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Bright and Faint Ends of Ly Luminosity Functions at Determined by the Subaru Survey: Implications for AGN, Magnification Bias, and ISM HI Evolution
Akira Konno, Masami Ouchi, Kimihiko Nakajima +4
We present the Lya luminosity functions (LFs) derived by our deep Subaru narrowband survey that identifies a total of 3,137 Lya emitters (LAEs) at in five independent bla…
Statistical Properties of Diffuse Lyman-alpha Halos around Star-forming Galaxies at z~2
Rieko Momose, Masami Ouchi, Kimihiko Nakajima +6
We present statistical properties of diffuse Lyman-alpha halos (LAHs) around high- star-forming galaxies with large Subaru samples of Lyman-alpha emitters (LAEs) at . We…
Early Science with the Large Millimeter Telescope: Observations of dust continuum and CO emission lines of cluster-lensed submillimetre galaxies at z=2.0-4.7
J. A. Zavala, M. S. Yun, I. Aretxaga +19
We present Early Science observations with the Large Millimeter Telescope, AzTEC 1.1 mm continuum images and wide bandwidth spectra (73-111 GHz) acquired with the Redshift Search R…
Thirty Meter Telescope International Observatory Detailed Science Case 2024
Warren Skidmore, Bob Kirshner, David Andersen +168
The Thirty Meter Telescope (TMT) International Observatory (TIO) will be a revolutionary leap forward in astronomical observing capabilities, enabling us to address some of the mos…
A Close Comparison between Observed and Modeled Lyα Lines for z ~ 2.2 Lyman Alpha Emitters
Takuya Hashimoto, Anne Verhamme, Masami Ouchi +7
We present the results of a Lya profile analysis of 12 Lya emitters (LAEs) at z = 2.2 with high-resolution Lya spectra. We find that all 12 objects have a Lya profile with the main…