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The Evolution Of The Faint End Of The UV Luminosity Function During The Peak Epoch Of Star Formation (1<z<3)

, , , , , , , , , , , and . (2016)cite arxiv:1606.00469Comment: 22 pages, 15 figures.

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Ultra-faint Ultraviolet Galaxies at z~2 Behind the Lensing Cluster Abell 1689: the Luminosity Function, Dust Extinction and Star Formation Rate Density, , , , , , , , , and 1 other author(s). (2013)cite arxiv:1305.2413Comment: 14 pages, 10 figures, 4 tables, submitted to ApJ.The MOSDEF Survey: Measurements of Balmer Decrements and the Dust Attenuation Curve at Redshifts z~1.4-2.6, , , , , , , , , and . (2015)cite arxiv:1504.02782Comment: 24 pages, 2 tables, 24 figures, accepted to the Astrophysical Journal.The Evolution Of The Faint End Of The UV Luminosity Function During The Peak Epoch Of Star Formation (1<z<3), , , , , , , , , and 2 other author(s). (2016)cite arxiv:1606.00469Comment: 22 pages, 15 figures.Study on Correlation Between Subjective and Objective Metrics for Multimodal Retinal Image Registration., , , , , , and . IEEE Access, (2020)Perspective Distortion Correction for Multi-Modal Registration between Ultra-Widefield and Narrow-Angle Retinal Images., , , , , and . EMBC, page 4086-4091. IEEE, (2021)The MOSDEF Survey: Mass, Metallicity, and Star-formation Rate at z~2.3, , , , , , , , , and 1 other author(s). (2014)cite arxiv:1408.2521Comment: 10 pages, 6 figures, submitted to ApJ.The MOSDEF Survey: Broad Emission Lines at z=1.4-3.8, , , , , , , , , and 5 other author(s). (2017)cite arxiv:1710.03230.Two-Step Registration on Multi-Modal Retinal Images via Deep Neural Networks., , , , , , , and . IEEE Trans. Image Process., (2022)Accurate Registration between Ultra-Wide-Field and Narrow Angle Retina Images with 3D Eyeball Shape Optimization., , , , , , , and . ICIP, page 2750-2754. IEEE, (2023)Learning to Correct Axial Motion in Oct for 3D Retinal Imaging., , , , , , and . ICIP, page 126-130. IEEE, (2021)