GALAXY CLUSTERS DISCOVERED WITH A SUNYAEV-ZEL'DOVICH EFFECT SURVEY
Open accessAbstract
The South Pole Telescope (SPT) is conducting a Sunyaev–Zel'dovich (SZ) effect survey over large areas of the southern sky, searching for massive galaxy clusters to high redshift. In this preliminary study, we focus on a 40 deg 2 area targeted by the Blanco Cosmology Survey (BCS), which is centered roughly at right ascension 5 h 30 m , declination −53° (J2000). Over two seasons of observations, this entire region has been mapped by the SPT at 95 GHz, 150 GHz, and 225 GHz. We report the four most significant SPT detections of SZ clusters in this field, three of which were previously unknown and, therefore, represent the first galaxy clusters discovered with an SZ survey. The SZ clusters are detected as decrements with greater than 5σ significance in the high-sensitivity 150 GHz SPT map. The SZ spectrum of these sources is confirmed by detections of decrements at the corresponding locations in the 95 GHz SPT map and nondetections at those locations in the 225 GHz SPT map. Multiband optical images from the BCS survey demonstrate significant concentrations of similarly colored galaxies at the positions of the SZ detections. Photometric redshift estimates from the BCS data indicate that two of the clusters lie at moderate redshift ( z ∼ 0.4) and two at high redshift ( z ≳ 0.8). One of the SZ detections was previously identified as a galaxy cluster in the optical as part of the Abell supplementary southern cluster catalog and in the X-ray using data from the ROSAT All-Sky Survey (RASS). Potential RASS counterparts (not previously identified as clusters) are also found for two of the new discoveries. These first four galaxy clusters are the most significant SZ detections from a subset of the ongoing SPT survey. As such, they serve as a demonstration that SZ surveys, and the SPT in particular, can be an effective means for finding galaxy clusters.
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LSST will identify optical counterparts and provide deep optical imaging for clusters detected in other wavebands.
“In addition, LSST will identify optical counterparts and provide deep optical imaging for clusters detected in other wavebands ( e.g., Staniszewski et al. 2009 ) .”
From LSST: From Science Drivers to Reference Design and Anticipated Data Products (2019) · cites this paper as Staniszewski et al. 2009
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Cites
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Self-citationRepresentations of celestial coordinates in FITS
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Catalog extraction in SZ cluster surveys: a matched filter approach
Melin, J.-B., Bartlett, J. G., & Delabrouille, J. (2006) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20065034 · Cited by 246 · cited 1× · see citing works
“We enhance the signal to noise in the SPT maps for sources with morphologies similar to that expected for SZ galaxy clusters through the application of matched spatial filters (Haehnelt & Tegmark 1996; Herranz et al. 2002a,b; Melin et al. 2006).”
MethodThe Hubble Deep Field North SCUBA Super-map - I. Submillimetre maps, sources and number counts
Borys, C., Chapman, S. C., Halpern, M., & Scott, D. (2003) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2003.06818.x · Cited by 237 · cited 2× · see citing works
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Self-citationMajumdar, S., & Mohr, J. J. (2004) · The Astrophysical Journal · doi:10.1086/422829 · Cited by 220 · cited 1× · see citing works
“Galaxy cluster catalogs selected via the SunyaevZel’dovich effect are promising in both respects (Carlstrom et al. 2002; Majumdar & Mohr 2004; Melin et al. 2005).”
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“The amplitude of the SZ spectral distortion is proportional to the integrated pressure along the line of sight through the cluster, and the relationship between integrated SZ flux and cluster mass is expected to have relatively low scatter (Motl et al. 2005; Nagai 2006; Shaw et al. 2008).”
BackgroundThe Impact of Galaxy Formation on the Sunyaev‐Zel'dovich Effect of Galaxy Clusters
Nagai, D. (2006) · The Astrophysical Journal · doi:10.1086/506467 · Cited by 191 · cited 1× · see citing works
“The amplitude of the SZ spectral distortion is proportional to the integrated pressure along the line of sight through the cluster, and the relationship between integrated SZ flux and cluster mass is expected to have relatively low scatter (Motl et al. 2005; Nagai 2006; Shaw et al. 2008).”
BackgroundROSAT—A New Look at the X-ray Sky
Trümper, J. (1993) · Science · doi:10.1126/science.260.5115.1769 · Cited by 189 · see citing works
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“We enhance the signal to noise in the SPT maps for sources with morphologies similar to that expected for SZ galaxy clusters through the application of matched spatial filters (Haehnelt & Tegmark 1996; Herranz et al. 2002a,b; Melin et al. 2006).”
MethodFiltering techniques for the detection of Sunyaev-Zel'dovich clusters in multifrequency maps
Herranz, D., Sanz, J. L., Hobson, M., Barreiro, R. B., Diego, J. M., Martínez-González, E., & Lasenby, A. N. (2002) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2002.05704.x · Cited by 148 · cited 1× · see citing works
“We enhance the signal to noise in the SPT maps for sources with morphologies similar to that expected for SZ galaxy clusters through the application of matched spatial filters (Haehnelt & Tegmark 1996; Herranz et al. 2002a,b; Melin et al. 2006).”
MethodMeasurements of Sunyaev‐Zel’dovich Effect Scaling Relations for Clusters of Galaxies
Benson, B. A., Church, S., Ade, P. A. R., Bock, J. J., Ganga, K. M., Henson, C. N., & Thompson, K. L. (2004) · The Astrophysical Journal · doi:10.1086/425677 · Cited by 107 · cited 1× · see citing works
“Significant SZ detections of previously known clusters have been reported in many tens of X-ray and optically selected galaxy clusters with observations spanning from radio to submillimeter wavelengths (e.g., Jones et al. 2005; Bonamente et al. 2006; Benson et al. 2004; Halverson et al. 2008).”
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Wang, S., Khoury, J., Haiman, Z., & May, M. (2004) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.70.123008 · Cited by 101 · cited 1× · see citing works
“A catalog of clusters with masses and redshifts can be used to constrain the matter density, the density fluctuation amplitude, and the dark energy equation of state (Wang & Steinhardt 1998; Haiman et al. 2001; Holder et al. 2001; Molnar et al. 2004; Wang et al. 2004; Lima & Hu 2007).”
MethodX-ray properties in massive galaxy clusters: XMM-Newton observations of the REFLEX-DXL sample
Zhang, Y.-Y., Böhringer, H., Finoguenov, A., Ikebe, Y., Matsushita, K., Schuecker, P., Guzzo, L., & Collins, C. A. (2006) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20053650 · Cited by 96 · cited 1× · see citing works
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ACBAR: The Arcminute Cosmology Bolometer Array Receiver
Runyan, M. C., Ade, P. A. R., Bhatia, R. S., Bock, J. J., Daub, M. D., Goldstein, J., Haynes, C. V., Holzapfel, W. L., Kuo, C.-L. L., Lange, A. E., et al. (2003) · The Astrophysical Journal Supplement Series · doi:10.1086/379099 · Cited by 77 · see citing works
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Herranz, D., Sanz, J. L., Barreiro, R. B., & Martinez‐Gonzalez, E. (2002) · The Astrophysical Journal · doi:10.1086/342651 · Cited by 61 · cited 1× · see citing works
“We enhance the signal to noise in the SPT maps for sources with morphologies similar to that expected for SZ galaxy clusters through the application of matched spatial filters (Haehnelt & Tegmark 1996; Herranz et al. 2002a,b; Melin et al. 2006).”
