Hostname: page-component-586b7cd67f-2plfb Total loading time: 0 Render date: 2024-11-23T05:54:50.695Z Has data issue: false hasContentIssue false
  • English
  • Français

The SAMI Galaxy Survey: first 1000 galaxies

Published online by Cambridge University Press:  09 February 2015

J. T. Allen  and
the SAMI Galaxy Survey Team
J. T. Allen
Affiliation:
Sydney Institute for Astronomy (SIfA), School of Physics, The University of Sydney, NSW 2006, Australia ARC Centre of Excellence for All-sky Astrophysics (CAASTRO) email: [email protected]
the SAMI Galaxy Survey Team
Affiliation:
Full list of team members is available at http://sami-survey.org/members
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.

The Sydney–AAO Multi-object Integral field spectrograph (SAMI) Galaxy Survey is an ongoing project to obtain integral field spectroscopic observations of ∼3400 galaxies by mid-2016. Including the pilot survey, a total of ∼1000 galaxies have been observed to date, making the SAMI Galaxy Survey the largest of its kind in existence. This unique dataset allows a wide range of investigations into different aspects of galaxy evolution.

The first public data from the SAMI Galaxy Survey, consisting of 107 galaxies drawn from the full sample, has now been released. By giving early access to SAMI data for the entire research community, we aim to stimulate research across a broad range of topics in galaxy evolution. As the sample continues to grow, the survey will open up a new and unique parameter space for galaxy evolution studies.

Keywords

galaxies: evolution – galaxies: kinematics and dynamics – galaxies: structure – techniques: imaging spectroscopy
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S309: Galaxies in 3D across the Universe , July 2014 , pp. 109 - 112
Copyright
Copyright © International Astronomical Union 2015 

References

Allen, J. T., et al., 2014a, Astrophysics Source Code Library, ascl:1407.006Google Scholar
Allen, J. T., et al., 2014b, MNRAS submitted, arXiv:1407.6068Google Scholar
Brough, S., et al., 2013, MNRAS, 435, 2903CrossRefGoogle Scholar
Bryant, J. J., Bland-Hawthorn, J., Fogarty, L. M. R., Lawrence, J. S., Croom, S. M., 2014a, MNRAS, 438, 869CrossRefGoogle Scholar
Bryant, J. J., et al., 2014b, MNRAS submitted, arXiv:1407.7335Google Scholar
Cappellari, M., et al., 2011, MNRAS, 416, 1680CrossRefGoogle Scholar
Croom, S. M., et al., 2012, MNRAS, 421, 872Google Scholar
Driver, S. P., et al., 2009, Astronomy and Geophysics, 50, 12CrossRefGoogle Scholar
Driver, S. P., et al., 2011, MNRAS, 413, 971CrossRefGoogle Scholar
Fogarty, L. M. R., et al., 2012, ApJ, 761, 169CrossRefGoogle Scholar
Fogarty, L. M. R., et al., 2014, MNRAS, 443, 485CrossRefGoogle Scholar
Ho, I.-T., et al., 2014, MNRAS accepted, arXiv:1407.2411Google Scholar
Sánchez, S. F., et al., 2012, A&A, 538, A8Google Scholar
Sharp, R., et al., 2006, in SPIE Conference Series Vol. 6269Google Scholar
Sharp, R., et al., 2014, MNRAS submitted, arXiv:1407.5237Google Scholar
York, D. G., et al., 2000, AJ, 120, 1579CrossRefGoogle Scholar