Zobrazeno 1 - 10
of 1 005
pro vyhledávání: '"Yee, H. A."'
Autor:
Cramer, William J., Noble, A. G., Rudnick, G., Pigarelli, A., Wilson, G., Bahé, Y. M., Cooper, M. C., Demarco, R., Matharu, J., Miller, T. B., Muzzin, A., Nantais, J., Sportsman, W., van Kampen, E., Webb, T. M. A., Yee, H. K. C.
The changes in colors across a galaxy are intimately connected to the galaxy's formation, growth, quenching history, and dust content. A particularly important epoch in the growth of galaxies is near $z \sim 2$ often referred to as `cosmic noon', whe
Externí odkaz:
http://arxiv.org/abs/2404.07355
Autor:
Graham, Mark S., Pinaya, Walter Hugo Lopez, Wright, Paul, Tudosiu, Petru-Daniel, Mah, Yee H., Teo, James T., Jäger, H. Rolf, Werring, David, Nachev, Parashkev, Ourselin, Sebastien, Cardoso, M. Jorge
Methods for out-of-distribution (OOD) detection that scale to 3D data are crucial components of any real-world clinical deep learning system. Classic denoising diffusion probabilistic models (DDPMs) have been recently proposed as a robust way to perf
Externí odkaz:
http://arxiv.org/abs/2307.03777
Autor:
Arslandok, M., Bass, S. A., Baty, A. A., Bautista, I., Beattie, C., Becattini, F., Bellwied, R., Berdnikov, Y., Berdnikov, A., Bielcik, J., Blair, J. T., Bock, F., Boimska, B., Bossi, H., Caines, H., Chen, Y., Chien, Y. -T., Chiu, M., Connors, M. E., Csanád, M., da Silva, C. L., Dash, A. P., David, G., Dehmelt, K., Dexheimer, V., Dong, X., Drees, A., Du, L., Durham, J. M., Ehlers, R. J., Elfner, H., Evdokimov, O., Finger, M., Finger Jr., M., Frantz, J., Frawley, A. D., Gale, C., Geurts, F., Gonzalez, V., Grau, N., Greene, S. V., Grossberndt, S. K., Hachiya, T., He, X., Heinz, U., Hong, B., Humanic, T. J., Ivanishchev, D., Jacak, B. V., Jahan, J., Jeon, S., Jheng, H. R., Jia, J., Judd, E. G., Kapusta, J. I., Karpenko, I., Khachatryan, V., Kharzeev, D. E., Kim, M., Kimelman, B., Klay, J. L., Klein, S. R., Knospe, A. G., Koch, V., Kotov, D, Krintiras, G. K., Elayavalli, R. Kunnawalkam, Kuo, C. M., Lajoie, J. G., Lee, Y. -J., Li, W., Liao, J., Likmeta, I., Lim, S. H., Liu, M. X., Loizides, C., Longo, R., Luo, X., Luzum, M., Ma, R., Majumder, A., Mak, S., Markert, C., Mehtar-Tani, Y., Mignerey, A. C., Minafra, N., Morrison, D. P., Mueller, B., Nagle, J. L., Narde, A., Nattrass, C. E., Niida, T., Noronha, J., Noronha-Hostler, J., Nouicer, R., Novitzky, N., O'Brien, E., Odyniec, G., Okorokov, V. A., Osborn, J. D., Paquet, J. -F., Park, S., Parotto, P., Perepelitsa, D. V., Petreczky, P., Pinkenburg, C., Praszalowicz, M., Pruneau, C., Putschke, J., Ramasubramanian, N. V., Rapp, R., Ratti, C., Read, K. F., Teles, P. Rebello, Reed, R., Rinn, T., Roland, G., Rosati, M., Royon, C., Ruan, L., Sakaguchi, T., Salur, S., Sarsour, M., Menon, A. S., Schenke, B., Schmidt, N. V., Schmier, A., Schäfer, T., Seger, J., Seto, R., Sheibani, Oveis, Shen, C., Shi, Z., Shulga, E., Sickles, A. M., Singh, M., Singh, B. K., Smirnov, N., Smith, K. L., Song, H., Soudi, I., Leiton, A. G. Stahl, Steinberg, P., Stephanov, M., Strickland, M., Sumbera, M., Cerci, D. Sunar, Tachibana, Y., Tang, A. H., Takaki, D. Tapia, Teaney, D., Thomas, D., Timmins, A. R., Tribedy, P., Tu, Z., Tuo, S., Rueda, O. V., Velkovska, J., Venugopalan, R., Videbæk, F., Voloshin, S. A., Vovchenko, V., Vujanovic, G., Wang, X., Wang, F., Wang, X. -N., Weyhmiller, S., Xie, W., Xu, N., Yang, Y., Yao, X., Ye, Z., Yee, H. -U., Zajc, W. A.
