paper

B-fields In STar-forming Region Observations (BISTRO): Technical Foundations for Quantitative 450/850 m JCMT SCUBA-2/POL-2 Polarimetry

arXiv:2610.29273

Abstract

We present five technical validations of SCUBA-2/POL-2 polarimetry on the James Clerk Maxwell Telescope at 450 and 850 m, using 174 archival fields in 69 molecular cloud regions and subsets appropriate to each test. Extended-source calibration avoids a deterministic shift of in the dust emissivity index that would result from calibrating extended emission using peak brightness. We modeled Stokes noise with additive and signal-dependent components. The measured median ratio of surface-brightness noise at 450/850 m is 25. Independent tests of Stokes noise support approximately equal additive variances and weak error correlations, providing a basis for propagating polarization uncertainties. Corrections determined for individual fields reduce additive zero-level offsets of order mJy arcsec in the 450 m Stokes and intensities. The three-step regression leaves a median combined residual amplitude of mJy arcsec. Independent comparisons with SOFIA/HAWC+ at 154 and 214 m support the correction in strongly affected fields. We matched the 450 m maps to the modeled 850 m beam and the common - range of angular scales. We compared three reductions of the same 450 m observations across 30 sources. Taking the median angular residual relative to the final product for each source, we find that beam matching reduces the median over sources from to . After matching, 29 of the 30 sources have median residuals below . We also quantified how residual offsets propagate in ratios of polarization fractions, differences in spectral indices, and polarization angles. These validations provide procedures and quantitative references for interpreting POL-2 measurements and combining them with polarimetry at other wavelengths.

arXiv comment75 pages, 33 figures, 10 tables. Submitted to PASJ. Paper T of a series of three (Papers T, S1, and S2); Paper S1 is posted at the same time, and Paper S2 will be posted in November 2026. The submitted versions of all three papers are available at https://github.com/450um1G/PASJ2026