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    Revealing the galaxy intrinsic alignment with self-calibration

    发布日期:2020-04-16

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    标题:Revealing the galaxy intrinsic alignment with self-calibration

    时间: 星期四, 4月 16, 2020, 02:00pm

    主讲人: Prof. Pengjie Zhang (SJTU)

    地点:Online via Zoom

    主讲人  Prof. Pengjie Zhang (SJTU) 地点 Online via Zoom
    时间  星期四, 4月 16, 2020, 02:00pm 报告语言
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    The galaxy intrinsic alignment (IA) is both a major source of systematic errors in weak lensing cosmology, and an emerging tracer of the large scale structure of the Universe. Separating IA from weak lensing (cosmic shear) usually requires a fiducial IA model and is thus IA model-dependent. We have proposed a self-calibration method to avoid this model dependency. Recently we applied it to KIDS450/KV450 and DECaLS DR3. We detected IA at ~20-sigma, without any assumptions of IA. We also detected its dependence on redshift and galaxy type.

    BIO

    Pengjie Zhang is a professor at the Department of Astronomy and an associate fellow at the Tsung-Dao Lee institute, Shanghai Jiao Tong University. He works on the the large scale structure of the universe and its applications in probing fundamental cosmological physics.

    Host: Dandan Xu

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