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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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“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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Citations
Cites
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…”
BackgroundThe 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…”
BackgroundA 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.”
BackgroundCosmology 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-citationWang, 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).”
MethodBirkinshaw, 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.”
MethodThe 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-citationEffects 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
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
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Items 101–200 of 319
Templates for the Sunyaev-Zel'dovich Angular Power Spectrum
Trac, H., Bode, P. W., & Ostriker, J. P. (2018) · KiltHub Repository · doi:10.1184/r1/6509291.v1 · Cited by 63
Accurate photometric redshift probability density estimation – method comparison and application
Rau, M. M., Seitz, S., Brimioulle, F., Frank, E., Friedrich, O., Gruen, D., & Hoyle, B. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv1567 · Cited by 58
“Photometric redshifts are used throughout astrophysics and cosmology, for example in large scale structure analyses (Staniszewski et al. 2009; de Simoni et al. 2013), in galaxy cluster weak lensing analyses (Gruen et al. 2013), and in galaxy-galaxy lensing analyses (Brimioulle 2013).”
MethodHand, N., Appel, J. W., Battaglia, N., Bond, J. R., Das, S., Devlin, M. J., Dunkley, J., Dünner, R., Essinger-Hileman, T., Fowler, J. W., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/736/1/39 · Cited by 57
“The SPT collaboration reported its first SZ detections in Staniszewski et al. (2009) and has since identified 22 cluster candidates in Vanderlinde et al. (2010).”
SPT-CL J2040–4451: AN SZ-SELECTED GALAXY CLUSTER ATz= 1.478 WITH SIGNIFICANT ONGOING STAR FORMATION
Bayliss, M. B., Ashby, M. L. N., Ruel, J., Brodwin, M., Aird, K. A., Bautz, M. W., Benson, B. A., Bleem, L. E., Bocquet, S., Carlstrom, J. E., et al. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/794/1/12 · Cited by 56
“Several SZ galaxy cluster surveys are underway; The Planck satellite (Planck Collaboration et al. 2013), the Atacama Cosmology Telescope (ACT; Marriage et al. 2011; Hasselfield et al. 2013), and the South Pole Telescope (Staniszewski et al. 2009; Vanderlinde et al. 2010; 30 Space Telescope Science Institute, 3700 San…”
BackgroundMethodInfluentialSelf-citationMenanteau, F., Sifón, C., Barrientos, L. F., Battaglia, N., Bond, J. R., Crichton, D., Das, S., Devlin, M. J., Dicker, S., Dünner, R., et al. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/765/1/67 · Cited by 56
“…Cosmology Telescope (ACT) and South Pole Telescope (SPT) are providing samples of galaxy clusters over hundreds of square degrees at all redshifts (Staniszewski et al. 2009; Hincks et al. 2010; Menanteau et al. 2010a; Marriage et al. 2011a; Vanderlinde et al. 2010; Williamson et al. 2011;…”
BackgroundThe Road to Precision Cosmology
Turner, M. S. (2022) · Annual Review of Nuclear and Particle Science · doi:10.1146/annurev-nucl-111119-041046 · Cited by 58
Multi-frequency imaging of the galaxy cluster Abell 2163 using the Sunyaev-Zel'dovich effect
Nord, M., Basu, K., Pacaud, F., Ade, P. A. R., Bender, A. N., Benson, B. A., Bertoldi, F., Cho, H.-M., Chon, G., Clarke, J., et al. (2009) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200911746 · Cited by 54
“A number of blind SZE imaging surveys are in progress (e.g. Ruhl et al. 2004; Kosowsky 2006) with the aim of tracing the large-scale structure of the Universe through the detection of galaxy clusters, and the first blind SZE detections have recently been reported (Staniszewski et al. 2009).”
