FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2038421608> ?p ?o ?g. }

• W2038421608 endingPage "57" @default.
• W2038421608 startingPage "46" @default.
• W2038421608 abstract "Secondary anisotropies of the cosmic microwave background (CMB) have the potential to reveal intricate details about the history of our universe between the present and recombination epochs. However, because the CMB we observe is the projected sum of a multitude of effects, the interpretation of small-scale anisotropies by future high-resolution experiments will be marred by uncertainty and speculation without the handles provided by other observations. The recent controversy over the excess small-scale anisotropy detected by CBI and the BIMA array is a foretaste of potential challenges that will be faced when interpreting future experiments. In this paper we show that cross-correlating the CMB with an overlapping weak-lensing survey will isolate the elusive kinetic Sunyaev-Zel'dovich (kSZ) effect from secondary anisotropies generated at higher redshifts. We show that if upcoming high angular resolution CMB experiments, like Planck/ACT/SPT, cover the same area of sky as current and future weak-lensing surveys, like CFTHLS/SNAP/LSST, the cross-correlation of cosmic shear with the kSZ effect will be detected with high signal-to-noise ratio, increasing the potential science accessible to both sets of surveys. For example, if ACT and a CFHTLS-like survey were to overlap, this cross-correlation would be detected with a total signal-to-noise ratio greater than 220, reaching 1.8 per individual multipole around l ~ 5000. Furthermore, this cross-correlation probes the three-point coupling between the underlying dark matter and the momentum of the ionized baryons in the densest regions of the universe at intermediate redshifts. Similar to the thermal Sunyaev-Zel'dovich (tSZ) power spectrum, its strength is extremely sensitive to the power spectrum normalization parameter, σ8, scaling roughly as σ. It provides an effective mechanism to isolate any component of anisotropy due to patchy reionization and rule out primordial small-scale anisotropy." @default.
• W2038421608 created "2016-06-24" @default.
• W2038421608 creator A5018266021 @default.
• W2038421608 creator A5027589256 @default.
• W2038421608 creator A5091900050 @default.
• W2038421608 date "2004-05-01" @default.
• W2038421608 modified "2023-09-24" @default.
• W2038421608 title "Beyond the Damping Tail: Cross‐Correlating the Kinetic Sunyaev‐Zel’dovich Effect with Cosmic Shear" @default.
• W2038421608 cites W1481865921 @default.
• W2038421608 cites W1490817231 @default.
• W2038421608 cites W1579845354 @default.
• W2038421608 cites W1942224731 @default.
• W2038421608 cites W1968124095 @default.
• W2038421608 cites W1974842200 @default.
• W2038421608 cites W1976462901 @default.
• W2038421608 cites W1977811708 @default.
• W2038421608 cites W1985612538 @default.
• W2038421608 cites W1986235445 @default.
• W2038421608 cites W1987801517 @default.
• W2038421608 cites W2005402395 @default.
• W2038421608 cites W2006588599 @default.
• W2038421608 cites W2007377530 @default.
• W2038421608 cites W2017232919 @default.
• W2038421608 cites W2017297207 @default.
• W2038421608 cites W2017416852 @default.
• W2038421608 cites W2018719255 @default.
• W2038421608 cites W2028829719 @default.
• W2038421608 cites W2028888846 @default.
• W2038421608 cites W2041064269 @default.
• W2038421608 cites W2043528675 @default.
• W2038421608 cites W2053463081 @default.
• W2038421608 cites W2056892528 @default.
• W2038421608 cites W2069480899 @default.
• W2038421608 cites W2073455076 @default.
• W2038421608 cites W2077539669 @default.
• W2038421608 cites W2083061716 @default.
• W2038421608 cites W2089881384 @default.
• W2038421608 cites W2090127881 @default.
• W2038421608 cites W2091953875 @default.
• W2038421608 cites W2097755895 @default.
• W2038421608 cites W2101090335 @default.
• W2038421608 cites W2105265841 @default.
• W2038421608 cites W2105896449 @default.
• W2038421608 cites W2117363750 @default.
• W2038421608 cites W2118265220 @default.
• W2038421608 cites W2140478436 @default.
• W2038421608 cites W2146084926 @default.
• W2038421608 cites W2167835957 @default.
• W2038421608 cites W2199319344 @default.
• W2038421608 cites W2597736258 @default.
• W2038421608 cites W2614349642 @default.
• W2038421608 cites W2949296060 @default.
• W2038421608 cites W2963270768 @default.
• W2038421608 cites W3098084545 @default.
• W2038421608 cites W3100170090 @default.
• W2038421608 cites W3101269875 @default.
• W2038421608 cites W3102597077 @default.
• W2038421608 cites W3102601368 @default.
• W2038421608 cites W3102677143 @default.
• W2038421608 cites W3103501527 @default.
• W2038421608 cites W3104181571 @default.
• W2038421608 cites W3104314455 @default.
• W2038421608 cites W3105982440 @default.
• W2038421608 cites W4299416410 @default.
• W2038421608 doi "https://doi.org/10.1086/382946" @default.
• W2038421608 hasPublicationYear "2004" @default.
• W2038421608 type Work @default.
• W2038421608 sameAs 2038421608 @default.
• W2038421608 citedByCount "40" @default.
• W2038421608 countsByYear W20384216082016 @default.
• W2038421608 countsByYear W20384216082017 @default.
• W2038421608 countsByYear W20384216082018 @default.
• W2038421608 countsByYear W20384216082019 @default.
• W2038421608 countsByYear W20384216082020 @default.
• W2038421608 countsByYear W20384216082021 @default.
• W2038421608 countsByYear W20384216082022 @default.
• W2038421608 countsByYear W20384216082023 @default.
• W2038421608 crossrefType "journal-article" @default.
• W2038421608 hasAuthorship W2038421608A5018266021 @default.
• W2038421608 hasAuthorship W2038421608A5027589256 @default.
• W2038421608 hasAuthorship W2038421608A5091900050 @default.
• W2038421608 hasConcept C111309251 @default.
• W2038421608 hasConcept C121332964 @default.
• W2038421608 hasConcept C127313418 @default.
• W2038421608 hasConcept C1276947 @default.
• W2038421608 hasConcept C135889238 @default.
• W2038421608 hasConcept C153385146 @default.
• W2038421608 hasConcept C156055797 @default.
• W2038421608 hasConcept C185544564 @default.
• W2038421608 hasConcept C187970030 @default.
• W2038421608 hasConcept C207297109 @default.
• W2038421608 hasConcept C2780740289 @default.
• W2038421608 hasConcept C44870925 @default.
• W2038421608 hasConcept C5900021 @default.
• W2038421608 hasConcept C59375849 @default.
• W2038421608 hasConcept C62520636 @default.
• W2038421608 hasConcept C62796785 @default.
• W2038421608 hasConcept C74650414 @default.

• next