MethodH0from an orientation-unbiased sample of Sunyaev-Zel'dovich and X-ray clusters
Jones, M. E., Edge, A. C., Grainge, K., Grainger, W., Kneißl, R., Pooley, G. G., Saunders, R. A., Miyoshi, S., Tsuruta, T., Yamashita, K., et al. (2005) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2005.08626.x · Cited by 60 · cited 1× · see citing works
“Significant SZ detections of previously known clusters have been reported in many tens of X-ray and optically selected galaxy clusters with observations spanning from radio to submillimeter wavelengths (e.g., Jones et al. 2005; Bonamente et al. 2006; Benson et al. 2004; Halverson et al. 2008).”
BackgroundPhotometric redshift requirements for self-calibration of cluster dark energy studies
Lima, M., & Hu, W. (2007) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.76.123013 · Cited by 60 · cited 1× · see citing works
“A catalog of clusters with masses and redshifts can be used to constrain the matter density, the density fluctuation amplitude, and the dark energy equation of state (Wang & Steinhardt 1998; Haiman et al. 2001; Holder et al. 2001; Molnar et al. 2004; Wang et al. 2004; Lima & Hu 2007).”
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BackgroundMethodSelf-citationPoint Sources in the Context of Future SZ Surveys
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MethodSource subtraction for the extended Very Small Array and 33-GHz source count estimates
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“…drawn from models based on the Borys et al. (2003) counts for dusty protogalaxies and a version of the Toffolatti et al. (1998) counts for radio-loud active galactic nuclei (AGN) modified to match the DASI, CBI, and VSA counts at 30 GHz (Kovac et al. 2002; Mason et al. 2003; Cleary et al. 2005).”
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Mélin, J.-B., Bartlett, J. G., & Delabrouille, J. (2004) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20048093 · Cited by 36 · cited 2× · see citing works
“Galaxy cluster catalogs selected via the SunyaevZel’dovich effect are promising in both respects (Carlstrom et al. 2002; Majumdar & Mohr 2004; Melin et al. 2005).”
MethodA SEARCH FOR COSMIC MICROWAVE BACKGROUND ANISOTROPIES ON ARCMINUTE SCALES WITH BOLOCAM
Sayers, J., Golwala, S. R., Rossinot, P., Ade, P. A. R., Aguirre, J. E., Bock, J. J., Edgington, S. F., Glenn, J., Goldin, A., Haig, D., et al. (2008) · The Astrophysical Journal · doi:10.1088/0004-637x/690/2/1597 · Cited by 26 · cited 1× · see citing works
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MethodSelf-citationConstraints on the Energy Content of the Universe from a Combination of Galaxy Cluster Observables
Molnar, S. M., Haiman, Z., Birkinshaw, M., & Mushotzky, R. F. (2004) · The Astrophysical Journal · doi:10.1086/380295 · Cited by 24 · cited 1× · see citing works
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“A deep survey of a relatively small field with the VLA at 8.4 GHz produced what appeared to be a significant flux decrement (Richards et al. 1997).”
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Holzapfel, W. L., Carlstrom, J. E., Grego, L., Joy, M., & Reese, E. D. (2000) · The Astrophysical Journal · doi:10.1086/309210 · Cited by 4 · cited 1× · see citing works
“However, subsequent BIMA observations at 30 GHz were found to be inconsistent with the interpretation of the VLA decrement as being due to the SZ effect (Holzapfel et al. 2000).”
BackgroundSelf-citationObservations of Galactic and Extra-galactic Sources From the BOOMERANG and SEST Telescopes
Coble, K., Ade, P. A. R., Bock, J. J., et al. (2003) · ORCA Online Research @Cardiff (Cardiff University) · doi:10.48550/arxiv.astro-ph/0301599 · Cited by 2 · see citing works
Self-citation
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Cited by
Sorted by citations
Komatsu, E., Smith, K. M., Dunkley, J., Bennett, C. L., Gold, B., Hinshaw, G., Jarosik, N., Larson, D., Nolta, M. R., Page, L., et al. (2011) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/192/2/18 · Cited by 8,802 · see citing works
“New measurements of the SZ effect toward many individual clusters with unprecedented sensitivity are now becoming available (Staniszewski et al. 2009; Hincks et al. 2009; Plagge et al. 2010).”
BackgroundSelf-citationLSST: From Science Drivers to Reference Design and Anticipated Data Products
Ivezić, Ž., Kahn, S. M., Tyson, J. A., Abel, B., Acosta, E., Allsman, R., Alonso, D., AlSayyad, Y., Anderson, S. F., Andrew, J., et al. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/ab042c · Cited by 4,357 · see citing works
“In addition, LSST will identify optical counterparts and provide deep optical imaging for clusters detected in other wavebands (e.g., Staniszewski et al. 2009).”
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BackgroundDusty Star Forming Galaxies at High Redshift
Casey, C., Narayanan, D., & Cooray, A. (2014) · Physics Reports · doi:10.1016/j.physrep.2014.02.009 · Cited by 653 · see citing works
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MethodThe 10 Meter South Pole Telescope
Carlstrom, J. E., Ade, P. A. R., Aird, K. A., Benson, B. A., Bleem, L. E., Busetti, S., Chang, C. L., Chauvin, E., Cho, H.-M., Crawford, T. M., et al. (2011) · Publications of the Astronomical Society of the Pacific · doi:10.1086/659879 · Cited by 690 · see citing works
Self-citationGALAXY CLUSTERS DISCOVERED VIA THE SUNYAEV-ZEL'DOVICH EFFECT IN THE 2500-SQUARE-DEGREE SPT-SZ SURVEY
Bleem, L. E., Stalder, B., de Haan, T., Aird, K. A., Allen, S. W., Applegate, D., Ashby, M. L. N., Bautz, M. W., Bayliss, M. B., Benson, B. A., et al. (2015) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/216/2/27 · Cited by 689 · see citing works
“Previous SPT publications first identified SPT-CL J0509−5342, SPT-CL J0546−5345 (Staniszewski et al. 2009), SPT-CL J0540−5744, SPT-CL J2331−5051 (High et al. 2010), SPT-CL J2011−5228, and SPT-CL J2011−5725 (Song et al. 2012) as strong-lensing clusters using optical imaging data.”
BackgroundMethodInfluentialSelf-citationHasselfield, M., Hilton, M., Marriage, T. A., Addison, G. E., Barrientos, L. F., Battaglia, N., Battistelli, E. S., Bond, J. R., Crichton, D., Das, S., et al. (2013) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2013/07/008 · Cited by 453 · see citing works
CMB-S4 Science Book, First Edition
Abazajian, K. N. (2016) · doi:10.2172/1352047 · Cited by 435 · see citing works
Planckearly results. VIII. The all-sky early Sunyaev-Zeldovich cluster sample
Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Balbi, A., Banday, A. J., Barreiro, R. B., Bartelmann, M., et al. (2011) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201116459 · Cited by 429 · see citing works
Self-citationBenson, B. A., Ade, P. A. R., Ahmed, Z., Allen, S. W., Arnold, K., Austermann, J. E., Bender, A. N., Bleem, L. E., Carlstrom, J. E., Chang, C. L., et al. (2014) · CaltechAUTHORS (California Institute of Technology) · Cited by 356 · see citing works
Self-citationVieira, J. D., Crawford, T. M., Switzer, E. R., Ade, P. A. R., Aird, K. A., Ashby, M. L. N., Benson, B. A., Bleem, L. E., Brodwin, M., Carlstrom, J. E., et al. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/719/1/763 · Cited by 331 · see citing works
“This survey is 763 currently underway and the SPT team recently published the first-ever discovery of galaxy clusters through their SZ signature (Staniszewski et al. 2009, hereafter S09).”
