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656:, Four-Quadrant Phase Mask and 8-Octant Phase Mask versions, and a shaped pupil coronagraph. The phase I of construction is complete and phase II construction to be complete by end of 2014 for science operations in 2015. SCExAO will initially use the HiCIAO camera but this will be replaced by CHARIS, an integral field spectrograph, around 2016.
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505:
noxious smoke that killed Marvin Arruda, 52, Ricky Del
Rosario, 38, and Warren K. "Kip" Kaleo, 36, and sent twenty-six other workers to the hospital in Hilo. All four workers are memorialized by a plaque outside the base of the telescope dome and a sign posted temporarily each January along the Mauna Kea access road.
513:
On July 2, 2011, the telescope operator in Hilo noted an anomaly from the top unit of the telescope. Upon further examination, coolant from the top unit was found to have leaked over the primary mirror and other parts of the telescope. Observation using
Nasmyth foci resumed on July 22, and Cassegrain
1321:
Mary Anne Peters-Limbach; Groff, Tyler D.; Jeremy Kasdin, N.; Driscoll, Dave; Galvin, Michael; Foster, Allen; Carr, Michael A.; LeClerc, Dave; Fagan, Rad; McElwain, Michael W.; Knapp, Gillian; Brandt, Timothy; Janson, Markus; Guyon, Olivier; Jovanovic, Nemanja; Martinache, Frantz; Hayashi, Masahiko;
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This 900-megapixel ultra-wide-field (1.5° field of view) camera saw first light in 2012, and was offered for open-use in 2014. The extremely large wide-field correction optics (a seven-element lens with some elements up to a meter in diameter) was manufactured by Canon and delivered March 29, 2011.
468:
A number of state-of-the-art technologies were worked into the telescope design. For example, 261 computer-controlled actuators press the main mirror from underneath, which corrects for primary mirror distortion caused by changes in the telescope orientation. The telescope enclosure building is also
751:
Iye, M.; Karoji, H.; Ando, H.; Kaifu, N.; Kodaira, K.; Aoki, K.; Aoki, W.; Chikada, Y.; Doi, Y.; Ebizuka, N.; Elms, B.; Fujihara, G.; Furusawa, H.; Fuse, T.; Gaessler, W.; Harasawa, S.; Hayano, Y.; Hayashi, M.; Hayashi, S.; Ichikawa, S.; Imanishi, M.; Ishida, C.; Kamata, Y.; Kanzawa, T.; Kashikawa,
472:
Subaru is one of the few state-of-the-art telescopes to have been used with the naked eye. For the dedication, an eyepiece was constructed so that
Princess Sayako could look through it directly. It was enjoyed by the staff for a few nights until it was replaced with the much more sensitive working
451:
formed an engineering working group to develop and study the concept of a 7.5-metre (300 in) telescope. In 1985, the astronomy committee of Japan's science council gave top priority to the development of a "Japan
National Large Telescope" (JNLT), and in 1986, the University of Tokyo signed an
504:
Two separate incidents claimed the lives of four workers during the construction of the telescope. On
October 13, 1993, 42-year-old Paul F. Lawrence was fatally injured when a forklift tipped over onto him. On January 16, 1996, sparks from a welder ignited insulation which smoldered, generating
460:
Construction of the Subaru
Telescope began in April 1991, and later that year, a public contest gave the telescope its official name, "Subaru Telescope". Construction was completed in 1998, and the first scientific images were taken in January 1999. In September 1999,
522:
On
September 15, 2023, an abnormal load sensor value of the primary mirror fixed point was observed during a maintenance operational test. Later, a part fell onto the primary mirror during repair work of the mirror cover. Science observation was suspended.
1238:
Jovanovic, N., Martinache, F., Guyon, O., Clergeon, C., Singh, G., Kudo, T., Vievard, S., Newman, K., Minowa, Y., Hayano, Y., Kuhn, J., Serabyn, E., Norris, B., Tuthill, P., Stewart, P., Huby, E., Perrin, G., Lacour, S., Murakami, N., Fumika, O., 2014,
456:
to build the telescope in Hawaii. In 1988, the
National Astronomical Observatory of Japan was formed through a reorganization of the University's Tokyo Astronomical Observatory, to oversee the JNLT and other large national astronomy projects.
1100:
Hikage, Chiaki; Oguri, Masamune; Hamana, Takashi; More, Surhud; Mandelbaum, Rachel; Takada, Masahiro; Köhlinger, Fabian; Miyatake, Hironao; Nishizawa, Atsushi J; Aihara, Hiroaki; Armstrong, Robert (April 1, 2019).
480:. Its large field of view, 75 times that of the Keck telescopes, and strong light-gathering power are suited for deep wide-field sky surveys. The search, split between a research group led by
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80-megapixel wide-field visible-light camera, mounts at the prime focus. Superseded by the Hyper
Suprime-Cam in 2012, decommissioned in May 2017.
