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- W4297183386 startingPage "140" @default.
- W4297183386 abstract "ABSTRACT We present a supervised machine learning classification of stellar populations in the Local Group spiral galaxy M 33. The Probabilistic Random Forest (PRF) methodology, previously applied to populations in NGC 6822, utilizes both near and far-IR classification features. It classifies sources into nine target classes: young stellar objects (YSOs), oxygen, and carbon-rich asymptotic giant branch stars, red giant branch, and red super-giant stars, active galactic nuclei, blue stars (e.g. O-, B-, and A-type main sequence stars), Wolf–Rayet stars, and Galactic foreground stars. Across 100 classification runs the PRF classified 162 746 sources with an average estimated accuracy of ∼86 per cent, based on confusion matrices. We identified 4985 YSOs across the disc of M 33, applying a density-based clustering analysis to identify 68 star forming regions (SFRs) primarily in the galaxy’s spiral arms. SFR counterparts to known H ii regions were recovered with ∼91 per cent of SFRs spatially coincident with giant molecular clouds identified in the literature. Using photometric measurements, as well as SFRs in NGC 6822 with an established evolutionary sequence as a benchmark, we employed a novel approach combining ratios of [Hα]/[24 μm] and [250 μm]/[500 μm] to estimate the relative evolutionary status of all M 33 SFRs. Masses were estimated for each YSO ranging from 6–27M⊙. Using these masses, we estimate star formation rates based on direct YSO counts of 0.63M⊙ yr−1 in M 33’s SFRs, 0.79 ± 0.16M⊙ yr−1 in its centre and 1.42 ± 0.16M⊙ yr−1 globally." @default.
- W4297183386 created "2022-09-27" @default.
- W4297183386 creator A5019066699 @default.
- W4297183386 creator A5037517484 @default.
- W4297183386 creator A5089033481 @default.
- W4297183386 date "2022-09-23" @default.
- W4297183386 modified "2023-10-16" @default.
- W4297183386 title "Massive young stellar objects in the Local Group spiral galaxy M 33 identified using machine learning" @default.
- W4297183386 cites W1657984092 @default.
- W4297183386 cites W1673633760 @default.
- W4297183386 cites W1871201175 @default.
- W4297183386 cites W1934387688 @default.
- W4297183386 cites W1967340141 @default.
- W4297183386 cites W1974782564 @default.
- W4297183386 cites W1975889887 @default.
- W4297183386 cites W1977412786 @default.
- W4297183386 cites W1979643632 @default.
- W4297183386 cites W1989718437 @default.
- W4297183386 cites W1991376423 @default.
- W4297183386 cites W1991559510 @default.
- W4297183386 cites W1995712697 @default.
- W4297183386 cites W1996538303 @default.
- W4297183386 cites W1999206227 @default.
- W4297183386 cites W2003897756 @default.
- W4297183386 cites W2003963647 @default.
- W4297183386 cites W2006813182 @default.
- W4297183386 cites W2007550785 @default.
- W4297183386 cites W2010008378 @default.
- W4297183386 cites W2010376972 @default.
- W4297183386 cites W2012244633 @default.
- W4297183386 cites W2018892872 @default.
- W4297183386 cites W2020596135 @default.
- W4297183386 cites W2026380070 @default.
- W4297183386 cites W2040322225 @default.
- W4297183386 cites W2041522238 @default.
- W4297183386 cites W2043452159 @default.
- W4297183386 cites W2043481277 @default.
- W4297183386 cites W2044669640 @default.
- W4297183386 cites W2054285578 @default.
- W4297183386 cites W2054318713 @default.
- W4297183386 cites W2055674375 @default.
- W4297183386 cites W2061574746 @default.
- W4297183386 cites W2062041224 @default.
- W4297183386 cites W2071306955 @default.
- W4297183386 cites W2073768640 @default.
- W4297183386 cites W2074238959 @default.
- W4297183386 cites W2077456416 @default.
- W4297183386 cites W2078958044 @default.
- W4297183386 cites W2080415259 @default.
- W4297183386 cites W2081383117 @default.
- W4297183386 cites W2086870800 @default.
- W4297183386 cites W2094429833 @default.
- W4297183386 cites W2095299194 @default.
- W4297183386 cites W2095558928 @default.
- W4297183386 cites W2096967293 @default.
- W4297183386 cites W2100163833 @default.
- W4297183386 cites W2102617261 @default.
- W4297183386 cites W2104471998 @default.
- W4297183386 cites W2120031672 @default.
- W4297183386 cites W2121404382 @default.
- W4297183386 cites W2121769952 @default.
- W4297183386 cites W2123267088 @default.
- W4297183386 cites W2125769353 @default.
- W4297183386 cites W2134710691 @default.
- W4297183386 cites W2135536375 @default.
- W4297183386 cites W2135615167 @default.
- W4297183386 cites W2135706491 @default.
- W4297183386 cites W2136206232 @default.
- W4297183386 cites W2147495837 @default.
- W4297183386 cites W2157791991 @default.
- W4297183386 cites W2164477565 @default.
- W4297183386 cites W2165760757 @default.
- W4297183386 cites W2167240457 @default.
- W4297183386 cites W2168110081 @default.
- W4297183386 cites W2231522987 @default.
- W4297183386 cites W2521932491 @default.
- W4297183386 cites W2526935107 @default.
- W4297183386 cites W2527802371 @default.
- W4297183386 cites W2574572616 @default.
- W4297183386 cites W2603070244 @default.
- W4297183386 cites W2606347516 @default.
- W4297183386 cites W2626779244 @default.
- W4297183386 cites W2772362066 @default.
- W4297183386 cites W2782918619 @default.
- W4297183386 cites W2806294049 @default.
- W4297183386 cites W2885863503 @default.
- W4297183386 cites W2900295657 @default.
- W4297183386 cites W2900872689 @default.
- W4297183386 cites W2911964244 @default.
- W4297183386 cites W2971875487 @default.
- W4297183386 cites W2972924288 @default.
- W4297183386 cites W3005329058 @default.
- W4297183386 cites W3014478080 @default.
- W4297183386 cites W3023688150 @default.
- W4297183386 cites W3042750865 @default.
- W4297183386 cites W3081225043 @default.
- W4297183386 cites W3086716767 @default.
- W4297183386 cites W3098416385 @default.