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@article{Smith:2019:mnras/stz1102,
author = {Smith, MWL and Clark, CJR and De, Looze I and Lamperti, I and Saintonge, A and Wilson, CD and Accurso, G and Brinks, E and Bureau, M and Chung, EJ and Cigan, PJ and Clements, DL and Dharmawardena, T and Fanciullo, L and Gao, Y and Gao, Y and Gear, WK and Gomez, HL and Greenslade, J and Hwang, HS and Kemper, F and Lee, JC and Li, C and Lin, L and Liu, L and Molnar, DC and Mok, A and Pan, H-A and Sargent, M and Scicluna, P and Smith, CMA and Urquhart, S and Williams, TG and Xiao, T and Yang, C and Zhu, M},
doi = {mnras/stz1102},
journal = {Monthly Notices of the Royal Astronomical Society},
pages = {4166--4185},
title = {JINGLE, a JCMT legacy survey of dust and gas for galaxy evolution studies: II. SCUBA-2 850 mu m data reduction and dust flux density catalogues},
url = {http://dx.doi.org/10.1093/mnras/stz1102},
volume = {486},
year = {2019}
}

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TY  - JOUR
AB  - We present the SCUBA-2 850μm component of JINGLE, the new JCMT large survey for dust and gas in nearby galaxies, which with 193 galaxies is the largest targeted survey of nearby galaxies at 850 μm. We provide details of our SCUBA-2 data reduction pipeline, optimized for slightly extended sources, and including a calibration model adjusted to match conventions used in other far-infrared (FIR) data. We measure total integrated fluxes for the entire JINGLE sample in 10 infrared/submillimetre bands, including all WISE, Herschel-PACS, Herschel-SPIRE, and SCUBA-2 850 μm maps, statistically accounting for the contamination by CO(J = 3–2) in the 850 μm band. Of our initial sample of 193 galaxies, 191 are detected at 250 μm with a ≥5σ significance. In the SCUBA-2 850 μm band we detect 126 galaxies with ≥3σ significance. The distribution of the JINGLE galaxies in FIR/sub-millimetre colour–colour plots reveals that the sample is not well fit by single modified-blackbody models that assume a single dust-emissivity index (β). Instead, our new 850 μm data suggest either that a large fraction of our objects require β < 1.5, or that a model allowing for an excess of sub-mm emission (e.g. a broken dust emissivity law, or a very cold dust component 10 K) is required. We provide relations to convert FIR colours to dust temperature and β for JINGLE-like galaxies. For JINGLE the FIR colours correlate more strongly with star-formation rate surface-density rather than the stellar surface-density, suggesting heating of dust is greater due to younger rather than older stellar-populations, consistent with the low proportion of early-type galaxies in the sample.
AU  - Smith,MWL
AU  - Clark,CJR
AU  - De,Looze I
AU  - Lamperti,I
AU  - Saintonge,A
AU  - Wilson,CD
AU  - Accurso,G
AU  - Brinks,E
AU  - Bureau,M
AU  - Chung,EJ
AU  - Cigan,PJ
AU  - Clements,DL
AU  - Dharmawardena,T
AU  - Fanciullo,L
AU  - Gao,Y
AU  - Gao,Y
AU  - Gear,WK
AU  - Gomez,HL
AU  - Greenslade,J
AU  - Hwang,HS
AU  - Kemper,F
AU  - Lee,JC
AU  - Li,C
AU  - Lin,L
AU  - Liu,L
AU  - Molnar,DC
AU  - Mok,A
AU  - Pan,H-A
AU  - Sargent,M
AU  - Scicluna,P
AU  - Smith,CMA
AU  - Urquhart,S
AU  - Williams,TG
AU  - Xiao,T
AU  - Yang,C
AU  - Zhu,M
DO  - mnras/stz1102
EP  - 4185
PY  - 2019///
SN  - 0035-8711
SP  - 4166
TI  - JINGLE, a JCMT legacy survey of dust and gas for galaxy evolution studies: II. SCUBA-2 850 mu m data reduction and dust flux density catalogues
T2  - Monthly Notices of the Royal Astronomical Society
UR  - http://dx.doi.org/10.1093/mnras/stz1102
UR  - http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000474903500091&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202
UR  - https://academic.oup.com/mnras/article/486/3/4166/5472920
UR  - http://hdl.handle.net/10044/1/80468
VL  - 486
ER  -

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