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Ali Ahmad Khostovan

University of California, Riverside

36

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2533

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The first blind H-alpha narrow-band survey of star-formation at z>6

2021
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A Lyman-{\alpha} protocluster at redshift 6.9.

2021 arXiv: Astrophysics of Galaxies
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Correlations between H$\alpha$ Equivalent Width and Galaxy Properties at $z = 0.47$: Physical or Selection-driven?

2021 arXiv: Astrophysics of Galaxies
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New spectroscopic confirmations of Lyman-$\alpha$ emitters at z $\sim$ 7 from the LAGER survey

2021 arXiv: Astrophysics of Galaxies
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LAGER Ly$\alpha$ Luminosity Function at $z\sim7$, Implications for Reionization

2021 arXiv: Astrophysics of Galaxies
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The evolution of the UV luminosity and stellar mass functions of Lyman-alpha emitters from z~2 to z~6

2021 arXiv: Astrophysics of Galaxies
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A comprehensive study of H-alpha emitters at z 0.62 in the DAWN survey: the need for deep and wide regions

2020
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A comprehensive study of H$\alpha$ emitters at $z \sim$ 0.62 in the DAWN survey: the need for deep and wide regions.

2020 arXiv: Astrophysics of Galaxies
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The clustering of typical Lyα emitters from z ∼ 2.5 − 6: host halo masses depend on Lyα and UV luminosities

2019 Monthly Notices of the Royal Astronomical Society
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Design for the First Narrowband Filter for the Dark Energy Camera: Optimizing the LAGER Survey for z ~ 7 Galaxies

2019 arXiv: Instrumentation and Methods for Astrophysics
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