
This repository contains a number of files related to the gas-phase kinetic sensitivity analysis presented and described in Byrne et al. 2024 (in prep). The raw abundances as a function of time for all analyses are contained in 'Sensitivity_raw.hdf5.zip', while the sensitivities are located in 'Sensitivity_data.hdf5.zip'. 'Sens_Walkthrough.ipynb' is a jupyter notebook that explains how to examine this data using functions defined in 'ranking.py' and 'plotting.py'. This notebook also requires the two reactions.in files. Finally, the input files used to generate the data along with the NAUTILUS modeling code can be found in 'Model-Inputs.zip'. These inputs primarily come from the development branch of cixue/BATMAN with minor changes described in a README file.
Kinetics, Sensitivity Analysis, Astrochemistry
Kinetics, Sensitivity Analysis, Astrochemistry
| selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 0 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
