Zobrazeno 1 - 10
of 93
pro vyhledávání: '"Godunova, V"'
Autor:
Howil, K., Wyrzykowski, Ł., Kruszyńska, K., Zieliński, P., Bachelet, E., Gromadzki, M., Mikołajczyk, P. J., Kotysz, K., Jabłońska, M., Kaczmarek, Z., Mróz, P., Ihanec, N., Ratajczak, M., Pylypenko, U., Rybicki, K., Sweeney, D., Hodgkin, S. T., Larma, M., Carrasco, J. M., Burgaz, U., Godunova, V., Simon, A., Cusano, F., Jelinek, M., Štrobl, J., Hudec, R., Merc, J., Kučáková, H., Erece, O., Kilic, Y., Olivares, F., Morrell, M., Wicker, M.
Identifying black holes is essential for comprehending the development of stars and uncovering novel principles of physics. Gravitational microlensing provides an exceptional opportunity to examine an undetectable population of black holes in the Mil
Externí odkaz:
http://arxiv.org/abs/2403.09006
Autor:
Maskoliūnas, M., Wyrzykowski, Ł., Howil, K., Rybicki, K. A., Zieliński, P., Kaczmarek, Z., Kruszyńska, K., Jabłońska, M., Zdanavičius, J., Pakštienė, E., Čepas, V., Mikołajczyk, P. J., Janulis, R., Gromadzki, M., Ihanec, N., Adomavičienė, R., Šiškauskaitė, K., Bronikowski, M., Sivak, P., Stankevičiūtė, A., Sitek, M., Ratajczak, M., Pylypenko, U., Gezer, I., Awiphan, S., Bachelet, E., Bąkowska, K., Boyle, R. P., Bozza, V., Brincat, S. M., Burgaz, U., Butterley, T., Carrasco, J. M., Cassan, A., Cusano, F., Damljanovic, G., Davidson, J. W., Dhillon, V. S., Dominik, M., Dubois, F., Esenoglu, H. H., Jaimes, R. Figuera, Fukui, A., Galdies, C., Garofalo, A., Godunova, V., Güver, T., Heidt, J., Hundertmark, M., Izviekova, I., Joachimczyk, B., Kamińska, M. K., Kamiński, K., Kaptan, S., Kvernadze, T., Kvaratskhelia, O., Littlefair, S., Michniewicz, O., Nakhatutai, N., Ogłoza, W., Ohsawa, R., Olszewska, J. M., Polińska, M., Popowicz, A., Qvam, J. K. T., Radziwonowicz, M., Reichart, D. E., Słowikowska, A., Simon, A., Sonbas, E., Stojanovic, M., Tsapras, Y., Vanaverbeke, S., Wambsganss, J., Wilson, R. W., Żejmo, M., Zola, S.
We present the results of our analysis of Gaia19dke, an extraordinary microlensing event in the Cygnus constellation that was first spotted by the {\gaia} satellite. This event featured a strong microlensing parallax effect, which resulted in multipl
Externí odkaz:
http://arxiv.org/abs/2309.03324
Autor:
Kann, D. A., Agayeva, S., Aivazyan, V., Alishov, S., Andrade, C. M., Antier, S., Baransky, A., Bendjoya, P., Benkhaldoun, Z., Beradze, S., Berezin, D., Boër, M., Broens, E., Brunier, S., Bulla, M., Burkhonov, O., Burns, E., Chen, Y., Chen, Y. P., Conti, M., Coughlin, M. W., Cui, W. W., Daigne, F., Delaveau, B., Devillepoix, H. A. R., Dietrich, T., Dornic, D., Dubois, F., Ducoin, J. -G., Durand, E., Duverne, P. -A., Eggenstein, H. -B., Ehgamberdiev, S., Fouad, A., Freeberg, M., Froebrich, D., Ge, M. Y., Gervasoni, S., Godunova, V., Gokuldass, P., Gurbanov, E., Han, D. W., Hasanov, E., Hello, P., Hussenot-Desenonges, T., Inasaridze, R., Iskandar, A., Ismailov, N., Janati, A., Laz, T. Jegou