Publications
368 results found
Masi S, De Bernardis P, De Troia G, et al., 2002, The BOOMERanG experiment and the curvature of the Universe, International School of Nuclear Physics, Publisher: ELSEVIER SCIENCE BV, Pages: 243-261, ISSN: 0146-6410
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- Citations: 78
Jaffe AH, 2002, A new era in the Cosmic Microwave Background: the CMB in 2002, San Francisco, Conference on a new era in cosmology, University of Durham, Durham, England, 11 - 15 September 2001, Publisher: Astronomical Society of the Pacific, Pages: 141-153
Richards PL, Abroe M, Ade P, et al., 2002, The Maxima and Maxipol experiments, Workshop on experimental cosmology at millimetre wavelengths, Breuil Cervinia, Italy, Publisher: American Institute of Physics, Pages: 12-17
Jaffe AH, 2002, Modern measurements of the cosmic microwave background, The Observatory, Vol: Need volume number, ISSN: 0029-7704
Balbi A, Ade P, Bock J, et al., 2002, Constraints on cosmological parameters from MAXIMA-1, 9th Marcel Grossman meeting on recent developments in theoretical and experimental general relativity, gravitation, and relativistic field theories, Rome, July 2000, Publisher: World Scientific, Pages: 2195-2196
de, Bernardis P, Ade PAR, et al., 2002, l-space spectroscopy of the Cosmic Microwave Background with the BOOMERanG experiment, Melville, Breuil-Cervinia workshop on experimental cosmology at millimetre wavelengths, Bruil-Cervinia, Italy, 9 - 13 July 2001, Publisher: American of Institute of Physics, Pages: 3-11
Wu JHP, Balbi A, Borrill J, et al., 2001, Tests for Gaussianity of the MAXIMA-1 cosmic microwave background map, PHYSICAL REVIEW LETTERS, Vol: 87, ISSN: 0031-9007
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- Citations: 84
Wu JHP, Balbi A, Borrill J, et al., 2001, Tests for Gaussianity of the MAXIMA-1 cosmic microwave background map, Physical Review Letters, Vol: 87, ISSN: 0031-9007
A series of Gaussianity tests were performed on the MAXIMA-1 CMB map. To optimize both the resolution and the signal-to-noise ratio for these tests, a map with 5972 square pixels of 8' each was used. Using these high-quality data, the Gaussianity of CMB anisotropy on subdegree scales was probed for the first time. It was found that the MAXIMA-1 CMB map is consistent with Gaussianity on angular scales between 10 arcmin and 5 deg.
Lee AT, Ade P, Balbi A, et al., 2001, A high spatial resolution analysis of the MAXIMA-1 cosmic microwave background anisotropy data, ASTROPHYSICAL JOURNAL, Vol: 561, Pages: L1-L5, ISSN: 0004-637X
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- Citations: 343
Stompor R, Abroe M, Ade P, et al., 2001, Cosmological implications of the MAXIMA-1 high-resolution cosmic microwave background anisotropy measurement, ASTROPHYSICAL JOURNAL, Vol: 561, Pages: L7-L10, ISSN: 0004-637X
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- Citations: 245
, 2001, ERRATUM, The Astrophysical Journal, Vol: 558, Pages: L145-L145, ISSN: 0004-637X
Gnedin NY, Jaffe AH, 2001, Secondary cosmic microwave background anisotropies from cosmological reionization, ASTROPHYSICAL JOURNAL, Vol: 551, Pages: 3-14, ISSN: 0004-637X
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- Citations: 44
Jaffe AH, Ade PAR, Balbi A, et al., 2001, Cosmology from MAXIMA-1, BOOMERANG, and COBE DMR cosmic microwave background observations, PHYSICAL REVIEW LETTERS, Vol: 86, Pages: 3475-3479, ISSN: 0031-9007
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- Citations: 465
Gnedin NY, Jaffe AH, 2001, Secondary cosmic microwave background anisotropies from cosmological reionization, Astrophysical Journal, Vol: 551, Pages: 3-14, ISSN: 0004-637X
We use numerical simulations of cosmological reionization to calculate the secondary CMB anisotropies in a representative flat low-density cosmological model. We show that the kinetic Sunyaev-Zeldovich effect (scattering off of moving electrons in the ionized intergalactic medium) is dominated by the nonlinear hydrodynamic and gravitational evolution of the density and velocity fields, rather than the detailed distribution of the ionization fraction (" patchy reionization ") on all angular scales. Combining our results with the recent calculation of secondary CMB anisotropies by Springel et al., we are able to accurately predict the power spectrum of the kinetic SZ effect on almost all angular scales.