BackgroundSelf-citationBattaglia, N., Leauthaud, A., Miyatake, H., Hasselfield, M., Gralla, M. B., Allison, R., Bond, J. R., Calabrese, E., Crichton, D., Devlin, M. J., et al. (2016) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2016/08/013 · Cited by 53
“…Telescope (ACT), the South Pole Telescope (SPT), and the Planck satellite are producing large catalogs of clusters detected using the tSZ (e.g., Staniszewski et al. 2009; Marriage et al. 2011; Reichardt et al. 2013; Hasselfield et al. 2013; Planck Collaboration et al. 2014a; Bleem et al. 2015;…”
BackgroundDetecting clusters of galaxies and active galactic nuclei in an eROSITA all-sky survey digital twin
Seppi, R., Comparat, J., Bülbül, E., Nandra, K., Merloni, A., Clerc, N., Liu, T., Ghirardini, V., Liu, A., Salvato, M., et al. (2022) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202243824 · Cited by 53
The GEEC2 spectroscopic survey of Galaxy groups at 0.8 < z < 1
Balogh, M. L., McGee, S., Mok, A., Wilman, D. J., Finoguenov, A., Bower, R. G., Mulchaey, J. S., Parker, L. C., & Tanaka, M. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu1332 · Cited by 50
“…have also been compiled out to much higher redshift, based on detection in X–ray (e.g. Rosati et al. 2002; Piffaretti et al. 2011), SZ decrement (Staniszewski et al. 2009; Vanderlinde et al. 2010; Williamson et al. 2011; Planck Collaboration et al. 2011), photometric overdensity (e.g. Gladders…”
BackgroundCharacterizing hydrostatic mass bias with mock-X
Barnes, D. J., Vogelsberger, M., Pearce, F. A., Pop, A.-R., Kannan, R., Cao, K., Kay, S. T., & Hernquist, L. (2021) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stab1276 · Cited by 50
Mather, J., Hinshaw, G. F., & Page, L. A. (2013) · Springer eBooks · doi:10.1007/978-94-007-5609-0_13 · Cited by 60
SPT-GMOS: A GEMINI/GMOS-SOUTH SPECTROSCOPIC SURVEY OF GALAXY CLUSTERS IN THE SPT-SZ SURVEY
Bayliss, M. B., Ruel, J., Stubbs, C. W., Allen, S. W., Applegate, D., Ashby, M. L. N., Bautz, M. W., Benson, B. A., Bleem, L. E., Bocquet, S., et al. (2016) · The Astrophysical Journal Supplement Series · doi:10.3847/0067-0049/227/1/3 · Cited by 49
“…et al. 2014), the Atacama Cosmology Telescope (ACT; Marriage et al. 2011; Hasselfield et al. 2013), and the South Pole Telescope (SPT) (Staniszewski et al. 2009; Vanderlinde et al. 2010; Williamson et al. 2011; Reichardt et al. 2013; Bleem et al. 2015) have all published SZ-based…”
BackgroundMethodSelf-citationIdentification of High-redshift Galaxy Overdensities in GOODS-N and GOODS-S
Helton, J. M., Sun, F., Woodrum, C., Hainline, K., Willmer, C. N. A., Rieke, M. J., Rieke, G. H., Alberts, S. L., Eisenstein, D. J., Tacchella, S., et al. (2024) · The Astrophysical Journal · doi:10.3847/1538-4357/ad6867 · Cited by 72
The galaxy clusterYSZ−LXandYSZ−Mrelations from the WMAP 5-yr data
Melin, J.-B., Bartlett, J. G., Delabrouille, J., Arnaud, M., Piffaretti, R., & Pratt, G. W. (2010) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201013999 · Cited by 48
“…from space with the Planck mission (Valenziano et al. 2007; Lamarre et al. 2003) and from the ground with several dedicated telescopes, such as the South Pole Telescope (Carlstrom et al. 2009) leading to the first discoveries of clusters solely through their SZ signal (Staniszewski et al. 2009).”
BackgroundOrigin of Low-Lying Enhanced E1 Strength in Rare-Earth Nuclei
Spieker, M., Pascu, S. I., Zilges, A., & IACHELLO, F. (2015) · Physical Review Letters · doi:10.1103/physrevlett.114.192504 · Cited by 48
The evolution in the stellar mass of brightest cluster galaxies over the past 10 billion years
Bellstedt, S., Lidman, C. E., Muzzin, A., Franx, M., Guatelli, S., Hill, A. R., Hoekstra, H., Kurinsky, N., Labbé, I., Marchesini, D., et al. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw1184 · Cited by 48
“Clusters in the MACS sample (Ebeling et al. 2010) are X-ray selected, whereas the clusters in the SPT/ACT samples (Staniszewski et al. 2009; Marriage et al. 2011; Williamson et al. 2011; Hasselfield et al. 2013) have been discovered through the Sunyaev–Zel’Dovich (SZ) effect.”
