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Improved Constraints on Primordial Gravitational Waves using Planck , WMAP, and BICEP/ Keck Observations through the 2018 Observing Season
Open accessAbstract
We present results from an analysis of all data taken by the BICEP2, Keck Array, and BICEP3 CMB polarization experiments up to and including the 2018 observing season. We add additional Keck Array observations at 220 GHz and BICEP3 observations at 95 GHz to the previous 95/150/220 GHz dataset. The Q/U maps now reach depths of 2.8, 2.8, and 8.8 μK_{CMB} arcmin at 95, 150, and 220 GHz, respectively, over an effective area of ≈600 square degrees at 95 GHz and ≈400 square degrees at 150 and 220 GHz. The 220 GHz maps now achieve a signal-to-noise ratio on polarized dust emission exceeding that of Planck at 353 GHz. We take auto- and cross-spectra between these maps and publicly available WMAP and Planck maps at frequencies from 23 to 353 GHz and evaluate the joint likelihood of the spectra versus a multicomponent model of lensed ΛCDM+r+dust+synchrotron+noise. The foreground model has seven parameters, and no longer requires a prior on the frequency spectral index of the dust emission taken from measurements on other regions of the sky. This model is an adequate description of the data at the current noise levels. The likelihood analysis yields the constraint r_{0.05}<0.036 at 95% confidence. Running maximum likelihood search on simulations we obtain unbiased results and find that σ(r)=0.009. These are the strongest constraints to date on primordial gravitational waves.
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TL;DR
The BICEP/Keck collaboration analyzed all BICEP2, Keck Array, and BICEP3 CMB polarization data through the 2018 observing season, combined with WMAP and Planck maps, to constrain primordial gravitational waves. They report the strongest limit to date, \(r_{0.05}<0.036\) at 95% confidence, with no significant evidence for \(r>0\).
Key findings
- The baseline likelihood gives \(r_{0.05}=0.014^{+0.010}_{-0.011}\) and \(r_{0.05}<0.036\) at 95% confidence; simulations give \(\sigma(r)=0.009\) and a median 95% upper limit of \(r_{0.05}<0.019\).
- Foreground parameters: \(A_{d,353}=4.4^{+0.8}_{-0.7}\,\mu\mathrm{K}^2\), \(A_{\mathrm{sync},23}<1.4\,\mu\mathrm{K}^2\) at 95% confidence, and \(\beta_d=1.49^{+0.13}_{-0.12}\); the synchrotron amplitude now peaks at zero.
- New maps reach depths of 2.8, 2.8, and 8.8 \(\mu\mathrm{K}_{\mathrm{cmb}}\,\mathrm{arcmin}\) at 95, 150, and 220 GHz over effective areas of \(\approx 600\) square degrees at 95 GHz and \(\approx 400\) square degrees at 150 and 220 GHz.
- The 220 GHz maps achieve signal-to-noise on polarized dust emission exceeding that of Planck at 353 GHz; the maximum-likelihood model has PTE 0.94, and the previous limits improved from \(r_{0.05}<0.12\) (BKP) to \(<0.09\) (BK14) to \(<0.07\) (BK15) to \(<0.036\) (BK18).
Methods
- Analysis of BICEP2, Keck Array, and BICEP3 CMB polarization data through the 2018 observing season, adding Keck 220 GHz and BICEP3 95 GHz data to the previous 95/150/220 GHz dataset; maps are made into Q/U, purified to B-modes, apodized, Fourier transformed, and used to form auto- and cross-spectra.
- Joint likelihood uses 66 BB auto- and cross-spectra between BICEP/Keck maps and WMAP 23/33 GHz plus Planck 30, 44, 143, 217, and 353 GHz maps, over \(20<\ell<330\) with 9 bandpowers per spectrum.
- The model is lensed \(\Lambda\)CDM + \(r\) + dust + synchrotron + noise with eight parameters, evaluated with Hamimeche-Lewis likelihood and CosmoMC MCMC; the dust frequency spectral index prior is removed, and the bandpower covariance matrix comes from 499 signal-and-noise simulations.
Limitations
- The paper states that dust decorrelation and foreground complexity more generally “will remain a serious concern” as sensitivity improves, and that the sample variance of the lensing component already dominates \(\sigma(r)\).
- The paper states that the baseline does not allow the dust decorrelation parameter \(\Delta_d\) to vary freely because it is biasing with respect to \(r\); it also notes that including EE spectra assumes an exact EE/BB ratio of 2 and “should not be overinterpreted.”
- The paper states residual uncertainties from point-source polarized flux may yield an upward bias on \(r\) of \(1-3\times10^{-3}\), and noise-bias imperfections may yield a downward bias of \(2\times10^{-3}\); these are subdominant to the statistical uncertainty.
- Evident from the text: the analysis fixes the tensor spectral index \(n_t=0\), assumes a power-law dust spatial spectrum and Gaussian dust fluctuations, and relies on external WMAP/Planck data for foreground separation.
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89 Own result · 32 Sources not found · 16 Own method · 10 No basis given · 8 Own interpretation
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“The BK18 result described in this letter, r 0 . 05 < 0 . 036, represents a fractional improvement equivalent to the two previous steps combined.”
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“This model is an adequate description of the data at the current noise levels.”
- Also stated in: § BICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck , WMAP, and BICEP/ Keck Observations through the 2018 Observing Season · p. 4 · plain
“This model is an acceptable fit to the data with the probability to exceed (PTE) the observed value of χ 2 being 0.94.”
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- The authors state this as an assumption: The synchrotron frequency spectrum is a simple power law A_sync ∝ ν^β_s.
- The authors state this as an assumption: The dust spatial power spectrum is a power law D_ℓ ∝ ℓ^α_d.
- The authors state this as an assumption: The synchrotron spatial power spectrum is a power law D_ℓ ∝ ℓ^α_s.
- Also stated in: § BICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck , WMAP, and BICEP/ Keck Observations through the 2018 Observing Season · p. 4 · plain
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“The 220GHz maps now achieve a signal-to-noise on polarized dust emission exceeding that of Planck at 353 GHz.”
- Also stated in: § BICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck , WMAP, and BICEP/ Keck Observations through the 2018 Observing Season · p. 6 · plain
“The signal-to-noise on polarized dust emission of our 220 GHz band is now considerably higher than that of the Planck 353 GHz band-i.e. the 220 × 220 noise point is much further below the dust band than the P353 × P353 point.”
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- Also stated in: § BICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck , WMAP, and BICEP/ Keck Observations through the 2018 Observing Season · p. 6 · plain
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“For r , the zero-to-peak likelihood ratio is 0.46.”
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“The likelihood analysis yields the constraint r 0 . 05 < 0 . 036 at 95% confidence.”
- Also stated in: § BICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck , WMAP, and BICEP/ Keck Observations through the 2018 Observing Season · p. 1 · plain
“r 0 . 05 < 0 . 036 at 95% confidence”
- Also stated in: § ACKNOWLEDGMENTS · p. 7 · plain
“The upper limit on the tensor-to-scalar ratio tightens to r 0 . 05 < 0 . 036 at 95% confidence.”
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- Also stated in: § BICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck , WMAP, and BICEP/ Keck Observations through the 2018 Observing Season · p. 1 · plain
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“r 0 . 05 = 0 . 014 +0 . 010 -0 . 011 ( r 0 . 05 < 0 . 036 at 95% confidence)”
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“A sync , 23 < 1 . 4 µ K 2 at 95% confidence”
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“and that the data do not prefer allowing decorrelation of the dust pattern in the model.”
