Zobrazeno 1 - 10
of 16 444
pro vyhledávání: '"P. Faber"'
Autor:
Wang, Xiaohan, Luo, Yifei, Faber, S. M., Koo, David C., Mao, Shude, Westfall, Kyle B., Lu, Shengdong, Wang, Weichen, Bundy, Kevin, Boardman, N., Avila-Reese, Vladimir, Fernández-Trincado, José G., Lane, Richard R.
We investigate how the stellar rotational support changes as a function of spatially resolved stellar population age ($\rm D_n4000$) and relative central stellar surface density ($\Delta \Sigma_1$) for MaNGA isolated/central disk galaxies. We find th
Externí odkaz:
http://arxiv.org/abs/2408.02669
Multiple Object Tracking (MOT) is a computer vision task that has been employed in a variety of sectors. Some common limitations in MOT are varying object appearances, occlusions, or crowded scenes. To address these challenges, machine learning metho
Externí odkaz:
http://arxiv.org/abs/2407.18288
Autor:
Faber, Xander
Let $K$ be a complete discretely valued field. An extension $L/K$ is weakly totally ramified if the residue extension is purely inseparable. We prove that elliptic curves over $K$ and dynamical systems on $\mathbb{P}^1_K$ achieve semistable reduction
Externí odkaz:
http://arxiv.org/abs/2407.12089
Autor:
Faber, Jakob T., Ravi, Vikram, Ocker, Stella Koch, Sherman, Myles B., Sharma, Kritti, Connor, Liam, Law, Casey, Kosogorov, Nikita, Hallinan, Gregg, Harnach, Charlie, Hellbourg, Greg, Hobbs, Rick, Hodge, David, Hodges, Mark, Lamb, James W., Rasmussen, Paul, Somalwar, Jean J., Weinreb, Sander, Woody, David P.
We present a multi-wavelength study of the apparently non-repeating, heavily scattered fast radio burst, FRB 20221219A, detected by the Deep Synoptic Array 110 (DSA-110). The burst exhibits a moderate dispersion measure (DM) of $706.7^{+0.6}_{-0.6}$
Externí odkaz:
http://arxiv.org/abs/2405.14182
The propagation of magnons along a symmetry path may depend on the direction of propagation, similar to many other quasiparticles in nature. This phenomenon is commonly referred to as nonreciprocity. In addition to the fact that it is of great intere
Externí odkaz:
http://arxiv.org/abs/2405.12854
The degree-diameter problem for graphs is to find the largest number of vertices a graph can have given its diameter and maximum degree. We show we can realize this problem in terms of quasigroups, 1-factors and permutation groups. Our investigation
Externí odkaz:
http://arxiv.org/abs/2405.12374
Walk on Spheres algorithms leverage properties of Brownian Motion to create Monte Carlo estimates of solutions to a class of elliptic partial differential equations. Until recently, estimates were constructed pointwise and did not utilize the relatio
Externí odkaz:
http://arxiv.org/abs/2404.17692
Autor:
Boonstra, Marjolein, Bruneault, Frédérick, Chakraborty, Subrata, Faber, Tjitske, Gallucci, Alessio, Hickman, Eleanore, Kema, Gerard, Kim, Heejin, Kooiker, Jaap, Hildt, Elisabeth, Lamadé, Annegret, Mathez, Emilie Wiinblad, Möslein, Florian, Pathuis, Genien, Sartor, Giovanni, Steege, Marijke, Stocco, Alice, Tadema, Willy, Tuimala, Jarno, van Vledder, Isabel, Vetter, Dennis, Vetter, Jana, Westerlund, Magnus, Zicari, Roberto V.
This report shares the experiences, results and lessons learned in conducting a pilot project ``Responsible use of AI'' in cooperation with the Province of Friesland, Rijks ICT Gilde-part of the Ministry of the Interior and Kingdom Relations (BZK) (b
Externí odkaz:
http://arxiv.org/abs/2404.14366
Maximal Center Gauge (MCG) aims to detect center vortices by maximizing a gauge functional and then projecting onto the center elements of the respective group. The requirement for unrestricted maximization of the gauge functional has proven to be un
Externí odkaz:
http://arxiv.org/abs/2404.13304
Autor:
Stephenson, Jimena, Rodriguez-Puebla, Aldo, Faber, S. M., Primack, Joel R., Avila-Reese, Vladimir, Calette, A. R., Cannarozzo, Carlo, Kakos, James, Cano-Díaz, Mariana, Koo, David C., Shankar, Francesco, Morell, D. F.
We investigate the relation between galaxy structure and star formation rate (SFR) in a sample of $\sim2.9\times10^{4}$ central galaxies with $z<0.0674$ and axial ratios $b/a>0.5$. The star-forming main sequence (SFMS) shows a bend around the stellar
Externí odkaz:
http://arxiv.org/abs/2404.10114