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Surface brightness profiles around massive galaxies in LSSTComCam data

  • Conghao Zhou
  • Tesla Jeltema
  • Anja von der Linden
  • Lee S. Kelvin
  • Ian Dell’Antonio
  • Dan S. Taranu
  • Anthony Englert
  • Alexie Leauthaud

Abstract

Low surface brightness photometry of massive galaxies can probe the extended stellar halos and intracluster light but is often limited by background subtraction and masking systematics. Here we present radial surface brightness profiles for the brightest cluster galaxy of Abell 360 and 2dFGRS TGS323Z113 using Rubin Observatory Commissioning Camera (LSSTComCam) Data Preview 1 in the g, r, and z bands. Our results show that the LSSTComCam data can go down to  ∼ 28 mag arcsec−2 in the r band. Comparison to DECaLS measurements processed with Legacyhalos shows good agreement of surface brightness profiles at small radii while the LSSTComCam data extend deeper at larger radii.

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