Year: 2020
Type: conference-paper
Abstract: We present preliminary results on the dependence of galaxy clustering on luminosity in different photometric bands and on stellar mass in the redshift range 0.1 < z < 0.16 using galaxies from Galaxy and Mass Assembly survey (GAMA) 1 .We measure luminosity-marked and stellar mass-marked correlation functions for a set of volume-limited subsamples.We then compare them to see which luminosity is a more accurate tracer of stellar mass and the underlying dark matter distribution.
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
OpenAlex ID: W3174691883
