Accounting for Stochastic Fluctuations when Analysing Integrated Light of Star Clusters. I: First Systematics
arXiv:1003.2334 · doi:10.1051/0004-6361/201014084
Abstract
Star clusters are studied widely both as benchmarks for stellar evolution models and in their own right. Cluster age and mass distributions within galaxies are probes of star formation histories, and of cluster formation and disruption processes. The vast majority of clusters in the Universe is small, and it is well known that the integrated fluxes and colors have broad probability distributions, due to small numbers of bright stars. This paper goes beyond the description of predicted probability distributions, and presents results of the analysis of cluster energy distributions in an explicitly stochastic context. The method developed is Bayesian. It provides posterior probability distributions in the age-mass-extinction space, using multi-wavelength photometric observations and a large collection of Monte-Carlo simulations of clusters of finite stellar masses. Both UBVI and UBVIK datasets are considered, and the study conducted in this paper is restricted to the solar metallicity. We first reassess and explain errors arising from the use of standard analysis methods, which are based on continuous population synthesis models: systematic errors on ages and random errors on masses are large, while systematic errors on masses tend to be smaller. The age-mass distributions obtained after analysis of a synthetic sample are very similar to those found for real galaxies in the literature. The Bayesian approach on the other hand, is very successful in recovering the input ages and masses. Taking stochastic effects into account is important, more important for instance than the choice of adding or removing near-IR data in many cases. We found no immediately obvious reason to reject priors inspired by previous (standard) analyses of cluster populations in galaxies, i.e. cluster distributions that scale with mass as M^-2 and are uniform on a logarithmic age scale.
17 pages, 13 figures, Accepted for publication in A&A.
References in corpus (6)
- Star formation efficiency in galaxy interactions and mergers: a statistical study
- New Tests for Disruption Mechanisms of Star Clusters: Methods and Application to the Antennae Galaxies
- Testing spectral models for stellar populations with star clusters: I. Methodology
- Testing spectral models for stellar populations with star clusters: II. Results
- MASSCLEANcolors - Mass Dependent Integrated Colors for Stellar Clusters Derived from 30 Million Monte Carlo Simulations -
- Why Simple Stellar Population models do not reproduce the colours of Galactic open clusters
Cited by in corpus (88)
- Star Clusters Across Cosmic Time
- Direct Oxygen Abundances for Low Luminosity LVL Galaxies
- SLUG - Stochastically Lighting Up Galaxies I: Methods and Validating Tests
- Probing the role of the galactic environment in the formation of stellar clusters; using M83 as a test bench
- Stellar Clusters in M83: Formation, evolution, disruption and the influence of environment
- SLUG -- Stochastically Lighting Up Galaxies. III: A Suite of Tools for Simulated Photometry, Spectroscopy, and Bayesian Inference with Stochastic Stellar Populations
- Studying the YMC population of M83: how long clusters remain embedded, their interaction with the ISM and implications for GC formation theories
- ASteCA - Automated Stellar Cluster Analysis
- Approximate Bayesian Computation for Astronomical Model Analysis: A Case Study in Galaxy Demographics and Morphological Transformation at High Redshift
- Constraining Globular Cluster Formation Through Studies of Young Massive Clusters: I. A lack of ongoing star formation within young clusters
- Using H-alpha Morphology and Surface Brightness Fluctuations to Age-Date Star Clusters in M83
- The star cluster - field star connection in nearby spiral galaxies. II. Field star and cluster formation histories and their relation
- Panchromatic Hubble Andromeda Treasury XVI. Star Cluster Formation Efficiency and the Clustered Fraction of Young Stars
- Panchromatic Hubble Andromeda Treasury XVIII. The High-mass Truncation of the Star Cluster Mass Function
- Effective Radii of Young, Massive Star Clusters in Two LEGUS Galaxies
- Detailed abundance analysis from integrated high-dispersion spectroscopy: Globular clusters in the Fornax Dwarf Spheroidal
- Star cluster formation in the most extreme environments: Insights from the HiPEEC survey
- PHAT Stellar Cluster Survey. II. Andromeda Project Cluster Catalog
- The Panchromatic Hubble Andromeda Treasury XV. The BEAST: Bayesian Extinction and Stellar Tool
- Discovery of Strongly Inverted Metallicity Gradients in Dwarf Galaxies at 2
- H Morphologies of Star Clusters: A LEGUS study of HII region evolution timescales and stochasticity in low mass clusters
- Analysing star cluster populations with stochastic models: the HST/WFC3 sample of clusters in M83
- Sizes and Shapes of Young Star Cluster Light Profiles in M83
- The Panchromatic Hubble Andromeda Treasury V: Ages and Masses of the Year 1 Stellar Clusters
- Age and Mass for 920 LMC Clusters Derived from 100 Million Monte Carlo Simulations
- Star Cluster Catalogs for the LEGUS Dwarf Galaxies
- The Next Generation Fornax Survey (NGFS): IV. Mass and Age Bimodality of Nuclear Clusters in the Fornax Core Region
- Resolved photometry of extragalactic young massive star clusters
- Star Clusters in Evolving Galaxies
- The Age Distribution of Clusters in M83
- On the Origin of Diffuse Ionized Gas in the Antennae Galaxy
- LEGUS and Halpha-LEGUS Observations of Star Clusters in NGC 4449: Improved Ages and the Fraction of Light in Clusters as a Function of Age
- The ACS Nearby Galaxy Survey Treasury. X. Quantifying the Star Cluster Formation Efficiency of Nearby Dwarf Galaxies
