Zobrazeno 1 - 10
of 2 989
pro vyhledávání: '"Torrey P"'
Automatic sound classification has a wide range of applications in machine listening, enabling context-aware sound processing and understanding. This paper explores methodologies for automatically classifying heterogeneous sounds characterized by hig
Externí odkaz:
http://arxiv.org/abs/2410.00980
Autor:
Chen, Qian-Hui, Grasha, Kathryn, Battisti, Andrew J., Wisnioski, Emily, Li, Zefeng, Park, Hye-Jin, Groves, Brent, Torrey, Paul, Mendel, Trevor, Madore, Barry F., Seibert, Mark, Sextl, Eva, Garcia, Alex M., Rich, Jeff A., Beaton, Rachael L., Kewley, Lisa J.
Most star formation in the local Universe occurs in spiral galaxies, but their origin remains an unanswered question. Various theories have been proposed to explain the development of spiral arms, each predicting different spatial distributions of th
Externí odkaz:
http://arxiv.org/abs/2409.05341
Autor:
Nguyen, Tri, Villaescusa-Navarro, Francisco, Mishra-Sharma, Siddharth, Cuesta-Lazaro, Carolina, Torrey, Paul, Farahi, Arya, Garcia, Alex M., Rose, Jonah C., O'Neil, Stephanie, Vogelsberger, Mark, Shen, Xuejian, Roche, Cian, Anglés-Alcázar, Daniel, Kallivayalil, Nitya, Muñoz, Julian B., Cyr-Racine, Francis-Yan, Roy, Sandip, Necib, Lina, Kollmann, Kassidy E.
The connection between galaxies and their host dark matter (DM) halos is critical to our understanding of cosmology, galaxy formation, and DM physics. To maximize the return of upcoming cosmological surveys, we need an accurate way to model this comp
Externí odkaz:
http://arxiv.org/abs/2409.02980
The merger timescales of isolated low-mass pairs ($\rm 10^8
Externí odkaz:
http://arxiv.org/abs/2409.02233
Modern interferometers such as LIGO have achieved sensitivities limited by quantum noise, comprised of radiation pressure and shot noise. To mitigate this noise, a static system is employed that minimizes the quantum noise within the measurement band
Externí odkaz:
http://arxiv.org/abs/2408.16171
Autor:
Narayanan, Desika, Stark, Daniel P., Finkelstein, Steven L., Torrey, Paul, Li, Qi, Cullen, Fergus, Topping, Micheal W., Marinacci, Federico, Sales, Laura V., Shen, Xuejian, Vogelsberger, Mark
JWST has enabled the detection of the UV continuum of galaxies at z>10, evidencing a population of extremely blue, potentially dust-free galaxies. Interpreting the UV spectra of galaxies as they redden is complicated by the well-known degeneracy betw
Externí odkaz:
http://arxiv.org/abs/2408.13312
Autor:
Sarkar, Arnab, Chakraborty, Priyanka, Vogelsberger, Mark, McDonald, Michael, Torrey, Paul, Garcia, Alex M., Khullar, Gourav, Ferland, Gary J., Forman, William, Wolk, Scott, Schneider, Benjamin, Bautz, Mark, Miller, Eric, Grant, Catherine, ZuHone, John
We present star formation rates (SFR), the mass-metallicity relation (MZR), and the SFR-dependent MZR across redshifts 4 to 10 using 81 star-forming galaxies observed by the JWST NIRSpec employing both low-resolution PRISM and medium-resolution grati
Externí odkaz:
http://arxiv.org/abs/2408.07974
Autor:
Garcia, Alex M., Torrey, Paul, Ellison, Sara L., Grasha, Kathryn, Chen, Qian-Hui, Hemler, Z. S., Zimmerman, Dhruv T., Wright, Ruby J., Zovaro, Henry R. M., Nelson, Erica J., Sanders, Ryan L., Kewley, Lisa J., Hernquist, Lars
The metal content of galaxies is a direct probe of the baryon cycle. A hallmark example is the relationship between a galaxy's stellar mass, star formation rate (SFR), and gas-phase metallicity: the Fundamental Metallicity Relation (FMR). While low-r
Externí odkaz:
http://arxiv.org/abs/2407.06254
Autor:
Bhowmick, Aklant K, Blecha, Laura, Torrey, Paul, Somerville, Rachel S, Kelley, Luke Zoltan, Vogelsberger, Mark, Weinberger, Rainer, Hernquist, Lars, Sivasankaran, Aneesh
JWST has recently revealed a large population of accreting black holes (BHs) in the early Universe. Even after accounting for possible systematic biases, the high-z $M_*-M_{\rm \rm bh}$ relation derived from these objects by Pacucci et al. (2023 P23
Externí odkaz:
http://arxiv.org/abs/2406.14658
Autor:
Zhang, Eric, Sales, Laura V, Marinacci, Federico, Torrey, Paul, Vogelsberger, Mark, Springel, Volker, Li, Hui, Pakmor, Rüdiger, Gutcke, Thales A
Simulations of galaxy formation are mostly unable to resolve the energy-conserving phase of individual supernova events, having to resort to subgrid models to distribute the energy and momentum resulting from stellar feedback. However, the properties
Externí odkaz:
http://arxiv.org/abs/2406.10338