Zobrazeno 1 - 10
of 95
pro vyhledávání: '"Oszkiewicz, D. A."'
Autor:
Postigo, A. de Ugarte, Michalowski, M., Thoene, C. C., Martin, S., Ashok, A., Fernandez, J. F. Agui, Bremer, M., Misra, K., Perley, D. A., Heintz, K. E., Cherukuri, S. V., Dimitrov, W., Geron, T., Ghosh, A., Izzo, L., Kann, D. A., Koprowski, M. P., Lesniewska, A., Leung, J. K., Levan, A., Omar, A., Oszkiewicz, D., Polinska, M., Resmi, L., Schulze, S.
GRBs produced by the collapse of massive stars are usually found near the most prominent star-forming regions of star-forming galaxies. GRB 171205A happened in the outskirts of a spiral galaxy, a peculiar location in an atypical GRB host. In this pap
Externí odkaz:
http://arxiv.org/abs/2406.16726
Autor:
Marciniak, A., Ďurech, J., Choukroun, A., Hanuš, J., Ogłoza, W., Szakáts, R., Molnár, L., Pál, A., Monteiro, F., Frappa, E., Beisker, W., Pavlov, H., Moore, J., Adomavičienė, R., Aikawa, R., Andersson, S., Antonini, P., Argentin, Y., Asai, A., Assoignon, P., Barton, J., Baruffetti, P., Bath, K. L., Behrend, R., Benedyktowicz, L., Bernasconi, L., Biguet, G., Billiani, M., Błażewicz, D., Boninsegna, R., Borkowski, M., Bosch, J., Brazill, S., Bronikowska, M., Bruno, A., Bąk, M. Butkiewicz, Caron, J., Casalnuovo, G., Castellani, J. J., Ceravolo, P., Conjat, M., Delincak, P., Delpau, J., Demeautis, C., Demirkol, A., Dróżdż, M., Duffard, R., Durandet, C., Eisfeldt, D., Evangelista, M., Fauvaud, S., Fauvaud, M., Ferrais, M., Filipek, M., Fini, P., Fukui, K., Gährken, B., Geier, S., George, T., Goffin, B., Golonka, J., Goto, T., Grice, J., Guhl, K., Halíř, K., Hanna, W., Harman, M., Hashimoto, A., Hasubick, W., Higgins, D., Higuchi, M., Hirose, T., Hirsch, R., Hofschulz, O., Horaguchi, T., Horbowicz, J., Ida, M., Ignácz, B., Ishida, M., Isobe, K., Jehin, E., Joachimczyk, B., Jones, A., Juan, J., Kamiński, K., Kamińska, M. K., Kankiewicz, P., Kasebe, H., Kattentidt, B., Kim, D. -H., Kim, M. -J., Kitazaki, K., Klotz, A., Komraus, M., Konstanciak, I., Tóth, R. Könyves, Kouno, K., Kowald, E., Krajewski, J., Krannich, G., Kreutzer, A., Kryszczyńska, A., Kubánek, J., Kudak, V., Kugel, F., Kukita, R., Kulczak, P., Lazzaro, D., Licandro, J., Livet, F., Maley, P., Manago, N., Mánek, J., Manna, A., Matsushita, H., Meister, S., Mesquita, W., Messner, S., Michelet, J., Michimani, J., Mieczkowska, I., Morales, N., Motyliński, M., Murawiecka, M., Newman, J., Nikitin, V., Nishimura, M., Oey, J., Oszkiewicz, D., Owada, M., Pakštienė, E., Pawłowski, M., Pereira, W., Perig, V., Perła, J., Pilcher, F., Podlewska-Gaca, E., Polák, J., Polakis, T., Polińska, M., Popowicz, A., Richard, F., Rives, J. J., Rodrigues, T., Rogiński, Ł., Rondón, E., Rottenborn, M., Schäfer, R., Schnabel, C., Schreurs, O., Selva, A., Simon, M., Skiff, B., Skrutskie, M., Skrzypek, J., Sobkowiak, K., Sonbas, E., Sposetti, S., Stuart, P., Szyszka, K., Terakubo, K., Thomas, W., Trela, P., Uchiyama, S., Urbanik, M., Vaudescal, G., Venable, R., Watanabe, Ha., Watanabe, Hi., Winiarski, M., Wróblewski, R., Yamamura, H., Yamashita, M., Yoshihara, H., Zawilski, M., Zelený, P., Żejmo, M., Żukowski, K., Żywica, S.
