Table G.1
Statistics of spectral index β distributions for different versions of the data.
θF a (′′) | Maskb | Aperture c | β(3 bands, U d) | β(3 bands, F e) | β(4 bands, F) | Clumps |
---|---|---|---|---|---|---|
FCF = 2.41 Jy (pW)−1 arcsec−2 | ||||||
500 | LM | τall | 1.72, 1.94, 2.07 | 1.69, 1.99, 2.29 | 1.38, 1.59, 1.86 | 27 |
200 | LM | τall | 1.73, 1.90, 2.04 | 1.75, 2.09, 2.50 | 1.53, 1.83, 2.12 | 29 |
500 | SM | τall | 1.69, 1.92, 2.04 | 1.73, 1.91, 2.22 | 1.38, 1.69, 1.84 | 17 |
200 | SM | τall | 1.74, 1.89, 2.06 | 1.83, 1.99, 2.41 | 1.51, 1.77, 1.91 | 18 |
500 | LM | τhigh | 1.64, 1.77, 1.93 | 1.70, 1.88, 2.17 | 1.40, 1.52, 1.65 | 22 |
200 | LM | τhigh | 1.62, 1.74, 1.97 | 1.88, 2.03, 2.29 | 1.41, 1.58, 1.76 | 23 |
500 | SM | τhigh | 1.54, 1.75, 1.93 | 1.55, 1.72, 1.92 | 1.23, 1.46, 1.61 | 14 |
200 | SM | τhigh | 1.68, 1.85, 1.98 | 1.92, 2.07, 2.22 | 1.31, 1.50, 1.72 | 15 |
200 | M850 | τall | 1.68, 1.82, 2.00 | 1.81, 2.04, 2.32 | 1.42, 1.67, 1.86 | 13 |
200 | No | τall | 1.61, 1.75, 1.98 | 2.12, 2.69, 3.08 | 2.11, 2.49, 2.85 | 16 |
FCF = 2.34 Jy (pW)−1 arcsec−2 | ||||||
500 | LM | τall | 1.69, 1.90, 2.06 | 1.69, 1.99, 2.34 | 1.43, 1.63, 1.91 | 27 |
200 | LM | τall | 1.73, 1.90, 2.04 | 1.75, 2.09, 2.50 | 1.58, 1.84, 2.12 | 29 |
500 | SM | τall | 1.63, 1.92, 2.04 | 1.73, 1.89, 2.17 | 1.48, 1.72, 1.88 | 17 |
200 | SM | τall | 1.69, 1.89, 2.06 | 1.76, 1.98, 2.40 | 1.53, 1.78, 1.96 | 18 |
500 | LM | τhigh | 1.64, 1.79, 1.93 | 1.70, 1.89, 2.30 | 1.44, 1.56, 1.66 | 22 |
200 | LM | τhigh | 1.62, 1.75, 1.99 | 1.88, 2.03, 2.38 | 1.48, 1.62, 1.78 | 23 |
500 | SM | τhigh | 1.53, 1.73, 1.89 | 1.54, 1.68, 1.89 | 1.28, 1.46, 1.64 | 14 |
200 | SM | τhigh | 1.68, 1.85, 1.98 | 1.92, 2.07, 2.22 | 1.35, 1.55, 1.75 | 15 |
200 | M850 | τall | 1.67, 1.81, 2.00 | 1.79, 2.04, 2.37 | 1.44, 1.70, 1.89 | 13 |
200 | No | τall | 1.61, 1.74, 1.97 | 2.15, 2.71, 3.09 | 2.09, 2.52, 3.00 | 16 |
Notes. The listed β values are the 25%, 50%, and 75% percentiles for the clumps in the P(χ2 ) = 25% samples. (a) Filtering scale in the SCUBA-2 map making. (b) Small or large masks made based on Herschel data. See Appendix C. (c) Apertures corresponding to Fellwalker clump footprints (τall) or, within them, only pixels above the median τ(250μm) value (τhigh). (d) U refers to original SPIRE data. (e) F refers to SPIRE maps processed through the SCUBA-2 pipeline.
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