These folders contain the original data used to develop the ACME software [1]. The Golden and Silver dataset come from simulations. They underrepresent the complexity in the CE-MS observations but provide additional data with known peak locations and peak properties. For more information see [1] The Dev-, Train-, and Test-set contain CE-MS [2] observations of Mix25 (a standard set of 25 organic compounds relevant to astrobiology) and labels for peak locations from subject matter experts. The ACME software is available at: https://github.com/JPLMLIA/OWLS-Autonomy When using the data please cite this dataset [3] and the two papers below. For further questions please reach out to: Steffen Mauceri, Steffen.Mauceri@jpl.nasa.gov References: [1] Mauceri, S., Lee, J., Wronkiewicz, M., et.al. (2022). Autonomous CE Mass-Spectra Examination (ACME) for the Ocean Worlds Life Surveyor (OWLS). (submitted) Earth and Space Science [2] Mora et al., F.(2021). Detection of biosignatures by capillary electrophoresis and mass spectrometry in the presence of salts relevant to missions to ocean worlds (submitted). Astrobiology. [3] 10.5281/zenodo.5849873 © 2022. California Institute of Technology. Government sponsorship acknowledged

{"references": ["Mauceri, S., Lee, J., Wronkiewicz, M., et.al. (2022). Autonomous CE Mass-Spectra Examination (ACME) for the Ocean Worlds Life Surveyor (OWLS) (submitted). Earth and Space Science", "Mora et al., F.(2021). Detection of biosignatures by capillary electrophoresis and mass spectrometry in the presence of salts relevant to missions to ocean worlds (submitted). Astrobiology."]}