Search Results - "Bowler, R."

Normal, dust-obscured galaxies in the epoch of reionization by Fudamoto, Y., Oesch, P. A., Schouws, S., Stefanon, M., Smit, R., Bouwens, R. J., Bowler, R. A. A., Endsley, R., Gonzalez, V., Inami, H., Labbe, I., Stark, D., Aravena, M., Barrufet, L., da Cunha, E., Dayal, P., Ferrara, A., Graziani, L., Hodge, J., Hutter, A., Li, Y., De Looze, I., Nanayakkara, T., Pallottini, A., Riechers, D., Schneider, R., Ucci, G., van der Werf, P., White, C.

“…Over the past decades, rest-frame ultraviolet (UV) observations have provided large samples of UV luminous galaxies at redshift ( z ) greater than 6 (refs. 1 –…”
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A lack of evolution in the very bright end of the galaxy luminosity function from z ≃ 8 to 10 by Bowler, R A A, Jarvis, M J, Dunlop, J S, McLure, R J, McLeod, D J, Adams, N J, Milvang-Jensen, B, McCracken, H J

“…ABSTRACT We utilize deep near-infrared survey data from the UltraVISTA fourth data release (DR4) and the VIDEO survey, in combination with overlapping optical…”
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Unveiling the nature of bright z ≃ 7 galaxies with the Hubble Space Telescope by Bowler, R. A. A., Dunlop, J. S., McLure, R. J., McLeod, D. J.

“…Abstract We present new Hubble Space Telescope/Wide Field Camera 3 (HST/WFC3) imaging of 25 extremely luminous (−23.2 ≤ M UV ≲ −21.2) Lyman-break galaxies…”
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The rapid transition from star formation to AGN-dominated rest-frame ultraviolet light at z ≃ 4 by Bowler, R A A, Adams, N J, Jarvis, M J, Häußler, B

“…ABSTRACT With the advent of deep optical-to-near-infrared extragalactic imaging on the degree scale, samples of high-redshift sources are being selected that…”
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Chemical accuracy for the van der Waals density functional by Klimeš, Jiří, Bowler, David R, Michaelides, Angelos

“…The non-local van der Waals density functional (vdW-DF) of Dion et al (2004 Phys. Rev. Lett. 92 246401) is a very promising scheme for the efficient treatment…”
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The evolution of the galaxy UV luminosity function at redshifts z ≃ 8 – 15 from deep JWST and ground-based near-infrared imaging by Donnan, C T, McLeod, D J, Dunlop, J S, McLure, R J, Carnall, A C, Begley, R, Cullen, F, Hamadouche, M L, Bowler, R A A, Magee, D, McCracken, H J, Milvang-Jensen, B, Moneti, A, Targett, T

“…ABSTRACT We reduce and analyse the available JWST ERO and ERS NIRCam imaging (SMACS0723, GLASS, CEERS) in combination with the latest deep ground-based…”
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Reionization Era Bright Emission Line Survey: Selection and Characterization of Luminous Interstellar Medium Reservoirs in the z > 6.5 Universe by Bouwens, R. J., Smit, R., Schouws, S., Stefanon, M., Bowler, R., Endsley, R., Gonzalez, V., Inami, H., Stark, D., Oesch, P., Hodge, J., Aravena, M., da Cunha, E., Dayal, P., Looze, I. de, Ferrara, A., Fudamoto, Y., Graziani, L., Li, C., Nanayakkara, T., Pallottini, A., Schneider, R., Sommovigo, L., Topping, M., van der Werf, P., Algera, H., Barrufet, L., Hygate, A., Labbé, I., Riechers, D., Witstok, J.

“…Abstract The Reionization Era Bright Emission Line Survey (REBELS) is a cycle-7 ALMA Large Program (LP) that is identifying and performing a first…”
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The ultraviolet continuum slopes (β) of galaxies at z ≃ 8-16 from JWST and ground-based near-infrared imaging by Cullen, Fergus, McLure, R J, McLeod, D J, Dunlop, J S, Donnan, C T, Carnall, A C, Bowler, R A A, Begley, R, Hamadouche, M L, Stanton, T M

“…ABSTRACT We study the rest-frame ultraviolet (UV) continuum slopes (β) of galaxies at redshifts 8 < z < 16 (〈z〉 = 10), using a combination of JWST ERO and ERS…”
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Dissipative production of a maximally entangled steady state of two quantum bits by Lin, Y., Gaebler, J. P., Reiter, F., Tan, T. R., Bowler, R., Sørensen, A. S., Leibfried, D., Wineland, D. J.

“…Engineered dissipation is used to deterministically produce and stabilize entanglement between two trapped-ion quantum bits, independently of their initial…”
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The galaxy luminosity function at z ≃ 6 and evidence for rapid evolution in the bright end from z ≃ 7 to 5 by Bowler, R. A. A., Dunlop, J. S., McLure, R. J., McCracken, H. J., Milvang-Jensen, B., Furusawa, H., Taniguchi, Y., Le Fèvre, O., Fynbo, J. P. U., Jarvis, M. J., Häußler, B.

