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・ Cosmia affinis
・ Cosmia calami
・ Cosmia diffinis
・ Cosmia poecila
・ Cosmia pyralina
・ Cosmia restituta
・ Cosmibuena
・ Cosmic
・ Cosmic age problem
・ Cosmic Air
・ Cosmic ancestry
・ Cosmic Anisotropy Polarization Mapper
・ Cosmic Anisotropy Telescope
・ Cosmic Ark
・ Cosmic Assault
Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey
・ Cosmic Avenger
・ Cosmic Award
・ Cosmic background
・ Cosmic Background Explorer
・ Cosmic Background Imager
・ Cosmic background radiation
・ Cosmic Balance II
・ Cosmic Banditos
・ Cosmic bliss
・ Cosmic Bomb (horse)
・ Cosmic bomb (phrase)
・ Cosmic Boy
・ Cosmic Break
・ Cosmic Brownies


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Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey : ウィキペディア英語版
Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey

CANDELS, the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey, is the largest project in the history of the Hubble Space Telescope, with 902 assigned orbits of observing time. It is being carried out with two cameras on board Hubble – WFC3 and ACS – and aims to explore galactic evolution in the early Universe, and the very first seeds of cosmic structure at less than one billion years after the Big Bang.〔(Hubble explores the origins of modern galaxies )〕
==Science Goals==

The Cosmic Assembly Near-IR Deep Extragalactic Legacy Survey is designed to document the first third of galactic evolution – on the redshifts from 8 to 1.5 – via deep imaging of more than 250,000 galaxies.
Another goal is to find the first Type Ia SNe beyond z > 1.5 and establish their accuracy as standard candles for cosmology.
Plus some "daytime" UVIS exposures in GOODS-N to exploit the CVZ opportunity in that field.〔(CANDELS Science Goals )〕


抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
ウィキペディアで「Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey」の詳細全文を読む



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