Zobrazeno 1 - 10
of 77
pro vyhledávání: '"Borczyk, W."'
Autor:
Hanuš, J., Ďurech, J., Brož, M., Marciniak, A., Warner, B. D., Pilcher, F., Stephens, R., Behrend, R., Carry, B., Čapek, D., Antonini, P., Audejean, M., Augustesen, K., Barbotin, E., Baudouin, P., Bayol, A., Bernasconi, L., Borczyk, W., Bosch, J. -G., Brochard, E., Brunetto, L., Casulli, S., Cazenave, A., Charbonnel, S., Christophe, B., Colas, F., Coloma, J., Conjat, M., Cooney, W., Correira, H., Cotrez, V., Coupier, A., Crippa, R., Cristofanelli, M., Dalmas, Ch., Danavaro, C., Demeautis, C., Droege, T., Durkee, R., Esseiva, N., Esteban, M., Fagas, M., Farroni, G., Fauvaud, M., Fauvaud, S., Del Freo, F., Garcia, L., Geier, S., Godon, C., Grangeon, K., Hamanowa, H., Heck, N., Hellmich, S., Higgins, D., Hirsch, R., Husarik, M., Itkonen, T., Jade, O., Kamiński, K., Kankiewicz, P., Klotz, A., Koff, R. A., Kryszczyńska, A., Kwiatkowski, T., Laffont, A., Leroy, A., Lecacheux, J., Leonie, Y., Leyrat, C., Manzini, F., Martin, A., Masi, G., Matter, D., Michałowski, J., Michałowski, M. J., Michałowski, T., Michelet, J., Michelsen, R., Morelle, E., Mottola, S., Naves, R., Nomen, J., Oey, J., Ogloza, W., Oksanen, A., Oszkiewicz, D., Pääkkönen, P., Paiella, M., Pallares, H., Paulo, J., Pavic, M., Payet, B., Polińska, M., Polishook, D., Poncy, R., Revaz, Y., Rinner, C., Rocca, M., Roche, A., Romeuf, D., Roy, R., Saguin, H., Salom, P. A., Sanchez, S., Santacana, G., Santana-Ros, T., Sareyan, J. -P., Sobkowiak, K., Sposetti, S., Starkey, D., Stoss, R., Strajnic, J., Teng, J. -P., Tregon, B., Vagnozzi, A., Velichko, F. P., Waelchli, N., Wagrez, K., Wücher, H.
The larger number of models of asteroid shapes and their rotational states derived by the lightcurve inversion give us better insight into both the nature of individual objects and the whole asteroid population. With a larger statistical sample we ca
Externí odkaz:
http://arxiv.org/abs/1301.6943
Autor:
Ratajczak, M., Kwiatkowski, T., Schwarzenberg-Czerny, A., Dimitrov, W., Konacki, M., Helminiak, K. G., Bartczak, P., Fagas, M., Kaminski, K., Kankiewicz, P., Borczyk, W., Rozek, A.
First spectroscopic and new photometric observations of the eclipsing binary FM Leo are presented. The main aims were to determine orbital and stellar parameters of two components and their evolutionary stage. First spectroscopic observations of the
Externí odkaz:
http://arxiv.org/abs/0911.0554
Autor:
Baranowski, R., Smolec, R., Dimitrov, W., Kwiatkowski, T., Schwarzenberg-Czerny, A., Bartczak, P., Fagas, M., Borczyk, W., Kaminski, K., Moskalik, P., Ratajczak, R., Rozek, A.
Publikováno v:
Mon.Not.Roy.Astron.Soc.396:2194-2200, 2009
V440 Per is a Population I Cepheid with the period of 7.57 day and low amplitude, almost sinusoidal light and radial velocity curves. With no reliable data on the 1st harmonic, its pulsation mode identification remained controversial. We obtained a r
Externí odkaz:
http://arxiv.org/abs/0904.0600
Autor:
Garcet, O., Gandhi, P., Gosset, E., Sprimont, P. G., Surdej, J., Borkowski, V., Tajer, M., Pacaud, F., Pierre, M., Chiappetti, L., Maccagni, D., Page, M. J., Carrera, F. J., Tedds, J. A., Mateos, S., Krumpe, M., Contini, T., Corral, A., Ebrero, J., Gavignaud, I., Schwope, A., Fevre, O. Le, Polletta, M., Rosen, S., Lonsdale, C., Watson, M., Borczyk, W., Vaisanen, P.
Publikováno v:
Astron.Astrophys.474:473-489,2007
Our goal is to characterize AGN populations by comparing their X-ray and optical classifications. We present a sample of 99 spectroscopically identified X-ray point sources in the XMM-LSS survey which are significantly detected in the [2-10] keV band
Externí odkaz:
http://arxiv.org/abs/0709.2077
Publikováno v:
In Chaos, Solitons and Fractals 2009 40(4):1697-1714
Autor:
Kryszczyńska, A., Colas, F., Polińska, M., Hirsch, R., Ivanova, V., Apostolovska, G., Bilkina, B., Velichko, F., Kwiatkowski, T., Kankiewicz, P., Vachier, F., Umlenski, V., Michałowski, T., Marciniak, A., Maury, A., Kamiński, K., Fagas, M., Dimitrov, W., Borczyk, W., Sobkowiak, K., Lecacheux, J., Behrend, R., Klotz, A., Bernasconi, L., Crippa, R., Manzini, F., Poncy, R., Antonini, P., Oszkiewicz, D., Santana-Ros, T.
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2012, 546, pp.A72. ⟨10.1051/0004-6361/201219199⟩
Astronomy and Astrophysics-A&A, 2012, 546, pp.A72. ⟨10.1051/0004-6361/201219199⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2012, 546, pp.A72. ⟨10.1051/0004-6361/201219199⟩
Astronomy and Astrophysics-A&A, 2012, 546, pp.A72. ⟨10.1051/0004-6361/201219199⟩
International audience; Context. Recent studies have uncovered evidence that the statistical properties of asteroids' physical parameters are a fundamental source of information on the physics of their collisions and evolution. The analysis of the sp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::eb15ce17d9b4edd98b9917c0a9f80d3c
https://hal.archives-ouvertes.fr/hal-03123875/file/aa19199-12.pdf
https://hal.archives-ouvertes.fr/hal-03123875/file/aa19199-12.pdf
Autor:
Kryszczynska, A., Colas, F., Polinska, M., Hirsch, R., Ivanova, V., Apostolovska, G., Bilkina, B., Velichko, F. P., Kwiatkowski, T., Kankiewicz, P., Vachier, F., Umlenski, V., Michalowski, T., Marciniak, A., Maury, A., Kaminski, K., Fagas, M., Dimitrov, W., Borczyk, W., Sobkowiak, K., Lecacheux, J., Behrend, R., Klotz, A., Bernasconi, L., Crippa, R., Manzini, F., Poncy, R., Antonini, P., Oszkiewicz, D., Santana-Ros, T.
The files contain asteroid brightness, aspect data and observing information for corresponding date. These files were used for obtaining synodic period rotation. Individual lightcurves within a files are identified with a light curve number, all ligh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______166::fc94baf3c72acc1859632f2d349ffe9d
https://hal-obspm.ccsd.cnrs.fr/obspm-03933647
https://hal-obspm.ccsd.cnrs.fr/obspm-03933647
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Akademický článek
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