Zobrazeno 71 - 80
of 53 913
pro vyhledávání: '"Smith, A. D."'
Autor:
Smith, Kevin D., Bullo, Francesco
Strongly contracting dynamical systems have numerous properties (e.g., incremental ISS), find widespread applications (e.g., in controls and learning), and their study is receiving increasing attention. This work starts with the simple observation th
Externí odkaz:
http://arxiv.org/abs/2209.10046
We present results from nine simulations that compare the standard $\Lambda$ Cold Dark Matter cosmology ($\Lambda$CDM) with counterfactual universes, for approximately $100\,{\rm Gyr}$ using the Enzo simulation code. We vary the value of $\Lambda$ an
Externí odkaz:
http://arxiv.org/abs/2209.08783
Autor:
Lai, Thomas S. -Y., Armus, Lee, U, Vivian, Diaz-Santos, Tanio, Larson, Kirsten L., Evans, Aaron, Malkan, Matthew A., Appleton, Philip, Rich, Jeff, Muller-Sanchez, Francisco, Inami, Hanae, Bohn, Thomas, McKinney, Jed, Finnerty, Luke, Law, David R., Linden, Sean, Medling, Anne M., Privon, George C., Song, Yiqing, Stierwalt, Sabrina, van der Werf, Paul P., Barcos-Muñoz, Loreto, Smith, J. D. T., Togi, Aditya, Aalto, Susanne, Böker, Torsten, Charmandaris, Vassilis, Howell, Justin, Iwasawa, Kazushi, Kemper, Francisca, Mazzarella, Joseph M., Murphy, Eric J., Brown, Michael J. I., Hayward, Christopher C., Marshall, Jason, Sanders, David, Surace, Jason
We present James Webb Space Telescope (JWST) Mid-InfraRed Instrument (MIRI) integral-field spectroscopy of the nearby merging, luminous infrared galaxy, NGC 7469. This galaxy hosts a Seyfert type-1.5 nucleus, a highly ionized outflow, and a bright, c
Externí odkaz:
http://arxiv.org/abs/2209.06741
Autor:
Li, Jinyang, da Silva, Gregório R. M., Kain, Schuyler, Bonacum, Jason, Smith, David D., Kovachy, Timothy, Shahriar, Selim M.
We theoretically investigate the feasibility of applying spin squeezing to a light pulse atom interferometer in the presence of large momentum transfer using off-resonant Raman transitions, in order to enhance the sensitivity of accelerometry close t
Externí odkaz:
http://arxiv.org/abs/2209.06549
Autor:
Fan, Siteng, Forget, François, Smith, Michael D., Guerlet, Sandrine, Badri, Khalid M., Atwood, Samuel A., Young, Roland M. B., Edwards, Christopher S., Christensen, Philip R., Deighan, Justin, Matroushi, Hessa R. Al, Bierjon, Antoine, Liu, Jiandong, Millour, Ehouarn
Temperature profiles retrieved using the first set of data of the Emirates Mars InfraRed Spectrometer (EMIRS) obtained during the science phase of the Emirates Mars Mission (EMM) are used for the analysis of migrating thermal tides in the Martian atm
Externí odkaz:
http://arxiv.org/abs/2209.01585
Autor:
Lelli, Federico, Davis, Timothy A., Bureau, Martin, Cappellari, Michele, Liu, Lijie, Ruffa, Ilaria, Smith, Mark D., Williams, Thomas G.
The mm-Wave Interferometric Survey of Dark Object Masses (WISDOM) is probing supermassive black holes (SMBHs) in galaxies across the Hubble sequence via molecular gas dynamics. We present the first WISDOM study of a luminous infrared galaxy with an a
Externí odkaz:
http://arxiv.org/abs/2209.00363
Autor:
Smith, Deborah G.1 (AUTHOR) deborah.smith@lsuhs.edu, Smith, Corey D.2 (AUTHOR), DeLeon, Jennifer A.1 (AUTHOR), Sandoz, Jillian L.2 (AUTHOR), Ochoa, Carolina O.2 (AUTHOR), Pearson, Martha P.3 (AUTHOR), Macena, Raimunda H. M.4 (AUTHOR)
Publikováno v:
PLoS ONE. 7/5/2024, Vol. 19 Issue 7, p1-15. 15p.
Publikováno v:
Journal of Teaching in Physical Education; Jul2024, Vol. 53 Issue 3, p501-509, 9p
Autor:
Smith, Jonathan D., Hall, Samuel, Coombs, George, Byrne, James, Thorne, Michael A. S., Brearley, J. Alexander, Long, Derek, Meredith, Michael, Fox, Maria
We introduce a method for long-distance maritime route planning in polar regions, taking into account complex changing environmental conditions. The method allows the construction of optimised routes, describing the three main stages of the process:
Externí odkaz:
http://arxiv.org/abs/2209.02389
Star clusters are known to be formed in turbulent molecular clouds. How turbulence is driven in molecular clouds and what effect this has on star formation is still unclear. We compare a simulation setup with turbulent driving everywhere in a periodi
Externí odkaz:
http://arxiv.org/abs/2208.05474