VizieR Online Data Catalog: SCUBA 2 Cosmology Legacy Survey (Geach+, 2017)

JE Geach,JS Dunlop,M Halpern, I Smail,P van der Werf, DM Alexander,O Almaini,I Aretxaga,V Arumugam, V Asboth,M Banerji, J Beanlands, PN Best,AW Blain, M Birkinshaw, EL Chapin,SC Chapman,C-C Chen, A Chrysostomou,C Clarke,DL Clements, C Conselice,KEK Coppin, WI Cowley,ALR Danielson,S Eales, AC Edge,D Farrah,A Gibb, CM Harrison,NK Hine, D Hughes, RJ Ivison, M Jarvis,T Jenness, SF Jones,A Karim,M Koprowski,KK Knudsen, CG Lacey,T MacKenzie, G Marsden,K McAlpine,R McMahon,R Meijerink,MJ Michalowski, SJ Oliver, MJ Page, JA Peacock, D Rigopoulou, EI Robson,I Roseboom,K Rotermund,D Scott,S Serjeant,C Simpson, JM Simpson, DJB Smith, M Spaans, F Stanley,JA Stevens,AM Swinbank,T Targett, AP Thomson,E Valiante,DA Wake, TMA Webb, C Willott,JA Zavala,M Zemcov

yCat（2018）

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摘要

The S2CLS survey has two tiers: wide and deep. The wide tier covers several well-explored extragalactic survey fields: Akari-Northern Ecliptic Pole, COSMOS, Extended Groth Strip, GOODS-North, Lockman Hole North, SSA22 and UKIDSS-UDS, mapping at 850um during conditions where the zenith optical depth at 225GHz was 0.05<{tau} 225<= 0.1 and field elevations exceeded 30. In the deep tier, several deep'keyhole'regions within the wide fields were mapped when {tau} 225<= 0.05, conditions suitable for obtaining 450um maps which require the lowest opacities (Geach et al., 2013MNRAS. 432... 53G). Note that SCUBA-2 simultaneously records 450um and 850um photons, and while the complementary 450um data exist for the wide 850um maps we present here, they have not been processed, since they are not expected to be of sufficient quality given the observing conditions. In this paper, we present the …

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