Zobrazeno 1 - 10
of 25
pro vyhledávání: '"M. Kitze"'
Autor:
D. J. Fritzewski, J. Greif, M. Kitze, B. Dincel, Ch. Adam, H. F. W. Gilbert, Ch. Ginski, St. Raetz, Ronny Errmann, W. P. Chen, T. O. B. Schmidt, Ralph Neuhäuser, A. Pannicke, Sven Buder, Timothy Butterley, P. C. Huang, Theodor Pribulla, Richard Wilson, C. Marka, V. Wolf, M. Seeliger, M. Mallonn, L. K. Hardy, J. G. Schmidt, Jesús Hernández, Aglae Kellerer, Z. Garai, S. P. Littlefair, Cesar Briceno, V. S. Dhillon, Markus Mugrauer, Emil Kundra
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 462:2396-2417
We present long-term photometric observations of the young open cluster IC 348 with a baseline time-scale of 2.4 yr. Our study was conducted with several telescopes from the Young Exoplanet Transit Initiative (YETI) network in the Bessel R band to fi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e3e58a53ad9b32d5625fbea65d125162
https://doi.org/10.1093/mnras/stw1797
https://doi.org/10.1093/mnras/stw1797
Autor:
Timothy Butterley, Ralph Neuhäuser, Richard Wilson, Martin Vaňko, S. Buder, R. Errmann, Z. Garai, T. O. B. Schmidt, Theodor Pribulla, Ľ. Hambálek, M. Seeliger, B. Dincel, S. P. Littlefair, V. S. Dhillon, A. Pannicke, Ch. Adam, Emil Kundra, J. G. Schmidt, Markus Mugrauer, H. Gilbert, St. Raetz, Ch. Ginski, M. Kitze, Aglae Kellerer, L. K. Hardy, J. Nedoroščík
Publikováno v:
Astronomische Nachrichten = Astronomical notes
We report results of the first five observing campaigns for the open stellar cluster NGC 7243 in the frame of project Young Exoplanet Transit Initiative (YETI). The project focuses on the monitoring of young and nearby stellar clusters, with the aim
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::80f4250ba1803e809549445aeb519665
https://doi.org/10.1002/asna.201512310
https://doi.org/10.1002/asna.201512310
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 442:3769-3776
An investigation of the G-type stellar population with Kepler (as done by Maehara et al.) shows that less than 1 per cent of those stars show superflares. Due to the large pixel scale of Kepler ($\sim4 arcsec \: px^{-1}$), it is still not clear wheth
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::815f2add9489819410aeba135dc8238b
https://doi.org/10.1093/mnras/stu1114
https://doi.org/10.1093/mnras/stu1114
Autor:
J. G. Schmidt, N. Pawellek, Ł. Bukowiecki, M. M. Hohle, Markus Mugrauer, V. Krushevska, S. Meibom, Ronny Errmann, D. Tomono, Ľ. Hambálek, V. Yotov, B. Dincel, H. Takahashi, V. S. Radeva, Hiroshi Terada, Andrew W. Howard, Katharina Schreyer, Ch. Graefe, Grzegorz Nowak, Gracjan Maciejewski, Guillermo Torres, Ch. Adam, Martin Vaňko, Laurence A. Marschall, Yumiko Oasa, L. Trepl, Ch. Ginski, T. Eisenbeiß, X. Zhou, Dinko Dimitrov, T. O. B. Schmidt, C. Marka, Emil Kundra, S.C.-L. Hu, A. Dathe, J. Budaj, T. Pribulla, St. Raetz, Cesar Briceno, C. Broeg, Wen Ping Chen, Alfredo Sota, A. Berndt, M. Kitze, Aglae Kellerer, Zhenyu Wu, M. Fernandez, Ralph Neuhäuser, R. Chini, Diana P. Kjurkchieva, M. Moualla, M. Seeliger, S. Fiedler
Publikováno v:
Astronomische Nachrichten. 335:345-356
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:
https://explore.openaire.eu/search/publication?articleId=doi_________::af646d0231398a46e5d5a3fff10be32f
https://doi.org/10.1002/asna.201412047
https://doi.org/10.1002/asna.201412047
Autor:
Tomáš Henych, Dinko Dimitrov, Ronny Errmann, Theodor Pribulla, M. Moualla, Ch. Adam, J. J. Downes, M. Seeliger, J. Gelszinnis, Jesús Hernández, Sven Buder, J. G. Schmidt, M. Kitze, L. Holmes, Ch. Ginski, T. Klocová, Xin Zhou, S. Czesla, V. S. Radeva, Hiromitsu Takahashi, Zhenyu Wu, Ralph Neuhäuser, Markus Mugrauer, M. Fernandez, M. M. Hohle, Alfredo Sota, N. Pawellek, T. O. B. Schmidt, C. Marka, S. Masda, St. Raetz, Cesar Briceno, Gracjan Maciejewski, L. Trepl, Diana P. Kjurkchieva
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 460(3), 2834-2852
instname
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 460(3), 2834-2852
Raetz, St. et. al.
