Showing 1–20 of 58 results
/ Date/ Name
Feb 11, 2003First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing Methods and Systematic Errors LimitsJan 15, 2009Zonal flow generation in collisionless trapped electron mode turbulenceJan 21, 2025A Measurement of the Largest-Scale CMB E-mode Polarization with CLASSJan 14, 2009Zonal flow generation in ion temperature gradient mode turbulenceJun 15, 2007On advanced fluid modelling of drift wave turbulenceFeb 11, 2003First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power SpectrumMay 1, 2023CLASS Data Pipeline and Maps for 40 GHz Observations through 2022Jan 26, 2010Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Power Spectra and WMAP-Derived ParametersApr 25, 2019Determination of the Cosmic Infrared Background from COBE/FIRAS and Planck HFI ObservationsJun 30, 2021Discovery of Super-Slow Rotating Asteroids with ATLAS and ZTF photometryMay 26, 1998The COBE Diffuse Infrared Background Experiment Search for the Cosmic Infrared Background: III. Separation of Galactic Emission from the Infrared Sky BrightnessSep 3, 2025Nearly full-sky low-multipole CMB temperature anisotropy: III. CMB anomaliesSep 24, 2018The ATLAS All-Sky Stellar Reference CatalogJul 4, 2019An Examination of Galactic Polarization with Application to the Planck TB CorrelationJan 12, 2021Comparison of the physical properties of the L4 and L5 Trojan asteroids from ATLAS dataJul 20, 2017Elucidating $Λ$CDM: Impact of Baryon Acoustic Oscillation Measurements on the Hubble Constant DiscrepancyMar 17, 2006Three Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Polarization AnalysisMar 17, 2006Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Beam Profiles, Data Processing, Radiometer Characterization and Systematic Error LimitsMar 4, 2008Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological InterpretationMar 5, 2008Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power Spectra