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Satoshi Hamano

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Papers (12)

  1. FeI lines in 0.91-1.33 ${\rm \mu}$m spectra of red giants for measuring the microturbulence and metallicities astro-ph.SR · 2019 · author #8
  2. A newly-identified emission-line region around P Cygni astro-ph.SR · 2018 · author #3
  3. Correction of near-infrared high-resolution spectra for telluric absorption at 0.90-1.35 microns astro-ph.IM · 2018 · author #5
  4. Star formation activity beyond the outer Arm I: WISE-selected candidate star-forming regions astro-ph.GA · 2017 · author #5
  5. Method to Estimate the Effective Temperatures of Late-Type Giants using Line-Depth Ratios in the Wavelength Range 0.97-1.32$\mu $m astro-ph.SR · 2017 · author #5
  6. Radial Velocity Measurements of an Orbiting Star Around Sgr A* astro-ph.GA · 2017 · author #7
  7. Near infrared diffuse interstellar bands toward the Cygnus OB2 association astro-ph.GA · 2016 · author #1
  8. Herbig Ae/Be candidate stars in the innermost Galactic disk: Quartet cluster astro-ph.SR · 2016 · author #3
  9. A Warm Near-Infrared High-Resolution Spectrograph with Very High Throughput (WINERED) astro-ph.IM · 2015 · author #13
  10. Near-infrared diffuse interstellar bands in 0.91-1.32 micron astro-ph.GA · 2014 · author #1
  11. Discovery of Star Formation in the Extreme Outer Galaxy Possibly Induced by a High-velocity Cloud Impact astro-ph.GA · 2014 · author #6
  12. Type-Ia Supernova Remnant Shell At $Z=3.5$ Seen In The Three Sightlines Toward The Gravitationally Lensed Qso B1422+231 astro-ph.CO · 2012 · author #1

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