Showing 1–20 of 38 results
/ Date/ Name
Aug 2, 2023Effect of Instrumental Polarization with a Half-Wave Plate on the $B$-Mode Signal: Prediction and CorrectionNov 13, 2003Multi-component power spectra estimation method for multi-detector observations of the Cosmic Microwave BackgroundMar 20, 2013Planck 2013 results X. Energetic particle effects: characterization, removal, and simulationOct 11, 2004CMB and foregrounds in WMAP first year dataOct 6, 2009BLAST05: Power Spectra of Bright Galactic Cirrus at Submillimeter WavelengthsApr 8, 2009Over half of the far-infrared background light comes from galaxies at z >= 1.2Apr 8, 2009A Bright Submillimeter Source in the Bullet Cluster (1E0657--56) Field Detected with BLASTApr 8, 2009BLAST: Correlations in the Cosmic Far-Infrared Background at 250, 350, and 500 microns Reveal Clustering of Star-Forming GalaxiesFeb 1, 2019Bandpass mismatch error for satellite CMB experiments II: Correcting for the spurious signalJun 30, 2021Simulations of systematic effects arising from cosmic rays in the LiteBIRD space telescope, and effects on the measurements of CMB $B$-modesDec 25, 2016Exploring Cosmic Origins with CORE: InflationJul 7, 2017Exploring cosmic origins with CORE: gravitational lensing of the CMBJul 20, 2010The Herschel-SPIRE Legacy Survey (HSLS): the scientific goals of a shallow and wide submillimeter imaging survey with SPIREApr 8, 2009BLAST: The Mass Function, Lifetimes, and Properties of Intermediate Mass Cores from a 50 Square Degree Submillimeter Galactic Survey in Vela (l = ~265)Jul 24, 2009Temperature Profiles and the Effect of AGN on Submillimeter Emission from BLAST Observations of Resolved GalaxiesJul 23, 2009BLAST: the Redshift SurveyMar 12, 2010Submillimetre observations of galaxy clusters with BLAST: the star-formation activity in Abell 3112Jun 15, 2021Detailed study of HWP non-idealities and their impact on future measurements of CMB polarization anisotropies from spaceNov 30, 2016Exploring Cosmic Origins with CORE: Cosmological ParametersSep 23, 2002Blind separation of noisy Gaussian stationary sources. Application to cosmic microwave background imaging