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tSZ candidate detection/catolog construction is not noise-aware and is insufficiently specified. The catalog uses a single global threshold ν = (y_peak − \bar{y})/σ_y (Eq. (3), Sec. III.A) despite explicitly strong spatial noise inhomogeneity in the NILC y map (σ_y^local varies by ~3; Sec. IV.A/Fig. 6). This makes “≥5σ” position-dependent and undermines interpretation of candidate counts, ν-distributions, morphology statistics of the “50 brightest,” and any inferred rarity (Secs. III.C–III.D, IV, VIII, XI–XII). In addition, the relationship between the reported 4194 >5σ peaks at 2′ smoothing (Sec. III.B) and the final 200-candidate ≥5σ catalog (Sec. III.C) is unclear (changes in smoothing scale, masking, peak merging, connected-component rules, edge handling, etc.). The text/captions also sometimes describe the smoothing-scale search as “matched filtering,” which it is not in the standard tSZ sense (Secs. III.B–III.C; Fig. 1).
Recommendation: Make the detection pipeline both reproducible and interpretable under inhomogeneous noise. Concretely: (i) define a local-noise significance ν_local using the σ_y^local map already computed in Sec. IV.A (same grid/resolution), and provide both ν_global and ν_local per object; (ii) explicitly list every step that maps the initial peak list to the final 200 (smoothing scale used for the published catalog; peak-finding method; connected-component definition; minimum area; deblending/merging radius; masking; edge cuts); (iii) quantify how candidate density depends on σ_y^local (or declination / distance to edges) and provide at least a coarse purity/completeness estimate via injections into representative low- and high-noise regions; (iv) rephrase “matched filter” as “Gaussian smoothing” unless a true matched filter (beam+template+noise PSD weighting) is implemented, and ensure Fig. 1/captions match the actual method.
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Multi-frequency spectral diagnostics (Secs. V.A–V.C, Table V) rely on single-pixel values in raw f090/f150/f220 maps without beam matching, consistent filtering/transfer functions, aperture photometry/background subtraction, or split-based uncertainties. Despite this, the manuscript draws quantitative-sounding conclusions (e.g., “only 1–2/20 show classical tSZ behavior,” most are foreground dominated) that are not supported by single-pixel, mismatched-resolution measurements in a CMB+foreground+anisotropic-noise field (Secs. V, XI–XIII).
Recommendation: Either strengthen Sec. V into a minimal but defensible photometric analysis or downscope the claims. Preferred: convolve all three frequency maps to a common beam (worst resolution), apply consistent filtering (or explicitly justify differences), and perform aperture photometry or matched-filter flux extraction at candidate positions with local annular background subtraction; use split maps to estimate per-band uncertainties and propagate them to spectral ratios (including covariances where relevant). Include bandpass/units details (µK_CMB; effective band centers; expected tSZ null not exactly at nominal 220) and show how many candidates are consistent with a tSZ SED within errors. If this is beyond scope, recast the section as qualitative “foreground complexity at candidate positions,” remove/soften hard fractions like “2/20,” and add uncertainty estimates that demonstrate the classification is not robust.
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The highlighted compact feature at (RA, Dec) ≈ (291.2°, −29.2°) (Sec. VI) is interpreted as synchrotron-like (α≈−0.4) yet very high-significance in Compton‑y (≈41σ), but the measurements are under-specified and lack uncertainty quantification and basic external validation. It is currently unclear (i) how α is estimated (single pixel vs aperture; whether f220 is included), (ii) whether the feature is stable in map splits, and (iii) whether it coincides with known radio/X-ray/optical/SZ sources. Given NILC’s sensitivity to foreground leakage/weighting, a radio source can plausibly bias a y reconstruction without being a true tSZ detection (Secs. VI.A–VI.C, XII.A, XIII).
Recommendation: Turn Sec. VI into a minimal, robust validation case study. Specify the photometric method (beam-homogenized aperture or matched-filter fluxes at f090/f150/f220 with background subtraction), fit α using all relevant bands, and report fluxes/temperatures and α with uncertainties (add error bars to Fig. 13). Repeat the measurement on independent splits (set0/set1 or equivalent) to demonstrate stability of both the y detection and the SED. Perform a basic cross-match (even a simple cone search) against appropriate radio catalogs (e.g., SUMSS/NVSS/PMN/AT20G depending on declination), major SZ catalogs (official ACT DR6; Planck; SPT), and X-ray catalogs (ROSAT/eROSITA if available), and report matches/non-matches explicitly. Based on these checks, adjust the language: either present it as a confirmed known system (cluster+radio AGN), or clearly label it as an exploratory “foreground/NILC-leakage flag” rather than a likely novel SZ+synchrotron object.
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Non-Gaussianity and “anomaly” claims (kurtosis, low-correlation cells, spectral outliers, morphology outliers) lack adequate null models, preprocessing detail, uncertainties, and consistent multiple-testing treatment. The kurtosis result κ≈47 in f150 (Sec. VII.A) is compared to overly simplified Gaussian-noise simulations (“>100σ”), which is not an appropriate null for ACT temperature maps that contain CMB fluctuations, foregrounds, anisotropic/correlated noise, and filtering/transfer-function effects. Similarly, outlier classes—four low f090–f150 correlation cells (Sec. VII.C), “spectral ratio outliers” (Sec. V.C), and five morphology profile outliers (Sec. VIII)—are flagged without p-values under an explicit null, error bars on the metrics, or a look-elsewhere correction consistently applied (Secs. XI–XII). There is also an internal inconsistency in the multiple-testing discussion (11 vs 12 analyses; Secs. XI and XII.B).
