Constraints on Cosmological Parameters from MAXIMA-1

By A. Balbi, P. Ade, J. Bock, J. Borrill, A. Boscaleri, P. Bernardis, Pedro G. Ferreira, S. Hanany, V. Hristov, Andrew H. Jaffe and 9 more. 2000

345 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/3c1a9d81e321ff05fa3ee37fb3f5ce226bca9397

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Citations in the corpus

• The First Cosmic Structures and Their Effects (2004, background): “The baryon contribution to matter, Ωbh 2 ≈ 0.020 − 0.030, is derived through measurements of CMB anisotropies (Balbi et al. 2000, 2001; Pryke et al. 2002) and D/H abundance in quasars spectra (Tytler et al. 2000; Pettini & Bowen 2001; Levshakov et al. 2002).”
• Multiple Peaks in the Angular Power Spectrum of the Cosmic Microwave Background: Significance and Consequences for Cosmology (2001, methodology): “…improving the constraints obtained from previous CMB analyses (see e.g. Dodelson & Knox 2000; Melchiorri et al. 1999; Lange et al. 2001; Balbi et al. 2000; Tegmark & Zaldarriaga 2000; Jaffe et al. 2001; Kinney et al. 2000; Bond et al. 2000; Bridle et al. 2000) on key cosmological…”
• Toward a Measurement of the Cosmological Geometry at z ~ 2: Predicting Lyα Forest Correlation in Three Dimensions and the Potential of Future Data Sets (2001, methodology): “…microwave background (CMB) anisotropy measurements, which constrain m þ , and will be a cross-check on the Type Ia supernova (SN Ia) measurements, which have contours similar to the Ly forest test (recent CMB and SN Ia constraints are combined in de Bernardis et al. 2000 and Balbi et al. 2000).”
• Cosmological Constraints from a Combination of Galaxy Clustering and Lensing -- III. Application to SDSS Data (2012, background): “…supported by the location of the first peak in the angular power spectrum of cosmic microwave background c© 2008 RAS (CMB) temperature fluctuations (e.g., Balbi et al. 2000; Lange et al. 2001; Pryke et al. 2002; Netterfield et al. 2002; Ruhl et al. 2003) combined with the results on the Hubble…”
• Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from two decades of spectroscopic surveys at the Apache Point Observatory (2020, result): “…in the cosmic microwave background (CMB), which provided the first convincing evidence for a nearly flat geometry (de Bernardis et al. 2000; Balbi et al. 2000; Jaffe et al. 2001) when assuming weak priors and fitting results from the BOOMERanG (Netterfield et al. 2002) and MAXIMA (Hanany…”
• The Detectability of the First Stars and Their Cluster Enrichment Signatures (2003, background): “The choice of these parameters is based mainly on measurements of cosmic microwave background anisotropies (e.g., Balbi et al. 2000; Netterfield et al. 2002; Pryke et al. 2002) and the abundance of galaxy clusters (e.g., Viana & Liddle 1996).”
• A High Spatial Resolution Analysis of the MAXIMA-1 Cosmic Microwave Background Anisotropy Data (2001, background): “The model has (Ωb, Ωcdm, ΩΛ, n, h) = (0.07, 0.61, 0.23, 1, 0.60) (Balbi et al. 2000).”
• The Deuterium to Hydrogen Abundance Ratio toward a Fourth QSO: HS 0105+1619 (2000, background): “Recent measurements of Ωbh 2 from the CMB are in agreement with our value from D/H and SBBN. Compared to our more accurate Ωbh 2 value, the value from BOOMERANG (Lange et al. 2000: Ωbh 2= 0.031± 0.004) is approximately 3σ higher, that from MAXIMA-I (Balbi et al. 2000: Ωbh 2= 0.025 ± 0.010) is 0.5σ h”
• Cosmological Implications of the MAXIMA-1 High-Resolution Cosmic Microwave Background Anisotropy Measurement (2001, background): “The best fit model parameters (Ωb,Ωcdm,ΩΛ, τc,ns,h) = (0.07,0.68,0.1,0.0,1.025,0.63) are characterized by high matter and low vacuum energy content (see also Balbi et al. 2000).”
• Signatures of short distance physics in the cosmic microwave background (2002, methodology): “This is directly measured by the COBE [6] satellite, and by the BOOMERanG [22] and MAXIMA [23] experiments, which set the normalization”