BackgroundPrediction of galaxy halo masses in SDSS DR7 via a machine learning approach
Calderon, V. F., & Berlind, A. A. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz2775 · Cited by 48
Constraining f(R) gravity with Planck data on galaxy cluster profiles
Martino, I. D., Laurentis, M. D., Atrio-Barandela, F., & Capozzıello, S. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu903 · Cited by 47
Non-parametric modeling of the intra-cluster gas using APEX-SZ bolometer imaging data
Basu, K., Zhang, Y.-Y., Sommer, M. W., Bender, A. N., Bertoldi, F., Dobbs, M., Eckmiller, H., Halverson, N. W., Holzapfel, W. L., Horellou, C., et al. (2010) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200913334 · Cited by 47
Self-citationThe Sunyaev–Zel'dovich effect at 5″: RX J1347.5−1145 imaged by ALMA
Kitayama, T., Ueda, S., Takakuwa, S., Tsutsumi, T., Komatsu, E., Akahori, T., Iono, D., Izumi, T., Kawabe, R., Kohno, K., et al. (2016) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/psw082 · Cited by 47
“The advent of large-area surveys by the South Pole Telescope (SPT) (e.g., Staniszewski et al. 2009; Vanderlinde et al. 2010; Williamson et al. 2011; Reichardt et al. 2013), the Atacama Cosmology Telescope (ACT) (e.g., Hincks et al. 2010; Marriage et al. 2011; Hasselfield et al. 2013), and the…”
BackgroundMicrowave spectro-polarimetry of matter and radiation across space and time
Delabrouille, J., Abitbol, M. H., Aghanim, N., Ali-Haïmoud, Y., Alonso, D., Alvarez, M. A., Banday, A. J., Bartlett, J. G., Baselmans, J. J. A., Basu, K., et al. (2021) · Experimental Astronomy · doi:10.1007/s10686-021-09721-z · Cited by 60
Mapping the allowed parameter space for decaying dark matter models
Peter, A. H. G. (2010) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.81.083511 · Cited by 47
Cosmological and astrophysical implications of the Sunyaev-Zel'dovich effect
Kitayama, T. (2014) · Progress of Theoretical and Experimental Physics · doi:10.1093/ptep/ptu055 · Cited by 45
Story, K. T., Aird, K. A., Andersson, K., Armstrong, R., Bazin, G., Benson, B. A., Bleem, L. E., Bonamente, M., Brodwin, M., Carlstrom, J. E., et al. (2011) · The Astrophysical Journal Letters · doi:10.1088/2041-8205/735/2/l36 · Cited by 45
Self-citationMenanteau, F., Hughes, J. P., Barrientos, L. F., Deshpande, A. J., Hilton, M., Infante, L., Jiménez, R., Kosowsky, A. B., Moodley, K., Spergel, D. N., et al. (2010) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/191/2/340 · Cited by 44
X-RAY GROUPS OF GALAXIES IN THE AEGIS DEEP AND WIDE FIELDS
Erfanianfar, G., Finoguenov, A., Tanaka, M., Lerchster, M., Nandra, K., Laird, E. S., Connelly, J. L., Bielby, R. M., Mirkazemi, M., Faber, S. M., et al. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/765/2/117 · Cited by 41
“…Astronomy Data Centre, Herzberg Institute of Astrophysics, 5071 West Saanich Road, Victoria, British Columbia, V9E 2E7, Canada et al. 2004; Staniszewski et al. 2009; X-ray emission from hot intracluster gas (e.g. Boehringer et al. 2000; Hasinger et al. 2001; Vikhlinin et al. 2009;…”
BackgroundSchrabback, T., Bocquet, S., Sommer, M. W., Zohren, H., van den Busch, J. L., Hernández-Martín, B., Hoekstra, H., Raihan, S. F., Schirmer, M., Applegate, D., et al. (2021) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stab1386 · Cited by 41
Self-citationMiyatake, H., Battaglia, N., Hilton, M., Medezinski, E., Nishizawa, A. J., More, S., Aiola, S., Bahcall, N. A., Bond, J. R., Calabrese, E., et al. (2019) · Institutional Repositories DataBase (IRDB) · Cited by 41
Self-citationCosmological and Astrophysical Implications of the Sunyaev-Zel’dovich EffectPreprint
Kitayama, T. (2016) · Cited by 41
Wilson, M. J., Sherwin, B. D., Hill, J. C., Addison, G. E., Battaglia, N., Bond, J. R., Das, S., Devlin, M. J., Dunkley, J., Dünner, R., et al. (2012) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.86.122005 · Cited by 40
Morphological estimators on Sunyaev–Zel'dovich maps of MUSIC clusters of galaxies
Cialone, G., Petris, M. D., Sembolini, F., Yepes, G., Baldi, A., & Rasia, E. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty621 · Cited by 39
“…available thanks to different surveys carried out either by ground-based facilities , as in the case of the South Pole Telescope (Chang et al. 2009; Staniszewski et al. 2009; Bleem et al. 2015) or the Atacama Cosmology Telescope (Swetz et al. 2011; Hasselfield et al. 2013), or space-based as in…”
BackgroundA future test of gravitation using galaxy cluster velocities
Kosowsky, A. B., & Bhattacharya, S. (2009) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.80.062003 · Cited by 39
Sajina, A., Partridge, B., Evans, T., Stefl, S., Vechik, N., Myers, S., Dicker, S., & Korngut, P. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/732/1/45 · Cited by 38
“The 10 m South Pole Telescope (SPT; Carlstrom et al. 2009) is conducting a survey for the SZ effect produced by clusters of galaxies (Staniszewski et al. 2009; Vanderlinde et al. 2010; Lueker et al. 2010), and is also measuring small fluctuations in the microwave background.”
BackgroundMukherjee, S., Khatri, R., & Wandelt, B. D. (2018) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2018/04/045 · Cited by 38
Initial conditions for idealized clusters mergers, simulating ‘El Gordo’
Donnert, J. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt2291 · Cited by 38
Galaxy populations in the 26 most massive galaxy clusters in the South Pole Telescope SPT-SZ survey
Zenteno, A., Mohr, J., Desai, S., Stalder, B., Saro, A., Dietrich, J., Bayliss, M., Bocquet, S., Chiu, I., Gonzalez, A., et al. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw1649 · Cited by 25
“For details on the SPT data processing there are several papers that describe the method in detail (Staniszewski et al. 2009; Vanderlinde et al. 2010; Shirokoff et al. 2011).”
