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Velocity Dispersion σ aper Aperture Corrections as a Function of Galaxy Properties from Integral-field Stellar Kinematics of 10,000 MaNGA Galaxies

Journal Article · · Research in Astronomy and Astrophysics
Abstract

The second moment of the stellar velocity within the effective radius, denoted by σe2 , is a crucial quantity in galaxy studies, as it provides insight into galaxy properties and their mass distributions. However, large spectroscopic surveys typically do not measureσedirectly, instead providingσaper, the second moment of the stellar velocity within a fixed fiber aperture. In this paper, we derive an empirical aperture correction formula, given by σaper / σe = ( Raper / Re ) α , using spatially resolved stellar kinematics extracted from approximately 10,000 Sloan Digital Sky Survey–Mapping Nearby Galaxies at Apache Point Observatory integral field unit observations. Our analysis reveals a strong dependence ofαon ther-band absolute magnitudeMr,g–icolor, and Sérsic indexnSer, whereαvalues are lower for brighter, redder galaxies with higher Sérsic indices. Our results demonstrate that the aperture correction derived from previous literature on early-type galaxies cannot be applied to predict the aperture corrections for galaxies with intermediate Sérsic indices. We provide a lookup table ofαvalues for different galaxy types, with parameters in the ranges of −18 >Mr> −24, 0.4 <g–i< 1.6, and 0 <nSer< 8. A Python script is provided to obtain the correction factors from the lookup table.

Research Organization:
US Department of Energy (USDOE), Washington, DC (United States). Office of Science, Sloan Digital Sky Survey (SDSS)
Sponsoring Organization:
USDOE
OSTI ID:
2425387
Journal Information:
Research in Astronomy and Astrophysics, Journal Name: Research in Astronomy and Astrophysics Journal Issue: 8 Vol. 23; ISSN 1674-4527
Publisher:
IOP Science
Country of Publication:
United States
Language:
English

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