Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO
E. ChaussidonLawrence Berkeley National LaboratoryMartin WhiteUniversity of California, BerkeleyArnaud de MattiaIRFURafaela GsponerÉcole Polytechnique Fédérale de Lausanne (EPFL)S. AhlenBoston UniversityDavide BianchiUniversità degli Studi di MilanoDavid BrooksUniversity College LondonT. ClaybaughLawrence Berkeley National LaboratoryS. ColeDurham UniversityA. CuceuLawrence Berkeley National LaboratoryAxel de la MacorraUniversidad Nacional Autónoma de MéxicoPeter DoelUniversity College LondonS. FerraroLawrence Berkeley National LaboratoryAndreu Font-RiberaInstitut de Física d’Altes Energies (IFAE)J. E. Forero-RomeroUniversidad de los AndesE. GaztañagaInstitute of Space SciencesSatya Gontcho A GontchoLawrence Berkeley National LaboratoryG. GutiérrezFermi National Accelerator LaboratoryJ. GuyLawrence Berkeley National LaboratoryC. HahnUniversity of ArizonaH. K. Herrera-AlcantarInstitut d’Astrophysique de ParisKlaus HonscheidChicago U., KICPM IshakThe University of Texas at DallasD. KirkbyUniversity of California, IrvineTheodore KisnerLawrence Berkeley National LaboratoryAnthony KreminLawrence Berkeley National LaboratoryMartin LandriauLawrence Berkeley National LaboratoryL. Le GuillouIN2P3M. E. LeviLawrence Berkeley National LaboratoryR. MiquelInstitut de Física d’Altes Energies (IFAE)John MoustakasSiena CollegeGustavo NizMexico U., ICNWill J. PercivalPerimeter InstituteFrancisco PradaInstituto de Astrofísica de AndalucíaIgnasi Pérez-RàfolsUniversitat Politècnica de CatalunyaA.J. RossOhio State UGraziano RossiSejong UniversityE. SánchezMadrid, CIEMATDavid J. SchlegelLawrence Berkeley National LaboratoryHee‐Jong SeoOhio UniversityD. SprayberryNSF NOIRLabMichael WaltherLudwig-Maximilians-UniversitätBenjamin Alan WeaverNSF NOIRLab
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Supplementary material to DESI's publication 'Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO' to comply with the data management plan.
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