Zobrazeno 1 - 10
of 3 548
pro vyhledávání: '"Yun, M"'
Beyond the Carnot Limit in the Internal Cycles of a Quantum Heat Engine under Finite Heat Reservoirs
We investigate, in an analytical fashion, quantum Carnot cycles of a microscopic heat engine coupled to two nite heat reservoirs, whose internal cycles could own higher e ciency than the standard Carnot limit without consuming extra quantum resources
Externí odkaz:
http://arxiv.org/abs/2409.00914
Autor:
Polletta, M., Frye, B. L., Garuda, N., Willner, S. P., Berta, S., Kneissl, R., Dole, H., Jansen, R. A., Lehnert, M. D., Cohen, S. H., Summers, J., Windhorst, R. A., D'Silva, J. C. J., Koekemoer, A. M., Coe, D., Conselice, C. J., Driver, S. P., Grogin, N. A., Marshall, M. A., Nonino, M., Ortiz III, R., Pirzkal, N., Robotham, A., Ryan, Jr., R. E., Willmer, C. N. A., Yan, H., Arumugam, V., Cheng, C., Gim, H. B., Hathi, N. P., Holwerda, B., Kamieneski, P., Keel, W. C., Li, J., Pascale, M., Rottgering, H., Smith, B. M., Yun, M. S.
Publikováno v:
A&A 690, A285 (2024)
Dusty star-forming galaxies (DSFGs) contribute significantly to the stellar buildup at cosmic noon. Major mergers and gas accretion are often invoked to explain DSFGs' prodigious star-formation rates (SFRs) and large stellar masses. We conducted a sp
Externí odkaz:
http://arxiv.org/abs/2405.07986
Due to its significant application in reducing algorithm depth, fSim gates have attracted a lot of attention. However, during the implementation of quantum gates, fluctuations in control parameters and decoherence caused by the environment may lead t
Externí odkaz:
http://arxiv.org/abs/2401.02234
Autor:
Calzetti, D., Wilson, G. W., Draine, B. T., Roussel, H., Johnson, K. E., Heyer, M. H., Wall, W. F., Grasha, K., Battisti, A., Andrews, J. E., Kirkpatrick, A., González, D. Rosa, Vega, O., Puschnig, J., Yun, M., Östlin, G., Evans, A. S., Tang, Y., Lowenthal, J., Sánchez-Arguelles, D.
We investigate the relation between gas and star formation in subgalactic regions, similar to 360. pc to similar to 1.5. kpc in size, within the nearby starburst dwarf NGC 4449, in order to separate the underlying relation from the effects of samplin
Externí odkaz:
http://hdl.handle.net/10150/626537
http://arizona.openrepository.com/arizona/handle/10150/626537
http://arizona.openrepository.com/arizona/handle/10150/626537
Autor:
Willner, S. P., Gim, H. B., Polletta, M. del Carmen, Cohen, S. H., Willmer, C. N. A., Zhao, X., D'Silva, J. C. J., Jansen, R. A., Koekemoer, A. M., Summers, J., Windhorst, R. A., Coe, D., Conselice, C. J., Driver, S. P., Frye, B., Grogin, N. A., Marshall, M. A., Nonino, M., Ortiz III, R., Pirzkal, N., Robotham, A., Rutkowski, M. J., Ryan, Jr., R. E., Tompkins, S., Yan, H., Hammel, H. B., Milam, S. N., Adams, N. J., Beacom, J. F., Bhatawdekar, R., Cheng, C., Civano, F., Cotton, W., Hyun, M., Kikuta, S., Nyland, K. E., Peters, W. M., Petric, A., Röttgering, H. J. A., Shimwell, T., Yun, M. S.
The Time Domain Field (TDF) near the North Ecliptic Pole in JWST's continuous-viewing zone will become a premier "blank field" for extragalactic science. JWST/NIRCam data in a 16 arcmin$^2$ portion of the TDF identify 4.4 $\mu$m counterparts for 62 o
Externí odkaz:
http://arxiv.org/abs/2309.13008
Autor:
Roberts-Borsani, G. W., Jiménez-Donaire, M. J., Daprà, M., Alatalo, K., Aretxaga, I., Álvarez-Márquez, J., Baker, A. J., Fujimoto, S., Gallardo, P. A., Gralla, M., Hilton, M., Hughes, J. P., Jiménez, C., Laporte, N., Marriage, T. A., Nati, F., Rivera, J., Sievers, A., Weiß, A., Wilson, G. W., Wollack, E. J., Yun, M. S.
