about
Characterization of the transmitted near-infrared wavefront error for the GRAVITY/VLTI Coudé Infrared Adaptive Optics System.METIS: the Mid-infrared E-ELT Imager and SpectrographFirst light for GRAVITY: Phase referencing optical interferometry for the Very Large Telescope InterferometerSimulated observations of high-redshift galaxies with the HARMONI spectrograph for the European Extremely Large TelescopeThe E-ELT first light spectrograph HARMONI: capabilities and modesCIAO: wavefront sensors for GRAVITYExoplanets with JWST: degeneracy, systematics and how to avoid themThe mid-infrared instrument for the James Webb Space Telescope: performance and operation of the Low-Resolution SpectrometerSimulated stellar kinematics studies of high-redshift galaxies with the HARMONI Integral Field SpectrographTelling twins apart: exo-Earths and Venuses with transit spectroscopyMolecular gas kinematics within the central 250 pc of the Milky WayDense gas in the Galactic central molecular zone is warm and heated by turbulencehsim: a simulation pipeline for the HARMONI integral field spectrograph on the European ELTErratum: Transit spectroscopy with JWST: systematics, star-spots and stitchingThe Mid-Infrared Instrument for theJames Webb Space Telescope, IV: The Low-Resolution SpectrometerTransit spectroscopy with James Webb Space Telescope: systematics, starspots and stitchingThe Milky Way Project: leveraging citizen science and machine learning to detect interstellar bubblesHARMONI: the first light integral field spectrograph for the E-ELTIntegration and bench testing for the GRAVITY Coudé IR adaptive optics (CIAO) wavefront sensorIntegral field spectroscopy of high redshift galaxies with the HARMONI spectrograph on the European Extremely Large TelescopeSimulating observations with HARMONI: the integral field spectrograph for the European Extremely Large TelescopeThe first SPIE software Hack DayAll quiet on the Western front? New evidence for massive star formation in Sgr CEarly-stage massive star formation near the galactic center: Sgr CSurface figure measurement of flat mirrors based on the subaperture stitching interferometryAn end-to-end instrument model for the proposed E-ELT instrument METISGRAVITY Coudé Infrared Adaptive Optics (CIAO) system for the VLT InterferometerInnovative technology for optical and infrared astronomyThe Milky Way Project First Data Release: a bubblier Galactic discThe Milky Way project: a statistical study of massive star formation associated with infrared bubblesOptimizing the transmission of the GRAVITY/VLTI near-infrared wavefront sensorExtreme adaptive optics in the mid-IR: The METIS AO systemSpS1-High-resolution infrared spectroscopy at high and low altitudesCorrecting METIS spectra for telluric absorption to maximize spectral fidelityInstrument concept and science case for the mid-IR E-ELT imager and spectrograph METISMETIS: system engineering and optical design of the mid-infrared E-ELT instrumentMid-infrared astronomy with the E-ELT: performance of METISOptical performance of the JWST/MIRI flight model: characterization of the point spread function at high resolutionPerformance verification of the MIRI imager flight model at CEAThe METIS AO system: bringing extreme adaptive optics to the mid-IR
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description
hulumtuese
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researcher
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wetenschapper
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հետազոտող
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name
Sarah Kendrew
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Sarah Kendrew
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Sarah Kendrew
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Sarah Kendrew
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type
label
Sarah Kendrew
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Sarah Kendrew
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Sarah Kendrew
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Sarah Kendrew
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prefLabel
Sarah Kendrew
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Sarah Kendrew
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Sarah Kendrew
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Sarah Kendrew
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sarahkendrew
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0000-0002-7612-0469