Cited by 322Galaxies: Formation, Evolution, PhenomenaCosmology and Gravitation TheoriesAstrophysics and Cosmic Phenomena

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GALAXY CLUSTERS DISCOVERED WITH A SUNYAEV-ZEL'DOVICH EFFECT SURVEY

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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.·2009·The Astrophysical Journal

DOI 10.1088/0004-637x/701/1/32

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Abstract

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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A Universal Density Profile from Hierarchical Clustering
Navarro, J. F., Frenk, C. S., & White, S. D. M. (1997) · The Astrophysical Journal · doi:10.1086/304888 · Cited by 9,917 · cited 1×
“…all motivated by some guess at the underlying threedimensional pressure profile of clusters: a modified version of the Navarro-Frenk-White (NFW; Navarro et al. 1996, 1997) model as suggested in Nagai et al. (2007), numerically integrated along the line of sight to produce a model for the SZ…”
Background
The Structure of Cold Dark Matter Halos
Navarro, J. F., Frenk, C. S., & White, S. D. M. (1996) · The Astrophysical Journal · doi:10.1086/177173 · Cited by 8,544 · cited 1×
“…all motivated by some guess at the underlying threedimensional pressure profile of clusters: a modified version of the Navarro-Frenk-White (NFW; Navarro et al. 1996, 1997) model as suggested in Nagai et al. (2007), numerically integrated along the line of sight to produce a model for the SZ…”
Background
A catalog of rich clusters of galaxies
Abell, G. O., Jr. Corwin Harold, G., & Olowin, R. P. (1989) · The Astrophysical Journal Supplement Series · doi:10.1086/191333 · Cited by 1,406 · cited 2×
“In SPT-CL 0517-5430, the cluster that was previously included in the Abell supplementary southern cluster catalog (Abell et al. 1989) and the REFLEX catalog (Böhringer et al. 2004), there is a strong red sequence population apparent in g − r versus r and a peak in the photo-z histogram.”
Background
Cosmology with the Sunyaev-Zel’dovich Effect
Carlstrom, J. E., Holder, G. P., & Reese, E. D. (2002) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.40.060401.093803 · Cited by 957
Self-citation
Cluster Abundance Constraints for Cosmological Models with a Time‐varying, Spatially Inhomogeneous Energy Component with Negative Pressure
Wang, L.-M., & Steinhardt, P. J. (1998) · The Astrophysical Journal · doi:10.1086/306436 · Cited by 932 · cited 1×
“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).”
Method
The Sunyaev–Zel'dovich effect
Birkinshaw, M. (1999) · Physics Reports · doi:10.1016/s0370-1573(98)00080-5 · Cited by 830 · cited 1×
“Observations of the SZ effect, therefore, permit the detection of clusters with a selection function that is nearly redshift-independent (Birkinshaw 1999; Carlstrom et al. 2002).”
SUMSS: a wide-field radio imaging survey of the southern sky - II. The source catalogue
Mauch, T., Murphy, T., Buttery, H. J., Curran, J., Hunstead, R. W., Piestrzynski, B., Robertson, J. G., & Sadler, E. M. (2003) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2003.06605.x · Cited by 823 · cited 1×
“The astrometry of the pointing model is tied to the PMN and SUMSS catalogs (Wright et al. 1994; Mauch et al. 2003) and is accurate to 10 arcsec in the final maps.”
Method
The ROSAT-ESO Flux Limited X-ray (REFLEX) Galaxy cluster survey
Böhringer, H., Schuecker, P., Guzzo, L., Collins, C. A., Voges, W. H., Cruddace, R. G., Gil, A. O., Chincarini, G. L., Grandi, S. D., Edge, A. C., et al. (2004) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20034484 · Cited by 652
Detection of polarization in the cosmic microwave background using DASI
Kovac, J. M., Leitch, E. M., Pryke, C. L., Carlstrom, J. E., Halverson, N. W., & Holzapfel, W. L. (2002) · Nature · doi:10.1038/nature01269 · Cited by 651 · cited 1×
“…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).”
MethodSelf-citation
Effects of Galaxy Formation on Thermodynamics of the Intracluster Medium
Nagai, D., Kravtsov, A. V., & Vikhlinin, A. (2007) · The Astrophysical Journal · doi:10.1086/521328 · Cited by 536 · cited 1×
“…threedimensional pressure profile of clusters: a modified version of the Navarro-Frenk-White (NFW; Navarro et al. 1996, 1997) model as suggested in Nagai et al. (2007), numerically integrated along the line of sight to produce a model for the SZ surface brightness; a Gaussian profile; and a…”
Method

Show all 46 references

Research works printed but not linked: 6

Carlstrom, 2009, PASP
Halverson, 2009, ApJ
Sunyaev, 1970, Comments Astrophys. Space Phys., 2, 66
Sunyaev, 1972, Comments Astrophys. Space Phys., 4, 173
Voges, 1999, A&A, 349, 389
Voges, 2000, VizieR Online Data Catalog

Sorted by citations

Items 201–300 of 319

Sunyaev-Zel’dovich observations of galaxy clusters out to the virial radius with the Arcminute Microkelvin Imager★
Zwart, J. T. L., Feroz, F., Davies, M. L., Franzen, T. M. O., Grainge, K., Hobson, M., Hurley-Walker, N., Kneißl, R., Lasenby, A. N., Olamaie, M., et al. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.19665.x · Cited by 16
“…Experiment (APEX; Dobbs et al. 2006), One Centimetre Receiver Array (OCRA; Lancaster et al. 2007), South Pole Telescope (SPT; Carlstrom et al. 2009; Staniszewski et al. 2009; Plagge et al. 2010), the Combined Array for Research in Millimeter-Wave Astronomy (CARMA) and Sunyaev–Zel’dovich Array…”
Background
The KISS Experiment
Fasano, A., Aguiar, M., Benoı̂t, A., Bideaud, A., Bourrion, O., Calvo, M., Catalano, A., de Taoro, A. P., Garde, G., Gómez, A., et al. (2019) · Journal of Low Temperature Physics · doi:10.1007/s10909-019-02289-1 · Cited by 16
XMM-Newton detection of two clusters of galaxies with strong SPT Sunyaev-Zel'dovich effect signatures
Šuhada, R., Song, J., Böhringer, H., Benson, B. A., Mohr, J. J., Fassbender, R., Finoguenov, A., Pierini, D., Pratt, G. W., Andersson, K., et al. (2010) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201014434 · Cited by 16
“…of the SunyaevZel’dovich effect (SZE, Sunyaev & Zeldovich 1972), i.e. the distortion of the cosmic microwave background spectrum by the hot gas in clusters of galaxies, we have entered a new era where the first clusters have been discovered by large-area SZE surveys (Staniszewski et al. 2009).”