937:
319:
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Mid-infrared camera and spectrometer with the ability to study cool interstellar dust, mounts on the
Cassegrain focus. Decommissioned in 2020.
549:
Several cameras and spectrographs can be mounted at Subaru Telescope's four focal points for observations in visible and infrared wavelengths.
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Visible-light camera and spectrograph with the ability to take spectra of up to 100 objects simultaneously, mounts on the Cassegrain focus.
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Wide-field camera and spectrograph with the ability to take spectra of multiple objects simultaneously, mounts at the Cassegrain focus.
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focal points in enclosures on the sides of the telescope mount, to which light can be directed with a tertiary mirror; or at the
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Infrared spectrograph using movable fiber optics to take spectra of up to 400 objects simultaneously. Mounts at the prime focus.
878:
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designs. For example, at a distance of 100 pc, the PIAA coronagraph on SCExAO would be able to image from 4 AU outwards while
526:
After the replacement of sensor and the repair work of the primary mirror damage, it returned to observation on 3 March 2024.
1322:
Takato, Naruhisa (2013). Shaklan, Stuart (ed.). "The Optical Design of CHARIS: An Exoplanet IFS for the Subaru Telescope".
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Used in conjunction with the new 188-element adaptive optics unit (AO188), mounted at the infrared Nasmyth focus.
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shaped to improve the quality of astronomical images by minimizing the effects caused by atmospheric turbulence.
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Infrared camera for hunting planets around other stars. Used with AO188, mounted at the infrared Nasmyth focus.
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The Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) instrument is a high-contrast imaging system for
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Comparison of nominal sizes of apertures of the Subaru Telescope and some notable optical telescopes
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640:(PIAA) design which means it will be able to image planets closer to their stars than conventional
448:
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Spie (2014). "Satoshi Miyazaki plenary: Hyper Suprime-Cam for Weak Gravitational Lensing Survey".
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1152:"Hyper Suprime-Cam Survey Maps Dark Matter in the Universe - News - Carnegie Mellon University"
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in lieu of a secondary mirror, an arrangement rare on large telescopes, to provide a wide
397:
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1103:"Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data"
752:
N.; Kawabata, K.; Kobayashi, N.; Komiyama, Y.; Kosugi, G.; et al. (April 25, 2004),
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It will be used for surveys of weak lensing to determine dark matter distribution.
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989:"Serious Hardware Incident with the Subaru Telescope Interrupts Its Operation"
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1055:"Regarding the suspension of Subaru Telescope night observation (7th report)"
1033:"Regarding the suspention of Subaru Telescope night observation (3rd report)"
652:
from 12 AU outwards. The system also has several other types of coronagraph:
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754:"Current Performance and On-Going Improvements of the 8.2m Subaru Telescope"
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700:, the English name of the asterism for which the Subaru Telescope is named
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1241:"SCExAO as a precursor to an ELT exoplanet direct imaging instrument"
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1012:"Report 4: Resumption of Open Use Observations at Cassegrain Focus"
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1326:. Techniques and Instrumentation for Detection of Exoplanets VI.
1010:
National Astronomical Observatory of Japan (September 13, 2011).
1191:
677:, a technique of compensating for aberrations in optical systems
590:
586:
Visible-light spectrograph mounted at the optical Nasmyth focus.
689:, an astronomical device for masking the direct light of a star
599:
High-Contrast Coronographic Imager for Adaptive Optics (HiCIAO)
1035:. National Astronomical Observatory of Japan. October 16, 2023
938:"Astronomers say a Neptune-sized planet lurks beyond Pluto"
297:
1379:
553:
Multi-Object Infrared Camera and Spectrograph (MOIRCS)
428:
reflecting telescope. Instruments can be mounted at a
1396:
1192:"Subaru Telescope HSC Wide Field Corrector completed"
964:"SUBARU 8-METER TELESCOPE DAMAGED BY LEAKING COOLANT"
625:
Subaru Coronagraphic Extreme Adaptive Optics (SCExAO)
565:
Cooled Mid Infrared Camera and Spectrometer (COMICS)
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SCExAO: The Subaru Coronagraphic Extreme AO Project
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1150:University, Carnegie Mellon (September 26, 2018).
723:"Corning Museum of Glass - Telescopes and Mirrors"
1528:Buildings and structures in Hawaii County, Hawaii
1107:Publications of the Astronomical Society of Japan
879:"On Hawaii, A Telescope Widens Orbit Of Japanese"
432:focus below the primary mirror; at either of two
388:is the 8.2-metre (320 in) telescope of the
381:
412:in the world from its commissioning until the
375:
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693:List of largest optical reflecting telescopes
613:map from 2018 by the Hyper Suprime-Cam survey
476:Subaru is the primary tool in the search for
8:
571:Faint Object Camera And Spectrograph (FOCAS)
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1513:Buildings and structures completed in 1998
1387:National Astronomical Observatory of Japan
390:National Astronomical Observatory of Japan
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887:. Japan; Hawaii; Mount Mauna Kea (Hawaii)
772:
877:French, Howard W. (September 19, 1999).
