473 results on '"Hanany S"'
Search Results
152. Tests for Gaussianity of the MAXIMA-1 Cosmic Microwave Background Map
- Author
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Wu, J. H. P., primary, Balbi, A., additional, Borrill, J., additional, Ferreira, P. G., additional, Hanany, S., additional, Jaffe, A. H., additional, Lee, A. T., additional, Rabii, B., additional, Richards, P. L., additional, Smoot, G. F., additional, Stompor, R., additional, and Winant, C. D., additional
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- 2001
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153. A High Spatial Resolution Analysis of the MAXIMA-1 Cosmic Microwave Background Anisotropy Data
- Author
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Lee, A. T., primary, Ade, P., additional, Balbi, A., additional, Bock, J., additional, Borrill, J., additional, Boscaleri, A., additional, de Bernardis, P., additional, Ferreira, P. G., additional, Hanany, S., additional, Hristov, V. V., additional, Jaffe, A. H., additional, Mauskopf, P. D., additional, Netterfield, C. B., additional, Pascale, E., additional, Rabii, B., additional, Richards, P. L., additional, Smoot, G. F., additional, Stompor, R., additional, Winant, C. D., additional, and Wu, J. H. P., additional
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- 2001
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154. Cosmological Implications of the MAXIMA-1 High-Resolution Cosmic Microwave Background Anisotropy Measurement
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Stompor, R., primary, Abroe, M., additional, Ade, P., additional, Balbi, A., additional, Barbosa, D., additional, Bock, J., additional, Borrill, J., additional, Boscaleri, A., additional, de Bernardis, P., additional, Ferreira, P. G., additional, Hanany, S., additional, Hristov, V., additional, Jaffe, A. H., additional, Lee, A. T., additional, Pascale, E., additional, Rabii, B., additional, Richards, P. L., additional, Smoot, G. F., additional, Winant, C. D., additional, and Wu, J. H. P., additional
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- 2001
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155. Cosmology from MAXIMA-1, BOOMERANG, and COBE DMR Cosmic Microwave Background Observations
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Jaffe, A. H., primary, Ade, P. A. R., additional, Balbi, A., additional, Bock, J. J, additional, Bond, J. R., additional, Borrill, J., additional, Boscaleri, A., additional, Coble, K., additional, Crill, B. P., additional, de Bernardis, P., additional, Farese, P., additional, Ferreira, P. G., additional, Ganga, K., additional, Giacometti, M., additional, Hanany, S., additional, Hivon, E., additional, Hristov, V. V., additional, Iacoangeli, A., additional, Lange, A. E., additional, Lee, A. T., additional, Martinis, L., additional, Masi, S., additional, Mauskopf, P. D., additional, Melchiorri, A., additional, Montroy, T., additional, Netterfield, C. B., additional, Oh, S., additional, Pascale, E., additional, Piacentini, F., additional, Pogosyan, D., additional, Prunet, S., additional, Rabii, B., additional, Rao, S., additional, Richards, P. L., additional, Romeo, G., additional, Ruhl, J. E., additional, Scaramuzzi, F., additional, Sforna, D., additional, Smoot, G. F., additional, Stompor, R., additional, Winant, C. D., additional, and Wu, J. H. P., additional
- Published
- 2001
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156. The MAXIMA and MAXIPOL experiments.
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Richards, P. L., Abroe, M., Ade, P., Balbi, A., Bock, J., Borrill, J., Boscaleri, A., de Bernardis, P., Collins, J., Ferreira, P. G., Hanany, S., Hristov, V. V., Jaffe, A. H., Johnson, B., Lee, A. T., Matsumu, T., Mauskopf, P. D., Netterfield, C. B., Pascale, E., and Rabii, B.
- Subjects
BOLOMETERS ,ANISOTROPY ,POWER spectra ,MEASUREMENT - Abstract
MAXIMA is a balloon-based bolometric experiment to measure the temperature anisotropy of the CMB over spatial frequency range 36≤l≤1235. The MAXIMA-1 flight produced a 124 square degree temperature anisotropy map with a beam diameter of 10 arcmin. These data have been used to produce a power spectrum which is in excellent agreement with data from BOOMERANG and DASI, but covers a wider range of angular scales. The MAXIMA power spectrum is consistent with the prediction of Λ CDM models and has been used to constrain cosmological models. The MAXIMA experiment is described and an outline is given of the contents and significance of papers written by the MAXIMA team. MAXIMA is being modified to measure the polarization anisotropy of the CMB. A brief description of this MAXIPOL experiment is also given. © 2002 American Institute of Physics. [ABSTRACT FROM AUTHOR]
- Published
- 2002
157. Asymmetric Beams in Cosmic Microwave Background Anisotropy Experiments
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Wu, J. H. P., primary, Balbi, A., additional, Borrill, J., additional, Ferreira, P. G., additional, Hanany, S., additional, Jaffe, A. H., additional, Lee, A. T., additional, Oh, S., additional, Rabii, B., additional, Richards, P. L., additional, Smoot, G. F., additional, Stompor, R., additional, and Winant, C. D., additional
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- 2001
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158. Cosmological constraints from Archeops
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Benoît, A., Ade, P., Amblard, A., Ansari, R., Aubourg, É., Bargot, S., Bartlett, J. G., Bernard, J.–Ph., Bhatia, R. S., Blanchard, A., Bock, J. J., Boscaleri, A., Bouchet, F. R., Bourrachot, A., Camus, P., Couchot, F., de Bernardis, P., Delabrouille, J., Désert, F.–X., Doré, O., Douspis, M., Dumoulin, L., Dupac, X., Filliatre, P., Fosalba, P., Ganga, K., Gannaway, F., Gautier, B., Giard, M., Giraud–Héraud, Y., Gispert, R., Guglielmi, L., Hamilton, J.–Ch., Hanany, S., Henrot–Versillé, S., Kaplan, J., Lagache, G., Lamarre, J.–M., Lange, A. E., Macías–Pérez, J. F., Madet, K., Maffei, B., Magneville, Ch., Marrone, D. P., Masi, S., Mayet, F., Murphy, A., Naraghi, F., Nati, F., Patanchon, G., Perrin, G., Piat, M., Ponthieu, N., Prunet, S., Puget, J.–L., Renault, C., Rosset, C., Santos, D., Starobinsky, A., Strukov, I., Sudiwala, R. V., Teyssier, R., Tristram, M., Tucker, C., Vanel, J.–C., Vibert, D., Wakui, E., Yvon, D., Benoît, A., Ade, P., Amblard, A., Ansari, R., Aubourg, É., Bargot, S., Bartlett, J. G., Bernard, J.–Ph., Bhatia, R. S., Blanchard, A., Bock, J. J., Boscaleri, A., Bouchet, F. R., Bourrachot, A., Camus, P., Couchot, F., de Bernardis, P., Delabrouille, J., Désert, F.–X., Doré, O., Douspis, M., Dumoulin, L., Dupac, X., Filliatre, P., Fosalba, P., Ganga, K., Gannaway, F., Gautier, B., Giard, M., Giraud–Héraud, Y., Gispert, R., Guglielmi, L., Hamilton, J.–Ch., Hanany, S., Henrot–Versillé, S., Kaplan, J., Lagache, G., Lamarre, J.–M., Lange, A. E., Macías–Pérez, J. F., Madet, K., Maffei, B., Magneville, Ch., Marrone, D. P., Masi, S., Mayet, F., Murphy, A., Naraghi, F., Nati, F., Patanchon, G., Perrin, G., Piat, M., Ponthieu, N., Prunet, S., Puget, J.–L., Renault, C., Rosset, C., Santos, D., Starobinsky, A., Strukov, I., Sudiwala, R. V., Teyssier, R., Tristram, M., Tucker, C., Vanel, J.–C., Vibert, D., Wakui, E., and Yvon, D.
- Abstract
We analyze the cosmological constraints that Archeops (Benoît et al. 2003) places on adiabatic cold dark matter models with passive power-law initial fluctuations. Because its angular power spectrum has small bins in $\ell$and large $\ell$coverage down to COBE scales, Archeops provides a precise determination of the first acoustic peak in terms of position at multipole $l_{\rm peak}=220\pm 6$, height and width. An analysis of Archeops data in combination with other CMB datasets constrains the baryon content of the Universe, $\Omega_{\rm b}h^2= 0.022^{+0.003}_{-0.004}$, compatible with Big-Bang nucleosynthesis and with a similar accuracy. Using cosmological priors obtained from recent non–CMB data leads to yet tighter constraints on the total density, e.g. $\Omega_{\rm tot}=1.00^{+0.03}_{-0.02}$using the HST determination of the Hubble constant. An excellent absolute calibration consistency is found between Archeops and other CMB experiments, as well as with the previously quoted best fit model. The spectral index nis measured to be $1.04^{+0.10}_{-0.12}$when the optical depth to reionization, τ, is allowed to vary as a free parameter, and $0.96^{+0.03}_{-0.04}$when τis fixed to zero, both in good agreement with inflation.
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- 2003
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159. Constraints on Cosmological Parameters from MAXIMA-1
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Balbi, A., primary, Ade, P., additional, Bock, J., additional, Borrill, J., additional, Boscaleri, A., additional, De Bernardis, P., additional, Ferreira, P. G., additional, Hanany, S., additional, Hristov, V., additional, Jaffe, A. H., additional, Lee, A. T., additional, Oh, S., additional, Pascale, E., additional, Rabii, B., additional, Richards, P. L., additional, Smoot, G. F., additional, Stompor, R., additional, Winant, C. D., additional, and Wu, J. H. P., additional
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- 2000
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160. MAXIMA-1: A Measurement of the Cosmic Microwave Background Anisotropy on Angular Scales of 10[arcmin]–5°
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Hanany, S., primary, Ade, P., additional, Balbi, A., additional, Bock, J., additional, Borrill, J., additional, Boscaleri, A., additional, de Bernardis, P., additional, Ferreira, P. G., additional, Hristov, V. V., additional, Jaffe, A. H., additional, Lange, A. E., additional, Lee, A. T., additional, Mauskopf, P. D., additional, Netterfield, C. B., additional, Oh, S., additional, Pascale, E., additional, Rabii, B., additional, Richards, P. L., additional, Smoot, G. F., additional, Stompor, R., additional, Winant, C. D., additional, and Wu, J. H. P., additional
- Published
- 2000
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161. Applications of wavelets to the analysis of cosmic microwave background maps
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Tenorio, L., primary, Jaffe, A. H., additional, Hanany, S., additional, and Lineweaver, C. H., additional
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- 1999
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162. MAXIMA: an experiment to measure temperature anisotropy in the cosmic microwave background
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Lee, A. T., primary, Ade, P., additional, Balbi, A., additional, Bock, J., additional, Borrill, J., additional, Boscaleri, A., additional, Crill, B. P., additional, De Bernardis, P., additional, Del Castillo, H., additional, Ferreira, P., additional, Ganga, K., additional, Hanany, S., additional, Hristov, V., additional, Jaffe, A. H., additional, Lange, A. E., additional, Mauskopf, P., additional, Netterfield, C. B., additional, Oh, S., additional, Pascale, E., additional, Rabii, B., additional, Richards, P. L., additional, Ruhl, J., additional, Smoot, G. F., additional, and Winant, C. D., additional
- Published
- 1999
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163. The effect of the detector response time on bolometric cosmic microwave background anisotropy experiments
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Hanany, S., primary, Jaffe, A. H., additional, and Scannapieco, E., additional
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- 1998
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164. The Second Measurement of Anisotropy in the Cosmic Microwave Background Radiation at 0[fdg]5 Scales near the Star μ Pegasi
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Lim, M. A., primary, Clapp, A. C., additional, Devlin, M. J., additional, Figueiredo, N., additional, Gundersen, J. O., additional, Hanany, S., additional, Hristov, V. V., additional, Lange, A. E., additional, Lubin, P. M., additional, Meinhold, P. R., additional, Richards, P. L., additional, Staren, J. W., additional, Smoot, G. F., additional, and Tanaka, S. T., additional
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- 1996
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165. Measurements of Anisotropy in the Cosmic Microwave Background Radiation at 0[fdg]5 Scales near the Stars HR 5127 and φ Herculis
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Tanaka, S. T., primary, Clapp, A. C., additional, Devlin, M. J., additional, Figueiredo, N., additional, Gundersen, J. O., additional, Hanany, S., additional, Hristov, V. V., additional, Lange, A. E., additional, Lim, M. A., additional, Lubin, P. M., additional, Meinhold, P. R., additional, Richards, P. L., additional, Smoot, G. F., additional, and Staren, J., additional
- Published
- 1996
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166. Grain Alignment by Ambipolar Diffusion in Molecular Clouds
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Roberge, W. G., primary, Hanany, S., additional, and Messinger, D. W., additional
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- 1995
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167. Systematic errors in polarization-dependent electron yield experiments
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Hanany, S., primary, Shaw, P.S., additional, Liu, Y., additional, Santangelo, A., additional, Kaaret, P., additional, and Novick, R., additional
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- 1995
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168. Measurement of the electron yield of CsI with polarized x rays
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Hanany, S., primary, Shaw, P. S., additional, Liu, Y., additional, Santangelo, A., additional, Kaaret, P., additional, and Novick, R., additional
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- 1993
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169. THE IMPACT OF THE SPECTRAL RESPONSE OF AN ACHROMATIC HALF-WAVE PLATE ON THE MEASUREMENT OF THE COSMIC MICROWAVE BACKGROUND POLARIZATION.
