Cosmological parameters from the first results of Boomerang

By A. Lange, P. Ade, J. Bock, J. Richard Bond, J. Borrill, A. Boscaleri, K. Coble, B. Crill, P. Bernardis, P. Farese and 22 more. 2001

250 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/75e51518b747bdcb77cd883a5e81abf2a77b05d1

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Citations in the corpus

A Measurement by BOOMERANG of Multiple Peaks in the Angular Power Spectrum of the Cosmic Microwave Background (2001, methodology): “Thus, just as in Lange et al. (2001), caseswith the weak priors applied are the focus of theextraction.”
Cosmological constraints from archeops (2002, background): “The spectacular results of Boomerang and Maxima have firmly established the fact that the geometry of the Universe is very close to flat (de Bernardis et al. 2000; Hanany et al. 2000; Lange et al. 2001; Balbi et al. 2000).”
Probing Dark Energy with Baryonic Acoustic Oscillations from Future Large Galaxy Redshift Surveys (2003, background): “…on how the combination of CMB anisotropy data and large-scale structure data, either present (Scott, Silk, & White 1995; Gawiser & Silk 1998; Lange et al. 2001; Tegmark et al. 2001; Efs- 1 2 tathiou et al. 2002; Spergel et al. 2003) or future (Hu et al. 1998; Eisenstein et al. 1998; Wang,…”
On the quantum origin of the seeds of cosmic structure (2005, methodology): “T (1) ii = −Φφ̇(2)0 + φ̇0δφ̇− Ψ(φ̇(2)0 − a(2)V [φ0]) − 1 2 a(2)∂φV [φ]δφ”
Cosmological Parameters from the 2003 Flight of BOOMERANG (2005, methodology): “Besides being generally agreed upon by cosmologists, our weak priors are consistent with those used in much of the CMB literature, e.g., Lange et al. (2001), Bond et al. (2003) and Readhead et al. (2004b).”
Median Statistics, H0, and the Accelerating Universe (2000, background): “…; Dodelson & Knox 2000 ; Peterson et al. 2000 ; Page 1999 ; Melchiorri et al. 2000 ; Tegmark & Zaldarriaga 2000 ; Knox & Page 2000 ; Le Dour et al. 2000), such suggestions must be viewed as tentative (see discussion in Ratra et al. 1999 and references therein) ; see, however, Lange et al. (2001).”
Feedback from Galaxy Formation: Production and Photodissociation of Primordial H2 (2000, unknown): “Recent measurements of the Cosmic Microwave Background (CMB) anisotropies (de Bernardis et al. 2000; Lange et al. 2001; Tegmark et al. 2000), large-scale structure (Hamilton & Tegmark 2000), Lyα power spectrum (Croft et al. 1999; McDonald et al. 2000), and distances of high redshift SNe (Perlmutter…”