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    SPT-selected protoclusters and the early emergence of the hot intracluster gas

    发布日期:2026-05-07

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    标题:SPT-selected protoclusters and the early emergence of the hot intracluster gas

    时间:2026-05-12, 10:00

    主讲人:Dazhi Zhou (UBC)

    地点:Physics Building E225

    报告语言:English

    主讲人 Dazhi Zhou (UBC) 地点 Physics Building E225
    时间 2026-05-12, 10:00 报告语言 English
    办公室

    The South Pole Telescope (SPT) has discovered a large sample of millimetre point sources in the 2500 deg^2 SPT-SZ survey. Follow-up observations with ALMA show that about 90% of these sources are strongly lensed dusty star-forming galaxies (DSFGs), while the remaining ~10% are compact groups of DSFGs at z~3-7, representing protocluster cores caught during their most intense phase of star formation. These systems are ideal laboratories for studying how intracluster gas first emerges and interacts with extreme star formation and AGN activity.

    In this talk, I will introduce the SPT-selected protocluster sample and highlight our recent ALMA detection of hot intracluster gas at z=4.3 via the thermal Sunyaev–Zeldovich effect. I will discuss its implications and briefly outline future prospects for high-redshift ICM studies, including opportunities with the upcoming facilities such as ALMA Wideband Sensitivity Upgrade (WSU), ngVLA, Athena, and Lynx.

    BIO

    Dazhi Zhou is a PhD student at the University of British Columbia in Canada. His research is mainly focused on galaxy evolution and cluster formation at high redshift, especially the interplay between galaxies and their cluster-scale environment, using multi-wavelength observations from ALMA, JWST, HST, and other facilities.

    Host: Zhijie Qu

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