“…We present the results of a search for bright (−22.7 ≤ M UV ≤ −20.5) Lyman-break galaxies at z ≃ 6 within a total of 1.65 deg2 of imaging in the…”
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Dust attenuation in 2 < z < 3 star-forming galaxies from deep ALMA observations of the Hubble Ultra Deep Field by McLure, R J, Dunlop, J S, Cullen, F, Bourne, N, Best, P N, Khochfar, S, Bowler, R A A, Biggs, A D, Geach, J E, Scott, D, Michałowski, M J, Rujopakarn, W, van Kampen, E, Kirkpatrick, A, Pope, A

“…Abstract We present the results of a new study of the relationship between infrared excess (IRX ≡ LIR/LUV), ultraviolet (UV) spectral slope (β) and stellar…”
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The bright end of the galaxy luminosity function at z≃7: before the onset of mass quenching? by Bowler, R. A. A., Dunlop, J. S., McLure, R. J., Rogers, A. B., McCracken, H. J., Milvang-Jensen, B., Furusawa, H., Fynbo, J. P. U., Taniguchi, Y., Afonso, J., Bremer, M. N., Le Fèvre, O.

“…We present the results of a new search for bright star-forming galaxies at redshift z ... 7 within the UltraVISTA second data release (DR2) and UKIDSS (UKIRT…”
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The discovery of rest-frame UV colour gradients and a diversity of dust morphologies in bright z ≃ 7 Lyman-break galaxies by Bowler, R A A, Cullen, F, McLure, R J, Dunlop, J S, Avison, A

“…ABSTRACT We present deep ALMA dust continuum observations for a sample of luminous (MUV < −22) star-forming galaxies at z ≃ 7. We detect five of the six…”
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Evolution of the galaxy stellar mass function: evidence for an increasing M from z = 2 to the present day by Adams, N J, Bowler, R A A, Jarvis, M J, Häußler, B, Lagos, C D P

“…ABSTRACT Utilizing optical and near-infrared broad-band photometry covering >5 deg2 in two of the most well-studied extragalactic legacy fields (COSMOS and…”
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Gate controlling of quantum interference and direct observation of anti-resonances in single molecule charge transport by Li, Yueqi, Buerkle, Marius, Li, Guangfeng, Rostamian, Ali, Wang, Hui, Wang, Zixiao, Bowler, David R., Miyazaki, Tsuyoshi, Xiang, Limin, Asai, Yoshihiro, Zhou, Gang, Tao, Nongjian

“…Quantum interference can profoundly affect charge transport in single molecules, but experiments can usually measure only the conductance at the Fermi energy…”
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A new multifield determination of the galaxy luminosity function at z = 7-9 incorporating the 2012 Hubble Ultra-Deep Field imaging by McLure, R. J., Dunlop, J. S., Bowler, R. A. A., Curtis-Lake, E., Schenker, M., Ellis, R. S., Robertson, B. E., Koekemoer, A. M., Rogers, A. B., Ono, Y., Ouchi, M., Charlot, S., Wild, V., Stark, D. P., Furlanetto, S. R., Cirasuolo, M., Targett, T. A.

“…We present a new determination of the ultraviolet (UV) galaxy luminosity function (LF) at redshift z 7 and 8, and a first estimate at z 9. An accurate…”
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Coherent diabatic ion transport and separation in a multizone trap array by Bowler, R, Gaebler, J, Lin, Y, Tan, T R, Hanneke, D, Jost, J D, Home, J P, Leibfried, D, Wineland, D J

“…We investigate the dynamics of single and multiple ions during transport between and separation into spatially distinct locations in a multizone linear Paul…”
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MIGHTEE: are giant radio galaxies more common than we thought? by Delhaize, J, Heywood, I, Prescott, M, Jarvis, M J, Delvecchio, I, Whittam, I H, White, S V, Hardcastle, M J, Hale, C L, Afonso, J, Ao, Y, Brienza, M, Brüggen, M, Collier, J D, Daddi, E, Glowacki, M, Maddox, N, Morabito, L K, Prandoni, I, Randriamanakoto, Z, Sekhar, S, An, Fangxia, Adams, N J, Blyth, S, Bowler, R A A, Leeuw, L, Marchetti, L, Randriamampandry, S M, Thorat, K, Seymour, N, Smirnov, O, Taylor, A R, Tasse, C, Vaccari, M

“…ABSTRACT We report the discovery of two new giant radio galaxies (GRGs) using the MeerKAT International GHz Tiered Extragalactic Exploration (MIGHTEE) survey…”
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The rest-frame UV luminosity function at z ≃ 4: a significant contribution of AGNs to the bright end of the galaxy population by Adams, N J, Bowler, R A A, Jarvis, M J, Häußler, B, McLure, R J, Bunker, A, Dunlop, J S, Verma, A

“…ABSTRACT We measure the rest-frame ultraviolet (UV) luminosity function (LF) at z ∼ 4 self-consistently over a wide range in absolute magnitude (−27 ≲ MUV ≲…”
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The total rest-frame UV luminosity function from 3 < z < 5: a simultaneous study of AGN and galaxies from −28 < MUV < −16 by Adams, N J, Bowler, R A A, Jarvis, M J, Varadaraj, R G, Häußler, B

“…ABSTRACT We present measurements of the rest-frame ultraviolet luminosity function (LF) at redshifts z = 3, z = 4, and z = 5, using 96894, 38655, and 7571…”
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