Zobrazeno 1 - 10
of 343
pro vyhledávání: '"Vachier F"'
Autor:
Melo, I. Tosta e, Ducoin, J. -G., Vidadi, Z., Andrade, C., Rupchandani, V., Agayeva, S., Abdelhadi, J., Abe, L., Aguerre-Chariol, O., Aivazyan, V., Alishov, S., Antier, S., Bai, J. -M., Baransky, A., Bednarz, S., Bendjoya, Ph., Benkhaldoun, Z., Beradze, S., Bizouard, M. A., Bhardwaj, U., Blazek, M., Boër, M., Broens, E., Burkhonov, O., Christensen, N., Cooke, J., Corradi, W., Coughlin, M. W., Culino, T., Daigne, F., Dornic, D., Duverne, P. -A., Ehgamberdiev, S., Eymar, L., Fouad, A., Freeberg, M., Gendre, B., Guo, F., Gokuldass, P., Guessoum, N., Gurbanov, E., Hainich, R., Hasanov, E., Hello, P., Inasaridze, R., Iskandar, A., Ismailov, N., Janati, A., Laz, T. Jegou du, Kann, D. A., Karpov, S., Kiendrebeogo, R. W., Klotz, A., Kneip, R., Kochiashvili, N., Kaeouach, A., Kruiswijk, K., Lamoureux, M., Leroy, N., Lin, W. L., Mao, J., Marchais, D., Mašek, M., Midavaine, T., Moller, A., Morris, D., Natsvlishvili, R., Navarete, F., Guelbenzu, A Nicuesa, Noonan, K., Noysena, K., Oksanen, A., Orange, N. B., Pellouin, C., Peloton, J., Peng, H. W., Pilloix, M., Popowicz, A., Pradier, T., Pyshna, O., Raaijmakers, G., Rajabov, Y., Rau, A., Rinner, C., Rivet, J. -P., Ryh, A. S., Sabil, M., Sadibekova, T., Sasaki, N., Serrau, M., Simon, A., Shokry, A., Smith, K., Sokoliuk, O., Song, X., Takey, A., Thierry, P., Tillayev, Y., Turpin, D., Postigo, A. de Ugarte, Vasylenko, V., Vernet, D., Wang, L., Vachier, F., Vignes, J. P., Wang, X. F., Zeng, X., Zhang, J., Zhu, Y.
We present a campaign designed to train the GRANDMA network and its infrastructure to follow up on transient alerts and detect their early afterglows. In preparation for O4 II campaign, we focused on GRB alerts as they are expected to be an electroma
Externí odkaz:
http://arxiv.org/abs/2310.17287
Autor:
Carry, B., Descamps, P., Ferrais, M., Rivet, J. -P., Berthier, J., Jehin, E., Vernet, D., Abe, L., Bendjoya, P., Vachier, F., Pajuelo, M., Birlan, M., Colas, F., Benkhaldoun, Z.
Publikováno v:
A&A 680, A21 (2023)
Every population of small bodies in the Solar system contains a sizable fraction of multiple systems. Among these, the Jupiter Trojans have the lowest number of known binary systems and the least characterized. We aim at characterizing the reported b
Externí odkaz:
http://arxiv.org/abs/2309.15537
Autor:
Marsset, M., Brož, M., Vermersch, J., Rambaux, N., Ferrais, M., Viikinkoski, M., Hanuš, J., Jehin, E., Podlewska-Gaca, E., Bartczak, P., Dudzinski, G., Carry, B., Vernazza, P., Szakáts, R., Duffard, R., Jones, A., Molina, D., Santana-Ros, T., Benkhaldoun, Z., Birlan, M., Dumas, C., Fétick, R., Fusco, T., Jorda, L., Marchis, F., Vachier, F., Yang, B.
Cybele asteroids constitute an appealing reservoir of primitive material genetically linked to the outer Solar System, and the physical properties of the largest members can be readily accessed by large telescopes. We took advantage of the bright app
Externí odkaz:
http://arxiv.org/abs/2212.00680
Autor:
Brož, M., Ďurech, J., Carry, B., Vachier, F., Marchis, F., Hanuš, J., Jorda, L., Vernazza, P., Vokrouhlický, D., Walterová, M., Behrend, R.
