arXiv · 1703.01000
The M33 Synoptic Stellar Survey. II. Mira Variables
Abstract
We present the discovery of 1847 Mira candidates in the Local Group galaxy M33 using a novel semi-parametric periodogram technique coupled with a Random Forest classifier. The algorithms were applied to ~2.4x10^5 I-band light curves previously obtained by the M33 Synoptic Stellar Survey. We derive preliminary Period-Luminosity relations at optical, near- & mid-infrared wavelengths and compare them to the corresponding relations in the Large Magellanic Cloud.
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Wenlong Yuan, Shiyuan He, Lucas M. Macri, James Long, Jianhua Z. Huang. 2017-03-24. The M33 Synoptic Stellar Survey. II. Mira Variables. https://doi.org/10.3847/1538-3881%2Faa63f1
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