Deriving accurate galaxy cluster masses using X-ray thermodynamic profiles and graph neural networks

Open Access

Fig. 3.

Number distribution of galaxy clusters in the THE THREE HUNDRED PROJECT as a function of $M_{500}^{True}$ $\text{M}^{\text{True}}_{500}$ . The magenta histogram represents the original sample (1655 clusters), while the orange and green histograms represent the augmented training sample (9305 clusters built with 1305 clusters) and testing sample (1950 clusters built with 350 clusters), respectively.

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.