BackgroundSelf-citation
Relativistic models and the expanding universe
Realdi, M. (2019) · Oxford University Press eBooks · doi:10.1093/oxfordhb/9780198817666.013.3 · Cited by 15
SALT spectroscopic observations of galaxy clusters detected by ACT and a type II quasar hosted by a brightest cluster galaxy
Kirk, B., Hilton, M., Cress, C. M., Crawford, S. M., Hughes, J. P., Battaglia, N., Bond, J. R., Burke, C., Gralla, M., Hajian, A., et al. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv595 · Cited by 15
“…of new clusters from large area surveys using the Sunyaev-Zel’dovich effect (SZ; Sunyaev & Zel’dovich 1970) began only in recent years (e.g., Staniszewski et al. 2009; Vanderlinde et al. 2010; Marriage et al. 2011; Reichardt et al. 2013; Planck Collaboration et al. 2013; Bleem et al.…”
Method
Quasar Sightline and Galaxy Evolution (QSAGE) survey – II. Galaxy overdensities around UV luminous quasars at z = 1–2
Stott, J. P., Bielby, R. M., Cullen, F., Burchett, J. N., Tejos, N., Fumagalli, M., Crain, R. A., Morris, S. L., Amos, N., Bower, R. G., et al. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa2096 · Cited by 15
“…al. 2012), the SunyaevZel’dovich (SZ) effect (Sunyaev & Zeldovich 1972) due to the scattering of cosmic microwave background photons by the ICM (e.g. Staniszewski et al. 2009; Vanderlinde et al. © 2019 The Authors 2010; Planck Collaboration et al. 2014; Bleem et al. 2015; Hilton et al. 2018), and…”
Background
Understanding X-ray and optical selection of galaxy clusters: a comparison of the XXL and CAMIRA cluster catalogues obtained in the common XXL-HSC SSP area
Willis, J. P., Oguri, M., Ramos-Ceja, M. E., Gastaldello, F., Sereno, M., Adami, C., Aliş, S., Altieri, B., Chiappetti, L., Corasaniti, P.-S., et al. (2021) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stab873 · Cited by 15
Constraining f ( R ) gravity using future galaxy cluster abundance and weak-lensing mass calibration datasets
Vogt, S. M. L., Bocquet, S., Davies, C. T., Mohr, J. J., & Schmidt, F. (2024) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.109.123503 · Cited by 14
Self-citation
The Oxford Handbook of the History of Modern Cosmology
Kragh, H., & Longair, M. (2019) · Oxford University Press eBooks · doi:10.1093/oxfordhb/9780198817666.001.0001 · Cited by 17
Probing dark energy with the next generation X-ray surveys of galaxy clusters
Sartoris, B., Borgani, S., Rosati, P., & Weller, J. (2012) · MPG.PuRe (Max Planck Society) · Cited by 14
X-ray versus infrared selection of distant galaxy clusters: a case study using the XMM–LSS and SpARCS cluster samples
Willis, J. P., Ramos-Ceja, M. E., Muzzin, A., Pacaud, F., Yee, H. K. C., & Wilson, G. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty975 · Cited by 14
“…and Sunyaev-Zeld’ovich (SZ) searches identify the apparent decrement in the brightness of the cosmic microwave background (CMB) caused by the inverse Compton scattering of CMB photons by energetic electrons in the ICM (e.g. Staniszewski et al. 2009; Marriage et al. 2011; Reichardt et al. 2013).”
Background
Mass–Richness Relations for X-Ray and SZE-selected Clusters at 0.4 < z < 2.0 as Seen by Spitzer at 4.5 μm
Rettura, A., Chary, R., Krick, J., & Ettori, S. (2018) · The Astrophysical Journal · doi:10.3847/1538-4357/aad818 · Cited by 13
“The resultant characteristic spectral distortion to the CMB is known as the Sunyaev-Zel’dovich effect (SZE, Sunyaev & Zeldovich 1972; Staniszewski et al. 2009; Hasselfield et al. 2013; Planck Collaboration et al. 2015; Bleem et al. 2015).”
Background
Sunyaev–Zel’dovich profile fitting with joint AMI-Planck analysis
Perrott, Y. C., Javid, K., Carvalho, P., Elwood, P., Hobson, M., Lasenby, A. N., Olamaie, M., & Saunders, R. D. E. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz826 · Cited by 13
“We consider simulations generated using three different sets of profile shape parameters: the UPP, the parameters fitted to a stacked Planck dataset in Planck Collaboration et al. (2013) (‘Planck Intermediate Profile’, PIP), and the parameters fitted to the cluster RXC J2319.”
