Science with UT's Dichroic-Mirror Camera (DMC), 15-band simultaneous imager

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dc.creatorKuncarayakti, Hanindyo
dc.creatorDoi, Mamoru
dc.creatorMalasan, Hakim L.
dc.creatorHayano, Junji
dc.creatorUtsunomiya, Hiroyuki
dc.creatorIhara, Yutaka
dc.creatorTokita, Kouichi
dc.creatorTakanashi, Naohiro
dc.creatorSako, Shigeyuki
dc.creatorOkamura, Sadanori
dc.creatorMorokuma, Tomoki
dc.creatorFurusawa, Hisanori
dc.creatorKomiyama, Yutaka
dc.creatorYagi, Masafumi
dc.creatorOkada, Norio
dc.creatorNakaya, Hidehiko
dc.creatorArai, Akira
dc.creatorUemura, Makoto
dc.creatorKawabata, Koji S.
dc.creatorYamashita, Takuya
dc.creatorOhsugi, Takashi
dc.creatorAbe, Masanao
dc.creatorHasegawa, Sunao
dc.date2008-10-31
dc.date.accessioned2026-07-07T10:14:32Z
dc.date.available2026-07-07T10:14:32Z
dc.descriptionWe introduce the Dichroic-Mirror Camera (DMC), an instrument developed at the University of Tokyo which is capable of performing simultaneous imaging in fifteen bands. The main feature of the DMC is the dichroic mirrors, which split incoming light into red and blue components. Combination of dichroic mirrors split light from the telescope focus into fifteen intermediate-width bands across 390 -- 950 nm. The fifteen bands of DMC provide measurements of the object's spectral energy distribution (SED) at fifteen wavelength points. During May -- June 2007 and March 2008, observing run of the DMC was carried out at Higashi-Hiroshima Observatory, Japan. We observed several objects i.e. planets, asteroids, standard stars & star clusters, planetary nebulae, galaxies, and supernovae. We describe several early scientific results from the DMC.
dc.description3 pages 6 figures Proceedings of 10th Asian-Pacific Regional IAU Meeting
dc.identifierhttps://arxiv.org/abs/0810.5607
dc.identifierhttp://arxiv.org/abs/0810.5607
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/172911
dc.subjectAstrophysics
dc.titleScience with UT's Dichroic-Mirror Camera (DMC), 15-band simultaneous imager
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