The SAMI Galaxy Survey: spatially resolving the main sequence of star formation

• Published in: Monthly Notices of the Royal Astronomical Society
• Main Authors: Medling, Anne M., Cortese, Luca, Croom, Scott M., Green, Andrew W., Groves, Brent, Hampton, Elise, Ho, I-Ting, Davies, Luke J. M., Kewley, Lisa J., Moffett, Amanda J., Schaefer, Adam L., Taylor, Edward, Zafar, Tayyaba, Bekki, Kenji, Bland-Hawthorn, Joss, Bloom, Jessica V., Brough, Sarah, Bryant, Julia J., Catinella, Barbara, Cecil, Gerald, Colless, Matthew, Couch, Warrick J., Drinkwater, Michael J., Driver, Simon P., Federrath, Christoph, Foster, Caroline, Goldstein, Gregory, Goodwin, Michael, Hopkins, Andrew, Lawrence, J. S., Leslie, Sarah K., Lewis, Geraint F., Lorente, Nuria P. F., Owers, Matt S., McDermid, Richard, Richards, Samuel N., Sharp, Robert, Scott, Nicholas, Sweet, Sarah M., Taranu, Dan S., Tescari, Edoardo, Tonini, Chiara, van de Sande, Jesse, Walcher, C. Jakob, Wright, Angus
• Format: Article in Journal/Newspaper
• Language: unknown
• Published: Royal Astronomical Society 2018
• Subjects: surveys; galaxies: evolution; galaxies: star formation; Hubble; sami
• Online Access: https://doi.org/10.1093/mnras/sty127

We present the ∼800 star formation rate maps for the Sydney-AAO Multi-object Integral field spectrograph (SAMI) Galaxy Survey based on H α emission maps, corrected for dust attenuation via the Balmer decrement, that are included in the SAMI Public Data Release 1. We mask out spaxels contaminate...