%0 Generic %1 krumholz2015cluster %A Krumholz, Mark R. %A Adamo, Angela %A Fumagalli, Michele %A Wofford, Aida %A Calzetti, Daniela %A Lee, Janice C. %A Whitmore, Bradley C. %A Bright, Stacey N. %A Grasha, Kathryn %A Gouliermis, Dimitrios A. %A Kim, Hwihyun %A Nair, Preethi %A Ryon, Jenna E. %A Smith, Linda J. %A Thilker, David %A Ubeda, Leonardo %A Zackrisson, Erik %D 2015 %K cluster slug star stochastic %T Star Cluster Properties in Two LEGUS Galaxies Computed with Stochastic Stellar Population Synthesis Models %U http://arxiv.org/abs/1509.05078 %X We investigate a novel Bayesian analysis method, based on the Stochastically Lighting Up Galaxies (slug) code, to derive the masses, ages, and extinctions of star clusters from integrated light photometry. Unlike many analysis methods, slug correctly accounts for incomplete IMF sampling, and returns full posterior probability distributions rather than simply probability maxima. We apply our technique to 621 visually-confirmed clusters in two nearby galaxies, NGC 628 and NGC 7793, that are part of the Legacy Extragalactic UV Survey (LEGUS). LEGUS provides Hubble Space Telescope photometry in the NUV, U, B, V, and I bands. We analyze the sensitivity of the derived cluster properties to choices of prior probability distribution, evolutionary tracks, IMF, metallicity, treatment of nebular emission, and extinction curve. We find that slug's results for individual clusters are insensitive to most of these choices, but that the posterior probability distributions we derive are often quite broad, and sometimes multi-peaked and quite sensitive to the choice of priors. In contrast, the properties of the cluster population as a whole are relatively robust against all of these choices. We also compare our results from slug to those derived with a conventional non-stochastic fitting code, Yggdrasil. We show that slug's stochastic models are generally a better fit to the observations than the deterministic ones used by Yggdrasil. However, the overall properties of the cluster populations recovered by both codes are qualitatively similar.

@misc{krumholz2015cluster, abstract = {We investigate a novel Bayesian analysis method, based on the Stochastically Lighting Up Galaxies (slug) code, to derive the masses, ages, and extinctions of star clusters from integrated light photometry. Unlike many analysis methods, slug correctly accounts for incomplete IMF sampling, and returns full posterior probability distributions rather than simply probability maxima. We apply our technique to 621 visually-confirmed clusters in two nearby galaxies, NGC 628 and NGC 7793, that are part of the Legacy Extragalactic UV Survey (LEGUS). LEGUS provides Hubble Space Telescope photometry in the NUV, U, B, V, and I bands. We analyze the sensitivity of the derived cluster properties to choices of prior probability distribution, evolutionary tracks, IMF, metallicity, treatment of nebular emission, and extinction curve. We find that slug's results for individual clusters are insensitive to most of these choices, but that the posterior probability distributions we derive are often quite broad, and sometimes multi-peaked and quite sensitive to the choice of priors. In contrast, the properties of the cluster population as a whole are relatively robust against all of these choices. We also compare our results from slug to those derived with a conventional non-stochastic fitting code, Yggdrasil. We show that slug's stochastic models are generally a better fit to the observations than the deterministic ones used by Yggdrasil. However, the overall properties of the cluster populations recovered by both codes are qualitatively similar.}, added-at = {2015-09-18T10:29:46.000+0200}, author = {Krumholz, Mark R. and Adamo, Angela and Fumagalli, Michele and Wofford, Aida and Calzetti, Daniela and Lee, Janice C. and Whitmore, Bradley C. and Bright, Stacey N. and Grasha, Kathryn and Gouliermis, Dimitrios A. and Kim, Hwihyun and Nair, Preethi and Ryon, Jenna E. and Smith, Linda J. and Thilker, David and Ubeda, Leonardo and Zackrisson, Erik}, biburl = {https://www.bibsonomy.org/bibtex/2452dfa70344aeb3f2ff0933fe9b286d7/miki}, description = {[1509.05078] Star Cluster Properties in Two LEGUS Galaxies Computed with Stochastic Stellar Population Synthesis Models}, interhash = {9bd8a1d29fc9d0ccab159781454e7ee0}, intrahash = {452dfa70344aeb3f2ff0933fe9b286d7}, keywords = {cluster slug star stochastic}, note = {cite arxiv:1509.05078Comment: Accepted to ApJ; 25 pages, 17 figures, 3 tables; machine-readable versions of the tables are available at https://sites.google.com/a/ucsc.edu/krumholz/publications}, timestamp = {2015-09-18T10:29:46.000+0200}, title = {Star Cluster Properties in Two LEGUS Galaxies Computed with Stochastic Stellar Population Synthesis Models}, url = {http://arxiv.org/abs/1509.05078}, year = 2015 }