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“The maximum likelihood model has parameters r 0 . 05 = 0 . 011, A d , 353 = 4 . 4 µ K 2 , A sync , 23 = 0 . 6 µ K 2 , β d = 1 . 5, β s = -3 . 0, α d = -0 . 66, α s = 0 . 00, and ϵ = -0 . 11.”
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- The authors state this as an assumption: The synchrotron frequency spectrum is a simple power law A_sync ∝ ν^β_s.
- The authors state this as an assumption: The dust spatial power spectrum is a power law D_ℓ ∝ ℓ^α_d.
- The authors state this as an assumption: The synchrotron spatial power spectrum is a power law D_ℓ ∝ ℓ^α_s.
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“Running without foreground parameters on simulations which contain neither lensing or dust gives σ ( r 0 . 05 ) = 0 . 002.”
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“This model is an acceptable fit to the data with the probability to exceed (PTE) the observed value of χ 2 being 0.94.”
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- The authors state this as an assumption: The synchrotron frequency spectrum is a simple power law A_sync ∝ ν^β_s.
- The authors state this as an assumption: The dust spatial power spectrum is a power law D_ℓ ∝ ℓ^α_d.
- The authors state this as an assumption: The synchrotron spatial power spectrum is a power law D_ℓ ∝ ℓ^α_s.
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“The BK18 simulations have a median 95% upper limit of r 0 . 05 < 0 . 019.”
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“The model plotted is a 'baseline' lensed-ΛCDM+dust model from our previous BK15 analysis, which remains a good description of the data.”
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“while running without foreground parameters on simulations which contain no dust gives σ ( r 0 . 05 ) = 0 . 007.”
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“β d = 1 . 49 +0 . 13 -0 . 12”
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“we estimate that the probability to get a likelihood ratio smaller than this is 11% if, in fact, r = 0.”
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“Figure 2 shows that the BK18 data is consistent with ΛCDM plus a remarkably simple dust only foreground model.”
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“Comparing this plot to Fig. 2 of BK15 we can see that the uncertainties are dramatically reduced for the autoand cross-spectra of the 95 and 220GHz bands.”
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“A d , 353 = 4 . 4 +0 . 8 -0 . 7 µ K 2”
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“Running the baseline BK18 analysis on simulations which contain no lensing B -modes gives σ ( r 0 . 05 ) = 0 . 004”
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“In the initial pass of the jackknife analysis there were a few χ 2 and χ values sitting sufficiently beyond the tails of the simulation distributions that it was unlikely to happen by chance.”
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“In addition the synchrotron amplitude constraint A sync shifts down to peak at zero.”
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- The authors state this as an assumption: The power spectrum of the polarized dust emission in the BICEP/Keck field follows a power law.
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“With β d now free, the Planck 353 GHz band provides a significant part of the β d constraint (red curve wider than black in the rightmost panel).”
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“The constraint on r tightens from r 0 . 05 < 0 . 11 to r 0 . 05 < 0 . 035.”
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“It appears that there is some tension between the WMAP bands (23 and 33 GHz) and the LFI bands (30 and 44 GHz) in terms of their cross correlation with the BICEP/ Keck maps.”
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“In contrast to Fig. 21 of BK15 the ∆ d curve peaks at unity (no decorrelation).”
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“Unsurprisingly dropping both WMAP and LFI results in a highly degraded constraint on A sync (cyan).”
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“The reduction of 0.3 for the real data offers no significant evidence for detection of decorrelation.”
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“The mean of simulations responds exactly as the sum of the ' -sync' and ' -r ' cases.”
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“With the improved sensitivity of BK18 the constraint becomes β d = 1 . 49 +0 . 13 -0 . 12 .”
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“Fixing r = 0 results in an increase of 1.0 for the mean of simulations (which have r = 0).”
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“The predicted lensing BB spectrum for the Planck 2018 baseline cosmological parameters [2, Table 2] has shifted down by 5% (for ℓ < 500).”
What the sources say
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“At 150 and 220 GHz the B maps are dominated by polarized dust emission.”
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“The increase for the real data is 0.6 indicating no significant evidence for r > 0.”
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“Through a long process we determined that removing two small sub-sets of data moved these values in such that there were no longer clear problems.”
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“The results are shown in Fig. 16-the resulting CMB values are consistent with lensed-ΛCDM while the dust values are consistent with the level of dust found in the baseline analysis.”
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“The upper part of Fig. 13 compares the two BB spectra-the large improvement in sensitivity is clear.”
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“In Fig. 17 dropping the β d prior corresponds to the transition from yellow to red curvesr and A sync show very little change while A d gets just slightly wider.”
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“The results are shown in Fig. 16-the resulting CMB values are consistent with lensed-ΛCDM while the dust values are consistent with the level of dust found in the baseline analysis.”
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“By doing this we also include the small additional constraining power on r which comes from the Planck TT,TE,EE+lowE+lensing likelihood.”
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“We show that, for all 8 parameters that we fit for in our maximum likelihood framework, the expected biases are low and within statistical uncertainties.”
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“We compute the realization-to-realization shift in the likelihood peak and found none of the shifts observed in real data for r and dust parameters to be statistically significant compared to random fluctuations in simulations.”
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In the paper
“Beam simulations with crosstalk deprojected (as described in Ref. [34]) show that the contribution to ∆( r ) from crosstalk is small.”
What the sources say
- Not matchedcites [34]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
plain- Asserted: passes — The authors put it forward as true.
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- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
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- Not matched
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“The + A L -ϵ case shows no preference for varying the lensing scale factor away from unity for either the real data (as expected given the results in Fig. 19 above) or the simulations.”
plain- Asserted: passes — The authors put it forward as true.
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- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
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A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“If we fix the lensing spectrum rescale factor A BB L = 0 . 5 we see very large increases in -2 log( L ) for simulations and data indicating strong incompatibility with such a model.”
boosteddirect- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
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None of the sources cited for this claim could be matched to a paper in Crossref, so there is nothing to check it against.
In the paper
“The MHD model [59, 60] is also unchanged from BK15 and has a level of synchrotron which is now in strong conflict with the data.”
What the sources say
- Not matchedcites [59]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- Not matchedcites [60]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
boostedcorrelational- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
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- Not matched
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“Compared to the BK18 baseline, the shift in the 95% upper limit on r due to the addition of these nuisance parameters is 3 × 10 -5 , negligible compared to the statistical uncertainty.”
plain- Asserted: passes — The authors put it forward as true.
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A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“We consider various sources of uncertainty in these measurements and estimate them to be small, at the 1% level or less.”
hedged- Asserted: passes — The authors put it forward as true.
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A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“Likewise setting A d , 353 = 2 µ K 2 is strongly incompatible with the simulations and data.”
boosted- Asserted: passes — The authors put it forward as true.
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- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
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A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“In particular, we show that the worst case scenario would result in a bias on r of | ∆( r ) | = 8 . 4 ± 5 × 10 -4 , well below the statistical uncertainty σ ( r ) = 0 . 009”
hedgeddirect- Asserted: passes — The authors put it forward as true.
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A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“However, in practice the third line of the table shows no detectable bias.”
plain- Asserted: passes — The authors put it forward as true.
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- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
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A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“Compared to BK15 results, the reduction in T → P bias (∆( r ) = 2 . 7 ± 1 . 9 × 10 -3 → 1 . 5 ± 1 . 1 × 10 -3 ) nearly matches the reduction in statistical uncertainty ( σ ( r ) = 0 . 020 → 0 . 009).”
plaincorrelational- Asserted: passes — The authors put it forward as true.