Publikováno v:
A&A 679, A60 (2023)
As evidenced by recent survey results, majority of asteroids are slow rotators (P>12 h), but lack spin and shape models due to selection bias. This bias is skewing our overall understanding of the spins, shapes, and sizes of asteroids, as well as of
Externí odkaz:
http://arxiv.org/abs/2310.08995
Publikováno v:
Astronomy & Astrophysics, Volume 670, id.A53, 16 pp (2023)
Infrared measurements of asteroids are crucial for the determination of physical and thermal properties of individual objects, and for the understanding of the small-body populations in the solar system as a whole. But standard radiometric methods ca
Externí odkaz:
http://arxiv.org/abs/2302.06921
Autor:
Wilawer, E., Oszkiewicz, D., Kryszczyńska, A., Marciniak, A., Shevchenko, V., Belskaya, I., Kwiatkowski, T., Kankiewicz, P., Horbowicz, J., Kudak, V., Kulczak, P., Perig, V., Sobkowiak, K.
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 513, Issue 3, July 2022, Pages 3242-3251
The amount of sparse asteroid photometry being gathered by both space- and ground-based surveys is growing exponentially. This large volume of data poses a computational challenge owing to both the large amount of information to be processed and the
Externí odkaz:
http://arxiv.org/abs/2205.11337
Autor:
Leśniewska, Aleksandra, Michałowski, M. J., Kamphuis, P., Dziadura, K., Baes, M., Cerón, J. M. Castro, Gentile, G., Hjorth, J., Hunt, L. K., Jespersen, C. K., Koprowski, M. P., Floc'h, E. Le, Miraghaei, H., Guelbenzu, A. Nicuesa, Oszkiewicz, D., Palazzi, E., Polińska, M., Rasmussen, J., Schady, P., Watson, D.
Long ($>2$ s) gamma ray bursts (GRBs) are associated with explosions of massive stars, although in three instances, supernovae (SNe) have not been detected, despite deep observations. With new HI line and archival optical integral field spectroscopy
Externí odkaz:
http://arxiv.org/abs/2202.01188
Autor:
Kwiatkowski, T., Koleńczuk, P., Kryszczyńska, A., Oszkiewicz, D., Kamiński, K., Kamińska, M. K., Troianskyi, V., Skiff, B., Moskowitz, N., Kashuba, V., Kim, M. -J., Kim, T., Mottola, S., Santana-Ros, T., Kluwak, T., Buzzi, L., Bacci, P., Birtwhistle, P., Miles, R., Chatelain, J.
Publikováno v:
A&A 656, A126 (2021)
On 4 March 2021 at 9 UTC a 30-m in diameter near-Earth asteroid 2021 DW1 passed the Earth at a distance of 570000 km, reaching the maximum brightness of V=14.6 mag. We observed it photometrically from 2 March, when it was visible at V=16.5 mag, until
Externí odkaz:
http://arxiv.org/abs/2109.11689
Autor:
Marciniak, A., Ďurech, J., Alí-Lagoa, V., Ogłoza, W., Szakáts, R., Müller, T. G., Molnár, L., Pál, A., Monteiro, F., Arcoverde, P., Behrend, R., Benkhaldoun, Z., Bernasconi, L., Bosch, J., Brincat, S., Brunetto, L., Bąk, M. Butkiewicz, Del Freo, F., Duffard, R., Evangelista-Santana, M., Farroni, G., Fauvaud, S., Fauvaud, M., Ferrais, M., Geier, S., Golonka, J., Grice, J., Hirsch, R., Horbowicz, J., Jehin, E., Julien, P., Kalup, Cs., Kamiński, K., Kamińska, M. K., Kankiewicz, P., Kecskeméthy, V., Kim, D. -H., Kim, M. -J., Konstanciak, I., Krajewski, J., Kudak, V., Kulczak, P., Kundera, T., Lazzaro, D., Manzini, F., Medeiros, H., Michimani-Garcia, J., Morales, N., Nadolny, J., Oszkiewicz, D., Pakštienė, E., Pawłowski, M., Perig, V., Pilcher, F., Pinel, P., Podlewska-Gaca, E., Polakis, T., Richard, F., Rodrigues, T., Rondon, E., Roy, R., Sanabria, J. J., Santana-Ros, T., Skiff, B., Skrzypek, J., Sobkowiak, K., Sonbas, E., Stachowski, G., Strajnic, J., Trela, P., Tychoniec, Ł., Urakawa, S., Verebelyi, E., Wagrez, K., Żejmo, M., Żukowski, K.
