A data-driven Bayesian approach for finding young stellar populations in early-type galaxies from their ultraviolet-optical spectra

Monthly Notices of the Royal Astronomical Society

Volumn 366, Issue 1, 2006, Pages 321-338

  Nolan, Louisa A ^a   Harva, Markus O ^b   Kabán, Ata ^a   Raychaudhury, Somak ^a  

^a UNIVERSITY OF BIRMINGHAM   (United Kingdom)

^b AALTO UNIVERSITY   (Finland)

Author keywords

Galaxies: elliptical and lenticular, cD; Galaxies: stellar content; Methods: data analysis

Indexed keywords

BAYESIAN NETWORKS; DATA HANDLING; FACTOR ANALYSIS; GALAXIES; INFORMATION ANALYSIS; INVERSE PROBLEMS; POPULATION STATISTICS; PRINCIPAL COMPONENT ANALYSIS; SPECTRUM ANALYSIS; STARS; SURVEYS;

DATA DRIVEN; EARLY TYPES; GALAXIES: ELLIPTICAL AND LENTICULAR CD; GALAXY:STELLAR CONTENT; METHODS. DATA ANALYSIS; OPTICAL SPECTRUM; PHYSICAL MODELLING; PRINCIPAL-COMPONENT ANALYSIS; SPECTRA'S; STELLAR POPULATIONS;

SPECTROSCOPIC ANALYSIS;

EID: 33645088417     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09868.x     Document Type: Article

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