CANDELS 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 supernova beyond z > 1.5 and establish their accuracy as standard candles for cosmology. Additional "daytime" WFC3/UV/Vis exposures in the GOODS-N field were conducted to take advantage of its continuous viewing zone opportunity.3
CANDELS' main instrument is the Wide Field Camera 3, a near-infrared camera installed on Hubble in May 2009. WFC3 works in tandem with the visible-light Advanced Camera for Surveys, which together gives unprecedented panchromatic coverage of galaxies from optical wavelengths to the near-infrared.4
"Hyperwall: CANDELS UDF". nasa.gov. 28 January 2019. https://svs.gsfc.nasa.gov/31020 ↩
"Hubble explores the origins of modern galaxies". Spacetelescope.org. 15 August 2013. https://www.spacetelescope.org/news/heic1315/ ↩
"Science Goals". CANDELS. University of California Observatories. http://arcoiris.ucolick.org/candels/survey/Science_Goals.html ↩
"About". CANDELS. University of California Observatories. http://arcoiris.ucolick.org/candels/survey/Science_Goals.html ↩