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A conclusion the paper draws from its own results — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“In addition, we are already in the regime where the sample variance of the lensing component dominates σ ( r ).”
plaindirect- Asserted: passes — The authors put it forward as true.
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In the paper
“In Ref. [11, hereafter BK14] we improved the constraint using Keck Array data at 95 GHz taken during the 2014 season”
What the sources say
- Not matchedcites [11]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
plaindirect- Asserted: passes — The authors put it forward as true.
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- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
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- Not matched
What the paper did — it cites no source for this, so there is none to check. The quote shows it is in the paper.
In the paper
“Running maximum likelihood search on simulations we obtain unbiased results and find that σ ( r ) = 0 . 009.”
- Also stated in: § BICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck , WMAP, and BICEP/ Keck Observations through the 2018 Observing Season · p. 4 · plain
“In Appendix E 3 we verify that the likelihood analysis is unbiased”
plain- Asserted: passes — The authors put it forward as true.
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- Also stated in: § BICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck , WMAP, and BICEP/ Keck Observations through the 2018 Observing Season · p. 4 · plain
In the paper
“we have recently demonstrated a path forward by adding a 'lensing template' derived from SPTpol and Planck data to the BK14 analysis, resulting in an improved constraint on r [49].”
What the sources say
- Not matchedcites [49]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
boosteddirect- Asserted: passes — The authors put it forward as true.
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- Not matched
In the paper
“and in Ref. [12, hereafter BK15] we improved again adding Keck Array data at 95 GHz and 220 GHz taken during the 2015 season.”
What the sources say
- Not matchedcites [12]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
plaindirect- Asserted: passes — The authors put it forward as true.
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- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
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- Not matched
In the paper
“Inflation makes an additional prediction which has not yet been observed-a background of tensor perturbations, also known as gravitational waves (see Ref. [3] for a review and citations to the original literature).”
What the sources say
- Not matchedcites [3]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
plaindirect- Asserted: passes — The authors put it forward as true.
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- Load-bearing: passes — The paper’s conclusions depend on it.
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- Not matched
A conclusion the paper draws from its own results — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“These are the strongest constraints to date on primordial gravitational waves.”
plain- Asserted: passes — The authors put it forward as true.
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What the paper did — it cites no source for this, so there is none to check. The quote shows it is in the paper.
In the paper
“In Appendix E2 we vary the baseline analysis choices and data selection, finding that these do not significantly alter the results”
plain- Asserted: passes — The authors put it forward as true.
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The paper states this without a source or data behind it here, so there is nothing to check it against. The quote shows it is in the paper.
In the paper
“However, the lensing B -modes can be spatially separated from a primordial component”
plaindirect- Asserted: passes — The authors put it forward as true.
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What the paper did — it cites no source for this, so there is none to check. The quote shows it is in the paper.
In the paper
“The agreement with the spectra involving 95 GHz and all the EE spectra (under the assumption that EE/BB = 2 for dust) is therefore a validation of the model.”
plaindirect- Asserted: passes — The authors put it forward as true.
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- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
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- The authors state this as an assumption: For dust, EE/BB = 2.
In the paper
“The Planck 2018 dust analysis [24] did not show any evidence for dust decorrelation.”
What the sources say
- Not matchedcites [24]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
plain- Asserted: passes — The authors put it forward as true.
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- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
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- Not matched
What the paper did — it cites no source for this, so there is none to check. The quote shows it is in the paper.
In the paper
“In addition we found it necessary to remove BICEP3 data from focal plane tile 1 in order to pass the tile jackknife.”
plaindirect- Asserted: passes — The authors put it forward as true.
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In the paper
“in BK15 it was found that allowing ∆ d to vary freely resulted in 72% of the r curves peaking at zero in simulations where there was no decorrelation.”
What the sources say
- Not matchedcites BK15
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
plaindirect- Asserted: passes — The authors put it forward as true.
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- Not matched
In the paper
“and that Ref. [31] analyzed the S-PASS and WMAP 23GHz data and found β s = -3 . 22 ± 0 . 06 in the BICEP2 sky patch.”
What the sources say
- Not matchedcites [31]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
plain- Asserted: passes — The authors put it forward as true.
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- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
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- Not matched
What the paper did — it cites no source for this, so there is none to check. The quote shows it is in the paper.
In the paper
“The lower panel again shows no evidence for inconsistency between the two spectra.”
plain- Asserted: passes — The authors put it forward as true.
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- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
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A conclusion the paper draws from its own results — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“The parametric model which we are using, including the approximation of Gaussian fluctuation of the dust (and synchrotron) sky patterns, remains an adequate description of the presently available data.”
plain- Asserted: passes — The authors put it forward as true.
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- The authors state this as an assumption: The dust and synchrotron sky patterns have Gaussian fluctuations.
What the paper did — it cites no source for this, so there is none to check. The quote shows it is in the paper.
In the paper
“However, we found evidence for failure of the season split jackknife when including this data which lead us to exclude it.”
plaindirect- Asserted: passes — The authors put it forward as true.
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- Load-bearing: passes — The paper’s conclusions depend on it.
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What the paper did — it cites no source for this, so there is none to check. The quote shows it is in the paper.
In the paper
“The lower part of the figure shows that this (not very stringent) test is passed.”
plain- Asserted: passes — The authors put it forward as true.
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- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
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What the paper did — it cites no source for this, so there is none to check. The quote shows it is in the paper.
In the paper
“We also make decorrelated simulations according to our parameterization of decorrelation, and these are thus also expected to give unbiased results when re-fit with that extension to the parameterization-as we see they do in the second line of the table.”
plain- Asserted: passes — The authors put it forward as true.
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A conclusion the paper draws from its own results — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“Given the importance of multi-frequency component separation to the current result, the most important non-additive systematic effect is spectral bandpass uncertainty.”
plain- Asserted: passes — The authors put it forward as true.
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- Load-bearing: passes — The paper’s conclusions depend on it.
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What the paper did — it cites no source for this, so there is none to check. The quote shows it is in the paper.
In the paper
“Our basic set of simulations includes Gaussian realizations of dust generated according to the parametric model which we use when re-fitting, and these are thus expected and to give unbiased results-as we see they do in the first row of the table.”
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
- It may state two separate claims as one. 53
- Probably not a substantial claim. 34
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“Running maximum likelihood search on simulations we obtain unbiased results and find that σ ( r ) = 0 . 009.”
- Also stated in: § BICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck , WMAP, and BICEP/ Keck Observations through the 2018 Observing Season · p. 5 · plain
“The distributions of maximum likelihood r values in simulations where the true value of r is zero gave σ ( r 0 . 05 ) = 0 . 020 for BK15 which is reduced to σ ( r 0 . 05 ) = 0 . 009 for BK18”
plaindirect- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
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It may state two separate claims as one.
- Also stated in: § BICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck , WMAP, and BICEP/ Keck Observations through the 2018 Observing Season · p. 5 · plain
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“The BK18 data shrinks the contours in the vertical ( r ) direction while the BAO data shrinks the contours in the horizontal ( n s ) direction and shifts the centroid slightly to the right.”
plaindirect- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“The Q/U maps now reach depths of 2.8, 2.8 and 8.8 µ K cmb arcmin at 95, 150 and 220 GHz respectively over an effective area of ≈ 600 square degrees at 95 GHz and ≈ 400 square degrees at 150 & 220GHz.”
plain- Asserted: passes — The authors put it forward as true.
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- Load-bearing: passes — The paper’s conclusions depend on it.
