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Optical validation and characterization of \\Planck\\ PSZ2 sources at the Canary Islands observatories. I. First year of LP15 observations
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Optical validation and characterization of \\Planck\\ PSZ2 sources at the Canary Islands observatories. I. First year of LP15 observations
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Optical validation and characterization of \\Planck\\ PSZ2 sources at the Canary Islands observatories. I. First year of LP15 observations
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Paper
Optical validation and characterization of \\Planck\\ PSZ2 sources at the Canary Islands observatories. I. First year of LP15 observations
2019
Overview
Using telescopes at the Canary Island observatories, we conducted the long-term observational programme 128-MULTIPLE-16/15B (LP15), a large and complete optical follow-up campaign of all the unidentified PSZ2 sources in the northern sky (Dec>-15 deg) and no correspondence in the first Planck catalogue PSZ1. We perform this optical validation of SZ clusters in order to contribute to the characterization of the actual purity and completeness of full Our validation procedure combines this optical information with SZ emission as traced by the publicly available Planck Compton y-maps. The clusters counterparts are classified according to redshift, velocity dispersion and richness of the clusters. This paper presents the detailed study of 106 objects out of the LP15 sample, corresponding to all the observations carried out during the first year of the programme. We confirmed the optical counterpart for 41 new PSZ2 sources, being 31 of them validated using also velocity dispersion based on our spectroscopic information. This is the largest dataset of newly confirmed PSZ2 sources without any previous optical information. All the confirmed counterparts are rich structures (i.e. they show high velocity dispersion), and are well aligned with the nominal Planck coordinates (~70% of them are located at less than 3 arcmin distance). In total, 65 SZ sources are classified as unconfirmed, being 57 of them due to the absence of an optical over-density, and 8 of them due to a weak association with the observed SZ decrement. Most of the sources with no optical counterpart are located at low galactic latitudes and present strong galactic cirrus in the optical images, being the dust contamination the most probable explanation for their inclusion in the PSZ2 catalogue.
Publisher
Cornell University Library, arXiv.org
Subject
