Catalog Service: Supermassive black holes masses upper limits
Description
Based on the modeling of the central emission-line width measured over subarcsecond apertures with the Hubble Space Telescope, we present stringent upper bounds on the mass of the central supermassive black hole, M_{blackhole}_, for a sample of 105 nearby galaxies (D<100Mpc) spanning a wide range of Hubble types (E-Sc) and values of the central stellar velocity dispersion, {sigma}_c_ (58-419km/s).
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Publisher: CDS[+]ivo://CDS[Pub. ID]
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This resource was registered on: 2012 Jan 06 12:04:17ZThis resource description was last updated on: 2021 Oct 21 00:00:00Z
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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/ApJ/692/856/table1 (Properties of the galaxies sample)
VERB=1
VERB=3
Cone search capability for table J/ApJ/692/856/table2 (Properties of the galaxies rejected from the main sample)
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