Hot QCD physics studies the nuclear strong force under extreme temperature and densities. Experimentally these conditions are achieved via high-energy collisions of heavy ions at the Relativistic Heavy Ion Collider (RHIC) and the Large Hadron Collide
Externí odkaz:
http://arxiv.org/abs/2303.17254
Autor:
Alcorn, Leo Y., Yee, H. K. C, Drissen, Laurent, Rhea, Carter, Sivanandam, Suresh, Hlavacek-Larrondo, Julie, Hsieh, Bau-Ching, Lin, Lihwai, Lin, Yen-Ting, Liu, Qing, Muzzin, Adam, Noble, Allison, Pintos-Castro, Irene
We report CFHT/SITELLE imaging Fourier Transform Spectrograph observations of the Brightest Cluster Galaxy (BCG) of galaxy cluster Abell 2390 at z=0.228. The BCG displays a prominent cone of emission in H$\alpha$, H$\beta$, [NII], and [OII] to the No
Externí odkaz:
http://arxiv.org/abs/2303.15557
Autor:
Cramer, W. J., Noble, A. G., Massingill, K., Cairns, J., Clements, D. L., Cooper, M. C., Demarco, R., Matharu, J., McDonald, M., Muzzin, A., Nantais, J., Rudnick, G., Übler, H., van Kampen, E., Webb, T. M. A., Wilson, G., Yee, H. K. C.
We investigate the resolved kinematics of the molecular gas, as traced by ALMA in CO (2-1), of 25 cluster member galaxies across three different clusters at a redshift of $z\sim1.6$. This is the first large-scale analysis of the molecular gas kinemat
Externí odkaz:
http://arxiv.org/abs/2209.06929
Autor:
Pinaya, Walter H. L., Graham, Mark S., Gray, Robert, Da Costa, Pedro F, Tudosiu, Petru-Daniel, Wright, Paul, Mah, Yee H., MacKinnon, Andrew D., Teo, James T., Jager, Rolf, Werring, David, Rees, Geraint, Nachev, Parashkev, Ourselin, Sebastien, Cardoso, M. Jorge
Deep generative models have emerged as promising tools for detecting arbitrary anomalies in data, dispensing with the necessity for manual labelling. Recently, autoregressive transformers have achieved state-of-the-art performance for anomaly detecti
Externí odkaz:
http://arxiv.org/abs/2206.03461
Autor:
Barfety, Capucine, Valin, Félix-Antoine, Webb, Tracy M. A., Yun, Min, Shipley, Heath, Boone, Kyle, Hayden, Brian, Hlavacek-Larrondo, Julie, Muzzin, Adam, Noble, Allison G., Perlmutter, Saul, Rhea, Carter, Wilson, Gillian, Yee, H. K. C
The formation of the stellar mass within galaxy cluster cores is a poorly understood process. It features the complicated physics of cooling flows, AGN feedback, star formation and more. Here, we study the growth of the stellar mass in the vicinity o
Externí odkaz:
http://arxiv.org/abs/2203.13764
Autor:
Ebenezer S. Nyadjro, Jennifer A. B. Webster, Tim P. Boyer, Just Cebrian, Leonard Collazo, Gunnar Kaltenberger, Kirsten Larsen, Yee H. Lau, Paul Mickle, Tiffany Toft, Zhankun Wang
Publikováno v:
Scientific Data, Vol 10, Iss 1, Pp 1-12 (2023)
Abstract Microplastics (
Externí odkaz:
https://doaj.org/article/0d8fc9c613f247128a65e0e00a82bfdc
Autor:
Biviano, A., van der Burg, R. F. J., Balogh, M. L., Munari, E., Cooper, M. C., De Lucia, G., Demarco, R., Jablonka, P., Muzzin, A., Nantais, J., Old, L. J., Rudnick, G., Vulcani, B., Wilson, G., Yee, H. K. C., Zaritsky, D., Cerulo, P., Chan, J., Finoguenov, A., Gilbank, D., Lidman, C., Pintos-Castro, I., Shipley, H.
Publikováno v:
A&A 650, A105 (2021)
We aim to determine the mass, velocity anisotropy, and pseudo phase-space density profiles (M(r), beta(r), and Q(r), respectively) of clusters of galaxies at the highest redshifts investigated in detail so far. We combine the GOGREEN and GCLASS spect
Externí odkaz:
http://arxiv.org/abs/2104.01183
Autor:
Dunne, Delaney A., Webb, Tracy M. A., Noble, Allison, Lidman, Christopher, Shipley, Heath, Muzzin, Adam, Wilson, Gillian, Yee, H. K. C.
We present ALMA CO (2-1) detections of 24 star-forming Brightest Cluster Galaxies (BCGs) over $0.2
Externí odkaz:
http://arxiv.org/abs/2103.02463