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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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 Više autora...

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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, br. 2, 2021, str. 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, br. 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), str. 1701-1732. doi: 10.1093/mnras/staa2330

Okabe N, Dicker S, Eckert D, Mroczkowski T, Gastaldello F, Lin YT, i 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. [pristupljeno 30.09.2024.];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, br. 2, str. 1701-1732, 2021. [Online]. Dostupno na: https://urn.nsk.hr/urn:nbn:hr:217:984088. [Citirano: 30.09.2024.]

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Naslov (engleski)Active gas features in three HSC-SSP CAMIRA clusters revealed by high angular resolution analysis of MUSTANG-2 SZE and XXL X-ray observations
AutorNobuhiro Okabe
AutorSimon Dicker
AutorDominique Eckert
AutorTony Mroczkowski
AutorFabio Gastaldello
AutorYen-Ting Lin
AutorMark Devlin
AutorCharles E Romero
AutorMark Birkinshaw
AutorCraig Sarazin
AutorCathy Horellou
AutorTetsu Kitayama
AutorKeiichi Umetsu
AutorMauro Sereno
AutorBrian S Mason
AutorJohn A ZuHone
AutorAyaka Honda
AutorHiroki Akamatsu
AutorI-Non Chiu
AutorKotaro Kohno
AutorKai-Yang Lin
AutorElinor Medezinski
AutorSatoshi Miyazaki
AutorIkuyuki Mitsuishi
AutorAtsushi J Nishizawa
AutorMasamune Oguri
AutorNaomi Ota
AutorFlorian Pacaud
AutorMarguerite Pierre
AutorJonathan Sievers
AutorVernesa Smolčić
AutorSara Stanchfield
AutorKeigo Tanaka
AutorRyoichi Yamamoto
AutorChong Yang
AutorAtsushi Yoshida
Autorova ustanovaSveučilište u Zagrebu
Prirodoslovno-matematički fakultet
(Fizički odsjek)
Znanstveno / umjetničko
područje, polje i grana		PRIRODNE ZNANOSTI
Fizika
Sažetak (engleski)
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.
Ključne riječi (engleski)
Jezikengleski
Vrsta publikacijeZnanstveni rad - Izvorni znanstveni rad
Status objaveObjavljen
Vrsta recenzijeRecenziran - međunarodna recenzija
Verzija publikacijeObjavljena verzija rada (izdavačev PDF)
Naslov časopisaMonthly Notices of the Royal Astronomical Society
Brojčani podacivol. 501, br. 2, str. 1701-1732
p-ISSN0035-8711
e-ISSN1365-2966
DOIhttps://doi.org/10.1093/mnras/staa2330
URN:NBNurn:nbn:hr:217:984088
Datum objave publikacije2021
URL dokumentahttps://academic.oup.com/mnras/article/501/2/1701/5903293
Vrsta resursaTekst
Prava pristupaOtvoreni pristup
Uvjeti korištenjaIkona licence Zaštićeno autorskim pravom.
Javna napomena© 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.
Datum i vrijeme pohrane2024-09-29 11:12:48