Publikováno v:
A&A 657, A76 (2022)
The orbit of the outer satellite Alexhelios of (216) Kleopatra is already constrained by adaptive-optics astrometry, obtained with the VLT/SPHERE instrument. However, there is also a preceding occultation event in 1980 attributed to this satellite. H
Externí odkaz:
http://arxiv.org/abs/2110.12702
Autor:
Marchis, F., Jorda, L., Vernazza, P., Brož, M., Hanuš, J., Ferrais, M., Vachier, F., Rambaux, N., Marsset, M., Viikinkoski, M., Jehin, E., Benseguane, S., Podlewska-Gaca, E., Carry, B., Drouard, A., Fauvaud, S., Birlan, M., Berthier, J., Bartczak, P., Dumas, C., Dudzinski, G., Durech, J., Castillo-Rogez, J., Cipriani, F., Colas, F., Fetick, R., Fusco, T., Grice, J., Kryszczynska, A., Lamy, P., Marciniak, A., Michalowski, T., Michel, P., Pajuelo, M., Santana-Ros, T., Tanga, P., Vigan, A., Witasse, O., Yang, B.
Publikováno v:
A&A 653, A57 (2021)
Context. The recent estimates of the 3D shape of the M/Xe-type triple asteroid system (216) Kleopatra indicated a density of 5 g.cm$^{-3}$. Such a high density implies a high metal content and a low porosity which is not easy to reconcile with its pe
Externí odkaz:
http://arxiv.org/abs/2108.07207
Autor:
Brož, M., Marchis, F., Jorda, L., Hanuš, J., Vernazza, P., Ferrais, M., Vachier, F., Rambaux, N., Marsset, M., Viikinkoski, M., Jehin, E., Benseguane, S., Podlewska-Gaca, E., Carry, B., Drouard, A., Fauvaud, S., Birlan, M., Berthier, J., Bartczak, P., Dumas, C., Dudziński, G., Ďurech, J., Castillo-Rogez, J., Cipriani, F., Colas, F., Fetick, R., Fusco, T., Grice, J., Kryszczynska, A., Lamy, P., Marciniak, A., Michalowski, T., Michel, P., Pajuelo, M., Santana-Ros, T., Tanga, P., Vigan, A., Vokrouhlický, D., Witasse, O., Yang, B.
Publikováno v:
A&A 653, A56 (2021)
To interpret adaptive-optics observations of (216) Kleopatra, we need to describe an evolution of multiple moons, orbiting an extremely irregular body and including their mutual interactions. Such orbits are generally non-Keplerian and orbital elemen
Externí odkaz:
http://arxiv.org/abs/2105.09134
Autor:
Carry, B., Vernazza, P., Vachier, F., Neveu, M., Hanus, J. Berthier J., Ferrais, M., Jorda, L., Marsset, M., Viikinkoski, M., Bartczak, P., Behrend, R., Benkhaldoun, Z., Birlan, M., Castillo-Rogez, J., Cipriani, F., Colas, F., Drouard, A., Dudzinski, G. P., Desmars, J., Dumas, C., Durech, J., Fetick, R., Fusco, T., Grice, J., Jehin, E., Kaasalainen, M., Kryszczynska, A., Lamy, P., Marchis, F., Marciniak, A., Michalowski, T., Michel, P., Pajuelo, M., Podlewska-Gaca, E., Rambaux, N., Santana-Ros, T., Storrs, A., Tanga, P., Vigan, A., Warner, B., Wieczorek, M., Witasse, O., Yang, B.
