The Spitzer-Cosmic Assembly Near-Infrared Deep Extragalactic Legacy
Survey (S-CANDELS) is a Spitzer Cycle 8 Exploration Program (PI G.
Fazio) that obtained deep IRAC channel 1 and 2 imaging in five widely
separated extragalactic fields: the UKIDSS Ultra-Deep Survey (UDS), the Extended Chandra Deep Field South
(ECDFS), COSMOS, the HST Deep
Field North (HDFN), and the Extended Groth Strip (EGS). S-CANDELS
builds upon the existing coverage of these fields obtained as part of
the Spitzer Extended Deep Survey (SEDS), a Cycle 6 Exploration
Program, by increasing the integration time from 12 hours to a total
of 50 hours within a smaller area of 0.16 deg2.
If you use S-CANDELS data, please cite both the journal article Ashby et al.
(2015) and the dataset Digital Object Identifier (DOI): 10.26131/IRSA419.
Jump to documentation.
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S-CANDELS Overview
S-CANDELS Data Access
S-CANDELS Cutouts