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(2016)
Planck 2015 results
XXVII. The second Planck catalogue of Sunyaev-Zeldovich sources.
Astronomy & Astrophysics, 594 (A24).
ISSN 0004-6361
Abstract
We present the all-sky Planck catalogue of Sunyaev-Zeldovich (SZ) sources detected from the 29 month full-mission data. The catalogue (PSZ2) is the largest SZ-selected sample of galaxy clusters yet produced and the deepest systematic all-sky surveyof galaxy clusters. It contains 1653 detections, of which 1203 are confirmed clusters with identified counterparts in external data sets, and is the first SZ-selected cluster survey containing >103 confirmed clusters. We present a detailed analysis of the survey selection function in terms of its completeness and statistical reliability, placing a lower limit of 83% on the purity. Using simulations, we find that the estimates of the SZ strength parameter Y5R500are robust to pressure-profile variation and beam systematics, but accurate conversion to Y500 requires the use of prior information on the cluster extent. We describe the multi-wavelength search for counterparts in ancillary data, which makes use of radio, microwave, infra-red, optical, and X-ray data sets, and which places emphasis on the robustness of the counterpart match. We discuss the physical properties of the new sample and identify a population of low-redshift X-ray under-luminous clusters revealed by SZ selection. These objects appear in optical and SZ surveys with consistent properties for their mass, but are almost absent from ROSAT X-ray selected samples.
Item Type: |
Article
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Keywords: |
Planck Collaboration; cosmology: observations; galaxies: clusters: general; catalogs; |
Academic Unit: |
Faculty of Science and Engineering > Experimental Physics |
Item ID: |
14371 |
Identification Number: |
https://doi.org/10.1051/0004-6361/201525823 |
Depositing User: |
Dr. Anthony Murphy
|
Date Deposited: |
22 Apr 2021 16:01 |
Journal or Publication Title: |
Astronomy & Astrophysics |
Publisher: |
EDP Sciences |
Refereed: |
Yes |
URI: |
|
Use Licence: |
This item is available under a Creative Commons Attribution Non Commercial Share Alike Licence (CC BY-NC-SA). Details of this licence are available
here |
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