Zobrazeno 1 - 10
of 16 508
pro vyhledávání: '"*, Lucas M"'
Frequency-bin encoding furnishes a compelling pathway for quantum information processing systems compatible with established lightwave infrastructures based on fiber-optic transmission and wavelength-division multiplexing. Yet although significant pr
Externí odkaz:
http://arxiv.org/abs/2412.17683
Even after decades of usage as an extragalactic standard candle, the universal bright end of the planetary nebula luminosity function (PNLF) still lacks a solid theoretical explanation. Until now, models have modeled planetary nebulae (PNe) from arti
Externí odkaz:
http://arxiv.org/abs/2412.08702
Autor:
Clark, Spencer K., Watt-Meyer, Oliver, Kwa, Anna, McGibbon, Jeremy, Henn, Brian, Perkins, W. Andre, Wu, Elynn, Bretherton, Christopher S., Harris, Lucas M.
While autoregressive machine-learning-based emulators have been trained to produce stable and accurate rollouts in the climate of the present-day and recent past, none so far have been trained to emulate the sensitivity of climate to substantial chan
Externí odkaz:
http://arxiv.org/abs/2412.04418
Autor:
Jordan, Lucas M., Rometsch, Thomas
Context. Binary star systems allow us to study the planet formation process under extreme conditions. In the early stages, these systems contain a circumbinary disk and a disk around each star. To model the interactions between these disks in the fra
Externí odkaz:
http://arxiv.org/abs/2411.19073
Autor:
Mun, Marcie, Wisnioski, Emily, Harborne, Katherine E., Lagos, Claudia D. P., Valenzuela, Lucas M., Remus, Rhea-Silvia, Mendel, J. Trevor, Battisti, Andrew J., Ellison, Sara L., Foster, Caroline, Bravo, Matias, Brough, Sarah, Croom, Scott M., Gao, Tianmu, Grasha, Kathryn, Gupta, Anshu, Mai, Yifan, Mailvaganam, Anilkumar, Muller, Eric G. M., Sharma, Gauri, Sweet, Sarah M., Taylor, Edward N., Zafar, Tayyaba
We investigate the internal and external mechanisms that regulate and quench star formation (SF) in galaxies at $z \sim 0.3$ using MAGPI observations and the EAGLE, Magneticum, and IllustrisTNG cosmological simulations. Using SimSpin to generate mock
Externí odkaz:
http://arxiv.org/abs/2411.17882
Autor:
Kudritzki, Rolf-Peter, Urbaneja, Miguel A., Bresolin, Fabio, Macri, Lucas M., Yuan, Wenlong, Li, Siyang, Anand, Gagandeep S., Riess, Adam G.
A quantitative spectroscopic study of blue supergiant stars in the Hubble constant anchor galaxy NGC 4258 is presented. The non-LTE analysis of Keck I telescope LRIS spectra yields a central logarithmic metallicity (in units of the solar value) of [Z
Externí odkaz:
http://arxiv.org/abs/2411.07974
The formation details of globular clusters (GCs) are still poorly understood due to their old ages and the lack of detailed observations of their formation. A large variety of models for the formation and evolution of GCs have been created to improve
Externí odkaz:
http://arxiv.org/abs/2410.12901
Autor:
Wu, Kaiyi, Cohen, Lucas M., Myilswamy, Karthik V., Lingaraju, Navin B., Lu, Hsuan-Hao, Lukens, Joseph M., Weiner, Andrew M.
We demonstrate spectral shaping of entangled photons with a six-channel microring-resonator-based silicon photonic pulse shaper. Through precise calibration of thermal phase shifters in a microresonator-based pulse shaper, we demonstrate line-by-line
Externí odkaz:
http://arxiv.org/abs/2409.13638
Autor:
Santucci, Giulia, Lagos, Claudia Del P., Harborne, Katherine E., Derkenne, Caro, Poci, Adriano, Thater, Sabine, McDermid, Richard M., Mendel, J. Trevor, Wisnioski, Emily, Croom, Scott M., Ferré-Mateu, Anna, Muller, Eric G. M., van de Sande, Jesse, Sharma, Gauri, Sweet, Sarah M., Tsukui, Takafumi, Valenzuela, Lucas M., van de Ven, Glenn, Zafar, Tayyaba
Schwarzschild dynamical models are now regularly employed in large surveys of galaxies in the local and distant Universe to derive information on galaxies' intrinsic properties such as their orbital structure and their (dark matter and stellar) mass
Externí odkaz:
http://arxiv.org/abs/2409.05940
Autor:
Mai, Yifan, Croom, Scott M., Wisnioski, Emily, Vaughan, Sam P., Varidel, Mathew R., Battisti, Andrew J., Mendel, J. Trevor, Mun, Marcie, Tsukui, Takafumi, Foster, Caroline, Harborne, Katherine E., Lagos, Claudia D. P., Wang, Di, Bellstedt, Sabine, Bland-Hawthorn, Joss, Colless, Matthew, D'Eugenio, Francesco, Grasha, Kathryn, Peng, Yingjie, Santucci, Giulia, Sweet, Sarah M., Thater, Sabine, Valenzuela, Lucas M., Ziegler, Bodo
We measure the ionised gas velocity dispersions of star-forming galaxies in the MAGPI survey ($z\sim0.3$) and compare them with galaxies in the SAMI ($z\sim0.05$) and KROSS ($z\sim1$) surveys to investigate how the ionised gas velocity dispersion evo
Externí odkaz:
http://arxiv.org/abs/2408.12224