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C. BAO, GOLD, B., BACCIGALUPI, C., DIDIER, J., HANANY, S., JAFFE, A., JOHNSON, B. R., LEACH, S., MATSUMURA, T., MILLER, A., and O'DEA, D.
- Subjects
LINEAR polarization ,COSMIC background radiation ,ASTROPHYSICS ,GRAVITATIONAL waves ,POLARIZATION spectroscopy - Abstract
We study the impact of the spectral dependence of the linear polarization rotation induced by an achromatic half-wave plate on measurements of cosmic microwave background polarization in the presence of astrophysical foregrounds. We focus on the systematic effects induced on the measurement of inflationary gravitational waves by uncertainties in the polarization and spectral index of Galactic dust. We find that for the experimental configuration and noise levels of the balloon-borne EBEX experiment, which has three frequency bands centered at 150, 250, and 410 GHz, a crude dust subtraction process mitigates systematic effects to below detectable levels for 10% polarized dust and tensor-to-scalar ratio of as low as r = 0.01. We also study the impact of uncertainties in the spectral response of the instrument. With a top-hat model of the spectral response for each band, characterized by band center and bandwidth, and with the same crude dust subtraction process, we find that these parameters need to be determined to within 1 and 0.8 GHz at 150 GHz; 9 and 2.0 GHz at 250 GHz; and 20 and 14 GHz at 410 GHz, respectively. The approach presented in this paper is applicable to other optical elements that exhibit polarization rotation as a function of frequency. [ABSTRACT FROM AUTHOR]
- Published
- 2012
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170. Frequentist estimation of cosmological parameters from theMAXIMA-1 cosmic microwave background anisotropy data.
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Abroe, M. E., Balbi, A., Borrill, J., Bunn, E. F., Hanany, S., Ferreira, P. G., Jaffe, A. H., Lee, A. T., Olive, K. A., Rabii, B., Richards, P. L., Smoot, G. F., Stompor, R., Winant, C. D., and Wu, J. H. P.
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COSMIC background radiation ,ASTROPHYSICAL radiation - Abstract
We use a frequentist statistical approach to set confidence intervals on the values of cosmological parameters using the MAXIMA-1 and COBE measurements of the angular power spectrum of the cosmic microwave background. We define a Δχ² statistic, simulate the measurements of MAXIMA-1 and COBE, determine the probability distribution of the statistic, and use it and the data to set confidence intervals on several cosmological parameters. We compare the frequentist confidence intervals with Bayesian credible regions. The frequentist and Bayesian approaches give best estimates for the parameters that agree within 15 per cent, and confidence interval widths that agree to within 30 per cent. The results also suggest that a frequentist analysis gives slightly broader confidence intervals than a Bayesian analysis. The frequentist analysis gives values of Ω = 089[sup +0.26, sub -0.19], Ω[sub B]h² = 0.026[sup + 0.020,sub 0.011] and n = 1.02[sup +0.31, sub -0.10], and the Bayesian analysis gives values of Ω = 0.98[sup +0.14, sub -0.19], Ω[sub B]h² = 0.029[sup +0.015, sub -0.010] and n = 1.18[sup +0.10, sub -0.23], all at the 95 per cent confidence level. [ABSTRACT FROM AUTHOR]
- Published
- 2002
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171. Neutrino Physics from the Cosmic Microwave Background and Large Scale Structure
- Author
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Abazajian, K. N., Arnold, K., Austermann, J., Benson, B. A., Bischoff, Colin A., Bock, J., Bond, J. R., Borrill, J., Calabrese, E., Carlstrom, J. E., Carvalho, C. S., Chang, C. L., Chiang, H. C., Church, S., Cooray, A., Crawford, T. M., Dawson, K. S., Das, S., Devlin, M. J., Dobbs, M., Dodelson, S., Doré, O., Dunkley, J., Errard, J., Fraisse, A., Gallicchio, J., Halverson, N. W., Hanany, S., Hildebrandt, S. R., Hincks, A., Hlozek, R., Holder, G., Holzapfel, W. L., Honscheid, K., Hu, W., Hubmayr, J., Irwin, K., Jones, W. C., Kamionkowski, M., Keating, B., Keisler, R., Knox, L., Komatsu, E., Kovac, John M, Kuo, C.-L., Lawrence, C., Lee, A. T., Leitch, E., Linder, E., Lubin, P., McMahon, J., Miller, A., Newburgh, L., Niemack, M. D., Nguyen, H., Nguyen, H. T., Page, L., Pryke, C., Reichardt, C. L., Ruhl, J. E., Sehgal, N., Seljak, U., Sievers, J., Silverstein, E., Slosar, A., Smith, K. M., Spergel, D., Staggs, S. T., Stark, Antony A., Stompor, R., Vieregg, A. G., Wang, G., Watson, S., Wollack, E. J., Wu, W. L. K., Yoon, K. W., and Zahn, O.
- Abstract
This is a report on the status and prospects of the quantification of neutrino properties through the cosmological neutrino background for the Cosmic Frontier of the Division of Particles and Fields Community Summer Study long-term planning exercise. Experiments planned and underway are prepared to study the cosmological neutrino background in detail via its influence on distance-redshift relations and the growth of structure. The program for the next decade described in this document, including upcoming spectroscopic galaxy surveys eBOSS and DESI and a new Stage-IV CMB polarization experiment CMB-S4, will achieve sigma(sum m_nu) = 16 meV and sigma(N_eff) = 0.020. Such a mass measurement will produce a high significance detection of non-zero sum m_nu, whose lower bound derived from atmospheric and solar neutrino oscillation data is about 58 meV. If neutrinos have a minimal normal mass hierarchy, this measurement will definitively rule out the inverted neutrino mass hierarchy, shedding light on one of the most puzzling aspects of the Standard Model of particle physics --- the origin of mass. This precise a measurement of N_eff will allow for high sensitivity to any light and dark degrees of freedom produced in the big bang and a precision test of the standard cosmological model prediction that N_eff = 3.046., Astronomy
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- 2013
172. Inflation Physics from the Cosmic Microwave Background and Large Scale Structure
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Abazajian, K. N., Arnold, K., Austermann, J., Benson, B. A., Bischoff, Colin A., Bock, J., Bond, J. R., Borrill, J., Buder, Immanuel D., Burke, D. L., Calabrese, E., Carlstrom, J. E., Carvalho, C. S., Chang, C. L., Chiang, H. C., Church, S., Cooray, A., Crawford, T. M., Crill, B. P., Dawson, K. S., Das, S., Devlin, M. J., Dobbs, M., Dodelson, S., Doré, O., Dunkley, J., Feng, J. L., Fraisse, A., Gallicchio, J., Giddings, S. B., Green, D., Halverson, N. W., Hanany, S., Hanson, D., Hildebrandt, S. R., Hincks, A., Hlozek, R., Holder, G., Holzapfel, W. L., Honscheid, K., Horowitz, G., Hu, W., Hubmayr, J., Irwin, K., Jackson, M., Jones, W. C., Kallosh, R., Kamionkowski, M., Keating, B., Keisler, R., Kinney, W., Knox, L., Komatsu, E., Kovac, John M, Kuo, C.-L., Kusaka, A., Lawrence, C., Lee, A. T., Leitch, E., Linde, A., Linder, E., Lubin, P., Maldacena, J., Martinec, E., McMahon, J., Miller, A., Mukhanov, V., Newburgh, L., Niemack, M. D., Nguyen, H., Nguyen, H. T., Page, L., Pryke, C., Reichardt, C. L., Ruhl, J. E., Sehgal, N., Seljak, U., Senatore, L., Sievers, J., Silverstein, E., Slosar, A., Smith, K. M., Spergel, D., Staggs, S. T., Stark, Antony A., Stompor, R., Vieregg, A. G., Wang, G., Watson, S., Wollack, E. J., Wu, W. L. K., Yoon, K. W., Zahn, O., and Zaldarriaga, M.
- Abstract
Fluctuations in the intensity and polarization of the cosmic microwave background (CMB) and the large-scale distribution of matter in the universe each contain clues about the nature of the earliest moments of time. The next generation of CMB and large-scale structure (LSS) experiments are poised to test the leading paradigm for these earliest moments---the theory of cosmic inflation---and to detect the imprints of the inflationary epoch, thereby dramatically increasing our understanding of fundamental physics and the early universe. A future CMB experiment with sufficient angular resolution and frequency coverage that surveys at least 1% of the sky to a depth of 1 uK-arcmin can deliver a constraint on the tensor-to-scalar ratio that will either result in a 5-sigma measurement of the energy scale of inflation or rule out all large-field inflation models, even in the presence of foregrounds and the gravitational lensing B-mode signal. LSS experiments, particularly spectroscopic surveys such as the Dark Energy Spectroscopic Instrument, will complement the CMB effort by improving current constraints on running of the spectral index by up to a factor of four, improving constraints on curvature by a factor of ten, and providing non-Gaussianity constraints that are competitive with the current CMB bounds., Astronomy
- Published
- 2013
173. MAXIMA: Millimeter-wave anisotropy experiment imaging array.
- Author
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Winant, C., Abroe, M., Ade, P., Balbi, A., Barbosa, D., Bock, J., Borrill, J., Boscaleri, A., Collins, J., de Bernardis, P., Ferreira, P., Hanany, S., Hristov, V., Jaffe, A. H., Johnson, B., Lange, A. E., Lee, A. T., Mauskopf, P. D., Netterfield, C. B., and Oh, S.
- Subjects
COSMIC background radiation ,ANISOTROPY ,POWER spectra ,INFLATIONARY universe ,PARAMETER estimation - Abstract
We discuss the status of the data obtained from the first two flights of the MAXIMA balloon-borne experiment. MAXIMA is sensitive to CMB fluctuations on angular scales from 10 arcmin to 5 degrees. The instrument uses a 16 element bolometric array with 3 frequency bands centered at 150, 240, and 410 GHz. An angular power spectrum of the CMB anisotropy has been obtained from the data of the first flight, MAXIMA-1, which shows a peak at ℓ ∼ 220 of 78 ± 6μK and an amplitude varying between 40 μK and 50 μK from 400 < ℓ < 785 [1]. During a second flight (MAXIMA-2), in 1999, we mapped an additional 225 square degree region of the sky, nearly twice the area of MAXIMA-1. Data from MAXIMA-1 are consistent with adiabatic inflationary models with the total energy density, Ω = 1.0[SUP+0.15,SUB-0.3], the total baryon density, Ω[SUBb]h[SUP2] = 0.03 ± 0.01, and the spectral index of the initial power spectrum, n[SUBs] = 1.08 ± 0.1 [2]. Limits are quoted at the 95% confidence level. Data from MAXIMA have been combined with those from LSS observations, SNIa observations, COBE, and BOOMERanG, and have been used for cosmological parameter estimation [3]. MAXIMA data can be obtained at http://cfpa.berkeley.edu/maxima. [ABSTRACT FROM AUTHOR]
- Published
- 2001
174. Evidence for a Flat Universe from the North American Flight of BOOMERANG
- Author
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Crill, B. P., Ade, P. A. R., Paolo de Bernardis, Bock, J. J., Borrill, J., Boscaleri, A., Gasperis, G., Troia, Grazia, Farese, P., Ferreira, P. G., Ganga, K., Giacometti, M., Hanany, S., Hivon, E. F., Hristov, V. V., Iacoangeli, Armando, Jaffe, A. H., Lange, A. E., Lee, A. T., Silvia Masi, Mauskopf, P. D., Melchiorri, Francesco, Alessandro Melchiorri, Miglio, L., Montroy, T., Netterfield, C. B., Enzo Pascale, Francesco Piacentini, Richards, L., Romeo, G., Ruhl, J. E., Scannapieco, E., Scaramuzzi, F., Stompor, R., and Vittorio, N.