Method
Biases on cosmological parameter estimators from galaxy cluster number counts
Penna-Lima, M., Makler, M., & Wuensche, C. A. (2014) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2014/05/039 · Cited by 13
On the ability of the spectroscopic Sunyaev-Zeldovich effect measurements to determine the temperature structure of galaxy clusters
Colafrancesco, S., & Marchegiani, P. (2010) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200913115 · Cited by 13
“…of the SZE are becoming increasingly accurate (e.g., LaRoque et al. 2002; De Petris et al. 2002; Battistelli et al. 2003, Halverson et al. 2009, Staniszewski et al. 2009), most analyses of SZ data are still made under the simplifying assumption of iso-thermality, or single temperature plasma.”
Background
The ACT-DR5 MCMF galaxy cluster catalog
Klein, M., Mohr, J. J., & Davies, C. T. (2024) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202451203 · Cited by 12
Self-citation
CROSS-CORRELATIONS OF THE Lyα FOREST WITH WEAK-LENSING CONVERGENCE. ANALYTICAL ESTIMATES OF SIGNAL-TO-NOISE RATIO AND IMPLICATIONS FOR NEUTRINO MASS AND DARK ENERGY
Vallinotto, A., Viel, M., Das, S., & Spergel, D. N. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/735/1/38 · Cited by 12
“Arcminute-scale CMB experiments such as Planck,6 the Atacama Cosmology Telescope7 (ACTPOL; Hincks et al. 2010), the South Pole Telescope8 (Staniszewski et al. 2009), QUIET,9 and PolarBeaR10 will chart out the small-scale anisotropies in the CMB.”
Method
Mass calibration of the CODEX cluster sample using SPIDERS spectroscopy – II. The X-ray luminosity–mass relation
Capasso, R., Mohr, J. J., Saro, A., Biviano, A., Clerc, N., Finoguenov, A., Klein, M., Grandis, S., Collins, C., Damsted, S., et al. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa888 · Cited by 12
“Many different mass proxies have been used over the years, including thermal Sunyaev–Zeldovich effect (SZE) measurements (Staniszewski et al. 2009; Hasselfield et al. 2013; Planck Collaboration XVI 2014), weak gravitational lensing features (Corless & King 2009; Becker & Kravtsov 2011; Dietrich et…”
MethodSelf-citation
The PSZ-MCMF catalogue of Planck clusters over the DES region
Hernández-Lang, D., Klein, M., Mohr, J. J., Grandis, S., Melin, J.-B., Tarrío, P., Arnaud, M., Pratt, G. W., Abbott, T. M. C., Aguena, M., et al. (2023) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stad2319 · Cited by 12
Self-citation
CosmoDM and its application to Pan-STARRS data
Desai, S., Mohr, J. J., Henderson, R., Kümmel, M., Paech, K., & Wetzstein, M. (2015) · Journal of Instrumentation · doi:10.1088/1748-0221/10/06/c06014 · Cited by 12
“The development version of this pipeline has been used to process the data from the Blanco Cosmology Survey [8] as well as pointed optical follow-up data of South Pole Telescope Sunyaev-Zeldovich effect (SZE) galaxy cluster candidates [9, 10].”
MethodSelf-citation
Sunyaev-Zel’dovich observations of a statistically complete sample of galaxy clusters with OCRA-p
Lancaster, K., Birkinshaw, M., Gawroński, M., Battye, R. A., Browne, I. W. A., Davis, R., Giles, P. A., Feiler, R., Kus, A. J., Lew, B., et al. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.19241.x · Cited by 12
“The dedicated SZ surveys, for example Planck (Ade et al. 2011), SPT (Staniszewski et al. 2009, Vanderlinde et al. 2010), ACT (Menanteau et al. 2010, Marriage et al. 2010) and the SZA (Muchovej et al. 2011) are now generating results.”
On the ability of the spectroscopic Sunyaev-Zeldovich effect measurements to determine\nthe temperature structure of galaxy clusters
Colafrancesco, S., & Marchegiani, ¶. (2010) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/200913115/pdf · Cited by 12
Sunyaev–Zel’Dovich Signal from Quasar Hosts: Implications for Detection of Quasar Feedback
Chowdhury, D. D., & Chatterjee, S. (2017) · The Astrophysical Journal · doi:10.3847/1538-4357/aa64d6 · Cited by 11
“Spacek et al. (2016) co-added the SPT (e.g., Staniszewski et al. 2009) SZ maps around quiescent elliptical galaxies and showed that the observed mean integrated Compton Y parameter is greater than what is expected from simple models without feedback.”
Background
Weak lensing mass bias and the alignment of centre proxies
Sommer, M. W., Schrabback, T., Ragagnin, A., & Rockenfeller, R. (2024) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stae1580 · Cited by 11
Multiprobe cosmology from the abundance of SPT clusters and DES galaxy clustering and weak lensing
Bocquet, S., Grandis, S., Krause, E., To, C., Bleem, L. E., Klein, M., Mohr, J. J., Schrabback, T., Alarcon, A., Alves, O., et al. (2025) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.111.063533 · Cited by 11
Self-citation
Absolute Calibration of Astronomical Flux Standards
Deustua, S. E., Kent, S., & Smith, J. A. (2013) · Springer eBooks · doi:10.1007/978-94-007-5618-2_8 · Cited by 11
Using clusters in Sunyaev-Zel’dovich effect plus x-ray surveys as an ensemble of rulers to constrain cosmology
Khedekar, S., & Majumdar, S. (2010) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.82.081301 · Cited by 11
MEASUREMENT OF GALAXY CLUSTER INTEGRATED COMPTONIZATION AND MASS SCALING RELATIONS WITH THE SOUTH POLE TELESCOPE
Saliwanchik, B. R. B., Montroy, T. E., Aird, K. A., Bayliss, M. B., Benson, B. A., Bleem, L. E., Bocquet, S., Brodwin, M., Carlstrom, J. E., Chang, C. L., et al. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/799/2/137 · Cited by 11
“Observing procedures, data processing, and detection algorithms for these clusters are described in detail in V10 and Staniszewski et al. (2009) and are summarized here.”
