2005
DOI: 10.1111/j.1365-2966.2005.08930.x
|View full text |Cite
|
Sign up to set email alerts
|

Applying machine learning to catalogue matching in astrophysics

Abstract: We present the results of applying automated machine learning techniques to the problem of matching different object catalogues in astrophysics. In this study, we take two partially matched catalogues where one of the two catalogues has a large positional uncertainty. The two catalogues we used here were taken from the H i Parkes All Sky Survey (HIPASS) and SuperCOSMOS optical survey. Previous work had matched 44 per cent (1887 objects) of HIPASS to the SuperCOSMOS catalogue. A supervised learning algorithm wa… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
1
1

Citation Types

0
19
0

Year Published

2006
2006
2022
2022

Publication Types

Select...
4
3
1

Relationship

0
8

Authors

Journals

citations
Cited by 19 publications
(19 citation statements)
references
References 24 publications
0
19
0
Order By: Relevance
“…Such an approach fits within a broad theme in the literature of using not only the counterpart's celestial position, but some property such as its color, morphology, or spectral energy distribution (e.g., Roseboom et al 2009), or even a combination of several properties (Rohde et al 2005(Rohde et al , 2006 to assign the likelihood of it being the counterpart. Although we do not know of such techniques being used for Galactic astronomy before, they are widely used in extra-galactic work, and most techniques trace their origins back to an increasingly influential paper by Sutherland & Saunders (1992).…”
Section: The Outline Solutionmentioning
confidence: 99%
“…Such an approach fits within a broad theme in the literature of using not only the counterpart's celestial position, but some property such as its color, morphology, or spectral energy distribution (e.g., Roseboom et al 2009), or even a combination of several properties (Rohde et al 2005(Rohde et al , 2006 to assign the likelihood of it being the counterpart. Although we do not know of such techniques being used for Galactic astronomy before, they are widely used in extra-galactic work, and most techniques trace their origins back to an increasingly influential paper by Sutherland & Saunders (1992).…”
Section: The Outline Solutionmentioning
confidence: 99%
“…In that case, spatial proximity alone cannot judge between the potential counterparts from A of each source in B, and it is necessary to either introduce prior astrophysical knowledge to help identify the most likely match, or use a machine learning algorithm [9,10]. Machine learning algorithms deduce relationships between the properties of the sources in the two catalogues and can aid the finding of associations between them.…”
Section: Matching Celestial Objects In Astronomy Cataloguesmentioning
confidence: 99%
“…Cao et al, 2006;Rohde et al, 2005Rohde et al, , 2006, especially for analyzing the vast amount of data being collected by sky surveys (e.g., SDSS). Simple matching approaches such as the 'closest match,' which depend on positions only, are considered adequate only when the positional uncertainties of the matched catalogues are all very small (e.g., matching SDSS and Spitzer IRAC catalogues, Wu et al, 2005).…”
Section: Introductionmentioning
confidence: 99%
“…Rohde et al (2005) applied automated machine learning techniques to the problem of matching catalogues where one of the two has large positional uncertainties. In their study, a model was first constructed based on a supervised learning algorithm and a set of training data.…”
Section: Introductionmentioning
confidence: 99%