Ultraviolet and Blue Optical Imaging of UVCANDELS

Author:

Wang XinORCID,Teplitz Harry I.ORCID,Sun LeiORCID,Rafelski MarcORCID,Grogin NormanORCID,Prichard LauraORCID,Sunnquist BenORCID,Alavi AnahitaORCID,Windhorst Rogier A.ORCID,Koekemoer Anton M.ORCID,Ashcraft TeresaORCID,Bagley MicaelaORCID,Baronchelli IvanoORCID,Barro GuillermoORCID,Blanche AlexORCID,Brammer GabrielORCID,Broussard AdamORCID,Carleton TimothyORCID,Chartab NimaORCID,Cheng YingjieORCID,Codoreanu AlexORCID,Cohen SethORCID,Colbert JamesORCID,Conselice ChristopherORCID,Dai Y. SophiaORCID,Darvish BehnamORCID,Davé RomeelORCID,DeGroot LauraORCID,De Mello DuiliaORCID,Dickinson MarkORCID,Emami NajmehORCID,Ferguson HenryORCID,Ferreira LeonardoORCID,Finkelstein KeelyORCID,Finkelstein StevenORCID,Gardner Jonathan P.ORCID,Gawiser EricORCID,Gburek TimothyORCID,Giavalisco MauroORCID,Grazian AndreaORCID,Gronwall CarylORCID,Guo YichengORCID,Arrabal Haro PabloORCID,Hathi Nimish P.ORCID,Hayes MatthewORCID,Hemmati ShoubanehORCID,Howell JustinORCID,Iyer KartheikORCID,Jansen Rolf A.ORCID,Ji ZhiyuanORCID,Kaviraj SugataORCID,Kurczynski PeterORCID,Lazar IlinORCID,Lucas Ray A.ORCID,MacKenty JohnORCID,Mehta VihangORCID,Mantha Kameswara BharadwajORCID,Martin AlecORCID,Martin GarrethORCID,McCabe TylerORCID,Mobasher BahramORCID,Nedkova Kalina V.ORCID,O’Connell RobertORCID,Olsen CharlotteORCID,Otteson LillianORCID,Ravindranath SwaraORCID,Redshaw CalebORCID,Robertson BrantORCID,Rutkowski MichaelORCID,Sattari ZahraORCID,Scarlata ClaudiaORCID,Siana BrianORCID,Smith Brent M.ORCID,Soto EmmarisORCID,Vanzella ErosORCID,Yung L. Y. AaronORCID,Zabelle BonnabelleORCID

Abstract

Abstract The UltraViolet Imaging of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey Fields (UVCANDELS) survey provided ultraviolet F275W imaging with coordinated parallel optical F435W imaging in four of the five CANDELS fields: GOODS-N, GOODS-S, EGS, and COSMOS, covering a total area of ∼426 arcmin2. UVCANDELS takes primary WFC3/UVIS F275W exposures at a uniform 3-orbit depth and ACS F435W exposures (in parallel) at slightly varying depth due to the roll angle constraints and the overlap from the increased field of view of the ACS camera, reaching a limiting magnitude of ∼27 and ∼28 ABmag (5σ in 0.″2 apertures) for F275W and F435W, respectively. We present the results of the UVCANDELS observations, custom calibrations, and the creation of F275W and F435W imaging mosaics, which have been made publicly available on the Barbara A. Mikulski Archive for Space Telescopes.

Publisher

American Astronomical Society

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