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It may state two separate claims as one.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“We also find that the value of A d is very similar when evaluated over the larger BICEP3 sky coverage region and the smaller BICEP2 / Keck sky region.”
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: fails — The paper’s conclusions may not depend on it.
- Based: passes — The paper gives a reason why it holds.
Probably not a substantial claim. The paper’s conclusions may not depend on it.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“This improves the constraint on primordial gravitational waves parameterized by the tensor-to-scalar ratio r by more than a factor of two over our previous result to r 0 . 05 < 0 . 036 at 95% confidence, setting important additional limits on inflationary models.”
plaindirect- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: passes — The paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“In the BK15 analysis the constraint on β d was prior dominated, but for BK18 we see that the data is able to constrain this parameter almost as well as the prior previously did.”
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“As compared to the previous BK15 analysis, the likelihood curve for r tightens considerably with the peak position shifting down slightly, and the A d curve tightens slightly.”
plaincorrelational- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: passes — The paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“Freeing the amplitude of the lensing power we obtain A BB L = 1 . 03 +0 . 08 -0 . 09 , and the r constraint hardly changes.”
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
In the paper
“Interestingly the peak value selected is very close to the mean value from Planck 2018 analysis of larger regions of sky β d = 1 . 53 [24].”
What the sources say
- Not matchedcites [24]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: fails — The paper’s conclusions may not depend on it.
- Based: passes — The paper gives a reason why it holds.
Probably not a substantial claim. The paper’s conclusions may not depend on it.
- Not matched
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“In addition the A sync curve now peaks at zero-the weak evidence for synchrotron we saw in BK15 is no longer present.”
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
The paper states this without a source or data behind it here, so there is nothing to check it against. The quote shows it is in the paper.
In the paper
“The 95GHz B map is approximately equal parts lensed-ΛCDM signal and noise.”
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: fails — The paper’s conclusions may not depend on it.
- Based: passes — The paper gives a reason why it holds.
Probably not a substantial claim. The paper’s conclusions may not depend on it.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“The increase of 1.5 for the real data is smaller than the average increase in the simulations indicating no evidence that synchrotron is present.”
hedged- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“With a uniform prior on A BB L (and marginalizing over all other parameters) we obtain A BB L = 1 . 03 +0 . 08 -0 . 09 showing no tension with ΛCDM.”
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“The r constraint hardly changes due to the fact that the lensing amplitude prefered by the BK18 data is very close to that predicted by the Planck 2018 cosmological parameters.”
plaindirect- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“In Fig. 17 switching to the updated Planck 2018 spectrum corresponds to the transition from red to black-the r constraint shifts slightly up indicating that this is a marginally relevant change at BK18 sensitivity levels.”
hedgeddirect- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
- The authors state this as an assumption: The power spectrum of the polarized dust emission in the BICEP/Keck field follows a power law.
The paper states this without a source or data behind it here, so there is nothing to check it against. The quote shows it is in the paper.
In the paper
“Due to the larger instantaneous field of view BICEP3 naturally maps a larger area of sky.”
plaindirect- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: fails — The paper’s conclusions may not depend on it.
- Based: passes — The paper gives a reason why it holds.
Probably not a substantial claim. The paper’s conclusions may not depend on it. It may state two separate claims as one.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“Removing synchrotron from the fit (i.e. fixing As = 0, β s = 0, α s = 0 and ϵ = 0) corresponds to a nominal reduction in the number of fit parameters of 4, but the increase in the mean -2 log( L ) for the simulations (which contain no synchrotron) suggests only 2.5 effective free parameters.”
hedgeddirect- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“For the 9 × 66 = 594 bandpowers shown in Fig. 15, χ 2 = ( d -m ) T C -1 ( d -m ) = 541 . 6, where d are the bandpower values, m are the model expectation values, and C is the bandpower covariance matrix for the maximum likelihood model. This has a PTE versus the simulations of 0 . 94.”
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“The effects are similar to those seen in BK15-the r peak position shifts up, the A d curve narrows, and the A sync curve peaks strongly away from zero.”
plaindirect- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
- The authors state this as an assumption: The EE/BB ratios for dust and synchrotron are both exactly 2.
The paper states this without a source or data behind it here, so there is nothing to check it against. The quote shows it is in the paper.
In the paper
“The χ 2 and χ jackknife statistics do not actually have the nominal theory distributions since they are summations of bandpower values which are themselves χ 2 rather than Gaussian distributed.”
plaindirect- Asserted: passes — The authors put it forward as true.
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- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“However, at 220 GHz we start to see dust contamination become comparable in amplitude to the ΛCDM E -modes at the edges of the field.”
plaincorrelational- Asserted: passes — The authors put it forward as true.
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Probably not a substantial claim. The paper’s conclusions may not depend on it.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“Interestingly the peak position of A d only shifts a very small amount under these variations showing no evidence for variation of the polarized dust amplitude as averaged across the BICEP3 coverage pattern versus the subset BICEP2 / Keck fi eld.”
plain- Asserted: passes — The authors put it forward as true.
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It may state two separate claims as one.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“In Fig. 17 dropping the β d prior corresponds to the transition from yellow to red curvesr and A sync show very little change while A d gets just slightly wider.”
plain- Asserted: passes — The authors put it forward as true.
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It may state two separate claims as one.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“As seen in Figures 8 and 9 the BICEP3 sky coverage is larger than the BICEP2 / Keck region.”
plain- Asserted: passes — The authors put it forward as true.
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Probably not a substantial claim. The paper’s conclusions may not depend on it.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“If instead we take the sum of the normalized deviations χ = ∑ (( d -m ) /e ) where e is the square-root of the diagonal of C , we find that the PTE versus the simulations is 0.22.”
plain- Asserted: passes — The authors put it forward as true.
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Probably not a substantial claim. The paper’s conclusions may not depend on it.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“In a simple study we find this to be 2.2% within the multipole range 20 < ℓ < 500 (with a distribution close to Gaussian).”
plaindirect- Asserted: passes — The authors put it forward as true.
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It may state two separate claims as one.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“The upper part of Fig. 14 compares the two BB spectra-a large improvement in sensitivity is again clear, and the BK18 220 GHz spectrum is sample variance limited out to ℓ ∼ 200.”
plain- Asserted: passes — The authors put it forward as true.
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Probably not a substantial claim. The paper’s conclusions may not depend on it.
The paper states this without a source or data behind it here, so there is nothing to check it against. The quote shows it is in the paper.
In the paper
“The E maps are dominated by ΛCDM signal, and hence are highly correlated across all three bands.”
plaincorrelational- Asserted: passes — The authors put it forward as true.
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- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
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It may state two separate claims as one.
The paper states this without a source or data behind it here, so there is nothing to check it against. The quote shows it is in the paper.
In the paper
“Comparing the three frequencies we see almost identical patterns in the T maps since ΛCDM signal is dominant.”
plaindirect- Asserted: passes — The authors put it forward as true.
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- Load-bearing: fails — The paper’s conclusions may not depend on it.
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Probably not a substantial claim. The paper’s conclusions may not depend on it.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“Dropping WMAP results in A sync peaking strongly at zero whereas dropping LFI results in A sync peaking well above zero.”
boosteddirect- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
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It may state two separate claims as one.
The paper states this without a source or data behind it here, so there is nothing to check it against. The quote shows it is in the paper.
In the paper
“Note that for the small field only version the A sync peak shifts above zero as it was in BK15.”
plain- Asserted: passes — The authors put it forward as true.
