Feb 23 – 26, 2021
Zoom Passcode: 990417
America/Chicago timezone

The Satellite Population Around Luminous Red Galaxies in the Legacy Surveys

Feb 23, 2021, 5:25 PM
Zoom Link: https://kansas.zoom.us/j/92389769214 (Zoom Passcode: 990417)

Zoom Link: https://kansas.zoom.us/j/92389769214

Zoom Passcode: 990417

Zoom Link: https://kansas.zoom.us/j/92389769214 Zoom Passcode: 990417 Zoom Meeting ID: 923 8976 9214


Mindy Townsend (University of Kansas)


Luminous Red Galaxies, or LRGs, were originally selected in the Sloan Digital Sky Survey as good tracers of large scale structure. Subsequent investigations showed them to be among the most massive galaxies in the Universe and dominated by uniformly old stellar populations. Despite being dominated by old stars, however, they have grown in stellar mass since z=1, implying that they grow predominantly via accretion of mostly passive satellites. This picture has not yet been tested because of the lack of deep imaging data sets that both covers a large enough area of the sky to contain substantial numbers of LRGs and also is deep enough to detect faint satellites. I will present our initial characterization the satellite galaxy population of LRGs out to z=0.65. To accomplish I use the Legacy Surveys, which are comprised of grz imaging to 2-2.5 mag deeper than SDSS, over a larger footprint, and with better image quality. Specifically, I will present our first measurement of the percentage of LRGs that have significant satellite populations.

Type of contribution Oral contribution (10 minutes)

Primary author

Mindy Townsend (University of Kansas)

Presentation materials