MethodSelf-citationClose-up view of a luminous star-forming galaxy at z = 2.95
Berta, S., Young, A. J., Cox, P., Neri, R., Jones, B., Baker, A. J., Omont, A., Dunne, L., Rosell, A. C., Marchetti, L., et al. (2020) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202039743 · Cited by 36
Multi-frequency imaging of the galaxy cluster Abell 2163 using the Sunyaev-Zel'dovich effect
Nord, M., Basu, K., Pacaud, F., Ade, P. A. R., Bender, A. N., Benson, B. A., Bertoldi, F., Cho, H.-M., Chon, G., Clarke, J., et al. (2009) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/200911746/pdf · Cited by 36
Self-citationDetection and removal of artifacts in astronomical images
Desai, S., Mohr, J., Bertin, E., Kummel, M., & Wetzstein, M. (2016) · Astronomy and Computing · doi:10.1016/j.ascom.2016.04.002 · Cited by 31
“CosmoDM and its precursor have been applied to a variety of data including those from the Mosaic-2 and DECam imagers on the Blanco telescope as well as data from Pan-Starrs, CFHT MegaCam, SOAR, and WFI to support the optical confirmation and photometric redshift measurement of galaxy cluster candidates detected throug…”
MethodSelf-citationAghanim, N., Douspis, M., Hurier, G., Crichton, D., Diego, J. M., Hasselfield, M., Macias-Perez, J. F., Marriage, T. A., Pointecouteau, É., Remazeilles, M., et al. (2019) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201935271 · Cited by 35
“As described in Remazeilles et al. (2013), such a combination can be performed using component separation techniques which aggregate the 5 It is based on the catalogs from Planck, ACT, SPT, CARMA, AMI.”
InfluentialFirst lensing measurements of SZ-detected clusters
McInnes, R. N., Menanteau, F., Heavens, A., Hughes, J. P., Jiménez, R., Massey, R. J., Simon, P., & Taylor, A. N. (2009) · Monthly Notices of the Royal Astronomical Society Letters · doi:10.1111/j.1745-3933.2009.00730.x · Cited by 35
“We focused on four clusters found in SZ (Staniszewski et al. 2009) and also 38 optical clusters selected from 8 deg2 (Menanteau et al. 2009).”
MethodProbing the existence of a rich galaxy overdensity at z = 5.2
Calvi, R., Dannerbauer, H., Haro, P. A., Rodríguez-Espinosa, J. M., Muñoz-Tuñón, C., Pérez‐González, P. G., & Geier, S. (2021) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa4037 · Cited by 34
“…shear selection (e.g., Wittman et al. 2006; Gavazzi & Soucail 2007; Shan et al. 2012; Jeffrey et al. 2018), the Sunyaev-Zeldovich signatures (e.g., Staniszewski et al. 2009; Mantz et al. 2014), emission lines such as Lyα and Hα through narrow-band imaging and subsequent spectroscopy (e.g., Kurk…”
BackgroundSUBMILLIMETER GALAXY NUMBER COUNTS AND MAGNIFICATION BY GALAXY CLUSTERS
Lima, M., Jain, B., Devlin, M., & Aguirre, J. (2010) · The Astrophysical Journal Letters · doi:10.1088/2041-8205/717/1/l31 · Cited by 34
“…have also aimed at detecting galaxy clusters via the Sunyaev Zel’dovich (SZ) effect (Hincks et al. 2008; Carlstrom et al. 2009); the first results, including CMB power spectra and cluster catalogs, have been released recently (Fowler et al. 2010; Staniszewski et al. 2009; Vanderlinde et al. 2010).”
MethodKinetic inductance detectors for the OLIMPO experiment: design and pre-flight characterization
Paiella, A., Coppolecchia, A., Lamagna, L., Ade, P. A. R., Battistelli, E. S., Castellano, M. G., Colantoni, I., Columbro, F., D'Alessandro, G., de Bernardis, P., et al. (2019) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2019/01/039 · Cited by 33
Self-citationZenteno, A., Song, J., Desai, S., Armstrong, R., Mohr, J. J., Ngeow, C., Barkhouse, W., Allam, S., Andersson, K., Bazin, G., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/734/1/3 · Cited by 33
“In the millimeter regime, the use of the SunyaevZel’dovich Effect (SZE, Sunyaev & Zel’dovich 1972) as a selection method for cluster of galaxies has recently produced the first results (Staniszewski et al. 2009; Vanderlinde et al. 2010).”