BackgroundSelf-citationVanderlinde, K., Crawford, T. M., de Haan, T., Dudley, J. P., Shaw, L., Ade, P. A. R., Aird, K. A., Benson, B. A., Bleem, L. E., Brodwin, M., et al. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/722/2/1180 · Cited by 328 · see citing works
“However, it was not until very recently that the first previously unknown clusters were identified through their thermal SZ effect (Staniszewski et al. 2009).”
Self-citationBenson, B. A., Ade, P. A. R., Ahmed, Z., Allen, S. W., Arnold, K., Austermann, J. E., Bender, A. N., Bleem, L. E., Carlstrom, J. E., Chang, C. L., et al. (2014) · Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE · doi:10.1117/12.2057305 · Cited by 326 · see citing works
Self-citationPlanck 2015 results - XXVII. The second Planck catalogue of Sunyaev-Zeldovich sources
Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Barrena, R., Bartlett, J. G., et al. (2015) · LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas) · doi:10.1051/0004-6361/201525823 · Cited by 321 · see citing works
“The method was later adopted by the SPT and ACT collaborations (Staniszewski et al. 2009; Marriage et al. 2011).”
Self-citationMarriage, T. A., Acquaviva, V., Ade, P. A. R., Aguirre, P., Amiri, M., Appel, J. W., Barrientos, L. F., Battistelli, E. S., Bond, J. R., Brown, B., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/737/2/61 · Cited by 300 · see citing works
“The first blind detections of galaxy clusters through their Sunyaev-Zel’dovich effect were reported by Staniszewski et al. (2009) for the South Pole Telescope (SPT; Carlstrom et al. 2009).”
BackgroundMethodSelf-citationThe Atacama Cosmology Telescope: A Catalog of >4000 Sunyaev–Zel’dovich Galaxy Clusters
Hilton, M., Sifón, C., Naess, S., Madhavacheril, M., Oguri, M., Rozo, E., Rykoff, E. S., Abbott, T. M. C., Adhikari, S., Aguena, M., et al. (2021) · The Astrophysical Journal Supplement Series · doi:10.3847/1538-4365/abd023 · Cited by 294 · see citing works
“In particular, we used redshifts from previously published SZ surveys by ACT (Menanteau et al. 2013; Sifón et al. 2016; Hilton et al. 2018), Planck (Planck Collaboration et al. 2016b), and SPT (Bleem et al. 2015b, 2020; Bocquet et al. 2019); optically selected cluster catalogs based on SDSS (Wen et al. 2012; Wen & Han…”
BackgroundInfluentialSelf-citationRadio and millimeter continuum surveys and their astrophysical implications
de Zotti, G., Massardi, M., Negrello, M., & Wall, J. V. (2009) · The Astronomy and Astrophysics Review · doi:10.1007/s00159-009-0026-0 · Cited by 291 · see citing works
“…the hot gas responsible for the X-ray emission of rich clusters of galaxies has been detected with high signal-to-noise and even imaged in many tens of objects (Carlstrom et al. 2002; Benson et al. 2004; Jones et al. 2005; Bonamente et al. 2006; Halverson et al. 2009; Staniszewski et al. 2009).”
BackgroundLeauthaud, A., Finoguenov, A., Kneib, J., Taylor, J. E., Massey, R. J., Rhodes, J. D., Ilbert, O., Bundy, K., Tinker, J. L., George, M. R., et al. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/709/1/97 · Cited by 286 · see citing works
Reichardt, C. L., Stalder, B., Bleem, L. E., Montroy, T. E., Aird, K. A., Andersson, K., Armstrong, R., Ashby, M. L. N., Bautz, M. W., Bayliss, M. B., et al. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/763/2/127 · Cited by 276 · see citing works
“The 2009 data in this work are calibrated using observations of RCW38, a galactic HII region (Staniszewski et al. 2009, W11), while the 2008 data are calibrated by cross-correlating dedicated SPT observations of large patches of sky with WMAP observations of those same regions (V10).”
MethodSelf-citationWilliamson, R., Benson, B. A., High, F. W., Vanderlinde, K., Ade, P. A. R., Aird, K. A., Andersson, K., Armstrong, R., Ashby, M. L. N., Bautz, M. W., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/738/2/139 · Cited by 271 · see citing works
Self-citationBenson, B. A., de Haan, T., Dudley, J. P., Reichardt, C. L., Aird, K. A., Andersson, K., Armstrong, R., Ashby, M. L. N., Bautz, M. W., Bayliss, M. B., et al. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/763/2/147 · Cited by 255 · see citing works
“Recently, the first SZ cluster catalogs from three surveys have been released: the South Pole Telescope (SPT; Staniszewski et al. 2009; Vanderlinde et al. 2010; Williamson et al. 2011), the Atacama Cosmology Telescope (Marriage et al. 2011), and the Planck satellite (Planck Collaboration et al.…”
BackgroundSelf-citationDesai, S., Armstrong, R., Mohr, J. J., Semler, D. R., Liu, J., Bertin, E., Allam, S., Barkhouse, W., Bazin, G., Buckley‐Geer, E., et al. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/757/1/83 · Cited by 238 · see citing works
“These clusters and their BCS derived redshifts have figured prominently in SPT publications to date (Staniszewski et al. 2009; Vanderlinde et al. 2010; High et al. 2010; Andersson et al. 2011; Williamson et al. 2011; Reichardt et al. 2012; Song et al. 2012).”
