2011ApJ...741...14B


Query : 2011ApJ...741...14B

2011ApJ...741...14B - Astrophys. J., 741, 14 (2011/November-1)

Classifying structures in the interstellar medium with support vector machines: the G16.05-0.57 supernova remnant.

BEAUMONT C.N., WILLIAMS J.P. and GOODMAN A.A.

Abstract (from CDS):

We apply Support Vector Machines (SVMs)–a machine learning algorithm–to the task of classifying structures in the interstellar medium (ISM). As a case study, we present a position-position-velocity (PPV) data cube of 12CO J = 3-2 emission toward G16.05-0.57, a supernova remnant that lies behind the M17 molecular cloud. Despite the fact that these two objects partially overlap in PPV space, the two structures can easily be distinguished by eye based on their distinct morphologies. The SVM algorithm is able to infer these morphological distinctions, and associate individual pixels with each object at >90% accuracy. This case study suggests that similar techniques may be applicable to classifying other structures in the ISM–a task that has thus far proven difficult to automate.

Abstract Copyright:

Journal keyword(s): ISM: individual (G16.05-0.57, M17) - ISM: supernova remnants - techniques: image processing

Simbad objects: 5

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Number of rows : 5
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2023
#notes
1 NAME Orion-KL SFR 05 35 14.16 -05 22 21.5           ~ 2251 1
2 IC 443 SNR 06 17 34.7 +22 28 03           ~ 1219 1
3 NGC 6618 OpC 18 20 47 -16 10.3           ~ 1589 0
4 SNR G016.0-00.5 SNR 18 21.9 -15 14           ~ 19 0
5 NAME Scutum Spiral Arm PoG ~ ~           ~ 340 0

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2023.09.27-12:44:48

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