Published January 3, 2022 | Version v1

iMAC data set

Authors/Creators

  • 1. Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, E\"otv\"os Lor\'and Research Network (ELKH)

Description

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Title: Comparison between core-collapse supernova nucleosynthesis and meteoric 
       stardust grains: investigating magnesium, aluminium, and chromium 
Authors: den Hartogh J., Peto M.K., Lawson T., Sieverding A., Brinkman H., 
    Pignatari M., Lugaro M. 
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Description of contents: the data files in this data deposit are either stellar profiles or stellar yields as used in the paper to create figures. All files are machine readable .txt files. Any text editor is able to open these files.  

    A complete list of the files in this repository are provided here:

        iMAC_profiles/m15exp_LAW_D_subm.txt
        iMAC_profiles/m15exp_LAW_R_subm.txt
        iMAC_profiles/m15exp_RIT_D_subm.txt
        iMAC_profiles/m15exp_RIT_R_subm.txt
        iMAC_profiles/m15exp_SIE_D_subm.txt
        iMAC_profiles/m15exp_SIE_R_subm.txt
        iMAC_profiles/m20exp_LAW_D_subm.txt
        iMAC_profiles/m20exp_LAW_R_subm.txt
        iMAC_profiles/m20exp_RIT_D_subm.txt
        iMAC_profiles/m20exp_RIT_R_subm.txt
        iMAC_profiles/m20exp_SIE_D_subm.txt
        iMAC_profiles/m20exp_SIE_R_subm.txt
        iMAC_profiles/m25exp_LAW_D_subm.txt
        iMAC_profiles/m25exp_LAW_R_subm.txt
        iMAC_profiles/m25exp_RIT_D_subm.txt
        iMAC_profiles/m25exp_RIT_R_subm.txt
        iMAC_profiles/m25exp_SIE_D_subm.txt
        iMAC_profiles/m25exp_SIE_R_subm.txt

        iMAC_yields/m15_yields_D.txt
        iMAC_yields/m20_yields_D.txt
        iMAC_yields/m25_yields_D.txt

    For the profiles the *R_subm.txt files have the following columns:
    mass,he4,c12,o16,ne20,si28,ni56,fe56,al26,al27,mg24,mg25,mg26,cr50,cr52,cr53,cr54
    All isotopes are radioactive or non-decayed. 

    For the profiles the *D_subm.txt files have the following columns:
    mass,al27,mg24,mg25,mg26,cr50,cr52,cr53,cr54
    All isotopes include all radioactive contributions and are thus fully decayed. 

    The yield files have the following columns:
    ref Mg24, Mg25, Mg26, Al26, Al27, Cr50, Cr52, Cr53, Cr54
    All yields are fully decayed. The refs are equal to the labels in Figure 2. 
    
    
    
System requirements: -

Additional comments: the Cr53 data for the middle row of Figure 3 is not included in these files.

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Files

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