Self-citationCui, W., Knebe, A., Yepes, G., Pearce, F. R., Power, C., Davé, R., Arth, A., Borgani, S., Dolag, K., Elahi, P. J., et al. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty2111 · Cited by 231 · see citing works
“Numerous works have been devoted to investigate and understand this effect, both observationally (e.g. Staniszewski et al. 2009; Marriage et al. 2011; Planck Collaboration XXXII 2015) and theoretically by means of cosmological simulations (e.g. da Silva et al. 2000; Sembolini et al. 2013; Le Brun,…”
BackgroundA MEASUREMENT OF GRAVITATIONAL LENSING OF THE MICROWAVE BACKGROUND USING SOUTH POLE TELESCOPE DATA
van Engelen, A., Keisler, R., Zahn, O., Aird, K. A., Benson, B. A., Bleem, L. E., Carlstrom, J. E., Chang, C. L., Cho, H. M., Crawford, T. M., et al. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/756/2/142 · Cited by 267 · see citing works
“…sample of galaxy clusters for cosmological studies, e.g., for measuring the growth of structure to constrain the dark energy equation of state (Staniszewski et al. 2009; Vanderlinde et al. 2010; Foley et al. 2011; Williamson et al. 2011) and to measure the power spectrum of the mm-wave sky…”
BackgroundSelf-citationPlanckearly results. XI. Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations
Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Balbi, A., Banday, A. J., Barreiro, R. B., Bartelmann, M., et al. (2011) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201116458 · Cited by 230 · see citing works
Self-citationVanderlinde, K., Crawford, T. M., de Haan, T., Dudley, J. P., Shaw, L. D., Ade, P. A. R., Aird, K. A., Benson, B. A., Bleem, L. E., Brodwin, M., et al. (2010) · Max Planck Digital Library · Cited by 220 · see citing works
Self-citationAstrophysics with the Spatially and Spectrally Resolved Sunyaev-Zeldovich Effects
Mroczkowski, T. K., Nagai, D., Basu, K., Chluba, J., Sayers, J., Adam, R., Churazov, E., Crites, A. T., Mascolo, L. D., Eckert, D., et al. (2019) · Space Science Reviews · doi:10.1007/s11214-019-0581-2 · Cited by 218 · see citing works
Self-citationMASS FUNCTION PREDICTIONS BEYOND ΛCDM
Bhattacharya, S., Heitmann, K., White, M. J., Lukić, Z., Wagner, C., & Habib, S. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/732/2/122 · Cited by 209 · see citing works
“2010; Abbott et al. 2005; Vikhlinin et al. 2009; Kosowsky 2003; Staniszewski et al. 2009; Bartlett et al. 2008; Fang & Haiman 2008).”
BackgroundThe SPTpol Extended Cluster Survey
Bleem, L. E., Bocquet, S., Stalder, B., Gladders, M. D., Ade, P. A. R., Allen, S. W., Anderson, A. J., Annis, J. T., Ashby, M. L. N., Austermann, J. E., et al. (2020) · The Astrophysical Journal Supplement Series · doi:10.3847/1538-4365/ab6993 · Cited by 208 · see citing works
Self-citationMcDonald, M., Benson, B. A., Vikhlinin, A. A., Stalder, B., Bleem, L. E., de Haan, T., Lin, H. W., Aird, K. A., Ashby, M. L. N., Bautz, M. W., et al. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/774/1/23 · Cited by 199 · see citing works
“The SPT-SZ survey was completed in November 2011, producing maps in three frequency bands (95, 150, and 220 GHz), with a key science goal of discovering clusters via the SZ effect (Staniszewski et al. 2009; Vanderlinde et al. 2010; Williamson et al. 2011; Benson et al. 2013; Reichardt et al. 2013).”
MethodSelf-citationACTPol: a polarization-sensitive receiver for the Atacama Cosmology Telescope
Niemack, M. D., Ade, P. A. R., Aguirre, J., Barrientos, L. F., Beall, J. A., Bond, J. R., Britton, J., Cho, H.-M., Das, S., Devlin, M. J., et al. (2010) · Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE · doi:10.1117/12.857464 · Cited by 199 · see citing works
Self-citationNext generation cosmology: constraints from theEuclidgalaxy cluster survey
Sartoris, B., Biviano, A., Fedeli, C., Bartlett, J. G., Borgani, S., Costanzi, M., Giocoli, C., Moscardini, L., Weller, J., Ascaso, B., et al. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw630 · Cited by 192 · see citing works
“…et al. 2001; Vikhlinin et al. 2009; Clerc et al. 2012; Rapetti et al.2013); sub-mm, through the Sunyaev & Zeldovich (1972) distortion (SZ henceforth, Staniszewski et al. 2009; Benson et al. 2013; Planck Collaboration et al. 2014b; Burenin & Vikhlinin 2012), and optical (Rozo et al. 2010) bands.”
BackgroundMEASUREMENTS OF SECONDARY COSMIC MICROWAVE BACKGROUND ANISOTROPIES WITH THE SOUTH POLE TELESCOPE
Lueker, M., Reichardt, C. L., Schaffer, K. K., Zahn, O., Ade, P. A. R., Aird, K. A., Benson, B. A., Bleem, L. E., Carlstrom, J. E., Chang, C. L., et al. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/719/2/1045 · Cited by 181 · see citing works
Self-citationReichardt, C. L., Stalder, B., Bleem, L. E., Montroy, T. E., Aird, K. A., Andersson, K., Armstrong, R., Ashby, M. L. N., Bautz, M. W., Bayliss, M. B., et al. (2012) · DSpace@MIT (Massachusetts Institute of Technology) · Cited by 181 · see citing works
Self-citationMass Profiles of Galaxy Clusters from X-ray Analysis
Ettori, S., Donnarumma, A., Pointecouteau, É., Reiprich, T. H., Giodini, S., Lovisari, L., & Schmidt, R. W. (2013) · Space Science Reviews · doi:10.1007/s11214-013-9976-7 · Cited by 178 · see citing works
“…many surveys over wide areas of the sky have started to produce results (e.g., the South Pole Telescope reported the first SZ-discovered clusters in Staniszewski et al. 2009; the Atacama Cosmology Telescope has also recently reported their initial catalog of SZ-discovered clusters in Marriage et…”
BackgroundAndersson, K., Benson, B. A., Ade, P. A. R., Aird, K. A., Armstrong, B., Bautz, M. W., Bleem, L. E., Brodwin, M., Carlstrom, J. E., Chang, C. L., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/738/1/48 · Cited by 175 · see citing works
“The data from the first of these fields was used to report the first SZ-discovered clusters (Staniszewski et al. 2009), to measure source counts of extragalactic mm-wavelength emitting objects (Vieira et al. 2009), and to measure small scale temperature anisotropies due to the SZ effect from…”
BackgroundMethodSelf-citationHilton, M., Hasselfield, M., Sifón, C., Battaglia, N., Aiola, S., Bharadwaj, V., Bond, J. R., Choi, S. K., Crichton, D., Datta, R., et al. (2018) · The Astrophysical Journal Supplement Series · doi:10.3847/1538-4365/aaa6cb · Cited by 172 · see citing works
“…using the thermal Sunyaev–Zel’dovich effect (SZ; Sunyaev & Zeldovich 1972) is now firmly established as a robust method for cluster detection (e.g., Staniszewski et al. 2009; Vanderlinde et al. 2010; Marriage et al. 2011; Hasselfield et al. 2013; Bleem et al. 2015; Planck Collaboration et al.…”
BackgroundMethodSelf-citationHlavacek-Larrondo, J., McDonald, M., Benson, B. A., Forman, W., Allen, S. W., Bleem, L. E., Ashby, M. L. N., Bocquet, S., Brodwin, M., Dietrich, J. P., et al. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/805/1/35 · Cited by 161 · see citing works
“These SZ surveys include: the South Pole Telescope (SPT) (Staniszewski et al. 2009; Vanderlinde et al. 2010; Reichardt et al. 2013; Bleem et al. 2014), the Planck satellite (Planck Collaboration 2011, Planck-29 1 We note that Chandra actually holds the potential to resolve X-ray cavities of ∼ 20…”
BackgroundSelf-citationThe Remarkable Similarity of Massive Galaxy Clusters from z ∼ 0 to z ∼ 1.9
McDonald, M., Allen, S. W., Bayliss, M. B., Benson, B. A., Bleem, L. E., Brodwin, M., Bülbül, E., Carlstrom, J. E., Forman, W., Hlavacek-Larrondo, J., et al. (2017) · The Astrophysical Journal · doi:10.3847/1538-4357/aa7740 · Cited by 159 · see citing works
“Since the first discovery of a galaxy cluster via the SZ effect (Staniszewski et al. 2009), the number of new, distant, SZ-selected galaxy clusters has, on average, more than doubled every year (Vanderlinde et al. 2010; Marriage et al. 2011; Planck Collaboration et al. 2011; Hasselfield et al.…”
BackgroundSelf-citationSUNYAEV–ZEL’DOVICH CLUSTER PROFILES MEASURED WITH THE SOUTH POLE TELESCOPE
Plagge, T., Benson, B. A., Ade, P. A. R., Aird, K. A., Bleem, L. E., Carlstrom, J. E., Chang, C. L., Cho, H.-M., Crawford, T. M., Crites, A. T., et al. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/716/2/1118 · Cited by 147 · see citing works
Self-citationMulti-wavelength study of XMMU J2235.3-2557: the most massive galaxy cluster at z > 1
Rosati, P., Tozzi, P., Gobat, R. A. S., Santos, J. S., Nonino, M., Demarco, R., Lidman, C. E., Mullis, C. R., Strazzullo, V., Böhringer, H., et al. (2009) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200913099 · Cited by 147 · see citing works
“Given its large mass, XMM2235 will also likely be an ideal target for a new array of Sunayev-Zeldovich (SZ) experiments which are already operational (e.g. Staniszewski et al. 2009) or are becoming available.”
