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Иш: Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO
Cosmological parameters derived from the final <i>Planck</i> data release (PR4)
M. Tristram, A. J. Banday, M. Douspis +10
Мақола20235 иқтибосABIAnalysis 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. Chen, Joseph DeRose, Rongpu Zhou +39
Мақола20243 иқтибосABIOverview of the Fiber System for the Dark Energy Spectroscopic Instrument
Claire Poppett, Luke Tyas, J. Aguilar +66
Мақола20243 иқтибосABIEarly Dark Energy can Resolve the Hubble Tension
Vivian Poulin, Tristan L. Smith, Tanvi Karwal +1
Мақола20193 иқтибосABIOptimal 1D Ly α forest power spectrum estimation – III. DESI early data
Naim Göksel Karaçaylı, Paul Martini, Julien Guy +59
Мақола20242 иқтибосABIObservational constraints on early dark energy
Evan McDonough, J. Colin Hill, Mikhail M. Ivanov +2
Мақола20242 иқтибосABI