BackgroundMethodSelf-citationLiu, J., Hennig, C., Desai, S., Hoyle, B., Koppenhoefer, J., Mohr, J. J., Paech, K., Burgett, W. S., Chambers, K. C., Cole, S., et al. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv458 · Cited by 32
“Since the first SZEdiscovered galaxy clusters were reported by the South Pole Telescope (SPT) collaboration (Staniszewski et al. 2009), large solid angle surveys have been completed, delivering many new galaxy clusters (Hasselfield et al. 2013; Reichardt et al. 2013; Planck Collaboration XXIX…”
BackgroundSelf-citationWu, H., Rozo, E., & Wechsler, R. H. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/713/2/1207 · Cited by 32
“…identified via X-ray (e.g., Ebeling et al. 1998, 2000, 2001; Vikhlinin et al. 1998; Böhringer et al. 2004) or Sunyaev–Zel’dovich (SZ) effects (e.g., Staniszewski et al. 2009; Hincks et al. 2009, see also Carlstrom et al. 2002); the mass concentrations can be identified using weak lensing shear…”
Establishing a new technique for discovering large-scale structure using 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., Wu, P.-F., et al. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz3164 · Cited by 32
A pan-chromatic view of the galaxy cluster XMMU J1230.3+1339 atz= 0.975
Fassbender, R., Böhringer, H., Santos, J., Pratt, G. W., Šuhada, R., Kohnert, J., Lerchster, M., Rovilos, E., Pierini, D., Chon, G., et al. (2010) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201015204 · Cited by 32
“Significant progress is yet to be made to establish robust mass-observable relations atz ∼ 1 and beyond and to compare vices and virtues of mass proxies derived from optical/IR, X-ray, WL, and SZE observations at these redshifts.”
BackgroundSelf-citationHilbert, S., & White, S. D. M. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.16310.x · Cited by 32
“…the weak-lensing signal (Tyson et al. 1990; Cypriano et al. 2004; Hoekstra 2007; Johnston et al. 2007b; Reyes et al. 2008), and the SunyaevZel’dovich signal induced by the cluster (White et al. 2002; Schulz and White 2003; Bonaldi et al. 2007; Staniszewski et al. 2009). c© 0000 RAS ar X iv :0 90 7.”
BackgroundSembolini, F., Petris, M. D., Yepes, G., Foschi, E., Lamagna, L., & Gottlöber, S. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu554 · Cited by 31
“…a viable tool for high-z object-finding, as proved from the success of blind cluster surveys from the current generation of millimeter telescopes (Staniszewski et al. 2009, Marriage et al. 2011, Planck Collaboration et al. 2011, Williamson et al. 2011, Planck Collaboration et al. 2013a,…”
MethodStern, C., Dietrich, J. P., Bocquet, S., Applegate, D., Mohr, J. J., Bridle, S., Kind, M. C., Gruen, D., Jarvis, M., Kacprzak, T., et al. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz234 · Cited by 31
Self-citationVavagiakis, E. M., Gallardo, P. A., Calafut, V., Amodeo, S., Aiola, S., Austermann, J. E., Battaglia, N., Battistelli, E. S., Beall, J. A., Bean, R., et al. (2021) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.104.043503 · Cited by 31
Self-citationSong, J., Mohr, J. J., Barkhouse, W., Warren, M. S., Dolag, K., & Rude, C. M. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/747/1/58 · Cited by 31
Self-citationNon-parametric modeling of the intra-cluster gas using APEX-SZ bolometer imaging data
Basu, K., Zhang, Y.-Y., Sommer, M. W., Bender, A. N., Bertoldi, F., Dobbs, M., Eckmiller, H. J., Halverson, N. W., Holzapfel, W. L., Horellou, C., et al. (2010) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/200913334/pdf · Cited by 31
Self-citationOptical validation and characterization of Planck PSZ1 sources at the Canary Islands observatories
Barrena, R., Streblyanska, A., Ferragamo, A., Rubiño-Martín, J. A., Aguado-Barahona, A., Tramonte, D., Génova-Santos, R. T., Hempel, A., Lietzen, H., Aghanim, N., et al. (2018) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201732315 · Cited by 30
Probing Cosmology with Dark Matter Halo Sparsity Using X-Ray Cluster Mass Measurements
Corasaniti, P.-S., Ettori, S., Rasera, Y., Sereno, M., Amodeo, S., Breton, M.-A., Ghirardini, V., & Eckert, D. (2018) · The Astrophysical Journal · doi:10.3847/1538-4357/aaccdf · Cited by 28
Solving the main cosmological puzzles with a generalized time varying vacuum energy
Basilakos, S. (2009) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200912575 · Cited by 28
“In particular, we have found that the Sunayev-Zeldovich cluster number-counts (as expected from the survey of the South Pole Telescope, Staniszewski et al. 2009, and the Atacama Cosmology Telescope, Hincks et al. 2009) indicate that we may be able to detect significant differences among the vacuum models in the redshi…”
MethodInfluentialA new probe of axion-like particles: CMB polarization distortions due to cluster magnetic fields
Mukherjee, S., Spergel, D. N., Khatri, R., & Wandelt, B. D. (2020) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2020/02/032 · Cited by 28
The Atacama Cosmology Telescope: A Catalog of >4000 Sunyaev–Zel’dovich Galaxy Clusters
Hilton, M., Sifón, C., Næss, S., Madhavacheril, M. S., Oguri, M., Rozo, E., Rykoff, E. S., Abbott, T. M. C., Adhikari, S., Aguena, M., et al. (2021) · Sussex Research Online (University of Sussex) · doi:10.17863/cam.66928 · Cited by 27
Self-citationExploring cosmic origins with CORE: Cluster science
Melin, J.-B., Bonaldi, A., Remazeilles, M., Hagstotz, S., Diego, J. M., Hernández-Monteagudo, C., Génova-Santos, R. T., Luzzi, G., Martins, C. J. A. P., Grandis, S., et al. (2018) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2018/04/019 · Cited by 27
Self-citationMass Estimation of Galaxy Clusters with Deep Learning. I. Sunyaev–Zel’dovich Effect
Gupta, N., & Reichardt, C. (2020) · Astrophysical Journal · doi:10.3847/1538-4357/aba694 · Cited by 17
“Since Staniszewski et al. (2009) presented the first SZ-discovered clusters, the South Pole Telescope (SPT; Carlstrom et al. 2011), the Atacama Cosmology Telescope (ACT; Fowler et al. 2007) and the Planck satellite (The Planck Collaboration 2006) have released catalogs of hundreds to thousands of…”
BackgroundSelf-citationTENTATIVE DETECTION OF QUASAR FEEDBACK FROM WMAP AND SDSS CROSS-CORRELATION
Chatterjee, S., Ho, S., Newman, J. A., & Kosowsky, A. B. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/720/1/299 · Cited by 27
“State-of-the-art SZ surveys like the Atacama Cosmology Telescope (ACT1) (Hincks et al. 2009) and the South Pole Telescope (SPT2) (Staniszewski et al. 2009) aim to detect large numbers of clusters in blind surveys via their SZ signatures.”
