GBT26A-644

Following up the EDGE sample with atomic hydrogen observations

Abstract

EDGE is a survey of gas in nearby galaxies based on the CALIFA and AMUSING++ IFU samples. Galaxies are diameter selected to be < 1 arcmin, matching the IFUs field of view. This diameter selection results in a good representation of the z=0 population, including galaxies above, below, and in the main sequence. EDGE follows up these galaxies using CO imaging. This proposal is to complement the CO imaging with HI spectroscopy, particularly for those galaxies that have poor quality of no HI observations.

Investigators

Name	Institution
GBT Operator	Green Bank Observatory
Yu-Hsuan Teng	Maryland, University of
Peter Teuben	Maryland, University of
Alberto Bolatto *	Maryland, University of

* indicates the PI