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Probably not a substantial claim. The paper’s conclusions may not depend on it.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“For Q and U the patterns are again extremely similar between 95 and 150 GHz, and dominated by the ΛCDM E -mode signal.”
plaincorrelational- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: fails — The paper’s conclusions may not depend on it.
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Probably not a substantial claim. The paper’s conclusions may not depend on it. It may state two separate claims as one.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“BICEP/ Keck alone (blue) constrains A sync and β d poorly with the r constraint peaking hard at zero.”
plain- Asserted: passes — The authors put it forward as true.
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- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
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It may state two separate claims as one.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“In Appendix D above we saw that the absolute goodness-of-fit of the baseline model to the data is adequate.”
plain- Asserted: passes — The authors put it forward as true.
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Probably not a substantial claim. The paper’s conclusions may not depend on it.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“We next switch from the BK15 data set to the BK18 one-i.e. including the improved sensitivity at 220 GHz and the improved sensitivity and sky area at 95 GHz (magenta to yellow). This makes a substantial difference: the r constraint narrows and its peak position shifts down.”
plaindirect- Asserted: passes — The authors put it forward as true.
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- Load-bearing: passes — The paper’s conclusions depend on it.
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It may state two separate claims as one.
- The authors state this as an assumption: The power spectrum of the polarized dust emission in the BICEP/Keck field follows a power law.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“Starting with the BK15 data set we first update the version of COSMOMC from Nov2016 to July2019 (green to magenta) which makes very little difference.”
plain- Asserted: passes — The authors put it forward as true.
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Probably not a substantial claim. The paper’s conclusions may not depend on it.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“Using different apodizations also in principle reduces the correlations of the auto- and cross-spectra which are key to the separation of foreground and CMB signals. However, in the current case the penalty turns out to be negligible.”
plain- Asserted: passes — The authors put it forward as true.
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Probably not a substantial claim. The paper’s conclusions may not depend on it.
In the paper
“Interestingly the peak value of β d = 1 . 50 selected by our data is close to the mean value from Planck 2018 analysis of larger regions of sky β P d = 1 . 53 ± 0 . 02 [24].”
What the sources say
- Not matchedcites [24]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: fails — The paper’s conclusions may not depend on it.
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Probably not a substantial claim. The paper’s conclusions may not depend on it.
- Not matched
The paper states this without a source or data behind it here, so there is nothing to check it against. The quote shows it is in the paper.
In the paper
“The two nominally 220 GHz receivers added before the 2015 season actually have passbands centered at ≈ 230 GHz, whereas the two added before the 2016 season have passbands centered at ≈ 220 GHz.”
plain- Asserted: passes — The authors put it forward as true.
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- Load-bearing: fails — The paper’s conclusions may not depend on it.
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Probably not a substantial claim. The paper’s conclusions may not depend on it. It may state two separate claims as one.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“We see that the r constraint shifts down slightly and the A sync constraint shifts up slightly.”
plaindirect- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“Allowing decorrelation parameter ∆ d to vary freely while fixing ϵ = 0 leaves the nominal number of parameters unchanged and as expected hardly changes the mean value of -2 log( L ) for the simulations.”
plain- Asserted: passes — The authors put it forward as true.
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- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
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It may state two separate claims as one.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“It is very interesting that dropping the 150 and 220 GHz bands does not substantially increase the width of the r constraint, although it is unsurprising that it does increase the widths of the A d and β d constraints.”
plaindirect- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
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It may state two separate claims as one.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“Synchrotron is tightly limited in all the multipole ranges, and not detected in any of them.”
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
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It may state two separate claims as one.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“Dropping the other HFI bands makes smaller additional changes (red to green).”
plaindirect- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: fails — The paper’s conclusions may not depend on it.
- Based: passes — The paper gives a reason why it holds.
Probably not a substantial claim. The paper’s conclusions may not depend on it.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“The shifts on dust parameters ( A d and β d ) are a few percent, and still within statistical uncertainty and upper bounds predicted using maximum likelihood searches on simulations.”
plaindirect- Asserted: passes — The authors put it forward as true.
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- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
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It may state two separate claims as one.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“We find that 60% of the simulations peak at zero, and 11% have a lower zero-to-peak ratio than the real data-i.e. show more evidence for r when the true value is in fact zero.”
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“They have A d in our sky region which is much greater that the actual level and this modestly increases σ ( r ), although interestingly by an amount that is fractionally less than the increase seen in BK15.”
plaindirect- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“Neither of these models produces detectable bias on r .”
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
In the paper
“The corresponding spectra for the Keck 95 GHz, 150 GHz and 220 GHz bands were found to be very similar to the BK15 results shown in Ref. [52].”
What the sources say
- Not matchedcites [52]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: fails — The paper’s conclusions may not depend on it.
- Based: passes — The paper gives a reason why it holds.
Probably not a substantial claim. The paper’s conclusions may not depend on it.
- Not matched
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“The real data shows an increase almost exactly equal to that in the mean of simulations-i.e. the data is perfectly compatible with the lensed-ΛCDM expectation plus the simple 3 parameter dust model.”
boostedn = 2- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: passes — The paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“The input values are recovered in the mean although formally there is a small bias detectable on A d .”
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
None of the sources cited for this claim could be matched to a paper in Crossref, so there is nothing to check it against.
In the paper
“More significant, but still subdominant for the current analysis, are uncertainties from the contributions of polarized flux from point sources in our field, which estimates suggest may yield an upward bias on r of 1-3 × 10 -3 [9, 64, and recent internal work], and imperfections in our noise bias estimates as they interact with leakage deprojection filtering, which recent preliminary work suggests”
What the sources say
- Not matchedcites [9]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- Not matchedcites [64]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
hedgedconditional- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
- Not matched
A result the paper reports from its own data — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“The recovered bias is ∆( r ) = 1 . 5 ± 1 . 1 × 10 -3 , which is subdominant compared to our statistical uncertainty σ ( r ) = 0 . 009.”
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: passes — The paper’s conclusions depend on it.
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It may state two separate claims as one.
In the paper
“In a joint analysis using multifrequency data from the Planck experiment it was shown that most or all of this is due to polarized emission from dust in our own galaxy [10, hereafter BKP].”
What the sources say
- Not matchedcites [10]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
plaindirect- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: passes — The paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
Probably not a substantial claim.
- Not matched
None of the sources cited for this claim could be matched to a paper in Crossref, so there is nothing to check it against.
In the paper
“As part of our standard data reduction we 'deproject' leading order temperature to polarization leakage [9, 34]-in Appendix F we quantify possible residual leakage and some other possible systematics.”
What the sources say
- Not matchedcites [9]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- Not matchedcites [34]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: passes — The paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
Probably not a substantial claim.
- Not matched
In the paper
“Our BICEP/ Keck program first reported detection of an excess over the lensing B -mode expectation at 150 GHz in Ref. [9].”
What the sources say
- Not matchedcites [9]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: fails — The paper’s conclusions may not depend on it.
- Based: passes — The paper gives a reason why it holds.
Probably not a substantial claim. The paper’s conclusions may not depend on it.
- Not matched
In the paper
“Under the ΛCDM standard model the CMB polarization pattern is mostly E -mode, with a much smaller B -mode component which arises due to gravitational deflections (lensing) of the CMB photons after their last scattering [5].”
What the sources say
- Not matchedcites [5]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
plaindirect- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: passes — The paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
- Not matched
None of the sources cited for this claim could be matched to a paper in Crossref, so there is nothing to check it against.
In the paper
“The EE spectra were not used to derive the model but agree well with it under the assumption that EE/BB = 2 for dust, as is known to be close to the case [23, 24].”