175. Exploring cosmic origins with CORE: Gravitational lensing of the CMB
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Challinor, A., Allison, R., Carron, J., Errard, J., Feeney, S., Kitching, T., Lesgourgues, Julien, Lewis, A., Zubeldía, Í., Achucarro, A., Ade, P., Ashdown, M., Ballardini, M., Banday, A. J., Banerji, R., Bartlett, J., Bartolo, N., Basak, S., Baumann, D., Bersanelli, M., Bonaldi, A., Bonato, M., Borrill, J., Bouchet, F., Boulanger, F., Brinckmann, Thejs, Bucher, M., Burigana, C., Buzzelli, A., Cai, Z.-Y., Calvo, M., Carvalho, C.-S., Castellano, G., Chluba, J., Clesse, Sébastien, Colantoni, I., Coppolecchia, A., Crook, M., D'Alessandro, G., De Bernardis, Paolo, De Gasperis, G., De Zotti, Gianfranco, Delabrouille, J., Di Valentino, Eleonora, Diego, J.-M., Fernandez-Cobos, R., Ferraro, S., Finelli, F., Forastieri, F., Galli, S., Génova-Santos, Ricardo T., Gerbino, M., González-Nuevo, Joaquin, Grandis, S., Greenslade, J., Hagstotz, S., Hanany, S., Handley, W., Hernández-Monteagudo, Carlos, Hervías-Caimapo, C., Hills, M., Hivon, E., Kiiveri, K., Kisner, T., Kunz, M., Kurki-Suonio, H., Lamagna, L., Lasenby, A., Lattanzi, M., Liguori, M., Lindholm, V., López-Caniego, Marcos, Luzzi, G., Maffei, B., Martínez-González, E., Martins, C. J. A. P., Masi, S., Matarrese, S., McCarthy, D., Melchiorri, A., Melin, J.-B., Molinari, D., Monfardini, A., Natoli, P., Negrello, M., Notari, A., Paiella, A., Paoletti, D., Patanchon, G., Piat, M., Pisano, G., Polastri, L., Polenta, G., Pollo, A., Poulin, Vivian, Quartin, M., Remazeilles, M., Roman, M., Rubiño-Martín, Jose Alberto, Salvati, L., Tartari, A., Tomasi, M., Tramonte, D., Trappe, N., Trombetti, T., Tucker, C., Valiviita, J., Van De Weijgaert, R., Van Tent, Bartjan, Vennin, V., Vielva, P., Vittorio, N., Young, K., and Zannoni, M.
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7. Clean energy - Abstract
Journal of cosmology and astroparticle physics 2018(April 2018), 018 (2018). doi:10.1088/1475-7516/2018/04/018, Published by IOP, London
176. Design of the detectors for EBEX, a balloon-borne cosmic microwave background polarimeter
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Westbrook, Benjamin, Aboobaker, A. M., Peter Ade, Aubin, F., Baccigalupi, C., Bandura, K., Bao, C., Borrill, J., Chapman, D., Didier, J., Dobbs, M., Gold, B., Grain, J., Grainger, W., Hanany, S., Helson, K., Hillbrand, S. N., Hilton, G., Hubmayr, H., Irwin, K., Johnson, B., Jaffe, A., Jones, T. J., Kisner, T., Klein, J., Korotkov, A., Leach, S., Lee, A. T., Levinson, L., Limon, M., Macdermid, K., Miller, A. D., Milligan, M., Pascale, E., Raach, K., Reichborn-Kjennerud, B., Sagiv, I., Smecher, G., Stompor, R., Tristram, M., Tucker, G. S., and Zilic, K.
177. The E and B EXperiment EBEX
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Helson, Kyle, Aboobaker, A. M., Peter Ade, Aubin, F., Baccigalupi, C., Bandura, K., Bao, C., Borrill, J., Chandra, B., Chapman, D., Didier, J., Dobbs, M., Gold, B., Grain, J., Grainger, W., Hanany, S., Hillbrand, S. N., Hilton, G., Hubmayr, H., Irwin, K., Johnson, B., Jaffe, A., Jones, T. J., Kisner, T., Klein, J., Korotkov, A., Leach, S., Lee, A. T., Levinson, L., Limon, M., Macdermid, K., Miller, A. D., Milligan, M., Pascale, E., Qiu, C., Raach, K., Reichborn-Kjennerud, B., Reintsema, C., Sagiv, I., Smecher, G., Stompor, R., Tristram, M., Tucker, G. S., Westbrook, B., Yadav, A. P., Zaldarriaga, M., and Zilic, K.
178. Prototype demonstration of the broadband anti-reflection coating on sapphire using a sub-wavelength structure
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Matsumura, T., Takaku, R., Hanany, S., Imada, H., Ishino, H., Katayama, N., Kobayashi, Y., Komatsu, K., Kuniaki Konishi, Kuwata-Gonokami, M., Nakamura, S., Sakurai, H., Sakurai, Y., Wen, Q., Young, K., and Yumoto, J.
179. The E and B EXperiment (EBEX); Progress and Status
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Sagiv, Ilan, Aboobaker, A. M., Ade, P., Aubin, F., Baccigalupi, C., Borrill, J., Chapman, D., Didier, J., Dobbs, M., Grainger, W., Hanany, S., Hilbrand, S., Hogen-Chin, C., Hubmayr, H., Johnson, B., Jaffe, A., Jones, T., Klein, J., Korotkov, A., Leach, S., Lee, A., Levinson, L., Michele Limon, Macaluso, J., Macdermid, K., Matsumura, T., Meng, X., Miller, A., Milligan, M., Pascale, E., Polsgrove, D., Ponthieu, N., Reichborn-Kjennerud, B., Renbarger, T., Stivoli, F., Stompor, R., Tran, H., Tucker, G., Vinokurov, J., Zaldarriaga, M., Zilic, K., Scuola Internazionale Superiore di Studi Avanzati / International School for Advanced Studies (SISSA / ISAS), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), APC - Gravitation (APC-Gravitation), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft-Max-Planck-Gesellschaft, Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Stompor, Radoslaw, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI)
- Subjects
[SDU.ASTR.CO] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,[PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,Astrophysics::Instrumentation and Methods for Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics - Abstract
We report on the status of EBEX, a NASA-funded balloon-borne polarimeter designed to measure the B-mode polarization of the cosmic microwave background radiation. The EBEX receiver is designed to set a 2σ upper limit on an inflationary tensor-to-scalar ratio of 0.02. This limit assumes a 14-day flight, a scan pattern covering 420 square degrees of the sky, and foreground subtraction to levels below detector noise. The instrument employs a 1.5 meter Gregorian-type telescope and 1440 bolometric transition edge sensor detectors distributed over two focal planes. Polarization is measured using a rotating achromatic half wave plate (AHWP) and a fixed polarizing grid. The AHWP is continuously rotated using a superconducting magnetic bearing. Sky signals will be observed in three bands centered at 150, 250 and 410 GHz, providing strong leverage against the polarized dust foreground. Integration of the gondola and the receiver will occur in fall 2008. A short-duration test flight employing 384 detectors in one focal plane is planned for 2009.
180. EBEX: A Balloon-Borne CMB Polarization Experiment
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Chapman, Daniel, Aboobaker, A. M., Peter Ade, Aubin, F., Baccigalupi, C., Bandura, K., Bao, C., Borrill, J., Didier, J., Dobbs, M., Gold, B., Grain, J., Grainger, W., Hanany, S., Helson, K., Hillbrand, S. N., Hilton, G., Hubmayr, H., Irwin, K., Johnson, B., Jaffe, A., Jones, T. J., Kisner, T., Klein, J., Korotkov, A., Leach, S., Lee, A. T., Levinson, L., Limon, M., Macdermid, K., Miller, A. D., Milligan, M., Pascale, E., Raach, K., Reichborn-Kjennerud, B., Sagiv, I., Smecher, G., Stompor, R., Tristram, M., Tucker, G. S., Westbrook, B., and Zilic, K.
181. MAXIMA-1: A measurement of the cosmic microwave background anisotropy on angular scales of 10′-5°
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Hanany, S., Ade, P., Balbi, A., Bock, J., Borrill, J., Boscaleri, A., Paolo de Bernardis, Ferreira, P. G., Hristov, V. V., Jaffe, A. H., Lange, A. E., Lee, A. T., Mauskopf, P. D., Netterfield, C. B., Oh, S., Pascale, E., Rabii, B., Richards, P. L., Smoot, G. F., Stompor, R., Winant, C. D., and Wu, J. H. P.
182. Exploring Cosmic Origins with CORE: Cluster Science
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Melin, J. -B, Bonaldi, A., Remazeilles, M., Hagstotz, S., Diego, J. M., Hernández-Monteagudo, C., Génova-Santos, R. T., Luzzi, G., Martins, C. J. A. P., Grandis, S., Mohr, J. J., Bartlett, J. G., Delabrouille, J., Ferraro, S., Tramonte, D., Rubiño-Martín, J. A., Macìas-Pérez, J. F., Achúcarro, A., Ade, P., Allison, R., Ashdown, M., Ballardini, M., Banday, A. J., Banerji, R., Bartolo, N., Basak, S., Baselmans, J., Basu, K., Battye, R. A., Baumann, D., Bersanelli, M., Bonato, M., Borrill, J., Bouchet, F., Boulanger, F., Brinckmann, T., Bucher, M., Burigana, C., Buzzelli, A., Cai, Z. -Y, Calvo, M., Carvalho, C. S., Castellano, M. G., Challinor, A., Chluba, J., Clesse, S., Colafrancesco, S., Colantoni, I., Coppolecchia, A., Crook, M., D Alessandro, G., Bernardis, P., Gasperis, G., Petris, M., Zotti, G., Di Valentino, E., Errard, J., Feeney, S. M., Fernández-Cobos, R., Finelli, F., Forastieri, F., Galli, S., Gerbino, M., González-Nuevo, J., Greenslade, J., Hanany, S., Handley, W., Hervias-Caimapo, C., Hills, M., Hivon, E., Kiiveri, K., Kisner, T., Kitching, T., Kunz, M., Kurki-Suonio, H., Lamagna, L., Lasenby, A., Lattanzi, M., Le Brun, A. M. C., Lesgourgues, J., Lewis, A., Liguori, M., Lindholm, V., Lopez-Caniego, M., Maffei, B., Martinez-Gonzalez, E., Masi, S., Mccarthy, D., Melchiorri, A., Molinari, D., Monfardini, A., Natoli, P., Negrello, M., Notari, A., Paiella, A., Paoletti, D., Patanchon, G., Piat, M., Pisano, G., Polastri, L., Polenta, G., Pollo, A., Poulin, V., Quartin, M., Roman, M., Salvati, L., Tartari, A., Tomasi, M., Trappe, N., Triqueneaux, S., Trombetti, T., Carole Tucker, Väliviita, J., Weygaert, R., Tent, B., Vennin, V., Vielva, P., Vittorio, N., Weller, J., Young, K., Zannoni, M., and Core, For The Collaboration
183. Exploring cosmic origins with CORE: mitigation of systematic effects
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Natoli, P., Ashdown, M., Banerji, R., Borrill, J., Buzzelli, A., Gasperis, G., Delabrouille, J., Eric Hivon, Molinari, D., Patanchon, G., Polastri, L., Tomasi, M., Bouchet, F. R., Henrot-Versillé, S., Hoang, D. T., Keskitalo, R., Kiiveri, K., Kisner, T., Lindholm, V., Mccarthy, D., Piacentini, F., Perdereau, O., Polenta, G., Tristram, M., Achucarro, A., Ade, P., Allison, R., Baccigalupi, C., Ballardini, M., Banday, A. J., Bartlett, J., Bartolo, N., Basak, S., Baselmans, J., Baumann, D., Bersanelli, M., Bonaldi, A., Bonato, M., Boulanger, F., Brinckmann, T., Bucher, M., Burigana, C., Cai, Z. -Y, Calvo, M., Carvalho, C. -S, Castellano, G., Challinor, A., Chluba, J., Clesse, S., Colantoni, I., Coppolecchia, A., Crook, M., D Alessandro, G., Bernardis, P., Zotti, G., Di Valentino, E., Diego, J. -M, Errard, J., Feeney, S., Fernandez-Cobos, R., Finelli, F., Forastieri, F., Galli, S., Genova-Santos, R., Gerbino, M., Gonzalez-Nuevo, J., Grandis, S., Greenslade, J., Gruppuso, A., Hagstotz, S., Hanany, S., Handley, W., Hernandez-Monteagudo, C., Hervias-Caimapo, C., Hills, M., Keihänen, E., Kitching, T., Kunz, M., Kurki-Suonio, H., Lamagna, L., Lasenby, A., Lattanzi, M., Lesgourgues, J., Lewis, A., Liguori, M., López-Caniego, M., Luzzi, G., Maffei, B., Mandolesi, N., Martinez-Gonzalez, E., Martins, C. J. A. P., Masi, S., Melchiorri, A., Melin, J. -B, Migliaccio, M., Monfardini, A., Negrello, M., Notari, A., Pagano, L., Paiella, A., Paoletti, D., Piat, M., Pisano, G., Pollo, A., Poulin, V., Quartin, M., Remazeilles, M., Roman, M., Rossi, G., Rubino-Martin, J. -A, Salvati, L., Signorelli, G., Tartari, A., Tramonte, D., Trappe, N., Trombetti, T., Tucker, C., Valiviita, J., Weijgaert, R., Tent, B., Vennin, V., Vielva, P., Vittorio, N., Wallis, C., Young, K., Zannoni, M., and Core, For The Collaboration
184. Measurements of CMB Polarization with MAXIPOL
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Proty Wu, Jiun-Huei, Abroe, M. E., Ade, Peter A. R., Bock, J., Borrill, J., Collins, J., Hanany, S., Jaffe, A. H., Johnson, B. R., Jones, T., Lee, A. T., Matsumura, T., Rabii, B., Renbarger, T., Richards, P. L., Smoot, G. F., Stompor, R., Tran, H. T., Winant, C. D., Zuntz, J., Proty Wu, Jiun-Huei, Abroe, M. E., Ade, Peter A. R., Bock, J., Borrill, J., Collins, J., Hanany, S., Jaffe, A. H., Johnson, B. R., Jones, T., Lee, A. T., Matsumura, T., Rabii, B., Renbarger, T., Richards, P. L., Smoot, G. F., Stompor, R., Tran, H. T., Winant, C. D., and Zuntz, J.
