Hostname: page-component-78c5997874-j824f Total loading time: 0 Render date: 2024-11-16T06:36:57.989Z Has data issue: false hasContentIssue false
  • English
  • Français

Stellar velocity dispersions and emission line properties of SDSS-III/BOSS galaxies

Published online by Cambridge University Press:  17 July 2013

D. Thomas ,
O. Steele ,
C. Maraston ,
J. Johansson ,
A. Beifiori ,
J. Pforr ,
G. Strömbäck ,
C. A. Tremonti ,
D. Wake  and
the BOSS collaboration
D. Thomas
Affiliation:
ICG, University of Portsmouth, Dennis Sciama Bldg, Burnaby Road, PO1 3FX, UK SEPnet, South East Physics Network, (www.sepnet.ac.uk)
O. Steele
Affiliation:
ICG, University of Portsmouth, Dennis Sciama Bldg, Burnaby Road, PO1 3FX, UK
C. Maraston
Affiliation:
ICG, University of Portsmouth, Dennis Sciama Bldg, Burnaby Road, PO1 3FX, UK SEPnet, South East Physics Network, (www.sepnet.ac.uk)
J. Johansson
Affiliation:
ICG, University of Portsmouth, Dennis Sciama Bldg, Burnaby Road, PO1 3FX, UK Max-Planck-Institut für Astrophysik, D-85748 Garching, Germany
A. Beifiori
Affiliation:
ICG, University of Portsmouth, Dennis Sciama Bldg, Burnaby Road, PO1 3FX, UK MPI für extraterrestrische Physik, Giessenbachstraße, D-85748 Garching, Germany
J. Pforr
Affiliation:
ICG, University of Portsmouth, Dennis Sciama Bldg, Burnaby Road, PO1 3FX, UK NOAO, 950 North Cherry Ave., Tucson, AZ 85719, USA
G. Strömbäck
Affiliation:
ICG, University of Portsmouth, Dennis Sciama Bldg, Burnaby Road, PO1 3FX, UK
C. A. Tremonti
Affiliation:
Department of Astronomy, University of Wisconsin-Madison, Madison, WI 53706, USA
D. Wake
Affiliation:
Yale Center for Astronomy and Astrophysics, Yale University, New Haven, CT, USA
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We perform a spectroscopic analysis of 492,450 galaxy spectra from the first two years of observations of the Sloan Digital Sky Survey-III/Baryonic Oscillation Spectroscopic Survey (BOSS) collaboration. This data set has been released in the ninth SDSS data release, the first public data release of BOSS spectra. We show that the typical signal-to-noise ratio of BOSS spectra is sufficient to measure stellar velocity dispersion and emission line fluxes for individual objects. The typical velocity dispersion of a BOSS galaxy is 240 km/s, with an accuracy of better than 30 per cent for 93 per cent of BOSS galaxies. The distribution in velocity dispersion is redshift independent between redshifts 0.15 and 0.7, which reflects the survey design targeting massive galaxies with an approximately uniform mass distribution in this redshift interval. The majority of BOSS galaxies lack detectable emission lines. We analyse the emission line properties and present diagnostic diagrams using the emission lines [OII], Hβ, [OIII], Halpha, and [NII] (detected in about 4 per cent of the galaxies). We show that the emission line properties are strongly redshift dependent and that there is a clear correlation between observed frame colours and emission line properties. Within in the low-z sample around 0.15 < z < 0.3, half of the emission-line galaxies have LINER-like emission line ratios, followed by Seyfert-AGN dominated spectra, and only a small fraction of a few per cent are purely star forming galaxies. AGN and LINER-like objects, instead, are less prevalent in the high-z sample around 0.4 < z < 0.7, where more than half of the emission line objects are star forming. This is a pure selection effect caused by the non-detection of weak Hβ emission lines in the BOSS spectra. Finally, we show that star forming, AGN and emission line free galaxies are well separated in the g - r vs r - i target selection diagram.

Keywords

surveysgalaxies: generalgalaxies: evolutiongalaxies: kinematics and dynamicsgalaxies: ISMgalaxies: active evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S295: The intriguing life of massive galaxies , August 2012 , pp. 129 - 132
Copyright
Copyright © International Astronomical Union 2013 

References

Ahn, C. P., et al., 2012, ApJS, 203, 21Google Scholar
Baldwin, J. A., Phillips, M. M., & Terlevich, R., 1981, PASP, 93, 5CrossRefGoogle Scholar
Cappellari, M., Emsellem, E., 2004, PASP, 116, 138Google Scholar
Dawson, K. S., et al., 2013, AJ, 145, 10Google Scholar
Eisenstein, D. J.et al., 2011, AJ, 142, 72Google Scholar
Lamareille, F., 2010, A&A, 509, 53Google Scholar
Maraston, C., Strömbäck, G., 2011, MNRAS, 418, 2785CrossRefGoogle Scholar
Masters, K., et al., 2011, MNRAS, 418, 1055Google Scholar
Sarzi, M.et al., 2006, MNRAS, 366, 1151CrossRefGoogle Scholar
Shu, Y., et al., 2011, ApJ, 143, 90CrossRefGoogle Scholar
Thomas, D.et al., 2013, MNRAS, 431, 1383Google Scholar
Tojeiro, R., et al., 2012, MNRAS, 424, 136Google Scholar
York, D. G., et al., 2000, AJ, 120, 1579Google Scholar