Zobrazeno 1 - 10
of 96
pro vyhledávání: '"Ihanec, N"'
Autor:
Bachelet, E., Rota, P., Bozza, V., Zielinski, P., Tsapras, Y., Hundertmark, M., Wambsganss, J., Wyrzykowski, L., Mikolajczyk, P. J., Street, R. A., Jaimes, R. Figuera, Cassan, A., Dominik, M., Buckley, D. A. H., Awiphan, S., Nakhaharutai, N., Zola, S., Rybicki, K. A., Gromadzki, M., Howil, K., Ihanec, N., Jablonska, M., Kruszynska, K., Pylypenko, U., Ratajczak, M., Sitek, M., Rabus, M.
During the last 25 years, hundreds of binary stars and planets have been discovered towards the Galactic Bulge by microlensing surveys. Thanks to a new generation of large-sky surveys, it is now possible to regularly detect microlensing events across
Externí odkaz:
http://arxiv.org/abs/2405.02223
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:
Kruszyńska, K., Wyrzykowski, Ł., Rybicki, K. A., Howil, K., Jabłońska, M., Kaczmarek, Z., Ihanec, N., Maskoliūnas, M., Bronikowski, M., Pylypenko, U., Udalski, A., Mróz, P., Poleski, R., Skowron, J., Szymański, M. K., Soszyński, I., Pietrukowicz, P., Kozłowski, S., Ulaczyk, K., Iwanek, P., Wrona, M., Gromadzki, M., Mróz, M. J., Abe, F., Bando, K., Barry, R., Bennett, D. P., Bhattacharya, A., Bond, I. A., Fukui, A., Hamada, R., Hamada, S., Hamasaki, N., Hirao, Y., Silva, S. Ishitani, Itow, Y., Koshimoto, N., Matsubara, Y., Miyazaki, S., Muraki, Y., Nagai, T., Nunota, K., Olmschenk, G., Ranc, C., Rattenbury, N. J., Satoh, Y., Sumi, T., Suzuki, D., Tristram, P. J., Vandorou, A., Yama, H.
Gravitational microlensing is a phenomenon that allows us to observe dark remnants of stellar evolution even if they no longer emit electromagnetic radiation. In particular, it can be useful to observe solitary neutron stars or stellar-mass black hol
Externí odkaz:
http://arxiv.org/abs/2401.13759
Autor:
Charalampopoulos, P., Kotak, R., Wevers, T., Leloudas, G., Kravtsov, T., Pursiainen, M., Ramsden, P., Reynolds, T. M., Aamer, A., Anderson, J. P., Arcavi, I., Cai, Y. -Z., Chen, T. -W., Dennefeld, M., Galbany, L., Gromadzki, M., Guti'errez, C. P., Ihanec, N., Kangas, T., Kankare, E., Kool, E., Lawrence, A., Lundqvist, P., Makrygianni, L., Mattila, S., Müller-Bravo, T. E., Nicholl, M., Onori, F., Sahu, A., Smartt, S. J., Sollerman, J., Wang, Y., Young, D. R.
Publikováno v:
A&A 689, A350 (2024)
We present an extensive analysis of the optical and UV properties of AT2023clx, the closest TDE to date, that occurred in the nucleus of the interacting LINER galaxy, NGC3799 (z=0.01107). After correcting for the host reddening (E(B-V) = 0.179 mag),
Externí odkaz:
http://arxiv.org/abs/2401.11773
Autor:
Gkini, A., Lunnan, R., Schulze, S., Dessart, L., Brennan, S. J., Sollerman, J., Pessi, P. J., Nichol, M., Yan, L., Omand, C. M. B., Kangas, T., Moore, T., Anderson, J. P., Chen, T. -W., Gonzalez, E. P., Gromadzki, M., Gutiérrez, Claudia P., Hiramatsu, D., Howell, D. A., Ihanec, N., Inserra, C., McCully, C., Müller-Bravo, T. E., Pellegrino, C., Pignata, G., Pursiainen, M., Young, D. R.