- Abstract
We discuss MAXIPOL, a bolometric balloon-borne experiment designed to measure the E-mode polarization of the cosmic microwave background (CMB). MAXIPOL is the first bolometric CMB experiment to observe the sky using rapid polarization modulation. To build MAXIPOL, the CMB temperature anisotropy experiment MAXIMA was retrofitted with a rotating half-wave plate and a stationary analyzer. We describe the instrument, the observations, the calibration and the reduction of data collected with twelve polarimeters operating at 140 GHz and with a FWHM beam size of 10 arcmin. We present maps of the Q and U Stokes parameters of an 8 deg2 region of the sky near the star Beta Ursae Minoris. The power spectra computed from these maps give weak evidence for an EE signal. The maximum-likelihood amplitude of l(l+1)ClEE/2π is 55+51-45 μK2 (68%), and the likelihood function is asymmetric and skewed positive such that with a uniform prior the probability that the amplitude is positive is 96%. This result is consistent with the expected concordance ΛCDM amplitude of 14 μK2. The maximum likelihood amplitudes for l(l+1)ClBB/2π and l(l+1)ClEB/2π are -31+31-19 and 18+27-34 μK2 (68%), respectively, which are consistent with zero. All of the results are for one bin in the range 151 ≤ l ≤ 693. Tests revealed no residual systematic errors in the time or map domain.
185. The E and B EXperiment (EBEX): progress and status
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Sagiv, Ilan, Aboobaker, A. M., Ade, Peter A. R., Aubin, F., Baccigalupi, C., Borrill, D., Chapman, D., Didier, J., Dobbs, M., Grainger, William F., Hanany, S., Hilbrand, S., Hogen-Chin, C., Hubmayr, H., Johnson, B., Jaffe, A., Jones, T., Klein, J., Korotkov, A., Leach, S., Lee, A., Levinson, L., Limon, M., Macaluso, J., MacDermid, K., Matsumura, T., Meng, X., Miller, A., Milligan, M., Pascale, Enzo, Polsgrove, D., Ponthieu, N., Reichborn-Kjennerud, B., Renbarger, T., Stivoli, F., Stompor, R., Tran, H., Tucker, G., Vinokurov, J., Zaldarriaga, M., Zilic, K., Sagiv, Ilan, Aboobaker, A. M., Ade, Peter A. R., Aubin, F., Baccigalupi, C., Borrill, D., Chapman, D., Didier, J., Dobbs, M., Grainger, William F., Hanany, S., Hilbrand, S., Hogen-Chin, C., Hubmayr, H., Johnson, B., Jaffe, A., Jones, T., Klein, J., Korotkov, A., Leach, S., Lee, A., Levinson, L., Limon, M., Macaluso, J., MacDermid, K., Matsumura, T., Meng, X., Miller, A., Milligan, M., Pascale, Enzo, Polsgrove, D., Ponthieu, N., Reichborn-Kjennerud, B., Renbarger, T., Stivoli, F., Stompor, R., Tran, H., Tucker, G., Vinokurov, J., Zaldarriaga, M., and Zilic, K.
- Abstract
We report on the status of EBEX, a NASA-funded balloon-borne polarimeter designed to measure the B-mode polarization of the cosmic microwave background radiation. The EBEX receiver is designed to set a 2σ upper limit on an inflationary tensor-to-scalar ratio of 0.02. This limit assumes a 14-day flight, a scan pattern covering 420 square degrees of the sky, and foreground subtraction to levels below detector noise. The instrument employs a 1.5 meter Gregorian-type telescope and 1440 bolometric transition edge sensor detectors distributed over two focal planes. Polarization is measured using a rotating achromatic half wave plate (AHWP) and a fixed polarizing grid. The AHWP is continuously rotated using a superconducting magnetic bearing. Sky signals will be observed in three bands centered at 150, 250 and 410 GHz, providing strong leverage against the polarized dust foreground. Integration of the gondola and the receiver will occur in fall 2008. A short-duration test flight employing 384 detectors in one focal plane is planned for 2009.
186. BOOMERanG: balloon observations of millimetric extragalactic radiation and geophysics
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Bouchet, François R., de Bernardis, P., Ade, Peter A. R., Aquilini, E., Bock, J., Boscaleri, A., Cardoni, P., Ganga, K., Giacometti, M., Griffin, Matthew, Hanany, S., Hristov, V., Lange, A., Lee, A., Martinis, L., Masi, S., Mauskopf, Philip Daniel, Melchiorri, F., Palangio, P., Pascale, Enzo, Raccanelli, A., Richards, P., Romeo, G., Scaramuzzi, F., Sforna, D., Bouchet, François R., de Bernardis, P., Ade, Peter A. R., Aquilini, E., Bock, J., Boscaleri, A., Cardoni, P., Ganga, K., Giacometti, M., Griffin, Matthew, Hanany, S., Hristov, V., Lange, A., Lee, A., Martinis, L., Masi, S., Mauskopf, Philip Daniel, Melchiorri, F., Palangio, P., Pascale, Enzo, Raccanelli, A., Richards, P., Romeo, G., Scaramuzzi, F., and Sforna, D.
- Abstract
The BOOMERanG experiment is an international effort to measure the Cosmic Microwave Background(CMB) anisotropy at an angular resolution of 12÷20 arcmin, with unprecedented sensitivity, sky and spectral coverage. The telescope will be flown from Antarctica by NASA-NSBF with a long duration stratospheric balloon (7 - 14 days), and is presently scheduled for a test flight in 1996 and an Antarctic flight in 1997. The experiment is designed to measure the power spectrum of the CMB anisotropies up to l ≡ 700 and to produce an image of the CMB sky with high sensitivity and angular resolution. It will be an important precursor of future space-borne missions, producing crucial cosmological data and testing new technologies which are essential to the design of a CMB mapping satellite experiment.
187. Preliminary cosmic microwave background anisotropy results from the MAXIMA balloon borne experiment
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Johnson, B. R., Hanany, S., Ade, Peter A. R., Balbi, A., Bock, J., Borrill, J., Boscaleri, A., DeBernardis, P., Ferreira, P., Hristov, V., Lange, A. E., Pascale, Enzo, Jaffe, A. H., Lee, A. T., Oh, S., Rabii, B., Richards, P. L., Winant, C. D., Mauskopf, Philip Daniel, Netterfield, C. B., Johnson, B. R., Hanany, S., Ade, Peter A. R., Balbi, A., Bock, J., Borrill, J., Boscaleri, A., DeBernardis, P., Ferreira, P., Hristov, V., Lange, A. E., Pascale, Enzo, Jaffe, A. H., Lee, A. T., Oh, S., Rabii, B., Richards, P. L., Winant, C. D., Mauskopf, Philip Daniel, and Netterfield, C. B.
- Abstract
We present preliminary cosmic microwave background anisotropy results from the first flight of the MAXIMA balloon borne experiment. The flight (MAXIMA-1) took place in August of 1998 from the National Scientific Ballooning Facility in Palestine, Texas. During the four hour flight we mapped a 124 deg2 section of the sky which has extremely low galactic dust contamination. The combination of the beam size and scan strategy make MAXIMA sensitive to CMB fluctuations on a range of angular scales from 10 arcmin to 5 degrees. The instrument consists of a Gregorian telescope with a 1.3m primary mirror and a receiver housing a 16 element bolometer array cooled to 100mK. Observations were made at 3 frequency bands centered on 150, 240, and 410 GHz. The results presented will include a map of the CMB anisotropy at 150 GHz. We will also briefly describe the second MAXIMA flight that took place in June of 1999. During this flight we observed 230 deg2 of sky with very low galactic dust contamination. About 20% of this region overlaps the MAXIMA-1 map. The MAXIMA experiment is supported by NASA through grant Nos. NAG5-4454, and NAG5-3941, and by the Center for Particle Astrophysics, a National Science Foundation Science and Technology Center operated by the University of California, Berkeley, under Cooperative Agreement No. AST-9120005.
188. Future plans for CMB anisotropy measurements with the MAXIMA array
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Bouchet, François R., Lee, A., Ade, Peter A. R., Bock, J., Boscaleri, A., Church, S., de Bernardis, P., Feldman, J., Ganga, K., Hanany, S., Hristov, V., Lange, A., Pascale, Enzo, Mauskopf, Philip Daniel, Richards, P., Smoot, G., Tanaka, S., Winant, C., Wu, J., Bouchet, François R., Lee, A., Ade, Peter A. R., Bock, J., Boscaleri, A., Church, S., de Bernardis, P., Feldman, J., Ganga, K., Hanany, S., Hristov, V., Lange, A., Pascale, Enzo, Mauskopf, Philip Daniel, Richards, P., Smoot, G., Tanaka, S., Winant, C., and Wu, J.
- Abstract
The Millimeter-Wave Anisotropy eXperiment Array (MAXIMA) experiment is an evolution of the degree-scale CMB anisotropy experiment MAX. MAXIMA is also based on a balloon-borne telescope and Adiabatic Demagnetization Refrigerator (ADR) cooled bolometers operated at 100 mK. The new experiment is designed to dramatically increase the amount of CMB anisotropy power spectrum information gathered compared to MAX. There are three main components to this improvement: (1) A large increase in sky coverage per flight is made possible by a large increase in the instrument sensitivity and an efficient observation strategy. (2) High resolution in l-space and sensitivity to high values of l is achieved by the total power mode observation strategy and small (11' FWHM) beams. (3) Robust checks for instrumental systematics and foregrounds are made by repeated measurements of the same area of sky on several time scales and wide frequency coverage.
189. MAXIMA: Observations of the Cosmic Microwave Background Anisotropy on Angular Scales of 10' to 5 Degrees
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Winant, C. D., Ade, Peter A. R., Balbi, A., Bock, J., Borrill, J., Boscaleri, A., De Bernardis, P., Ferreira, P., Hanany, S., Hristov, V., Jaffe, A. H., Johnson, B., Lange, A. E., Lee, A. T., Mauskopf, Philip Daniel, Netterfield, C. B., Oh, S., Pascale, Enzo, Rabii, B., Richards, P. L., Smoot, G. F., Stompor, R., Wu, J. H. P., Winant, C. D., Ade, Peter A. R., Balbi, A., Bock, J., Borrill, J., Boscaleri, A., De Bernardis, P., Ferreira, P., Hanany, S., Hristov, V., Jaffe, A. H., Johnson, B., Lange, A. E., Lee, A. T., Mauskopf, Philip Daniel, Netterfield, C. B., Oh, S., Pascale, Enzo, Rabii, B., Richards, P. L., Smoot, G. F., Stompor, R., and Wu, J. H. P.
