Euclid: Early Release Observations – The intracluster light and intracluster globular clusters of the Perseus cluster

Open Access

Table 3

Results of the single Gaussian fits to the GCLF in each annulus.

Annulus (kpc)	µ (mag)	σ (mag)	Reduced χ²
20–40	26.24 ± 0.12	1.39 ± 0.05	1.01
40–100	26.24*	1.33 ± 0.01	1.38
100–200	26.24*	1.18 ± 0.02	2.60
200–500	26.24*	1.05 ± 0.03	2.28

Notes. Parameters marked with an asterisk were fixed during the fit. The goodness-of-fit of the model is given by the reduced χ² metric.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.