Bergström L, Goobar A, Jaffe AH, 2001, <i>Cosmology and Particle Astrophysics</i>, American Journal of Physics, Vol: 69, Pages: 394-394, ISSN: 0002-9505
Lange AE, Ade PAR, Bock JJ, et al., 2001, Cosmological parameters from the first results of boomerang, PHYSICAL REVIEW D, Vol: 63, ISSN: 1550-7998
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- Citations: 323
Lange AE, Ade PAR, Bock JJ, et al., 2001, Cosmological parameters from the first results of Boomerang, Physical Review D, Vol: 63, ISSN: 0556-2821
The anisotropy of the cosmic microwave background radiation contains information about the contents and history of the universe. We report new limits on cosmological parameters derived from .the angular power spectrum measured in the first Antarctic flight of the Boomerang experiment. Within the framework of models, : with adiabatic perturbations, and using only'weakly restrictive prior probabilities on the age of the universe and the Hubble expansion parameter h, we find.that the curvature is consistent with flat and that the primordial fluctuation spectrum is consistent with scale invariant, in agreement with the basic inflation paradigm. We find that the data prefer a baryon density Ωbh2 above, though similar to, the estimates from light element abundances and big bang nucleosynthesis. When combined with large scale structure observations, the Boomerang data provide clear detections of both dark matter and dark energy contributions to the total energy density fltot, independent of data from high-redshift supernovae. ©2001 The American Physical Society.
Wu JHP, Balbi A, Borrill J, et al., 2001, Asymmetric beams in cosmic microwave background anisotropy experiments, ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, Vol: 132, Pages: 1-17, ISSN: 0067-0049
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- Citations: 47
Balbi A, Ade P, Bock J, et al., 2001, [no title supplied on import], Memorie - Societa Astronomica Italiana, Vol: 72, Pages: 849-852, ISSN: 0037-8720
de, Bernardis P, Ade PAR, et al., 2001, First results from the BOOMERanG experiment, Melville, International conference on cosmology and particle physics (CAPP 2000), Verberier, Switzerland, 17 - 28 July 2000, Publisher: American Institute of Physics, Pages: 85-94
Borrill J, Ferreira PG, Jaffe AH, et al., 2001, Cosmic microwave background data analysis with MADCAP, Berlin, MPA/ESO/MPE workshop on mining the sky, Garching, Germany, 31 July - 4 August 2000, Publisher: Springer-Verlag, Pages: 403-413
Winant C, Abroe M, Ade P, et al., 2001, MAXIMA: Millimeter-wave anisotropy experiment imaging array, Melville, 20th Texas symposium on relativistic astrophysics, Austin, Texas, 10 - 15 December 2000, Publisher: American Institute of Physics, Pages: 214-216
Prunet S, Ade PAR, Bock JJ, et al., 2001, Noise estimation in CMB time-streams and fast iterative map-making, Berlin, MPA/ESO/MPE workshop on mining the sky, Garching, Germany, 31 July - 4 August 2000, Publisher: Springer-Verlag, Pages: 421-427
Church S, Jaffe AH, Knox L, 2001, CMB and inflation: the report from SNOWMASS 2001 (P406), Snowmass 2001: the future of particle physics, Snowmass, Colorado, 30 June - 21 July 2001, Publisher: SLAC Technical Publications
Kamionkowski M, Jaffe AH, 2001, Detection of gravitational waves from inflation, International Journal of Modern Physics A, Vol: 16, Pages: 116-128, ISSN: 0217-751X
de, Bernardis P, Ade PAR, et al., 2001, Images of the early universe from the BOOMERanG experiment, Melville, 20th texas symposium on relativistic astrophysics, Austin, Texas, 10 - 15 2000, Publisher: American Institute of Physics, Pages: 157-171
de, Bernardis P, Ade PAR, et al., 2001, The deepest field, Berlin, ESO workshop on deep fields, Garching, Germany, 9 -12 October 2000, Publisher: Springer-Verlag, Pages: 362-368
Hanany S, Ade P, Balbi A, et al., 2000, MAXIMA-1: A measurement of the cosmic microwave background anisotropy on angular scales of 10′-5°, Astrophysical Journal, Vol: 545, ISSN: 0004-637X
We present a map and an angular power spectrum of the anisotropy of the cosmic microwave background (CMB) from the first flight of the Millimeter-wave Anisotropy Experiment Imaging Array (MAXIMA). MAXIMA is a balloon-borne experiment with an array of 16 bolometric photometers operated at 100 mK. MAXIMA observed a 124 deg2 region of the sky with 10′ resolution at frequencies of 150, 240, and 410 GHz. The data were calibrated using in-flight measurements of the CMB dipole anisotropy. A map of the CMB anisotropy was produced from three 150 and one 240 GHz photometer without need for foreground subtractions. Analysis of this CMB map yields a power spectrum for the CMB anisotropy over the range 36 ≤ l ≤ 785. The spectrum shows a peak with an amplitude of 78 ± 6 μK at l ≃ 220 and an amplitude varying between ∼40 and ∼50 μK for 400 ≲ l ≲ 785.
Hanany S, Ade P, Balbi A, et al., 2000, MAXIMA-1: A Measurement of the Cosmic Microwave Background Anisotropy on Angular Scales of 10[arcmin]–5°, The Astrophysical Journal, Vol: 545, Pages: L5-L9, ISSN: 0004-637X
Balbi A, Ade P, Bock J, et al., 2000, Constraints on Cosmological Parameters from MAXIMA-1, The Astrophysical Journal, Vol: 545, Pages: L1-L4, ISSN: 0004-637X
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