Publikováno v:
A&A 654, A87 (2021)
Results from the TESS mission showed that previous studies strngly underestimated the number of slow rotators, revealing the importance of studying those asteroids. For most slowly rotating asteroids (P > 12), no spin and shape model is available bec
Externí odkaz:
http://arxiv.org/abs/2109.00463
Autor:
Shevchenko, V., Mikhalchenko, O., Belskaya, I., Slyusarev, I., Chiorny, V., Krugly, Yu., Hromakina, T., Dovgopol, A., Kiselev, N., Rublevsky, A., Antonyuk, K., Novichonok, A., Kusakin, A., Reva, I., Inasaridze, R., Ayvazian, V., Kapanadze, G., Molotov, I., Oszkiewicz, D., Kwiatkowski, T.
We present new photometric observations for twelve asteroids ((122) Gerda, (152) Atala, (260) Huberta, (665) Sabine, (692) Hippodamia, (723) Hammonia, (745) Mauritia, (768) Struveana, (863) Benkoela, (1113) Katja, (1175) Margo, (2057) Rosemary) from
Externí odkaz:
http://arxiv.org/abs/2105.09763
Autor:
Marciniak, A., Alí-Lagoa, V., Müller, T. G., Szakáts, R., Molnár, L., Pál, A., Gaca, E. Podlewska, Parley, N., Antonini, P., Barbotin, E., Behrend, R., Bernasconi, L., Bąk, M. Butkiewicz, Crippa, R., Duffard, R., Ditteon, R., Feuerbach, M., Fauvaud, S., Garlitz, J., Geier, S., Goncalves, R., Grice, J., Grześkowiak, I., Hirsch, R., Horbowicz, J., Kamiński, K., Kamińska, M. K., Kim, D. -H., Kim, M. -J., Konstanciak, I., Kudak, V., Kulczak, P., Maestre, J. L., Manzini, F., Marks, S., Monteiro, F., Ogłoza, W., Oszkiewicz, D., Pilcher, F., Perig, V., Polakis, T., Polińska, M., Roy, R., Sanabria, J. J., Santana-Ros, T., Skiff, B., Skrzypek, J., Sobkowiak, K., Sonbas, E., Thizy, O., Trela, P., Urakawa, S., Żejmo, M., Żukowski, K.
Publikováno v:
A&A 625, A139 (2019)
Context. Earlier work suggests that slowly rotating asteroids should have higher thermal inertias than faster rotators because the heat wave penetrates deeper into the sub-surface. However, thermal inertias have been determined mainly for fast rotato
Externí odkaz:
http://arxiv.org/abs/1905.06056
Autor:
Snodgrass, C., Carry, B., Berthier, J., Eggl, S., Mommert, M., Petit, J. -M., Spoto, F., Granvik, M., Laureijs, R., Altieri, B., Vavrek, R., Conversi, L., Nucita, A., Popescu, M., Kleijn, G. Verdoes, Kidger, M., Jones, G. H., Oszkiewicz, D., Juric, M., Jones, L.
The ESA Euclid mission is a space telescope that will survey ~15,000 square degrees of the sky, primarily to study the distant universe (constraining cosmological parameters through the lensing of galaxies). It is also expected to observe ~150,000 So
Externí odkaz:
http://arxiv.org/abs/1812.00607