On the Separation Between the Brightest Cluster Galaxy and the Intracluster Light
Abstract
We present a model-based framework to define an aperture separation between the brightest cluster galaxy (BCG) and the intracluster light (ICL). Using the intrinsic BCG and ICL components predicted by the semi-analytic model \texttt{FEGA25}, we determine, for each halo, the aperture radius that minimizes the bias in the recovered ICL mass. The optimal radius is obtained by balancing the BCG stellar mass lying outside the aperture with the ICL mass enclosed within it. At z=0, the optimal aperture in physical units increases with halo mass approximately as rcut∝ Mhalo0.28, close to the expected virial scaling. When expressed in units of the virial radius, the aperture becomes nearly independent of halo mass, with rcut/Rvir≃ 0.045 at 1014M⊙. Applying the resulting aperture prescriptions, we recover the intrinsic BCG mass to better than 8\% (lowest percentile), while the ICL mass is recovered with median values very close to unity, and an average scatter of ± 3%. Extending the analysis to z=1 and z=2, we find that the mass trends remain similar, with the slope and intercept of rcut/Rvir that stay stable. Robustness tests show that the inferred aperture is most sensitive to the ICL concentration and BCG size, but the main trends are preserved. Our results provide a physically motivated aperture definition for connecting observational BCG--ICL measurements to intrinsic model components.
Related
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- Euclid Quick Data Release (Q1). The shape of cluster haloes revealed by intracluster light
- The extended globular cluster system of the archetypal "failed galaxy" Dragonfly-44 from deep white-light Hubble Space Telescope imaging
- Constraining Effective Viscosity in the Intracluster Medium via the Thermal Sunyaev-Zeldovich Effect -- Predictions from the SLOW Constrained Coma Cluster Simulations
BibTeX
@misc{contini2026separation,
title = {{On the Separation Between the Brightest Cluster Galaxy and the Intracluster Light}},
author = {Emanuele Contini and Sukyoung K. Yi},
howpublished = {arXiv},
year = {2026},
month = oct,
doi = {10.48550/arxiv.2607.17616},
eprint = {2607.17616},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2607.17616},
note = {CC0},
}
RIS
TY - UNPB
TI - On the Separation Between the Brightest Cluster Galaxy and the Intracluster Light
AU - Emanuele Contini
AU - Sukyoung K. Yi
PY - 2026
DA - 2026/10/07
PB - arXiv
DO - 10.48550/arxiv.2607.17616
UR - https://arxiv.org/abs/2607.17616
AB - We present a model-based framework to define an aperture separation between the brightest cluster galaxy (BCG) and the intracluster light (ICL). Using the intrinsic BCG and ICL components predicted by the semi-analytic model \texttt{FEGA25}, we determine, for each halo, the aperture radius that minimizes the bias in the recovered ICL mass. The optimal radius is obtained by balancing the BCG stellar mass lying outside the aperture with the ICL mass enclosed within it. At z=0, the optimal aperture in physical units increases with halo mass approximately as r_cut∝ M_halo^0.28, close to the expected virial scaling. When expressed in units of the virial radius, the aperture becomes nearly independent of halo mass, with r_cut/R_vir≃ 0.045 at 10^14M_⊙. Applying the resulting aperture prescriptions, we recover the intrinsic BCG mass to better than 8\% (lowest percentile), while the ICL mass is recovered with median values very close to unity, and an average scatter of ± 3%. Extending the analysis to z=1 and z=2, we find that the mass trends remain similar, with the slope and intercept of r_cut/R_vir that stay stable. Robustness tests show that the inferred aperture is most sensitive to the ICL concentration and BCG size, but the main trends are preserved. Our results provide a physically motivated aperture definition for connecting observational BCG--ICL measurements to intrinsic model components.
ER -