What the sources say
- Not matchedcites [23]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- Not matchedcites [24]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
boosted- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
- The authors state this as an assumption: For dust, EE/BB = 2.
- Not matched
In the paper
“At the South Pole the atmosphere is exceptionally transparent and stable at the observation frequencies [17, Fig. 5].”
What the sources say
- Not matchedcites [17, Fig. 5]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: fails — The paper’s conclusions may not depend on it.
- Based: passes — The paper gives a reason why it holds.
Probably not a substantial claim. The paper’s conclusions may not depend on it. It may state two separate claims as one.
- Not matched
What the paper did — it cites no source for this, so there is none to check. The quote shows it is in the paper.
In the paper
“To test for systematic contamination we carry out our usual 'jackknife' internal consistency (null) tests on the new 95GHz and 220GHz data as described in Appendices B and C.”
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: fails — The paper’s conclusions may not depend on it.
- Based: passes — The paper gives a reason why it holds.
Probably not a substantial claim. The paper’s conclusions may not depend on it.
None of the sources cited for this claim could be matched to a paper in Crossref, so there is nothing to check it against.
In the paper
“Planck analysis consistently finds approximate power law behavior of both the EE and BB dust spectra with exponents ≈ -0 . 4 [23, 24].”
What the sources say
- Not matchedcites [23]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- Not matchedcites [24]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
plaincorrelational- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: fails — The paper’s conclusions may not depend on it.
- Based: passes — The paper gives a reason why it holds.
Probably not a substantial claim. The paper’s conclusions may not depend on it.
- Not matched
None of the sources cited for this claim could be matched to a paper in Crossref, so there is nothing to check it against.
In the paper
“Since primordial gravitational waves will produce E -modes and B -modes approximately equally it was realized in the late 1990's that the best way to search for them is to look for an excess B -mode signal [6-8].”
What the sources say
- Not matchedcites [6]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- Not matchedcites [7]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- Not matchedcites [8]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
plaindirect- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: passes — The paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
- Not matched
In the paper
“(Using the S-PASS data [30] we estimate that the expectation is A sync , 23 ≈ 0 . 4 µ K 2 in the BICEP/ Keck fi eld, which is consistent with our A sync likelihood curve.)”
What the sources say
- Not matchedcites [30]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
hedgedcorrelational- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
- Not matched
A conclusion the paper draws from its own results — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“The φ 2 / 3 model now lies outside the 95% contour as does the band of natural inflation models.”
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: passes — The paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
In the paper
“If we can detect or set limits on primordial gravitational waves we can set limits on these models [4], and probe physics at energy scales far higher than can ever be accessed in laboratory experiments.”
What the sources say
- Not matchedcites [4]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
plaindirect- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: passes — The paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
- Not matched
In the paper
“This is an interesting result given the Planck 2018 TT,TE,EE+lowE result A L = 1 . 18 ± 0 . 065 [2, Eqn. 36b].”
What the sources say
- Not matchedcites [2]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: fails — The paper’s conclusions may not depend on it.
- Based: passes — The paper gives a reason why it holds.
Probably not a substantial claim. The paper’s conclusions may not depend on it.
- Not matched
A conclusion the paper draws from its own results — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“In addition in the right panel of Fig. 19 we see that there is very little degeneracy between r and A BB L implying that all one now needs from ΛCDM is the template shape of the lensing B -mode spectrum, and not the amplitude.”
plaincorrelational- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
What the paper did — it cites no source for this, so there is none to check. The quote shows it is in the paper.
In the paper
“We note that we did not look at the non-jackknife spectra until the above data removals had been done and the null tests determined to be satisfactory.”
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: fails — The paper’s conclusions may not depend on it.
- Based: passes — The paper gives a reason why it holds.
Probably not a substantial claim. The paper’s conclusions may not depend on it.
In the paper
“Recently Ref. [55] reported evidence for line-of-sight decorrelation in Planck data by using HI data to select sight lines which integrate over multiple dust clouds.”
What the sources say
- Not matchedcites [55]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
plaindirect- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: fails — The paper’s conclusions may not depend on it.
- Based: passes — The paper gives a reason why it holds.
Probably not a substantial claim. The paper’s conclusions may not depend on it.
- Not matched
What the paper did — it cites no source for this, so there is none to check. The quote shows it is in the paper.
In the paper
“To keep down the total number of spectra we drop the other Planck bands since these provide a negligible amount of additional information.”
plaindirect- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: fails — The paper’s conclusions may not depend on it.
- Based: passes — The paper gives a reason why it holds.
Probably not a substantial claim. The paper’s conclusions may not depend on it.
In the paper
“We note that analysis of 2.3 GHz data from S-PASS in conjunction with WMAP and Planck fi nds β s = -3 . 2 with no detected trends with galactic latitude or angular scale [30]”
What the sources say
- Not matchedcites [30]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: fails — The paper’s conclusions may not depend on it.
- Based: passes — The paper gives a reason why it holds.
Probably not a substantial claim. The paper’s conclusions may not depend on it. It may state two separate claims as one.
- Not matched
None of the sources cited for this claim could be matched to a paper in Crossref, so there is nothing to check it against.
In the paper
“Using different apodizations suppresses the amplitude of the cross-spectra as compared to the auto-spectra but this is automatically taken into account in the bandpower window function calculations [18, 53].”
What the sources say
- Not matchedcites [18]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- Not matchedcites [53]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
plaindirect- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
- Not matched
In the paper
“This study uses maps of the effective number of clouds taken from Ref. [56] which in Sec. 4.2 specifically examines the BICEP/ Keck patch and states that 'one cloud dominates the column density in the majority of pixels in the BICEP/ Keck region'.”
What the sources say
- Not matchedcites [56]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: passes — The paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
Probably not a substantial claim.
- Not matched
None of the sources cited for this claim could be matched to a paper in Crossref, so there is nothing to check it against.
In the paper
“In this section we perform tests of the new 2016, 2017 and 2018 data which are the same as those performed on the previous BICEP/ Keck data in Sec. VII.C of Ref. [9], Sec. 6.3 of Ref. [14], Appendix B of BK14, and Appendix B of BK15.”
What the sources say
- Not matchedcites [9]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- Not matchedcites [14]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: fails — The paper’s conclusions may not depend on it.
- Based: passes — The paper gives a reason why it holds.
Probably not a substantial claim. The paper’s conclusions may not depend on it.
- Not matched
What the paper did — it cites no source for this, so there is none to check. The quote shows it is in the paper.
In the paper
“Running maximum likelihood searches on simulations indicates that this results in σ ( r ) as low as any other option with no detectable bias on r .”
hedgeddirect- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
In the paper
“Ref. [30] finds a value at the bottom end of this range ( ≈ -1) from the S-PASS data for BB at high galactic latitude.”
What the sources say
- Not matchedcites [30]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: fails — The paper’s conclusions may not depend on it.
- Based: passes — The paper gives a reason why it holds.
Probably not a substantial claim. The paper’s conclusions may not depend on it.
- Not matched
What the paper did — it cites no source for this, so there is none to check. The quote shows it is in the paper.
In the paper
“For all effects considered, the magnitude of the estimated bias on r is significantly smaller than our statistical uncertainty, and not all of the biases have the same sign, which should lead to partial cancelation.”
plaindirect- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: passes — The paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
What the paper did — it cites no source for this, so there is none to check. The quote shows it is in the paper.
In the paper
“In this leakage analysis for BK18, care was taken to minimize systematic contamination in the composite beam maps from the FFBM analysis pipeline itself, e.g. by minimizing non-Gaussian noise and excess smoothing.”
