TY - JOUR
T1 - The Atacama Cosmology Telescope
T2 - The Two-season ACTPol Sunyaev-Zel'dovich Effect Selected Cluster Catalog
AU - Hilton, Matt
AU - Hasselfield, Matthew
AU - Sifón, Cristóbal
AU - Battaglia, Nicholas
AU - Aiola, Simone
AU - Bharadwaj, V.
AU - Bond, J. Richard
AU - Choi, Steve K.
AU - Crichton, Devin
AU - Datta, Rahul
AU - Devlin, Mark J.
AU - Dunkley, Joanna
AU - Dünner, Rolando
AU - Gallardo, Patricio A.
AU - Gralla, Megan
AU - Hincks, Adam D.
AU - Ho, Shuay Pwu P.
AU - Hubmayr, Johannes
AU - Huffenberger, Kevin M.
AU - Hughes, John P.
AU - Koopman, Brian J.
AU - Kosowsky, Arthur
AU - Louis, Thibaut
AU - Madhavacheril, Mathew S.
AU - Marriage, Tobias A.
AU - Maurin, Loïc
AU - McMahon, Jeff
AU - Miyatake, Hironao
AU - Moodley, Kavilan
AU - Nss, Sigurd
AU - Nati, Federico
AU - Newburgh, Laura
AU - Niemack, Michael D.
AU - Oguri, Masamune
AU - Page, Lyman A.
AU - Partridge, Bruce
AU - Schmitt, Benjamin L.
AU - Sievers, Jon
AU - Spergel, David N.
AU - Staggs, Suzanne T.
AU - Trac, Hy
AU - Engelen, Alexander Van
AU - Vavagiakis, Eve M.
AU - Wollack, Edward J.
N1 - Publisher Copyright:
© 2018. The American Astronomical Society. All rights reserved..
PY - 2018/3
Y1 - 2018/3
N2 - We present a catalog of 182 galaxy clusters detected through the Sunyaev-Zel'dovich (SZ) effect by the Atacama Cosmology Telescope in a contiguous 987.5 deg2 field. The clusters were detected as SZ decrements by applying a matched filter to 148 GHz maps that combine the original ACT equatorial survey with data from the first two observing seasons using the ACTPol receiver. Optical/IR confirmation and redshift measurements come from a combination of large public surveys and our own follow-up observations. Where necessary, we measured photometric redshifts for clusters using a pipeline that achieves accuracy Δz/(1 + z) = 0.015 when tested on Sloan Digital Sky Survey data. Under the assumption that clusters can be described by the so-called universal pressure profile (UPP) and its associated mass scaling law, the full signal-to-noise ratio > 4 sample spans the mass range , with median . The sample covers the redshift range 0.1 < z < 1.4 (median z = 0.49), and 28 clusters are new discoveries (median z = 0.80). We compare our catalog with other overlapping cluster samples selected using the SZ, optical, and X-ray wavelengths. We find that the ratio of the UPP-based SZ mass to richness-based weak-lensing mass is . After applying this calibration, the mass distribution for clusters with M 500c > 4 1014 M o is consistent with the number of such clusters found in the South Pole Telescope SZ survey.
AB - We present a catalog of 182 galaxy clusters detected through the Sunyaev-Zel'dovich (SZ) effect by the Atacama Cosmology Telescope in a contiguous 987.5 deg2 field. The clusters were detected as SZ decrements by applying a matched filter to 148 GHz maps that combine the original ACT equatorial survey with data from the first two observing seasons using the ACTPol receiver. Optical/IR confirmation and redshift measurements come from a combination of large public surveys and our own follow-up observations. Where necessary, we measured photometric redshifts for clusters using a pipeline that achieves accuracy Δz/(1 + z) = 0.015 when tested on Sloan Digital Sky Survey data. Under the assumption that clusters can be described by the so-called universal pressure profile (UPP) and its associated mass scaling law, the full signal-to-noise ratio > 4 sample spans the mass range , with median . The sample covers the redshift range 0.1 < z < 1.4 (median z = 0.49), and 28 clusters are new discoveries (median z = 0.80). We compare our catalog with other overlapping cluster samples selected using the SZ, optical, and X-ray wavelengths. We find that the ratio of the UPP-based SZ mass to richness-based weak-lensing mass is . After applying this calibration, the mass distribution for clusters with M 500c > 4 1014 M o is consistent with the number of such clusters found in the South Pole Telescope SZ survey.
KW - cosmology: large-scale structure of universe
KW - cosmology: observations
KW - galaxies: clusters: general Supporting material: tar.gz file
UR - http://www.scopus.com/inward/record.url?scp=85044126675&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85044126675&partnerID=8YFLogxK
U2 - 10.3847/1538-4365/aaa6cb
DO - 10.3847/1538-4365/aaa6cb
M3 - Article
AN - SCOPUS:85044126675
SN - 0067-0049
VL - 235
JO - Astrophysical Journal, Supplement Series
JF - Astrophysical Journal, Supplement Series
IS - 1
M1 - 20
ER -