- Abstract
We discuss the status of our analysis of the data obtained from the first flight of the MAXIMA balloon borne experiment. The flight (MAXIMA-1) took place in August of 1998 from the National Scientific Ballooning Facility in Palestine, Texas. During the four hour flight we mapped a 124 deg2 section of the sky which has extremely low galactic dust contamination. The combination of the beam size and scan strategy make MAXIMA sensitive to CMB fluctuations on a range of angular scales from 10 arcmin to 5 degrees. The instrument consists of a Gregorian telescope with a 1.3 m primary mirror and a receiver housing a 16 element bolometer array cooled to 100 mK. Observations were made at 3 frequency bands centered on 150, 240, and 410 GHz. The results presented will include maps of the CMB anisotropy at 150 GHz. We will also briefly describe the second MAXIMA flight that took place in June of 1999 and our plans for the future. During the second flight we observed 230 deg2 of sky with very low galactic dust contamination. About 20% of this region overlaps the MAXIMA-1 map. The MAXIMA experiment is supported by NASA through grants NAG5-4454, and NAG5-3941, and by the Center for Particle Astrophysics, a National Science Foundation Science and Technology Center operated by the University of California, Berkeley, under Cooperative Agreement No. AST-9120005.
190. Measuring the cosmic microwave background anisotropy power spectrum using boomerang
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Signore, M., Melchiorri, F., Masi, S., de Bernardis, P., Giacometti, M., Raccanelli, A., Sforna, D., Ade, Peter A. R., Griffin, Matthew Joseph, Aquilini, E., Cardoni, P., Martinis, L., Scaramuzzi, F., Bock, J. J., Church, S. E., Contensou, M., Crill, B. P., Hristov, V., Lange, A. E., Pascale, C. B., Netterfield, E., Boscaleri, A., Ganga, K. M., Hanany, S., Lee, A., Richards, P. L., Mauskopf, Philip Daniel, Palangio, P., Romeo, G., Ruhl, J., Signore, M., Melchiorri, F., Masi, S., de Bernardis, P., Giacometti, M., Raccanelli, A., Sforna, D., Ade, Peter A. R., Griffin, Matthew Joseph, Aquilini, E., Cardoni, P., Martinis, L., Scaramuzzi, F., Bock, J. J., Church, S. E., Contensou, M., Crill, B. P., Hristov, V., Lange, A. E., Pascale, C. B., Netterfield, E., Boscaleri, A., Ganga, K. M., Hanany, S., Lee, A., Richards, P. L., Mauskopf, Philip Daniel, Palangio, P., Romeo, G., and Ruhl, J.
191. MAXIMA: an experiment to measure temperature anisotropy in the cosmic microwave background
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Maiani, Luciano, Melchiorri, Francesco, Vittorio, Nicola, Lee, A. T., Ade, Peter A. R., Balbi, A., Bock, J., Borrill, J., Boscaleri, A., Crill, B. P., De Bernardis, P., Del Castillo, H., Ferreira, P., Ganga, K., Hanany, S., Hristov, V., Jaffe, A. H., Lange, A. E., Mauskopf, Philip Daniel, Netterfield, C. B., Oh, S., Pascale, Enzo, Rabii, B., Richards, P. L., Ruhl, J., Smoot, G. F., Winant, C. D., Maiani, Luciano, Melchiorri, Francesco, Vittorio, Nicola, Lee, A. T., Ade, Peter A. R., Balbi, A., Bock, J., Borrill, J., Boscaleri, A., Crill, B. P., De Bernardis, P., Del Castillo, H., Ferreira, P., Ganga, K., Hanany, S., Hristov, V., Jaffe, A. H., Lange, A. E., Mauskopf, Philip Daniel, Netterfield, C. B., Oh, S., Pascale, Enzo, Rabii, B., Richards, P. L., Ruhl, J., Smoot, G. F., and Winant, C. D.
- Abstract
We describe the MAXIMA experiment, a balloon-borne measurement designed to map temperature anisotropy in the Cosmic Microwave Background (CMB) from l=80 to l=800. The experiment consists of a 1.3 m diameter off-axis Gregorian telescope and a receiver with a 16 element array of bolometers cooled to 100 mK. The frequency bands are centered at 150, 240, and 410 GHz. The 10′ FWHM beam sizes are well matched to the scale of acoustic peaks expected in the angular power spectrum of the CMB. The first flight of the experiment in its full configuration was launched in August 1998. A 122 deg2 map of the sky was made near the Draco constellation during the 7 hour flight in a region of extremely low galactic dust contamination. This map covers 0.3% of the sky and has 3200 independent beamsize pixels. We describe the MAXIMA instrument and its performance during the recent flight.
192. MAXIMA: Millimeter-wave anisotropy experiment imaging array
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Wheeler, J. Craig, Martel, Hugo, Winant, C., Abroe, M., Ade, Peter A. R., Balbi, D., Bock, J., Borrill, J., Boscaleri, A., Collins, J., de Bernardis, P., Ferreira, P., Hanany, S., Hristov, V., Jaffe, A. H., Johnson, B., Lange, A. E., Lee, A. T., Mauskopf, Philip Daniel, Netterfield, C. B., Oh, S., Pascale, E., Rabii, B., Richards, P. L., Stompor, R., Smoot, G. F., Wu, H. P., Wheeler, J. Craig, Martel, Hugo, Winant, C., Abroe, M., Ade, Peter A. R., Balbi, D., Bock, J., Borrill, J., Boscaleri, A., Collins, J., de Bernardis, P., Ferreira, P., Hanany, S., Hristov, V., Jaffe, A. H., Johnson, B., Lange, A. E., Lee, A. T., Mauskopf, Philip Daniel, Netterfield, C. B., Oh, S., Pascale, E., Rabii, B., Richards, P. L., Stompor, R., Smoot, G. F., and Wu, H. P.
193. Constraints on cosmological parameters from MAXMIA-1
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Gurzadyan, Vahe G., Jantzen, Robert T., Ruffini, Remo, Balbi, A., Ade, Peter A. R., Bock, J., Borrill, J., Boscaleri, A., de Bernardis, P., Ferreira, P. G., Hanany, S., Hristov, V., Jaffe, A .H., Lee, A. T., Oh, S., Pascale, E., Rabii, B., Richards, P. L., Smoot, G. F., Stompor, R., Winant, C. D., Wu, J. H. P., Gurzadyan, Vahe G., Jantzen, Robert T., Ruffini, Remo, Balbi, A., Ade, Peter A. R., Bock, J., Borrill, J., Boscaleri, A., de Bernardis, P., Ferreira, P. G., Hanany, S., Hristov, V., Jaffe, A .H., Lee, A. T., Oh, S., Pascale, E., Rabii, B., Richards, P. L., Smoot, G. F., Stompor, R., Winant, C. D., and Wu, J. H. P.
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Using the angular power spectrum of the cosmic microwave background measured over a wide range of ℓ in the first flight of the MAXIMA balloon-borne experiment (MAXIMA-1) and the low ℓ results from COBE/DMR, we set constraints on a suite of cosmological parameters within the framework of inflationary adiabatic models. Our results are consistent with the basic predictions of inflation: a flat universe with nearly scale-invariant primordial fluctuations. They are also consistent with large scale structure observations, and in marginal agreement with the baryon density from big bang nucleosynthesis.
194. Mapping the CMB with the MAXIMA experiment
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Kawasaki, Masahiro, Sato, Katsuhiko, Rabbi, B., Ade, Peter A. R., Balbi, A., Bock, J., Borrill, J., Boscaleri, A., de Bernardis, P., Ferreira, P., Hanany, S., Hristov, V., Jaffe, A. H., Lange, A. E., Lee, A. T., Mauskopf, Philip Daniel, Netterfield, C. B., Oh, S., Pascale, E., Richards, P. L., Stompor, R., Smoot, G. F., Winant, C. D., Kawasaki, Masahiro, Sato, Katsuhiko, Rabbi, B., Ade, Peter A. R., Balbi, A., Bock, J., Borrill, J., Boscaleri, A., de Bernardis, P., Ferreira, P., Hanany, S., Hristov, V., Jaffe, A. H., Lange, A. E., Lee, A. T., Mauskopf, Philip Daniel, Netterfield, C. B., Oh, S., Pascale, E., Richards, P. L., Stompor, R., Smoot, G. F., and Winant, C. D.
195. OLIMPO: A balloon-borne SZE imager to probe ICM dynamics and the WHIM.
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Sayers, J., Avestruz, C., Thakur, R. Basu, Battistelli, E., Bulbul, E., Cacciotti, F., Columbro, F., Coppolecchia, A., Cray, S., D'Alessandro, G., de Bernardis, P., De Petris, M., Hanany, S., Lamagna, L., Lau, E., Masi, S., Paiella, A., Pettinari, G., Piacentini, F., and Rapaport, E.
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SUNYAEV-Zel'dovich effect , *INTERSTELLAR medium , *COSMIC background radiation , *KINEMATICS , *POWER spectra - Abstract
OLIMPO is a proposed Antarctic balloon-borne Sunyaev-Zel'dovich effect (SZE) imager to study gas dynamics associated with structure formation along with the properties of the warm-hot intergalactic medium (WHIM) residing in the connective filaments. During a 25 day flight OLIMPO will image a total of 10 z∼0.05 galaxy clusters and 8 bridges at 145, 250, 365, and 460 GHz at an angular resolution of 1.0′–3.3′. The maps will be significantly deeper than those planned from CMB-S4 and CCAT-P, and will have excellent fidelity to the large angular scales of our low-z targets, which are difficult to probe from the ground. In combination with X-ray data from eROSITA and XRISM we will transform our current static view of galaxy clusters into a full dynamic picture by measuring the internal intra-cluster medium (ICM) velocity structure with the kinematic SZE, X-ray spectroscopy, and the power spectrum of ICM fluctuations. Radio observations from ASKAP and MeerKAT will be used to better understand the connection between ICM turbulence and shocks with the relativistic plasma. Beyond the cluster boundary, we will combine thermal SZE maps from OLIMPO with X-ray imaging from eROSITA to measure the thermodynamics of the WHIM residing in filaments, providing a better understanding of its properties and its contribution to the total baryon budget. [ABSTRACT FROM AUTHOR]
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- 2024
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196. Erratum: "Constraints on Cosmological Parameters from MAXIMA-1" (ApJ 545, L1 [2000]).
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Balbi, A., Ade, P., Bock, J., Borrill, J., Boscaleri, A., De Bernardis, P., Ferreira, P. G., Hanany, S., Hristov, V., Jaffe, A. H., Lee, A. T., Oh, S., Pascale, E., Rabii, B., Richards, P. L., Smoot, G. F., Stompor, R., Winant, C. D., and Wu, J. H. P.
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- 2001
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197. A 350 GHz array of LEKIDs for balloon-borne CMB observations.
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Cacciotti, F., Paiella, A., Avestruz, C., Tackur, R. Basu, Battistelli, E.S., de Bernardis, P., Bulbul, E., Columbro, F., Coppolecchia, A., Cray, S., D'Alessandro, G., De Petris, M., Hanany, S., Lamagna, L., Lau, E., Masi, S., Pettinari, G., Piacentini, F., Sayers, J., and Zhuravleva, I.