BackgroundMethodSelf-citation
Constraints on the duality relation from ACT cluster data
Gonçalves, R. S., Bernui, A., Holanda, R. F. L., & Alcaniz, J. S. (2014) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201424429 · Cited by 11
“Recently, however, a new window of information regarding galaxy cluster physics has opened with the release of cluster surveys (e.g., Staniszewski et al. 2009; Marriage et al. 2011; Williamson et al. 2011; Planck Collaboration VIII 2011; Reichardt et al. 2013) that make use of the SZ effect, which…”
Background
An optical observational cluster mass function at z ∼ 1 with the ORELSE survey
Hung, D., Lemaux, B. C., Gal, R. R., Tomczak, A., Lubin, L. M., Cucciati, O., Pelliccia, D., Shen, L., Fèvre, O. C. L., Zamorani, G., et al. (2021) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stab300 · Cited by 11
“Clusters may be found through searching for signatures of the thermal Sunyaev-Zel’dovich (SZ; Sunyaev & Zeldovich 1972) effect (e.g. Staniszewski et al. 2009; Menanteau et al. 2010; Bocquet et al. 2019; Bleem et al. 2020; Hilton et al. 2020; Huang et al. 2020), which is a distortion in the CMB…”
THE THERMAL SUNYAEV-ZEL'DOVICH TOMOGRAPHY
Shao, J., Zhang, P., Lin, W., & Jing, Y. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/730/2/127 · Cited by 11
The Sunyaev–Zeldovich effect in superclusters of galaxies using gasdynamical simulations: the case of Corona Borealis
Flores-Cacho, I., Rubiño-Martín, J. A., Luzzi, G., Rebolo, R., Petris, M. D., Yepes, G., Lamagna, L., Gregori, S. D., Battistelli, E. S., Coratella, R., et al. (2009) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2009.15578.x · Cited by 11
“Recently, it has also been proven that SZ surveys are effective means of finding new galaxy clusters in blind surveys (Staniszewski et al. 2009).”
Background
Timing the last major merger of galaxy clusters with large halo sparsity
Richardson, T. R. G., & Corasaniti, P.-S. (2022) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stac1241 · Cited by 13
Probing hot gas in galaxy groups through the Sunyaev-Zeldovich effect
Li, R., Mo, H. J., Fan, Z., van den Bosch, F. C., & Yang, X. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.18378.x · Cited by 11
“Many investigations (e.g. White & Majumdar 2004; Staniszewski et al. 2009; Plagge et al. 2010) have shown that the contamination by unresolved radio sources is lower than that of the IR sources and unlikely to be an important contribution to the SZE noise.”
Background
FSD: Frequency Space Differential measurement of CMB spectral distortions
Mukherjee, S., Silk, J. I., & Wandelt, B. D. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty888 · Cited by 11
“With the recent CMB anisotropy data, measurements of Sunyaev-Zel’dovich (SZ) clusters (Hasselfield et al. 2013; Bleem et al. 2015; Ade et al. 2016; Staniszewski et al. 2009) and bounds on the fluctuating y and µ have also been obtained (Khatri & Sunyaev 2015a,b).”
Method
Biases on cosmological parameter estimators from galaxy cluster number counts
Penna-Lima, M., Makler, M., & Souza, C. A. W. D. (2014) · Biblioteca Digital da Memória Científica do INPE (National Institute for Space Research) · Cited by 11
A blind detection of a large, complex, Sunyaev-Zel’dovich structure★
Shimwell, T. W., Barker, R. W., Biddulph, P., Bly, D., Boysen, R. C., Brown, A., Brown, M. D., Clementson, C., Crofts, M., Culverhouse, T. L., et al. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.20970.x · Cited by 10
“Now, however, SZ blind surveying isunderway, with ACT and SPT having produced initial results (Hincks et al. 2010, Menanteau et al. 2010, Staniszewski et al. 2009, Vanderlinde et al. 2010 and High et al. 2010).”
Background
Strong Lensing Model of SPT-CL J0356–5337, a Major Merger Candidate at Redshift 1.0359
Mahler, G., Sharon, K., Gladders, M. D., Bleem, L. E., Bayliss, M. B., Calzadilla, M. S., Floyd, B., Khullar, G., McDonald, M., González, J. D. R., et al. (2020) · The Astrophysical Journal · doi:10.3847/1538-4357/ab886b · Cited by 10
“…2017), which has only one multiply-imaged system; SPT-CLJ0546−5345 at z = 1.066 (Brodwin et al. 2010), which shows evidence of strong lensing features (Staniszewski et al. 2009); and SPT-CLJ0205−5829 (Stalder et al. 2013; Bleem et al. 2015) at z = 1.322 which has one arc with no published…”
BackgroundInfluentialSelf-citation
Discovery of a Powerful >1061 erg AGN Outburst in the Distant Galaxy Cluster SPT-CLJ0528-5300
Calzadilla, M. S., McDonald, M., Bayliss, M. B., Benson, B. A., Bleem, L. E., Brodwin, M., Edge, A. C., Floyd, B. T., Gupta, N., Hlavacek-Larrondo, J., et al. (2019) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/ab5b07 · Cited by 10
“The SZ effect is a particularly useful mechanism enabling the detection of distant galaxy clusters independent of redshift (e.g. Staniszewski et al. 2009; Reichardt et al. 2013; Hasselfield et al. 2013; Planck Collaboration et al. 2014).”
