claude

gpcam

Skills that guide an AI assistant through designing autonomous experiments with gpCAM — kernels, acquisition, prior mean, noise, cost, gp2Scale, and multi-task GPs.

34 on GitHubby CAMERA — Lawrence Berkeley National LaboratoryGPL-3.0updated 9 days agoscientific-computing
/

Plugin gpcam from marketplace gpcam in lbl-camera/gpCAM. Commands read from the repo's manifest — 9 days ago.

What it installs

Skills (11)

  • acquisition-functions

    Use when choosing or writing an acquisition function for gpCAM — selecting a built-in criterion for exploration, optimization, batch, or multi-task runs, or implementing a custom callable for UCB/LCB, minimization EI, constraints, radical gradient, or threshold finding.

  • cost-functions

    Use when modeling the real expense of moving between gpCAM measurement points — motor travel time, settling, directional costs, sample damage, beam time, or zone-based penalties.

  • experiment-designer

    Use for end-to-end autonomous experiment design with gpCAM. Translates a scientist's description of their measurement into a complete, runnable gpCAM script — useful for replacing raster scans with adaptive sampling, peak-finding, or parameter optimization.

  • gp2scale-advanced

    Use for large-scale gpCAM experiments (>10k points up to millions) using sparse compactly-supported kernels and Dask distributed computing for exact GP computation at scale.

  • kernel-designer

    Use when designing or composing custom kernel (covariance) functions for gpCAM — smoothness, periodicity, symmetry, anisotropy, non-stationary amplitude/length-scale kernels (`non_stat_kernel`, Gibbs), non-Euclidean inputs, or neural-network-warped deep kernels (`Network`).

  • multi-task-advanced

    Use for multi-output, vector-valued, or function-valued gpCAM experiments using GPOptimizer with several output columns and multi_task_mode (or migrating legacy fvGPOptimizer code) — useful when a single measurement returns multiple correlated quantities (e.g., spectra, multi-channel detectors).

  • noise-functions

    Use when modeling position-dependent, heteroscedastic, or otherwise structured noise in gpCAM — e.g., detector characteristics, count-rate-dependent variance, or non-uniform measurement uncertainty.

  • prior-mean-functions

    Use when encoding known physics, theoretical models, or expected trends as prior mean functions for gpCAM — useful when there's a baseline expectation or physical model the GP should regress against rather than the default constant data-mean prior (mean(y_data)).

  • transformed-optimizers-advanced

    Use when observations are constrained — strictly positive (intensities, rates, concentrations) or bounded in [a, b] (fractions, probabilities, yields). LogGPOptimizer and LogitGPOptimizer fit a GP on transformed observations and push the posterior back through the inverse link, so predictions and cr

  • troubleshooting

    Use when a gpCAM script crashes or misbehaves — Cholesky/non-positive-definite errors, singular covariance, hyperparameter bounds mismatches, NaNs, kernel signature errors, Dask hangs, pickling failures, or an ask/tell loop that keeps picking the same point. Maps the actual error text to the cause a

  • uncertainty-calibration

    Use to validate that a gpCAM posterior's error bars are trustworthy before publishing them or letting an autonomous loop act on them — scoring rules (NLPD, CRPS, MSLL), calibration/coverage curves, PICP and interval width, and what to do when the model is over- or under-confident.

View source on GitHub gpcam.lbl.gov

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