Publikováno v:
A&A 650, A129 (2021)
Dynamical models of Solar System evolution have suggested that P-/D-type volatile-rich asteroids formed in the outer Solar System and may be genetically related to the Jupiter Trojans, the comets and small KBOs. Indeed, their spectral properties rese
Externí odkaz:
http://arxiv.org/abs/2103.06349
Autor:
Souami, D., Braga-Ribas, F., Sicardy, B., Morgado, B., Ortiz, J. L., Desmars, J., Camargo, J. I. B., Vachier, F., Berthier, J., Carry, B., Anderson, C. J., Showers, R., Thomason, K., Maley, P. D., Thomas, W., Buie, M. W., Leiva, R., Keller, J. M., Vieira-Martins, R., Assafin, M., Santos-Sanz, P., Morales, N., Duffard, R., Benedetti-Rossi, G., Gomes-Júnior, A. R., Boufleur, R., Pereira, C. L., Margoti, G., Pavlov, H., George, T., Oesper, D., Bardecker, J., Dunford, R., Kehrli, M., Spencer, C., Cota, J. M., Garcia, M., Lara, C., McCandless, K. A., Self, E., Lecacheux, J., Frappa, E., Dunham, D., Emilio, M.
Publikováno v:
A&A 643, A125 (2020)
We present results from the first recorded stellar occultation by the large trans-Neptunian object (174567) Varda that was observed on September 10$^{\rm th}$, 2018. Varda belongs to the high-inclination dynamically excited population, and has a sate
Externí odkaz:
http://arxiv.org/abs/2008.04818
Autor:
Agayeva, S., Alishov, S., Antier, S., Ayvazian, V. R., Bai, J. M., Baransky, A., Barynova, K., Basa, S., Beradze, S., Bertin, E., Berthier, J., Blažek, M., Boër, M., Burkhonov, O., Burrell, A., Cailleau, A., Chabert, B., Chen, J. C., Christensen, N., Coleiro, A., Corre, D., Coughlin, M. W., Coward, D., Crisp, H., Delattre, C., Dietrich, T., Ducoin, J. G., Duverne, P. A., Eymar, L., Fock-Hang, P., Gendre, B., Hello, P., Howell, E. J., Inasaridze, R. Ya., Ismailov, N., Kann, D. A., Kapanadze, G. V., Karpov, S., Klotz, A., Kochiashvili, N., Lachaud, C., Leroy, N., Van Su, A. Le, Li, W. X., Lin, W. L., Lognone, P., Marchal-Duval, G., Marron, R., Mašek, M., Mo, J., Moore, J. A., Morris, D., Natsvlishvili, R., Noysena, K., Orange, N. B., Perrigault, S., Peyrot, A., Prouza, M., Sadibekova, T., Samadov, D., Simon, A., Stachie, C., Teng, J. P., Thierry, P., Thöne, C. C., Tillayev, Y., Turpin, D., Postigo, A. de Ugarte, Vachier, F., Vardosanidze, M., Vasylenko, V., Vidadi, Z., Wang, C. J., Wang, X. F., Yan, S. Y., Zhang, J. C., Zhang, J. J., Zhang, X. H.
GRANDMA is an international project that coordinates telescope observations of transient sources with large localization uncertainties. Such sources include gravitational wave events, gamma-ray bursts and neutrino events. GRANDMA currently coordinate
Externí odkaz:
http://arxiv.org/abs/2008.03962
Autor:
Yang, B., Hanus, J., Carry, B., Vernazza, P., Broz, M., Vachier, F., Rambaux, N., Marsset, M., Chrenko, O., Sevecek, P., Viikinkoski, M., Jehin, E., Ferrais, M., Gaca, E. Podlewska, Drouard, A., Marchis, F., Birlan, M., Benkhaldoun, Z., Berthier, J., Bartczak, P., Dumas, C., Dudzinski, G., Durech, J., Castillo-Rogez, J., Cipriani, F., Colas, F., Fetick, R., Fusco, T., Grice, J., Jorda, L., Kaasalainen, M., Kryszczynska, A., Lamy, P., Marciniak, A., Michalowski, T., Michel, P., Pajuelo, M., Santana-Ros, T., Tanga, P., Vigan, A., Witasse, O.
Publikováno v:
A&A 641, A80 (2020)
Asteroid (31) Euphrosyne is one of the biggest objects in the asteroid main belt and the Euphrosyne family occupies a highly inclined region in the outer main belt and contains a remarkably large number of members, which is interpreted as an outcome
Externí odkaz:
http://arxiv.org/abs/2007.08059