du, Jia, S. M., Karpov, S., Kaeouach, A., Kiendrebeogo, R. W., Klotz, A., Kneip, R., Kochiashvili, N., Kunert, N., Lekic, A., Leonini, S., Li, C. K., Li, W., Li, X. B., Liao, J. Y., Logie, L., Lu, F. J., Mao, J., Marchais, D., Ménard, R., Morris, D., Natsvlishvili, R., Nedora, V., Noonan, K., Noysena, K., Orange, N. B., Pang, P. T. H., Peng, H. W., Pellouin, C., Peloton, J., Pradier, T., Pyshna, O., Rajabo, Y., Rau, S., Rinner, C., Rivet, J. -P., Romanov, F. D., Rosi, P., Rupchandani, V. A., Serrau, M., Shokry, A., Simon, A., Smith, K., Sokoliuk, O., Soliman, M., Song, L. M., Takey, A., Tillayev, Y., Ramirez, L. M. Tinjaca, Melo, I. Tosta e, Turpin, D., Postigo, A. de Ugarte, Vanaverbeke, S., Vasylenko, V., Vernet, D., Vidadi, Z., Wang, C., Wang, J., Wang, L. T., Wang, X. F., Xiong, Shaolin L., Xu, Y. P., Xue, W. C., Zeng, X., Zhang, S. N., Zhao, H. S., Zhao, X. F.
GRB 221009A is the brightest Gamma-Ray Burst (GRB) detected in more than 50 years of study. In this paper, we present observations in the X-ray and optical domains after the GRB obtained by the GRANDMA Collaboration (which includes observations from
Externí odkaz:
http://arxiv.org/abs/2302.06225
Autor:
Agayeva, S., Aivazyan, V., Alishov, S., Almualla, M., Andrade, C., Antier, S., Bai, J. -M., Baransky, A., Basa, S., Bendjoya, P., Benkhaldoun, Z., Beradze, S., Berezin, D., Bhardwaj, U., Blazek, M., Burkhonov, O., Burns, E., Caudill, S., Christensen, N., Colas, F., Coleiro, A., Corradi, W., Coughlin, M. W., Culino, T., Darson, D., Datashvili, D., Dietrich, T., Dolon, F., Dornic, D., Dubouil, J., Ducoin, J. -G., Duverne, P. -A., Esamdin, A., Fouad, A., Guo, F., Godunova, V., Gokuldass, P., Guessoum, N., Gurbanov, E., Hainich, R., Hasanov, E., Hello, P., Hussenot-Desenonges, T., Inasaridze, R., Iskandar, A., Ishida, E. E. O., Ismailov, N., Laz, T. Jegou du, Kann, D. A., Kapanadze, G., Karpov, S., Kiendrebeogo, R. W., Klotz, A., Kochiashvili, N., Kaeouach, A., Kneib, J. -P., Kou, W., Kruiswijk, K., Lombardo, S., Lamoureux, M., Leroy, N., Van Su, A. Le, Mao, J., Masek, M., Midavaine, T., Moeller, A., Morris, D., Natsvlishvili, R., Navarete, F., Nissanke, S., Noonan, K., Noysena, K., Orange, N. B., Peloton, J., Pilloix, M., Pradier, T., Raaijmakers, G., Rajabov, Y., Rivet, J. -P., Romanyuk, Y., Rousselot, L., Ruenger, F., Rupchandani, V., Sadibekova, T., Sasaki, N., Smith, K., Sokoliuk, O., Song, X., Simon, A., Takey, A., Tillayev, Y., Melo, I. Tosta e, Turpin, D., Postigo, A. de Ugarte, Vardosanidze, M., Wang, X. F., de Wasseige, G., Vernet, D., Vidadi, Z., Zhu, J., Zhu, Y.