BackgroundWeak lensing mass modeling bias and the impact of miscentring
Sommer, M. W., Schrabback, T., Applegate, D., Hilbert, S., Ansarinejad, B., Floyd, B. T., & Grandis, S. (2021) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stab3052 · Cited by 26
Chiu, I.-N. T., Saro, A., Mohr, J. J., Desai, S., Bocquet, S., Capasso, R., Gangkofner, C., Gupta, N., & Liu, J. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw292 · Cited by 26
“…been undertaken in the X-ray (e.g. Böhringer et al. 2004; Pierre et al. 2004; Mantz et al. 2008; Vikhlinin et al. 2009a), at mm wavelengths (e.g. Staniszewski et al. 2009; Planck Collaboration et al. 2011; Hasselfield et al. 2013) employing the SunyaevZel’dovich Effect (SZE; Sunyaev &…”
MethodSelf-citationDetection and removal of artifacts in astronomical images
Desai, S., Mohr, J., Bertin, E., Kümmel, M., & Wetzstein, M. (2016) · Max Planck Digital Library · Cited by 25
Self-citationA MULTIWAVELENGTH STUDY OF BINARY QUASARS AND THEIR ENVIRONMENTS
Green, P. J., Myers, A. D., Barkhouse, W., Aldcroft, T. L., Trichas, M., Richards, G. T., Ruiz, Á., & Hopkins, P. F. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/743/1/81 · Cited by 24
“Burgeoning detections of galaxy clusters based on the SunyaevZeldovich effect (SZE) (Staniszewski et al. 2009; Vanderlinde et al. 2010) may help widen the overlap.”
BackgroundSpectroscopic Confirmation of Five Galaxy Clusters at z > 1.25 in the 2500 deg2 SPT-SZ Survey
Khullar, G., Bleem, L. E., Bayliss, M. B., Gladders, M. D., Benson, B. A., McDonald, M., Allen, S. W., Applegate, D., Ashby, M. L. N., Bocquet, S., et al. (2018) · The Astrophysical Journal · doi:10.3847/1538-4357/aaeed0 · Cited by 24
Self-citationMenanteau, F., Hughes, J., Jimenez, R., Hernandez-Monteagudo, C., Verde, L., Kosowsky, A., Moodley, K., Infante, L., & Roche, N. (2009) · Max Planck Digital Library · Cited by 24
THE DARK ENERGY SURVEY: PROSPECTS FOR RESOLVED STELLAR POPULATIONS
Rossetto, B. M., Santiago, B. X., Girardi, L., Camargo, J. I. B., Balbinot, E., da Costa, L. N., Yanny, B., Maia, M. A. G., Makler, M., Ogando, R. L. C., et al. (2011) · The Astronomical Journal · doi:10.1088/0004-6256/141/6/185 · Cited by 26
Self-citationGalaxy clusters and groups in the ALHAMBRA survey
Ascaso, B., Benítez, N., Fernández-Soto, A., Arnalte-Mur, P., López-Sanjuán, C., Molino, A., Schoenell, W., Jiménez-Teja, Y., Merson, A. I., Díaz-García, L. A., et al. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv1317 · Cited by 23
“…et al. 2014; Blanton et al. 2014) (4) searches using the Sunyaev-Zel’dovich (SZ) signature in cosmic microwave background maps (e.g. Bartlett 2004; Staniszewski et al. 2009); (5) searches using the WeakLensing (WL) effect (see Wittman et al. 2006 for a detailed explanation and references…”
MethodProbing cosmology with dark matter halo sparsity using X-ray cluster mass measurements
Corasaniti, P.-S., Ettori, S., Rasera, Y., Sereno, M., Amodeo, S., Breton, M.-A., Ghirardini, V., & Eckert, D. (2018) · MPG.PuRe (Max Planck Society) · Cited by 23
Shannon Limits for Low-Temperature Detector Readout
Irwin, K. D., Young, B., Cabrera, B., & Miller, A. (2009) · AIP conference proceedings · doi:10.1063/1.3292320 · Cited by 23
Non-Gaussianity of secondary anisotropies from ACTPol and Planck
Coulton, W. R., Aiola, S., Battaglia, N., Calabrese, E., Choi, S. K., Devlin, M. J., Gallardo, P. A., Hill, J. C., Hincks, A. D., Hubmayr, J., et al. (2018) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2018/09/022 · Cited by 23
“The thermal SZ effect in galaxy clusters has been studied through cluster number counts (e.g. Staniszewski et al. 2009; Hasselfield et al. 2013; de Haan et al. 2016; Planck Collaboration 2016g) and through cross-correlations with numerous other tracers (e.g. Planck Collaboration 2016f; Hill &…”
BackgroundPSZSPT: A joint Planck and SPT-SZ cluster catalog
Melin, J.-B., Bartlett, J. G., Tarrío, P., & Pratt, G. W. (2021) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202039471 · Cited by 22
“Progress in detecting numerous new clusters has been made in recent years with the advent of SZ surveys (Staniszewski et al. 2009; Menanteau et al. 2010; Planck Collaboration VIII 2011).”
