Zobrazeno 1 - 10
of 162
pro vyhledávání: '"Pauline Barmby"'
Autor:
Callum Dewsnap, Pauline Barmby, Sarah C. Gallagher, C. Megan Urry, Aritra Ghosh, Meredith C. Powell
Publikováno v:
The Astrophysical Journal, Vol 944, Iss 2, p 137 (2023)
The COSMOS field has been extensively observed by most major telescopes, including Chandra, HST, and Subaru. HST imaging boasts very high spatial resolution and is used extensively in morphological studies of distant galaxies. Subaru provides lower s
Externí odkaz:
https://doaj.org/article/9f9071b96e794060ab4df66585a080ec
Autor:
Pauline Barmby
Publikováno v:
The Open Journal of Astrophysics, Vol 2 (2019)
Observational astrophysics uses sophisticated technology to collect and measure electromagnetic and other radiation from beyond the Earth. Modern observatories produce large, complex datasets and extracting the maximum possible information from them
Externí odkaz:
https://doaj.org/article/7b570ed1f2c04a7fa31c46086d43e088
Autor:
Edmund M Hart, Pauline Barmby, David LeBauer, François Michonneau, Sarah Mount, Patrick Mulrooney, Timothée Poisot, Kara H Woo, Naupaka B Zimmerman, Jeffrey W Hollister
Publikováno v:
PLoS Computational Biology, Vol 12, Iss 10, p e1005097 (2016)
Externí odkaz:
https://doaj.org/article/0f414210ec9441a1a3d58ffb328983e8
Autor:
Pauline Barmby, Samantha Wong
Publikováno v:
Studies in Big Data ISBN: 9783031299360
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3954c6ecfc776d5b4c998b2c18bdbbe6
https://doi.org/10.1007/978-3-031-29937-7_2
https://doi.org/10.1007/978-3-031-29937-7_2
Automating classification of galaxy components is important for understanding the formation and evolution of galaxies. Traditionally, only the larger galaxy structures such as the spiral arms, bulge, and disc are classified. Here we use machine learn
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::53a8b53e09a201ebf2c2923e89eeb556
http://arxiv.org/abs/2205.04374
http://arxiv.org/abs/2205.04374
Publikováno v:
Physics and Astronomy Publications
Precise and accurate measurements of distances to Galactic X-ray binaries (XRBs) reduce uncertainties in the determination of XRB physical parameters. We have cross-matched the XRB catalogues of Liu et al. (2006, 2007) to the results of Gaia Data Rel
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2b827bc3dfbbe3527e4a677300a43b4e
https://ir.lib.uwo.ca/physicspub/80
https://ir.lib.uwo.ca/physicspub/80
Autor:
Christopher J. R. Clark, Walter Kieran Gear, Sarah Ragan, Pauline Barmby, Gayathri Athikkat-Eknath, Scott Chapman, Mark G. Rawlings, Matthew W. L. Smith, En-Tzu Lin, Xindi Tang, Francisca Kemper, Thomas G. Williams, Haley Louise Gomez, Sihan Jiao, Zongnan Li, Ilse De Looze, Eun Jung Chung, Brian Cho, Jinhua He, Junfeng Wang, C. D. Wilson, Richard de Grijs, Dimitra Rigopoulou, Anthony Peter Whitworth, Albert K. H. Kong, David L. Clements, Eric W. Koch, Hui-Hsuan Chung, Luis C. Ho, Kate Pattle, Steve Mairs, Chien-Hsiu Lee, Andreas Schruba, Martin Bureau, G. P. Ford, Stephen Anthony Eales, T. M. Hughes, Bumhyun Lee, Aeree Chung, Michał J. Michałowski, Timothy A. Davis, Yingjie Peng, David Eden, Amélie Saintonge, Ming Zhu, Florian Kirchschlager, Yu Gao, Kijeong Yim, Zhiyuan Li
Publikováno v:
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
The Astrophysical Journal Supplement Series
Physics and Astronomy Publications
Astrophysical Journal Supplement Series
The Astrophysical Journal Supplement Series
Physics and Astronomy Publications
Astrophysical Journal Supplement Series
Observing nearby galaxies with submillimeter telescopes on the ground has two major challenges. First, the brightness is significantly reduced at long submillimeter wavelengths compared to the brightness at the peak of the dust emission. Second, it i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2bf10b2300c8a9397569ba9ac619bb3e
https://hdl.handle.net/1854/LU-8745310
https://hdl.handle.net/1854/LU-8745310
Autor:
Pauline Barmby, Mark Gorski
Publikováno v:
Physics and Astronomy Publications
It is imperative to map the strength and distribution of feedback in galaxies to understand how feedback affects the galactic ecosystems. H$_2$O masers act as indicators of energy injection into the ISM. Our goal is to measure the strength and distri
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5dd6d37780a0a7f3e04b84f774fcbcca
http://arxiv.org/abs/2005.04121
http://arxiv.org/abs/2005.04121
Autor:
Pauline Barmby, Dayi Li
Publikováno v:
Physics and Astronomy Publications
We demonstrate the power of Gibbs point process models from the spatial statistics literature when applied to studies of resolved galaxies. We conduct a rigorous analysis of the spatial distributions of objects in the star formation complexes of M33,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1bf5faf2b058832a0b2644424958ad2a