most citedThe SAMI Galaxy Survey: Spatially Resolving the Main Sequence of Star Formation

117 citations · 238 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2018117 cited

The SAMI Galaxy Survey: Spatially Resolving the Main Sequence of Star Formation

Anne M. Medling, Luca Cortese, Scott M. Croom +42

We present the ~800 star formation rate maps for the SAMI Galaxy Survey based on Hα emission maps, corrected for dust attenuation via the Balmer decrement, that are included in the…

astro-ph.GA20178 cited

The SAMI Galaxy Survey: understanding observations of large-scale outflows at low redshift with EAGLE simulations

E. Tescari, L. Cortese, C. Power +23

This work presents a study of galactic outflows driven by stellar feedback. We extract main sequence disc galaxies with stellar mass MM$_{\odot} \le 5.7\times1…

astro-ph.GA201778 cited

The SAMI Galaxy Survey: Data Release One with Emission-line Physics Value-Added Products

Andrew W. Green, Scott M. Croom, Nicholas Scott +48

We present the first major release of data from the SAMI Galaxy Survey. This data release focuses on the emission-line physics of galaxies. Data Release One includes data for 772 g…

astro-ph.GA20175 cited

The SAMI Galaxy Survey: Disk-halo interactions in radio-selected star-forming galaxies

S. K. Leslie, J. J. Bryant, I. -T. Ho +20

In this paper, we compare the radio emission at 1.4 GHz with optical outflow signatures of edge-on galaxies. We report observations of six edge-on star-forming galaxies in the Sydn…

astro-ph.CO201719 cited

Simulated metal and HI absorption lines at the conclusion of Reionization

L. A. Garcia, E. Tescari, E. V. Ryan-Weber +1

We present a theoretical study of intergalactic metal absorption lines imprinted in the spectra of distant quasars during and after the Epoch of Reionization (EoR). We use high res…

astro-ph.GA2017

Detection of a possible superluminous supernova in the epoch of reionization

Jeremy Mould, Tim Abbott, Jeff Cooke +7

An interesting transient has been detected in one of our three Dark Energy Camera deep fields. Observations of these deep fields take advantage of the high red sensitivity of DECam…