k-dense-ai/spectroscopist
v1.0.0MIT
Reasons from selection rules, line shapes as convolutions of intrinsic and instrument broadening, and Beer-Lambert linearity through UV-Vis, fluorescence, IR/Raman, NMR, CD, EPR, and XAS/XPS with calibration standards (polystyrene 1601 cm⁻¹, TMS/DSS, C 1s 284.8 eV) while treating inner filter effects, baseline artifacts inventing peaks, Fermi resonances, and X-ray beam damage as first-class failure modes.
What this package declares
The file a client reads when it loads this plugin, exactly as this revision carries it.
plugin.json
{
"$schema": "https://agent-plugins.org/schemas/1.0.0/plugin.schema.json",
"name": "spectroscopist",
"version": "1.0.0",
"description": "Reasons from selection rules, line shapes as convolutions of intrinsic and instrument broadening, and Beer-Lambert linearity through UV-Vis, fluorescence, IR/Raman, NMR, CD, EPR, and XAS/XPS with calibration standards (polystyrene 1601 cm⁻¹, TMS/DSS, C 1s 284.8 eV) while treating inner filter effects, baseline artifacts inventing peaks, Fermi resonances, and X-ray beam damage as first-class failure modes.",
"author": {
"name": "K-Dense",
"url": "https://www.k-dense.ai"
},
"homepage": "https://github.com/K-Dense-AI/scientific-agents",
"repository": "https://github.com/K-Dense-AI/scientific-agents",
"license": "MIT",
"keywords": [
"science",
"agents-md",
"expert-profile",
"spectroscopist"
]
}