Search Results - "Maciejewski, G."

A hot super-Earth planet in the WASP-84 planetary system by Maciejewski, G, Golonka, J, Łoboda, W, Ohlert, J, Fernández, M, Aceituno, F

“…ABSTRACT Hot Jupiters have been perceived as loners devoid of planetary companions in close orbital proximity. However, recent discoveries based on space-borne…”
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BD+15 2940 AND HD 233604: TWO GIANTS WITH PLANETS CLOSE TO THE ENGULFMENT ZONE by Nowak, G, Niedzielski, A, Wolszczan, A, Adamow, M, Maciejewski, G

“…We report the discovery of planetary-mass companions to two red giants by the ongoing Penn State-Torun Planet Search (PTPS) conducted with the 9.2 m…”
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Identifying birth places of young isolated neutron stars by Tetzlaff, N., Neuhäuser, R., Hohle, M. M., Maciejewski, G.

“…Young isolated radio-quiet neutron stars are still hot enough to be detectable at X-ray and optical wavelengths due to their thermal emission and can hence…”
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A Planetary-Mass Companion to the K0 Giant HD 17092 by Niedzielski, A, Konacki, M, Wolszczan, A, Nowak, G, Maciejewski, G, Gelino, C. R, Shao, M, Shetrone, M, Ramsey, L. W

“…We report the discovery of a substellar-mass companion to the K0 giant HD 17092 with the Hobby-Eberly Telescope. In the absence of any correlation of the…”
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WASP-14 b: transit timing analysis of 19 light curves by Raetz, St, Maciejewski, G., Seeliger, M., Marka, C., Fernández, M., Güver, T., Göğüş, E., Nowak, G., Vaňko, M., Berndt, A., Eisenbeiss, T., Mugrauer, M., Trepl, L., Gelszinnis, J.

“…Although WASP-14 b is one of the most massive and densest exoplanets on a tight and eccentric orbit, it has never been a target of photometric follow-up…”
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THREE RED GIANTS WITH SUBSTELLAR-MASS COMPANIONS by Niedzielski, A, Wolszczan, A, Nowak, G, Adamow, M, Kowalik, K, Maciejewski, G, Deka-Szymankiewicz, B, Adamczyk, M

“…We present three giant stars from the ongoing Penn State-Torun Planet Search with the Hobby-Eberly Telescope, which exhibit radial velocity (RV) variations…”
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YETI observations of the young transiting planet candidate CVSO 30 b by Raetz, St, Schmidt, T. O. B., Czesla, S., Klocová, T., Holmes, L., Errmann, R., Kitze, M., Fernández, M., Sota, A., Briceño, C., Hernández, J., Downes, J. J., Dimitrov, D. P., Kjurkchieva, D., Radeva, V., Wu, Z.-Y., Zhou, X., Takahashi, H., Henych, T., Seeliger, M., Mugrauer, M., Adam, Ch, Marka, C., Schmidt, J. G., Hohle, M. M., Ginski, Ch, Pribulla, T., Trepl, L., Moualla, M., Pawellek, N., Gelszinnis, J., Buder, S., Masda, S., Maciejewski, G., Neuhäuser, R.

“…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…”
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Interfacial energy and dissipation in martensitic phase transformations. Part II: Size effects in pseudoelasticity by Petryk, H., Stupkiewicz, S., Maciejewski, G.

“…This paper is a continuation of the Part I (H. Petryk, S. Stupkiewicz, Interfacial energy and dissipation in martensitic phase transformations. Part I: Theory…”
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Transit timing variation in exoplanet WASP-3b by Maciejewski, G., Dimitrov, D., Neuhäuser, R., Niedzielski, A., Raetz, St, Ginski, Ch, Adam, Ch, Marka, C., Moualla, M., Mugrauer, M.

