Acknowledging SAMI
SAMI
If using SAMI data products, please include this acknowledgement:
The SAMI Galaxy Survey is based on observations made at the Anglo-Australian Telescope. The Sydney-AAO Multi-object Integral field spectrograph (SAMI) was developed jointly by the University of Sydney and the Australian Astronomical Observatory. The SAMI input catalogue is based on data taken from the Sloan Digital Sky Survey, the GAMA Survey, and the VST ATLAS Survey. The SAMI Galaxy Survey is funded by the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project number CE110001020, and other participating institutions."
Please also cite the following papers:
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"The SAMI Galaxy Survey: Survey Overview and First Data Release", Green et al. 2017. Details about SAMI DR1.
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"LZIFU: an emission-line fitting toolkit for integral field spectroscopy data", Ho et al., Ap&SS, 361, 270 (2016). Details on emission line fits procedure.
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"The SAMI Galaxy Survey: Target selection and instrument specification", Bryant et al., MNRAS 447, 2857 (2015). Details of survey target selection and revised instrument description for upgraded SAMI instrument.
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"The SAMI Galaxy Survey: Cubism and covariance, putting round pegs into square holes", Sharp et al., MNRAS, 446, 1551 (2015). Data processing pipeline, including flux calibration and drizzle cubing.
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"The SAMI Galaxy Survey: Early Data Release", Allen et al., MNRAS, 446, 1567 (2015). Description of early data release, including quality metrics and details of data products.
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"The Sydney-AAO Multi-object Integral field spectrograph", Croom et al., MNRAS, 421, 872 (2012). Instrument description paper.
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"The SAMI Galaxy Survey: Spatially Resolving the Main Sequence of Star Formation", Medling et al. submitted. Details about emission line data products.