Showing 1–20 of 25 results
/ Date/ Name
Nov 11, 2025Euclid preparation: LXXXVII. Non-Gaussianity of 2-point statistics likelihood: Precise analysis of the matter power spectrum distributionOct 20, 2025Euclid preparation: The flat-sky approximation for the clustering of Euclid's photometric galaxiesOct 10, 2025Euclid preparation. Cosmology Likelihood for Observables in Euclid (CLOE). 3. Inference and ForecastsJun 10, 2025Euclid preparation: The NISP spectroscopy channel, on ground performance and calibrationMay 7, 2025Euclid preparation. The impact of redshift interlopers on the two-point correlation function analysisSep 25, 2019SUGAR: An improved empirical model of Type Ia Supernovae based on spectral featuresOct 22, 2018SNEMO: Improved Empirical Models for Type Ia SupernovaeApr 10, 2018Correcting for peculiar velocities of Type Ia Supernovae in clusters of galaxiesOct 16, 2017Follow up of GW170817 and its electromagnetic counterpart by Australian-led observing programsJan 5, 2017The Extinction Properties of and Distance to the Highly Reddened Type Ia Supernova SN 2012cuMar 19, 2015New measurement of the excited states in $^{11}$B via the elastic resonance scattering of $^{10}$Be + pDec 19, 2014Confirmation of a Star Formation Bias in Type Ia Supernova Distances and its Effect on Measurement of the Hubble ConstantFeb 27, 2014Type Ia supernova bolometric light curves and ejected mass estimates from the Nearby Supernova FactoryJan 14, 2014Type Ia Supernova Hubble Residuals and Host-Galaxy PropertiesOct 15, 2013Measuring cosmic bulk flows with Type Ia Supernovae from the Nearby Supernova FactoryApr 17, 2013Host Galaxy Properties and Hubble Residuals of Type Ia Supernovae from the Nearby Supernova FactoryApr 17, 2013Host Galaxies of Type Ia Supernovae from the Nearby Supernova FactoryFeb 12, 2013Standardizing Type Ia Supernova Absolute Magnitudes Using Gaussian Process Data RegressionOct 9, 2012Atmospheric extinction properties above Mauna Kea from the Nearby Supernova Factory spectro-photometric data setMar 21, 2012Constraining Type Ia supernova models: SN 2011fe as a test case