Validation of the HITRAN 2016 and GEISA 2015 line lists using ACE-FTS solar occultation observations
Journal of Quantitative Spectroscopy and Radiative Transfer Elsevier 236 (2019) 106590
2.5-D retrieval of atmospheric properties from exoplanet phase curves: Application to WASP-43b observations
(2019)
Small bodies science with the Twinkle space telescope
JOURNAL OF ASTRONOMICAL TELESCOPES INSTRUMENTS AND SYSTEMS 5:3 (2019) 34004
Abstract:
© 2019 Society of PhotoOptical Instrumentation Engineers (SPIE). Twinkle is an upcoming 0.45-m space-based telescope equipped with a visible and two near-infrared spectrometers covering the spectral range 0.4 to 4.5 μm with a resolving power R 250 (λ < 2.42 μm) and R 60 (λ > 2.42 μm). We explore Twinkle's capabilities for small bodies science and find that, given Twinkle's sensitivity, pointing stability, and spectral range, the mission can observe a large number of small bodies. The sensitivity of Twinkle is calculated and compared to the flux from an object of a given visible magnitude. The number, and brightness, of asteroids and comets that enter Twinkle's field of regard is studied over three time periods of up to a decade. We find that, over a decade, several thousand asteroids enter Twinkle's field of regard with a brightness and nonsidereal rate that will allow Twinkle to characterize them at the instrumentation's native resolution with SNR > 100. Hundreds of comets can also be observed. Therefore, Twinkle offers researchers the opportunity to contribute significantly to the field of Solar System small bodies research.Detection of Propadiene on Titan
ASTROPHYSICAL JOURNAL LETTERS 881:2 (2019) ARTN L33
Ethane in Titan's Stratosphere from Cassini CIRS Far- and Mid-Infrared Spectra
(2019)