Modeling Atmospheric Emission for CMB Ground-based Observations
| العنوان: | Modeling Atmospheric Emission for CMB Ground-based Observations |
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| المؤلفون: | Nathan Stebor, Tomotake Matsumura, Christian L. Reichardt, Michael J. Myers, S. Takakura, Masaya Hasegawa, Giuseppe Puglisi, Adrian T. Lee, Kaori Hattori, Charles A. Hill, Julian Borrill, Nobuhiko Katayama, K. M. Rotermund, Stephen M. Feeney, Kam Arnold, Davide Poletti, E. M. Leitch, Darcy Barron, Neil Goeckner-Wald, Yuji Chinone, Peter A. R. Ade, Nathan Whitehorn, M. Atlas, Y. Akiba, Greg Jaehnig, Andrew H. Jaffe, Chang Feng, Scott Chapman, Gabriel M. Rebeiz, Brian Keating, A. Gilbert, Colin Ross, M. Navaroli, Aritoki Suzuki, Tucker Elleflot, Graeme Smecher, Hans P. Paar, Ted Kisner, J. Peloton, Oliver Jeong, Amit P. S. Yadav, Giulio Fabbian, J. P. Kaufman, D. E. Schenck, N. W. Halverson, A. Ducout, A. Tikhomirov, Masashi Hazumi, Takayuki Tomaru, Radek Stompor, Praween Siritanasak, Zigmund Kermish, Oliver Zahn, Blake D. Sherwin, D. Boettger, M. Le Jeune, Takahiro Okamura, A. Cukierman, B. Wilson, D. Leon, Nathan J. Miller, Reijo Keskitalo, Bryan Steinbach, M. A. Dobbs, Yuki Inoue, Josquin Errard, W. L. Holzapfel, Y. Hori, Jacques Delabrouille, Paul L. Richards, Frederick Matsuda, H. Nishino, Osamu Tajima, Eric V. Linder, Carlo Baccigalupi |
| المساهمون: | Biological Imaging Core, Department of Biological Sciences, University of Notre Dame [Indiana] (UND), 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), Regional Virus Laboratory, Royal Victoria Hospital, Laboratoire de glaciologie et géophysique de l'environnement (LGGE), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Department of Physics [Berkeley], University of California [Berkeley], University of California-University of California, Korea Research Institute for Human Settlements (KRIHS), Korea Research Institute for Human Settlements, Department of Endocrinology, Universiteit Gent = Ghent University [Belgium] (UGENT), Centre interdisciplinaire de recherches sur les valeurs, les idées, les identités et les compétences en Éducation et en formation (CIVIIC), Université de Rouen Normandie (UNIROUEN), Normandie Université (NU)-Normandie Université (NU), Department of Computer Science [Amherst], University of Massachusetts [Amherst] (UMass Amherst), University of Massachusetts System (UMASS)-University of Massachusetts System (UMASS), Department of Atmospheric Science [Laramie], University of Wyoming (UW), The University of Tokyo (UTokyo), Carnegie Mellon University [Pittsburgh] (CMU), Columbia University [New York], University of California [San Diego] (UC San Diego), University of California, 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), Observatoire des Sciences de l'Univers de Grenoble (OSUG), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS), University of California [Berkeley] (UC Berkeley), University of California (UC)-University of California (UC), Universiteit Gent = Ghent University (UGENT), University of California (UC), 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 Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS), Ghent University [Belgium] (UGENT), The University of Tokyo, Science and Technology Facilities Council (STFC), Imperial College Trust, Science and Technology Facilities Council [2006-2012], 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), Errard, J, Ade, P, Akiba, Y, Arnold, K, Atlas, M, Baccigalupi, C, Barron, D, Boettger, D, Borrill, J, Chapman, S, Chinone, Y, Cukierman, A, Delabrouille, J, Dobbs, M, Ducout, A, Elleflot, T, Fabbian, G, Feng, C, Feeney, S, Gilbert, A, Goeckner-Wald, N, Halverson, N, Hasegawa, M, Hattori, K, Hazumi, M, Hill, C, Holzapfel, W, Hori, Y, Inoue, Y, Jaehnig, G, Jaffe, A, Jeong, O, Katayama, N, Kaufman, J, Keating, B, Kermish, Z, Keskitalo, R, Kisner, T, Le Jeune, M, Lee, A, Leitch, E, Leon, D, Linder, E, Matsuda, F, Matsumura, T, Miller, N, Myers, M, Navaroli, M, Nishino, H, Okamura, T, Paar, H, Peloton, J, Poletti, D, Puglisi, G, Rebeiz, G, Reichardt, C, Richards, P, Ross, C, Rotermund, K, Schenck, D, Sherwin, B, Siritanasak, P, Smecher, G, Stebor, N, Steinbach, B, Stompor, R, Suzuki, A, Tajima, O, Takakura, S, Tikhomirov, A, Tomaru, T, Whitehorn, N, Wilson, B, Yadav, A, Zahn, O |
