Zobrazeno 1 - 10
of 43
pro vyhledávání: '"Zangari, Amanda M"'
Autor:
Buie, Marc W., Spencer, John R., Porter, Simon B., Benecchi, Susan D., Parker, Alex H., Stern, S. Alan, Belton, Michael, Binzel, Richard P., Borncamp, David, DeMeo, Francesca, Fabbro, S., Fuentes, Cesar, Furusawa, Hisanori, Fuse, Tetsuharu, Gay, Pamela L., Gwyn, Stephen, Holman, Matthew J., Karoji, H., Kavelaars, J. J., Kinoshita, Daisuke, Miyazaki, Satoshi, Mountain, Matt, Noll, Keith S., Osip, David J., Petit, Jean-Marc, Reid, Neill I., Sheppard, Scott S., Showalter, Mark, Steffl, Andrew J., Sterner, Ray E., Tajitsu, Akito, Tholen, David J., Trilling, David E., Weaver, Harold A., Verbiscer, Anne J., Wasserman, Lawrence H., Yamashita, Takuji, Yanagisawa, Toshifumi, Yoshida, Fumi, Zangari, Amanda M.
Following the Pluto fly-by of the New Horizons spacecraft, the mission provided a unique opportunity to explore the Kuiper Belt in-situ. The possibility existed to fly-by a Kuiper Belt object (KBO) as well as to observe additional objects at distance
Externí odkaz:
http://arxiv.org/abs/2403.04927
Autor:
Showalter, Mark R., Benecchi, Susan D., Buie, Marc W., Grundy, William M., Keane, James T., Lisse, Carey M., Olkin, Cathy B., Porter, Simon B., Robbins, Stuart J., Singer, Kelsi N., Verbiscer, Anne J., Weaver, Harold A., Zangari, Amanda M., Hamilton, Douglas P., Kaufmann, David E., Lauer, Tod R., Mehoke, D. S., Mehoke, T. S., Spencer, J. R., Throop, H. B., Parker, J. W., Stern, S. Alan
Publikováno v:
Icarus 356, id. 114098 (2021)
We investigate what can be learned about a population of distant KBOs by studying the statistical properties of their light curves. Whereas others have successfully inferred the properties of individual, highly variable KBOs, we show that the fractio
Externí odkaz:
http://arxiv.org/abs/2105.03543
Autor:
Mottola, Stefano, Hellmich, Stephan, Buie, Marc W., Zangari, Amanda M., Marchi, Simone, Brown, Michael E., Levison, Harold F.
We report new photometric lightcurve observations of the Lucy Mission target (11351) Leucus acquired during the 2017, 2018 and 2019 apparitions. We use these data in combination with stellar occultations captured during five epochs (Buie et al. 2020)
Externí odkaz:
http://arxiv.org/abs/2009.08951
Autor:
Buie, Marc W., Porter, Simon B., Tamblyn, Peter, Terrell, Dirk, Parker, Alex Harrison, Baratoux, David, Kaire, Maram, Leiva, Rodrigo, Verbiscer, Anne J., Zangari, Amanda M., Colas, François, Diop, Baïdy Demba, Samaniego, Joseph I., Wasserman, Lawrence H., Benecchi, Susan D., Caspi, Amir, Gwyn, Stephen, Kavelaars, J. J., Uría, Adriana C. Ocampo, Rabassa, Jorge, Skrutskie, M. F., Soto, Alejandro, Tanga, Paolo, Young, Eliot F., Stern, S. Alan, Andersen, Bridget C., Pérez, Mauricio E. Arango, Arredondo, Anicia, Artola, Rodolfo Alfredo, Bâ, Abdoulaye, Ballet, Romuald, Blank, Ted, Bop, Cheikh Tidiane, Bosh, Amanda S., López, Matías Aarón Camino, Carter, Christian M., Castro-Chacón, J. H., Desprez, Alfonso Caycedo, Guerra, Nicolás Caycedo, Conard, Steven J., Dauvergne, Jean-Luc, Dean, Bryan, Dean, Michelle, Desmars, Josselin, Dieng, Abdou Lahat, Dieng, Mame Diarra Bousso, Diouf, Omar, Dorego, Gualbert Séraphin, Dunham, David W., Dunham, Joan, Luca, Hugo A. Durantini, Edwards, Patrick, Erasmus, Nicolas, Faye, Gayane, Faye, Mactar, Ferrario, Lucas Ezequiel, Ferrell, Chelsea L., Finley, Tiffany J., Fraser, Wesley C., Friedli, Alison J., Serna, Julián Galvez, Garcia-Migani, Esteban A., Genade, Anja, Getrost, Kai, Gil-Hutton, Ricardo A., Gimeno, German N., Golub, Eli Joseph, Murillo, Giovanni Francisco González, Grusin, Michael D., Gurovich, Sebastian, Hanna, William H., Henn, Santiago M., Hinton, P. C., Hughes, Paul J., Josephs Jr, John David, Joya, Raul, Kammer, Joshua A., Keeney, Brian A., Keller, John M., Kramer, Emily A., Levine, Stephen E., Lisse, Carey M., Lovell, Amy J., Mackie, Jason A., Makarchuk, Stanislav, Manzano, Luis E., Mbaye, Salma Sylla, Mbaye, Modou, Melia, Raul Roberto, Moreno, Freddy, Moss, Sean K., Ndaiye, Diene, Ndiaye, Mapathe, Nelson, Matthew J., Olkin, Catherine B., Olsen, Aart M., Moreno, Victor Jonathan Ospina, Pasachoff, Jay M., Pereyra, Mariana Belen, Person, Michael J., Pinzón, Giovanni, Pulver, Eduardo Alejandro, Quintero, Edwin A., Regester, Jeffrey R., Resnick, Aaron Caleb, Reyes-Ruiz, Mauricio, Rolfsmeier, Alex D., Ruhland, Trina R., Salmon, Julien, Santos-Sanz, Pablo, Santucho, Marcos Ariel, Niño, Diana Karina Sepúlveda, Sickafoose, Amanda A., Silva, José S., Singer, Kelsi N., Skipper, Joy N., Slivan, Stephen M., Smith, Rose J. C., Spagnotto, Julio C., Stephens, Andrew W., Strabala, Samuel D., Tamayo, Francisco J., Throop, Henry B., Cañas, Andrés David Torres, Toure, Labaly, Traore, Alassane, Tsang, Constantine C. C., Turner, Jake D., Vanegas, Santiago, Venable, Roger, Wilson, John C., Zuluaga, Carlos A., Zuluaga, Jorge I.
