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Naji, M. |
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Motta, Antonella |
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Aletan, Dirar |
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Mohamed, Tarek |
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Ertürk, Emre |
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Taccardi, Nicola |
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Kononenko, Denys |
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Petrov, R. H. | Madrid |
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Alshaaer, Mazen | Brussels |
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Bih, L. |
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Casati, R. |
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Muller, Hermance |
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Kočí, Jan | Prague |
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Šuljagić, Marija |
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Kalteremidou, Kalliopi-Artemi | Brussels |
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Azam, Siraj |
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Ospanova, Alyiya |
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Blanpain, Bart |
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Ali, M. A. |
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Popa, V. |
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Rančić, M. |
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Ollier, Nadège |
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Azevedo, Nuno Monteiro |
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Landes, Michael |
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Rignanese, Gian-Marco |
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Wollack, Edward
in Cooperation with on an Cooperation-Score of 37%
Topics
Publications (17/17 displayed)
- 2022Plasma based production of AlF<SUB>3</SUB>-passivated aluminum mirrors for UVOIR astronomycitations
- 2022Characterization of aerogel scattering filters for astronomical telescopes
- 2022Testing CMB Anomalies in E-mode Polarization with Current and Future Data
- 2021Process for fabricating one or more ultra-large area nanoscale polymer films
- 2021Fabricating ultra-thin structured polymer films
- 2021The Simons Observatory: metamaterial microwave absorber and its cryogenic applications.citations
- 2020The CLASS 150/220 GHz Polarimeter Array: Design, Assembly, and Characterizationcitations
- 2019Low-Loss Microstrip Transmission Line Fabricated with Improved Liftoff Process
- 2018Modeling Strategies for Superconducting Microstrip Transmission Line Structurescitations
- 2017Superconducting Vacuum-Gap Crossovers for High Performance Microwave Applicationscitations
- 2016Superconducting Vacuum-Gap Crossovers for High Performance Microwave Applications
- 2016Wide-stopband aperiodic phononic filterscitations
- 2016Silicon-Based Antenna-Coupled Polarization-Sensitive Millimeter-Wave Bolometer Arrays for Cosmic Microwave Background Instrumentscitations
- 2014A Cryogenic Infrared Calibration Targetcitations
- 2008Compact Low-Loss Planar Magic-T
- 2007Electromagnetic and Thermal Properties of a Conductively Loaded Epoxycitations
- 2005Ultra-Compact Broadband High-Spurious Suppression Bandpass Filter Using Double Split-end Stepped Impedance Resonators
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document
Testing CMB Anomalies in E-mode Polarization with Current and Future Data
Abstract
In this paper, we explore the power of the cosmic microwave background (CMB) polarization (E-mode) data to corroborate four potential anomalies in CMB temperature data: the lack of large angular-scale correlations, the alignment of the quadrupole and octupole (Q-O), the point-parity asymmetry, and the hemispherical power asymmetry. We use CMB simulations with noise representative of three experiments -- the Planck satellite, the Cosmology Large Angular Scale Surveyor (CLASS), and the LiteBIRD satellite -- to test how current and future data constrain the anomalies. We find the correlation coefficientsbetween temperature and E-mode estimators to be less than $0.1$, except for the point-parity asymmetry ($=0.17$ for cosmic-variance-limited simulations), confirming that E-modes provide a check on the anomalies that is largely independent of temperature data. Compared to Planck component-separated CMB data (SMICA), the putative LiteBIRD survey would reduce errors on E-mode anomaly estimators by factors of $ 3$ for hemispherical power asymmetry and point-parity asymmetry, and by $ 26$ for lack of large-scale correlation. The improvement in Q-O alignment is not obvious due to large cosmic variance, but we found the ability to pin down the estimator value will be improved by a factor . Improvements with CLASS are intermediate to these.