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Subaru Telescope
Recent science highlights
and future prospects
Masato Onodera
Subaru Telescope ( )
National Astronomical Observatory of Japan
@SubaruTel_Eng
Credit: Hideaki Fujiwara
Subaru Telescope
Named after the Pleiades in Japanese
Optical and infrared telescope
27 ft. diameter and 7.9 inches thick single
dish primary mirror
Construction : 1991 — 1999
Science operation : 2000 — present
Credit: Hana Hou! (August/September 2018)
What we are good at
👍 Wide

Cover a large patch of the sky at once; chances of
serendipity
👍 Sharp

Extrasolar planets, structures within distant galaxies,
dark matter distributions
👍 Large

Faint astronomical objects
Credit:
ESO & Andy Strappazzon
Hiromitsu Kosaka, HSC project, & NAOJ
HSC : wide field imager
Hyper Suprime-Cam mounted on the prime focus
870-megapixel camera (cf. 12-megapixel in

iPhone Xs) for optical wavelength
1.5 degree diameter FoV (3x Moon diameter)
Good image quality
Credit: HSC-SSP & NAOJ
New extremely distant dwarf planet, orbiting
the edge of the solar system
Implication on even further, unknown dwarf
planet, so-called "Planet X"
Discovery of "The Goblin"
Sheppard et al. (2018)
Follow-up campaign of the binary
neutron star merger event GW170817
August 18-19, 2017 August 24-25, 2017
Days after the GW event
Brightness(magnitude)
Optical light
Near-IR light
1. Search : wide-field capability
2. Measure : large light collecting area
3. Physics : comparison with theory
Good model! (kilonova)
Bad model
Tominaga et al. (2017); Utsumi et al. (2017); Tanaka et al. (2017)
Widest 3D dark matter maps
Ongoing large survey using HSC for 300 nights in 5 years
Wide field : large patches of the sky, more galaxies
Good image quality : distortion of galaxy shapes due to gravity
from dark matter
Large aperture : faint galaxies at more distant universe
All data is public! You can freely download everything from the
survey and dig them by yourself. Visit https://hsc.mtk.nao.ac.jp/
ssp/
Credit: HSC-SSP & NAOJ
1.3 billion
years ago
7.8 billion
years ago
You

are

here
Less structure
in the pastMore structure
now
Oguri et al. (2018); Miyazaki et al. (2018)
Structure growth over cosmic time
🌕x6
Exoplanet studies with
ultrasharp imaging
Atlas of protoplanetary disks taken
with HiCIAO instrument with adaptive
optics (Credit: SEEDS project)
CHARIS : imager and spectrograph
for extrasolar planet hunting
Optimized to obtain image and spectra simultaneously for
extrasolar planets with ultrasharp image quality
First scientific results are just arriving
Currie et al. (2018)
κ And b
Future prospects
IRD : another extrasolar
planet hunting machine
Science operation started in 2018
Extremely precise velocity measurement in near-IR
wavelength
Detect 4.5 mph movement of stars due to planets
around them
Goal is to find earth-like planets around low-mass stars
Credit: Astrobiology Center
Enhancing the wide field capability
PFS (under construction; 2021–)
Measure precise distance by taking optical to near-IR
spectra of 2000+ galaxies at once to study dark energy
ULTIMATE-Subaru (concept design; 2026–)
Panoramic view and sharp image quality in the infrared
wavelength to study galaxies from the birth to the death
PFS ULTIMATE-Subaru

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Recent Science Highlights and Future Prospects

  • 1. Subaru Telescope Recent science highlights and future prospects Masato Onodera Subaru Telescope ( ) National Astronomical Observatory of Japan @SubaruTel_Eng Credit: Hideaki Fujiwara
  • 2. Subaru Telescope Named after the Pleiades in Japanese Optical and infrared telescope 27 ft. diameter and 7.9 inches thick single dish primary mirror Construction : 1991 — 1999 Science operation : 2000 — present Credit: Hana Hou! (August/September 2018)
  • 3. What we are good at 👍 Wide
 Cover a large patch of the sky at once; chances of serendipity 👍 Sharp
 Extrasolar planets, structures within distant galaxies, dark matter distributions 👍 Large
 Faint astronomical objects Credit: ESO & Andy Strappazzon Hiromitsu Kosaka, HSC project, & NAOJ
  • 4. HSC : wide field imager Hyper Suprime-Cam mounted on the prime focus 870-megapixel camera (cf. 12-megapixel in
 iPhone Xs) for optical wavelength 1.5 degree diameter FoV (3x Moon diameter) Good image quality Credit: HSC-SSP & NAOJ
  • 5. New extremely distant dwarf planet, orbiting the edge of the solar system Implication on even further, unknown dwarf planet, so-called "Planet X" Discovery of "The Goblin" Sheppard et al. (2018)
  • 6. Follow-up campaign of the binary neutron star merger event GW170817 August 18-19, 2017 August 24-25, 2017 Days after the GW event Brightness(magnitude) Optical light Near-IR light 1. Search : wide-field capability 2. Measure : large light collecting area 3. Physics : comparison with theory Good model! (kilonova) Bad model Tominaga et al. (2017); Utsumi et al. (2017); Tanaka et al. (2017)
  • 7. Widest 3D dark matter maps Ongoing large survey using HSC for 300 nights in 5 years Wide field : large patches of the sky, more galaxies Good image quality : distortion of galaxy shapes due to gravity from dark matter Large aperture : faint galaxies at more distant universe All data is public! You can freely download everything from the survey and dig them by yourself. Visit https://hsc.mtk.nao.ac.jp/ ssp/ Credit: HSC-SSP & NAOJ
  • 8. 1.3 billion years ago 7.8 billion years ago You
 are
 here Less structure in the pastMore structure now Oguri et al. (2018); Miyazaki et al. (2018) Structure growth over cosmic time 🌕x6
  • 9. Exoplanet studies with ultrasharp imaging Atlas of protoplanetary disks taken with HiCIAO instrument with adaptive optics (Credit: SEEDS project)
  • 10. CHARIS : imager and spectrograph for extrasolar planet hunting Optimized to obtain image and spectra simultaneously for extrasolar planets with ultrasharp image quality First scientific results are just arriving Currie et al. (2018) κ And b
  • 12. IRD : another extrasolar planet hunting machine Science operation started in 2018 Extremely precise velocity measurement in near-IR wavelength Detect 4.5 mph movement of stars due to planets around them Goal is to find earth-like planets around low-mass stars Credit: Astrobiology Center
  • 13. Enhancing the wide field capability PFS (under construction; 2021–) Measure precise distance by taking optical to near-IR spectra of 2000+ galaxies at once to study dark energy ULTIMATE-Subaru (concept design; 2026–) Panoramic view and sharp image quality in the infrared wavelength to study galaxies from the birth to the death PFS ULTIMATE-Subaru