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LUMPED elements , *GALAXY clusters , *QUALITY factor , *ELECTRIC inductance , *FREQUENCY discriminators , *COSMIC background radiation - Abstract
We present the design, optimization and laboratory characterization of an array of Lumped Element Kinetic Inductance Detectors sensitive in a frequency band centered at 350 GHz. The array consists of 313 feed-horn coupled pixels with resonant frequencies spread over 250 MHz. We present measured yield, quality factor, responsivity, quasiparticle lifetime, noise equivalent power and optical efficiency. The array is a prototype for one of the four frequency bands of OLIMPO, a balloon-borne instrument with a 2.6 m primary mirror proposed for an Antarctic flight to measure the Sunyaev–Zel'dovich effect in clusters of galaxies and their connecting filaments. Similar arrays could also be used with instruments studying the polarization of the cosmic microwave background radiation. [ABSTRACT FROM AUTHOR]
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- 2024
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- View/download PDF
198. Exploring cosmic origins with CORE: Inflation
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F. Finelli, M. Bucher, A. Achúcarro, M. Ballardini, N. Bartolo, D. Baumann, S. Clesse, J. Errard, W. Handley, M. Hindmarsh, K. Kiiveri, M. Kunz, A. Lasenby, M. Liguori, D. Paoletti, C. Ringeval, J. Väliviita, B. van Tent, V. Vennin, P. Ade, R. Allison, F. Arroja, M. Ashdown, A.J. Banday, R. Banerji, J.G. Bartlett, S. Basak, P. de Bernardis, M. Bersanelli, A. Bonaldi, J. Borril, F.R. Bouchet, F. Boulanger, T. Brinckmann, C. Burigana, A. Buzzelli, Z.-Y. Cai, M. Calvo, C.S. Carvalho, G. Castellano, A. Challinor, J. Chluba, I. Colantoni, A. Coppolecchia, M. Crook, G. D'Alessandro, G. D'Amico, J. Delabrouille, V. Desjacques, G. De Zotti, J.M. Diego, E. Di Valentino, S. Feeney, J.R. Fergusson, R. Fernandez-Cobos, S. Ferraro, F. Forastieri, S. Galli, J. García-Bellido, G. de Gasperis, R.T. Génova-Santos, M. Gerbino, J. González-Nuevo, S. Grandis, J. Greenslade, S. Hagstotz, S. Hanany, D.K. Hazra, C. Hernández-Monteagudo, C. Hervias-Caimapo, M. Hills, E. Hivon, B. Hu, T. Kisner, T. Kitching, E.D. Kovetz, H. Kurki-Suonio, L. Lamagna, M. Lattanzi, J. Lesgourgues, A. Lewis, V. Lindholm, J. Lizarraga, M. López-Caniego, G. Luzzi, B. Maffei, N. Mandolesi, E. Martínez-González, C.J.A.P. Martins, S. Masi, D. McCarthy, S. Matarrese, A. Melchiorri, J.-B. Melin, D. Molinari, A. Monfardini, P. Natoli, M. Negrello, A. Notari, F. Oppizzi, A. Paiella, E. Pajer, G. Patanchon, S.P. Patil, M. Piat, G. Pisano, L. Polastri, G. Polenta, A. Pollo, V. Poulin, M. Quartin, A. Ravenni, M. Remazeilles, A. Renzi, D. Roest, M. Roman, J.A. Rubiño-Martin, L. Salvati, A.A. Starobinsky, A. Tartari, G. Tasinato, M. Tomasi, J. Torrado, N. Trappe, T. Trombetti, M. Tucci, C. Tucker, J. Urrestilla, R. van de Weygaert, P. Vielva, N. Vittorio, K. Young, M. Zannoni, ITA, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut Lagrange de Paris, Sorbonne Université (SU), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Théorique d'Orsay [Orsay] (LPT), Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11), Institut de recherche en astrophysique et planétologie (IRAP), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Institut Nanosciences et Cryogénie (INAC), Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Département de Physique des Particules (ex SPP) (DPP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut Néel (NEEL), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Université Pierre et Marie Curie - Paris 6 (UPMC), Laboratoire d'Annecy-le-Vieux de Physique Théorique (LAPTH), Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), CORE, Department of Physics, Helsinki Institute of Physics, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Sorbonne Universités, Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS), Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Université Grenoble Alpes (UGA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Grenoble Alpes (UGA), Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF), Finelli, F, Bucher, M, Achúcarro, A, Ballardini, M, Bartolo, N, Baumann, D, Clesse, S, Errard, J, Handley, W, Hindmarsh, M, Kiiveri, K, Kunz, M, Lasenby, A, Liguori, M, Paoletti, D, Ringeval, C, Väliviita, J, Tent, B, Vennin, V, Ade, P, Allison, R, Arroja, F, Ashdown, M, Banday, A, Banerji, R, Bartlett, J, Basak, S, de Bernardis, P, Bersanelli, M, Bonaldi, A, Borril, J, Bouchet, F, Boulanger, F, Brinckmann, T, Burigana, C, Buzzelli, A, Cai, Z, Calvo, M, Carvalho, C, Castellano, G, Challinor, A, Chluba, J, Colantoni, I, Coppolecchia, A, Crook, M, D'Alessandro, G, D'Amico, G, Delabrouille, J, Desjacques, V, Zotti, G, Diego, J, Valentino, E, Feeney, S, Fergusson, J, Fernandez-Cobos, R, Ferraro, S, Forastieri, F, Galli, S, García-Bellido, J, de Gasperis, G, Génova-Santos, R, Gerbino, M, González-Nuevo, J, Grandis, S, Greenslade, J, Hagstotz, S, Hanany, S, Hazra, D, Hernández-Monteagudo, C, Hervias-Caimapo, C, Hills, M, Hivon, E, Hu, B, Kisner, T, Kitching, T, Kovetz, E, Kurki-Suonio, H, Lamagna, L, Lattanzi, M, Lesgourgues, J, Lewis, A, Lindholm, V, Lizarraga, J, López-Caniego, M, Luzzi, G, Maffei, B, Mandolesi, N, Martínez-González, E, Martins, C, Masi, S, Mccarthy, D, Matarrese, S, Melchiorri, A, Melin, J, Molinari, D, Monfardini, A, Natoli, P, Negrello, M, Notari, A, Oppizzi, F, Paiella, A, Pajer, E, Patanchon, G, Patil, S, Piat, M, Pisano, G, Polastri, L, Polenta, G, Pollo, A, Poulin, V, Quartin, M, Ravenni, A, Remazeilles, M, Renzi, A, Roest, D, Roman, M, Rubiño-Martin, J, Salvati, L, Starobinsky, A, Tartari, A, Tasinato, G, Tomasi, M, Torrado, J, Trappe, N, Trombetti, T, Tucci, M, Tucker, C, Urrestilla, J, de Weygaert, R, Vielva, P, Vittorio, N, Young, K, Zannoni, M, Finelli F., Bucher M., Achucarro A., Ballardini M., Bartolo N., Baumann D., Clesse S., Errard J., Handley W., Hindmarsh M., Kiiveri K., Kunz M., Lasenby A., Liguori M., Paoletti D., Ringeval C., Valiviita J., Tent B.V., Vennin V., Ade P., Allison R., Arroja F., Ashdown M., Banday A.J., Banerji R., Bartlett J.G., Basak S., De Bernardis P., Bersanelli M., Bonaldi A., Borril J., Bouchet F.R., Boulanger F., Brinckmann T., Burigana C., Buzzelli A., Cai Z.-Y., Calvo M., Carvalho C.S., Castellano G., Challinor A., Chluba J., Colantoni I., Coppolecchia A., Crook M., D'Alessandro G., D'Amico G., Delabrouille J., Desjacques V., Zotti G.D., Diego J.M., Valentino E.D., Feeney S., Fergusson J.R., Fernandez-Cobos R., Ferraro S., Forastieri F., Galli S., Garcia-Bellido J., De Gasperis G., Genova-Santos R.T., Gerbino M., Gonzalez-Nuevo J., Grandis S., Greenslade J., Hagstotz S., Hanany S., Hazra D.K., Hernandez-Monteagudo C., Hervias-Caimapo C., Hills M., Hivon E., Hu B., Kisner T., Kitching T., Kovetz E.D., Kurki-Suonio H., Lamagna L., Lattanzi M., Lesgourgues J., Lewis A., Lindholm V., Lizarraga J., Lopez-Caniego M., Luzzi G., Maffei B., Mandolesi N., Martinez-Gonzalez E., Martins C.J.A.P., Masi S., McCarthy D., Matarrese S., Melchiorri A., Melin J.-B., Molinari D., Monfardini A., Natoli P., Negrello M., Notari A., Oppizzi F., Paiella A., Pajer E., Patanchon G., Patil S.P., Piat M., Pisano G., Polastri L., Polenta G., Pollo A., Poulin V., Quartin M., Ravenni A., Remazeilles M., Renzi A., Roest D., Roman M., Rubino-Martin J.A., Salvati L., Starobinsky A.A., Tartari A., Tasinato G., Tomasi M., Torrado J., Trappe N., Trombetti T., Tucci M., Tucker C., Urrestilla J., De Weygaert R.V., Vielva P., Vittorio N., Young K., Zannoni M., String Theory (ITFA, IoP, FNWI), High-Energy Frontier, Astronomy, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Cryogénie (NEEL - Cryo), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Département de Physique des Particules (ex SPP) (DPhP), and Hélium : du fondamental aux applications (NEEL - HELFA)
- Subjects
cosmological model ,reheating ,Cosmic microwave background ,cosmic background radiation: polarization ,SPECTRAL DISTORTIONS ,astro-ph.CO ,Astrophysics ,cosmic background radiation ,7. Clean energy ,01 natural sciences ,GRAVITATIONAL-WAVES ,law.invention ,law ,010303 astronomy & astrophysics ,CMBR theory ,ination ,Astronomy and Astrophysics ,CMBR theory, inflation ,QC ,QB ,Physics ,COSMIC cancer database ,ST/J005673/1 ,ST/H008586/1 ,inflation: model ,MICROWAVE BACKGROUND ANISOTROPY ,Core inflation ,Astrophysics - Cosmology and Nongalactic Astrophysics ,Big Bang ,scale: grand unified theory ,Astrophysics and Astronomy ,noise ,Cosmology and Nongalactic Astrophysics (astro-ph.CO) ,STANDARD MODEL ,satellite ,FOS: Physical sciences ,Astrophysics::Cosmology and Extragalactic Astrophysics ,isocurvature: perturbation ,frequency: high ,PRIMORDIAL NON-GAUSSIANITY ,NO ,Telescope ,power spectrum: primordial ,FIS/05 - ASTRONOMIA E ASTROFISICA ,Settore FIS/05 - Astronomia e Astrofisica ,LARGE-SCALE STRUCTURE ,0103 physical sciences ,inflation ,cosmic string ,STFC ,MODEL SELECTION ,Inflation (cosmology) ,non-Gaussianity: primordial ,ST/K00333X/1 ,ISOCURVATURE PERTURBATIONS ,010308 nuclear & particles physics ,string tension ,big bang ,inflation: slow-roll approximation ,RCUK ,Spectral density ,115 Astronomy, Space science ,cosmic background radiation: temperature ,Cosmic string ,detector: sensitivity ,angular resolution ,13. Climate action ,PRE-BIG-BANG ,BAYESIAN-INFERENCE ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,cosmic background radiation: anisotropy - Abstract
We forecast the scientific capabilities to improve our understanding of cosmic inflation of CORE, a proposed CMB space satellite submitted in response to the ESA fifth call for a medium-size mission opportunity. The CORE satellite will map the CMB anisotropies in temperature and polarization in 19 frequency channels spanning the range 60-600 GHz. CORE will have an aggregate noise sensitivity of $1.7 ��$K$\cdot \,$arcmin and an angular resolution of 5' at 200 GHz. We explore the impact of telescope size and noise sensitivity on the inflation science return by making forecasts for several instrumental configurations. This study assumes that the lower and higher frequency channels suffice to remove foreground contaminations and complements other related studies of component separation and systematic effects, which will be reported in other papers of the series "Exploring Cosmic Origins with CORE." We forecast the capability to determine key inflationary parameters, to lower the detection limit for the tensor-to-scalar ratio down to the $10^{-3}$ level, to chart the landscape of single field slow-roll inflationary models, to constrain the epoch of reheating, thus connecting inflation to the standard radiation-matter dominated Big Bang era, to reconstruct the primordial power spectrum, to constrain the contribution from isocurvature perturbations to the $10^{-3}$ level, to improve constraints on the cosmic string tension to a level below the presumptive GUT scale, and to improve the current measurements of primordial non-Gaussianities down to the $f_{NL}^{\rm local} < 1$ level. For all the models explored, CORE alone will improve significantly on the present constraints on the physics of inflation. Its capabilities will be further enhanced by combining with complementary future cosmological observations., Latex 107 pages, revised with updated author list and minor modifications
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- 2018