BackgroundTOWARD UNBIASED GALAXY CLUSTER MASSES FROM LINE-OF-SIGHT VELOCITY DISPERSIONS
Saro, A., Mohr, J. J., Bazin, G., & Dolag, K. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/772/1/47 · Cited by 141 · see citing works
“…Yee 2005; Koester et al. 2007; Hao et al. 2010; Szabo et al. 2011), and as distortions of the cosmic microwave background as predicted by Sunyaev & Zel’dovich (1972; e.g., Staniszewski et al. 2009; Vanderlinde et al. 2010; Marriage et al. 2011; Planck Collaboration et al. 2011; Song et al. 2012b).”
Self-citationOPTICAL SPECTROSCOPY AND VELOCITY DISPERSIONS OF GALAXY CLUSTERS FROM THE SPT-SZ SURVEY
Ruel, J., Bazin, G., Bayliss, M. B., Brodwin, M., Foley, R. J., Stalder, B., Aird, K. A., Armstrong, R., Ashby, M. L. N., Bautz, M. W., et al. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/792/1/45 · Cited by 138 · see citing works
“…South Pole Telescope (SPT), Atacama Cosmology Telescope (ACT), and Planck having identified over 1000 clusters by their SZ distortion (see, e.g., Staniszewski et al. 2009; Vanderlinde et al. 2010; Williamson et al. 2011; Reichardt et al. 2013; Marriage et al. 2011; Hasselfield et al. 2013;…”
BackgroundSelf-citationReiprich, T. H., Basu, K., Ettori, S., Israel, H., Lovisari, L., Molendi, S., Pointecouteau, É., & Roncarelli, M. (2013) · Space Science Reviews · doi:10.1007/s11214-013-9983-8 · Cited by 138 · see citing works
“Recent advances in detector technology have made the first blind detection of SZ clusters possible (Staniszewski et al. 2009), and three large-scale experiments are currently in operation which are providing many more SZ selected clusters out to z = 1 and beyond: the South Pole Telescope…”
BackgroundDobbs, M., Lueker, M., Aird, K. A., Bender, A. N., Benson, B. A., Bleem, L. E., Carlstrom, J. E., Chang, C. L., Cho, H.-M., Clarke, J. L., et al. (2012) · Review of Scientific Instruments · doi:10.1063/1.4737629 · Cited by 137 · see citing works
Self-citationMass profiles of Galaxy Clusters from X-ray analysisPreprint
Ettori, S., Donnarumma, A., Pointecouteau, É., Stefania, R., Lorenzo, G., Robert, L., & Schmidt, W. (2013) · Cited by 136 · see citing works
Scaling Relations for Galaxy Clusters: Properties and Evolution
Giodini, S., Lovisari, L., Pointecouteau, É., Ettori, S., Reiprich, T. H., & Hoekstra, H. (2013) · Space Science Reviews · doi:10.1007/s11214-013-9994-5 · Cited by 135 · see citing works
“The first clusters discovered in a blind SZ survey were reported by Staniszewski et al. (2009) who used data from the South Pole Telescope (SPT; Carlstrom et al. 2011) and demonstrated the capability of the SZ signal for cluster-finding.”
MethodSzabo, T., Pierpaoli, E., Dong, F., Pipino, A., & Gunn, J. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/736/1/21 · Cited by 134 · see citing works
“In addition, galaxy clusters have now been detected via their SZ effect (Staniszewski et al. 2009).”
BackgroundSaro, A., Bocquet, S., Rozo, E., Benson, B. A., Mohr, J. J., Rykoff, E. S., Soares-Santos, M., Bleem, L. E., Dodelson, S., Melchior, P., et al. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv2141 · Cited by 130 · see citing works
“Large, homogeneously selected samples of clusters are useful for both cosmological and astrophysical studies, and such samples have recently begun to be produced using SZE selection (Staniszewski et al. 2009; Hasselfield et al. 2013; Bleem et al. 2015b; Planck Collaboration 2015).”
BackgroundSelf-citationDISCOVERY AND COSMOLOGICAL IMPLICATIONS OF SPT-CL J2106-5844, THE MOST MASSIVE KNOWN CLUSTER AT z>1
Foley, R. J., Andersson, K., Bazin, G., de Haan, T., Ruel, J., Ade, P. A. R., Aird, K. A., Armstrong, R., Ashby, M. L. N., Bautz, M. W., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/731/2/86 · Cited by 126 · see citing works
“The first three SZ-discovered clusters were reported by the SPT collaboration (Staniszewski et al. 2009).”
BackgroundMethodSelf-citationPlanckearly results. XII. Cluster Sunyaev-Zeldovich optical scaling relations
Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Balbi, A., Banday, A. J., Barreiro, R. B., Bartelmann, M., Bartlett, J. G., et al. (2011) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201116489 · Cited by 123 · see citing works
Weak lensing analysis of SZ-selected clusters of galaxies from the SPT and Planck surveys
Gruen, D., Seitz, S., Brimioulle, F., Kosyra, R., Koppenhoefer, J., Lee, C., Bender, R., Riffeser, A., Eichner, T., Weidinger, T., et al. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu949 · Cited by 119 · see citing works
“Staniszewski et al. (2009) describe the system as one of the first clusters discovered in an SZ survey.”
BackgroundCluster galaxy dynamics and the effects of large-scale environment
White, M. J., Cohn, J. D., & Smit, R. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.17248.x · Cited by 118 · see citing works
“…Herzog & Wild 1966), they are now also routinely found as luminous, extended X-ray sources (Schwartz 1978; McHardy 1978; Bohringer et al. 2000, 2001), as peaks in the shear field (Wittman et al. 2006) and as ‘holes’ in the microwave E-mail: mwhite@berkeley.edu sky (Staniszewski et al. 2009).”