SN\,2020zbf is a hydrogen-poor superluminous supernova (SLSN) at $z = 0.1947$ that shows conspicuous \ion{C}{II} features at early times, in contrast to the majority of H-poor SLSNe. Its peak magnitude is $M_{\rm g}$ = $-21.2$~mag and its rise time (
Externí odkaz:
http://arxiv.org/abs/2310.06814
Autor:
Wu, Zexuan, Dong, Subo, Yi, Tuan, Liu, Zhuokai, El-Badry, Kareem, Gould, Andrew, Wyrzykowski, L., Rybicki, K. A., Bachelet, Etienne, Christie, Grant W., de Almeida, L., Monard, L. A. G., McCormick, J., Natusch, Tim, Zielinski, P., Chen, Huiling, Huang, Yang, Liu, Chang, Merand, A., Mroz, Przemek, Shangguan, Jinyi, Udalski, Andrzej, Woillez, J., Zhang, Huawei, Hambsch, Franz-Josef, Mikolajczyk, P. J., Gromadzki, M., Ratajczak, M., Kruszynska, Katarzyna, Ihanec, N., Pylypenko, Uliana, Sitek, M., Howil, K., Zola, Staszek, Michniewicz, Olga, Zejmo, Michal, Lewis, Fraser, Bronikowski, Mateusz, Potter, Stephen, Andrzejewski, Jan, Merc, Jaroslav, Street, Rachel, Fukui, Akihiko, Jaimes, R. Figuera, Bozza, V., Rota, P., Cassan, A., Dominik, M., Tsapras, Y., Hundertmark, M., Wambsganss, J., Bakowska, K., Slowikowska, A.
We report discovering an exoplanet from following up a microlensing event alerted by Gaia. The event Gaia22dkv is toward a disk source rather than the traditional bulge microlensing fields. Our primary analysis yields a Jovian planet with M_p = 0.59^
Externí odkaz:
http://arxiv.org/abs/2309.03944
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:
Wiseman, P., Wang, Y., Hönig, S., Castro-Segura, N., Clark, P., Frohmaier, C., Fulton, M. D., Leloudas, G., Middleton, M., Müller-Bravo, T. E., Mummery, A., Pursiainen, M., Smartt, S. J., Smith, K., Sullivan, M., Anderson, J. P., Pulido, J. A. Acosta, Charalampopoulos, P., Banerji, M., Dennefeld, M., Galbany, L., Gromadzki, M., Gutiérrez, C. P., Ihanec, N., Kankare, E., Lawrence, A., Mockler, B., Moore, T., Nicholl, M., Onori, F., Petrushevska, T., Ragosta, F., Rest, S., Smith, M., Wevers, T., Carini, R., Chen, T. -W., Chambers, K., Gao, H., Huber, M., Inserra, C., Magnier, E., Makrygianni, L., Toy, M., Vincentelli, F., Young, D. R.
We present observations from X-ray to mid-infrared wavelengths of the most energetic non-quasar transient ever observed, AT2021lwx. Our data show a single optical brightening by a factor $>100$ to a luminosity of $7\times10^{45}$ erg s$^{-1}$, and a
Externí odkaz:
http://arxiv.org/abs/2303.04412
Autor:
Petrushevska, T., Leloudas, G., Ilic, D., Bronikowski, M., Charalampopoulos, P., Jaisawal, G. K., Paraskeva, E., Pursiainen, M., Rakic, N., Schulze, S., Taggart, K., Wedderkopp, C. K., Anderson, J. P., de Boer, T., Chambers, K., Chen, T. W., Damljanovic, G., Fraser, M., Gao, H., Gomboc, A., Gromadzki, M., Ihanec, N., Maguire, K., Marcun, B., Muller-Bravo, T. E., Nicholl, M., Onori, F., Reynolds, T. M., Smartt, S. J., Sollerman, J., Smith, K. W., Wevers, T., Wyrzykowski, L.
Thanks to the advent of large-scale optical surveys, a diverse set of flares from the nuclear regions of galaxies has recently been discovered. These include the disruption of stars by supermassive black holes at the centers of galaxies - nuclear tra
Externí odkaz:
http://arxiv.org/abs/2211.17097
Autor:
Onori, F., Cannizzaro, G., Jonker, P. G., Kim, M., Nicholl, M., Mattila, S., Reynolds, T. M., Fraser, M., Wevers, T., Brocato, E., Anderson, J. P., Carini, R., Charalampopoulos, P., Clark, P., Gromadzki, M., Gutiérrez, C. P., Ihanec, N., Inserra, C., Lawrence, A., Leloudas, G., Lundqvist, P., Müller-Bravo, T. E., Piranomonte, S., Pursiainen, M., Rybicki, K. A., Somero, A., Young, D. R., Chambers, K. C., Gao, H., de Boer, T. J. L., Magnier, E. A.
We present the results from a dense multi-wavelength (optical/UV, near-infrared (IR), and X-ray) follow-up campaign of the nuclear transient AT2017gge, covering a total of 1698 days from the transient's discovery. The bolometric lightcurve, the black
Externí odkaz:
http://arxiv.org/abs/2206.00049