FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W4320026051> ?p ?o ?g. }

• W4320026051 abstract "High resolution cosmic microwave background (CMB) experiments have allowed us to precisely measure the CMB temperature power spectrum down to very small scales (multipole $ensuremath{ell}ensuremath{sim}3000$). Such measurements at multiple frequencies enable separating the power spectrum of the primary CMB anisotropies with the power spectrum of other signals like CMB lensing, thermal and kinematic Sunyaev-Zel'dovich effects (tSZ and kSZ), and cosmic infrared background (CIB). In this paper, we explore another signal of interest at these frequencies that should be present in the CMB maps: extragalactic CO molecular rotational line emissions, which are the most widely used tracers of molecular gas in the line intensity mapping experiments. Using the SIDES simulations adopted for top hat bandpasses at 150 and 220 GHz, we show that the cross-correlation of the CIB with CO lines has a contribution similar to the CIB-tSZ correlation and the kSZ power, thereby contributing a non-negligible amount to the total power at these scales. This signal, therefore, may significantly impact the recently reported $ensuremath{ge}3ensuremath{sigma}$ detection of the kSZ power spectrum from the South Pole Telescope collaboration, as the contribution of the CO lines is not considered in such analyses. Our results also provide a new way of measuring the CO power spectrum in cross-correlation with the CIB. Finally, these results show that the CO emissions present in the CMB maps will have to be accounted for in all the CMB auto-power spectrum and cross-correlation studies involving a large-scale structure tracer." @default.
• W4320026051 created "2023-02-12" @default.
• W4320026051 creator A5011721458 @default.
• W4320026051 creator A5034399725 @default.
• W4320026051 creator A5040019445 @default.
• W4320026051 creator A5056958476 @default.
• W4320026051 creator A5065901451 @default.
• W4320026051 creator A5074837816 @default.
• W4320026051 date "2023-06-07" @default.
• W4320026051 modified "2023-09-26" @default.
• W4320026051 title "Extragalactic CO emission lines in the CMB experiments: A forgotten signal and a foreground" @default.
• W4320026051 cites W1972700440 @default.
• W4320026051 cites W2014415007 @default.
• W4320026051 cites W2019398523 @default.
• W4320026051 cites W2020460381 @default.
• W4320026051 cites W2028626541 @default.
• W4320026051 cites W2051206400 @default.
• W4320026051 cites W2127928502 @default.
• W4320026051 cites W2128317762 @default.
• W4320026051 cites W2294612193 @default.
• W4320026051 cites W2624412542 @default.
• W4320026051 cites W2771701331 @default.
• W4320026051 cites W2888259247 @default.
• W4320026051 cites W2990113658 @default.
• W4320026051 cites W3001660683 @default.
• W4320026051 cites W3035898086 @default.
• W4320026051 cites W3045842115 @default.
• W4320026051 cites W3065408639 @default.
• W4320026051 cites W3097823144 @default.
• W4320026051 cites W3098038714 @default.
• W4320026051 cites W3098345056 @default.
• W4320026051 cites W3100971600 @default.
• W4320026051 cites W3102034977 @default.
• W4320026051 cites W3102677143 @default.
• W4320026051 cites W3103504115 @default.
• W4320026051 cites W3103868583 @default.
• W4320026051 cites W3104532525 @default.
• W4320026051 cites W3104860562 @default.
• W4320026051 cites W3105933244 @default.
• W4320026051 cites W3111203717 @default.
• W4320026051 cites W3117531260 @default.
• W4320026051 cites W3122385173 @default.
• W4320026051 cites W3124793477 @default.
• W4320026051 cites W3127201510 @default.
• W4320026051 cites W3131323078 @default.
• W4320026051 cites W4221142036 @default.
• W4320026051 cites W4225081376 @default.
• W4320026051 cites W4288079944 @default.
• W4320026051 cites W4289812967 @default.
• W4320026051 cites W4295886719 @default.
• W4320026051 cites W4311636805 @default.
• W4320026051 doi "https://doi.org/10.1103/physrevd.107.123504" @default.
• W4320026051 hasPublicationYear "2023" @default.
• W4320026051 type Work @default.
• W4320026051 citedByCount "1" @default.
• W4320026051 countsByYear W43200260512023 @default.
• W4320026051 crossrefType "journal-article" @default.
• W4320026051 hasAuthorship W4320026051A5011721458 @default.
• W4320026051 hasAuthorship W4320026051A5034399725 @default.
• W4320026051 hasAuthorship W4320026051A5040019445 @default.
• W4320026051 hasAuthorship W4320026051A5056958476 @default.
• W4320026051 hasAuthorship W4320026051A5065901451 @default.
• W4320026051 hasAuthorship W4320026051A5074837816 @default.
• W4320026051 hasBestOaLocation W43200260513 @default.
• W4320026051 hasConcept C105795698 @default.
• W4320026051 hasConcept C120665830 @default.
• W4320026051 hasConcept C121332964 @default.
• W4320026051 hasConcept C1276947 @default.
• W4320026051 hasConcept C168110828 @default.
• W4320026051 hasConcept C207297109 @default.
• W4320026051 hasConcept C2779770503 @default.
• W4320026051 hasConcept C33923547 @default.
• W4320026051 hasConcept C44870925 @default.
• W4320026051 hasConcept C4839761 @default.
• W4320026051 hasConcept C52765159 @default.
• W4320026051 hasConcept C60318249 @default.
• W4320026051 hasConcept C62520636 @default.
• W4320026051 hasConcept C85725439 @default.
• W4320026051 hasConceptScore W4320026051C105795698 @default.
• W4320026051 hasConceptScore W4320026051C120665830 @default.
• W4320026051 hasConceptScore W4320026051C121332964 @default.
• W4320026051 hasConceptScore W4320026051C1276947 @default.
• W4320026051 hasConceptScore W4320026051C168110828 @default.
• W4320026051 hasConceptScore W4320026051C207297109 @default.
• W4320026051 hasConceptScore W4320026051C2779770503 @default.
• W4320026051 hasConceptScore W4320026051C33923547 @default.
• W4320026051 hasConceptScore W4320026051C44870925 @default.
• W4320026051 hasConceptScore W4320026051C4839761 @default.
• W4320026051 hasConceptScore W4320026051C52765159 @default.
• W4320026051 hasConceptScore W4320026051C60318249 @default.
• W4320026051 hasConceptScore W4320026051C62520636 @default.
• W4320026051 hasConceptScore W4320026051C85725439 @default.
• W4320026051 hasFunder F4320309911 @default.
• W4320026051 hasFunder F4320334678 @default.
• W4320026051 hasIssue "12" @default.
• W4320026051 hasLocation W43200260511 @default.
• W4320026051 hasLocation W43200260512 @default.
• W4320026051 hasLocation W43200260513 @default.
• W4320026051 hasLocation W43200260514 @default.
• W4320026051 hasOpenAccess W4320026051 @default.

• next