Search Results - "Baluďansky, D."

VW LMi: tightest quadruple system known. Light-time effect and possible secular changes of orbits by Pribulla, T., Baluďanský, D., Dubovský, P., Kudzej, I., Parimucha, Š., Siwak, M., Vaňko, M.

“…Tightest known quadruple system VW LMi consists of contact eclipsing binary with P12= 0.477 551 d and detached binary with P34= 7.930 63 d revolving in rather…”
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The Dwarf project: Eclipsing binaries - precise clocks to discover exoplanets by Pribulla, T., Vaňko, M., Ammler-von Eiff, M., Andreev, M., Aslantürk, A., Awadalla, N., Baluďansky, D., Bonanno, A., Božić, H., Catanzaro, G., Çelik, L., Christopoulou, P.E., Covino, E., Cusano, F., Dimitrov, D., Dubovský, P., Eigmueller, P., Esmer, E.M., Frasca, A., Hambálek, Ľ., Hanna, M., Hanslmeier, A., Kalomeni, B., Kjurkchieva, D.P., Krushevska, V., Kudzej, I., Kundra, E., Kuznyetsova, Yu, Lee, J.W., Leitzinger, M., Maciejewski, G., Moldovan, D., Morais, M.H.M., Mugrauer, M., Neuhäuser, R., Niedzielski, A., Odert, P., Ohlert, J., Özavcı, İ., Papageorgiou, A., Parimucha, Š., Poddaný, S., Pop, A., Raetz, M., Raetz, S., Romanyuk, Ya, Ruždjak, D., Schulz, J., Şenavcı, H.V., Srdoc, G., Szalai, T., Székely, P., Sudar, D., Tezcan, C.T., Törün, M.E., Turcu, V., Vince, O., Zejda, M.

“…We present a new observational campaign, Dwarf, aimed at detection of circumbinary extrasolar planets using the timing of the minima of low‐mass eclipsing…”
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KOROAPS - SYSTEM FOR A LARGE SCALE MONITORING AND VARIABLE STARS SEARCHING by S. Parimucha, D. Baludansky, M. Vadila

“…We give an introduction information about the KOROAPS (KOsice ROztoky Automatic Photometry System). It is a system for a large scale automatic multicolor…”
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Ccd Photometry of the Neglected Contact Binaries V344 Lac and V1191 Cyg by Pribulla, Theodor, Vanko, Martin, Chochol, DrahomIr, Parimucha, tefan, Baludansky, Daniel

“…New photoelectric and CCD observations of the eclipsing contact binary systems V344 Lac and V1191 Cyg are presented and analyzed. All available times of…”
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VW LMi: tightest quadruple system known. Light-time effect and possible secular changes of orbits by Pribulla, T, Baludansky, D, Dubovsky, P, Kudzej, I, Parimucha, S, Siwak, M, Vanko, M

“…Tightest known quadruple systems VW LMi consists of contact eclipsing binary with P_12 = 0.477551 days and detached binary with P_34 = 7.93063 days revolving…”
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The DWARF project: Eclipsing binaries - precise clocks to discover exoplanets by Pribulla, T, Vaňko, M, von Eiff, M. Ammler, Andreev, M, Aslantürk, A, Awadalla, N, Baluďanský, D, Bonanno, A, Božić, H, Catanzaro, G, Çelik, L, Christopoulou, P. E, Covino, E, Cusano, F, Dimitrov, D, Dubovský, P, Esmer, E. M, Frasca, A, Hambálek, Ľ, Hanna, M, Hanslmeier, A, Kalomeni, B, Kjurkchieva, D. P, Krushevska, V, Kudzej, I, Kundra, E, Kuznyetsova, Yu, Lee, J. W, Leitzinger, M, Maciejewski, G, Moldovan, D, Morais, M. H. M, Mugrauer, M, Neuhäuser, R, Niedzielski, A, Odert, P, Ohlert, J, Özavcı, İ, Papageorgiou, A, Parimucha, Š, Poddaný, S, Pop, A, Raetz, M, Raetz, S, Romanyuk, Ya, Ruždjak, D, Schulz, J, Şenavcı, H. V, Szalai, T, Székely, P, Sudar, D, Tezcan, C. T, Törün, M. E, Turcu, V, Vince, O, Zejda, M

“…We present a new observational campaign, DWARF, aimed at detection of circumbinary extrasolar planets using the timing of the minima of low-mass eclipsing…”
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