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Discovery of a Powerful >10^61 erg AGN Outburst in Distant Galaxy Cluster SPT-CLJ0528-5300
Calzadilla, M. S., McDonald, M., Bayliss, M. B., Benson, B. A., Bleem, L. E., Brodwin, M., Edge, A. C., Floyd, B. T., Gupta, N., Hlavacek-Larrondo, J., et al. (2019) · DSpace@MIT (Massachusetts Institute of Technology) · doi:10.48550/arxiv.1911.12828 · Cited by 10
“The SZ effect is a particularly useful mechanism enabling the detection of distant galaxy clusters independent of redshift (e.g. Staniszewski et al. 2009; Reichardt et al. 2013; Hasselfield et al. 2013; Planck Collaboration et al. 2014).”
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A joint analysis of AMI and CARMA observations of the recently discovered SZ galaxy cluster system AMI-CL J0300+2613
Shimwell, A. C. T. W., Carpenter, J. M., Feroz, F., Grainge, K., Hobson, M., Hurley-Walker, N., Lasenby, A. N., Olamaie, M., Perrott, Y. C., Pooley, G. G., et al. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt873 · Cited by 10
“…Array for Research in Millimeter-wave Astronomy (CARMA) and Planck have produced initial results (e.g. Hincks et al. 2010, Menanteau et al. 2010, Staniszewski et al. 2009, AMI Consortium: Shimwell et al. 2012, Muchovej et al. 2011, Vanderlinde et al. 2010, High et al. 2010 and Planck…”
Result
ChandraX-ray observations of the hyper-luminous infrared galaxy IRAS F15307+3252
Hlavacek-Larrondo, J., Gandhi, P., Hogan, M. T., Gendron-Marsolais, M.-L., Edge, A. C., Fabian, A. C., Russell, H. R., Iwasawa, K., & Mezcua, M. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw2468 · Cited by 10
“However, none of these have the sensitivity to detect ∼1014M groups at z ∼ 1, although the upcoming SPT-3G might be able to reach this limit (Benson et al. 2014).”
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Average dark matter halo sparsity relations as consistency check of mass estimates in galaxy cluster samples
Corasaniti, P.-S., & Rasera, Y. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz1579 · Cited by 10
“…Piffaretti et al. 2011; Pierre et al. 2016), the imprint of the Sunyaev-Zeldovich (SZ) effect on the cosmic microwave background radiation (see e.g. Staniszewski et al. 2009; Menanteau et al. 2013; Planck Collaboration: Ade et al. 2016b,c), the richness of member galaxies in the optical and IR…”
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Probing interacting dark sector models with future weak lensing-informed galaxy cluster abundance constraints from SPT-3G and CMB-S4
Mazoun, A., Bocquet, S., Garny, M., Mohr, J. J., Rubira, H., & Vogt, S. M. L. (2024) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.109.063536 · Cited by 9
Self-citation
Strong Lensing Model of SPT-CL J0356–5337, a Major Merger Candidate at Redshift 1.0359
Mahler, G., Sharon, K., Gladders, M. D., Bleem, L. E., Bayliss, M. B., Calzadilla, M. S., Floyd, B. T., Khullar, G., McDonald, M., Remolina González, J. D., et al. (2020) · DSpace@MIT (Massachusetts Institute of Technology) · Cited by 9
Self-citation
Low noise electronics in practical applications
Spieler, H. G. (2010) · Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment · doi:10.1016/j.nima.2010.04.100 · Cited by 9
Self-citation
X-RAY AND SUNYAEV-ZEL'DOVICH PROPERTIES OF THE WARM-HOT INTERGALACTIC MEDIUM
Ursino, E., Galeazzi, M., & Huffenberger, K. M. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/789/1/55 · Cited by 9
“The largest SZ surveys performed with the South Pole Telescope (Ruhl et al. 2004; Staniszewski et al. 2009; Van-derlinde et al. 2010), the Atacama Cosmology Telescope (Kosowsky 2003; Marriage et al. 2011; Hasselﬁeld et al. 2013), and the Planck satellite (Ade et al. 2013a) have mapped thousands of…”
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Signature of cool core in Sunyaev-Zeldovich clusters: a multiwavelength approach
Pipino, A., & Pierpaoli, E. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.16393.x · Cited by 9
“However, now that the first SZ detected clusters (Staniszewski et al. 2009) are available it is important to pay more attention to the intracluster medium (ICM) details.”
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A power spectrum approach to the search for axion-like particles from resolved galaxy clusters using CMB as a backlight
Mehta, H., & Mukherjee, S. (2024) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2024/09/037 · Cited by 8
“Late-time spectral distortions include those caused due to the inverse-Compton effects in galaxy clusters, also called the Sunyaev-Zeldovich (SZ) effects [29, 49].”
