Zobrazeno 1 - 10
of 30 360
pro vyhledávání: '"Hales"'
Autor:
Allamon, Zachary J., Hales, Quentin A., Royston, Andrew B., Rutledge, Douglas L., Yozie, Erica A.
The forced soliton equation is the starting point for semiclassical computations with solitons away from the small momentum transfer regime. This paper develops necessary analytical and numerical tools for analyzing solutions to the forced soliton eq
Externí odkaz:
http://arxiv.org/abs/2412.09487
Polycyclic aromatic hydrocarbons (PAHs) are responsible for strong mid-IR emission features near star-forming regions. It is well known that low-metallicity environments exhibit weaker PAH emission, but it is not clear how the metallicity affects the
Externí odkaz:
http://arxiv.org/abs/2410.18909
Autor:
Hales, Jonathon
In 1984, H. W. Lenstra described an algorithm finding divisors of $N$ congruent to $r \mod S$. When $S^3 > N$, this algorithm runs in polynomial time and hence factors $N$ in time $N^{1/3+o(1)}$. Lenstra's algorithm relies on a sign change in a const
Externí odkaz:
http://arxiv.org/abs/2410.05030
Autor:
Blair R. Peters, MD, Alvin A. Annen, MD, Jens U. Berli, MD, Sandra Gallagher, PT, Caitlin Smigelski, PT, Lorna H. Kahn, PT, Hales E. Skelton, BA
Publikováno v:
Plastic and Reconstructive Surgery, Global Open, Vol 10, Iss 10, p e4616 (2022)
Background:. Sensory nerve transfers are performed as part of phalloplasty surgery. Despite this, sensory re-education to rehabilitate these nerve transfers has not been employed. Additionally, little attention has been paid to the role of the centra
Externí odkaz:
https://doaj.org/article/b035638adf9c40ebbc9b3f110db29874
Publikováno v:
Plastic and Reconstructive Surgery, Global Open, Vol 10, Iss 9, p e4545 (2022)
Background:. Sensation following anterolateral thigh (ALT) phalloplasty is traditionally viewed as inferior to sensation following radial forearm phalloplasty, potentially due to fewer nerve coaptations performed. Neural anatomy of the ALT is well de
Externí odkaz:
https://doaj.org/article/0791f2c0cb984ad4b436234fceb10a71
Autor:
Hales, J., Barmby, P.
Gaia Data Release 3 (DR3) provides the first classifications for the sources in Gaia's all-sky database. Most Gaia sources are stars in the Milky Way, but DR3 also contains many sources that belong to nearby galaxies, as well as background galaxies a
Externí odkaz:
http://arxiv.org/abs/2408.12717
Autor:
Brennan, Aoife, Matrà, Luca, Marino, Sebastián, Wilner, David, Qi, Chunhua, Hughes, A. Meredith, Roberge, Aki, Hales, Antonio S., Redfield, Seth
The origin and evolution of CO gas in debris disks has been debated since its initial detection. The gas could have a primordial origin, as a remnant of the protoplanetary disk or a secondary exocometary origin. This paper investigates the origin of
Externí odkaz:
http://arxiv.org/abs/2405.13116
Autor:
Hales, Thomas, Vajjha, Koundinya
This book uses optimal control theory to prove that the most unpackable centrally symmetric convex disk in the plane is a smoothed polygon. A smoothed polygon is a polygon whose corners have been rounded in a special way by arcs of hyperbolas. To be
Externí odkaz:
http://arxiv.org/abs/2405.04331
Autor:
Hales, A. S., Gupta, A., Ruiz-Rodriguez, D., Williams, J. P., Perez, S., Cieza, L., Gonzalez-Ruilova, C., Pineda, J. E., Santamaria-Miranda, A., Tobin, J., Weber, P., Zhu, Z., Zurlo, A.
Publikováno v:
2024, ApJ, 966, 96H
We present ALMA 12-m, 7-m & Total Power (TP) Array observations of the FU Orionis outbursting system, covering spatial scales ranging from 160 to 25,000 au. The high-resolution interferometric data reveals an elongated $^{12}$CO(2-1) feature previous
Externí odkaz:
http://arxiv.org/abs/2405.03033
Polarimetric differential imaging with VLT/NACO. A comprehensive PDI pipeline for NACO data (PIPPIN)
Autor:
de Regt, S., Ginski, C., Kenworthy, M. A., Caceres, C., Garufi, A., Gledhill, T. M., Hales, A. S., Huelamo, N., Kospal, A., Millar-Blanchaer, M. A., Perez, S., Schreiber, M. R.
The observed diversity of exoplanets can possibly be traced back to the planet formation processes. Planet-disk interactions induce sub-structures in the circumstellar disk that can be revealed via scattered light observations. However, a high-contra
Externí odkaz:
http://arxiv.org/abs/2404.02222