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I will introduce our works on probing high-z emission-line galaxies (ELGs) through deep narrow-band surveys.We obtained our deep Near-infrared and optical narrow-band imaging data through CFHT/WIRCam
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I will introduce our works on probing high-z emission-line galaxies (ELGs) through deep narrow-band surveys.We obtained our deep Near-infrared and optical narrow-band imaging data through CFHT/WIRCam and Magellan/Megacam respectively.We identified the samples of Hα and Lyman-α ELGs at z=2.24 in the Extended Chandra Deep Field South based on the data from this two narrow-bands.I will present the results from two works of ours:one on the properties of these high-z ELGs,such as stellar mass,extinction,SFR,luminosity function,etc.,and the other on the Lyman-α escape fraction of star-forming galaxies at this redshift.
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