# Dark Energy Survey Year 1 results: Detection of Intra-cluster Light at   Redshift $\sim$ 0.25

**Authors:** Y. Zhang, B. Yanny, A. Palmese, D. Gruen, C. To, E. S. Rykoff, Y., Leung, C. Collins, M. Hilton, T. M. C. Abbott, J. Annis, S. Avila, E. Bertin,, D. Brooks, D. L. Burke, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, C., E. Cunha, C. B. D'Andrea, L. N. Da Costa, J. De Vicente, S. Desai, H. T., Diehl, J. P. Dietrich, P. Doel, A. Drlica-Wagner, T. F. Eifler, A. E. Evrard,, B. Flaugher, P. Fosalba, J. Frieman, J. Garc'Ia-Bellido, E. Gaztanaga, D. W., Gerdes, R. A. Gruendl, J. Gschwend, G. Gutierrez, W. G. Hartley, D. L., Hollowood, K. Honscheid, B. Hoyle, D. J. James, T. Jeltema, K. Kuehn, N., Kuropatkin, T. S. Li, M. Lima, M. A. G. Maia, M. March, J. L. Marshall, P., Melchior, F. Menanteau, C. J. Miller, R. Miquel, J. J. Mohr, R. L. C. Ogando,, A. A. Plazas, A. K. Romer, E. Sanchez, V. Scarpine, M. Schubnell, S. Serrano,, I. Sevilla-Noarbe, M. Smith, M. Soares-Santos, F. Sobreira, E. Suchyta, M. E., C. Swanson, G. Tarle, D. Thomas, W. Wester

arXiv: 1812.04004 · 2019-04-17

## TL;DR

This paper reports the first detection and analysis of intra-cluster light in galaxy clusters at redshift ~0.25 using DES data, revealing its properties, distribution, and relation to cluster mass.

## Contribution

It introduces new methods for masking and stacking to measure faint ICL, and demonstrates its self-similarity and correlation with cluster mass distribution.

## Key findings

- ICL extends to at least 1 Mpc from cluster centers.
- ICL accounts for about 44% of total stellar luminosity within 1 Mpc.
- ICL brightness correlates with cluster mass distribution.

## Abstract

Using data collected by the Dark Energy Survey (DES), we report the detection of intracluster light (ICL) with $\sim300$ 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 to $44\%\pm17$\% 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 $R_\mathrm{200m}$, 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.

## Full text

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## Figures

23 figures with captions in the complete paper: https://tomesphere.com/paper/1812.04004/full.md

## References

122 references — full list in the complete paper: https://tomesphere.com/paper/1812.04004/full.md

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Source: https://tomesphere.com/paper/1812.04004