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The Fifth International Workshop on Ice Nucleation phase 2 (FIN-02): laboratory intercomparison of ice nucleation measurements
Published 2022“…For Argentinian soil dust particles, there was excellent agreement across all measurement methods; measures ranged within 1 order of magnitude for INP number concentrations, active fractions and calculated active site densities over a 25 to 30°C range and 5 to 8 orders of corresponding magnitude change in number concentrations. …”
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The TESS–Keck Survey. VI. Two Eccentric Sub-Neptunes Orbiting HIP-97166
Published 2023“…We confirmed the planetary nature of HIP-97166b with ground-based radial-velocity measurements and measured a mass of Mb = 20 ± 2 M⊕ along with a radius of Rb = 2.7 ± 0.1 R⊕ from photometry. …”
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Gravity Recovery and Interior Laboratory (GRAIL): Mapping the Lunar Interior from Crust to Core
Published 2016“…Each GRAIL orbiter contains a Lunar Gravity Ranging System instrument that conducts dual-one-way ranging measurements to measure precisely the relative motion between them, which in turn are used to develop the lunar gravity field map. …”
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PHOTOMETRICALLY DERIVED MASSES AND RADII OF THE PLANET AND STAR IN THE TrES-2 SYSTEM
Published 2015“…The ratio of the ellipsoidal variation to the Doppler beaming amplitudes agrees to better than 2σ with theoretical predications, while our measured planet mass and radius agree within 2σ of previously published values based on spectroscopic radial velocity measurements. We measure a geometric albedo of 0.0136[superscript +0.0022] [subscript –0.0033] and an occultation (secondary eclipse) depth of 6.5 [superscript +1.7] [subscript –1.8] ppm which we combined with the day/night planetary flux ratio to model the atmosphere of TrES-2b. …”
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