UCL Discovery Stage
UCL home » Library Services » Electronic resources » UCL Discovery Stage

Dark Energy Survey Year 1 Results: Detection of Intracluster Light at Redshift ~ 0.25

Zhang, Y; Yanny, B; Palmese, A; Gruen, D; To, C; Rykoff, ES; Leung, Y; ... Wester, W; + view all (2019) Dark Energy Survey Year 1 Results: Detection of Intracluster Light at Redshift ~ 0.25. The Astrophysical Journal , 874 (2) , Article 165. 10.3847/1538-4357/ab0dfd. Green open access

[thumbnail of Doel_Dark Energy Survey Year 1 Results. Detection of Intracluster Light at Redshift ~ 0.25_VoR.pdf]
Preview
Text
Doel_Dark Energy Survey Year 1 Results. Detection of Intracluster Light at Redshift ~ 0.25_VoR.pdf - Published Version

Download (3MB) | Preview

Abstract

Using data collected by the Dark Energy Survey (DES), we report the detection of intracluster light (ICL) with ~300 galaxy clusters in the redshift range of 0.2–0.3. We design methods to mask detected galaxies and stars in the images and stack the cluster light profiles, while accounting for several systematic effects (sky subtraction, instrumental point-spread function, cluster selection effects, and residual light in the ICL raw detection from background and cluster galaxies). The methods allow us to acquire high signal-to-noise measurements of the ICL and central galaxies (CGs), which we separate with radial cuts. The ICL appears as faint and diffuse light extending to at least 1 Mpc from the cluster center, reaching a surface brightness level of 30 mag arcsec⁻². The ICL and the cluster CG contribute 44% ± 17% of the total cluster stellar luminosity within 1 Mpc. The ICL color is overall consistent with that of the cluster red sequence galaxies, but displays the trend of becoming bluer with increasing radius. The ICL demonstrates an interesting self-similarity feature—for clusters in different richness ranges, their ICL radial profiles are similar after scaling with cluster R_{200m}, and the ICL brightness appears to be a good tracer of the cluster radial mass distribution. These analyses are based on the DES redMaPPer cluster sample identified in the first year of observations.

Type: Article
Title: Dark Energy Survey Year 1 Results: Detection of Intracluster Light at Redshift ~ 0.25
Open access status: An open access version is available from UCL Discovery
DOI: 10.3847/1538-4357/ab0dfd
Publisher version: http://doi.org/10.3847/1538-4357/ab0dfd
Language: English
Additional information: This version is the version of record. For information on re-use, please refer to the publisher’s terms and conditions.
Keywords: galaxies: clusters: general, galaxies: evolution
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery-pp.ucl.ac.uk/id/eprint/10073233
Downloads since deposit
5,494Downloads
Download activity - last month
Download activity - last 12 months
Downloads by country - last 12 months

Archive Staff Only

View Item View Item