Catalog Service: Spectroscopy in A2199 and Virgo clusters
Description
We report a new determination of the faint end of the galaxy luminosity function (LF) in the nearby clusters Abell 2199 and Virgo using data from the Sloan Digital Sky Survey (SDSS) and the Hectospec multifiber spectrograph on the MMT. The luminosity function of A2199 is consistent with a single Schechter function to M_r_=-15.6+5log(h_70_) with a faint-end slope of alpha=-1.13+/-0.07 (statistical). The LF in Virgo extends to M_r_~-13.5~M*+8 and has a slope of alpha=-1.28+/-0.06 (statistical).
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Publisher: CDSivo://CDS[Pub. ID]
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This resource was registered on: 2011 Jan 31 09:54:12ZThis resource description was last updated on: 2021 Oct 21 00:00:00Z
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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/AJ/135/1837/table1 (Spectroscopic Data for A2199)
VERB=1
VERB=3
Cone search capability for table J/AJ/135/1837/table3 (SDSS data for probable Virgo members)
Cone search capability for table J/AJ/135/1837/table2 (SDSS data for spectroscopically confirmed Virgo members)
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
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