Sérsic profile

E823176

The Sérsic profile is a mathematical model that describes how the intensity of light from a galaxy varies with distance from its center, widely used to characterize galaxy structure and morphology.

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Statements (48)

Predicate Object
instanceOf galaxy light profile
surface brightness profile model
alsoKnownAs Sérsic law NERFINISHED
r^{1/n} law
appliesTo disk galaxies
elliptical galaxies
galactic bulges
galaxies
characterizes light concentration of galaxies
shape of galaxy surface brightness profiles
dependsOn Sérsic index n controlling profile curvature
effective radius Re setting scale
describes radial variation of galaxy surface brightness
field astrophysics
extragalactic astronomy
galaxy morphology
generalizes de Vaucouleurs profile NERFINISHED
exponential disk profile
hasParameter Sérsic index n NERFINISHED
central surface brightness I0
effective radius Re
effective surface brightness Ie
scale radius
shape parameter b_n
hasProperty can fit a wide range of galaxy types
flexible shape controlled by index n
monotonically decreasing intensity with radius
implementedIn GALFIT NERFINISHED
GIM2D NERFINISHED
IMFIT NERFINISHED
introducedIn 1963
mathematicalForm I(R) = I_e * exp{-b_n[(R/R_e)^{1/n} - 1]}
namedAfter José Luis Sérsic NERFINISHED
publication Atlas de Galaxias Australes NERFINISHED
relatedTo Petrosian radius NERFINISHED
galaxy concentration index
half-light radius
specialCase de Vaucouleurs profile when n = 4
exponential profile when n = 1
usedFor bulge–disk decomposition
classifying galaxy morphology
fitting galaxy images
galaxy structural decomposition
measuring galaxy concentration
measuring galaxy sizes
usedIn galaxy evolution studies
photometric analysis of galaxies
survey data analysis

Referenced by (2)

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Einasto density profile generalizes Sérsic profile
Einasto density profile similarTo Sérsic profile