The JCMT Gould Belt Survey: A Quantitative Comparison Between SCUBA-2 Data Reduction Methods
S. Mairs, D. Johnstone, H. Kirk, S. Graves, J. Buckle, S.F. Beaulieu,, D.S. Berry, H. Broekhoven-Fiene, M.J. Currie, M. Fich, J. Hatchell, T., Jenness, J.C. Mottram, D. Nutter, K. Pattle, J.E. Pineda, C. Salji, J. Di, Francesco, M.R. Hogerheijde, D. Ward-Thompson

TL;DR
This study compares two data reduction methods for SCUBA-2 submillimetre observations, highlighting their suitability for different astrophysical analyses and emphasizing the importance of parameter choices in data processing.
Contribution
It provides a quantitative comparison of two reduction methods, demonstrating how parameter tuning affects the recovery of compact and extended astronomical structures.
Findings
GBS LR1 recovers compact sources at low brightness levels
JCMT LR1 is better for detecting compact emission presence
Extended structures require careful boundary setting to avoid errors
Abstract
Performing ground-based submillimetre observations is a difficult task as the measurements are subject to absorption and emission from water vapour in the Earth's atmosphere and time variation in weather and instrument stability. Removing these features and other artifacts from the data is a vital process which affects the characteristics of the recovered astronomical structure we seek to study. In this paper, we explore two data reduction methods for data taken with the Submillimetre Common-User Bolometer Array-2 (SCUBA-2) at the James Clerk Maxwell Telescope (JCMT). The JCMT Legacy Reduction 1 (JCMT LR1) and The Gould Belt Legacy Survey Legacy Release 1 (GBS LR1) reduction both use the same software, Starlink, but differ in their choice of data reduction parameters. We find that the JCMT LR1 reduction is suitable for determining whether or not compact emission is present in a given…
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