An improved quasar detection method in EROS-2 and MACHO LMC datasets
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Abstract (arXiv)
We present a new classification method for quasar identification in the EROS-2 and MACHO datasets based on a boosted version of Random Forest classifier. We use a set of variability features including parameters of a continuous auto regressive model. We prove that continuous auto regressive parameters are very important discriminators in the classification process. We create two training sets (one for EROS-2 and one for MACHO datasets) using known quasars found in the LMC. Our model's accuracy in both EROS-2 and MACHO training sets is about 90% precision and 86% recall, improving the state of the art models accuracy in quasar detection. We apply the model on the complete, including 28 million objects, EROS-2 and MACHO LMC datasets, finding 1160 and 2551 candidates respectively. To further validate our list of candidates, we crossmatched our list with a previous 663 known strong candidates, getting 74% of matches for MACHO and 40% in EROS-2. The main difference on matching level is because EROS-2 is a slightly shallower survey which translates to significantly lower signal-to-noise ratio lightcurves.
Key facts. Cited by 3 papers in the map (data through 7 Oct 2026). First posted on arXiv 1 Apr 2013.
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Citing papers per year: 2021: 2; 2022: 0; 2023: 1.
3 papers.
- 2021Informative Bayesian model selection for RR Lyrae star classifierscited by 1
- 2021The effect of phased recurrent units in the classification of multiple catalogs of astronomical lightcurvescited by 1
- 2023Informative regularization for a multi-layer perceptron RR Lyrae classifier under data shiftcited by 0
- 2023Informative regularization for a multi-layer perceptron RR Lyrae classifier under data shift12 Mar 2023
- 2021The effect of phased recurrent units in the classification of multiple catalogs of astronomical lightcurves7 Jun 2021
- 2021Informative Bayesian model selection for RR Lyrae star classifiers24 May 2021