Skip to main content

Hyper Suprime-Cam

Author(s): Miyazaki, S; Komiyama, Y; Nakaya, H; Kamata, Y; Doi, Y; et al

Download
To refer to this page use: http://arks.princeton.edu/ark:/88435/pr1wm13t1c
Full metadata record
DC FieldValueLanguage
dc.contributor.authorMiyazaki, S-
dc.contributor.authorKomiyama, Y-
dc.contributor.authorNakaya, H-
dc.contributor.authorKamata, Y-
dc.contributor.authorDoi, Y-
dc.contributor.authorHamana, T-
dc.contributor.authorKaroji, H-
dc.contributor.authorFurusawa, H-
dc.contributor.authorKawanomoto, S-
dc.contributor.authorMorokuma, T-
dc.contributor.authorIshizuka, Y-
dc.contributor.authorNariai, K-
dc.contributor.authorTanaka, Y-
dc.contributor.authorUraguchi, F-
dc.contributor.authorUtsumi, Y-
dc.contributor.authorObuchi, Y-
dc.contributor.authorOkura, Y-
dc.contributor.authorOguri, M-
dc.contributor.authorTakata, T-
dc.contributor.authorTomono, D-
dc.contributor.authorKurakami, T-
dc.contributor.authorNamikawa, K-
dc.contributor.authorUsuda, T-
dc.contributor.authorYamanoi, H-
dc.contributor.authorTerai, T-
dc.contributor.authorUekiyo, H-
dc.contributor.authorYamada, Y-
dc.contributor.authorKoike, M-
dc.contributor.authorAihara, H-
dc.contributor.authorFujimori, Y-
dc.contributor.authorMineo, S-
dc.contributor.authorMiyatake, H-
dc.contributor.authorYasuda, N-
dc.contributor.authorNishizawa, J-
dc.contributor.authorSaito, T-
dc.contributor.authorTanaka, M-
dc.contributor.authorUchida, T-
dc.contributor.authorKatayama, N-
dc.contributor.authorWang, SY-
dc.contributor.authorChen, HY-
dc.contributor.authorLupton, R-
dc.contributor.authorLoomis, C-
dc.contributor.authorBickerton, S-
dc.contributor.authorPrice, P-
dc.contributor.authorGunn, James E-
dc.contributor.authorSuzuki, H-
dc.contributor.authorMiyazaki, Y-
dc.contributor.authorMuramatsu, M-
dc.contributor.authorYamamoto, K-
dc.contributor.authorEndo, M-
dc.contributor.authorEzaki, Y-
dc.contributor.authorItoh, N-
dc.contributor.authorMiwa, Y-
dc.contributor.authorYokota, H-
dc.contributor.authorMatsuda, T-
dc.contributor.authorEbinuma, R-
dc.contributor.authorTakeshi, K-
dc.date.accessioned2022-01-25T15:00:57Z-
dc.date.available2022-01-25T15:00:57Z-
dc.date.issued2012-12-01en_US
dc.identifier.citationMiyazaki, S, Komiyama, Y, Nakaya, H, Kamata, Y, Doi, Y, Hamana, T, Karoji, H, Furusawa, H, Kawanomoto, S, Morokuma, T, Ishizuka, Y, Nariai, K, Tanaka, Y, Uraguchi, F, Utsumi, Y, Obuchi, Y, Okura, Y, Oguri, M, Takata, T, Tomono, D, Kurakami, T, Namikawa, K, Usuda, T, Yamanoi, H, Terai, T, Uekiyo, H, Yamada, Y, Koike, M, Aihara, H, Fujimori, Y, Mineo, S, Miyatake, H, Yasuda, N, Nishizawa, J, Saito, T, Tanaka, M, Uchida, T, Katayama, N, Wang, SY, Chen, HY, Lupton, R, Loomis, C, Bickerton, S, Price, P, Gunn, J, Suzuki, H, Miyazaki, Y, Muramatsu, M, Yamamoto, K, Endo, M, Ezaki, Y, Itoh, N, Miwa, Y, Yokota, H, Matsuda, T, Ebinuma, R, Takeshi, K. (2012). Hyper Suprime-Cam. Proceedings of SPIE - The International Society for Optical Engineering, 8446 (10.1117/12.926844en_US
dc.identifier.issn0277-786X-
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr1wm13t1c-
dc.description.abstractHyper Suprime-Cam (HSC) is an 870 Mega pixel prime focus camera for the 8.2 m Subaru telescope. The wide field corrector delivers sharp image of 0.25 arc-sec FWHM in r-band over the entire 1.5 degree (in diameter) field of view. The collimation of the camera with respect to the optical axis of the primary mirror is realized by hexapod actuators whose mechanical accuracy is few microns. As a result, we expect to have seeing limited image most of the time. Expected median seeing is 0.67 arc-sec FWHM in i-band. The sensor is a p-ch fully depleted CCD of 200 micron thickness (2048 x 4096 15 μm square pixel) and we employ 116 of them to pave the 50 cm focal plane. Minimum interval between exposures is roughly 30 seconds including reading out arrays, transferring data to the control computer and saving them to the hard drive. HSC uniquely features the combination of large primary mirror, wide field of view, sharp image and high sensitivity especially in red. This enables accurate shape measurement of faint galaxies which is critical for planned weak lensing survey to probe the nature of dark energy. The system is being assembled now and will see the first light in August 2012. © 2012 SPIE.en_US
dc.language.isoen_USen_US
dc.relation.ispartofProceedings of SPIE - The International Society for Optical Engineeringen_US
dc.rightsFinal published version. Article is made available in OAR by the publisher's permission or policy.en_US
dc.titleHyper Suprime-Camen_US
dc.typeConference Articleen_US
dc.identifier.doidoi:10.1117/12.926844-
dc.date.eissued2012-10-05en_US
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/conference-proceedingen_US

Files in This Item:
File Description SizeFormat 
84460Z.pdf3.85 MBAdobe PDFView/Download


Items in OAR@Princeton are protected by copyright, with all rights reserved, unless otherwise indicated.