Acknowledgements
If using S7 data products, please include this acknowledgement:
"The S7 Galaxy Survey is based on observations made at the ANU 2.3m telescope at Siding Spring Observatory. The Wide Field Spectrograph (WiFeS) was developed by the Australian National University. The S7 input catalogue is based on data taken from the [ADD]. The S7 Galaxy Survey is supported by the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project number CE110001020, and other participating institutions. The S7 Galaxy Survey website is https://miocene.anu.edu.au/S7/ "
Please also cite all relevant works from the following papers:
- "Probing the Physics of Narrow-line Regions in Active Galaxies. IV. Full Data Release of the Siding Spring Southern Seyfert Spectroscopic Snapshot Survey (S7)", Thomas et al., ApJS, 232, 11 (2017). Details of S7 DR2.
- "Probing the Physics of Narrow Line Regions in Active Galaxies. II. The Siding Spring Southern Seyfert Spectroscopic Snapshot Survey (S7)", Dopita et al., ApJS, 217, 12, (2015). Details of S7 DR1.
- "The Wide Field Spectrograph (WiFeS): performance and data reduction", Dopita et al., Ap&SS, 327, 245 (2010). WiFeS data reduction and performance.
- "PyWiFeS: a rapid data reduction pipeline for the Wide Field Spectrograph (WiFeS)", Childress et al., Ap&SS, 349, 617 (2014)PyWiFeS data reduction pipeline.
- "The Wide Field Spectrograph (WiFeS)", Dopita et al., Ap&SS, 310, 255 (2010). WiFeS instrument description paper.
- "LZIFU: an emission-line fitting toolkit for integral field spectroscopy data", Ho et al., Ap&SS, 361, 270 (2016). Details on emission line fitting procedure.