prikaz prve stranice dokumenta Active gas features in three HSC-SSP CAMIRA clusters revealed by high angular resolution analysis of MUSTANG-2 SZE and XXL X-ray observations
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Scientific paper - Original scientific paper
Active gas features in three HSC-SSP CAMIRA clusters revealed by high angular resolution analysis of MUSTANG-2 SZE and XXL X-ray observations
Monthly Notices of the Royal Astronomical Society, 501 (2021), 2; 1701-1732. https://doi.org/10.1093/mnras/staa2330
Okabe, Nobuhiro; Dicker, Simon; Eckert, Dominique; Mroczkowski, Tony; Gastaldello, Fabio; Lin, Yen-Ting; Devlin, Mark; Romero, Charles E; Birkinshaw, Mark; Sarazin, Craig; Horellou, Cathy; Kitayama, Tetsu; Umetsu, Keiichi; Sereno, Mauro; Mason, Brian S; ZuHone, John A; Honda, Ayaka; Akamatsu, Hiroki; Chiu, I-Non; Kohno, Kotaro; Lin, Kai-Yang; Medezinski, Elinor; Miyazaki, Satoshi; Mitsuishi, Ikuyuki; Nishizawa, Atsushi J; Oguri, Masamune; Ota, Naomi; Pacaud, Florian; Pierre, Marguerite; Sievers, Jonathan; Smolčić, Vernesa; Stanchfield, Sara; Tanaka, Keigo; Yamamoto, Ryoichi; Yang, Chong; Yoshida, Atsushi More authors...

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Okabe, N., Dicker, S., Eckert, D., Mroczkowski, T., Gastaldello, F., Lin, Y. T. ... Yoshida, A. (2021). Active gas features in three HSC-SSP CAMIRA clusters revealed by high angular resolution analysis of MUSTANG-2 SZE and XXL X-ray observations. Monthly Notices of the Royal Astronomical Society, 501. (2), 1701-1732. doi: 10.1093/mnras/staa2330

Okabe, Nobuhiro, et al. "Active gas features in three HSC-SSP CAMIRA clusters revealed by high angular resolution analysis of MUSTANG-2 SZE and XXL X-ray observations." Monthly Notices of the Royal Astronomical Society, vol. 501, no. 2, 2021, pp. 1701-1732. https://doi.org/10.1093/mnras/staa2330

Okabe, Nobuhiro, Simon Dicker, Dominique Eckert, Tony Mroczkowski, Fabio Gastaldello, Yen Ting Lin, Mark Devlin, et al. "Active gas features in three HSC-SSP CAMIRA clusters revealed by high angular resolution analysis of MUSTANG-2 SZE and XXL X-ray observations." Monthly Notices of the Royal Astronomical Society 501, no. 2 (2021): 1701-1732. https://doi.org/10.1093/mnras/staa2330

Okabe, N., et al. (2021) 'Active gas features in three HSC-SSP CAMIRA clusters revealed by high angular resolution analysis of MUSTANG-2 SZE and XXL X-ray observations', Monthly Notices of the Royal Astronomical Society, 501(2), pp. 1701-1732. doi: 10.1093/mnras/staa2330

Okabe N, Dicker S, Eckert D, Mroczkowski T, Gastaldello F, Lin YT, and sur.. Active gas features in three HSC-SSP CAMIRA clusters revealed by high angular resolution analysis of MUSTANG-2 SZE and XXL X-ray observations. Monthly Notices of the Royal Astronomical Society [Internet]. 2021 [cited 2024 December 19];501(2):1701-1732. doi: 10.1093/mnras/staa2330

N. Okabe, et al., "Active gas features in three HSC-SSP CAMIRA clusters revealed by high angular resolution analysis of MUSTANG-2 SZE and XXL X-ray observations", Monthly Notices of the Royal Astronomical Society, vol. 501, no. 2, pp. 1701-1732, 2021. [Online]. Available at: https://urn.nsk.hr/urn:nbn:hr:217:984088. [Accessed: 19 December 2024]