- Star Cluster Properties in Two LEGUS Galaxies Computed with Stochastic Stellar Population Synthesis Models
- Being WISE I: Validating Stellar Population Models and M/L ratios at 3.4 and 4.6 microns
- The stochastic nature of stellar population modelling
- H Morphologies of Star Clusters in 16 LEGUS Galaxies: Constraints on HII region evolution timescales
- The galactocentric radius dependent upper mass limit of young star clusters: stochastic star formation ruled out
- Revealing a Ring-like Cluster Complex in a Tidal Tail of the Starburst Galaxy NGC 2146
- Deriving physical parameters of unresolved star clusters. I. Age, mass, and extinction degeneracies
- The NGC 5253 star cluster system. I. Standard modelling and infrared-excess sources
- A variation of the fraction of stars that form in bound clusters within M83
- The Next Generation Virgo cluster Survey (NGVS). XXV. Fiducial panchromatic colors of Virgo core globular clusters and their comparison to model predictions
- Detailed abundances from integrated-light spectroscopy: Milky Way globular clusters
- The Panchromatic Hubble Andromeda Treasury III. Measuring Ages and Masses of Partially Resolved Stellar Clusters
- Improving Star Cluster Age Estimates in PHANGS-HST Galaxies and the Impact on Cluster Demographics in NGC 628
- Integrated J- and H-band spectra of globular clusters in the LMC: implications for stellar population models and galaxy age dating
- The Snapshot Hubble U-Band Cluster Survey (SHUCS). I. Survey Description and First Application to the Mixed Star Cluster Population of NGC 4041
- The Snapshot Hubble U-Band Cluster Survey (SHUCS) II. Star Cluster Population of NGC 2997
- Deriving physical parameters of unresolved star clusters. II. The degeneracies of age, mass, extinction, and metallicity
- Stellar associations powering HII regions $\unicode{x2013}$ I. Defining an evolutionary sequence
- High-Resolution Mapping of Dust via Extinction in the M31 Bulge
- Properties of the cluster population of NGC 1566 and their implications
- Crucial aspects of the initial mass function (I): The statistical correlation between the total mass of an ensemble of stars and its most massive star
- STEP Survey II: Structural Analysis of 170 star clusters in the SMC
- The Panchromatic Hubble Andromeda Treasury: Triangulum Extended Region (PHATTER). IV. Star Cluster Catalog
- Stochastic stellar cluster IMFs: Models and impact on integrated cluster parameter determination
- The evolution of luminosity, colour and the mass-to-luminosity ratio of Galactic open clusters: comparison of discrete vs. continuous IMF models
- The Prevalence and Impact of Wolf-Rayet Stars in Emerging Massive Star Clusters
- No compelling evidence of significant early star cluster disruption in the Large Magellanic Cloud
- An Emerging Wolf-Rayet Massive Star Cluster in NGC 4449
- A revisited study of Cepheids in open clusters in the Gaia era
- Optical-NIR analysis of globular clusters in the IKN dwarf spheroidal: a complex star formation history
- Synthetic photometry of OB star clusters with stochastically sampled IMFs: analysis of models and HST observations
- NLTE modelling of integrated light spectra. Abundances of barium, magnesium, and manganese in a metal-poor globular cluster
- Empirical SED Templates for Star Clusters Observed with HST and JWST: No Strong PAH or IR Dust Emission after Five Myr
- The effect of spatial resolution on optical and near-IR studies of stellar clusters: Implications for the origin of the red excess
- Deriving physical parameters of unresolved star clusters III. Application to M31 PHAT clusters
- The star cluster mass--galactocentric radius relation: Implications for cluster formation
- Linking stellar populations to HII regions across nearby galaxies. II. Infrared Reprocessed and UV Direct Radiation Pressure in HII Regions
- Arp 220: A Post-Starburst Galaxy With Little Star Formation Outside of It's Nuclear Disks
- Young Massive Clusters: Their Population Properties, Formation and Evolution, and Their Relation to the Ancient Globular Clusters
- Systematic differences in simple stellar population model results: Application to the M31 globular-like cluster system
- A starburst in the core of a galaxy cluster: The dwarf irregular NGC 1427A in Fornax
- On the precision of full-spectrum fitting of simple stellar populations. II. The dependence on star cluster mass in the wavelength range 0.3-5.0 m
- Deriving physical parameters of unresolved star clusters IV. The M33 star cluster system
- Comparing Mid-Infrared Globular Cluster Colors With Population Synthesis Models
- Resolved photometry of Young Massive Clusters in the starburst galaxy NGC 4214
- Deriving physical parameters of unresolved star clusters. VII. Adaptive aperture photometry of the M31 PHAT star clusters
- Synthetic stellar spectra to study multiple populations in globular clusters: an extended grid and the effects on the integrated light
- Deriving star cluster parameters with convolutional neural networks. II. Extinction and cluster/background classification
- Euclid: Early Release Observations -- The star cluster systems of the Local Group dwarf galaxies IC 10 and NGC 6822
- Effect of dynamical interactions on integrated properties of globular clusters
- The Star Formation History of a Post-Starburst Galaxy Determined From Its Cluster Population
- Deriving physical parameters of unresolved star clusters. VIII. Limits of aperture photometry for star cluster studies
- Massive star clusters and clumps in the collisional ring galaxy Arp 147
- Deriving physical parameters of unresolved star clusters. IX. Sky background effects in the aperture photometry
- Stellar associations powering HII regions $\unicode{x2013}$ II. Escape fraction of ionizing photons