BFORE: The B-mode Foreground Experiment
Niemack, M. D., Ade, P. A. R., de Bernardis, F., Boulanger, F., Bryan, S., Devlin, M., Dunkley, J., Eales, S., Gomez, H., Groppi, C., et al. (2015) · Journal of Low Temperature Physics · doi:10.1007/s10909-015-1395-6 · Cited by 8
Self-citation
ThePlanckSZ Cluster Catalog: expected X-ray properties
Chamballu, A., Bartlett, J. G., & Melin, J.-B. (2012) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201015431 · Cited by 8
“…South Pole Telescope (SPT), Atacama Cosmology Telescope (ACT) and the Planck satellite are all discovering clusters solely through their SZ signal (Staniszewski et al. 2009; Vanderlinde et al. 2010; Menanteau et al. 2010; Planck Collaboration et al. 2011a) In particular, thePlanck satellite1 is…”
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Galaxy clusters as probes for cosmology and dark matter
Battistelli, E. S., Burigana, C., de Bernardis, P., Kirillov, A. A., Neto, G. B. L., Masi, S., Nørgaard-Nielsen, H. U., Ostermann, P., Roman, M., Rosati, P., et al. (2016) · International Journal of Modern Physics D · doi:10.1142/s0218271816300238 · Cited by 8
The MeerKAT Massive Distant Clusters Survey: detection of diffuse radio emission in galaxy clusters at z > 1
Phuravhathu, D. G., Hilton, M., Sikhosana, S. P., Perrott, Y. C., Mroczkowski, T. K., Mascolo, L. D., Klutse, D. Y., Knowles, K., van Marrewijk, J., Moodley, K., et al. (2025) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staf1315 · Cited by 7
THE STRUCTURE OF 2MASS GALAXY CLUSTERS
Blackburne, J. A., & Kochanek, C. S. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/744/1/76 · Cited by 7
“…Carlstrom et al. 2000; LaRoque 1 Department of Astronomy, The Ohio State University, 140 West 18th Avenue, Columbus, OH 43210, USA 2 Center for Cosmology and AstroParticle Physics, The Ohio State University, 191 West Woodruff Avenue, Columbus, OH 43210, USA et al. 2003; Staniszewski et al. 2009).”
Background
Galaxy clusters at z ∼ 1 imaged by ALMA with the Sunyaev–Zel’dovich effect
Kitayama, T., Ueda, S., Okabe, N., Akahori, T., Hilton, M., Hughes, J. P., Ichinohe, Y., Kohno, K., Komatsu, E., Lin, Y., et al. (2023) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/psac110 · Cited by 7
Analysis of the Amplitude of the Sunyaev–Zel’dovich Effect out to Redshift z = 0.8
López-Corredoira, M., Gutiérrez, C. M., & Génova-Santos, R. (2017) · The Astrophysical Journal · doi:10.3847/1538-4357/aa6d81 · Cited by 7
“…of previously known clusters (see, e.g., Carlstrom et al. 2002 and references therein), to the first discoveries of new objects in blind SZ surveys (Staniszewski et al. 2009) and, more recently, to the compilation of catalogs of many new SZ clusters, thanks to the improved angular resolution…”
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Constraining ultra-light axions with galaxy cluster number counts
Diehl, J., & Weller, J. (2021) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2021/08/004 · Cited by 7
Optically detected galaxy cluster candidates in the AKARI North Ecliptic Pole field based on photometric redshift from the Subaru Hyper Suprime-Cam
Huang, T.-C., Matsuhara, H., Goto, T., Santos, D. J. D., Ho, S. C.-C., Kim, S. J., Hashimoto, T., Ikeda, H., Oi, N., Malkan, M. A., et al. (2021) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stab2128 · Cited by 7
KISS: a spectrometric imager for millimetre cosmology
Fasano, A., Aguiar, M., Benoit, A. D., Bideaud, A., Bourrion, O., Calvo, M., Catalano, A., de Taoro, A. P., Garde, G., Gomez, A., et al. (2020) · EPJ Web of Conferences · doi:10.1051/epjconf/202022800010 · Cited by 7
SOUTHERN COSMOLOGY SURVEY. III. QSOs FROM COMBINED GALEX AND OPTICAL PHOTOMETRY
Jiménez, R., Spergel, D. N., Niemack, M. D., Menanteau, F., Hughes, J. P., Verde, L., & Kosowsky, A. B. (2009) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/181/2/439 · Cited by 5
Partial CMB maps: bias removal and optimal binning of the angular power spectrum
Ansari, R., & Magneville, C. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.16561.x · Cited by 5
NIKA2 Cosmological Legacy Survey
Cherouvrier, D., Macias-Perez, J. F., Désert, F. –., Adam, R., Ade, P. A. R., Ajeddig, H., Amarantidis, S., André, P., Aussel, H., Barrena, R., et al. (2025) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202554450 · Cited by 4
Self-citation
Comparison of physical and observational galaxy cluster modellingPreprint
Javid, K., Perrott, Y. C., Hobson, M. P., Olamaie, M., Rumsey, C., & Saunders, R. D. E. (2018) · arXiv (Cornell University) · doi:10.17863/cam.38865 · Cited by 4
SLICE: SPT-CL J0546-5345—A Prominent Strong-lensing Cluster at z = 1.07
Allingham, J. F. V., Zitrin, A., Golubchik, M., Furtak, L. J., Bayliss, M. B., Cerny, C., Diego, J. M., Edge, A. C., Gassis, R., Gladders, M. D., et al. (2025) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/adfa85 · Cited by 3
An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: an unbiased study of SMG environments measured with narrow-band imaging
Cornish, T., Wardlow, J. L., Wade, H., Sobral, D., Brandt, W. N., Cox, P., Dannerbauer, H., Decarli, R., Gullberg, B., Knudsen, K. K., et al. (2024) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stae1868 · Cited by 3
HST Grism Observations of a z ∼ 1.8 Cluster Candidate from the Clusters Occupied by Bent Radio AGN (COBRA) Survey
Watson, C. B., Blanton, E. L., Golden-Marx, E., Ashby, M. L. N., Randall, S. W., Wing, J., & Douglass, E. M. (2025) · The Astrophysical Journal · doi:10.3847/1538-4357/adc410 · Cited by 3
The XMM-BCS galaxy cluster survey: I. The X-ray selected cluster catalog from the initial 6 deg$^2$
Šuhada, R., Song, J., Böhringer, H., Mohr, J. J., Chon, G., Finoguenov, A., Fassbender, R., Desai, S., Armstrong, R., Zenteno, A., et al. (2011) · OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information) · doi:10.48550/arxiv.1111.0141 · Cited by 3
“Both have already provided their first SZE-selected cluster samples (Williamson et al. 2011; Vanderlinde et al. 2010; Marriage et al. 2010; Staniszewski et al. 2009) as well as observations of already known clusters (Plagge et al. 2010; Hincks et al. 2010).”