BackgroundMenanteau, F., González, J., Juin, J. B., Marriage, T. A., Reese, E. D., Acquaviva, V., Aguirre, P., Appel, J. W., Baker, A. J., Barrientos, L. F., et al. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/723/2/1523 · Cited by 118 · see citing works
“Four clusters in our sample overlap with SZE discovered systems previously reported by SPT.”
BackgroundResultInfluentialThe Websky extragalactic CMB simulations
Stein, G., Alvarez, M. A., Bond, J. R., van Engelen, A., & Battaglia, N. (2020) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2020/10/012 · Cited by 116 · see citing works
Sembolini, F., Yepes, G., Petris, M. D., Gottlöber, S., Lamagna, L., & Comis, B. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sts339 · Cited by 116 · see citing works
“…have shown the possibility of detecting undiscovered clusters only through SZ effect observations, as in the claims by South Pole Telescope (SPT, Staniszewski et al. 2009; Vanderlindeet al. 2010; (Andersson & SPT Collaboration 2010); Williamson et al. 2011), Atacama Cosmology Telescope (ACT,…”
BackgroundSong, J., Zenteno, A., Stalder, B., Desai, S., Bleem, L. E., Aird, K. A., Armstrong, R., Ashby, M. L. N., Bayliss, M. B., Bazin, G., et al. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/761/1/22 · Cited by 115 · see citing works
“Originally we imaged regions of the sky with uniformly deep, multiband observations in griz optical bands to confirm SZ detections and estimate redshifts as in Staniszewski et al. (2009).”
MethodSelf-citationOutskirts of Galaxy ClustersPreprint
Ettori, S., Lorenzo, H. I., Silvano, L., Etienne, M., Roncarelli, M., Reiprich, T. H., Basu, K., Israel, H., Lovisari, L., Ettori, S., et al. (2016) · Cited by 115 · see citing works
Brodwin, M., Ruel, J., Ade, P. A. R., Aird, K. A., Andersson, K., Ashby, M. L. N., Bautz, M. W., Bazin, G., Benson, B. A., Bleem, L. E., et al. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/721/1/90 · Cited by 114 · see citing works
Self-citationSifón, C., Menanteau, F., Hasselfield, M., Marriage, T. A., Hughes, J. P., Barrientos, L. F., González, J., Infante, L., Addison, G. E., Baker, A. J., et al. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/772/1/25 · Cited by 111 · see citing works
“This number is consistent with previous optical and X-ray studies of local clusters (e.g., Girardi et al. 1997; Schuecker et al. 2001) and is also consistent with the X-ray follow-up of SPT SZE-detected clusters by Andersson et al. (2011).”
BackgroundMethodInfluentialTEMPLATES FOR THE SUNYAEV–ZEL’DOVICH ANGULAR POWER SPECTRUM
Trac, H., Bode, P., & Ostriker, J. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/727/2/94 · Cited by 95 · see citing works
“These templates have recently been used by ACT and SPT, as discussed above.”
BackgroundInfluentialStrazzullo, V., Rosati, P., Pannella, M., Gobat, R. A. S., Santos, J., Nonino, M., Demarco, R., Lidman, C. E., Tanaka, M., Mullis, C. R., et al. (2010) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201015251 · Cited by 100 · see citing works
LoCuSS: THE SUNYAEV–ZEL'DOVICH EFFECT AND WEAK-LENSING MASS SCALING RELATION
Marrone, D. P., Smith, G. P., Okabe, N., Bonamente, M., Carlstrom, J. E., Culverhouse, T. L., Gralla, M., Greer, C. H., Hasler, N., Hawkins, D., et al. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/754/2/119 · Cited by 100 · see citing works
“…can be used to identify large numbers of clusters via the Sunyaev-Zel’dovich (SZ) effect, as has been demonstrated by the South Pole Telescope (SPT; Staniszewski et al. 2009; Vanderlinde et al. 2010; Williamson et al. 2011), the Atacama Cosmology Telescope (ACT; Marriage et al. 2011), and the…”
MethodSelf-citationMiyatake, H., Battaglia, N., Hilton, M., Medezinski, E., Nishizawa, A. J., More, S., Aiola, S., Bahcall, N., Bond, J. R., Calabrese, E., et al. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/ab0af0 · Cited by 98 · see citing works
“…Carlstrom et al. 2011), and the Planck satellite (Planck Collaboration et al. 2016a) have provided large catalogs of SZ-selected clusters (e.g., Staniszewski et al. 2009; Marriage et al. 2011; Hasselfield et al. 2013; Reichardt et al. 2013; Planck Collaboration et al. 2014a, 2016b; Bleem et…”
BackgroundSelf-citationCosmological constraints from Planck galaxy clusters with CMB lensing mass bias calibration
Zubeldía, Í., & Challinor, A. D. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz2153 · Cited by 98 · see citing works
“…signature (Sunyaev & Zeldovich 1972), have provided useful observations of this abundance from which cosmological constraints have been obtained (e.g. Staniszewski et al. 2009; Mantz et al. 2010; Hasselfield et al. 2013; Bleem et al. 2015; de Haan et al. 2016; Planck 2015 Results XXVII 2016;…”
BackgroundAndreon, S., Maughan, B. J., Trinchieri, G., & Kurk, J. D. (2009) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200912299 · Cited by 98 · see citing works
Dietrich, J. P., Bocquet, S., Schrabback, T., Applegate, D., Hoekstra, H., Grandis, S., Mohr, J. J., Allen, S. W., Bayliss, M. B., Benson, B. A., et al. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty3088 · Cited by 97 · see citing works
“Details of the survey strategy and data processing are provided elsewhere (Staniszewski et al. 2009; Vanderlinde et al. 2010; Williamson et al. 2011).”
MethodSelf-citationAde, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Balbi, A., Banday, A. J., Barreiro, R. B., et al. (2013) · Maynooth University ePrints and eTheses Archive (Maynooth University) · doi:10.1051/0004-6361/201220941 · Cited by 96 · see citing works
Self-citationTHE FIRST PUBLIC RELEASE OF SOUTH POLE TELESCOPE DATA: MAPS OF A 95 deg2FIELD FROM 2008 OBSERVATIONS
Schaffer, K. K., Crawford, T. M., Aird, K. A., Benson, B. A., Bleem, L. E., Carlstrom, J. E., Chang, C. L., Cho, H.-M., Crites, A. T., de Haan, T., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/743/1/90 · Cited by 95 · see citing works
“…to extract power spectrum measurements (Lueker et al. 2010; Hall et al. 2010; Shirokoff et al. 2011; Keisler et al. 2011) and to produce catalogs of emissive sources (Vieira et al. 2010) and SZselected galaxy clusters (Staniszewski et al. 2009; Vanderlinde et al. 2010; Williamson et al. 2011).”
BackgroundMethodInfluentialSelf-citationTHE ATACAMA COSMOLOGY TELESCOPE: EXTRAGALACTIC SOURCES AT 148 GHz IN THE 2008 SURVEY
Marriage, T. A., Juin, J. B., Lin, Y., Marsden, D. W., Nolta, M. R., Partridge, B., Ade, P. A. R., Aguirre, P., Amiri, M., Appel, J. W., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/731/2/100 · Cited by 93 · see citing works
“This approach has been proposed and used in previous work to find both sources (Tegmark & de Oliveira-Costa 1998; Wright et al. 2009; Vieira et al. 2010) and the Sunyaev-Zel’dovich effect from clusters (Melin et al. 2006; Staniszewski et al. 2009).”