| المصدر: | The Astrophysical Journal The Astrophysical Journal, American Astronomical Society, 2015, 809, pp.63. ⟨10.1088/0004-637X/809/1/63⟩ The Astrophysical Journal, 2015, 809, pp.63. ⟨10.1088/0004-637X/809/1/63⟩ Astrophysical Journal Artículos CONICYT CONICYT Chile instacron:CONICYT |
| بيانات النشر: | HAL CCSD, 2015. |
| سنة النشر: | 2015 |
| مصطلحات موضوعية: | COMPONENT SEPARATION, POLARIZATION, Cosmology and Nongalactic Astrophysics (astro-ph.CO), 0306 Physical Chemistry (Incl. Structural), atmospheric effect, Cosmic microwave background, FOS: Physical sciences, Astronomy & Astrophysics, 0305 Organic Chemistry, 01 natural sciences, NOISE, Weather station, Atmosphere, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Settore FIS/05 - Astronomia e Astrofisica, 0103 physical sciences, Instrumentation and Methods for Astrophysics (astro-ph.IM), 010303 astronomy & astrophysics, Physics::Atmospheric and Oceanic Physics, ComputingMilieux_MISCELLANEOUS, SITES, Science & Technology, Settore FIS/05, 010308 nuclear & particles physics, Linear polarization, Detector, Astronomy and Astrophysics, FLUCTUATIONS, methods: data analysis, Computational physics, 0201 Astronomical And Space Sciences, Wavelength, methods: observational, 13. Climate action, Space and Planetary Science, Physical Sciences, astro-ph.CO, TURBULENCE, Environmental science, Millimeter, MICROWAVE BACKGROUND EXPERIMENTS, Astrophysics - Instrumentation and Methods for Astrophysics, methods: data analysi, Noise (radio), Astrophysics - Cosmology and Nongalactic Astrophysics, astro-ph.IM, atmospheric effects |
| الوصف: | Atmosphere is one of the most important noise sources for ground-based cosmic microwave background (CMB) experiments. By increasing optical loading on the detectors, it amplifies their effective noise, while its fluctuations introduce spatial and temporal correlations between detected signals. We present a physically motivated 3d-model of the atmosphere total intensity emission in the millimeter and sub-millimeter wavelengths. We derive a new analytical estimate for the correlation between detectors time-ordered data as a function of the instrument and survey design, as well as several atmospheric parameters such as wind, relative humidity, temperature and turbulence characteristics. Using an original numerical computation, we examine the effect of each physical parameter on the correlations in the time series of a given experiment. We then use a parametric-likelihood approach to validate the modeling and estimate atmosphere parameters from the POLARBEAR-I project first season data set. We derive a new 1.0% upper limit on the linear polarization fraction of atmospheric emission. We also compare our results to previous studies and weather station measurements. The proposed model can be used for realistic simulations of future ground-based CMB observations. Comment: 20 pages, 16 figures |
| اللغة: | English |
| تدمد: | 0004-637X 1538-4357 |
| الوصول الحر: | https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7caf15a1af991702235e3c30b583d198Test http://hal.in2p3.fr/in2p3-01184756Test |
| حقوق: | OPEN |
| رقم الانضمام: | edsair.doi.dedup.....7caf15a1af991702235e3c30b583d198 |
| قاعدة البيانات: | OpenAIRE |
| تدمد: | 0004637X 15384357 |
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