan, H., Downes, J. J., Hernandez, J., Hoffmeister, V. H., Cohen, D. H., Abel, I., Ahmad, R., Chapman, S., Eckert, S., Goodman, J., Guerard, A., Kim, H. M., Koontharana, A., Sokol, J., Trinh, J., Wang, Y., Zhou, X., Redmer, R., Kramm, U., Nettelmann, N., Mugrauer, M., Schmidt, J., Moualla, M., Ginski, C., Marka, C., Adam, C., Seeliger, M., Baar, S., Roell, T., Schmidt, T. O. B., Trepl, L., Eisenbeiß, T., Fiedler, S., Tetzlaff, N., Schmidt, E., Hohle, M. M., Kitze, M., Chakrova, N., Gräfe, C., Schreyer, K., Hambaryan, V. V., Broeg, C. H., Koppenhoefer, J., Pandey, A. K.
We present the Young Exoplanet Transit Initiative (YETI), in which we use several 0.2 to 2.6m telescopes around the world to monitor continuously young (< 100 Myr), nearby (< 1 kpc) stellar clusters mainly to detect young transiting planets (and to s
Externí odkaz:
http://arxiv.org/abs/1106.4244