The atacama cosmology telescope: A catalog of >4000 Sunyaev–Zel’dovich galaxy clusters
View / Open Files
Authors
Naess, S
Rozo, E
Adhikari, S
Aguena, M
Aiola, S
Allam, S
Amodeo, S
Amon, A
Ansarinejad, B
Abbott, TMC
Austermann, JE
Avila, S
Bacon, D
Battaglia, N
Beall, JA
Becker, DT
Bertin, E
Bhandarkar, T
Bhargava, S
Bond, JR
Burke, DL
Calabrese, E
Choi, SK
Choi, A
Da Costa, LN
Crowley, KT
Dünner, R
Denison, EV
Devlin, MJ
Doel, P
Duff, SM
Duivenvoorden, AJ
Dunkley, J
Everett, S
Ferté, A
Ferrero, I
Gallardo, PA
Giles, P
Golec, JE
Gralla, MB
Grandis, S
Han, D
Hartley, WG
Hasselfield, M
Hill, JC
Hilton, GC
Ho, SPP
Hubmayr, J
Jaelani, AT
Jain, B
Jeltema, T
Kent, S
Knowles, K
Koopman, BJ
Lima, M
Lin, YT
Lokken, M
Loubser, SI
MacCrann, N
Marriage, TA
Martin, J
McMahon, J
Publication Date
2021-03Journal Title
Astrophysical Journal, Supplement Series
ISSN
0067-0049
Publisher
American Astronomical Society
Volume
253
Issue
1
Type
Article
This Version
VoR
Metadata
Show full item recordCitation
Hilton, M., Sifón, C., Naess, S., Madhavacheril, M., Oguri, M., Rozo, E., Rykoff, E., et al. (2021). The atacama cosmology telescope: A catalog of >4000 Sunyaev–Zel’dovich galaxy clusters. Astrophysical Journal, Supplement Series, 253 (1) https://doi.org/10.3847/1538-4365/abd023
Abstract
We present a catalog of 4195 optically confirmed Sunyaev-Zel'dovich (SZ)
selected galaxy clusters detected with signal-to-noise > 4 in 13,211 deg$^2$ of
sky surveyed by the Atacama Cosmology Telescope (ACT). Cluster candidates were
selected by applying a multi-frequency matched filter to 98 and 150 GHz maps
constructed from ACT observations obtained from 2008-2018, and confirmed using
deep, wide-area optical surveys. The clusters span the redshift range 0.04 < z
< 1.91 (median z = 0.52). The catalog contains 222 z > 1 clusters, and a total
of 868 systems are new discoveries. Assuming an SZ-signal vs. mass scaling
relation calibrated from X-ray observations, the sample has a 90% completeness
mass limit of M500c > 3.8 x 10$^{14}$ MSun, evaluated at z = 0.5, for clusters
detected at signal-to-noise ratio > 5 in maps filtered at an angular scale of
2.4'. The survey has a large overlap with deep optical weak-lensing surveys
that are being used to calibrate the SZ-signal mass-scaling relation, such as
the Dark Energy Survey (4566 deg$^2$), the Hyper Suprime-Cam Subaru Strategic
Program (469 deg$^2$), and the Kilo Degree Survey (825 deg$^2$). We highlight
some noteworthy objects in the sample, including potentially projected systems;
clusters with strong lensing features; clusters with active central galaxies or
star formation; and systems of multiple clusters that may be physically
associated. The cluster catalog will be a useful resource for future
cosmological analyses, and studying the evolution of the intracluster medium
and galaxies in massive clusters over the past 10 Gyr.
Identifiers
External DOI: https://doi.org/10.3847/1538-4365/abd023
This record's URL: https://www.repository.cam.ac.uk/handle/1810/319803
Rights
All rights reserved
Licence:
http://www.rioxx.net/licenses/all-rights-reserved
Statistics
Total file downloads (since January 2020). For more information on metrics see the
IRUS guide.