MethodSelf-citationThe synergy between CMB spectral distortions and anisotropies
Lucca, M., Schöneberg, N., Hooper, D. C., Julien Lesgourgues, A., & Chluba, J. (2020) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2020/02/026 · Cited by 103 · see citing works
THE ATACAMA COSMOLOGY TELESCOPE (ACT): BEAM PROFILES AND FIRST SZ CLUSTER MAPS
Hincks, A. D., Acquaviva, V., Ade, P. A. R., Aguirre, P., Amiri, M., Appel, J. W., Barrientos, L. F., Battistelli, E. S., Bond, J. R., Brown, B., et al. (2010) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/191/2/423 · Cited by 93 · see citing works
Self-citationA MACHINE LEARNING APPROACH FOR DYNAMICAL MASS MEASUREMENTS OF GALAXY CLUSTERS
Ntampaka, M., Trac, H., Sutherland, D. J., Battaglia, N., Póczos, B., & Schneider, J. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/803/2/50 · Cited by 87 · see citing works
“…signature in the cosmic microwave background, as a decrement below 218 GHz and an increment above, as predicted by Sunyaev & Zeldovich (1972) (e.g. Staniszewski et al. 2009; Marriage et al. 2011; Planck Collaboration et al. 2014c). ntampaka@cmu.edu 1 McWilliams Center for Cosmology, Department of…”
MethodSunyaev-Zeldovich clusters in Millenium gas simualtions
Kay, S., Peel, M., Short, C., Thomas, P., Young, O., Battye, R., Liddle, A., & Pearce, F. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.20623.x · Cited by 54 · see citing works
“In the past few years, SZ science has entered the exciting new phase of blind surveys, where detections of new clusters have become possible (Staniszewski et al. 2009).”
BackgroundSPTpol: an instrument for CMB polarization measurements with the South Pole Telescope
Austermann, J. E., Lueker, M., Shirokoff, E. D., & Vieira, J. D. (2012) · CaltechAUTHORS (California Institute of Technology) · Cited by 81 · see citing works
Self-citationGalaxy Clusters Selected via the Sunyaev–Zel’dovich Effect in the SPTpol 100-square-degree Survey
Huang, N., Bleem, L. E., Stalder, B., Ade, P. A. R., Allen, S. W., Anderson, A. J., Austermann, J. E., Avva, J. S., Beall, J. A., Bender, A. N., et al. (2020) · The Astronomical Journal · doi:10.3847/1538-3881/ab6a96 · Cited by 80 · see citing works
Self-citationHilton, M., Hasselfield, M., Sifón, C., Battaglia, N., Aiola, S., Bharadwaj, V., Bond, J. R., Choi, S. K., Crichton, D., Datta, R., et al. (2018) · Americanae (AECID Library) · Cited by 79 · see citing works
Self-citationScaling relations for galaxy clusters: Properties and evolution
Giodini, S., Lovisari, L., Pointecouteau, É., Ettori, S., Reiprich, T. H., & Hoekstra, H. (2013) · TNO Repository · Cited by 78 · see citing works
The XMM Cluster Survey: X-ray analysis methodology
Lloyd-Davies, E. J., Romer, A. K., Mehrtens, N., Hosmer, M., Davidson, M., Sabirli, K., Mann, R. G., Hilton, M., Liddle, A. R., Viana, P. T. P., et al. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.19117.x · Cited by 78 · see citing works
“Increasing numbers of clusters are also being discovered at millimetre wavelengths (e.g. Staniszewski et al. 2009; Marriage et al. 2011; Menanteau et al. 2010; Vanderlinde et al. 2010; Ade et al. 2011; Foley et al. 2011; Williamson et al. 2011) using the Sunyaev–Zel’dovich (SZ) effect (Sunyaev &…”
MethodDiehl, H. T., Buckley‐Geer, E., Lindgren, K. A., Nord, B., Gaitsch, H., Gaitsch, S., Lin, H., Allam, S., Collett, T. E., Furlanetto, C., et al. (2017) · The Astrophysical Journal Supplement Series · doi:10.3847/1538-4365/aa8667 · Cited by 77 · see citing works
“Many of the clusters have strong lens systems apparent in optical imaging follow-up observations (Staniszewski et al. 2009; Song et al. 2012; Aravena et al. 2013; Bleem et al. 2015).”
BackgroundThe synergy between CMB spectral distortions and anisotropies
Lucca, M., Schöneberg, N., Hooper, D. C., Julien Lesgourgues, A., & Chluba, J. (2020) · RWTH Publications (RWTH Aachen) · Cited by 75 · see citing works
Foley, R., Andersson, K., Bazin, G., de Haan, T., Ruel, J., Ade, P. A. R., Aird, K. A., Armstrong, R., Ashby, M. L. N., Bautz, M. W., et al. (2011) · DSpace@MIT (Massachusetts Institute of Technology) · Cited by 74 · see citing works
Self-citationIMPLICATIONS OF A HIGH ANGULAR RESOLUTION IMAGE OF THE SUNYAEV-ZEL'DOVICH EFFECT IN RXJ1347–1145
Mason, B., Dicker, S., Korngut, P., Devlin, M. J., Cotton, W. D., Koch, P. M., Molnar, S. M., Sievers, J. L., Aguirre, J., Benford, D. J., et al. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/716/1/739 · Cited by 74 · see citing works
Self-citationMacCrann, N., Sherwin, B. D., Qu, F. J., Namikawa, T., Madhavacheril, M. S., Abril-Cabezas, I., An, R., Austermann, J. E., Battaglia, N., Battistelli, E. S., et al. (2024) · The Astrophysical Journal · doi:10.3847/1538-4357/ad2610 · Cited by 73 · see citing works
Self-citationConstraining ƒ(R) Gravity by the Large-Scale Structure
Martino, I. D., Laurentis, M. D., & Capozzıello, S. (2015) · Universe · doi:10.3390/universe1020123 · Cited by 73 · see citing works
SZE observables, pressure profiles and centre offsets in Magneticum simulation galaxy clusters
Gupta, N., Saro, A., Mohr, J., Dolag, K., & Liu, J.-Y. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx715 · Cited by 42 · see citing works
“Since Staniszewski et al. (2009) presented the first SZE selected clusters, ongoing surveys in microwave bands such as the South Pole Telescope (SPT), the Atacama Cosmology Telescope (ACT) and Planck have yielded hundreds to thousands of newly discovered clusters (e.g. Vanderlinde et al. 2010;…”
BackgroundSelf-citationThe Atacama Cosmology Telescope (ACT): Beam Profiles and First SZ Cluster Maps
Hincks, A. D., Acquaviva, V., Ade, P. A. R., Aguirre, P., Amiri, M., Appel, J. W., Barrientos, L. F., Battistelli, E., Bond, J. R., Brown, B., et al. (2010) · NASA STI Repository (National Aeronautics and Space Administration) · Cited by 71 · see citing works
Self-citationSaro, A., Liu, J., Mohr, J. J., Aird, K. A., Ashby, M. L. N., Bayliss, M. B., Benson, B. A., Bleem, L. E., Bocquet, S., Brodwin, M., et al. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu575 · Cited by 70 · see citing works
“Finally, from these mock maps we identify clusters with the same approach adopted for real SPT clusters (e.g., Staniszewski et al. 2009; Reichardt et al. 2013), obtaining a sample of 212 clusters above signal to noiseξ = 4.5.”
