Planck 2015 results. XXVII. The Second Planck Catalogue of
Sunyaev-Zeldovich Sources
Sunyaev-Zeldovich Sources
File(s)1502.01598v1.pdf (4.2 MB)
Accepted version
Author(s)
Type
Journal Article
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
all-sky catalogue of 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 > $10^3$ 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 Y5R500 estimates are
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.
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
all-sky catalogue of 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 > $10^3$ 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 Y5R500 estimates are
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.
Date Issued
2016-09-20
Date Acceptance
2015-06-11
Citation
Astronomy & Astrophysics, 2016, 594
ISSN
0004-6361
Publisher
EDP Sciences
Journal / Book Title
Astronomy & Astrophysics
Volume
594
Copyright Statement
© 2016 ESO
Sponsor
Science and Technology Facilities Council (STFC)
Science and Technology Facilities Council (STFC)
Imperial College Trust
Science and Technology Facilities Council (STFC)
Science and Technology Facilities Council (STFC)
Science and Technology Facilities Council (STFC)
Grant Number
ST/F01239X/1
ST/H001239/1
N/A
ST/K001051/1
ST/K004131/1
ST/N001206/1
Subjects
astro-ph.CO
astro-ph.CO
Notes
41 pages. Submitted to A&A. Part of the 2015 Planck data release
Publication Status
Published
Article Number
A27