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: passes — The paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
Probably not a substantial claim.
A conclusion the paper draws from its own results — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“Such variation of the dust amplitude across the field can potentially produce bias on r given that our re-fit model assumes a single A d value applies to both the smaller BICEP2 / Keck fi eld and the larger BICEP3 fi eld.”
hedgedconditional- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: fails — The paper’s conclusions may not depend on it.
- Based: passes — The paper gives a reason why it holds.
Probably not a substantial claim. The paper’s conclusions may not depend on it.
- The authors state this as an assumption: The re-fit model assumes a single A_d value applies to both the smaller BICEP2/Keck field and the larger BICEP3 field.
In the paper
“Other additive systematic effects including EMI, magnetic, thermal, and other scan-synchronous sources of residual contamination, and ghost beams, were studied in Ref. [34] and upper limits placed on their contributions equivalent to r < 10 -4 , except in the case of EMI contamination from the satellite uplink transmitter, which was bounded at r < 1 . 7 × 10 -3 with 95% confidence.”
What the sources say
- Not matchedcites [34]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: unclear — It is unclear whether the paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
- Not matched
A conclusion the paper draws from its own results — it cites no other source for it, so there is none to check. The quote shows it is in the paper.
In the paper
“The driving factor in this improvement in the recovered bias is the inclusion of BICEP3 , which demonstrates lower differential beam power than Keck and BICEP2 , both before and after deprojection.”
boosteddirect- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: passes — The paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
What the paper did — it cites no source for this, so there is none to check. The quote shows it is in the paper.
In the paper
“Levels of these potential sources of contamination have been monitored throughout collection of the current dataset (including EMI reduction from additional shielding at the satellite uplink), and contributions from these effects remain negligible.”
plain- Asserted: passes — The authors put it forward as true.
- Checkable: passes — It can be checked against evidence.
- Load-bearing: passes — The paper’s conclusions depend on it.
- Based: passes — The paper gives a reason why it holds.
It may state two separate claims as one.
The authors state this as an assumption.
For dust, EE/BB = 2.
“under the assumption that EE/BB = 2 for dust, as is known to be close to the case [23, 24]”
“under the assumption that EE/BB = 2 for dust”
The authors state this as an assumption.
The synchrotron frequency spectrum is a simple power law A_sync ∝ ν^β_s.
“assuming a simple power law for the frequency spectral behavior A sync ∝ ν β s”
The authors state this as an assumption.
The dust spatial power spectrum is a power law D_ℓ ∝ ℓ^α_d.
“The spatial power spectrum is taken as a power law D ℓ ∝ ℓ α d marginalizing uniformly over the (generous) range -1 < α d < 0”
The authors state this as an assumption.
The synchrotron spatial power spectrum is a power law D_ℓ ∝ ℓ^α_s.
“The spatial power spectrum is taken as a power law D ℓ ∝ ℓ α s marginalizing over the range -1 < α s < 0 [32].”
The authors state this as an assumption.
The power spectrum of the polarized dust emission in the BICEP/Keck field follows a power law.
“We note that this figure offers empirical backing for an assumption which we make in our mainline analysis: that the power spectrum of the polarized dust emission in our field follows a power law.”
The authors state this as an assumption.
The dust and synchrotron sky patterns have Gaussian fluctuations.
“The parametric model which we are using, including the approximation of Gaussian fluctuation of the dust (and synchrotron) sky patterns, remains an adequate description of the presently available data.”
The paper relies on this without support.
Dust decorrelation exists in the BICEP/Keck sky patch at some level.
“Nonetheless, decorrelation surely exists in our sky patch at some level-the question is whether it is relevant as compared to the BK18 experimental noise.”
The authors state this as an assumption.
The EE/BB ratios for dust and synchrotron are both exactly 2.
“under the artificial assumption that the EE/BB ratios for dust and synchrotron are both exactly 2”
The authors state this as an assumption.
The re-fit model assumes a single A_d value applies to both the smaller BICEP2/Keck field and the larger BICEP3 field.
“given that our re-fit model assumes a single A d value applies to both the smaller BICEP2 / Keck fi eld and the larger BICEP3 fi eld.”
The paper relies on this without support.
When running on simulations generated according to the model being re-fit, the input parameter values should be recovered in the mean.
“we then have an a priori expectation that the input parameter values should be recovered in the mean.”
The paper relies on this without support.
The Planck 2018 cosmological parameters predict a specific lensing BB spectrum as used in the BK18 baseline analysis.
“The Planck 2018 cosmological parameters predict a specific lensing BB spectrum as used in the 'BK18 baseline' analysis described above.”
Citations
Cites
Planck 2018 results: VI. Cosmological parameters
Planck Collaboration, Aghanim, N., Akrami, Y., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., et al. (2020) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201833910 · Cited by 14,258
Self-citationCosmological parameters from CMB and other data: A Monte Carlo approach
Lewis, A., & Bridle, S. (2002) · Physical Review D · doi:10.1103/physrevd.66.103511 · Cited by 3,495
NINE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE ( WMAP ) OBSERVATIONS: FINAL MAPS AND RESULTS
Bennett, C. L., Larson, D., Weiland, J. L., Jarosik, N., Hinshaw, G., Odegard, N., Smith, K. M., Hill, R. S., Gold, B., Halpern, M., et al. (2013) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/208/2/20 · Cited by 2,639
Self-citationA Measurement of Excess Antenna Temperature at 4080 Mc/s.
