The Supernova Legacy Survey: measurement of Ωm, Ω∧ and w from the first year data set. Commentary

By P. Astier, J. Guy, N. Regnault, R. Pain, E. Aubourg, D. Balam, S. Basa, R. Carlberg, S. Fabbro, D. Fouchez and 33 more. 2006

348 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/affd62171e6139d2ff40baebff9f6dd9ad02735e

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Citations in the corpus

• The effect of inhomogeneous expansion on the supernova observations (2006, background): “2.1 The Lemaitre-Tolman-Bondi metric 5 2.2 Relation of the inhomogeneities to the observations of light 7”
• Cosmological Models with Linearly Varying Deceleration Parameter (2011, background): “Within the context of general relativity, the current cosmological data from SNIa (Supernova Legacy Survey [13], Gold sample of Hubble Space Telescope [14]), CMB (WMAP, BOOMERANG) [15] and large scale structure (SDSS) [16] do not rule out DE with a dynamical equation of state parameter that can evol”
• Constraints on holographic dark energy from the latest supernovae, galaxy clustering, and cosmic microwave background anisotropy observations (2007, background): “96) from the first year release of the Supernova Legacy Survey (SNLS) sample [80] out of a total of 73 distant SNIa.”
• Observables sensitive to absolute neutrino masses. II (2008, background): “07 [20], and the luminosity distance SN-Ia data of [21]; (4) the data in (3) plus the BAO data from [22]; (5) the data in (4), plus the small scale primordial spectrum from Lyman-alpha (Lyα) forest clouds [23, 24].”
• Revisiting Bimaximal Neutrino Mixing in a Model with S(4) Discrete Symmetry (2009, methodology): “60 eV corresponds to the combination of the Cosmic Microwave Background (CMB) anisotropy data (from WMAP 5y [24], Arcminute Cosmology Bolometer Array Receiver (ACBAR) [25], Very Small Array (VSA) [26], Cosmic Background Imager (CBI) [27] and BOOMERANG [28] experiments) plus the large-scale structure”
• Lyman-alpha constraints on warm and on warm-plus-cold dark matter models (2008, background): “We performed a Bayesian parameter estimation for the ΛCWDM model, using the following data set: VHS Ly-α data; WMAP5 [118] and small-scale CMB experiments (ACBAR [119], CBI [120], Boomerang [121, 122, 123, 124]); galaxy power spectrum from the SDSS LRGs [125]; supernovae from the SNLS [126].”
• Modified Gravity and Cosmology (2011, methodology): “Rydbeck, Fairnbairm and Goobar [1080] repeated the analysis of [467] by including SN-Ia data from ESSENCE [893, 1280], and constraints on the CMB shift parameter from WMAP-3 [1173] to disfavour the self-accelerating model at the 1 − 2σ level, depending on whether a peculiar velocity error on the SN-”
• From cosmic deceleration to acceleration: new constraints from SN Ia and BAO/CMB (2012, methodology): “in [10] two different SN Ia datasets were used: the Gold182 sample [22], processed with the light-curve fitter MLCS2k2, and the SNLS survey [23], analyzed with SALT.”