BackgroundA MULTI-WAVELENGTH MASS ANALYSIS OF RCS2 J232727.6-020437, A ∼3 × 1015M⊙GALAXY CLUSTER ATz= 0.7
Sharon, K., Gladders, M. D., Marrone, D. P., Hoekstra, H., Rasia, E., Bourdin, H., Gifford, D., Hicks, A. K., Greer, C., Mroczkowski, T., et al. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/814/1/21 · Cited by 22
“…2011; Gettings et al. 2012; Stanford et al. 2012; Zeimann et al. 2012; Stanford et al. 2014), and detection of the the Sunyaev Zel’dovich (SZ) effect (Staniszewski et al. 2009; Vanderlinde et al. 2010; Williamson et al. 2011; Marriage et al. 2011; Planck Collaboration et al. 2013; Hasselfield et…”
BackgroundSelf-citationBayliss, M. B., Zengo, K., Ruel, J., Benson, B. A., Bleem, L. E., Bocquet, S., Bülbül, E., Brodwin, M., Capasso, R., Chiu, I.-N. T., et al. (2017) · The Astrophysical Journal · doi:10.3847/1538-4357/aa607c · Cited by 22
“Most of these clusters are from the South Pole Telescope (SPT) SZ survey (Staniszewski et al. 2009; Vanderlinde et al. 2010; Carlstrom et al. 2011; Williamson et al. 2011; Reichardt et al. 2013; Bleem et al. 2015), with additional clusters drawn from the Atacama Cosmology Telescope (ACT) SZ survey…”
MethodSelf-citationSolving the main cosmological puzzles with a generalized time varying vacuum energy
Basilakos, S. (2009) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/200912575/pdf · Cited by 22
GALAXY CLUSTERS AS A PROBE OF EARLY DARK ENERGY
Alam, U., Lukić, Z., & Bhattacharya, S. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/727/2/87 · Cited by 21
“Total number density of objects with masses above the given threshold as predicted by Tinker et al. (2008) is shown in lower left panels of Figures 2 and 3, for eROSITA and SPT survey, respectively.”
BackgroundInfluentialCOMPARISON OF HECTOSPEC VIRIAL MASSES WITH SUNYAEV-ZEL'DOVICH EFFECT MEASUREMENTS
Rines, K., Geller, M. J., & Diaferio, A. (2010) · The Astrophysical Journal Letters · doi:10.1088/2041-8205/715/2/l180 · Cited by 21
“…tests the robustness of the SZE as a proxy for cluster mass and the physical relationship between the SZE signal and cluster mass. Large SZ cluster surveys are underway and are beginning to yield cosmological constraints (Carlstrom et al. 2010; Hincks et al. 2010; Staniszewski et al. 2009).”
CMB Telescopes and Optical Systems
Hanany, S., Niemack, M. D., & Page, L. (2013) · Springer eBooks · doi:10.1007/978-94-007-5621-2_10 · Cited by 21
Fassbender, R., Böhringer, H., Santos, J. S., Pratt, G. W., Šuhada, R., Kohnert, J., Lerchster, M., Rovilos, M., Pierini, D., Chon, G., et al. (2010) · arXiv (Cornell University) · doi:10.48550/arxiv.1009.0264 · Cited by 21
“Significant progress is yet to be made to establish robust mass-observable relations atz ∼ 1 and beyond and to compare vices and virtues of mass proxies derived from optical/IR, X-ray, WL, and SZE observations at these redshifts.”
