An alternative validation strategy for the Planck cluster catalog and $y$-distortion maps
Rishi Khatri

TL;DR
This paper introduces a new component separation method for Planck data that effectively distinguishes $y$-distortion from CO emission, improving cluster catalog validation and contamination assessment.
Contribution
It presents an alternative validation strategy using parametric model fitting to identify and mitigate CO contamination in the Planck cluster catalog.
Findings
At least 93% of clusters are free of CO contamination.
59% of unconfirmed candidates may have significant molecular cloud contamination.
The proposed method improves cluster catalog reliability.
Abstract
We present an all sky map of the -type distortion calculated from the full mission Planck HFI (High Frequency Instrument) data using the recently proposed approach to component separation based on parametric model fitting and model selection. This simple model selection approach allows us to distinguish between carbon monoxide (CO) line emission and -type distortion, something that is not possible using the internal linear combination based methods. We create a mask to cover the regions of significant CO emission relying on the information in the map obtained when fitting for the -distortion and CO emission to the lowest four HFI channels. We revisit the second Planck cluster catalog and try to quantify the quality of the cluster candidates in an approach that is similar in spirit to Aghanim et al. (2014). We find that at least of the clusters in the cosmology…
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