GRANDMA is a world-wide collaboration with the primary scientific goal of studying gravitational-wave sources, discovering their electromagnetic counterparts and characterizing their emission. GRANDMA involves astronomers, astrophysicists, gravitatio
Externí odkaz:
http://arxiv.org/abs/2207.10178
Autor:
Valtonen, Mauri J., Dey, Lankeswar, Zola, S., Ciprini, S., Kidger, M., Pursimo, T., Gopakumar, A., Matsumoto, K., Sadakane, K., Caton, D. B., Nilsson, K., Komossa, S., Bagaglia, M., Baransky, A., Boumis, P., Boyd, D., Castro-Tirado, A. J., Debski, B., Drozdz, M., Pérez, A. Escartin, Fiorucci, M., Garcia, F., Gazeas, K., Ghosh, S., Godunova, V., Gomez, J. L., Gredel, R., Grupe, D., Haislip, J. B., Henning, T., Hurst, G., Janík, J., Kouprianov, V. V., Lehto, H., Liakos, A., Mathur, S., Mugrauer, M., Nogues, R. Naves, Nucciarelli, G., Ogloza, W., Ojha, D. K., Pajdosz-Śmierciak, U., Pascolini, S., Poyner, G., Reichart, D. E., Rizzi, N., Roncella, F., Sahu, D. K., Sillanpää, A., Simon, A., Siwak, M., Alfaro, F. C. Soldán, Sonbas, E., Tosti, G., Vasylenko, V., Webb, J. R., Zielinski, P.
OJ 287 is a BL Lacertae type quasar in which the active galactic nucleus (AGN) outshines the host galaxy by an order of magnitude. The only exception to this may be at minimum light when the AGN activity is so low that the host galaxy may make quite
Externí odkaz:
http://arxiv.org/abs/2205.15589
Autor:
Aivazyan, V., Almualla, M., Antier, S., Baransky, A., Barynova, K., Basa, S., Bayard, F., Beradze, S., Berezin, D., Blazek, M., Boutigny, D., Boust, D., Broens, E., Burkhonov, O., Cailleau, A., Christensen, N., Cejudo, D., Coleiro, A., Coughlin, M. W., Datashvili, D., Dietrich, T., Dolon, F., Ducoin, J. -G., Duverne, P. -A., Marchal-Duval, G., Galdies, C., Granier, L., Godunova, V., Gokuldass, P., Eggenstein, H. B., Freeberg, M., Hello, P., Inasaridze, R., Ishida, E. O., Jaquiery, P., Kann, D. A., Kapanadze, G., Karpov, S., Kiendrebeogo, R. W., Klotz, A., Kneip, R., Kochiashvili, N., Kou, W., Kugel, F., Lachaud, C., Leonini, S., Leroy, A., Leroy, N., Van Su, A. Le, Marchais, D., Masek, M., Midavaine, T., Moller, A., Morris, D., Natsvlishvili, R., Navarete, F., Noysena, K., Nissanke, S., Noonan, K., Orange, N. B., Peloton, J., Popowicz, A., Pradier, T., Prouza, M., Raaijmakers, G., Rajabov, Y., Richmond, M., Romanyuk, Ya., Rousselot, L., Sadibekova, T., Serrau, M., Sokoliuk, O., Song, X., Simon, A., Stachie, C., Taylor, A., Tillayev, Y., Turpin, D., Vardosanidze, M., Vlieghe, J., Melo, I. Tosta e, Wang, X. F., Zhu, J.
We present our follow-up observations with GRANDMA of transient sources revealed by the Zwicky Transient Facility (ZTF). Over a period of six months, all ZTF triggers were examined in real time by a dedicated science module implemented in the Fink br
Externí odkaz:
http://arxiv.org/abs/2202.09766
Autor:
Pavlenko, E., Kato, T., Antonyuk, K., Pit, N., Keir, L., Udovichenko, S., Dubovsk'y, P., Sosnovskij, A., Antonyuk, O., Shimansky, V., Gabdeev, M., Rakhmatullaeva, F., Kokhirova, G., Belan, S., Simon, A., Baklanov, A., Kojiguchi, N., Godunova, V.
