J/MNRAS/428/389  SLUGGS globular clusters in early-type galaxies   (Pota+, 2013)
The following files can be converted to FITS (extension .fit or fit.gz)
	ngc[0135]* ngc4365.dat ngc2768.dat ngc4278.dat ngc7457.dat
Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/MNRAS/428/389

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Beginning of ReadMe : J/MNRAS/428/389 SLUGGS globular clusters in early-type galaxies (Pota+, 2013) ================================================================================ The SLUGGS survey: kinematics for over 2500 globular clusters in 12 early-type galaxies. Pota V., Forbes D.A., Romanowsky A.J., Brodie J.P., Spitler L.R., Strader J., Foster C., Arnold J.A., Benson A., Blom C., Hargis J.R., Rhode K.L., Usher C. <Mon. Not. R. Astron. Soc., 428, 389-420 (2013)> =2013MNRAS.428..389P ================================================================================ ADC_Keywords: Galaxies, nearby ; Clusters, globular ; Photometry, SDSS Keywords: globular clusters: general - galaxies: evolution - galaxies: kinematics and dynamics - galaxies: star clusters: general Abstract: We present a spectrophotometric survey of 2522 extragalactic globular clusters (GCs) around 12 early-type galaxies, nine of which have not been published previously. Combining space-based and multicolour wide-field ground-based imaging, with spectra from the Keck/DEep Imaging Multi-Object Spectrograph (DEIMOS) instrument, we obtain an average of 160 GC radial velocities per galaxy, with a high-velocity precision of  15km/s per GC. After studying the photometric properties of the GC systems, such as their spatial and colour distributions, we focus on the kinematics of metal-poor (blue) and metal-rich (red) GC subpopulations to an average distance of  8 effective radii from the galaxy centre. Description: In this paper, we discuss a subset sample from our survey. This includes nine new galaxies, in addition to other three galaxies already published: NGC 4494 (Foster et al., 2011, Cat. J/MNRAS/415/3393), NGC 3115 (Arnold et al. 2011ApJ...736L..26A) and NGC 4486 (Strader et al. 2011, J/ApJS/197/33). The analysis and the specific results for these three galaxies have been extensively discussed in the respective papers.

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