A method for classification of red, blue and green galaxies using fuzzy set theory
arXiv:2005.11678 · doi:10.1093/mnrasl/slaa152
Abstract
Red and blue galaxies are traditionally classified using some specific cuts in colour or other galaxy properties, which are supported by empirical arguments. The vagueness associated with such cuts are likely to introduce a significant contamination in these samples. Fuzzy sets are vague boundary sets which can efficiently capture the classification uncertainty in the absence of any precise boundary. We propose a method for classification of galaxies according to their colours using fuzzy set theory. We use data from the SDSS to construct a fuzzy set for red galaxies with its members having different degrees of `redness'. We show that the fuzzy sets for the blue and green galaxies can be obtained from it using different fuzzy operations. We also explore the possibility of using fuzzy relation to study the relationship between different galaxy properties and discuss its strengths and limitations.
arXiv comment6 pages, 2 figures, Accepted for publication in MNRAS Letters
References in corpus (23)
- The Sloan Digital Sky Survey: Technical Summary
- The Optical and Near-Infrared Properties of Galaxies: I. Luminosity and Stellar Mass Functions
- Color Separation of Galaxy Types in the Sloan Digital Sky Survey Imaging Data
- Quantifying the bimodal color-magnitude distribution of galaxies
- First results from the IllustrisTNG simulations: the galaxy color bimodality
- Galaxy bimodality versus stellar mass and environment
- Galaxy Clustering in the Completed SDSS Redshift Survey: The Dependence on Color and Luminosity
- The Broad-band Optical Properties of Galaxies with Redshifts 0.0 < z < 0.2
- The bimodal galaxy color distribution: dependence on luminosity and environment
- Modelling the Galaxy Bimodality: Shutdown Above a Critical Halo Mass
- The Millennium Galaxy Catalogue: morphological classification and bimodality in the colour-concentration plane
- The Bimodal Galaxy Stellar Mass Function in the COSMOS Survey to z~1: A Steep Faint End and a New Galaxy Dichotomy
- Galaxy And Mass Assembly: Deconstructing Bimodality - I. Red ones and blue ones
- It's not easy being green: The evolution of galaxy colour in the EAGLE simulation
- Bimodal Color Distribution in Hierarchical Galaxy Formation
- The X-Ray Derived Cosmological Star Formation History and the Galaxy X-Ray Luminosity Functions in the Chandra Deep Fields North and South
- Accretion, feedback and galaxy bimodality: a comparison of the GalICS semi-analytic model and cosmological SPH simulations
- Three-point Correlation Functions of SDSS Galaxies in Redshift Space: Morphology, Color, and Luminosity Dependence
- The Millennium Galaxy Catalogue: Exploring the Color-Concentration Bimodality via Bulge-Disc Decomposition
- Two-Dimensional Topology of the Sloan Digital Sky Survey
- The Luminosity, Colour and Morphology dependence of galaxy filaments in the Sloan Digital Sky Survey Data Release Four
- The origin of the red sequence galaxy population in the EAGLE simulation
- The bimodality of the 10k zCOSMOS-bright galaxies up to z ~ 1: a new statistical and portable classification based on the optical galaxy properties
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- On the origin of red spirals: Does assembly bias play a role?
- Do minor interactions trigger star formation in galaxy pairs?
- The correlations between galaxy properties in different environments of the cosmic web
- Modeling the Spectral Diversity of Quasars in the Sixteenth Data Release from the Sloan Digital Sky Survey
- Tracing the green valley with entropic thresholding
- The long road to the Green Valley: Tracing the evolution of the Green Valley galaxies in the EAGLE simulation
- Clustering and physical properties of AGN and Star-Forming Galaxies at fixed stellar mass: does assembly bias have a role in AGN activity?
- Galaxy quenching across the Cosmic Web: disentangling mass and environment with SDSS DR18