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20142026
most citedThe SAMI Galaxy Survey: instrument specification and target selection

506 citations · 3.7k across the 109 of their papers we have counts for

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astro-ph.GA2014★ 98 cited

The SAMI Galaxy Survey: Towards a unified dynamical scaling relation for galaxies of all types

L. Cortese, L. M. R. Fogarty, I. -T. Ho +27

We take advantage of the first data from the Sydney-AAO Multi-object Integral field (SAMI) Galaxy Survey to investigate the relation between the kinematics of gas and stars, and st…

astro-ph.GA2014★ 25 cited

The SAMI Galaxy Survey: The discovery of a luminous, low-metallicity H II complex in the dwarf galaxy GAMA J141103.98-003242.3

S. N. Richards, A. L. Schaefer, A. R. Lopez-Sanchez +18

We present the discovery of a luminous unresolved H II complex on the edge of dwarf galaxy GAMA J141103.98-003242.3 using data from the Sydney-AAO Multi-object Integral field spect…

astro-ph.GA2014★ 506 cited

The SAMI Galaxy Survey: instrument specification and target selection

J. J. Bryant, M. S. Owers, A. S. G. Robotham +54

The SAMI Galaxy Survey will observe 3400 galaxies with the Sydney-AAO Multi-object Integral-field spectrograph (SAMI) on the Anglo-Australian Telescope (AAT) in a 3-year survey whi…

astro-ph.GA2014★ 159 cited

The SAMI Galaxy Survey: Early Data Release

J. T. Allen, S. M. Croom, I. S. Konstantopoulos +45

We present the Early Data Release of the Sydney-AAO Multi-object Integral field spectrograph (SAMI) Galaxy Survey. The SAMI Galaxy Survey is an ongoing integral field spectroscopic…

astro-ph.IM2014★ 111 cited

The SAMI Galaxy Survey: Cubism and covariance, putting round pegs into square holes

R. Sharp, J. T. Allen, L. M. R. Fogarty +46

We present a methodology for the regularisation and combination of sparse sampled and irregularly gridded observations from fibre-optic multi-object integral-field spectroscopy. Th…

astro-ph.GA2014★ 32 cited

Choirs HI Galaxy Groups: The metallicity of dwarf galaxies

Sarah M. Sweet, Michael J. Drinkwater, Gerhardt Meurer +4

We present a recalibration of the luminosity-metallicity relation for gas-rich, star-forming dwarfs to magnitudes as faint as M ~ -13. We use the Dopita et al. (2013) metallici…