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Part 1: Document Description
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Citation |
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Title: |
Replication Data for: Mathematica code for Olivine Family analysed using Asymmetric Gaussian Method |
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Identification Number: |
doi:10.7910/DVN/TCCT7H |
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Distributor: |
Harvard Dataverse |
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Date of Distribution: |
2022-01-18 |
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Version: |
2 |
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Bibliographic Citation: |
Brown, Adrian, 2022, "Replication Data for: Mathematica code for Olivine Family analysed using Asymmetric Gaussian Method", https://doi.org/10.7910/DVN/TCCT7H, Harvard Dataverse, V2 |
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Citation |
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Title: |
Replication Data for: Mathematica code for Olivine Family analysed using Asymmetric Gaussian Method |
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Identification Number: |
doi:10.7910/DVN/TCCT7H |
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Authoring Entity: |
Brown, Adrian (Plancius Research) |
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Producer: |
Adrian Brown |
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Distributor: |
Harvard Dataverse |
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Access Authority: |
Brown, Adrian |
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Depositor: |
Brown, Adrian |
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Date of Deposit: |
2022-01-18 |
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Holdings Information: |
https://doi.org/10.7910/DVN/TCCT7H |
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Study Scope |
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Keywords: |
Astronomy and Astrophysics, Chemistry, Computer and Information Science, Earth and Environmental Sciences, Mathematical Sciences, Physics |
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Abstract: |
Replication Data for: Mathematica code for "Olivine Family for Asymmetric Gaussian Method". This code was used to create the plots in the paper submitted in 2022 and resubmitted in March 2024 as "Resolving Asymmetric Spectral Bands" to GRL then to ESS in January 2025 |
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Notes: |
This archive contains two Mathematica notebooks, a large one that contain the Asymmetric Gaussian code (first section of paper), and a smaller one that contains the fitting of the olivine bands (final section of paper). They were created in 2021-2024 using Wolfram Mathematica 12-14 |
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Methodology and Processing |
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Sources Statement |
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Data Access |
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Other Study Description Materials |
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Related Publications |
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Citation |
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Title: |
Paper was just been submitted to Nature Communications, then Scientific Reports. It was refined a large amount and resubmitted to Nature Communications in March 2024. |
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Bibliographic Citation: |
Paper was just been submitted to Nature Communications, then Scientific Reports. It was refined a large amount and resubmitted to Nature Communications in March 2024. |
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Label: |
asymm-gauss-paper-1.nb |
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Text: |
Updated file submitted Jan 2025 for ESS submission |
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Notes: |
application/mathematica |
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Label: |
asymm-gauss-paper.nb |
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Notes: |
application/mathematica |
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Label: |
calcs-1.ods |
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Text: |
Update for calcs file Jan 2025 for ESS submission |
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Notes: |
application/vnd.oasis.opendocument.spreadsheet |
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Label: |
calcs.ods |
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Text: |
8b |
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Notes: |
application/vnd.oasis.opendocument.spreadsheet |
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Label: |
Figure 7-big.pdf |
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Notes: |
application/pdf |
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Label: |
Figure 7-big.svg |
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Notes: |
image/svg+xml |
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Label: |
Figure 7.pdf |
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Notes: |
application/pdf |
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Label: |
Figure 7.svg |
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Notes: |
image/svg+xml |
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Label: |
olivineFourBandParameters-1.nb |
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Text: |
Update in 2024 after significant enhancements to analysis, including production of applets for exploring Fo# vs. spectra for three and four band complexes in energy and wavelength plots simultaneously. |
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Notes: |
application/mathematica |
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Label: |
olivineFourBandParameters.nb |
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Text: |
2nd update Jan 2025 on submission of ESS document |
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Notes: |
application/mathematica |