BackgroundSelf-citationYang, H.-Y. K., Bhattacharya, S., & Ricker, P. M. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/725/1/1124 · Cited by 20
“This distortion of the Planck spectrum can be measured by sensitive, high-resolution CMB telescopes from the ground (Hincks et al. 2009; Staniszewski et al. 2009; Vanderlinde et al. 2010), and it is one of the best ways to find clusters at higher redshifts (Brodwin et al. 2010), since the SZ effect…”
BackgroundLimits on the fluctuating part ofy-type distortion monopole from Planck and SPT results
Khatri, R., & Sunyaev, R. (2015) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2015/08/013 · Cited by 20
Gupta, N., Saro, A., Mohr, J. J., Benson, B. A., Bocquet, S., Capasso, R., Carlstrom, J. E., Chiu, I.-N. T., Crawford, T. M., de Haan, T., et al. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx095 · Cited by 20
Self-citationPHYSICAL PROPERTIES OF FOUR SZE-SELECTED GALAXY CLUSTERS IN THE SOUTHERN COSMOLOGY SURVEY
Menanteau, F., & Hughes, J. P. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/694/2/l136 · Cited by 20
SARCS strong-lensing galaxy groups
Foëx, G., Motta, V., Limousin, M., Verdugo, T., More, A., Cabanac, R., Gavazzi, R., & Muñoz, R. P. (2013) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201321112 · Cited by 19
“…& Yee 2005; Koester et al. 2007a), detection of variations in the cosmic microwave radiation due to the SZ effect (e.g. Carlstrom et al. 2002; Staniszewski et al. 2009; Planck Collaboration et al. 2011a), detection of the ICM diffuse X-ray emission (e.g. Mulchaey & Zabludoff 1998; Böhringer…”
BackgroundPrecision cosmology with a combination of wide and deep Sunyaev-Zel’dovich cluster surveys
Khedekar, S., Majumdar, S., & Das, S. (2010) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.82.041301 · Cited by 19
Zwart, J., Feroz, F., Davies, M., Franzen, T. M. O., Grainge, K., Hobson, M., Hurley-Walker, N., Kneissl, R., Lasenby, A. N., Olamaie, M., et al. (2011) · eSpace (Curtin University) · Cited by 19
Li, Q., Conselice, C. J., Sarron, F., Harvey, T., Austin, D., Adams, N., Trussler, J., Duan, Q., Ferreira, L., Westcott, L., et al. (2025) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staf543 · Cited by 18
Yoo, J., Zaldarriaga, M., & Hernquist, L. (2010) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.81.123006 · Cited by 18
Pierini, D., Šuhada, R., Fassbender, R., Nastasi, A., Böhringer, H., Salvato, M., Pratt, G. W., Lerchster, M., Rosati, P., Santos, J., et al. (2011) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201116674 · Cited by 18
“With the SZ-effect this has become possible very recently but only for massive clusters (Staniszewski et al. 2009; Vanderlinde et al. 2010; Marriage et al. 2011).”
BackgroundSelf-citationConstraints on non-resonant photon-axion conversion from the Planck satellite data
Mukherjee, S., Khatri, R., & Wandelt, B. D. (2019) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2019/06/031 · Cited by 18
Deep-CEE I: fishing for galaxy clusters with deep neural nets
Chan, M., & Stott, J. P. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz2936 · Cited by 18
“…al. 2000b, Böhringer et al. 2004, Takey et al. 2011, Mehrtens et al. 2012 and Adami, C. et al. 2018) and SZ surveys (e.g. E. Carlstrom et al. 2009, Staniszewski et al. 2009, Vanderlinde et al. 2010, Planck Collaboration et al. 2014, Bleem et al. 2015, Planck Collaboration: et al. 2015, Planck…”
BackgroundThe X-ray properties of weak-lensing-selected galaxy clusters
Giles, P. A., Maughan, B. J., Hamana, T., Miyazaki, S., Birkinshaw, M., Ellis, R. S., & Massey, R. J. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu2679 · Cited by 18
“Recently, the first clusters have been detected in blind surveys using the Sunyaev–Zel’dovich effect (SZE; Staniszewski et al. 2009; Vanderlinde et al. 2010; Planck Collaboration 2011a).”
MethodPSZSPT: a joint Planck and SPT-SZ cluster cataloguePreprint
Jeffrey, N., Alsing, J., & Lanusse, F. (2020) · HAL · Cited by 18
Sillassen, N. B., Jin, S., Magdis, G., Daddi, E., Wang, T., Lu, S., Sun, H., Arumugam, V., Liu, D., Brinch, M., et al. (2024) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202450760 · 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) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21064.x · Cited by 17
“…(2011) used the EDE parametrization by Corasaniti & Copeland (2003) to forecast constraints on these models from the abundance of X-ray clusters expected in the eROSITA survey (e.g. Predehl et al. 2007) and from the SZ power spectrum from the South Pole Telescope (SPT; Staniszewski et al. 2009).”
MethodA space mission to map the entire observable universe using the CMB as a backlight
Basu, K., Remazeilles, M., Melin, J.-B., Alonso, D., Bartlett, J. G., Battaglia, N., Chluba, J., Churazov, E., Delabrouille, J., Erler, J., et al. (2021) · Experimental Astronomy · doi:10.1007/s10686-021-09748-2 · Cited by 17
Metadata
- 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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Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
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