664:
496:, is expected to take up to five years.
326:
1403:
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577:Subaru Prime Focus Camera (Suprime-Cam)
559:Infrared Camera and Spectrograph (IRCS)
962:Atkinson, Nancy (December 24, 2015).
7:
1523:Astronomical observatories in Hawaii
638:Phase Induced Amplitude Apodization
444:suited to deep wide-field surveys.
583:High Dispersion Spectrograph (HDS)
465:of Japan dedicated the telescope.
16:Japanese telescope and observatory
14:
1285:SCExAO Science ready Capabilities
1057:. Subaru Telescope. March 5, 2024
589:Fiber Multi Object Spectrograph (
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1078:冷却中間赤外線分光撮像装置 COMICS の「ファイナルライト」
408:. It had the largest monolithic
346:
325:
318:
246:53 m (570 sq ft)
1392:Micro-lens for Subaru Telescope
1081:(in Japanese). October 26, 2022
936:Hand, Eric (January 20, 2016).
683:, a signal processing technique
223:
215:
538:The Subaru alongside the twin
163:4,139 m (13,579 ft)
1:
1518:1998 establishments in Hawaii
906:Ferris, Timothy (July 2009),
500:Accidents during construction
514:focus resumed on August 26.
335:Location of Subaru Telescope
856:"A Brief History of Subaru"
544:Infrared Telescope Facility
382:
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1303:SCExAO Future Capabilities
991:. web-subarutelescope.org/
424:The Subaru Telescope is a
203:Ritchey–Chrétien telescope
1533:Exoplanet search projects
414:Large Binocular Telescope
376:
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220:8.3 m (8.2 m usable)
26:
1172:. Subaru Telescope, NAOJ
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404:known in English as the
400:. It is named after the
352:Related media on Commons
761:Publ. Astron. Soc. Jpn.
618:Hyper Suprime-Cam (HSC)
225:Secondary diameter
43:Mauna Kea Observatories
1308:April 8, 2014, at the
1290:April 8, 2014, at the
1246:April 8, 2014, at the
812:"The Subaru Telescope"
670:
614:
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540:W. M. Keck Observatory
281:cylindrical dome
791:10.1093/pasj/56.2.381
668:
642:Lyot type coronagraph
609:
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394:Mauna Kea Observatory
141:Observatory code
1215:10.1117/2.3201407.17
646:Gemini Planet Imager
454:University of Hawaii
243:Collecting area
199:reflecting telescope
191:Telescope style
101:19.8256°N 155.4761°W
33:The Subaru Telescope
1346:2013SPIE.8864E..1NP
1324:Proceedings of SPIE
1129:10.1093/pasj/psz010
912:National Geographic
836:. Subaru Telescope"
783:2004PASJ...56..381I
542:telescopes and the
488:and another led by
452:agreement with the
449:University of Tokyo
97: /
23:
1354:10.1117/12.2024070
884:The New York Times
671:
615:
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482:Konstantin Batygin
234:Angular resolution
106:19.8256; -155.4761
402:open star cluster
392:, located at the
368:
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261:f/1.83 (15.000 m)
228:1330/1400/1265 mm
195:optical telescope
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1380:Official website
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834:"Specifications"
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632:exoplanets. The
630:directly imaging
426:Ritchey-Chretien
416:opened in 2005.
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361:edit on Wikidata
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1156:www.cmu.edu
947:January 20,
704:Yūko Kakazu
687:Coronagraph
681:Apodization
634:coronagraph
611:Dark matter
530:Instruments
478:Planet Nine
438:prime focus
104: /
92:155°28′34″W
80:Coordinates
61:Location(s)
1538:Telescopes
1507:Categories
1330:: 88641N.
1270:August 21,
1261:"Overview"
1120:1809.09148
858:. Naoj.org
725:. Cmog.org
710:References
650:VLT-SPHERE
430:Cassegrain
174:Wavelength
89:19°49′32″N
1485:Education
1425:Astronomy
1362:108283811
1337:1309.3586
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973:April 10,
278:Enclosure
69:Mauna Kea
65:Mauna Kea
1306:Archived
1288:Archived
1244:Archived
1061:March 7,
698:Pleiades
661:See also
420:Overview
406:Pleiades
267:Mounting
217:Diameter
160:Altitude
1497:Science
1399:Portals
1342:Bibcode
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636:uses a
434:Nasmyth
293:Website
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377:すばる望遠鏡
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183:Built
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1272:2014
1178:2013
1133:ISSN
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1063:2024
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1019:2011
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975:2017
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924:2009
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842:2010
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591:FMOS
492:and
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