CVSO 30 is a unique young low-mass system, because, for the first time, a close-in transiting and a wide directly imaged planet candidates are found around a common host star. The inner companion, CVSO 30 b, is the first possi
CVSO 30 is a unique young low-mass system, because, for the first time, a close-in transiting and a wide directly imaged planet candidates are found around a common host star. The inner companion, CVSO 30 b, is the first possi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fe5fcea8ccae50ca71167d5e037e8b33
Autor:
F. J. Aceituno, Diana P. Kjurkchieva, Martin Vaňko, T. O. B. Schmidt, A. Özdönmez, S. Buder, M. Haas, J. K. Guo, Ch. Adam, K. Werner, E. Güzel, Tansel Ak, A. Pannicke, M. Hackstein, Laurence A. Marschall, J. G. Schmidt, Rolf Chini, Markus Mugrauer, M. Kitze, C. Marka, Tolga Guver, Theodor Pribulla, A. Dathe, Wen Ping Chen, J. Budaj, V. Wolf, Xin Zhou, David H. Cohen, Eric L. N. Jensen, Ronny Errmann, S. Hellmich, M. Seeliger, Ralph Neuhäuser, Ersin Gogus, S. Richter, Ch. Ginski, D. Puchalski, A. Ide, Berk Aydin, J. M. Ohlert, Dinko Dimitrov, J. Greif, Raetz, Emil Kundra, Zhenyu Wu, M. Fernandez, Stefano Mottola, Matthias Mallonn, B. Dincel
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 451(4), 4060-4072
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society
As part of our ongoing effort to investigate transit timing variations (TTVs) of known exoplanets, we monitored transits of the four exoplanets HAT-P-18b, HAT-P-19b, HAT-P-27b/WASP-40b and WASP-21b. All of them are suspected to show TTVs due to the k
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::229fa7f0599df40b976874d866fb96b8
http://hdl.handle.net/1887/49339
http://hdl.handle.net/1887/49339
Autor:
M. M. Hohle, T. O. B. Schmidt, Selçuk Bilir, J. M. Ohlert, G. Saral, Ralph Neuhäuser, Dinko Dimitrov, I. Bernt, D. Puchalski, V. Casanova, Diana P. Kjurkchieva, Matthias Mallonn, Ersin Gogus, Ronny Errmann, M. Fernandez, M. Seeliger, Laurence A. Marschall, Tolga Guver, Eric L. N. Jensen, Gracjan Maciejewski, Tansel Ak, A. Pannicke, David H. Cohen, Cezary Galan, M. Kitze, E. Derman, J. G. Schmidt
We present the results of 45 transit observations obtained for the transiting exoplanet HAT-P-32b. The transits have been observed using several telescopes mainly throughout the YETI network. In 25 cases, complete transit light curves with a timing p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c15723463a51cdc7d83f1c1b5ad8857e
Autor:
Theodor Pribulla, Martin Vaňko, Gracjan Maciejewski, Ł. Bukowiecki, St. Raetz, M. Kitze, Ch. Adam, Markus Mugrauer, J. G. Schmidt, T. O. B. Schmidt, T. Eisenbeiss, C. Marka, Ralph Neuhäuser, N. Tetzlaff, M. Raetz, M. M. Hohle, M. Seeliger, A. Berndt, J. M. Ohlert, Daniel Sebastian, D. Puchalski, T. Roell, Ch. Ginski, Ronny Errmann
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8e0be59d57faf84fb0259cede4292f5f
Autor:
Ralph Neuhäuser, J. G. Schmidt, J. M. Ohlert, Gracjan Maciejewski, M. Fernandez, F. J. Aceituno, Dinko Dimitrov, M. Seeliger, A. Pannicke, H. Gilbert, M. Kitze, D. Puchalski, St. Raetz, Ronny Errmann
Publikováno v:
Astronomy & Astrophysics. 577:A109
The transiting hot Jupiter planet Qatar-1 b was presented to exhibit variations in transit times that could be of perturbative nature. A hot Jupiter with a planetary companion on a nearby orbit would constitute an unprecedented planetary configuratio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0f8423ad433d089a6de251c81003f4d1
https://doi.org/10.1051/0004-6361/201526031
https://doi.org/10.1051/0004-6361/201526031
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