Showing 1–20 of 26 results
/ Date/ Name
Mar 23, 2023JWST MIRI flight performance: The Medium-Resolution SpectrometerDec 10, 2020Characterization of the optical properties of the buried contact of the JWST MIRI Si:As infrared blocked impurity band detectorsJul 31, 2020The nature of point source fringes in mid-infrared spectra acquired with the James Webb Space TelescopeJun 16, 2024The MIRI/MRS Library I. Empirically correcting detector charge migration in unresolved sourcesJul 13, 2023MINDS. Abundant water and varying C/O across the disk of Sz 98 as seen by JWST/MIRIMar 23, 2023The Brighter-Fatter Effect in the JWST MIRI Si:As IBC detectors I. Observations, impact on science, and modellingNov 14, 202315NH3 in the atmosphere of a cool brown dwarfApr 10, 2023The James Webb Space Telescope MissionDec 16, 2024Combined analysis of the 12.8 and 15 $μm$ JWST/MIRI eclipse observations of TRAPPIST-1 bJul 12, 2022The Science Performance of JWST as Characterized in CommissioningJun 8, 2023A 3D Drizzle Algorithm for JWST and Practical Application to the MIRI Medium Resolution SpectrometerOct 12, 2022Nested Dust Shells around the Wolf-Rayet Binary WR 140 observed with JWSTJul 31, 2023The Chemical Inventory of the Inner Regions of Planet-forming Disks -- The JWST/MINDS ProgramFeb 19, 2025HCN and C2H2 in the atmosphere of a T8.5+T9 brown dwarf binarySep 23, 2024The James Webb Space Telescope Absolute Flux Calibration. III. Mid-Infrared Instrument Medium Resolution IFU SpectrometerNov 24, 2020The quantum efficiency and diffractive image artifacts of Si:As IBC mid-IR detector arrays at 5 $-$ 10 $μ$m: Implications for the JWST/MIRI detectorsNov 21, 2023SO2, silicate clouds, but no CH4 detected in a warm NeptuneSep 15, 2018Stellar pulsation and granulation as noise sources in exoplanet transit spectroscopy in the ARIEL space missionDec 15, 2022MINDS. The detection of $^{13}$CO$_{2}$ with JWST-MIRI indicates abundant CO$_{2}$ in a protoplanetary diskMar 20, 2024MINDS. The DR Tau disk I: combining JWST-MIRI data with high-resolution CO spectra to characterise the hot gas