TY - JOUR
T1 - A Concise Reference to (Projected) Sersic R1Quantities, Including Concentration, Profile Slopes, Petrosian Indices, and Kron Magnitudes
AU - Graham, Alister W.
AU - Driver, Simon P.
PY - 2005
Y1 - 2005
N2 - Given the growing use of Sersic's (1963, 1968) Rnmodel for describing the stellar distributions in galaxies, and the lack of any single reference that provides the various associated mathematical expressions, we have endeavoured to compile such a resource here. We present the standard intensity profile, and its various guises such as the luminosity, surface-brightness, and aperture–magnitude profile. Expressions to transform the effective surface brightness into the mean effective and central surface brightness are also given, as is the expression to transform between effective radii and exponential scale-lengths. We additionally provide expressions for deriving the ‘concentration’ of an Rlinprofile, and two useful equations for the logarithmic slope of the light-profile are given. Petrosian radii and fluxes are also derived for a range of Sersic profiles and compared with the effective radii and total flux. Similarly, expressions to obtain Kron radii and fluxes are presented as a function of the Sersic index n and the number of effective radii sampled. Illustrative figures are provided throughout. Finally, the core–Sersic model, consisting of an inner power-law and an outer Sersic function, is presented.
AB - Given the growing use of Sersic's (1963, 1968) Rnmodel for describing the stellar distributions in galaxies, and the lack of any single reference that provides the various associated mathematical expressions, we have endeavoured to compile such a resource here. We present the standard intensity profile, and its various guises such as the luminosity, surface-brightness, and aperture–magnitude profile. Expressions to transform the effective surface brightness into the mean effective and central surface brightness are also given, as is the expression to transform between effective radii and exponential scale-lengths. We additionally provide expressions for deriving the ‘concentration’ of an Rlinprofile, and two useful equations for the logarithmic slope of the light-profile are given. Petrosian radii and fluxes are also derived for a range of Sersic profiles and compared with the effective radii and total flux. Similarly, expressions to obtain Kron radii and fluxes are presented as a function of the Sersic index n and the number of effective radii sampled. Illustrative figures are provided throughout. Finally, the core–Sersic model, consisting of an inner power-law and an outer Sersic function, is presented.
KW - galaxies: fundamental parameters
KW - galaxies: structure
KW - methods: analytical
KW - methods: data analysis
UR - http://www.scopus.com/inward/record.url?scp=24944434491&partnerID=8YFLogxK
U2 - 10.1071/AS05001
DO - 10.1071/AS05001
M3 - Article
SN - 1323-3580
VL - 22
SP - 118
EP - 127
JO - Publications of the Astronomical Society of Australia
JF - Publications of the Astronomical Society of Australia
IS - 2
ER -