16 February 2024
Asia/Tokyo timezone

[English] Physical Origin of the Strong [OIII] Emitters with High Equivalent Widths Abundant at High Redshift: Strong Emission lines Boosted by Hidden AGN

16 Feb 2024, 11:43
12m
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https://u-tokyo-ac-jp.zoom.us/j/81774304178

Speaker

ZHU Chenghao

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