We present CI(2-1) and multi-transition (CO)-C-12 observations of a dusty star-forming galaxy, ACT J2029+0120, which we spectroscopically confirm to lie at z = 2.64. We detect CO(3-2), CO(5-4), CO(7-6), CO(8-7), and CI (2-1) at high significance, ten
Externí odkaz:
http://hdl.handle.net/10150/625330
http://arizona.openrepository.com/arizona/handle/10150/625330
http://arizona.openrepository.com/arizona/handle/10150/625330
Autor:
Dunlop, J. S., McLure, R. J., Biggs, A. D., Geach, J. E., Michałowski, M. J., Ivison, R. J., Rujopakarn, W., van Kampen, E., Kirkpatrick, A., Pope, A., Scott, D., Swinbank, A. M., Targett, T. A., Aretxaga, I., Austermann, J. E., Best, P. N., Bruce, V. A., Chapin, E. L., Charlot, S., Cirasuolo, M., Coppin, K., Ellis, R. S., Finkelstein, S. L., Hayward, C. C., Hughes, D. H., Ibar, E., Jagannathan, P., Khochfar, S., Koprowski, M. P., Narayanan, D., Nyland, K., Papovich, C., Peacock, J. A., Rieke, G. H., Robertson, B., Vernstrom, T., Werf, P. P. van der, Wilson, G. W., Yun, M.
We present the results of the first, deep Atacama Large Millimeter Array ( ALMA) imaging covering the full similar or equal to 4.5 arcmin(2) of the Hubble Ultra Deep Field ( HUDF) imaged with Wide Field Camera 3/IR on HST. Using a 45-pointing mosaic,
Externí odkaz:
http://hdl.handle.net/10150/623849
http://arizona.openrepository.com/arizona/handle/10150/623849
http://arizona.openrepository.com/arizona/handle/10150/623849
Autor:
Polletta, M., Nonino, M., Frye, B., Gargiulo, A., Bisogni, S., Garuda, N., Thompson, D., Lehnert, M., Pascale, M., Willner, S. P., Kamieneski, P., Leimbach, R., Cheng, C., Coe, D., Cohen, S. H., Conselice, C. J., Dai, L., Diego, J., Dole, H., Driver, S. P., D'Silva, J. C. J., Fontana, A., Foo, N., Furtak, L. J., Grogin, N. A., Harrington, K., Hathi, N. P., Jansen, R. A., Kelly, P., Koekemoer, A. M., Mancini, C., Marshall, M. A., Pierel, J. D. R., Pirzkal, N., Robotham, A., Rutkowski, M. J., Ryan, Jr., R. E., Snigula, J. M., Summers, J., Tompkins, S., Willmer, C. N. A., Windhorst, R. A., Yan, H., Yun, M. S., Zitrin, A.
Publikováno v:
A&A 675, L4 (2023)
Supernova (SN) H0pe was discovered as a new transient in James Webb Space Telescope (JWST) NIRCam images of the galaxy cluster PLCK G165.7+67.0 taken as part of the "Prime Extragalactic Areas for Reionization and Lensing Science" (PEARLS) JWST GTO pr
Externí odkaz:
http://arxiv.org/abs/2306.12385
Due to strong zero-phonon line emission, narrow inhomogeneous broadening, and stable optical transition frequencies, the quantum system consisting of negatively charged silicon-vacancy (SiV) centers in diamond is highly expected to develop universal
Externí odkaz:
http://arxiv.org/abs/2303.10053
UV-FIR SED modeling is an effective way to disentangle emission between star formation (SF) and active galactic nuclei (AGN) in galaxies; however, this approach becomes uncertain for composite AGN/SF galaxies that comprise 50-70% of IR-samples. Cosmi
Externí odkaz:
http://arxiv.org/abs/2302.10374