Analysis of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>DESI</mml:mi><mml:mo stretchy="false">×</mml:mo><mml:mi>DES</mml:mi></mml:mrow></mml:math> using the Lagrangian effective theory of LSS
S. ChenJoseph DeRoseLawrence Berkeley National LaboratoryRongpu ZhouLawrence Berkeley National LaboratoryMartin WhiteUniversity of CaliforniaS. FerraroLawrence Berkeley National LaboratoryChris BlakeSwinburne University of TechnologyJ. LangeUniversity of MichiganR.H. WechslerSLAC National Accelerator LaboratoryJosé Edgar Madriz AguilarLawrence Berkeley National LaboratoryS. AhlenD. BrooksUniversity College LondonT. ClaybaughLawrence Berkeley National LaboratoryKyle DawsonThe University of UtahAxel de la MacorraUniversidad Nacional Autónoma de MéxicoP. DoelUniversity College LondonAndreu Font-RiberaBarcelona Institute of Science and TechnologyE. GaztañagaInstitut d’Estudis Espacials de Catalunya (IEEC)Satya Gontcho A GontchoLawrence Berkeley National LaboratoryG. GutierrezFermi National Accelerator LaboratoryKlaus HonscheidThe Ohio State UniversityCullan HowlettUniversity of QueenslandR. KehoeSouthern Methodist UniversityD. KirkbyUniversity of CaliforniaTheodore KisnerLawrence Berkeley National LaboratoryA. KreminLawrence Berkeley National LaboratoryMartin LandriauLawrence Berkeley National LaboratoryL. Le GuillouSorbonne UniversitéMarc ManeraBarcelona Institute of Science and TechnologyAaron MeisnerR. MiquelBarcelona Institute of Science and TechnologyJeffrey A. NewmanUniversity of PittsburghGustavo NizInstituto Avanzado de Cosmología A. CN. Palanque‐DelabrouilleLawrence Berkeley National LaboratoryWill J. PercivalPerimeter Institute for Theoretical PhysicsFrancisco PradaInstituto de Astrofísica de Andalucía (CSIC)Graziano RossiSejong UniversityE. SánchezDavid J. SchlegelLawrence Berkeley National LaboratoryM. SchubnellUniversity of MichiganD. SprayberryG. TarléUniversity of MichiganBenjamin Alan Weaver
2024lv
ABI
Аннотация
The paper combines galaxy data targeted with the Dark Energy Spectroscopic Instrument (DESI) with the associated galaxy lensing signal from the Year-3 Dark Energy Survey. The modeling implements novel effective and hybrid effective field theory aspects, independently confirming previous Cosmic Microwave Background results on the amplitude of the lensing signal, S8.
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Цитирования и источники
Цитирований: 3Использованных источников: 0
Показатели — AkademScholar · Скоро