Zobrazeno 1 - 10
of 14 683
pro vyhledávání: '"A Telford"'
Autor:
Feuer, Margalit L., Thinel, Morgan, Huang, Xiong, Cui, Zhi-Hao, Shao, Yinming, Kundu, Asish K., Chica, Daniel G., Han, Myung-Geun, Pokratath, Rohan, Telford, Evan J., Cox, Jordan, York, Emma, Okuno, Saya, Huang, Chun-Ying, Bukula, Owethu, Nashabeh, Luca M., Qiu, Siyuan, Nuckolls, Colin P., Dean, Cory R., Billinge, Simon J. L., Zhu, Xiaoyang, Zhu, Yimei, Basov, Dmitri N., Millis, Andrew J., Reichman, David R., Pasupathy, Abhay N., Roy, Xavier, Ziebel, Michael E.
In materials with one-dimensional electronic bands, electron-electron interactions can produce intriguing quantum phenomena, including spin-charge separation and charge density waves (CDW). Most of these systems, however, are non-magnetic, motivating
Externí odkaz:
http://arxiv.org/abs/2412.08631
Autor:
Gómez-González, V. M. A., Oskinova, L. M., Hamann, W. -R., Todt, H., Pauli, D., Serantes, S. Reyero, Bernini-Peron, M., Sander, A. C., Ramachandran, V., Vink, J. S., Crowther, P. A., Berlanas, S. R., ud-Doula, A., Gormaz-Matamala, A. C., Kehrig, C., Kuiper, R., Leitherer, C., Mahy, L., McLeod, A. F., Mehner, A., Morrell, N., Shenar, T., Telford, O. G., van Loon, J. Th., Tramper, F., Wofford, A.
Massive stars lead the ionization and mechanical feedback within young star-forming regions. The Large Magellanic Cloud (LMC) is an ideal galaxy for studying individual massive stars and quantifying their feedback contribution to the environment. We
Externí odkaz:
http://arxiv.org/abs/2411.14149
Autor:
Telford, O. Grace, Sandstrom, Karin M., McQuinn, Kristen B. W., Glover, Simon C. O., Tarantino, Elizabeth J., Bolatto, Alberto D., Vaught, Ryan J. Rickards
The James Webb Space Telescope (JWST) has revealed unexpectedly rapid galaxy assembly in the early universe, in tension with models of star and galaxy formation. In the gas conditions typical of early galaxies, particularly their low abundances of he
Externí odkaz:
http://arxiv.org/abs/2410.21368
The first few cycles of JWST have identified an overabundance of UV-bright galaxies and a general excess of UV luminosity density at $z\gtrsim10$ compared to expectations from most (pre-JWST) theoretical models. Moreover, some of the brightest high-r
Externí odkaz:
http://arxiv.org/abs/2410.14846
Autor:
Cohen, Roger E., McQuinn, Kristen B. W., Murray, Claire E., Williams, Benjamin F., Choi, Yumi, Lindberg, Christina W., Burhenne, Clare, Gordon, Karl D., Merica-Jones, Petia Yanchulova, Bot, Caroline, Dolphin, Andrew E., Gilbert, Karoline M., Goldman, Steven, Hirschauer, Alec S., Sandstrom, Karin M., Telford, O. Grace
The proximity of the Large and Small Magellanic Clouds (LMC and SMC) provides the opportunity to study the impact of dwarf-dwarf interactions on their mass assembly with a unique level of detail. To this end, we analyze two-filter broadband imaging o
Externí odkaz:
http://arxiv.org/abs/2410.11697
Autor:
Cohen, Roger E., McQuinn, Kristen B. W., Murray, Claire E., Williams, Benjamin F., Choi, Yumi, Lindberg, Christina W., Burhenne, Clare, Gordon, Karl D., Merica-Jones, Petia Yanchulova, Gilbert, Karoline M., Boyer, Martha L., Goldman, Steven, Dolphin, Andrew E., Telford, O. Grace
The proximity of the Magellanic Clouds provides the opportunity to study interacting dwarf galaxies near a massive host, and spatial trends in their stellar population properties in particular, with a unique level of detail. The Scylla pure parallel
Externí odkaz:
http://arxiv.org/abs/2410.11696
Autor:
McQuinn, Kristen B. W., Newman, Max J. B., Skillman, Evan D., Telford, O. Grace, Brooks, Alyson, Adams, Elizabeth A. K., Berg, Danielle A., Boyer, Martha L., Cannon, John M., Dolphin, Andrew E., Pahl, Anthony, Rhode, Katherine L., Salzer, John J., Cohen, Roger E., Goldman, Steve R.
Isolated, low-mass galaxies provide the opportunity to assess the impact of reionization on their star formation histories (SFHs) without the ambiguity of environmental processes associated with massive host galaxies. There are very few isolated, low
Externí odkaz:
http://arxiv.org/abs/2409.19050
Autor:
Telford, O. Grace, Chisholm, John, Sander, Andreas A. C., Ramachandran, Varsha, McQuinn, Kristen B. W., Berg, Danielle A.
Metal-poor massive stars drive the evolution of low-mass galaxies, both locally and at high redshift. However, quantifying the feedback they impart to their local surroundings remains uncertain because models of stellar evolution, mass loss, and ioni
Externí odkaz:
http://arxiv.org/abs/2407.20313
Autor:
Rizzo, Daniel J., Seewald, Eric, Zhao, Fangzhou, Cox, Jordan, Xie, Kaichen, Vitalone, Rocco A., Ruta, Francesco L., Chica, Daniel G., Shao, Yinming, Shabani, Sara, Telford, Evan J., Strasbourg, Matthew C., Darlington, Thomas P., Xu, Suheng, Qiu, Siyuan, Devarakonda, Aravind, Taniguchi, Takashi, Watanabe, Kenji, Zhu, Xiaoyang, Schuck, P. James, Dean, Cory R., Roy, Xavier, Millis, Andrew J., Cao, Ting, Rubio, Angel, Pasupathy, Abhay N., Basov, D. N.
Graphene is a privileged 2D platform for hosting confined light-matter excitations known as surface plasmon-polaritons (SPPs), as it possesses low intrinsic losses with a high degree of optical confinement. However, the inherently isotropic optical p
Externí odkaz:
http://arxiv.org/abs/2407.07178
Autor:
Ziffer, Mark E., Machado, Francisco, Ursprung, Benedikt, Lozovoi, Artur, Tazi, Aya Batoul, Yuan, Zhiyang, Ziebel, Michael E., Delord, Tom, Zeng, Nanyu, Telford, Evan, Chica, Daniel G., deQuilettes, Dane W., Zhu, Xiaoyang, Hone, James C., Shepard, Kenneth L., Roy, Xavier, de Leon, Nathalie P., Davis, Emily J., Chatterjee, Shubhayu, Meriles, Carlos A., Owen, Jonathan S., Schuck, P. James, Pasupathy, Abhay N.
Dynamic critical fluctuations in magnetic materials encode important information about magnetic ordering in the associated critical exponents. Using nitrogen-vacancy centers in diamond, we implement $T_2$ (spin-decoherence) noise magnetometry to stud
Externí odkaz:
http://arxiv.org/abs/2407.05614