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- W2797727811 abstract "We present a comparison of two samples of z>0.8 galaxy clusters selected using different wavelength-dependent techniques and examine the physical differences between them. We consider 18 clusters from the X-ray selected XMM-LSS distant cluster survey and 92 clusters from the optical-MIR selected SpARCS cluster survey. Both samples are selected from the same approximately 9 square degree sky area and we examine them using common XMM-Newton, Spitzer-SWIRE and CFHT Legacy Survey data. Clusters from each sample are compared employing aperture measures of X-ray and MIR emission. We divide the SpARCS distant cluster sample into three sub-samples: a) X-ray bright, b) X-ray faint, MIR bright, and c) X-ray faint, MIR faint clusters. We determine that X-ray and MIR selected clusters display very similar surface brightness distributions of galaxy MIR light. In addition, the average location and amplitude of the galaxy red sequence as measured from stacked colour histograms is very similar in the X-ray and MIR-selected samples. The sub-sample of X-ray faint, MIR bright clusters displays a distribution of BCG-barycentre position offsets which extends to higher values than all other samples. This observation indicates that such clusters may exist in a more disturbed state compared to the majority of the distant cluster population sampled by XMM-LSS and SpARCS. This conclusion is supported by stacked X-ray images for the X-ray faint, MIR bright cluster sub-sample that display weak, centrally-concentrated X-ray emission, consistent with a population of growing clusters accreting from an extended envelope of material." @default.
- W2797727811 created "2018-04-24" @default.
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- W2797727811 date "2018-04-18" @default.
- W2797727811 modified "2023-10-16" @default.
- W2797727811 title "X-ray versus infrared selection of distant galaxy clusters: a case study using the XMM–LSS and SpARCS cluster samples" @default.
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- W2797727811 cites W1965283242 @default.
- W2797727811 cites W1986299038 @default.
- W2797727811 cites W1986350100 @default.
- W2797727811 cites W1994671833 @default.
- W2797727811 cites W1999468056 @default.
- W2797727811 cites W2003180569 @default.
- W2797727811 cites W2007772592 @default.
- W2797727811 cites W2008548976 @default.
- W2797727811 cites W2017856226 @default.
- W2797727811 cites W2024655466 @default.
- W2797727811 cites W2034287759 @default.
- W2797727811 cites W2039993523 @default.
- W2797727811 cites W2043177648 @default.
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- W2797727811 cites W2121162701 @default.
- W2797727811 cites W2130818124 @default.
- W2797727811 cites W2133390284 @default.
- W2797727811 cites W2138422812 @default.
- W2797727811 cites W2140771927 @default.
- W2797727811 cites W2147854849 @default.
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- W2797727811 cites W2170857649 @default.
- W2797727811 cites W2296455390 @default.
- W2797727811 cites W2337671770 @default.
- W2797727811 cites W2466694234 @default.
- W2797727811 cites W2492665415 @default.
- W2797727811 cites W2511441103 @default.
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- W2797727811 cites W3103277254 @default.
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- W2797727811 cites W3103465215 @default.
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- W2797727811 doi "https://doi.org/10.1093/mnras/sty975" @default.
- W2797727811 hasPublicationYear "2018" @default.
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