Metadata
Title (english)Active gas features in three HSC-SSP CAMIRA clusters revealed by high angular resolution analysis of MUSTANG-2 SZE and XXL X-ray observations
AuthorNobuhiro Okabe
AuthorSimon Dicker
AuthorDominique Eckert
AuthorTony Mroczkowski
AuthorFabio Gastaldello
AuthorYen-Ting Lin
AuthorMark Devlin
AuthorCharles E Romero
AuthorMark Birkinshaw
AuthorCraig Sarazin
AuthorCathy Horellou
AuthorTetsu Kitayama
AuthorKeiichi Umetsu
AuthorMauro Sereno
AuthorBrian S Mason
AuthorJohn A ZuHone
AuthorAyaka Honda
AuthorHiroki Akamatsu
AuthorI-Non Chiu
AuthorKotaro Kohno
AuthorKai-Yang Lin
AuthorElinor Medezinski
AuthorSatoshi Miyazaki
AuthorIkuyuki Mitsuishi
AuthorAtsushi J Nishizawa
AuthorMasamune Oguri
AuthorNaomi Ota
AuthorFlorian Pacaud
AuthorMarguerite Pierre
AuthorJonathan Sievers
AuthorVernesa Smolčić
AuthorSara Stanchfield
AuthorKeigo Tanaka
AuthorRyoichi Yamamoto
AuthorChong Yang
AuthorAtsushi Yoshida
Author's institutionUniversity of Zagreb
Faculty of Science
(Department of Physics)
Scientific / art field,
discipline and subdiscipline		NATURAL SCIENCES
Physics
Abstract (english)
We present results from simultaneous modelling of high angular resolution GBT/MUSTANG-2 90 GHz Sunyaev–Zel’dovich effect (SZE) measurements and XMM-XXL X-ray images of three rich galaxy clusters selected from the HSC-SSP Survey. The combination of high angular resolution SZE and X-ray imaging enables a spatially resolved multicomponent analysis, which is crucial to understand complex distributions of cluster gas properties. The targeted clusters have similar optical richnesses and redshifts, but exhibit different dynamical states in their member galaxy distributions: a single-peaked cluster, a double-peaked cluster, and a cluster belonging to a supercluster. A large-scale residual pattern in both regular Compton-parameter y and X-ray surface brightness distributions is found in the single-peaked cluster, indicating a sloshing mode. The double-peaked cluster shows an X-ray remnant cool core between two SZE peaks associated with galaxy concentrations. The temperatures of the two peaks reach ∼20–30 keV in contrast to the cool core component of ∼2 keV, indicating a violent merger. The main SZE signal for the supercluster is elongated along a direction perpendicular to the major axis of the X-ray core, suggesting a minor merger before core passage. The SX and y distributions are thus perturbed at some level, regardless of the optical properties. We find that the integrated Compton y parameter and the temperature for the major merger are boosted from those expected by the weak-lensing mass and those for the other two clusters show no significant deviations, which is consistent with predictions of numerical simulations.
Keywords (english)
Languageenglish
Publication typeScientific paper - Original scientific paper
Publication statusPublished
Peer reviewPeer review - international
Publication versionPublished version
Journal titleMonthly Notices of the Royal Astronomical Society
Numberingvol. 501, no. 2, pp. 1701-1732
p-ISSN0035-8711
e-ISSN1365-2966
DOIhttps://doi.org/10.1093/mnras/staa2330
URN:NBNurn:nbn:hr:217:984088
Publication2021
Document URLhttps://academic.oup.com/mnras/article/501/2/1701/5903293
Type of resourceText
Access conditionsOpen access
Terms of useLicence In copyright icon
Public note© 2020 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. Accepted 2020 July 31. Received 2020 July 30; in original form 2019 November 21.
Created on2024-09-29 11:12:48