Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Wan, Jenny T"'
Autor:
Machacek, Marie E., Jones, Christine, Kraft, Ralph P., Forman, William R., Roediger, Elke, Sheardown, Alex, Wan, Jenny T.
Publikováno v:
The Astrophysical Journal, 958, (2023), 93
Analyses of major group mergers are key to understanding the evolution of large-scale structure in the Universe and the microphysical properties of the hot gas in these systems. We present imaging and spectral analyses of deep Chandra observations of
Externí odkaz:
http://arxiv.org/abs/2410.06196
Autor:
Turner, Crispin, Tacchella, Sandro, D'Eugenio, Francesco, Carniani, Stefano, Curti, Mirko, Glazebrook, Karl, Johnson, Benjamin D., Lim, Seunghwan, Looser, Tobias, Maiolino, Roberto, Nanayakkara, Themiya, Wan, Jenny T.
We present a detailed analysis of JWST/NIRSpec and NIRCam observations of ZF-UDS-7329, a massive, quiescent galaxy at redshift $z=3.2$, which has been put forward to challenge cosmology and galaxy formation physics. Our study extends previous works b
Externí odkaz:
http://arxiv.org/abs/2410.05377
Autor:
Wan, Jenny T., Tacchella, Sandro, Johnson, Benjamin D., Iyer, Kartheik G., Speagle, Joshua S., Maiolino, Roberto
The amount of power contained in the variations in galaxy star-formation histories (SFHs) across a range of timescales encodes key information about the physical processes which modulate star formation. Modelling the SFHs of galaxies as stochastic pr
Externí odkaz:
http://arxiv.org/abs/2404.14494
Autor:
Sayers, Jack, Mantz, Adam B., Rasia, Elena, Allen, Steven W., Cui, Weiguang, Golwala, Sunil R., Morris, R. Glenn, Wan, Jenny T.
We have combined X-ray observations from Chandra with Sunyaev-Zel'dovich (SZ) effect data from Planck and Bolocam to measure intra-cluster medium pressure profiles from 0.03R$_{500}$ $\le$ R $\le$ 5R$_{500}$ for a sample of 21 low-$z$ galaxy clusters
Externí odkaz:
http://arxiv.org/abs/2206.00091
Autor:
Wan, Jenny T., Mantz, Adam B., Sayers, Jack, Allen, Steven W., Morris, R. Glenn, Golwala, Sunil R.
We use a sample of 14 massive, dynamically relaxed galaxy clusters to constrain the Hubble Constant, $H_0$, by combining X-ray and Sunyaev-Zel'dovich (SZ) effect signals measured with Chandra, Planck and Bolocam. This is the first such analysis to ma
Externí odkaz:
http://arxiv.org/abs/2101.09389
Autor:
Wan, Jenny T, Tacchella, Sandro, Johnson, Benjamin D, Iyer, Kartheik G, (沈佳士), Joshua S Speagle, Maiolino, Roberto
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Aug2024, Vol. 532 Issue 4, p4002-4025, 24p
Autor:
Wan, Jenny T., Mantz, Adam B., Sayers, Jack, Allen, Steven W., Morris, R. Glenn, Golwala, Sunil R.
We use a sample of 14 massive, dynamically relaxed galaxy clusters to constrain the Hubble constant, H₀, by combining X-ray and Sunyaev–Zel’dovich (SZ) effect signals measured with Chandra, Planck, and Bolocam. This is the first such analysis t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od________38::bf7f3ea31b05a3ceb27422d13c03df5c
https://resolver.caltech.edu/CaltechAUTHORS:20210331-083800968
https://resolver.caltech.edu/CaltechAUTHORS:20210331-083800968