TY - JOUR
T1 - A Concise Reference to (Projected) Sérsic R1/n Quantities, Including Concentration, Profile Slopes, Petrosian Indices, and Kron Magnitudes
AU - Graham, A
AU - Driver, Simon Peter
N1 - Alister Graham was a PDRA working for Driver. Driver instigated this paper and assisted Alister in all aspects of the paper.
PY - 2005/1
Y1 - 2005/1
N2 - Given the growing use of Sersic's (1963, 1968) R-1/n model 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 R-1/n profile, 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) R-1/n model 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 R-1/n profile, 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 : structure
KW - galaxies : fundamental parameters
KW - methods : analytical
KW - methods : data analysis
KW - EARLY-TYPE GALAXIES
KW - DWARF-ELLIPTIC GALAXIES
KW - SURFACE BRIGHTNESS GALAXIES
KW - SUPERMASSIVE BLACK-HOLES
KW - ON SPIRAL GALAXIES
KW - FUNDAMENTAL PLANE
KW - DISK GALAXIES
KW - GALACTIC DISKS
KW - PRELIMINARY CLASSIFICATION
KW - LUMINOSITY DISTRIBUTION
UR - http://www.scopus.com/inward/record.url?scp=24944434491&partnerID=8YFLogxK
UR - http://www.publish.csiro.au/nid/138/paper/AS05001.htm
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 -