Publikováno v:
The Astronomical Journal, Vol. 159, Issue 4, 130 (27pp); 2020 April
We present the results from four stellar occultations by (486958) Arrokoth, the flyby target of the New Horizons extended mission. Three of the four efforts led to positive detections of the body, and all constrained the presence of rings and other d
Externí odkaz:
http://arxiv.org/abs/2001.00125
Preliminary spacecraft trajectories for 45 Kuiper Belt Objects (KBOs) and Pluto suitable for launch between 2025 and 2040 are presented. These 46 objects comprise all objects with H magnitude < 4.0 or which have received a name from the International
Externí odkaz:
http://arxiv.org/abs/1810.07811
Autor:
Porter, Simon B., Spencer, John R., Benecchi, Susan, Verbiscer, Anne, Zangari, Amanda M., Weaver, H. A., Lauer, Tod R., Parker, Alex H., Buie, Marc W., Cheng, Andrew F., Young, Leslie A., Olkin, Cathy B., Ennico, Kimberly, Stern, S. Alan, Team, the New Horizons Science
Publikováno v:
The Astrophysical Journal Letters (2016), Volume 828, Number 2
NASA's New Horizons spacecraft observed (15810) 1994 JR$_1$, a 3:2 resonant Kupier Belt Object (KBO), using the LOng Range Reconnaissance Imager (LORRI) on November 2, 2015 from a distance of 1.85 AU, and again on April 7, 2016 from a distance of 0.7
Externí odkaz:
http://arxiv.org/abs/1605.05376
Autor:
Moore, Jeffrey M., McKinnon, William B., Spencer, John R., Howard, Alan D., Schenk, Paul M., Beyer, Ross A., Nimmo, Francis, Singer, Kelsi N., Umurhan, Orkan M., White, Oliver L., Stern, S. Alan, Ennico, Kimberly, Olkin, Cathy B., Weaver, Harold A., Young, Leslie A., Binzel, Richard P., Buie, Marc W., Buratti, Bonnie J., Cheng, Andrew F., Cruikshank, Dale P., Grundy, Will M., Linscott, Ivan R., Reitsema, Harold J., Reuter, Dennis C., Showalter, Mark R., Bray, Veronica J., Chavez, Carrie L., Howett, Carly J. A., Lauer, Tod R., Lisse, Carey M., Parker, Alex Harrison, Porter, S. B., Robbins, Simon J., Runyon, Kirby, Stryk, Ted, Throop, Henry B., Tsang, Constantine C. C., Verbiscer, Anne J., Zangari, Amanda M., Chaikin, Andrew L., Wilhelms, Don E.
Publikováno v:
Science 351, 1284 (2016)
NASA's New Horizons spacecraft has revealed the complex geology of Pluto and Charon. Pluto's encounter hemisphere shows ongoing surface geological activity centered on a vast basin containing a thick layer of volatile ices that appears to be involved
Externí odkaz:
http://arxiv.org/abs/1604.05702
Autor:
Nimmo, Francis, Umurhan, Orkan M, Lisse, Carey M, Bierson, Carver J, Lauer, Tod R, Buie, Marc W, Throop, Henry B, Kammer, Josh A, Roberts, James H, McKinnon, William B, Zangari, Amanda M, Moore, Jeffrey M, Stern, S Alan, Young, Leslie A, Weaver, Harold A, Olkin, Cathy B, Ennico, Kim, team, the New Horizons GGI
Approach images taken by the LORRI imaging system during the New Horizons spacecraft encounter have been used to determine the mean radii and shapes of Pluto and Charon. The primary observations are limb locations derived using three independent appr
Externí odkaz:
http://arxiv.org/abs/1603.00821
Autor:
Massey, Philip, Zangari, Amanda M., Morrell, Nidia I., Puls, Joachim, DeGioia-Eastwood, Kathleen, Bresolin, Fabio, Kudrtizki, Rolf-Peter
In order to better determine the physical properties of hot, massive stars as a function of metallicity, we obtained very high SNR optical spectra of 26 O and early B stars in the Magellanic Clouds. These allow accurate modeling even in cases where t
Externí odkaz:
http://arxiv.org/abs/0810.3962
We investigate the massive star content of NGC 3603, the closest known giant H II region. We have obtained spectra of 26 stars in the central cluster using the Baade 6.5-m telescope (Magellan I). Of these 26 stars, 16 had no previous spectroscopy. We
Externí odkaz:
http://arxiv.org/abs/0712.2621