2014ApJS..214....3B


Query : 2014ApJS..214....3B

2014ApJS..214....3B - Astrophys. J., Suppl. Ser., 214, 3 (2014/September-0)

The Milky Way Project: leveraging citizen science and machine learning to detect interstellar bubbles.

BEAUMONT C.N., GOODMAN A.A., KENDREW S., WILLIAMS J.P. and SIMPSON R.

Abstract (from CDS):

We present Brut, an algorithm to identify bubbles in infrared images of the Galactic midplane. Brut is based on the Random Forest algorithm, and uses bubbles identified by >35,000 citizen scientists from the Milky Way Project to discover the identifying characteristics of bubbles in images from the Spitzer Space Telescope. We demonstrate that Brut's ability to identify bubbles is comparable to expert astronomers. We use Brut to re-assess the bubbles in the Milky Way Project catalog, and find that 10%-30% of the objects in this catalog are non-bubble interlopers. Relative to these interlopers, high-reliability bubbles are more confined to the mid-plane, and display a stronger excess of young stellar objects along and within bubble rims. Furthermore, Brut is able to discover bubbles missed by previous searches–particularly bubbles near bright sources which have low contrast relative to their surroundings. Brut demonstrates the synergies that exist between citizen scientists, professional scientists, and machine learning techniques. In cases where "untrained" citizens can identify patterns that machines cannot detect without training, machine learning algorithms like Brut can use the output of citizen science projects as input training sets, offering tremendous opportunities to speed the pace of scientific discovery. A hybrid model of machine learning combined with crowdsourced training data from citizen scientists can not only classify large quantities of data, but also address the weakness of each approach if deployed alone.

Abstract Copyright: ∼

Journal keyword(s): H II regions - ISM: bubbles - methods: data analysis - stars: formation

Simbad objects: 15

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Number of rows : 15
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME Dragonfish Nebula SFR 12 11 -62.9           ~ 10 0
2 [ABB2014] WISE G309.075+00.172 bub 13 44 08.3 -62 04 38           ~ 7 0
3 [ABB2014] WISE G312.979-00.432 bub 14 17 31.3 -61 37 00           ~ 10 0
4 [ABB2014] WISE G316.796-00.056 bub 14 45 13.2 -59 51 13           ~ 10 0
5 [ABB2014] WISE G316.875+00.041 bub 14 45 36.0 -59 43 38           ~ 4 0
6 [ABB2014] WISE G331.020-00.143 bub 16 10 00.0 -51 51 05           ~ 7 0
7 [ABB2014] WISE G345.486+00.399 bub 17 04 05.7 -40 43 26           ~ 8 0
8 [ABB2014] WISE G348.261+00.485 bub 17 12 24.0 -38 27 14           ~ 5 0
9 [ABB2014] WISE G354.175-00.062 bub 17 31 14.9 -33 52 55           ~ 10 0
10 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 16269 0
11 [JDP2019] MWP2G0058964-0045843 bub 18 00 46.9 -24 05 24           ~ 3 0
12 [ABB2014] WISE G013.725-00.024 bub 18 15 24.5 -17 01 32           ~ 9 0
13 [ABB2014] WISE G018.253-00.298 bub 18 25 17.1 -13 09 56           ~ 25 0
14 [ABB2014] WISE G018.187-00.415 bub 18 25 31.8 -13 16 26           ~ 5 0
15 NAME Sgr Arm PoG 19 00 -30.0           ~ 710 1

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