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COOL-LAMPS. VI. Lens Model and New Constraints on the Properties of COOL J1241+2219, a Bright z = 5 Lyman Break Galaxy and its z = 1 Cluster Lens
Klein, M., Sharon, K., Napier, K., Gladders, M. D., Khullar, G., Bayliss, M. B., Dahle, H., Owens, M. R., Stark, A. A., Brownsberger, S. R., et al. (2024) · The Astrophysical Journal · doi:10.3847/1538-4357/ad22de · Cited by 3
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SpectrAx: spectral search of axion-like particles using multi-band observations of galaxy clusters from SKA, SO, CMB-S4 and eROSITA
Mehta, H., & Mukherjee, S. (2025) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2025/02/050 · Cited by 3
“In addition to X-rays, information on the electron densities and temperature profiles can be obtained using the SZ-effect in clusters [15, 76, 77].”
Constraints on Nonthermal Pressure at Galaxy Cluster Outskirts from a Joint SPT and XMM-Newton Analysis
Sarkar, A., McDonald, M., Bleem, L. E., Bautz, M. W., Benson, B. A., Chakraborty, P., Grant, C. E., Jones, C. J., Kéruzoré, F., Miller, E. D., et al. (2025) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/adc676 · Cited by 3
Self-citation
The cosmic microwave background: from discovery to precision cosmology
Partridge, R. B. (2019) · Oxford University Press eBooks · doi:10.1093/oxfordhb/9780198817666.013.8 · Cited by 3
LENSING NOISE IN MILLIMETER-WAVE GALAXY CLUSTER SURVEYS
Hezaveh, Y., Vanderlinde, K., Holder, G. P., & de Haan, T. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/772/2/121 · Cited by 3
“Using data from the South Pole Telescope (SPT) (Carlstrom et al. 2011), the first discovery of galaxy clusters via the SZ effect was reported in Staniszewski et al. (2009), followed by the first cosmological constraints from a catalog of SZ-detected clusters in Vanderlinde et al. (2010).”
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Alternative cosmological theories
Kragh, H. (2019) · Oxford University Press eBooks · doi:10.1093/oxfordhb/9780198817666.013.4 · Cited by 3
Philosophical aspects of cosmology
Smeenk, C. (2019) · Oxford University Press eBooks · doi:10.1093/oxfordhb/9780198817666.013.13 · Cited by 4
Simulations and Observations of the Microwave UniversePreprint
Peel, M. (2010) · arXiv (Cornell University) · doi:10.48550/arxiv.1006.2760 · Cited by 3
An optimal and model-independent measurement of the intracluster pressure profile – I. Methodology and first applications
Aslanbeigi, S., Lavaux, G., Hajian, A., & Afshordi, N. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt1416 · Cited by 2
“Within the last few years, cluster surveys exploiting the SZ effect have started delivering cluster samples (e.g., Staniszewski et al. 2009; Marriage et al. 2011; Williamson et al. 2011; Planck Collaboration VIII 2011a) as well as constraints on cosmological parameters (Vanderlinde et al. 2010;…”
Background
Cosmic Microwave Background Carries Imprint of Moving Galaxies
Holder, G. P. (2012) · Physics · doi:10.1103/physics.5.81 · Cited by 2
Self-citation
Relativistic astrophysics and cosmology
Longair, M. S. (2019) · Oxford University Press eBooks · doi:10.1093/oxfordhb/9780198817666.013.7 · Cited by 2
The Atacama Cosmology Telescope: Mitigating the impact of extragalactic foregrounds for the DR6 CMB lensing analysisPreprint
MacCrann, 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. (2023) · arXiv (Cornell University) · doi:10.48550/arxiv.2304.05196 · Cited by 2
Self-citation
Inference of the morphology and dynamical state of nearby Planck-SZ galaxy clusters with Zernike polynomials
Capalbo, V., Petris, M. D., Ferragamo, A., Cui, W., Ruppin, F., & Yepes, G. (2025) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202452649 · Cited by 1
An X-ray-emitting protocluster at z ≈ 5.7 reveals rapid structure growth
Bogdan, A., Schellenberger, G., Li, Q., & Conselice, C. J. (2026) · Nature · doi:10.1038/s41586-025-09973-1 · Cited by 1
“However, detecting protoclusters is demanding: their member galaxies are loosely bound and the emerging hot intracluster medium (ICM) may only be in the initial stages of virialization 2–4 .”
