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The average dust attenuation curve at z ∼ 1.3 based on HST grism surveys
UploadSpectroscopically Identified Emission Line Galaxy Pairs in the WISP Survey*
Download from doi.orgCoevolution of black hole accretion and star formation in galaxies up to z = 3.5
UploadActive Galactic Nuclei in Dusty Starbursts at z = 2: Feedback Still to Kick in
UploadA High Space Density of Luminous Lyα Emitters at z ∼ 6.5
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