Zobrazeno 1 - 10
of 227
pro vyhledávání: '"Kiss, Cs."'
In this paper, we present a large-scale dynamical survey of the trans-Neptunian region, with particular attention to mean-motion resonances (MMRs). We study a set of 4121 trans-Neptunian objects (TNOs), a sample far larger than in previous works. We
Externí odkaz:
http://arxiv.org/abs/2302.01221
Autor:
Szakáts, R., Kiss, Cs., Ortiz, J. L., Morales, N., Pál, A., Müller, T. G., Greiner, J., Santos-Sanz, P., Marton, G., Duffard, R., Sági, P., Forgács-Dajka, E.
Publikováno v:
A&A 669, L3 (2023)
The rotational states of the members in the dwarf planet - satellite systems in the transneptunian region are determined by the formation conditions and the tidal interaction between the components, and these rotational characteristics are the prime
Externí odkaz:
http://arxiv.org/abs/2211.07987
Autor:
Santos-Sanz, P., Ortiz, J. L., Sicardy, B., Popescu, M., Benedetti-Rossi, G., Morales, N., Vara-Lubiano, M., Camargo, J. I. B., Pereira, C. L., Rommel, F. L., Assafin, M., Desmars, J., Braga-Ribas, F., Duffard, R., Oliveira, J. Marques, Vieira-Martins, R., Fernández-Valenzuela, E., Morgado, B. E., Acar, M., Anghel, S., Atalay, E., Ateş, A., Bakış, H., Bakış, V., Eker, Z., Erece, O., Kaspi, S., Kayhan, C., Kilic, S. E., Kilic, Y., Manulis, I., Nedelcu, D. A., Niaei, M. S., Nir, G., Ofek, E., Ozisik, T., Petrescu, E., Satir, O., Solmaz, A., Sonka, A., Tekes, M., Unsalan, O., Yesilyaprak, C., Anghel, R., Berteşteanu, D., Curelaru, L., Danescu, C., Dumitrescu, V., Gherase, R., Hudin, L., Stoian, A-M., Tercu, J. O., Truta, R., Turcu, V., Vantdevara, C., Belskaya, I., Dementiev, T. O., Gazeas, K., Karampotsiou, S., Kashuba, V., Kiss, Cs., Koshkin, N., Kozhukhov, O. M., Krugly, Y., Lecacheux, J., Pal, A., Püsküllü, Ç., Szakats, R., Zhukov, V., Bamberger, D., Mondon, B., Perelló, C., Pratt, A., Schnabel, C., Selva, A., Teng, J. P., Tigani, K., Tsamis, V., Weber, C., Wells, G., Kalkan, S., Kudak, V., Marciniak, A., Ogloza, W., Ozdemir, T., Pakstiene, E., Perig, V., Zejmo, M.
Publikováno v:
A&A 664, A130 (2022)
Within our international program to obtain accurate physical properties of trans-Neptunian objects (TNOs) we predicted a stellar occultation by the TNO (38628) Huya of the star Gaia DR2 4352760586390566400 (mG = 11.5 mag.) for March 18, 2019. After a
Externí odkaz:
http://arxiv.org/abs/2205.12882
Autor:
Santos-Sanz, P., Ortiz, J. L., Sicardy, B., Benedetti-Rossi, G., Morales, N., Fernández-Valenzuela, E., Duffard, R., Iglesias-Marzoa, R., Lamadrid, J. L., Maícas, N., Pérez, L., Gazeas, K., Guirado, J. C., Peris, V., Ballesteros, F. J., Organero, F., Ana-Hernández, L., Fonseca, F., Alvarez-Candal, A., Jiménez-Teja, Y., Vara-Lubiano, M., Braga-Ribas, F., Camargo, J. I. B., Desmars, J., Assafin, M., Vieira-Martins, R., Alikakos, J., Boutet, M., Bretton, M., Carbognani, A., Charmandaris, V., Ciabattari, F., Delincak, P., Leiva, A. Fuambuena, González, H., Haymes, T., Hellmich, S., Horbowicz, J., Jennings, M., Kattentidt, B., Kiss, Cs., Komžík, R., Lecacheux, J., Marciniak, A., Moindrot, S., Mottola, S., Pal, A., Paschalis, N., Pastor, S., Perello, C., Pribulla, T., Ratinaud, C., Reyes, J. A., Sanchez, J., Schnabel, C., Selva, A., Signoret, F., Sonbas, E., Alí-Lagoa, V.
We predicted a stellar occultation of the bright star Gaia DR1 4332852996360346368 (UCAC4 385-75921) (m$_{\rm V}$= 14.0 mag) by the centaur 2002 GZ$_{32}$ for 2017 May 20$^{\rm th}$. Our latest shadow path prediction was favourable to a large region
Externí odkaz:
http://arxiv.org/abs/2012.06621
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
Autor:
Farkas-Takács, A., Kiss, Cs., Vilenius, E., Marton, G., Müller, T. G., Mommert, M., Stansberry, J., Lellouch, E., Lacerda, P., Pál, A.
Publikováno v:
A&A 638, A23 (2020)
The goal of this work is to determine the physical characteristics of resonant, detached and scattered disk objects in the transneptunian region, observed mainly in the framework of the "TNOs are Cool!" Herschel Open Time Key Program. Based on therma
Externí odkaz:
http://arxiv.org/abs/2002.12712
Autor:
Marton, G., Kiss, Cs., Molnár, L., Pál, A., Farkas-Takács, A., Szabó, Gy. M., Müller, T., Alí-Lagoa, V., Szabó, R., Vinkó, J., Sárneczky, K., Kalup, Cs. E., Marciniak, A., Duffard, R., Kiss, L. L.
Here we present the results of visible range light curve observations of ten Centaurs using the Kepler Space Telescope in the framework of the K2 mission. Well defined periodic light curves are obtained in six cases allowing us to derive rotational p
Externí odkaz:
http://arxiv.org/abs/2002.11388
Autor:
Marton, G., Ábrahám, P., Szegedi-Elek, E., Varga, J., Kun, M., Kóspál, Á., Varga-Verebélyi, E., Hodgkin, S., Szabados, L., Beck, R., Kiss, Cs.
The second $Gaia$ Data Release (DR2) contains astrometric and photometric data for more than 1.6 billion objects with mean $Gaia$ $G$ magnitude $<$20.7, including many Young Stellar Objects (YSOs) in different evolutionary stages. In order to explore
Externí odkaz:
http://arxiv.org/abs/1905.03063
Autor:
Müller, T., Kiss, Cs., Ali-Lagoa, V., Ortiz, J. L., Lellouch, E., Santos-Sanz, P., Fornasier, S., Marton, G., Mommert, M., Farkas-Takacs, A., Thirouin, A., Vilenius, E.
A recent occultation measurement of the dwarf planet Haumea (Ortiz et al. 2017) revealed an elongated shape with the longest axis comparable to Pluto's mean diameter. The chords also indicate a ring around Haumea's equatorial plane, where its largest
Externí odkaz:
http://arxiv.org/abs/1811.09476
Autor:
Farkas-Takács, A., Kiss, Cs., Pál, A., Molnár, L., Szabó, Gy. M., Hanyecz, O., Sárneczky, K., Szabó, R., Marton, G., Mommert, M., Szakáts, R., Müller, T., Kiss, L. L.
In this paper we present visible range light curves of the irregular Uranian satellites Sycorax, Caliban, Prospero, Ferdinand and Setebos taken with Kepler Space Telescope in the course of the K2 mission. Thermal emission measurements obtained with t
Externí odkaz:
http://arxiv.org/abs/1706.06837