The detection of ozone (O3) in the surface ices of Ganymede, Jupiter's largest moon, and of
the Saturnian moons Rhea and Dione, has motivated several studies on the route of …

Context. Molecular oxygen, nitrogen, and ozone have been detected on some satellites of
Saturn and Jupiter, as well as on comets. They are also expected to be present in ice-grain …

ABSTRACT Methyl acetate (${\mathrm {CH}} _ {3}{\mathrm {COOCH}} _ {3} $) has been
recently observed by the IRAM 30 m radio telescope in Orion, though the presence of its …

To establish the spectroscopy of the solids α-and β-oxygen, we measured the thermal
ramping spectra of the solid O2 in visible and near-infrared (near-IR) wavelength range 450 …

We report spectra in the visible and near-infrared wavelength range 350–1155 nm and in
the mid-infrared range 500–5000 cm–1 (2–20 m) of molecular oxygen at temperatures 6–33 …

We report ultraviolet and far-vacuum ultraviolet (FUV) absorption spectra of solid molecular
oxygen recorded over the wavelength region 110–365 nm for temperatures between 9 and …

Sulphur dioxide (SO 2) is known to be present on Callisto. In this paper, we studied the
chemical evolution of SO 2 astrochemical ice induced by irradiation using 9 eV (137.7 nm) …

We propose a new model for treating solid-phase photoprocesses in interstellar ice analogs.
In this approach, photoionization and photoexcitation are included in more detail, and the …

We present the first analysis of far-ultraviolet reflectance spectra of regions on Rhea's
leading and trailing hemispheres collected by the Cassini Ultraviolet Imaging Spectrograph …

The recent discovery of hydroxylamine (NH2OH) molecule in the interstellar medium
emphasizes the need to study the molecule in laboratory astrochemical ice analogues …