Matches in SemOpenAlex for { <https://semopenalex.org/work/W4297383695> ?p ?o ?g. }
- W4297383695 abstract "The search for primordial $B$-mode polarization of the cosmic microwave background (CMB) is limited by the sample variance of $B$-modes produced at later times by gravitational lensing. Constraints can be improved by ``delensing'': using some proxy of the matter distribution to partially remove the lensing-induced $B$-modes. Current and soon-upcoming experiments will infer a matter map---at least in part---from the temperature anisotropies of the CMB. These reconstructions are contaminated by extragalactic foregrounds: radio-emitting galaxies, the cosmic infrared background, or the Sunyaev-Zel'dovich effects. Using the Websky simulations, we show that the foregrounds add spurious power to the angular autospectrum of delensed $B$-modes via non-Gaussian higher-point functions, biasing constraints on the tensor-to-scalar ratio, $r$. We consider an idealized experiment similar to the Simons Observatory, with no Galactic or atmospheric foregrounds. After removing point sources detectable at 143 GHz and reconstructing lensing from CMB temperature modes $l<3500$ using a Hu-Okamoto quadratic estimator (QE), we infer a value of $r$ that is $1.5ensuremath{sigma}$ higher than the true $r=0$. Reconstructing instead from a minimum-variance internal linear combination map only exacerbates the problem, bringing the bias above $3ensuremath{sigma}$. When the $TT$ estimator is co-added with other QEs or with external matter tracers, new couplings ensue which partially cancel the diluted bias from $TT$. We provide a simple and effective prescription to model these effects. In addition, we demonstrate that the point-source-hardened or shear-only QEs can not only mitigate the biases to acceptable levels but also lead to lower power than the Hu-Okamoto QE after delensing. Thus, temperature-based reconstructions remain powerful tools in the quest to measure $r$." @default.
- W4297383695 created "2022-09-28" @default.
- W4297383695 creator A5041152487 @default.
- W4297383695 creator A5056485248 @default.
- W4297383695 date "2022-09-27" @default.
- W4297383695 modified "2023-10-06" @default.
- W4297383695 title "Impact of extragalactic foregrounds on internal delensing of the CMB <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:mi>B</mml:mi></mml:math> -mode polarization" @default.
- W4297383695 cites W1647293269 @default.
- W4297383695 cites W1786274528 @default.
- W4297383695 cites W1949071448 @default.
- W4297383695 cites W1964777539 @default.
- W4297383695 cites W1966550139 @default.
- W4297383695 cites W1971994589 @default.
- W4297383695 cites W1973018404 @default.
- W4297383695 cites W1973861971 @default.
- W4297383695 cites W1976579441 @default.
- W4297383695 cites W1980684657 @default.
- W4297383695 cites W2011301426 @default.
- W4297383695 cites W2012869970 @default.
- W4297383695 cites W2016888141 @default.
- W4297383695 cites W2017232919 @default.
- W4297383695 cites W2020460381 @default.
- W4297383695 cites W2021296731 @default.
- W4297383695 cites W2026905218 @default.
- W4297383695 cites W2038341054 @default.
- W4297383695 cites W2040443229 @default.
- W4297383695 cites W2047767939 @default.
- W4297383695 cites W2049537569 @default.
- W4297383695 cites W2054899182 @default.
- W4297383695 cites W2056330559 @default.
- W4297383695 cites W2064423559 @default.
- W4297383695 cites W2073455076 @default.
- W4297383695 cites W2082064932 @default.
- W4297383695 cites W2085858674 @default.
- W4297383695 cites W2090349414 @default.
- W4297383695 cites W2107889393 @default.
- W4297383695 cites W2128317762 @default.
- W4297383695 cites W2132845056 @default.
- W4297383695 cites W2134251287 @default.
- W4297383695 cites W2136954147 @default.
- W4297383695 cites W2164261152 @default.
- W4297383695 cites W2395255940 @default.
- W4297383695 cites W2575579273 @default.
- W4297383695 cites W2592719621 @default.
- W4297383695 cites W2608279899 @default.
- W4297383695 cites W2613940254 @default.
- W4297383695 cites W2618889709 @default.
- W4297383695 cites W2788763092 @default.
- W4297383695 cites W2798180987 @default.
- W4297383695 cites W2806579556 @default.
- W4297383695 cites W2888259247 @default.
- W4297383695 cites W2889474840 @default.
- W4297383695 cites W2908554219 @default.
- W4297383695 cites W2922580882 @default.
- W4297383695 cites W2969471574 @default.
- W4297383695 cites W2975076899 @default.
- W4297383695 cites W2979899281 @default.
- W4297383695 cites W2990113658 @default.
- W4297383695 cites W2995509084 @default.
- W4297383695 cites W3001660683 @default.
- W4297383695 cites W3004198491 @default.
- W4297383695 cites W3004929706 @default.
- W4297383695 cites W3035898086 @default.
- W4297383695 cites W3038615835 @default.
- W4297383695 cites W3041346959 @default.
- W4297383695 cites W3081572918 @default.
- W4297383695 cites W3085816351 @default.
- W4297383695 cites W3097441239 @default.
- W4297383695 cites W3098003348 @default.
- W4297383695 cites W3098702070 @default.
- W4297383695 cites W3098899650 @default.
- W4297383695 cites W3099878876 @default.
- W4297383695 cites W3100955764 @default.
- W4297383695 cites W3101618571 @default.
- W4297383695 cites W3102060030 @default.
- W4297383695 cites W3102368526 @default.
- W4297383695 cites W3103145119 @default.
- W4297383695 cites W3103268559 @default.
- W4297383695 cites W3103776278 @default.
- W4297383695 cites W3105609887 @default.
- W4297383695 cites W3112823195 @default.
- W4297383695 cites W3118482222 @default.
- W4297383695 cites W3121960866 @default.
- W4297383695 cites W3122385173 @default.
- W4297383695 cites W3123452516 @default.
- W4297383695 cites W3124826262 @default.
- W4297383695 cites W3126663254 @default.
- W4297383695 cites W3167662530 @default.
- W4297383695 cites W3202438181 @default.
- W4297383695 cites W3208521960 @default.
- W4297383695 cites W4200632998 @default.
- W4297383695 cites W4206419720 @default.
- W4297383695 cites W4206634613 @default.
- W4297383695 cites W4233975723 @default.
- W4297383695 cites W4281631670 @default.
- W4297383695 cites W4288079944 @default.
- W4297383695 cites W4292918236 @default.
- W4297383695 cites W4296816715 @default.
- W4297383695 cites W4297439620 @default.
- W4297383695 doi "https://doi.org/10.1103/physrevd.106.063534" @default.