“…Photometric follow-ups of transiting exoplanets may lead to discoveries of additional, less massive bodies in extrasolar systems. This is possible by detecting…”
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Substellar-mass Companions to the K-giants HD 240237, BD +48 738, and HD 96127 by Gettel, S, Wolszczan, A, Niedzielski, A, Nowak, G, Adamów, M, Zieliński, P, Maciejewski, G

“…We present the discovery of substellar-mass companions to three giant stars by the ongoing Penn State-Torun Planet Search conducted with the 9.2 m Hobby-Eberly…”
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Transit timing variation and activity in the WASP-10 planetary system by Maciejewski, G., Dimitrov, D., Neuhäuser, R., Tetzlaff, N., Niedzielski, A., Raetz, St, Chen, W. P., Walter, F., Marka, C., Baar, S., Krejcová, T., Budaj, J., Krushevska, V., Tachihara, K., Takahashi, H., Mugrauer, M.

“…Transit timing analysis may be an effective method of discovering additional bodies in extrasolar systems that harbour transiting exoplanets. The deviations…”
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Low-energy morphology of the interface layer between austenite and twinned martensite by Stupkiewicz, S., Maciejewski, G., Petryk, H.

“…A micromechanical scheme is developed for predicting the morphology and interfacial energy of the interface layer between the parent phase and internally…”
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Transit timing of TrES-2: a combined analysis of ground- and space-based photometry by Raetz, St, Maciejewski, G., Ginski, Ch, Mugrauer, M., Berndt, A., Eisenbeiss, T., Adam, Ch, Raetz, M., Roell, T., Seeliger, M., Marka, C., Vaňko, M., Bukowiecki, Ł., 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.

“…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…”
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PLANETS AROUND THE K-GIANTS BD+20 274 AND HD 219415 by Gettel, S, Wolszczan, A, Niedzielski, A, Nowak, G, Adamow, M, Zielinski, P, Maciejewski, G

“…We present the discovery of planet-mass companions to two giant stars by the ongoing Penn State-Torun Planet Search conducted with the 9.2 m Hobby-Eberly…”
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Transit timing analysis in the HAT-P-32 system by Seeliger, M., Dimitrov, D., Kjurkchieva, D., Mallonn, M., Fernandez, M., Kitze, M., Casanova, V., Maciejewski, G., Ohlert, J. M., Schmidt, J. G., Pannicke, A., Puchalski, D., Göğüş, E., Güver, T., Bilir, S., Ak, T., Hohle, M. M., Schmidt, T. O. B., Errmann, R., Jensen, E., Cohen, D., Marschall, L., Saral, G., Bernt, I., Derman, E., Gałan, C., Neuhäuser, R.

“…We present the results of 45 transit observations obtained for the transiting exoplanet HAT-P-32b. The transits have been observed using several telescopes…”
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Photometric follow-up of the transiting planetary system TrES-3: transit timing variation and long-term stability of the system by Va ko, M., Maciejewski, G., Jakubík, M., Krej ová, T., Budaj, J., Pribulla, T., Ohlert, J., Raetz, St, Parimucha, Š., Bukowiecki, L.

“…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…”
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A transit timing analysis with combined ground- and space-based photometry by Raetz, St, Fernandez, M, Marka, C, Heras, A M, Maciejewski, G

“…The analysis of timing variations of transiting exoplanets allows one to discover additional planets in the system. Such bodies can be very low in mass and…”
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Investigation of a transiting planet candidate in Trumpler 37: An astro-physical false positive eclipsing spectroscopic binary star by 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., Hambälek, 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…”
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X-ray diffraction micro-imaging of strain in laterally overgrown GaAs layers. Part I: analysis of a single GaAs stripe by Czyzak, A., Domagala, J.Z., Maciejewski, G., Zytkiewicz, Z.R.

“…Spatially resolved X-ray diffraction (SRXRD) is used for micro-imaging of strain in GaAs:Si layers grown by liquid phase epitaxial lateral overgrowth (ELO) on…”
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Piezoelectric field around threading dislocation in GaN determined on the basis of high‐resolution transmission electron microscopy image by MACIEJEWSKI, G., KRET, S., RUTERANA, P.

“…Summary A new method of determining the piezoelectric field around dislocations from high‐resolution transmission electron microscopy images is presented. In…”
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