Showing 1–15 of 15 results
/ Date/ Name
Nov 6, 2025Combining CMB datasets with consistent foreground modellingFeb 13, 2025Predicting the detectability of sulphur-bearing molecules in the solid phase with simulated spectra of JWST instrumentsJul 19, 2024Formation and desorption of sulfur chains (H$_2$S$_x$ and S$_x$) in cometary ice: effects of ice composition and temperatureDec 4, 2023UV-photoprocessing of acetic acid (CH3COOH)-bearing interstellar ice analogsAug 11, 2023Physical properties of methanol (CH$_3$OH) ice as a function of temperature: Density, infrared band strengths, and crystallizationApr 25, 2023Multi-scale stamps for real-time classification of alert streamsAug 8, 2022DELIGHT: Deep Learning Identification of Galaxy Hosts of Transients using Multi-resolution ImagesApr 6, 2022Gas phase Elemental abundances in Molecular cloudS (GEMS) VI. A sulphur journey across star-forming regions: study of thioformaldehyde emissionApr 7, 2020Gas phase Elemental abundances in Molecular cloudS (GEMS). II. On the quest for the sulphur reservoir in molecular clouds: the $H_{2}S$ caseJan 6, 2020On The Photodesorption of CO$_2$ Ice Analogues: The Formation of Atomic C in The Ice and the Effect of The VUV Emission SpectrumeDec 8, 2017First detection of interstellar S2HFeb 23, 2016Study of the photon-induced formation and subsequent desorption of CH3 OH and H2 CO in interstellar ice analogsJan 11, 2016The sulfur depletion problem: upper limits on the H2S2, HS2, and S2 gas-phase abundances toward the low-mass warm core IRAS16293-2422Oct 19, 2015UV photoprocessing of CO2 ice: a complete quantification of photochemistry and photon-induced desorption processesJun 30, 2014Interstellar ice analogs: band strengths of H$_2$O, CO$_2$, CH$_3$OH, and NH$_3$ in the far-infrared region