Galaxy properties and their environmental dependence in GAMA survey

Unnikrishnan Sureshkumar, Anna Durkalec, Agnieszka Pollo, Maciej Bilicki, the GAMA Collaboration

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). 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.

Proceedings of the Polish Astronomical Society, vol. 10, 346-348 (2020)

Download full article as PDF file: