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arxiv: 2607.01175 · v1 · pith:NM7DBVGJnew · submitted 2026-07-01 · 🌌 astro-ph.CO · astro-ph.GA

Galaxy Clusters Selected via the Sunyaev-Zel'dovich Effect in 5 year data from the SPT-3G Main Survey

L. E. Bleem , M. Klein , K. Kornoelje , S. Bocquet , J. A. Sobrin , M. Aguena , E. Anderes , A. J. Anderson
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F. Andrade-Oliveira B. Ansarinejad M. Archipley L. Balkenhol D. R. Barron P. S. Barry M. Bayliss K. Benabed A. N. Bender B. A. Benson F. Bianchini F. R. Bouchet D. Brooks D. L. Burke M. Calzadilla R. Camilleri E. Camphuis M. G. Campitiello J. E. Carlstrom A. Carnero Rosell J. Carretero J. Carron C. L. Chang P. M. Chichura A. Chokshi T.-L. Chou A. Coerver M. Costanzi T. M. Crawford L. N. da Costa C. Daley T. M. Davis T. de Haan J. De Vicente S. Desai K. R. Dibert H. T. Diehl M. A. Dobbs M. Doohan D. Dutcher S. Everett G. Evrard C. Feng K. R. Ferguson N. C. Ferree K. Fichman B. Flaugher B. Floyd K. Fosdick A. Foster S. Galli A. E. Gambrel A. K. Gao J. Garc\'ia-Bellido F. Ge M. D. Gladders S. Grandis F. Guidi S. Guns G. Gutierrez N. W. Halverson S. R. Hinton E. Hivon G. P. Holder D. L. Hollowood W. L. Holzapfel J. C. Hood A. Hryciuk N. Huang T. Jhaveri S. Kent F. K\'eruzor\'e A. R. Khalife G. Khullar L. Knox K. Kuehn C.-L. Kuo O. Lahav K. Levy Y. Li A. E. Lowitz C. Lu G. P. Lynch T. J. Maccarone G. Mahler A. S. Maniyar J. L. Marshall E. S. Martsen M. McDonald J. Mena-Fern\'andez F. Menanteau M. Millea R. Miquel J. J. Mohr J. Montgomery J. Myles Y. Nakato T. Natoli R. C. Nichol V. Novosad R. L. C. Ogando Y. Omori A. Ouellette Z. Pan K. A. Phadke A. A. Plazas Malag\'on A. W. Pollak A. Porredon K. Prabhu J. Prat W. Quan S. Raghunathan M. Rahimi A. Rahlin C. L. Reichardt A. K. Romer M. Rouble J. E. Ruhl E. Sanchez D. Sanchez Cid T. Schrabback I. Sevilla-Noarbe A. C. Silva Oliveira A. Simpson T. Somboonpanyakul A. A. Stark E. Suchyta M. E. C. Swanson C. Tandoi C. To C. Trendafilova J. D. Vieira A. G. Vieregg V. Vikram A. Vitrier Y. Wan N. Weaverdyck J. Weller N. Whitehorn W. L. K. Wu M. R. Young J. A. Zebrowski J. Zhan
This is my paper

Pith reviewed 2026-07-02 06:17 UTC · model grok-4.3

classification 🌌 astro-ph.CO astro-ph.GA
keywords galaxy clustersSunyaev-Zel'dovich effectSPT-3Gcluster cataloghigh-redshift clusterscosmology
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The pith

The paper presents a catalog of 7190 confirmed galaxy clusters selected via the Sunyaev-Zel'dovich effect from five years of SPT-3G observations.

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

This work constructs a new sample of galaxy clusters by detecting their thermal imprint on the cosmic microwave background in high-resolution millimeter-wave maps. The resulting catalog reaches lower masses and higher redshifts than earlier SZ surveys while maintaining high purity after optical and infrared confirmation. Such a large, uniformly selected sample supports statistical studies of cluster abundance, mass calibration, and evolution across cosmic time. The data also enable direct comparisons with X-ray observations from eROSITA and internal tests for astrophysical contaminants.

Core claim

The central claim is a catalog of 8892 SZ cluster candidates above detection significance ξ=4 (expected purity >82 percent), with 7190 confirmed as real clusters; the sample covers masses 7.9×10^13 to 1.6×10^15 solar masses per h70 and redshifts 0.037 to roughly 2, achieving a surface density of 4.5 confirmed clusters per square degree and 2-4 times higher per-cluster signal-to-noise than prior SPT or ACT catalogs.

What carries the argument

Detection of the thermal Sunyaev-Zel'dovich effect, which produces a frequency-dependent temperature decrement in the cosmic microwave background proportional to the integrated electron pressure along the line of sight through a cluster.

If this is right

  • The catalog contains 1780 clusters above redshift 1 and 271 above redshift 1.5, extending the reach of SZ selection into the epoch when clusters first assembled.
  • Cross-matches yield 1279 clusters in common with the eRASS1 X-ray catalog, with mass estimates in relatively good agreement.
  • Validation tests reveal a seventeen-fold increase in 220 GHz emission for clusters at z approximately 1.5 compared with z approximately 0.25, indicating stronger correlated dusty emission at higher redshift.
  • A subset of clusters is identified as candidate strong gravitational lenses for follow-up study.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • The higher cluster density and improved mass reach could tighten cosmological constraints on structure growth when combined with weak-lensing or velocity-dispersion mass calibration.
  • The redshift-dependent dusty emission trend suggests that multi-frequency modeling will become increasingly important for SZ surveys targeting z greater than 1.
  • The flagged lens candidates provide a ready target list for high-resolution imaging to measure cluster masses independently of the SZ signal.

Load-bearing premise

Optical and infrared imaging reliably distinguishes true clusters from false detections across the full redshift range, especially above redshift 1.

What would settle it

Finding that the number of clusters confirmed at z greater than 1.5 falls well below the expected count from the purity estimates, or that SPT and eROSITA mass estimates show large systematic offsets for the same objects.

Figures

Figures reproduced from arXiv: 2607.01175 by A. A. Plazas Malag\'on, A. A. Stark, A. Carnero Rosell, A. Chokshi, A. Coerver, A. C. Silva Oliveira, A. E. Gambrel, A. E. Lowitz, A. Foster, A. G. Vieregg, A. Hryciuk, A. J. Anderson, A. K. Gao, A. K. Romer, A. N. Bender, A. Ouellette, A. Porredon, A. Rahlin, A. R. Khalife, A. Simpson, A. S. Maniyar, A. Vitrier, A. W. Pollak, B. A. Benson, B. Ansarinejad, B. Flaugher, B. Floyd, C. Daley, C. Feng, C. L. Chang, C.-L. Kuo, C. L. Reichardt, C. Lu, C. Tandoi, C. To, C. Trendafilova, D. Brooks, D. Dutcher, D. L. Burke, D. L. Hollowood, D. R. Barron, D. Sanchez Cid, E. Anderes, E. Camphuis, E. Hivon, E. Sanchez, E. S. Martsen, E. Suchyta, F. Andrade-Oliveira, F. Bianchini, F. Ge, F. Guidi, F. K\'eruzor\'e, F. Menanteau, F. R. Bouchet, G. Evrard, G. Gutierrez, G. Khullar, G. Mahler, G. P. Holder, G. P. Lynch, H. T. Diehl, I. Sevilla-Noarbe, J. A. Sobrin, J. A. Zebrowski, J. Carretero, J. Carron, J. C. Hood, J. De Vicente, J. D. Vieira, J. E. Carlstrom, J. E. Ruhl, J. Garc\'ia-Bellido, J. J. Mohr, J. L. Marshall, J. Mena-Fern\'andez, J. Montgomery, J. Myles, J. Prat, J. Weller, J. Zhan, K. A. Phadke, K. Benabed, K. Fichman, K. Fosdick, K. Kornoelje, K. Kuehn, K. Levy, K. Prabhu, K. R. Dibert, K. R. Ferguson, L. Balkenhol, L. E. Bleem, L. Knox, L. N. da Costa, M. A. Dobbs, M. Aguena, M. Archipley, M. Bayliss, M. Calzadilla, M. Costanzi, M. D. Gladders, M. Doohan, M. E. C. Swanson, M. G. Campitiello, M. Klein, M. McDonald, M. Millea, M. Rahimi, M. Rouble, M. R. Young, N. C. Ferree, N. Huang, N. Weaverdyck, N. W. Halverson, N. Whitehorn, O. Lahav, P. M. Chichura, P. S. Barry, R. Camilleri, R. C. Nichol, R. L. C. Ogando, R. Miquel, S. Bocquet, S. Desai, S. Everett, S. Galli, S. Grandis, S. Guns, S. Kent, S. Raghunathan, S. R. Hinton, T. de Haan, T. Jhaveri, T. J. Maccarone, T.-L. Chou, T. M. Crawford, T. M. Davis, T. Natoli, T. Schrabback, T. Somboonpanyakul, V. Novosad, V. Vikram, W. L. Holzapfel, W. L. K. Wu, W. Quan, Y. Li, Y. Nakato, Y. Omori, Y. Wan, Z. Pan.

Figure 1
Figure 1. Figure 1: — Footprint of the SPT-3G survey plotted with those of several other multi-wavelength surveys discussed in this work. The footprints are overlaid on a dust map from Planck Collaboration et al. (2016a). The full SPT-3G 10,000 deg2 survey is shown in pale blue, the boundaries of the SPT-Euclid Deep field South (Archipley et al. 2026) and SPT 100d Deep field (Kornoelje et al. 2026) are white-dashed, and the S… view at source ↗
Figure 2
Figure 2. Figure 2: — (Left) Cutout of 3o × 6.5 o of SPT-3G Main field survey data (approximately 1.2% of the Main field survey area). The rgb image is constructed using the 95 (red), 150 GHz (green), and 220 (blue) GHz data with peak-to-peak fluctuations in each channel of ±110µKCMB. This figure illustrates the main constituents of the SPT-3G temperature maps. As the maps are calibrated in µKCMB units, CMB fluctuations have … view at source ↗
Figure 3
Figure 3. Figure 3: — Distribution of cluster sample properties in terms of detection significance, ξ, (top) and corresponding filter scales (bot￾tom). In orange we show the full sample and, over-plotted in blue, the clusters confirmed by the optical analysis as discussed in Sec. 4. In the top panel we also highlight several massive well-known clusters in the SPT footprint. The distribution in θc of the pre￾dominately low-ξ u… view at source ↗
Figure 4
Figure 4. Figure 4: — Top: The expected purity (orange) and number of false detections (green) for the SPT-3G Main field cluster catalog as a function of minimum ξ without additional optical follow-up. We find an expected purity of 82% above ξmin = 4, and 99% above ξmin = 5. Bottom: The expected purity of the cluster sample as a function of filter core size, θc. Here the label “Peak Core Size” reflects that the simulated clus… view at source ↗
Figure 5
Figure 5. Figure 5: — MCMF richness λ vs. redshift for the SPT-3G candi￾date list at ξ > 4. In solid lines we overplot the richness confirma￾tion thresholds of fmax cont =0.2 for the LS-DR10 and WISE datasets. In blue we plot clusters confirmed by MCMF in the sample, in black we mark clusters confirmed using other datasets (see Sec. 4.5.), and in gray SPT candidates with optical associations below our confirmation threshold. … view at source ↗
Figure 6
Figure 6. Figure 6: — SPT-CL J2128.4−5658.0, a ξ = 10 cluster at z ≳ 1.6 confirmed using the combination of WISE and Magellan/FourStar data. The 3′ diameter rgb image is constructed from FourStar/J￾band and LS-DR10 z- and r-band data; SZ detection countours are overlaid on the image. solved for by SCAMP (Bertin 2006) based on source po￾sitions extracted using SExtractor (Bertin & Arnouts 1996). Images are then resampled and r… view at source ↗
Figure 7
Figure 7. Figure 7: — DECam imaging of SPT-3G clusters from the LS-DR10 release (Dey et al. 2019) with SZ detection contours overlaid. The rgb images were created from z−, r−, g−band data and are 3. ′8 in diameter. Clusters were selected to illustrate the SZ significance and redshift reach of the sample. The highest-redshift clusters were confirmed with additional observations from Spitzer, FourStar (Sec. 4.3), and WISE. scal… view at source ↗
Figure 8
Figure 8. Figure 8: — Redshift distribution of the 7,190 confirmed clusters in the SPT-3G Main field sample confirmed using optical-IR data as discussed in Sec. 4. As noted in Sec. 4.5, owing to color degeneracies in the IR, we assign clusters with redshifts estimated at z > 1.6 using the 1.6 µm bump method to a value of z = 1.6 in the catalog table, but we use their raw best-fit redshifts in the histogram here to illustrate … view at source ↗
Figure 9
Figure 9. Figure 9: — Parameters of the SZ and richness observable-mass relations assuming a fixed reference cosmology (68% and 95% credibility). Gold contours show an analysis of the cluster counts where we model the sample selection in detection significance ξ and redshift z (we fix σln ζ = 0.2 in this case as shown by the dashed line). Blue contours show an analysis of the cluster counts where we model the sample selection… view at source ↗
Figure 10
Figure 10. Figure 10: — Distribution of the (ξ > 5, 0.25 < z < 1) subsample of SPT-3G clusters in the space of SPT significance and optical richness. The straight line shows the mean model and contours show the expected distribution. We find 27 out of 3,005 clusters outside of the 99% contour, in line with the expectation. Clusters whose richness estimates are likely to be affected by masking are shown with gray crosses and ar… view at source ↗
Figure 11
Figure 11. Figure 11: — The mass-redshift distribution of the five-year SPT-3G Main field sample compared to other recent large ICM-selected cluster samples, including those from ACT (ACTDESHSC Collaboration et al. 2026), eROSITA (Bulbul et al. 2024), Planck (Planck Collaboration et al. 2016b), and previously published samples from the SPT-SZ, SPTpol, and SPT-3G collaborations (Bleem et al. 2015, 2020, 2024; Klein et al. 2024b… view at source ↗
Figure 12
Figure 12. Figure 12: — Estimated completeness of the SPT-3G Main cluster sample above ξ = 4 at several different redshifts. As discussed in Sec. 6, the sample has a declining mass threshold as a function of redshift. The sample is expected to be > 90% complete for masses M500c ≳ 2 × 1014 M⊙/h70 at z > 0.25. SPT-3G cluster sample using DECALS and archival SPT follow-up data. We additionally flag potential lenses in Sec. 10.1.1… view at source ↗
Figure 13
Figure 13. Figure 13: — Redshift-scaled (Sec. 5) SPT detection significance, ξ, vs. X-ray mass for clusters at z > 0.25 in the eRASS1 cosmol￾ogy sample (Bulbul et al. 2024). In bold we plot eRASS1 clusters that have counterparts within the SPT-3G catalog (89%), while in pale gray we plot force-photometered ξ values for clusters with￾out matches; note that the y-axis scaling transitions from log to linear below the SPT detectio… view at source ↗
Figure 14
Figure 14. Figure 14: — Optical richness vs. SZ-inferred mass for the subset of 1,909 clusters at 0.2 < z < 0.95 found in all four (SPT-3G, redMaPPer Y3, MaDCoWS2, and WH24) cluster samples. MCMF, our baseline confirmation method (Sec. 4) shows the smallest scatter with SZ mass, followed by the redMaPPer sample. The WH24 sample, while having large scatter, is the most complete (∼ 78%) of the external catalogs. peaking in the s… view at source ↗
Figure 15
Figure 15. Figure 15: — [PITH_FULL_IMAGE:figures/full_fig_p030_15.png] view at source ↗
Figure 16
Figure 16. Figure 16: — Redshift evolution of the median correlated 220 GHz emission at SPT-3G cluster locations; this emission increases by over an order of magnitude over the redshift range probed by the SPT sample (0.25 < z ≲ 2), while the median Compton-y value in each bin is comparable. As above, the region z > 1.6 is shaded to denote higher redshift uncertainties; the plotted redshifts in each bin are the median of the b… view at source ↗
read the original abstract

We report a new galaxy cluster catalog, selected using the thermal Sunyaev-Zel'dovich (SZ) effect, from 5 years of observations of the SPT-3G Main field. Drawn from arcminute-resolution data with white noise levels of 3.2, 2.5, and 8.9 $\mu$K-arcmin at 95, 150, and 220 GHz, respectively, the sample consists of 8,892 cluster candidates detected above significance $\xi=4$, with an expected purity of $>82\%$ (4,480 at $\xi\ge5$ with purity $>99\%$). Using optical and infrared data we have confirmed 7,190 candidates as clusters. The sample spans a mass range $7.9 \times 10^{13}$ $M_\odot/h_{70}$ \ $< M_\textrm{500c} < $ $1.6 \times 10^{15}$ $M_\odot/h_{70}$ with a median mass of $1.65 \times 10^{14}$ $M_\odot/h_{70}$, and a redshift range of $0.037<z\lesssim 2$ with a median redshift of $z_{\textrm{med}}$ = 0.73; 1,780 clusters are at $z>1$ and 271 at $z>1.5$. Compared to previous SZ cluster samples from South Pole Telescope and Atacama Cosmology Telescope data, the SPT-3G sample is highly consistent in mass and redshift but is significantly deeper, with per-cluster detection signal-to-noise 2-4 times higher and a cluster density of 4.5 confirmed clusters/deg$^2$. We cross match with eRASS1 cluster and point source catalogs, finding 1,279 and 1,319 matches, respectively. The SPT and eROSITA cluster mass estimates are in relatively good agreement. We perform a series of validation checks using both internal data splits and comparisons to external samples. These tests show increasing correlated (dusty) emission with redshift, with a $\sim17\times$ larger 220 GHz temperature increment for clusters at $z\sim1.5$ than $z\sim0.25$, but only weak evidence for correlated synchrotron emission. Finally, a number of clusters are flagged as candidate strong gravitational lenses.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

0 major / 3 minor

Summary. The manuscript reports a new SZ-selected galaxy cluster catalog from 5 years of SPT-3G Main Survey observations. It contains 8,892 candidates detected at ξ ≥ 4 (expected purity >82%) and 4,480 at ξ ≥ 5 (purity >99%), with 7,190 confirmed as clusters via optical and infrared data. The sample spans 7.9×10^13 M⊙/h70 < M500c < 1.6×10^15 M⊙/h70 (median 1.65×10^14 M⊙/h70) and 0.037 < z ≲ 2 (median z=0.73), including 1,780 clusters at z>1. It includes cross-matches with eRASS1 (1,279 clusters, 1,319 point sources), internal validation splits, and notes on redshift-dependent dusty emission.

Significance. If the reported purities and confirmations hold, this catalog is a substantial advance over prior SPT and ACT SZ samples due to its greater depth, 2-4× higher per-cluster S/N, and cluster density of 4.5 confirmed clusters/deg². The large high-redshift subsample and eRASS1 cross-matches support improved cosmological constraints and studies of cluster astrophysics at z>1. The validation checks using data splits and external comparisons add credibility to the catalog's utility.

minor comments (3)
  1. The abstract and text use ξ for detection significance without an explicit definition or reference to its construction in the methods section; adding a brief equation or citation to prior SPT papers would improve clarity for readers.
  2. Mass and redshift ranges are reported with h70 and M500c; ensure consistent notation and units are used throughout all tables and figures.
  3. The statement on increasing correlated dusty emission (∼17× larger 220 GHz increment at z∼1.5 vs z∼0.25) is presented without an accompanying figure or table quantifying the trend; a supplemental plot would strengthen the validation section.

Simulated Author's Rebuttal

0 responses · 0 unresolved

We thank the referee for their positive assessment of the manuscript and their recommendation to accept. We are pleased that the referee finds the catalog to be a substantial advance and that the validation checks add credibility.

Circularity Check

0 steps flagged

No significant circularity in derivation chain

full rationale

This is an observational catalog paper reporting counts of SZ-selected cluster candidates, confirmation statistics via optical/IR data, mass/redshift ranges, and validation checks against external catalogs. No equations, fitted parameters, or self-citation chains are invoked to derive the headline numbers; the reported quantities are direct outputs of the detection and confirmation pipeline rather than predictions that reduce to inputs by construction. The paper is self-contained against external benchmarks with no load-bearing self-referential steps.

Axiom & Free-Parameter Ledger

2 free parameters · 2 axioms · 0 invented entities

The central claim rests on the SZ detection pipeline and optical/IR confirmation, which rely on standard field assumptions rather than new derivations or invented entities.

free parameters (2)
  • significance threshold ξ=4
    Chosen to achieve stated purity of >82%; value is a selection cut.
  • purity estimates from simulations
    Expected purity values are simulation-derived and affect the reported sample.
axioms (2)
  • domain assumption The thermal SZ effect dominates the detected signal in galaxy clusters
    Standard assumption invoked for all SZ cluster selection.
  • domain assumption Optical and infrared data provide reliable cluster confirmation
    Directly invoked to convert candidates to confirmed clusters.

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Reference graph

Works this paper leans on

298 extracted references · 212 canonical work pages · 42 internal anchors

  1. [1]

    Shear-selected Clusters from the Deep Lens Survey. III. Masses from Weak Lensing. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/702/1/603 , adsurl =

    work page doi:10.1088/0004-637x/702/1/603

  2. [2]

    The Seventh Data Release of the Sloan Digital Sky Survey

    The Seventh Data Release of the Sloan Digital Sky Survey. , archivePrefix = "arXiv", eprint =. doi:10.1088/0067-0049/182/2/543 , adsurl =

    work page internal anchor Pith review doi:10.1088/0067-0049/182/2/543

  3. [3]

    Astroparticle Physics , year = 2015, month = mar, volume = 63, pages =

    Inflation physics from the cosmic microwave background and large scale structure. Astroparticle Physics , year = 2015, month = mar, volume = 63, pages =. doi:10.1016/j.astropartphys.2014.05.013 , adsurl =

    work page doi:10.1016/j.astropartphys.2014.05.013 2015

  4. [4]

    Astroparticle Physics , year = 2015, month = mar, volume = 63, pages =

    Neutrino physics from the cosmic microwave background and large scale structure. Astroparticle Physics , year = 2015, month = mar, volume = 63, pages =. doi:10.1016/j.astropartphys.2014.05.014 , adsurl =

    work page doi:10.1016/j.astropartphys.2014.05.014 2015

  5. [5]

    ArXiv e-prints , archivePrefix = "arXiv", eprint =

    CMB-S4 Science Book, First Edition. ArXiv e-prints , archivePrefix = "arXiv", eprint =

  6. [6]

    arXiv e-prints , keywords =

    CMB-S4 Science Case, Reference Design, and Project Plan. arXiv e-prints , keywords =. 2019

    2019

  7. [7]

    The base models and a new line index system

    The VIMOS-VLT Deep Survey: evolution in the halo occupation number since z \ 1. , archivePrefix = "arXiv", eprint =. doi:10.1111/j.1365-2966.2010.16764.x , adsurl =

    work page doi:10.1111/j.1365-2966.2010.16764.x 2010

  8. [8]

    Physics Letters B , year = 1983, month = jan, volume =

    A cosmological bound on the invisible axion. Physics Letters B , year = 1983, month = jan, volume =. doi:10.1016/0370-2693(83)90638-X , adsurl =

    work page doi:10.1016/0370-2693(83)90638-x 1983

  9. [9]

    , archivePrefix = "arXiv", eprint =

    Cosmology from cosmic shear with Dark Energy Survey Science Verification data. , archivePrefix = "arXiv", eprint =. doi:10.1103/PhysRevD.94.022001 , adsurl =

    work page doi:10.1103/physrevd.94.022001

  10. [10]

    Dark Energy Survey Year 1 Results: A Precise H0 Measurement from DES Y1, BAO, and D/H Data

    Dark Energy Survey Year 1 Results: A Precise H _ 0 Estimate from DES Y1, BAO, and D/H Data. , keywords =. 2018. doi:10.1093/mnras/sty1939 , archivePrefix =. 1711.00403 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1093/mnras/sty1939 2018

  11. [11]

    The Dark Energy Survey Data Release 1

    The Dark Energy Survey: Data Release 1. The Astrophysical Journal Supplement Series , keywords =. 2018. doi:10.3847/1538-4365/aae9f0 , archivePrefix =. 1801.03181 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.3847/1538-4365/aae9f0 2018

  12. [12]

    , keywords =

    Dark Energy Survey year 1 results: Joint analysis of galaxy clustering, galaxy lensing, and CMB lensing two-point functions. , keywords =. 2019. doi:10.1103/PhysRevD.100.023541 , archivePrefix =. 1810.02322 , primaryClass =

    work page doi:10.1103/physrevd.100.023541 2019

  13. [13]

    , keywords =

    The Dark Energy Survey Data Release 2. , keywords =. doi:10.3847/1538-4365/ac00b3 , archivePrefix =. 2101.05765 , primaryClass =

    work page doi:10.3847/1538-4365/ac00b3

  14. [14]

    Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing

    Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and weak lensing. , keywords =. doi:10.1103/PhysRevD.105.023520 , archivePrefix =. 2105.13549 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.105.023520

  15. [15]

    Joint analysis of Dark Energy Survey Year 3 data and CMB lensing from SPT and Planck. III. Combined cosmological constraints. , keywords =. doi:10.1103/PhysRevD.107.023531 , archivePrefix =. 2206.10824 , primaryClass =

    work page doi:10.1103/physrevd.107.023531

  16. [16]

    Abbott, M

    DES Y3 + KiDS-1000: Consistent cosmology combining cosmic shear surveys. The Open Journal of Astrophysics , keywords =. doi:10.21105/astro.2305.17173 , archivePrefix =. 2305.17173 , primaryClass =

    work page doi:10.21105/astro.2305.17173

  17. [17]

    Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies

    Cosmology intertwined: A review of the particle physics, astrophysics, and cosmology associated with the cosmological tensions and anomalies. Journal of High Energy Astrophysics , keywords =. doi:10.1016/j.jheap.2022.04.002 , archivePrefix =. 2203.06142 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1016/j.jheap.2022.04.002 2022

  18. [18]

    The second catalog of flaring gamma-ray sources from the Fermi All-sky Variability Analysis

    The Second Catalog of Flaring Gamma-Ray Sources from the Fermi All-sky Variability Analysis. , keywords =. doi:10.3847/1538-4357/aa8092 , archivePrefix =. 1612.03165 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.3847/1538-4357/aa8092

  19. [19]

    arXiv e-prints , keywords =

    Abdollahi, Soheila and others , title = ". arXiv e-prints , keywords =

  20. [20]

    Measurement of neutrino and antineutrino oscillations by the T2K experiment including a new additional sample of $\nu_e$ interactions at the far detector

    Measurement of neutrino and antineutrino oscillations by the T2K experiment including a new additional sample of _ e interactions at the far detector. , keywords =. 2017. doi:10.1103/PhysRevD.96.092006 , archivePrefix =. 1707.01048 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.96.092006 2017

  21. [21]

    , year = 1958, month = may, volume = 3, pages =

    The Distribution of Rich Clusters of Galaxies. , year = 1958, month = may, volume = 3, pages =. doi:10.1086/190036 , adsurl =

    work page doi:10.1086/190036 1958

  22. [22]

    , keywords =

    A catalog of rich clusters of galaxies. , keywords =. doi:10.1086/191333 , adsurl =

    work page doi:10.1086/191333

  23. [23]

    , archivePrefix = "arXiv", eprint =

    Characterizing and Propagating Modeling Uncertainties in Photometrically Derived Redshift Distributions. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/734/1/36 , adsurl =

    work page doi:10.1088/0004-637x/734/1/36

  24. [24]

    Correlations Between the WMAP and MAXIMA Cosmic Microwave Background Anisotropy Maps , journal =

  25. [25]

    , keywords =

    Partially constrained internal linear combination: A method for low-noise CMB foreground mitigation. , keywords =. doi:10.1103/PhysRevD.103.103510 , archivePrefix =. 2012.04032 , primaryClass =

    work page doi:10.1103/physrevd.103.103510 2012

  26. [26]

    arXiv e-prints , keywords =

    First measurement of neutrino oscillation parameters using neutrinos and antineutrinos by NOvA. arXiv e-prints , keywords =. 2019

    2019

  27. [27]

    Nuclear Physics B , eprint =

    Gauge-invariant second-order perturbations and non-Gaussianity from inflation. Nuclear Physics B , eprint =. doi:10.1016/S0550-3213(03)00550-9 , adsurl =

    work page doi:10.1016/s0550-3213(03)00550-9

  28. [28]

    Next Generation Redshift Surveys and the Origin of Cosmic Acceleration

    doi:10.1103/PhysRevD.78.043514 , Eid =. arXiv , Author =:0803.2236 , Journal =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.78.043514

  29. [29]

    How to falsify the

    Acquaviva, Viviana and Gawiser, Eric , journal =. How to falsify the. 2010 , month =. doi:10.1103/PhysRevD.82.082001 , url =

    work page doi:10.1103/physrevd.82.082001 2010

  30. [30]

    , keywords =

    Improved Upper Limit on Degree-scale CMB B-mode Polarization Power from the 670 Square-degree POLARBEAR Survey. , keywords =. doi:10.3847/1538-4357/ac6809 , archivePrefix =. 2203.02495 , primaryClass =

    work page doi:10.3847/1538-4357/ac6809

  31. [31]

    and Bartalucci, I

    Adam, R. and Bartalucci, I. and Pratt, G. W. and Ade, P. and Andr\'. Mapping the kinetic Sunyaev-Zel'dovich effect toward MACS J0717.5+3745 with NIKA , volume=. 2017 , month=. doi:10.1051/0004-6361/201629182 , journal=

    work page doi:10.1051/0004-6361/201629182 2017

  32. [32]

    The XXL Survey. XX. The 365 cluster catalogue. , keywords =. 2018. doi:10.1051/0004-6361/201731606 , archivePrefix =. 1810.03849 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1051/0004-6361/201731606 2018

  33. [33]

    Natural Inflation: Particle Physics Models, Power Law Spectra for Large Scale Structure, and Constraints from COBE

    Natural inflation: Particle physics models, power-law spectra for large-scale structure, and constraints from the Cosmic Background Explorer. , keywords =. doi:10.1103/PhysRevD.47.426 , archivePrefix =. hep-ph/9207245 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.47.426

  34. [34]

    Physical Review Letters , archivePrefix = "arXiv", eprint =

    Measurement of _ μ and _ e Events in an Off-Axis Horn-Focused Neutrino Beam. Physical Review Letters , archivePrefix = "arXiv", eprint =. doi:10.1103/PhysRevLett.102.211801 , adsurl =

    work page doi:10.1103/physrevlett.102.211801

  35. [35]

    , archivePrefix = "arXiv", eprint =

    Power-law Template for Infrared Point-source Clustering. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/752/2/120 , adsurl =

    work page doi:10.1088/0004-637x/752/2/120

  36. [36]

    2012, , 427, 127, 10.1111/j.1365-2966.2012.21948.x

    Modelling the correlation between the thermal Sunyaev Zel'dovich effect and the cosmic infrared background. , archivePrefix = "arXiv", eprint =. doi:10.1111/j.1365-2966.2012.21664.x , adsurl =

    work page doi:10.1111/j.1365-2966.2012.21664.x 2012

  37. [37]

    , archivePrefix = "arXiv", eprint =

    Constraining thermal dust emission in distant galaxies with number counts and angular power spectra. , archivePrefix = "arXiv", eprint =. doi:10.1093/mnras/stt1703 , adsurl =

    work page doi:10.1093/mnras/stt1703

  38. [38]

    , archivePrefix = "arXiv", eprint =

    Quantifying Discordance in the 2015 Planck CMB Spectrum. , archivePrefix = "arXiv", eprint =. doi:10.3847/0004-637X/818/2/132 , adsurl =

    work page doi:10.3847/0004-637x/818/2/132 2015

  39. [39]

    , archivePrefix = "arXiv", eprint =

    Elucidating CDM: Impact of Baryon Acoustic Oscillation Measurements on the Hubble Constant Discrepancy. , archivePrefix = "arXiv", eprint =. doi:10.3847/1538-4357/aaa1ed , adsurl =

    work page doi:10.3847/1538-4357/aaa1ed

  40. [40]

    arXiv e-prints , keywords =

    High H_0 Values from CMB E-mode Data: A Clue for Resolving the Hubble Tension?. arXiv e-prints , keywords =

  41. [41]

    Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series , year = 2006, series =

    A review of metal mesh filters. Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series , year = 2006, series =. doi:10.1117/12.673162 , adsurl =

    work page doi:10.1117/12.673162 2006

  42. [42]

    The Simons Observatory: Science goals and forecasts

    The Simons Observatory: science goals and forecasts. , keywords =. 2019. doi:10.1088/1475-7516/2019/02/056 , archivePrefix =. 1808.07445 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/1475-7516/2019/02/056 2019

  43. [43]

    P. A. R. Ade and Z. Ahmed and M. Amiri and D. Barkats and R. Basu Thakur and C. A. Bischoff and D. Beck and J. J. Bock and H. Boenish and E. Bullock and V. Buza and J. R. Cheshire IV and J. Connors and J. Cornelison and M. Crumrine and A. Cukierman and E. V. Denison and M. Dierickx and L. Duband and M. Eiben and S. Fatigoni and J. P. Filippini and S. Flie...

    work page doi:10.3847/1538-4357/acc85c 2023

  44. [44]

    and Braine , T

    ADMX Collaboration and Bartram , C. and Braine , T. and Burns , E. and Cervantes , R. and Crisosto , N. and Du , N. and Korandla , H. and Leum , G. and Mohapatra , P. and Nitta , T. and Rosenberg , L. J and Rybka , G. and Yang , J. and Clarke , John and Siddiqi , I. and Agrawal , A. and Dixit , A. V. and Awida , M. H. and Chou , A. S. and Hollister , M. a...

    work page doi:10.1103/physrevlett.127.261803 2021

  45. [45]

    Cosmology with Sunyaev-Zel'dovich observations from space

    "Cosmology with Sunyaev-Zel'dovich observations from space." , journal =

  46. [46]

    PACT. I. Combining ACT and Planck data for improved extraction of tSZ signal. , keywords =. doi:10.1051/0004-6361/201935271 , archivePrefix =. 1902.00350 , primaryClass =

    work page doi:10.1051/0004-6361/201935271 1902

  47. [47]

    and Akrami, Y

    Aghanim, N. and Akrami, Y. and Ashdown, M. and Aumont, J. and Baccigalupi, C. and Ballardini, M. and Banday, A. J. and Barreiro, R. B. and Bartolo, N. and Basak, S. and Benabed, K. and Bernard, J.-P. and Bersanelli, M. and Bielewicz, P. and Bock, J. J. and Bond, J. R. and Borrill, J. and Bouchet, F. R. and Boulanger, F. and Bucher, M. and Burigana, C. and...

    work page doi:10.1051/0004-6361/201936386

  48. [48]

    , keywords =

    Laboratory Results on Millimeter-Wave Absorption in Silicate Grain Materials at Cryogenic Temperatures. , keywords =. doi:10.1086/177217 , adsurl =

    work page doi:10.1086/177217

  49. [49]

    New technological development for far-infrared bolometer arrays. Proc. SPIE Vol. 3698, p. 284-290, Infrared Technology and Applications XXV, Bjorn F. Andresen; Marija Strojnik Scholl; Eds. , year = 1999, month = jul, pages =

    1999

  50. [50]

    On the Location of the Gamma-ray Emission in the 2008 Outburst in the BL Lacertae Object AO 0235+164 through Observations across the Electromagnetic Spectrum

    On the Location of the -Ray Outburst Emission in the BL Lacertae Object AO 0235+164 Through Observations Across the Electromagnetic Spectrum. , keywords =. doi:10.1088/2041-8205/735/1/L10 , archivePrefix =. 1105.0549 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/2041-8205/735/1/l10 2041

  51. [51]

    , eprint =

    Evidence for neutrino oscillations from the observation of _ e appearance in a _ ? beam. , eprint =. doi:10.1103/PhysRevD.64.112007 , adsurl =

    work page doi:10.1103/physrevd.64.112007

  52. [52]

    , keywords =

    Event Excess in the MiniBooNE Search for _ μ _ e Oscillations. , keywords =. doi:10.1103/PhysRevLett.105.181801 , adsurl =

    work page doi:10.1103/physrevlett.105.181801

  53. [53]

    , eprint =

    The Spectrum of Integrated Millimeter Flux of the Magellanic Clouds and 30 Doradus from TopHat and DIRBE Data. , eprint =. doi:10.1086/377601 , adsurl =

    work page doi:10.1086/377601

  54. [54]

    Ahmad, Q. R. and Allen, R. C. and Andersen, T. C. and D.Anglin, J. and Barton, J. C. and Beier, E. W. and Bercovitch, M. and Bigu, J. and Biller, S. D. and Black, R. A. and Blevis, I. and Boardman, R. J. and Boger, J. and Bonvin, E. and Boulay, M. G. and Bowler, M. G. and Bowles, T. J. and Brice, S. J. and Browne, M. C. and Bullard, T. V. and B\"uhler, G....

    work page doi:10.1103/physrevlett.89.011301 2002

  55. [55]

    BICEP3: a 95 GHz refracting telescope for degree-scale CMB polarization

    BICEP3: a 95GHz refracting telescope for degree-scale CMB polarization. Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series , year = 2014, series =. doi:10.1117/12.2057224 , adsurl =. arXiv:1407.5928 , primaryClass = "astro-ph.IM", month = aug, eid =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1117/12.2057224 2014

  56. [56]

    JCAP , keywords =

    The Atacama Cosmology Telescope: DR4 maps and cosmological parameters. , keywords =. doi:10.1088/1475-7516/2020/12/047 , archivePrefix =. 2007.07288 , primaryClass =

    work page doi:10.1088/1475-7516/2020/12/047 2020

  57. [57]

    Akeson, R. L. Millimeter Interferometric Polarimetry of Magnetic Field Structure in Protostellar Condensations

  58. [58]

    , number =

    Nature Phys. , number =. 2022 , Bdsk-Url-1 =. doi:10.1038/s41567-021-01463-1 , eprint =

    work page doi:10.1038/s41567-021-01463-1 2022

  59. [59]

    Akeson, R. L. and Carlstrom, J. E. and Phillips, J. A. and Woody, D. P. Millimeter Interferometric Polarization Imaging of the Young Stellar Object NGC-1333 IRAS-4A

  60. [60]

    Akeson, R. L. and Carlstrom, J. E. Magnetic Field Structure in Protostellar Envelopes

  61. [61]

    , archivePrefix = "arXiv", eprint =

    Galaxy Clusters as a Probe of Early Dark Energy. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/727/2/87 , adsurl =

    work page doi:10.1088/0004-637x/727/2/87

  62. [62]

    , archivePrefix = "arXiv", eprint =

    The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample. , archivePrefix = "arXiv", eprint =. doi:10.1093/mnras/stx721 , adsurl =

    work page doi:10.1093/mnras/stx721

  63. [63]

    The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory

    Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from two decades of spectroscopic surveys at the Apache Point Observatory. , keywords =. doi:10.1103/PhysRevD.103.083533 , archivePrefix =. 2007.08991 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.103.083533 2007

  64. [64]

    Star Formation and AGN Activity in Galaxy Clusters from $z=1-2$: a Multi-wavelength Analysis Featuring $Herschel$/PACS

    Star Formation and AGN Activity in Galaxy Clusters from z=1-2: a Multi-Wavelength Analysis Featuring Herschel/PACS. The Astrophysical Journal , keywords =. 2016. doi:10.3847/0004-637X/825/1/72 , archivePrefix =. 1604.03564 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.3847/0004-637x/825/1/72 2016

  65. [65]

    Universe , keywords =

    From Clusters to Proto-Clusters: The Infrared Perspective on Environmental Galaxy Evolution. Universe , keywords =. doi:10.3390/universe8110554 , archivePrefix =. 2209.02781 , primaryClass =

    work page doi:10.3390/universe8110554

  66. [66]

    and Steinhardt, P

    Albrecht, A. and Steinhardt, P. J. COSMOLOGY FOR GRAND UNIFIED THEORIES WITH RADIATIVELY INDUCED SYMMETRY BREAKING. Phys. Rev. Lett. 1982

    1982

  67. [67]

    Causality and the microwave background

    Andreas Albrecht and David Coulson and Pedro Ferreira and Joao Magueijo. Causality and the microwave background. Phys. Rev. Lett. 1996

    1996

  68. [68]

    ArXiv Astrophysics e-prints , eprint =

    Report of the Dark Energy Task Force. ArXiv Astrophysics e-prints , eprint =

  69. [69]

    Physical Review Letters , archivePrefix = "arXiv", eprint =

    Cosmic Curvature from de Sitter Equilibrium Cosmology. Physical Review Letters , archivePrefix = "arXiv", eprint =. doi:10.1103/PhysRevLett.107.151102 , adsurl =

    work page doi:10.1103/physrevlett.107.151102

  70. [70]

    , year = 1979, month = oct, volume = 281, pages =

    An evolution free test for non-zero cosmological constant. , year = 1979, month = oct, volume = 281, pages =. doi:10.1038/281358a0 , adsurl =

    work page doi:10.1038/281358a0 1979

  71. [71]

    Inflationary birefringence and baryogenesis , volume=

    Alexander, Stephon , year=. Inflationary birefringence and baryogenesis , volume=. International Journal of Modern Physics D , publisher=. doi:10.1142/s0218271816400137 , number=

    work page doi:10.1142/s0218271816400137

  72. [72]

    , keywords =

    Improved constraints on dark energy from Chandra X-ray observations of the largest relaxed galaxy clusters. , archivePrefix = "arXiv", eprint =. doi:10.1111/j.1365-2966.2007.12610.x , adsurl =

    work page doi:10.1111/j.1365-2966.2007.12610.x 2007

  73. [73]

    , keywords =

    Constraints on dark energy from Chandra observations of the largest relaxed galaxy clusters. , year = 2004, month = sep, volume = 353, pages =. doi:10.1111/j.1365-2966.2004.08080.x , adsurl =

    work page doi:10.1111/j.1365-2966.2004.08080.x 2004

  74. [74]

    , year = 1998, month = jul, volume = 297, pages =

    The Impact of Cooling Flows on the T_X - L_ Bol Relation for the Most Luminous Clusters. , year = 1998, month = jul, volume = 297, pages =

    1998

  75. [75]

    , archivePrefix = "arXiv", eprint =

    Cosmological Parameters from Observations of Galaxy Clusters. , archivePrefix = "arXiv", eprint =. doi:10.1146/annurev-astro-081710-102514 , adsurl =

    work page doi:10.1146/annurev-astro-081710-102514

  76. [76]

    Journal of Astrophysics and Astronomy , archivePrefix = "arXiv", eprint =

    Radio Band Observations of Blazar Variability. Journal of Astrophysics and Astronomy , archivePrefix = "arXiv", eprint =. doi:10.1007/s12036-011-9025-4 , adsurl =

    work page doi:10.1007/s12036-011-9025-4

  77. [77]

    , keywords =

    The evolution of galaxies in radio-selected groups. , keywords =. doi:10.1086/172305 , adsurl =

    work page doi:10.1086/172305

  78. [78]

    , keywords =

    Observational future of cosmological scalar-tensor theories. , keywords =. doi:10.1103/PhysRevD.95.063502 , archivePrefix =. 1610.09290 , primaryClass =

    work page doi:10.1103/physrevd.95.063502

  79. [79]

    A unified pseudo-$C_\ell$ framework

    A unified pseudo-C _ framework. , keywords =. doi:10.1093/mnras/stz093 , archivePrefix =. 1809.09603 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1093/mnras/stz093

  80. [80]

    ALMA Observations of Asteroid 3 Juno at 60 Kilometer Resolution

    The 2014 ALMA Long Baseline Campaign: Observations of Asteroid 3 Juno at 60 Kilometer Resolution. , keywords =. doi:10.1088/2041-8205/808/1/L2 , archivePrefix =. 1503.02650 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/2041-8205/808/1/l2 2014

Showing first 80 references.