BackgroundMethodInfluentialSelf-citationAtacama Cosmology Telescope: High-resolution component-separated maps across one third of the sky
Coulton, W. R., Madhavacheril, M. S., Duivenvoorden, A. J., Hill, J. C., Abril-Cabezas, I., Ade, P. A. R., Aiola, S., Alford, T., Amiri, M., Amodeo, S., et al. (2024) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.109.063530 · Cited by 70 · see citing works
Self-citationLin, Y., Partridge, B., Pober, J. C., Bouchefry, K. E., Burke, S., Klein, J. N., Coish, J. W., & Huffenberger, K. M. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/694/2/992 · Cited by 70 · see citing works
Deutsch, A.-S., Dimastrogiovanni, E., Johnson, M. C., Münchmeyer, M., & Terrana, A. (2018) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.98.123501 · Cited by 70 · see citing works
High, F. W., Stalder, B., Song, J., Ade, P. A. R., Aird, K. A., Allam, S., Armstrong, R., Barkhouse, W., Benson, B. A., Bertin, E., et al. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/723/2/1736 · Cited by 69 · see citing works
Self-citationDark-matter decays and self-gravitating halos
Peter, A. H. G., Moody, C. E., & Kamionkowski, M. (2010) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.81.103501 · Cited by 69 · see citing works
CMB/kSZ and Compton-y Maps from 2500 deg 2 of SPT-SZ and Planck Survey Data
Bleem, L. E., Crawford, T. M., Ansarinejad, B., Benson, B. A., Bocquet, S., Carlstrom, J. E., Chang, C. L., Chown, R., Crites, A. T., de Haan, T., et al. (2022) · The Astrophysical Journal Supplement Series · doi:10.3847/1538-4365/ac35e9 · Cited by 67 · see citing works
Self-citationBaryon content of massive galaxy clusters at 0.57 < z < 1.33
Chiu, I.-N. T., Mohr, J. J., McDonald, M., Bocquet, S., Ashby, M. L. N., Bayliss, M. B., Benson, B. A., Bleem, L. E., Brodwin, M., Desai, S., et al. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv2303 · Cited by 67 · see citing works
“Since the first SZE selected clusters were discov- ered in the SPT-SZ survey (Staniszewski et al. 2009), this method has been demonstrated to be a useful tool for discovering and studying galaxy cluster populations out to high redshift (Zenteno et al. 2011; Hilton et al. 2013, hereafter H13;…”
MethodSelf-citationBurton, M. (2010) · The Astronomy and Astrophysics Review · doi:10.1007/s00159-010-0032-2 · Cited by 66 · see citing works
Chiu, I.-N. T., Klein, M., Mohr, J. J., & Bocquet, S. (2023) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stad957 · Cited by 65 · see citing works
Self-citationStalder, B., Ruel, J., Šuhada, R., Brodwin, M., Aird, K. A., Andersson, K., Armstrong, R., Ashby, M. L. N., Bautz, M. W., Bayliss, M. B., et al. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/763/2/93 · Cited by 64 · see citing works
“The survey strategy and data analysis are detailed in the previous SPTSZ survey papers Staniszewski et al. (2009), Vanderlinde et al. (2010), Williamson et al. (2011, W11), and R12.”
BackgroundMethodSelf-citationAddison, G. E., Dunkley, J., & Spergel, D. N. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21664.x · Cited by 63 · see citing works
“…by guest on 28 July 2018 We remove the brightest 0.1 clusters per square degree in our model, roughly corresponding to a level of cluster detection currently achieved in deep ACT and SPT maps (Staniszewski et al. 2009; Benson et al. 2011; Marriage et al. 2011).”
MethodInfluentialPlanck Sunyaev–Zel’dovich cluster mass calibration using Hyper Suprime-Cam weak lensing
Medezinski, E., Battaglia, N., Umetsu, K., Oguri, M., Miyatake, H., Nishizawa, A. J., Sifón, C., Spergel, D. N., Chiu, I.-N. T., Lin, Y.-T., et al. (2017) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/psx128 · Cited by 63 · see citing works
“…(ACT; Kosowsky 2003), the South Pole Telescope (SPT; Carlstrom et al. 2011) and their successors, keep pushing the detection limits to lower masses and higher redshifts (e.g., Staniszewski et al. 2009; Marriage et al. 2011; Reichardt et al. 2013; Hasselfield et al. 2013; Bleem et al. 2015).”
Background
- Authors
- Staniszewski, Z., Ade, P. A. R., Aird, K. A., Benson, B. A., Bleem, L. E., Carlstrom, J. E., Chang, C. L., Cho, H.-M., Crawford, T. M., Crites, A. T., de Haan, T., Dobbs, M. A., Halverson, N. W., Holder, G. P., Holzapfel, W. L., Hrubes, J. D., Joy, M., Keisler, R., Lanting, T. M., Lee, A. T., Leitch, E. M., Loehr, A., Lueker, M., McMahon, J. J., Mehl, J., Meyer, S. S., Mohr, J. J., Montroy, T. E., Ngeow, C.-C., Padin, S., Plagge, T., Pryke, C., Reichardt, C. L., Ruhl, J. E., Schaffer, K. K., Shaw, L., Shirokoff, E., Spieler, H. G., Stalder, B., Stark, A. A., Vanderlinde, K., Vieira, J. D., Zahn, O., & Zenteno, A.
- Affiliations
- Case Western Reserve University (US)
- Cardiff University (GB)
- University of Chicago (US)
- University of California, Berkeley (US)
- McGill University (CA)
- University of Colorado Boulder (US)
- Marshall Space Flight Center (US)
- Lawrence Berkeley National Laboratory (US)
- Center for Astrophysics Harvard & Smithsonian (US)
- University of Illinois Urbana-Champaign (US)
- ORCID
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2009-07-20
- Volume
- 701
- Issue
- 1
- Pages
- 32-41
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2149892437
- Cited by
- 322
- References
- 46
- Citations by year
- 2026: 4 · 2025: 11 · 2024: 12 · 2023: 5 · 2022: 4 · 2021: 14 · 2020: 15 · 2019: 35 · 2018: 19 · 2017: 9 · 2016: 17 · 2015: 19 · 2014: 17 · 2013: 24 · 2012: 21
- FWCI
- 19.66
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- The Astrophysical Journal (publishedVersion)
- arXiv (Cornell University) (publishedVersion)
- arXiv (Cornell University)
- Funders
- National Science Foundation (0114422, 0813534, 0130612, 0715036, 0638937, 0708539)
- Gordon and Betty Moore Foundation
- University of Chicago
- Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley
- McGill University
- Kavli Institute for Cosmological Physics, University of Chicago
- Office of Polar Programs
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Astrophysics and Cosmic Phenomena
- Keywords
- galaxy clusters, Sunyaev-Zel'dovich effect, South Pole Telescope, high-redshift clusters, photometric redshifts, millimeter-wave observations
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