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199. CMB-S4
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Collaboration, The CMB-S4, Abazajian, Kevork, Addison, Graeme E., Adshead, Peter, Ahmed, Zeeshan, Akerib, Daniel, Ali, Aamir, Allen, Steven W., Alonso, David, Alvarez, Marcelo, Amin, Mustafa A., Anderson, Adam, Arnold, Kam S., Ashton, Peter, Baccigalupi, Carlo, Bard, Debbie, Barkats, Denis, Barron, Darcy, Barry, Peter S., Bartlett, James G., Thakur, Ritoban Basu, Battaglia, Nicholas, Bean, Rachel, Bebek, Chris, Bender, Amy N., Benson, Bradford A., Bianchini, Federico, Bischoff, Colin A., Bleem, Lindsey, Bock, James J., Bocquet, Sebastian, Boddy, Kimberly K., Bond, J. Richard, Borrill, Julian, Bouchet, François R., Brinckmann, Thejs, Brown, Michael L., Bryan, Sean, Buza, Victor, Byrum, Karen, Caimapo, Carlos Hervias, Calabrese, Erminia, Calafut, Victoria, Caldwell, Robert, Carlstrom, John E., Carron, Julien, Cecil, Thomas, Challinor, Anthony, Chang, Clarence L., Chinone, Yuji, Cho, Hsiao-Mei Sherry, Cooray, Asantha, Coulton, Will, Crawford, Thomas M., Crites, Abigail, Cukierman, Ari, Cyr-Racine, Francis-Yan, de Haan, Tijmen, Delabrouille, Jacques, Devlin, Mark, Di Valentino, Eleonora, Dierickx, Marion, Dobbs, Matt, Duff, Shannon, Dunkley, Jo, Dvorkin, Cora, Eimer, Joseph, Elleflot, Tucker, Errard, Josquin, Essinger-Hileman, Thomas, Fabbian, Giulio, Feng, Chang, Ferraro, Simone, Filippini, Jeffrey P., Flauger, Raphael, Flaugher, Brenna, Fraisse, Aurelien A., Frolov, Andrei, Galitzki, Nicholas, Gallardo, Patricio A., Galli, Silvia, Ganga, Ken, Gerbino, Martina, Gluscevic, Vera, Goeckner-Wald, Neil, Green, Daniel, Grin, Daniel, Grohs, Evan, Gualtieri, Riccardo, Gudmundsson, Jon E., Gullett, Ian, Gupta, Nikhel, Habib, Salman, Halpern, Mark, Halverson, Nils W., Hanany, Shaul, Harrington, Kathleen, Hasegawa, Masaya, Hasselfield, Matthew, Hazumi, Masashi, Heitmann, Katrin, Henderson, Shawn, Hensley, Brandon, Hill, Charles, Hill, J. Colin, Hlozek, Renée, Ho, Shuay-Pwu Patty, Hoang, Thuong, Holder, Gil, Holzapfel, William, Hood, John, Hubmayr, Johannes, Huffenberger, Kevin M., Hui, Howard, Irwin, Kent, Jeong, Oliver, Johnson, Bradley R., Jones, William C., Kang, Jae Hwan, Karkare, Kirit S., Katayama, Nobuhiko, Keskitalo, Reijo, Kisner, Theodore, Knox, Lloyd, Koopman, Brian J., Kosowsky, Arthur, Kovac, John, Kovetz, Ely D., Kuhlmann, Steve, Kuo, Chao-lin, Kusaka, Akito, Lähteenmäki, Anne, Lawrence, Charles R., Lee, Adrian T., Lewis, Antony, Li, Dale, Linder, Eric, Loverde, Marilena, Lowitz, Amy, Lubin, Phil, Madhavacheril, Mathew S., Mantz, Adam, Marques, Gabriela, Matsuda, Frederick, Mauskopf, Philip, McCarrick, Heather, McMahon, Jeffrey, Meerburg, P. Daniel, Melin, Jean-Baptiste, Menanteau, Felipe, Meyers, Joel, Millea, Marius, Mohr, Joseph, Moncelsi, Lorenzo, Monzani, Maria, Mroczkowski, Tony, Mukherjee, Suvodip, Nagy, Johanna, Namikawa, Toshiya, Nati, Federico, Natoli, Tyler, Newburgh, Laura, Niemack, Michael D., Nishino, Haruki, Nord, Brian, Novosad, Valentine, O'Brient, Roger, Padin, Stephen, Palladino, Steven, Partridge, Bruce, Petravick, Don, Pierpaoli, Elena, Pogosian, Levon, Prabhu, Karthik, Pryke, Clement, Puglisi, Giuseppe, Racine, Benjamin, Rahlin, Alexandra, Rao, Mayuri Sathyanarayana, Raveri, Marco, Reichardt, Christian L., Remazeilles, Mathieu, Rocha, Graca, Roe, Natalie A., Roy, Anirban, Ruhl, John E., Salatino, Maria, Saliwanchik, Benjamin, Schaan, Emmanuel, Schillaci, Alessandro, Schmitt, Benjamin, Schmittfull, Marcel M., Scott, Douglas, Sehgal, Neelima, Shandera, Sarah, Sherwin, Blake D., Shirokoff, Erik, Simon, Sara M., Slosar, Anze, Spergel, David, Germaine, Tyler St., Staggs, Suzanne T., Stark, Antony, Starkman, Glenn D., Stompor, Radek, Stoughton, Chris, Suzuki, Aritoki, Tajima, Osamu, Teply, Grant P., Thompson, Keith, Thorne, Ben, Timbie, Peter, Tomasi, Maurizio, Tristram, Matthieu, Tucker, Gregory, Umiltà, Caterina, van Engelen, Alexander, Vavagiakis, Eve M., Vieira, Joaquin D., Vieregg, Abigail G., Wagoner, Kasey, Wallisch, Benjamin, Wang, Gensheng, Watson, Scott, Westbrook, Ben, Whitehorn, Nathan, Wollack, Edward J., Wu, W. L. Kimmy, Xu, Zhilei, Yang, H. Y. Eric, Yasini, Siavash, Yefremenko, Volodymyr G., Yoon, Ki Won, Young, Edward, Yu, Cyndia, Zonca, Andrea, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Théorique - UMR CNRS 3681 (IPHT), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), CMB-S4, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Université Paris-Sud - Paris 11 (UP11), Apollo - University of Cambridge Repository, Van Swinderen Institute for Particle Physics and G, Cosmic Frontier, Abazajian, K, Addison, G, Adshead, P, Ahmed, Z, Akerib, D, Ali, A, Allen, S, Alonso, D, Alvarez, M, Amin, M, Anderson, A, Arnold, K, Ashton, P, Baccigalupi, C, Bard, D, Barkats, D, Barron, D, Barry, P, Bartlett, J, Basu Thakur, R, Battaglia, N, Bean, R, Bebek, C, Bender, A, Benson, B, Bianchini, F, Bischoff, C, Bleem, L, Bock, J, Bocquet, S, Boddy, K, Richard Bond, J, Borrill, J, Bouchet, F, Brinckmann, T, Brown, M, Bryan, S, Buza, V, Byrum, K, Hervias Caimapo, C, Calabrese, E, Calafut, V, Caldwell, R, Carlstrom, J, Carron, J, Cecil, T, Challinor, A, Chang, C, Chinone, Y, Sherry Cho, H, Cooray, A, Coulton, W, Crawford, T, Crites, A, Cukierman, A, Cyr-Racine, F, De Haan, T, Delabrouille, J, Devlin, M, Di Valentino, E, Dierickx, M, Dobbs, M, Duff, S, Dvorkin, C, Eimer, J, Elleflot, T, Errard, J, Essinger-Hileman, T, Fabbian, G, Feng, C, Ferraro, S, Filippini, J, Flauger, R, Flaugher, B, Fraisse, A, Frolov, A, Galitzki, N, Gallardo, P, Galli, S, Ganga, K, Gerbino, M, Gluscevic, V, Goeckner-Wald, N, Green, D, Grin, D, Grohs, E, Gualtieri, R, Gudmundsson, J, Gullett, I, Gupta, N, Habib, S, Halpern, M, Halverson, N, Hanany, S, Harrington, K, Hasegawa, M, Hasselfield, M, Hazumi, M, Heitmann, K, Henderson, S, Hensley, B, Hill, C, Colin Hill, J, Hlozek, R, Patty Ho, S, Hoang, T, Holder, G, Holzapfel, W, Hood, J, Hubmayr, J, Huffenberger, K, Hui, H, Irwin, K, Jeong, O, Johnson, B, Jones, W, Hwan Kang, J, Karkare, K, Katayama, N, Keskitalo, R, Kisner, T, Knox, L, Koopman, B, Kosowsky, A, Kovac, J, Kovetz, E, Kuhlmann, S, Kuo, C, Kusaka, A, Lahteenmaki, A, Lawrence, C, Lee, A, Lewis, A, Li, D, Linder, E, Loverde, M, Lowitz, A, Lubin, P, Madhavacheril, M, Mantz, A, Marques, G, Matsuda, F, Mauskopf, P, Mccarrick, H, Mcmahon, J, Daniel Meerburg, P, Melin, J, Menanteau, F, Meyers, J, Millea, M, Mohr, J, Moncelsi, L, Monzani, M, Mroczkowski, T, Mukherjee, S, Nagy, J, Namikawa, T, Nati, F, Natoli, T, Newburgh, L, Niemack, M, Nishino, H, Nord, B, Novosad, V, O'Brient, R, Padin, S, Palladino, S, Partridge, B, Petravick, D, Pierpaoli, E, Pogosian, L, Prabhu, K, Pryke, C, Puglisi, G, Racine, B, Rahlin, A, Sathyanarayana Rao, M, Raveri, M, Reichardt, C, Remazeilles, M, Rocha, G, Roe, N, Roy, A, Ruhl, J, Salatino, M, Saliwanchik, B, Schaan, E, Schillaci, A, Schmitt, B, Schmittfull, M, Scott, D, Sehgal, N, Shandera, S, Sherwin, B, Shirokoff, E, Simon, S, Slosar, A, Spergel, D, S, T, Staggs, S, Stark, A, Starkman, G, Stompor, R, Stoughton, C, Suzuki, A, Tajima, O, Teply, G, Thompson, K, Thorne, B, Timbie, P, Tomasi, M, Tristram, M, Tucker, G, Umilta, C, Van Engelen, A, Vavagiakis, E, Vieira, J, Vieregg, A, Wagoner, K, Wallisch, B, Wang, G, Watson, S, Westbrook, B, Whitehorn, N, Wollack, E, Kimmy Wu, W, Xu, Z, Eric Yang, H, Yasini, S, Yefremenko, V, Won Yoon, K, Young, E, Yu, C, Zonca, A, University of California Irvine, Johns Hopkins University, University of Illinois at Urbana-Champaign, SLAC National Accelerator Laboratory, University of California Berkeley, Stanford University, University of Oxford, Rice University, Fermi National Accelerator Laboratory, University of California San Diego, International School for Advanced Studies, Lawrence Berkeley National Laboratory, Harvard University, University of New Mexico, Argonne National Laboratory, Université Paris-Diderot, California Institute of Technology, Cornell University, University of Melbourne, University of Cincinnati, Ludwig Maximilian University of Munich, University of Toronto, UMR7095, Stony Brook University, University of Manchester, Arizona State University, Florida State University, Cardiff University, Dartmouth College, University of Geneva, University of Cambridge, The University of Tokyo, University of Groningen, University of Chicago, University of Pennsylvania, McGill University, National Institute of Standards and Technology, NASA Goddard Space Flight Center, University of Sussex, Princeton University, Simon Fraser University, National Institute for Nuclear Physics, Haverford College, Stockholm University, Case Western Reserve University, University of British Columbia, University of Colorado Boulder, University of Minnesota Twin Cities, University of Michigan, Ann Arbor, Simons Foundation, Columbia University, University of Virginia, University of California Davis, Yale University, University of Pittsburgh, Ben-Gurion University of the Negev, Department of Electronics and Nanoengineering, Jet Propulsion Laboratory, University of California Santa Barbara, Perimeter Institute for Theoretical Physics, Service d'Astrophysique CEA, European Southern Observatory, Washington University St. Louis, University of Milan - Bicocca, University of Southern California, Institute for Advanced Studies, Pennsylvania State University, Brookhaven National Laboratory, Kyoto University, University of Wisconsin-Madison, University of Milano, Université Paris-Saclay, Brown University, Syracuse University, University of California Los Angeles, Aalto-yliopisto, and Aalto University
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Astrophysics and Astronomy ,Cosmology and Nongalactic Astrophysics (astro-ph.CO) ,Cosmology, CMB ,Settore FIS/05 ,Space and Planetary Science ,astro-ph.CO ,FOS: Physical sciences ,Astronomy and Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,Galaxies and Cosmology ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
CMB-S4---the next-generation ground-based cosmic microwave background (CMB) experiment---is set to significantly advance the sensitivity of CMB measurements and enhance our understanding of the origin and evolution of the Universe, from the highest energies at the dawn of time through the growth of structure to the present day. Among the science cases pursued with CMB-S4, the quest for detecting primordial gravitational waves is a central driver of the experimental design. This work details the development of a forecasting framework that includes a power-spectrum-based semi-analytic projection tool, targeted explicitly towards optimizing constraints on the tensor-to-scalar ratio, $r$, in the presence of Galactic foregrounds and gravitational lensing of the CMB. This framework is unique in its direct use of information from the achieved performance of current Stage 2--3 CMB experiments to robustly forecast the science reach of upcoming CMB-polarization endeavors. The methodology allows for rapid iteration over experimental configurations and offers a flexible way to optimize the design of future experiments given a desired scientific goal. To form a closed-loop process, we couple this semi-analytic tool with map-based validation studies, which allow for the injection of additional complexity and verification of our forecasts with several independent analysis methods. We document multiple rounds of forecasts for CMB-S4 using this process and the resulting establishment of the current reference design of the primordial gravitational-wave component of the Stage-4 experiment, optimized to achieve our science goals of detecting primordial gravitational waves for $r > 0.003$ at greater than $5��$, or, in the absence of a detection, of reaching an upper limit of $r < 0.001$ at $95\%$ CL., 24 pages, 8 figures, 9 tables, submitted to ApJ. arXiv admin note: text overlap with arXiv:1907.04473
