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Paper Citation Record · LEDGER
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Thawing Quintessence: Priors, evidence, and likely trajectories Efficient Computation of CMB anisotropies in closed FRW models
Reference 50
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Observation 30ccc18b-56b3-493b-a6bc-9334f9cd55fe · inbound
Robust Preference for Dark Sector Interactions Efficient Computation of CMB anisotropies in closed FRW models
Reference 119
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Observation 09766cfa-01d2-4738-9bab-e120b79c3657 · inbound
An essential building block for cosmological zoom-in perturbation theory Efficient Computation of CMB anisotropies in closed FRW models
Reference 55
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Observation 7392432c-e893-4699-9139-dc11c4f35294 · inbound
Cosmological analysis of the DESI DR1 Lyman alpha 1D power spectrum Efficient Computation of CMB anisotropies in closed FRW models
Reference 100
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Observation 1cd0460e-ce47-4b91-80b5-af68a24bad7d · inbound
A Variable-Slope Smooth-$k$ Filter for Modeling Halo Abundances with Damped and Oscillatory Power Spectra Efficient Computation of CMB anisotropies in closed FRW models
Reference 57
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Observation 7a1f1a92-365f-4c50-8bc3-2ccda92745a3 · inbound
ACT DR6+Planck impact on inflation with non-zero vacuum expectation value and the post-inflationary behavior Efficient Computation of CMB anisotropies in closed FRW models
Reference 51
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Observation cb8d9a5f-dc3e-4b4e-92e6-4838b89f7e0c · inbound
Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology Efficient Computation of CMB anisotropies in closed FRW models
Reference 63
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Observation 7de4d59d-23db-4dc4-8130-f32f2096cc4b · inbound
DESI DR2 Baryon Acoustic Oscillations from the Lyman Alpha Forest Multipoles Efficient Computation of CMB anisotropies in closed FRW models
Reference 45
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Observation c0cc731f-77f2-4837-956c-4a018aec13a4 · inbound
The Bayesian view of DESI DR2 with unimpeded: Evidence and tension in a combined analysis with CMB and supernovae across cosmological models Efficient Computation of CMB anisotropies in closed FRW models
Reference 32
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Observation 004a494b-b7f3-49e5-a722-3d3317c4e2dd · inbound
Constraining Neutrino Mass with the Void Weak Lensing Effect Efficient Computation of CMB anisotropies in closed FRW models
Reference 80
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Observation eb7a25d5-7565-4a47-a336-dd9aeaa03604 · inbound
Measuring neutrino mass in light of ACT DR6 and DESI DR2 Efficient Computation of CMB anisotropies in closed FRW models
Reference 185
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Observation 140097b6-3f9a-452e-9325-3b844ddd242d · inbound
Blind mitigation of foreground-induced biases on primordial $B$ modes for ground-based CMB experiments Efficient Computation of CMB anisotropies in closed FRW models
Reference 36
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Observation d472bd4b-6a1c-4d41-9fee-debb9cdc3f79 · inbound
Revisiting observational constraints on coupled exponential quintessence with energy and momentum transfers: degeneracy with massive neutrinos Efficient Computation of CMB anisotropies in closed FRW models
Reference 71
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Observation 901843e9-a02e-48ce-bea5-af6ce7d8a8d6 · inbound
Visual Prompt Discovery via Semantic Exploration Efficient Computation of CMB anisotropies in closed FRW models
Reference 23
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Observation f9d6faf6-3884-45a6-8014-2d314358e343 · inbound
Nonminimally coupled quintessence with sign-switching interaction Efficient Computation of CMB anisotropies in closed FRW models
Reference 65
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Observation 79340149-7ec1-4cd2-b733-3d49a0235ecb · inbound
A generic $\omega_b$ tension in early-time solutions to the Hubble tension Efficient Computation of CMB anisotropies in closed FRW models
Reference 61
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Observation 071a3319-5fa1-4274-bfc7-766f6cda6bed · inbound
Late-Transition Interacting Thawer Dark Energy: Model Definition and Benchmark Consistency Tests Efficient Computation of CMB anisotropies in closed FRW models
Reference 9
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Observation 973dbdd9-a043-43d2-a955-87bd2e9800b3 · inbound
Joint Curvature and Growth Rate measurements with Supernova Peculiar Velocities and the CMB Efficient Computation of CMB anisotropies in closed FRW models
Reference 57
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Observation 208d960b-738b-4fdc-abcf-28168b901974 · inbound
Analytic compression of the effective field theory of the Lyman-alpha forest Efficient Computation of CMB anisotropies in closed FRW models
Reference 71
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