Recommendation: For Sec. VII.A, document preprocessing step-by-step (masking/apodization; monopole/gradient removal; beam smoothing; any filtering; handling of masked pixels/edges; patch-selection scheme for 2000×2000 pixel patches), and calibrate κ against a realistic baseline (at minimum: lensed CMB + anisotropic noise consistent with splits; ideally also point sources/foreground residuals or apply a point-source mask and state it). Report κ with uncertainty (across patches) and show robustness to masking choices. For Secs. V.C, VII.C, VIII: define explicit null hypotheses and compute per-test p-values (via simulations or analytic approximations), include uncertainties on each statistic (spectral ratios, Pearson ρ per cell, morphology metrics), and then apply a clearly defined trials correction using a single, consistent N (list which analyses count toward it). Summarize per-test and global (post-trials) significance in a compact table in Sec. XI or XII.B, and reframe items that do not survive corrections as exploratory “flags.”
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Large-scale / harmonic-space methods are not sufficiently documented for reproducibility or for judging reliability on a partial CAR footprint. This affects (i) the hemispherical power ratio test (Sec. VII.B) at very low multipoles (e.g., 2 ≤ ℓ ≤ 50) where ACT map filtering/transfer functions and cut-sky mode coupling can be important, and (ii) the cross-frequency coherence analysis and associated “scale-cut recommendations” (Sec. IX, Table IV), which are largely deferred to an internal report [23] without enough details to reproduce or assess (masks and f_sky, estimator type, beam/calibration treatment, noise debiasing, ℓ-binning, covariance estimation, null tests).
Recommendation: Add a concise but complete methods description in Secs. VII.B and IX. For hemispherical asymmetry: specify the exact sky regions/declination cuts, masks, apodization, pseudo-Cℓ/MASTER (or alternative) estimator, mode-coupling correction, transfer-function/beam treatment, binning, and how uncertainties are obtained (splits vs sims). Justify the inclusion of ℓ ≤ 50 for these map products or restrict to a validated ℓ-range. For coherence (Sec. IX): describe preprocessing, the spectra used (cross-spectra between splits vs auto-spectra), noise debiasing, beam/calibration handling, binning, and uncertainties; state whether [23] is public, and if not, ensure Sec. IX alone is sufficient to reproduce Table IV. Rephrase “recommended scale cuts” as either diagnostic suggestions or analysis requirements, but make that distinction explicit in Sec. XII.C and the Conclusions.
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Several null/consistency-test claims are currently under-defined or potentially overstated, particularly those framed as constraints. The cosmic birefringence bound |β|<0.01° (Sec. X.B; Eq. (5)) is presented without the explicit TB/EB-to-β estimator equations, weighting, sign conventions, ℓ-range/binning, E/B purification and mode-coupling corrections, or inclusion of instrument polarization-angle systematics—details essential to assess whether such a tight bound is realistic for the dataset. Similarly, the “isocurvature limits” based on TB/EB consistency with zero (Sec. X.C) are not connected to a defined isocurvature parameter/model, and the rSZ–y sign-consistency discussion (Sec. X.E) is largely qualitative.
Recommendation: In Sec. X.B, provide the explicit small-angle rotation relations and the exact estimator used to infer β from Cℓ^{EB} and/or Cℓ^{TB}, including ℓ-weighting/bandpower combination, sign conventions for Q/U→E/B, and treatment of masks/mode coupling (and whether E/B purification is used). State which systematics are included in the β uncertainty (especially polarization-angle calibration and leakage). In Sec. X.C, either reframe as a parity/null test (preferred given current content) or introduce a specific isocurvature model and show how TB/EB map to a parameter constraint. In Sec. X.E, quantify the rSZ–y check (e.g., pixel-wise or patch-wise correlation coefficients; dependence on y S/N; association with NILC weights/foreground templates) and provide at least one summary plot/table beyond anecdotal regions.
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Reproducibility-critical numerical/coordinate and figure/caption inconsistencies are present. Most urgently, Table III lists declinations outside the physical range (e.g., +166.3°, +173.8°), which invalidates follow-up of the Sec. VIII morphology outliers. There are also smaller inconsistencies (e.g., Bullet Cluster ν quoted with different rounding across sections; unclear identification of the νmax=51.2σ object; ratio-definition flips between T90/T150 and T150/T090), and at least one figure/caption mismatch (Fig. 1 labeled as matched-filter optimization though Gaussian smoothing is used; mention of missing panels).
Recommendation: Perform a full audit of tables, coordinates, and repeated numeric claims (Secs. III–IV, VI, VIII, XI–XIII). Correct Table III positions and clearly state the coordinate system/epoch (e.g., ICRS/J2000 RA/Dec in degrees). Ensure the νmax object is identified by catalog ID and coordinates in Secs. XII–XIII. Harmonize ratio definitions and sign/inequality interpretations across Sec. V and related figures. Fix figure completeness and ensure captions exactly match what is plotted and the method actually used (e.g., rename “matched filter” to “Gaussian smoothing” unless upgraded).