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- 2022
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200. Exploring cosmic origins with CORE:mitigation of systematic effects
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M. Tristram, Daniela Paoletti, Eric Hivon, Jose M. Diego, M. López-Caniego, Hannu Kurki-Suonio, D. Tramonte, J. Borrill, M. Piat, Shaul Hanany, Guillaume Patanchon, M. Bonato, Matthieu Roman, J. González-Nuevo, F. Piacentini, G. Signorelli, Stephen M. Feeney, Silvia Galli, Miguel Quartin, M. Migliaccio, François R. Bouchet, A. Bonaldi, E. Di Valentino, R. Van de Weijgaert, Ricardo Genova-Santos, L. Salvati, Zhen-Yi Cai, Nicola Bartolo, Martino Calvo, Julien Lesgourgues, Reijo Keskitalo, Alessandro Coppolecchia, Jens Chluba, Carlo Burigana, G. Castellano, Bruno Maffei, D. McCarthy, R. Banerji, Daniel Baumann, Martina Gerbino, Thomas Kitching, Alessandro Monfardini, Francois Boulanger, M. Tomasi, Carlos Hernández-Monteagudo, L. Polastri, Alessandro Melchiorri, Ted Kisner, S. Basak, Giuseppe D'Alessandro, Peter A. R. Ade, Massimiliano Lattanzi, Sebastien Clesse, Marco Bersanelli, Mario Zannoni, R. Allison, Will Handley, J. Valiviita, P. Vielva, Diego Molinari, Mathieu Remazeilles, A. Gruppuso, Matthew Hills, K. Kiiveri, A. Lewis, Mattia Negrello, Michele Liguori, Carole Tucker, Gemma Luzzi, G. Polenta, Silvia Masi, Alessandro Paiella, Giampaolo Pisano, L. Pagano, P. de Bernardis, Anthony Challinor, Sebastian Grandis, Martin Bucher, Luca Lamagna, R. Fernandez-Cobos, Tiziana Trombetti, G. de Gasperis, C. S. Carvalho, A. Tartari, Jacques Delabrouille, Nazzareno Mandolesi, C. Baccigalupi, Vivian Poulin, Ana Achúcarro, Alessio Notari, Alessandro Buzzelli, I. Colantoni, Enrique Martinez-Gonzalez, Fabio Finelli, James G. Bartlett, Francesco Forastieri, Mario Ballardini, Anthony Lasenby, Vincent Vennin, Christopher G. R. Wallis, E. Keihänen, D. T. Hoang, J. J. A. Baselmans, Jean-Baptiste Melin, M. Ashdown, Sophie Henrot-Versille, M. Kunz, S. Hagstotz, Josquin Errard, Jose Alberto Rubino-Martin, C. J. A. P. Martins, G. de Zotti, Neil Trappe, Nicola Vittorio, V. Lindholm, J. Greenslade, Karl Young, O. Perdereau, B. Van Tent, A. J. Banday, Thejs Brinckmann, Graziano Rossi, A. Pollo, C. Hervias-Caimapo, Martin Crook, Paolo Natoli, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Institut de recherche en astrophysique et planétologie (IRAP), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Institut Néel (NEEL), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Institut Lagrange de Paris, Sorbonne Université (SU), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Département de Physique des Particules (ex SPP) (DPP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Laboratoire d'Annecy-le-Vieux de Physique Théorique (LAPTH), Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Théorique d'Orsay [Orsay] (LPT), Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11), CORE, Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF), Sorbonne Universités, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Cryogénie (NEEL - Cryo), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Département de Physique des Particules (ex SPP) (DPhP), Hélium : du fondamental aux applications (NEEL - HELFA), Helsinki Institute of Physics, Department of Physics, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Natoli, P, Ashdown, M, Banerji, R, Borrill, J, Buzzelli, A, de Gasperis, G, Delabrouille, J, Hivon, E, Molinari, D, Patanchon, G, Polastri, L, Tomasi, M, Bouchet, F, Henrot-Versillé, S, Hoang, D, Keskitalo, R, Kiiveri, K, Kisner, T, Lindholm, V, Mccarthy, D, Piacentini, F, Perdereau, O, Polenta, G, Tristram, M, Achucarro, A, Ade, P, Allison, R, Baccigalupi, C, Ballardini, M, Banday, A, Bartlett, J, Bartolo, N, Basak, S, Baumann, D, Bersanelli, M, Bonaldi, A, Bonato, M, Boulanger, F, Brinckmann, T, Bucher, M, Burigana, C, Cai, Z, Calvo, M, Carvalho, C, Castellano, M, Challinor, A, Chluba, J, Clesse, S, Colantoni, I, Coppolecchia, A, Crook, M, D'Alessandro, G, de Bernardis, P, Zotti, G, Valentino, E, Diego, J, Errard, J, Feeney, S, Fernandez-Cobos, R, Finelli, F, Forastieri, F, Galli, S, Genova-Santos, R, Gerbino, M, González-Nuevo, J, Grandis, S, Greenslade, J, Gruppuso, A, Hagstotz, S, Hanany, S, Handley, W, Hernandez-Monteagudo, C, Hervías-Caimapo, C, Hills, M, Keihänen, E, Kitching, T, Kunz, M, Kurki-Suonio, H, Lamagna, L, Lasenby, A, Lattanzi, M, Lesgourgues, J, Lewis, A, Liguori, M, López-Caniego, M, Luzzi, G, Maffei, B, Mandolesi, N, Martinez-González, E, Martins, C, Masi, S, Matarrese, S, Melchiorri, A, Melin, J, Migliaccio, M, Monfardini, A, Negrello, M, Notari, A, Pagano, L, Paiella, A, Paoletti, D, Piat, M, Pisano, G, Pollo, A, Poulin, V, Quartin, M, Remazeilles, M, Roman, M, Rossi, G, Rubino-Martin, J, Salvati, L, Signorelli, G, Tartari, A, Tramonte, D, Trappe, N, Trombetti, T, Tucker, C, Valiviita, J, de Weijgaert, R, Tent, B, Vennin, V, Vielva, P, Vittorio, N, Wallis, C, Young, K, Zannoni, M, String Theory (ITFA, IoP, FNWI), AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), Institut d'Astrophysique de Paris ( IAP ), Université Pierre et Marie Curie - Paris 6 ( UPMC ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire de l'Accélérateur Linéaire ( LAL ), Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), Institut de recherche en astrophysique et planétologie ( IRAP ), Université Paul Sabatier - Toulouse 3 ( UPS ) -Observatoire Midi-Pyrénées ( OMP ) -Centre National de la Recherche Scientifique ( CNRS ), Institut d'astrophysique spatiale ( IAS ), Université Paris-Sud - Paris 11 ( UP11 ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Centre National de la Recherche Scientifique ( CNRS ), Institut Néel ( NEEL ), Université Grenoble Alpes [Saint Martin d'Hères]-Centre National de la Recherche Scientifique ( CNRS ), Laboratoire de Physique Nucléaire et de Hautes Énergies ( LPNHE ), Université Pierre et Marie Curie - Paris 6 ( UPMC ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ), Département de Physique des Particules (ex SPP) ( DPP ), Institut de Recherches sur les lois Fondamentales de l'Univers ( IRFU ), Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Université Paris-Saclay, Laboratoire d'Annecy-le-Vieux de Physique Théorique ( LAPTH ), Université Savoie Mont Blanc ( USMB [Université de Savoie] [Université de Chambéry] ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire de Physique Théorique d'Orsay [Orsay] ( LPT ), and Université Paris-Sud - Paris 11 ( UP11 ) -Centre National de la Recherche Scientifique ( CNRS )
- Subjects
[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph] ,Cosmic microwave background ,Astrophysics ,Residual ,01 natural sciences ,NOISE ,Photometric calibration ,CMBR experiments ,[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] ,010303 astronomy & astrophysics ,media_common ,Physics ,COSMIC cancer database ,INSTRUMENT ,FLIGHT ,Astrophysics::Instrumentation and Methods for Astrophysics ,symbols ,astro-ph.CO ,CMBR experiment ,Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - Cosmology and Nongalactic Astrophysics ,CMBR polarisation ,Cosmology and Nongalactic Astrophysics (astro-ph.CO) ,media_common.quotation_subject ,POLARIZATION MAPS ,FOS: Physical sciences ,ComputerApplications_COMPUTERSINOTHERSYSTEMS ,NO ,LIKELIHOOD ,symbols.namesake ,FIS/05 - ASTRONOMIA E ASTROFISICA ,Settore FIS/05 - Astronomia e Astrofisica ,Robustness (computer science) ,0103 physical sciences ,SPECTRA ,[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] ,Planck ,Instrumentation and Methods for Astrophysics (astro-ph.IM) ,CMBR polarization ,010308 nuclear & particles physics ,MAP-MAKING ALGORITHM ,Astronomy and Astrophysics ,PLANCK SURVEYOR ,115 Astronomy, Space science ,CMBR experiments, CMBR polarisation, gravitational waves and CMBR polarization ,Reliability engineering ,Future study ,CMB EXPERIMENTS ,Sky ,astro-ph.IM ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,gravitational waves and CMBR polarization ,astronomy and astrophysics - Abstract
This research used resources of the National Energy Research Scientific Computing Center, which is supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. We also thank CSC — IT Center for Science (Finland) for computational resources. We acknowledge financial support by ASI Grant 2016-24-H.0 and Academy of Finland grant 295113. This work has received funding from the European Union’s Horizon 2020 research and innovation programme under grant agreement number 687312. CJM is supported by an FCT Research Professorship, contract reference IF/00064/2012, funded by FCT/MCTES (Portugal) and POPH/FSE (EC). JGN acknowledges financial support from the Spanish MINECO for a ‘Ramon y Cajal’ fellowship (RYC-2013-13256) and the I+D 2015 project AYA2015-65887-P (MINECO/FEDER). GR acknowledges support from the National Research Foundation of Korea (NRF) through Grant No. 2017R1E1A1A01077508 funded by the Korean Ministry of Education, Science and Technology (MoEST), and from the faculty research fund of Sejong University in 2018. We thank Jean Kaplan for useful comments on the manuscript., Natoli, P., Ashdown, M., Banerji, R., Borrill, J., Buzzelli, A., De Gasperis, G., Delabrouille, J., Hivon, E., Molinari, D., Patanchon, G., Polastri, L., Tomasi, M., Bouchet, F.R., Henrot-Versillé, S., Hoang, D.T., Keskitalo, R., Kiiveri, K., Kisner, T., Lindholm, V., McCarthy, D., Piacentini, F., Perdereau, O., Polenta, G., Tristram, M., Achucarro, A., Ade, P., Allison, R., Baccigalupi, C., Ballardini, M., Banday, A.J., Bartlett, J., Bartolo, N., Basak, S., Baumann, D., Bersanelli, M., Bonaldi, A., Bonato, M., Boulanger, F., Brinckmann, T., Bucher, M., Burigana, C., Cai, Z.-Y., Calvo, M., Carvalho, C.-S., Castellano, M.G., Challinor, A., Chluba, J., Clesse, S., Colantoni, I., Coppolecchia, A., Crook, M., D'Alessandro, G., De Bernardis, P., Zotti, G.D., Valentino, E.D., Diego, J.-M., Errard, J., Feeney, S., Fernandez-Cobos, R., Finelli, F., Forastieri, F., Galli, S., Genova-Santos, R., Gerbino, M., González-Nuevo, J., Grandis, S., Greenslade, J., Gruppuso, A., Hagstotz, S., Hanany, S., Handley, W., Hernandez-Monteagudo, C., Hervías-Caimapo, C., Hills, M., Keihänen, E., Kitching, T., Kunz, M., Kurki-Suonio, H., Lamagna, L., Lasenby, A., Lattanzi, M., Lesgourgues, J., Lewis, A., Liguori, M., López-Caniego, M., Luzzi, G., Maffei, B., Mandolesi, N., Martinez-González, E., Martins, C.J.A.P., Masi, S., Matarrese, S., Melchiorri, A., Melin, J.-B., Migliaccio, M., Monfardini, A., Negrello, M., Notari, A., Pagano, L., Paiella, A., Paoletti, D., Piat, M., Pisano, G., Pollo, A., Poulin, V., Quartin, M., Remazeilles, M., Roman, M., Rossi, G., Rubino-Martin, J.-A., Salvati, L., Signorelli, G., Tartari, A., Tramonte, D., Trappe, N., Trombetti, T., Tucker, C., Valiviita, J., De Weijgaert, R.V., Tent, B.V., Vennin, V., Vielva, P., Vittorio, N., Wallis, C., Young, K., Zannoni, M.
- Published
- 2018
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