Zobrazeno 1 - 10
of 943
pro vyhledávání: '"PARKER, ALEX"'
Autor:
Kiss, Csaba, Müller, Thomas G., Farkas-Takács, Anikó, Moór, Attila, Protopapa, Silvia, Parker, Alex H., Santos-Sanz, Pablo, Ortiz, Jose Luis, Holler, Bryan J., Wong, Ian, Stansberry, John, Fernández-Valenzuela, Estela, Glein, Christopher R., Lellouch, Emmanuel, Vilenius, Esa, Kalup, Csilla E., Regály, Zsolt, Szakáts, Róbert, Marton, Gábor, Pál, András, Szabó, Gyula M.
We report on the discovery of a very prominent mid-infrared (18-25 {\mu}m) excess associated with the trans-Neptunian dwarf planet (136472) Makemake. The excess, detected by the MIRI instrument of the James Webb Space Telescope, along with previous m
Externí odkaz:
http://arxiv.org/abs/2410.22544
Autor:
Baker, Dustin, Gomez-Leos, Enrique, Halfpap, Anastasia, Heath, Emily, Martin, Ryan R., Miller, Joe, Parker, Alex, Pungello, Hope, Schwieder, Coy, Veldt, Nick
Given a graph $H$, we say a graph $G$ is properly rainbow $H$-saturated if there is a proper edge-coloring of $G$ which contains no rainbow copy of $H$, but adding any edge to $G$ makes such an edge-coloring impossible. The proper rainbow saturation
Externí odkaz:
http://arxiv.org/abs/2409.15258
Autor:
Valei, Zahra, Wamsler, Karolina, Parker, Alex J., Obara, Therese A., Klotz, Alexander R., Shendruk, Tyler N.
Polymers are a primary building block in many biomaterials, often interacting with anisotropic backgrounds. While previous studies have considered polymer dynamics within nematic solvents, rarely are the the effects of anisotropic viscosity and polym
Externí odkaz:
http://arxiv.org/abs/2408.06533
Autor:
Parker, Alex
For a $k$-uniform hypergraph $H$, let $\nu^{(m)}(H)$ denote the maximum size of a set $S$ of edges of $H$ whose pairwise intersection has size less than $m$. Let $\tau^{(m)}(H)$ denote the minimum size of a set $S$ of $m$-sets of $V(H)$ such that eve
Externí odkaz:
http://arxiv.org/abs/2406.06501
Autor:
Porter, Simon B., Benecchi, Susan D., Verbiscer, Anne J., Grundy, W. M., Noll, Keith S., Parker, Alex H.
Binaries in the Kuiper Belt are common. Here we present our analysis of the Solar System Origins Legacy Survey (SSOLS) to show that using a PSF-fitting method can roughly double the number of binaries identified in that dataset. Out of 198 Kuiper Bel
Externí odkaz:
http://arxiv.org/abs/2406.02808
Write $W^{(n)}$ to mean the $n$-letter word obtained by repeating a fixed word $W$ and let $R_n$ denote a uniformly random $n$-letter word sampled from the same alphabet as $W$. We are interested in the average length of the longest common subsequenc
Externí odkaz:
http://arxiv.org/abs/2404.07285
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
Let $f(n,p,q)$ denote the minimum number of colors needed to color the edges of $K_n$ so that every copy of $K_p$ receives at least $q$ distinct colors. In this note, we show $\frac{6}{7}(n-1) \leq f(n,5,8) \leq n + o(n)$. The upper bound is proven u
Externí odkaz:
http://arxiv.org/abs/2308.16365
We calculate the upper bounds of the population of theoretically stable Centaur orbits between Uranus and Neptune. These small bodies are on low-eccentricity, low-inclination orbits in two specific bands of semi-major axis, centred at $\sim$24.6 au a
Externí odkaz:
http://arxiv.org/abs/2305.11412
Autor:
Bannister, Michele T., Alexandersen, Mike, Benecchi, Susan D., Chen, Ying-Tung, Delsanti, Audrey, Fraser, Wesley C., Gladman, Brett J., Granvik, Mikael, Grundy, Will M., Guilbert-Lepoutre, Aurélie, Gwyn, Stephen D. J., Ip, Wing-Huen, Jakubik, Marian, Jones, R. Lynne, Kaib, Nathan, Kavelaars, J. J., Lacerda, Pedro, Lawler, Samantha, Lehner, Matthew J., Lin, Hsing Wen, Lykawka, Patryk Sofia, Marsset, Michael, Murray-Clay, Ruth, Noll, Keith S., Parker, Alex, Petit, Jean-Marc, Pike, Rosemary E., Rousselot, Philippe, Schwamb, Megan E., Shankman, Cory, Veres, Peter, Vernazza, Pierre, Volk, Kathryn, Wang, Shiang-Yu, Weryk, Robert
We report the discovery and orbit of a new dwarf planet candidate, 2015 RR245, by the Outer Solar System Origins Survey (OSSOS). The orbit of 2015 RR245 is eccentric (e = 0.586), with a semimajor axis near 82 au, yielding a perihelion distance of 34
Externí odkaz:
http://hdl.handle.net/10150/622433
http://arizona.openrepository.com/arizona/handle/10150/622433
http://arizona.openrepository.com/arizona/handle/10150/622433