Penzias, A. A., & Wilson, R. W. (1965) · The Astrophysical Journal · doi:10.1086/148307 · Cited by 2,606
Akrami, Y., Arroja, F. M. A., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., Basak, S., et al. (2019) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201833887 · Cited by 2,435
Self-citationDetection of B -Mode Polarization at Degree Angular Scales by BICEP2
Ade, P. A. R., Aikin, R. W., Barkats, D., Benton, S. J., Bischoff, C. A., Bock, J. J., Brevik, J. A., Buder, I., Bullock, E., Dowell, C. D., et al. (2014) · Physical Review Letters · doi:10.1103/physrevlett.112.241101 · Cited by 1,572
Self-citationJoint Analysis of BICEP2/ Keck Array and Planck Data
Ade, P. A. R., Aghanim, N., Ahmed, Z., Aikin, R. W., Alexander, K. D., Arnaud, M., Aumont, J., Baccigalupi, C., Banday, A. J., Barkats, D., et al. (2015) · Physical Review Letters · doi:10.1103/physrevlett.114.101301 · Cited by 1,013
Self-citationSignature of Gravity Waves in the Polarization of the Microwave Background
Seljak, U., & Zaldarriaga, M. (1997) · Physical Review Letters · doi:10.1103/physrevlett.78.2054 · Cited by 982
A Probe of Primordial Gravity Waves and Vorticity
Kamionkowski, M., Kosowsky, A. B., & Stebbins, A. J. (1997) · Physical Review Letters · doi:10.1103/physrevlett.78.2058 · Cited by 838
Ade, P. A. R., Ahmed, Z., Aikin, R. W., Alexander, K. D., Barkats, D., Benton, S. J., Bischoff, C. A., Bock, J. J., Bowens-Rubin, R., Brevik, J. A., et al. (2016) · Physical Review Letters · doi:10.1103/physrevlett.116.031302 · Cited by 649
Self-citation
Cited by
Sorted by citations
Probing cosmic inflation with the LiteBIRD cosmic microwave background polarization survey
Allys, E., Arnold, K., Aumont, J., Aurlien, R., Azzoni, S., Baccigalupi, C., Banday, A. J., Banerji, R., Barreiro, R. B., Bartolo, N., et al. (2022) · Progress of Theoretical and Experimental Physics · doi:10.1093/ptep/ptac150 · Cited by 374
Self-citationCosmology with the Laser Interferometer Space Antenna
Auclair, P., Bacon, D., Baker, T., Barreiro, T., Bartolo, N., Belgacem, E., Bellomo, N., Ben-Dayan, I., Bertacca, D., Besançon, M., et al. (2023) · Living Reviews in Relativity · doi:10.1007/s41114-023-00045-2 · Cited by 556
Valentino, E. D., Said, J. L., Riess, A. G., Pollo, A., Poulin, V., Gómez-Valent, A., Weltman, A., Palmese, A., Huang, C. D., van de Bruck, C., et al. (2025) · Physics of the Dark Universe · doi:10.1016/j.dark.2025.101965 · Cited by 590
Self-citationImproved limits on the tensor-to-scalar ratio using BICEP and P l a n c k data
Tristram, M., Banday, A. J., Gorski, K. M., Keskitalo, R., Lawrence, C. R., Andersen, K. J., Barreiro, R. B., Borrill, J., Colombo, L. P. L., Eriksen, H. K., et al. (2022) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.105.083524 · Cited by 266
The Atacama Cosmology Telescope: DR6 power spectra, likelihoods and ΛCDM parameters
Louis, T., Posta, A. L., Atkins, Z., Jense, H. T., Abril-Cabezas, I., Addison, G. E., Ade, P. A. R., Aiola, S., Alford, T., Alonso, D., et al. (2025) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2025/11/062 · Cited by 239
Self-citation
Metadata
- Authors
- Ade, P. A. R., Ahmed, Z., Amiri, M., Barkats, D., Thakur, R. B., Bischoff, C. A., Beck, D., Bock, J. J., Boenish, H., Bullock, E., Buza, V., Cheshire, J. R., Connors, J., Cornelison, J., Crumrine, M., Cukierman, A., Denison, E. V., Dierickx, M., Duband, L., Eiben, M., Fatigoni, S., Filippini, J. P., Fliescher, S., Goeckner-Wald, N., Goldfinger, D. C., Grayson, J., Grimes, P., Hall, G., Halal, G., Halpern, M., Hand, E., Harrison, S., Henderson, S., Hildebrandt, S. R., Hilton, G. C., Hubmayr, J., Hui, H., Irwin, K. D., Kang, J., Karkare, K. S., Karpel, E., Kefeli, S., Kernasovskiy, S. A., Kovac, J. M., Kuo, C. L., Lau, K., Leitch, E. M., Lennox, A., Megerian, K. G., Minutolo, L., Moncelsi, L., Nakato, Y., Namikawa, T., Nguyen, H. T., O’Brient, R., Ogburn, R. W., Palladino, S., Prouve, T., Pryke, C., Racine, B., Reintsema, C. D., Richter, S., Schillaci, A., Schwarz, R., Schmitt, B. L., Sheehy, C. D., Soliman, A., Germaine, T. S., Steinbach, B., Sudiwala, R. V., Teply, G. P., Thompson, K. L., Tolan, J. E., Tucker, C., Turner, A. D., Umiltà, C., Vergès, C., Vieregg, A. G., Wandui, A., Weber, A. C., Wiebe, D. V., Willmert, J., Wong, C. L., Wu, W. L. K., Yang, H., Yoon, K. W., Young, E., Yu, C., Zeng, L., Zhang, C., Zhang, S., & BICEP/<i>Keck</i> Collaboration
- Affiliations
- Cardiff University (GB)
- SLAC National Accelerator Laboratory (US)
- University of British Columbia (CA)
- Center for Astrophysics Harvard & Smithsonian (US)
- California Institute of Technology (US)
- University of Cincinnati (US)
- University of Minnesota (US)
- University of Chicago (US)
- National Institute of Standards and Technology (US)
- Commissariat à l'Énergie Atomique et aux Énergies Alternatives (FR)
- University of Illinois Urbana-Champaign (US)
- Stanford University (US)
- Harvard University (US)
- Jet Propulsion Laboratory (US)
- Kavli Institute for the Physics and Mathematics of the Universe (JP)
- Service des Basses Températures, Commissariat à l’Energie Atomique, 38054 Grenoble, France
- Centre National de la Recherche Scientifique (FR)
- Brookhaven National Laboratory (US)
- ORCID
- Ade, P. A. R.
- Ahmed, Z.
- Barkats, D.
- Bischoff, C. A.
- Beck, D.
- Bock, J. J.
- Buza, V.
- Cheshire, J. R.
- Cukierman, A.
- Dierickx, M.
- Eiben, M.
- Filippini, J. P.
- Goldfinger, D. C.
- Grimes, P.
- Halal, G.
- Halpern, M.
- Henderson, S.
- Hildebrandt, S. R.
- Irwin, K. D.
- Karkare, K. S.
- Kovac, J. M.
- Kuo, C. L.
- Leitch, E. M.
- Nakato, Y.
- Namikawa, T.
- Ogburn, R. W.
- Pryke, C.
- Racine, B.
- Schillaci, A.
- Sudiwala, R. V.
- Thompson, K. L.
- Tolan, J. E.
- Vergès, C.
- Vieregg, A. G.
- Wandui, A.
- Wiebe, D. V.
- Willmert, J.
- Wu, W. L. K.
- Young, E.
- Yu, C.
- Zeng, L.
- Venue
- Physical Review Letters
- Publisher
- American Physical Society (APS)
- Published
- 2021-10-04
- Volume
- 127
- Issue
- 15
- Pages
- 151301-151301
- ISSN
- 0031-9007 (ISSN-L)
- 1079-7114
- OpenAlex
- W3202102945
- Semantic Scholar
- 93637369c8e398b920a6f82f83adf5ffc4fbba76
- Cited by
- 1,014
- References
- 57
- Citations by year
- 2026: 163 · 2025: 253 · 2024: 218 · 2023: 203 · 2022: 162 · 2021: 15
- FWCI
- 80.49
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Licence
- Locations
- Physical Review Letters (publishedVersion)
- PubMed (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- CaltechAUTHORS (California Institute of Technology) (submittedVersion)
- HAL AMU (submittedVersion)
- OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information) (submittedVersion)
- arXiv (Cornell University)
- Funders
- National Science Foundation (0742818, 0742592, 1044978, 1110087, 1145172, 1145143, 1145248, 1639040, 1638957, 1638978, 1638970)
- W. M. Keck Foundation
- Jet Propulsion Laboratory
- National Aeronautics and Space Administration (06-ARPA206-0040, 10-SAT10-0017, 12-SAT12-0031, 14-SAT14-0009, 16-SAT-16-0002)
- Gordon and Betty Moore Foundation
- Canada Foundation for Innovation
- University of British Columbia
- Science and Technology Facilities Council (ST/N000706/1)
- Faculty of Arts and Sciences, Harvard University
- U.S. Department of Energy
- Office of Science
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Dark Matter and Cosmic Phenomena
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Noncommutative and Quantum Gravity Theories
- Keywords
- primordial gravitational waves, BICEP2, Keck Array, CMB polarization, tensor-to-scalar ratio, foreground modeling, polarized dust emission, synchrotron radiation, Planck, WMAP
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
A language model drew the claims from the paper on 2026-10-23, under version 3 of the claim definition (model deepseek-v4.1-flash, prompt extract-v3).
A second model labelled each claim on 2026-10-23 (model jev-1.13-20260917, definition revision gold-guideline-v0.2).
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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