SCIENCE ENABLE PRODUCTS
- Supporting material – Gas-phase Elemental abundances in Molecular cloudS (GEMS) XI. The evolution of HCN, HNC, and N2H+ isotopic ratios in starless Credits to Tasa-Chaveli et al. 2025, A&A, 700, A226. doi:10.1051/0004-6361/202554121
- Supporting material – PRODIGE – Envelope to Disk with NOEMA VI: The missing Sulfur Problem Credits to Miranzo-Pastor et al. 2025, A&A, 700, A251. doi:10.1051/0004-6361/202554018
- SynthIceSpec: Synthetic Ice Spectra generator (Taillard et al., 2025, A&A, 694, A266)
- RAIRS spectrum of a H2O:CS2 (400:60 ML) ice mixture at 6 K (Taillard et al., 2025, A&A, 694, A266)
- IRAM 30m Large Program “Gas-phase elemental abundances in molecular clouds” (GEMS)
GEMS is a large program at the IRAM 30-meter telescope that was granted 458 hours of observing time. The GEMS project aims to determine the gas ionization degree, X(e-), and the elemental depletions (C, O, S, N) as a function of visual extinction in a set of prototypical star forming filaments located in Taurus, Perseus and Orion (TMC1, B213/L1495, B1b, NGC 1333, IC348, L1448, B5, Orion A). - Neural emulator for interstellar chemistry
Credits to Asensio Ramos, A., Westendorp Plaza, C., Navarro-Almaida, D., et al. 2024, MNRAS, 531, 4930. doi:10.1093/mnras/stae1432 ownload software from https://github.com/aasensio/neural_chemistry
