Dataset
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update: {"hold_state"=>["none", "files temporarily suppressed"]}
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2025-01-31T21:06:29Z
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Dataset
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update: {"description"=>["***<b>ATTENTION:</b> Per the authors' request, the data files for this dataset are now suppressed. Please visit this new dataset for the complete and updated data files: Huang, Yijing; Fahad , Mahmood (2025): Data for Observation of a Magneto-chiral Instability in Photoexcited Tellurium. University of Illinois Urbana-Champaign.<a href=\"https://doi.org/10.13012/B2IDB-1409842_V1\">https://doi.org/10.13012/B2IDB-1409842_V1</a>***\r\n\r\nThe data and code provided in this dataset can be used to generate key plots in the manuscript. It is divided into four subfolders (B parallel/perpendicular to the tellurium c axis and field/ temperature dependence), each containing the raw data (saved in .mat format), the oscillator parameters obtained through linear prediction (saved in .mat format), and the plot-generating code (.m files). The code was written using MATLAB R2024a. To run the code, go to each folder, and run the .m file in that folder, which generates two plots. ", "Per the authors' request, the data files for this dataset are now suppressed. Please visit this new dataset for the complete and updated data files: Huang, Yijing; Fahad , Mahmood (2025): Data for Observation of a Magneto-chiral Instability in Photoexcited Tellurium. University of Illinois Urbana-Champaign.<a href=\"https://doi.org/10.13012/B2IDB-1409842_V1\">https://doi.org/10.13012/B2IDB-1409842_V1</a>\r\n\r\n====================\r\n\r\nThe data and code provided in this dataset can be used to generate key plots in the manuscript. It is divided into four subfolders (B parallel/perpendicular to the tellurium c axis and field/ temperature dependence), each containing the raw data (saved in .mat format), the oscillator parameters obtained through linear prediction (saved in .mat format), and the plot-generating code (.m files). The code was written using MATLAB R2024a. To run the code, go to each folder, and run the .m file in that folder, which generates two plots. "], "subject"=>["", "Physical Sciences"]}
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2025-01-31T21:06:16Z
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RelatedMaterial
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update: {"note"=>[nil, ""]}
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2025-01-31T21:05:39Z
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Dataset
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update: {"publisher"=>["University of Illinois at Urbana-Champaign", "University of Illinois Urbana-Champaign"], "description"=>["The data and code provided in this dataset can be used to generate key plots in the manuscript. It is divided into four subfolders (B parallel/perpendicular to the tellurium c axis and field/ temperature dependence), each containing the raw data (saved in .mat format), the oscillator parameters obtained through linear prediction (saved in .mat format), and the plot-generating code (.m files). The code was written using MATLAB R2024a. To run the code, go to each folder, and run the .m file in that folder, which generates two plots. ", "***<b>ATTENTION:</b> Per the authors' request, the data files for this dataset are now suppressed. Please visit this new dataset for the complete and updated data files: Huang, Yijing; Fahad , Mahmood (2025): Data for Observation of a Magneto-chiral Instability in Photoexcited Tellurium. University of Illinois Urbana-Champaign.<a href=\"https://doi.org/10.13012/B2IDB-1409842_V1\">https://doi.org/10.13012/B2IDB-1409842_V1</a>***\r\n\r\nThe data and code provided in this dataset can be used to generate key plots in the manuscript. It is divided into four subfolders (B parallel/perpendicular to the tellurium c axis and field/ temperature dependence), each containing the raw data (saved in .mat format), the oscillator parameters obtained through linear prediction (saved in .mat format), and the plot-generating code (.m files). The code was written using MATLAB R2024a. To run the code, go to each folder, and run the .m file in that folder, which generates two plots. "], "version_comment"=>[nil, ""], "subject"=>[nil, ""]}
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2025-01-31T21:05:39Z
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Creator
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update: {"identifier"=>["0000-0002-5453-7722", ""]}
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2024-09-29T21:09:11Z
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RelatedMaterial
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create: {"material_type"=>"Dataset", "availability"=>nil, "link"=>"https://doi.org/10.13012/B2IDB-9143327_V2", "uri"=>"10.13012/B2IDB-9143327_V2", "uri_type"=>"DOI", "citation"=>"Huang, Yijing (2024): tellurium_magneto_chiral_instability. University of Illinois at Urbana-Champaign. https://doi.org/10.13012/B2IDB-9143327_V2", "dataset_id"=>2797, "selected_type"=>"Dataset", "datacite_list"=>"IsPreviousVersionOf", "note"=>nil, "feature"=>nil}
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2024-09-28T05:03:02Z
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RelatedMaterial
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destroy: {"material_type"=>"Dataset", "availability"=>nil, "link"=>"https://doi.org/10.13012/B2IDB-9143327_V2", "uri"=>"10.13012/B2IDB-9143327_V2", "uri_type"=>"DOI", "citation"=>"Huang, Yijing (2024): tellurium_magneto_chiral_instability. University of Illinois at Urbana-Champaign. https://doi.org/10.13012/B2IDB-9143327_V2", "dataset_id"=>2797, "selected_type"=>"Dataset", "datacite_list"=>"IsPreviousVersionOf", "note"=>nil, "feature"=>nil}
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2024-09-28T05:02:14Z
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RelatedMaterial
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create: {"material_type"=>"Dataset", "availability"=>nil, "link"=>"https://doi.org/10.13012/B2IDB-9143327_V2", "uri"=>"10.13012/B2IDB-9143327_V2", "uri_type"=>"DOI", "citation"=>"Huang, Yijing (2024): tellurium_magneto_chiral_instability. University of Illinois at Urbana-Champaign. https://doi.org/10.13012/B2IDB-9143327_V2", "dataset_id"=>2797, "selected_type"=>"Dataset", "datacite_list"=>"IsPreviousVersionOf", "note"=>nil, "feature"=>nil}
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2024-09-28T05:01:22Z
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Dataset
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update: {"description"=>["The data and code provided in this dataset can be used to generate key plots in the manuscript. It is divided into four subfolders (B parallel/perpendicular to the tellurium c axis and field/ temperature dependence), each containing the raw data (save in .mat format), the oscillator parameters obtained through linear prediction (save in .mat format), and the plot-generating code (.m files). The code was written using MATLAB R2024a. ", "The data and code provided in this dataset can be used to generate key plots in the manuscript. It is divided into four subfolders (B parallel/perpendicular to the tellurium c axis and field/ temperature dependence), each containing the raw data (saved in .mat format), the oscillator parameters obtained through linear prediction (saved in .mat format), and the plot-generating code (.m files). The code was written using MATLAB R2024a. To run the code, go to each folder, and run the .m file in that folder, which generates two plots. "]}
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2024-09-28T05:00:46Z
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