KMOS: Assembly, integration and testing of three 0.8-2.5 micron spectrographs
GROUND-BASED AND AIRBORNE INSTRUMENTATION FOR ASTRONOMY III 7735 (2010) ARTN 773551
Mapping Titan's HCN in the far infra-red: implications for photochemistry.
Faraday Discuss 147 (2010) 51-64
Abstract:
Observations of Titan's far infra-red spectra by the Cassini orbiter's Composite InfraRed Spectrometer have been used to determine the latitude distribution of HCN at 1 mbar by fitting the HCN and CO rotational lines in the 18-60 cm(-1) (160-550 microm) spectral range. Results confirm the north polar HCN enrichment previously observed using mid-IR data and support the conclusion that Titan's nitrile species are significantly more enriched than hydrocarbons species with similar predicted photochemical lifetimes. This suggests Titan's photochemical cycle includes an additional sink for nitrogen bearing species. The abundance of CO was also determined, and had a mean value of 55 +/- 6 ppm at 20 mbar. However, it was not possible to reliably determine the CO latitude variation due to unconstrained temperatures in the north polar lower stratosphere.Martian atmosphere as observed by VIRTIS-M on Rosetta spacecraft
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS 115 (2010) ARTN E04004
Pixel Multiplexing for Simultaneous High Resolution High Speed Image Capture
BIOPHYSICAL JOURNAL 98:3 (2010) 178A-178A
Recent progress on the KMOS multi-object integral-field spectrograph for ESO VLT
GROUND-BASED AND AIRBORNE INSTRUMENTATION FOR ASTRONOMY III 7735 (2010) ARTN 773515