Showing 21–40 of 99 results
/ Date/ Name
May 17, 2004Discovery of kilogauss magnetic fields in three DA white dwarfsNov 12, 2015First light of the VLT planet finder SPHERE. I. Detection and characterization of the sub-stellar companion GJ 758 BNov 12, 2015First light of the VLT planet finder SPHERE. IV. Physical and chemical properties of the planets around HR8799Jul 16, 2020On weakly informative prior distributions for the heterogeneity parameter in Bayesian random-effects meta-analysisOct 17, 2025Multiwavelength analysis of polarized light in HD 100453Jan 21, 2025The SPHERE infrared survey for exoplanets (SHINE). V. Complete observations, data reduction and analysis, detection performances, and final resultsMar 5, 2021The SPHERE infrared survey for exoplanets (SHINE) -- II. Observations, Data reduction and analysis Detection performances and early-resultsNov 23, 2025Resolution and calibration effects in high contrast polarimetric imaging of circumstellar scattering regionsMay 23, 2022PCA-Boosted Autoencoders for Nonlinear Dimensionality Reduction in Low Data RegimesNov 21, 2022The high-albedo, low polarization disk around HD 114082 harbouring a Jupiter-sized transiting planetOct 19, 2018Mapping the global design space of nanophotonic components using machine learning pattern recognitionDec 6, 2018Investigating the presence of two belts in the HD 15115 systemMar 30, 2020Isolator-free Integration of C-band InAs-InP Quantum Dash Buried Heterostructure Lasers with Silicon WaveguidesMay 9, 2019Optical polarized phase function of the HR\,4796A dust ringJun 17, 2019The SPHERE view of the jet and the envelope of RY TauDec 18, 2018Active learning for efficiently training emulators of computationally expensive mathematical modelsJul 9, 2021Fibre Fabry-Pérot Astrophotonic Correlation Spectroscopy for Remote Gas Identification and Radial Velocity MeasurementsMar 15, 2021HD142527: Quantitative disk polarimetry with SPHEREDec 10, 2020Investigating three Sirius-like systems with SPHERENov 13, 2015The close circumstellar environment of Betelgeuse - III. SPHERE/ZIMPOL visible polarimetry of the inner envelope and photosphere