Suplementary material for the article "Modeling the Radiolysis in H₂O:HCOOH Ice: Connecting Laboratory Experiments with Astronomical Measurements"
Abstract
SUPPORTING INFORMATION FOR THE ARTCILE "Modeling the Radiolysis in H₂O:HCOOH Ice: Connecting Laboratory Experiments with Astronomical Measurements" AUTHORS: Fargnoli, C. M. F; Moraes, L.; Pilling, S. SUPPORTING INFORMATION S1 - complete system of coupled equations used in the PROCODA code to model the chemical evolution of ice H₂O:HCOOH (1:1) at 15 K under irradiation by cosmic ray analogues H2O:HCOOH (1:1) ice. SUPPORTING INFORMATION S2 - An excel file with the list All the coupled reactions and calculated effective rate coefficients (ERCs) for the studied H2O:HCOOH (1:1) ice. SUPPORTING INFORMATION S3 - An excel file with the list the computed columns densities (and also desorption information), normalized by the column density of parent species, for all modeled species as function of time for the studied H2O:HCOOH (1:1) ice.
Fields of Study & Subjects
Astrophysics and Star Formation Studies
Astro and Planetary Science
Chemical Reactions and Mechanisms
Publication details
- Journal / source
- Zenodo (CERN European Organization for Nuclear Research)
- Publication date
- 26 January 2026