Open Access

Table 1

Summary of model setup and behaviour for the selected star formation regions.

Orion Cygnus X Perseus Taurus
l bounds (°) 180 ≤ l ≤ 217 73 ≤ l ≤ 87 154 ≤ l ≤ 164 165 ≤ l ≤ 180
b bounds (°) −25.5 ≤ b ≤−3.8 −4 ≤ b ≤ 6 −25 ≤ b ≤−14 −20 ≤ b ≤−10
d bounds (pc) 250 ≤ d ≤ 550 800 ≤ d ≤ 2200 180 ≤ d ≤ 500 40 ≤ d ≤ 350
Stars incorporated from (pc) 270 1200 200 90
Training nl, nb, nd (cells) 40, 40, 55 40, 40, 65 30, 30, 35 30, 30, 35
Training resolution (pc) 2.3 3.5 1.0 0.23
Number of sources 87283 703291 92829 107051
Initial scale length (x, y, z; pc) 10 15 10 5
Final scale length (x, y, z; pc) 9.5, 9.3, 9.5 19.1, 19.1, 19.2 12.8, 5.8, 6.4 9.2, 6.7, 4.9
Initial mean density (mag pc−1) 4.6 × 10−4 3.0 × 10−3 4.6 × 10−4 1.5 × 10−3
Final mean density (mag pc−1) 1.06 × 10−3 1.2 × 10−3 6.0 × 10−4 1.1 × 10−3
Initial scale factor (dex) 0.297 0.060 0.297 0.291
Final scale factor (dex) 0.231 0.057 0.293 0.136
Learning rate 0.01 0.01 0.01 0.005
Number of iterations 500 500 1000 1500
Number of inducing points 1000 1000 1000 500
Predicting nl, nb, nd (cells) 100, 100, 105 100, 100, 105 100, 100, 105 100, 100, 105
Predicting resolution (pc) 0.9 1.4 0.3 0.07
Run time (hours) (1) 132 287 39 59

Notes. (1) The run times quoted here are the wall clock times for a machine setup of a single node with 2 × Intel(R) Xeon(R) CPU E5-2680 v3 at 2.50 GHz, no hyperthreading, 24 cores, 180 GB RAM.

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