Measurement of the Full Shape of the Thermal Sunyaev–Zel’dovich Power Spectrum from the South Pole Telescope and Herschel–SPIRE Observations
Raghunathan, S., Ade, P. A. R., Anbajagane, D., Anderson, A. J., B.Ansarinejad, Archipley, M., Austermann, J. E., Balkenhol, L., Barron, D. R., Barry, P. S., et al. (2026) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/ae5c07 · Cited by 1
Self-citation
Measurement of the cosmological distance scale using X-ray and Sunyaev–Zel'dovich effect observations of galaxy clusters
Bonamente, M., Carlstrom, J. E., Leitch, E. M., Joy, M. K., Marrone, D. P., Mantz, A. B., Muchovej, S. J., Plagge, T. J., & Reese, E. D. (2012) · Proceedings of the International Astronomical Union · doi:10.1017/s1743921312021680 · Cited by 1
Self-citation
The Cosmic Microwave Background: a window on the early universe
de Bernardis, P. (2013) · Nuclear Physics B - Proceedings Supplements · doi:10.1016/j.nuclphysbps.2013.09.009 · Cited by 1
Recent topics in front-end electronics—Systems considerations in high energy physics and other fields
Spieler, H. G. (2010) · Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment · doi:10.1016/j.nima.2010.02.151 · Cited by 1
Self-citation
Steady-State theory and the cosmological controversy
Kragh, H. (2019) · Oxford University Press eBooks · doi:10.1093/oxfordhb/9780198817666.013.5 · Cited by 1
Observational and astrophysical cosmology: 1940–1980
Longair, M. S. (2019) · Oxford University Press eBooks · doi:10.1093/oxfordhb/9780198817666.013.6 · Cited by 1
Thermal Sunyaev–Zeldovich measurements and cosmic infrared background leakage mitigation combining upcoming ground-based telescopes
Charmetant, M., & Erler, J. (2023) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202245834 · Cited by 1
Selecting Clusters and Protoclusters via Stellar Mass Density. I. Method and Tests on Mock HSC-SSP Catalogs
Vicentin, M. C., Araya-Araya, P., Junior, L. S., & Strauss, M. A. (2025) · The Astrophysical Journal · doi:10.3847/1538-4357/adff86 · Cited by 1
Inflation, dark matter, and dark energy
Longair, M. S., & Smeenk, C. (2019) · Oxford University Press eBooks · doi:10.1093/oxfordhb/9780198817666.013.11 · Cited by 1
Observations and the universe
Smith, R. W. (2019) · Oxford University Press eBooks · doi:10.1093/oxfordhb/9780198817666.013.2 · Cited by 2
The Atacama Cosmology Telescope: Development and preliminary results of point source observations
Fisher, R. P. (2009) · ProQuest Demo Repository · Cited by 1
The XMM-BCS galaxy cluster survey
Šuhada, R., Song, J., Böhringer, H., Mohr, J. J., Chon, G., Finoguenov, A., Fassbender, R., Desai, S., Armstrong, R., Zenteno, A., et al. (2011) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201117214
“Both have already provided their first SZE-selected cluster samples (Williamson et al. 2011; Vanderlinde et al. 2010; Marriage et al. 2010; Staniszewski et al. 2009) as well as observations of already known clusters (Plagge et al. 2010; Hincks et al. 2010).”
BackgroundSelf-citation
Cosmology from Antarctica
Stark, A. A. (2011) · Smithsonian Institution Scholarly Press eBooks · doi:10.5479/si.9781935623069.197
Self-citation
Slicing cluster mass functions with a Bayesian razor
Sealfon, C. D. (2010) · Astronomische Nachrichten · doi:10.1002/asna.201011409
“Current and future experiments will observe thousands of galaxy clusters (Geisbüsch and Hobson 2007; Menanteau et al. 2010; Rozo et al. 2010; Sehgal et al. 2007; Staniszewski et al. 2009), producing galaxy cluster catalogs which can be used to constrain the shape of the cluster mass function.”
Background
Optical followup of galaxy clusters detected by the South Pole Telescope
Desai, S., Armstrong, R., Ashby, M. L. N., Bayliss, B., Bazin, G., Benson, B. A., Bertin, E., Bleem, L. E., Brodwin, M., Clochiatti, A., et al. (2012) · Journal of Physics Conference Series · doi:10.1088/1742-6596/375/1/032011
Self-citation
The SCAR Astronomy & Astrophysics from Antarctica Scientific Research Programme
Storey, J. W. V., Abe, L., Andersen, M. I., Anderson, P. S., Burton, M., Cui, X., Ichikawa, T., KARLE, A., Lloyd, J. P., Masi, S., et al. (2012) · Proceedings of the International Astronomical Union · doi:10.1017/s1743921312017000
“…background anisotropies: determination of the flat Universe (BOOMERanG; de Bernardis et al. 2000), first detection of CMBR polarization (DASI; Kovac et al. 2002), high angular scale anisotropy (ACBAR; Kuo et al. 2004), SunyaevZeldovich effect in galaxy clusters (SPT; Staniszewski et al. 2009).”
Background
TES Development for a Frequency Selective Bolometer Camera
Datesman, A., Downes, T. P., Perera, T. A., Wang, G., Yefremenko, V. G., Pearson, J. E., Novosad, V., Divan, R. N. S., Chang, C. L., Logan, D. W., et al. (2009) · IEEE Transactions on Applied Superconductivity · doi:10.1109/tasc.2009.2017954
Self-citation
Up to the Present, and Beyond
Evans, R. (2014) · Astronomers' universe · doi:10.1007/978-3-319-09928-6_7
Lsst Observing Strategy
Ivezić, Ž. (2016) · Zenodo (CERN European Organization for Nuclear Research) · doi:10.5281/zenodo.44697

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: 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.
Dobbs, M. A.
Halverson, N. W.
Holzapfel, W. L.
Keisler, R.
Lee, A. T.
Leitch, E. M.
Meyer, S. S.
Ngeow, C.-C.
Padin, S.
Reichardt, C. L.
Ruhl, J. E.
Shirokoff, E.
Stalder, B.
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
DOI: 10.1088/0004-637x/701/1/32
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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GALAXY CLUSTERS DISCOVERED WITH A SUNYAEV-ZEL'DOVICH EFFECT SURVEY

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