Zobrazeno 1 - 10
of 51
pro vyhledávání: '"Blyth, Sarah"'
Autor:
Glowacki, Marcin, Collier, Jordan D., Kazemi-Moridani, Amir, Frank, Bradley, Roberts, Hayley, Darling, Jeremy, Klöckner, Hans-Rainer, Adams, Nathan, Baker, Andrew J., Bershady, Matthew, Blecher, Tariq, Blyth, Sarah-Louise, Bowler, Rebecca, Catinella, Barbara, Chemin, Laurent, Crawford, Steven M., Cress, Catherine, Davé, Romeel, Deane, Roger, de Blok, Erwin, Delhaize, Jacinta, Duncan, Kenneth, Elson, Ed, February, Sean, Gawiser, Eric, Hatfield, Peter, Healy, Julia, Henning, Patricia, Hess, Kelley M., Heywood, Ian, Holwerda, Benne W., Hoosain, Munira, Hughes, John P., Hutchens, Zackary L., Jarvis, Matt, Kannappan, Sheila, Katz, Neal, Kereš, Dušan, Korsaga, Marie, Kraan-Korteweg, Renée C., Lah, Philip, Lochner, Michelle, Maddox, Natasha, Makhathini, Sphesihle, Meurer, Gerhardt R., Meyer, Martin, Obreschkow, Danail, Oh, Se-Heon, Oosterloo, Tom, Oppor, Joshua, Pan, Hengxing, Pisano, D. J., Randriamiarinarivo, Nandrianina, Ravindranath, Swara, Schröder, Anja C., Skelton, Rosalind, Smirnov, Oleg, Smith, Mathew, Somerville, Rachel S., Srianand, Raghunathan, Staveley-Smith, Lister, Tanaka, Masayuki, Vaccari, Mattia, van Driel, Wim, Verheijen, Marc, Walter, Fabian, Wu, John F., Zwaan, Martin A.
In the local Universe, OH megamasers (OHMs) are detected almost exclusively in infrared-luminous galaxies, with a prevalence that increases with IR luminosity, suggesting that they trace gas-rich galaxy mergers. Given the proximity of the rest freque
Externí odkaz:
http://arxiv.org/abs/2204.02523
Autor:
Ramraj, Riona, Gilbank, David G., Blyth, Sarah-Louise, Skelton, Rosalind E., Glazebrook, Karl, Bower, Richard G., Balogh, Michael L.
We present measurements of star formation rates (SFRs) for dwarf galaxies (M*~10^8.5 Msun ) at z~1 using near-infrared slitless spectroscopy from the Hubble Space Telescope (HST) by targetting and measuring the luminosity of the H{\alpha} emission li
Externí odkaz:
http://arxiv.org/abs/1612.06082
Akademický článek
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Autor:
Blyth, Sarah-Louise
Includes bibliographical references.
This thesis presents first results on jet reconstruction in simulated Pb+Pb collisions using the ALICE detectors and a UAl-based cone jet finding algorithm which has been modified and optimised to reconstruct
This thesis presents first results on jet reconstruction in simulated Pb+Pb collisions using the ALICE detectors and a UAl-based cone jet finding algorithm which has been modified and optimised to reconstruct
Externí odkaz:
http://hdl.handle.net/11427/10168
Publikováno v:
Phys. Rev. ST Phys. Educ. Res. 10, 020126 (2014)
We report on research carried out to improve teaching and student engagement in the introductory astronomy course at the University of Cape Town. This course is taken by a diverse range of students, including many from educationally disadvantaged bac
Externí odkaz:
http://arxiv.org/abs/1409.2363
Publikováno v:
Canadian Journal of Public Health / Revue Canadienne de Santé Publique, 2018 Apr 01. 109(2), 231-232.
Externí odkaz:
https://www.jstor.org/stable/27173283
Autor:
Blyth, Sarah-Louise
Publikováno v:
J.Phys.G34:S933-936,2007
We present the centrality dependence of the $N(\Omega)/N(\phi)$ ratios and $\phi$ $v_{2}$ measured in Au+Au collisions at $\sqrt{s_{NN}}=200$ GeV by the STAR experiment at RHIC. The results are compared to measurements of other identified particles a
Externí odkaz:
http://arxiv.org/abs/nucl-ex/0701052
Autor:
Blyth, Sarah-Louise
Publikováno v:
J.Phys. G32 (2006) S461-S464
We present the first elliptic flow, $v_{2}$, measurement for the $\phi$-meson in Au+Au collisions at $\sqrt{s_{NN}}$=200 GeV. At low $p_{T}$ (<2 GeV/c), the $v_{2}$ is consistent with mass ordering expected from hydrodynamics, while at higher $p_{T}$
Externí odkaz:
http://arxiv.org/abs/nucl-ex/0608019
Autor:
Blyth, Sarah-Louise
In ultra-relativistic heavy-ion collisions at $\sqrt{s_{NN}}$ = 5.5 TeV at the ALICE experiment at the LHC, interactions between the high-$p_{T}$ partons and the hot, dense medium produced in the collisions, are expected to lead to jet energy loss (j
Externí odkaz:
http://arxiv.org/abs/nucl-ex/0510065
Autor:
Duncan, Kenneth, Baker, Andrew, Best, Philip, Blyth, Sarah, Hatch, Nina, Holwerda, Benne, Jarvis, Matt, Maddox, Natasha, Smith, Daniel J. B., Arnaudova, Marina, Chemin, Laurent, Davé, Romeel, Dunlop, James, Frank, Bradley, Gawiser, Eric, Gloudemans, Anniek, Hale, Catherine, Heywood, Ian, Kannappan, Sheila, Kondapally, Rohit, McLure, Ross, Morabito, Leah, Nesvadba, Nicole, Pan, Hengxing, Ponomareva, Anastasia, Prescott, Matt, Roberts, Hayley, Röttgering, Huub, Somerville, Rachel, Tudorache, Madalina, Vaccari, Mattia, Whittam, Imogen, Wu, John, Zwaan, Martin
Publikováno v:
Duncan, K, Baker, A, Best, P, Blyth, S, Hatch, N, Holwerda, B, Jarvis, M, Maddox, N, Smith, D J B, Arnaudova, M, Chemin, L, Davé, R, Dunlop, J, Frank, B, Gawiser, E, Gloudemans, A, Hale, C, Heywood, I, Kannappan, S, Kondapally, R, McLure, R, Morabito, L, Nesvadba, N, Pan, H, Ponomareva, A, Prescott, M, Roberts, H, Rottgering, H, Somerville, R, Tudorache, M, Whittam, I, Wu, J & Zwaan, M 2023, ' Optical, Radio Continuum and HI Deep Spectroscopic Survey (ORCHIDSS) ', The Messenger, vol. 190, no. 2023, pp. 25-27 . https://doi.org/10.18727/0722-6691/5306
Galaxy evolution is regulated by the continuous cycle of gas accretion, consumption and feedback. Crucial in this cycle is the availability of neutral atomic (HI) and molecular hydrogen. Our current inventory of HI, however, is very limited beyond th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9f4c8e97d1e5e6473b9548597d07ad24
https://www.pure.ed.ac.uk/ws/files/348582830/messenger_no190_25_27.pdf
https://www.pure.ed.ac.uk/ws/files/348582830/messenger_no190_25_27.pdf