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Satoshi Yamanaka

Identifiers

  • name variant Satoshi Yamanaka 0.60 · backfill

Papers (18)

  1. JWST/NIRSpec spectroscopy of intermediate-mass quiescent galaxies at $z \sim 3-4$ astro-ph.GA · 2024 · author #9
  2. Gas conditions of a star-formation selected sample in the first billion years astro-ph.GA · 2024 · author #23
  3. JWST, ALMA, and Keck Spectroscopic Constraints on the UV Luminosity Functions at z~7-14: Clumpiness and Compactness of the Brightest Galaxies in the Early Universe astro-ph.GA · 2024 · author #18
  4. SILVERRUSH. XIII. A Catalog of 20,567 Ly$\alpha$ Emitters at $z=2-7$ Identified in the Full-depth Data of the Subaru/HSC-SSP and CHORUS Surveys astro-ph.GA · 2023 · author #11
  5. Detections of [C II] 158 $\mu$m and [O III] 88 $\mu$m in a Local Lyman Continuum Emitter, Mrk 54, and its Implications to High-redshift ALMA Studies astro-ph.GA · 2023 · author #15
  6. Bridging Optical and Far-Infrared Emission-Line Diagrams of Galaxies from Local to the Epoch of Reionization: Characteristic High [O III] 88 $\mathrm{\mu m}$/SFR at $z > 6$ astro-ph.GA · 2022 · author #6
  7. Possible Systematic Rotation in the Mature Stellar Population of a $z=9.1$ Galaxy astro-ph.GA · 2022 · author #13
  8. Big Three Dragons: Molecular Gas in a Bright Lyman-Break Galaxy at $z=7.15$ astro-ph.GA · 2022 · author #9
  9. CHORUS IV: Mapping the Spatially Inhomogeneous Cosmic Reionization with Subaru HSC astro-ph.GA · 2022 · author #4
  10. A Search for H-Dropout Lyman Break Galaxies at z~12-16 astro-ph.GA · 2021 · author #5
  11. A Morphological Study on Galaxies Hosting Optical Variability-Selected AGNs in the COSMOS Field astro-ph.GA · 2021 · author #3
  12. SILVERRUSH XI: Constraints on the Ly$\alpha$ luminosity function and cosmic reionization at $z=7.3$ with Subaru/Hyper Suprime-Cam astro-ph.GA · 2021 · author #3
  13. The SSA22 HI Tomography Survey (SSA22-HIT). I. Data Set and Compiled Redshift Catalog astro-ph.GA · 2021 · author #10
  14. Big Three Dragons: A [N II] 122 $\mu$m Constraint and New Dust-continuum Detection of A $z = 7.15$ Bright Lyman Break Galaxy with ALMA astro-ph.GA · 2021 · author #4
  15. SILVERRUSH X: Machine Learning-Aided Selection of $9318$ LAEs at $z=2.2$, $3.3$, $4.9$, $5.7$, $6.6$, and $7.0$ from the HSC SSP and CHORUS Survey Data astro-ph.GA · 2021 · author #6
  16. Testing an indirect method for identifying galaxies with high levels of Lyman continuum leakage astro-ph.GA · 2020 · author #1
  17. Balmer Break Galaxy Candidates at $z \sim 6$: a Potential View on the Star-Formation Activity at $z \gtrsim 14$ astro-ph.GA · 2019 · author #6
  18. The UV spectral slope beta and stellar population of most active star-forming galaxies at z~4 astro-ph.GA · 2019 · author #1

Mentions

  • 2406.18352 #18 · arxiv_oai · confidence 0.70 Satoshi Yamanaka
  • 2410.08745 #9 · arxiv_oai · confidence 0.70 Satoshi Yamanaka
  • 2406.19439 #23 · arxiv_oai · confidence 0.70 Satoshi Yamanaka
  • 2305.08921 #11 · arxiv_oai · confidence 0.70 Satoshi Yamanaka
  • 2203.01345 #9 · arxiv_oai · confidence 0.70 Satoshi Yamanaka
  • 2303.11036 #15 · arxiv_oai · confidence 0.70 Satoshi Yamanaka
  • 2110.11977 #10 · arxiv_oai · confidence 0.70 Satoshi Yamanaka
  • 2207.05236 #6 · arxiv_oai · confidence 0.70 Satoshi Yamanaka
  • 2205.14378 #13 · arxiv_oai · confidence 0.70 Satoshi Yamanaka
  • 2112.09141 #5 · arxiv_oai · confidence 0.70 Satoshi Yamanaka
  • 2201.07261 #4 · arxiv_oai · confidence 0.70 Satoshi Yamanaka
  • 2111.15289 #3 · arxiv_oai · confidence 0.70 Satoshi Yamanaka
  • 2110.14474 #3 · arxiv_oai · confidence 0.70 Satoshi Yamanaka
  • 2104.02201 #4 · arxiv_oai · confidence 0.70 Satoshi Yamanaka
  • 2104.02177 #6 · arxiv_oai · confidence 0.70 Satoshi Yamanaka
  • 2003.03905 #1 · arxiv_oai · confidence 0.70 Satoshi Yamanaka
  • 1912.10954 #6 · arxiv_oai · confidence 0.70 Satoshi Yamanaka
  • 1904.01373 #1 · arxiv_oai · confidence 0.70 Satoshi Yamanaka

Frequent Coauthors