Catalog Service: Stars and globulars in NGC4494
Description
We present a comprehensive analysis of the spatial, kinematic and chemical properties of stars and globular clusters (GCs) in the 'ordinary' elliptical galaxy NGC 4494 using data from the Keck and Subaru telescopes. We derive galaxy surface brightness and colour profiles out to large galactocentric radii. We compare the latter to metallicities derived using the near-infrared Calcium Triplet. We obtain stellar kinematics out to ~3.5 effective radii.
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Publisher: CDSivo://CDS[Pub. ID]
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This resource was registered on: 2012 May 13 17:06:39ZThis resource description was last updated on: 2021 Oct 21 00:00:00Z
This section describes what the resource is, what it contains, and how it might be relevant.
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This section describes the data's coverage over the sky, frequency, and time.
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This is service that does not comply with any IVOA standard but instead provides access to special capabilities specific to this resource.
This is a standard IVOA service that takes as input an ADQL or PQL query and returns tabular data.
This is a standard IVOA service that takes as input a position in the sky and a radius and returns catalog records with positions within that radius.
Cone search capability for table J/MNRAS/415/3393/tablea1 (Individual values for NGC 4494 galaxy light)
VERB=1
VERB=3
Cone search capability for table J/MNRAS/415/3393/tablea2 (Individual spectroscopically confirmed globular clusters and Ultra-Compact Dwarfs around NGC 4494)
Cone search capability for table J/MNRAS/415/3393/table3 (Catalog of photometrically selected globular cluster candidates with i0<24)
Cone search capability for table J/MNRAS/415/3393/table4 (List of spectroscopically identified contaminants and non-globular cluster fillers)
Developed with the support of the National Science Foundation under Cooperative Agreement AST0122449 with the Johns Hopkins University The NAVO project is a member of the International Virtual Observatory Alliance
This NAVO Application is hosted by the Space Telescope Science Institute