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 - Funding Information:
IRAF is distributed by the National Optical Astronomy Observatories, which are operated by the Association of Universities for Research in Astronomy, Inc., under cooperative agreement with the National Science Foundation.
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.
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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 -