A CCD photometry of the dwarf nova MASTER OT J172758.09 +380021.5 was carried out in 2019 during 134 nights. Observations covered three superoutbursts, five normal outbursts and quiescence between them. The available ASASSN and ZTF data for 2014-2020
Externí odkaz:
http://arxiv.org/abs/2103.14369
Autor:
Carry, B., Thuillot, W., Spoto, F., David, P., Berthier, J., Tanga, P., Mignard, F., Bouquillon, S., Mendez, R . A., Rivet, J. -P., Van Suu, A. Le, Dell'Oro, A., Fedorets, G., Frezouls, B., Granvik, M., Guiraud, J., Muinonen, K., Panem, C., Pauwels, T., Roux, W., Walmsley, G., Petit, J. -M., Abe, L., azian, V. Ayv, Baillié, K., Baransky, A., Bendjoya, P., Dennefeld, M., Desmars, J., Eggl, S., Godunova, V., Hestroffer, D ., Inasaridze, R., Kashuba, V., Krugly, Y. N., Molotov, I. E., Robert, V., Simon, A., Sokolov, I., Souami, D., Tarady, V., Taris, F., Troianskyi, V., Vasylenko, V., Vernet, D.
Publikováno v:
A&A 648, A96 (2021)
Since July 2014, the ESA Gaia mission has been surveying the entire sky down to magnitude 20.7 in the visible. In addition to the millions of stars, thousands of Solar System Objects (SSOs) are observed daily. By comparing their positions to those of
Externí odkaz:
http://arxiv.org/abs/2010.02553
Autor:
Merc, J., Mikołajewska, J., Gromadzki, M., Gałan, C., Iłkiewicz, K., Skowron, J., Wyrzykowski, Ł., Hodgkin, S. T., Rybicki, K. A., Zieliński, P., Kruszyńska, K., Godunova, V., Simon, A., Reshetnyk, V., Lewis, F., Kolb, U., Morrell, M., Norton, A. J., Awiphan, S., Poshyachinda, S., Reichart, D. E., Greet, M., Kolgjini, J.
Publikováno v:
A&A 644, A49 (2020)
Besides the astrometric mission of the Gaia satellite, its repeated and high-precision measurements serve also as an all-sky photometric transient survey. The sudden brightenings of the sources are published as Gaia Photometric Science Alerts and are
Externí odkaz:
http://arxiv.org/abs/2009.14709
Autor:
Szegedi-Elek, E., Ábrahám, P., Wyrzykowski, L., Kun, M., Kóspál, A., Chen, L., Marton, G., Moór, A., Kiss, Cs., Pál, A., Szabados, L., Varga, J., Varga-Verebélyi, E., Andreas, C., Bachelet, E., Bischoff, R., Bódi, A., Breedt, E., Burgaz, U., Butterley, T., Čepas, V., Damljanovic, G., Gezer, I., Godunova, V., Gromadzki, M., Gurgul, A., Hardy, L., Hildebrandt, F., Hoffmann, S., Hundertmark, M., Ihanec, N., Janulis, R., Kalup, Cs., Kaczmarek, Z., Könyves-Tóth, R., Krezinger, M., Kruszyńska, K., Littlefair, S., Maskoliūnas, M., Mészáros, L., Mikołajczyk, P., Mugrauer, M., Netzel, H., Ordasi, A., Pakštienė, E., Rybicki, K. A., Sárneczky, K., Seli, B., Simon, A., Šiškauskaitė, K., Sódor, Á., Sokolovsky, K. V., Stenglein, W., Street, R., Szakáts, R., Tomasella, L., Tsapras, Y., Vida, K., Zdanavičius, J., Zieliński, M., Zieliński, P., Ziółkowska, O.
We present optical-infrared photometric and spectroscopic observations of Gaia18dvy, located in the Cygnus OB3 association at a distance of 1.88 kpc. The object was noted by the Gaia alerts system when its lightcurve exhibited a $\gtrsim$4 mag rise i
Externí odkaz:
http://arxiv.org/abs/2005.11537