
Claude Skills by HolobiomicsLab
github.com/HolobiomicsLabUse when when you have spectroscopic measurements (1D ¹H or ¹³C NMR)
Use when when you have completed ORCA single-point energy calculations
Use when you have preprocessed mass spectrometry fragmentation data (neutral
Use when you have a tandem MS/MS spectrum of a structurally modified
Use when when you have an experimental MS/MS spectrum (query spectrum
Use when you have tandem mass spectra for compounds with known binary
Use when you have a collection of MS/MS spectra (≥2 spectra) and wish
Use when after converting a decision tree path into a MassQL query string,
Use when after feature detection and alignment have produced a feature
Use when when you have detected m/z values from LC-IM-MS/MS that match
Use when you have raw or peak-detected mass spectrometry data (mzXML,
'Use when you have two MS/MS spectra (precursor m/z and fragment ion
Use when you have extracted a chemical mixture from a real mzML acquisition
Use when after completing multidimensional smoothing and saturation repair
Use when you have loaded a table of entity–attribute pairs (e.
Use when after feature clustering has grouped co-eluting features and
Use when you are evaluating or selecting FT-ICR MS software for a specific
Use when when you have raw or processed FT-ICR MS peak-abundance .
Use when you have FT-ICR MS peak abundance data in Formularity .
'Use when after applying mass calibration functions (LedFord, linear,
Use when you have FTICR-MS direct injection (mzML) data with identified
Use when when you have a processed Bruker Solarix FT-ICR mass spectrum
Use when you have loaded an FT-ICR raw spectrum (e.g., ESI_NEG_SRFA.d
Use when you have received raw FT-ICR transient data from Bruker Solarix
Use when you have a Bruker Solarix FT-ICR transient file in .d format
Use when you need to assess MS1-level ionization efficiency, peak detection
Use when when you have Spectra objects in R and need to apply Python
Use when after running CPAT, signalP, Pfam, and fimo tools on differentially
Use when you have a set of query chemicals (chemical names or structures)
Use when you have reconstructed the structural topology of two metabolic
Use when when you have two metabolic networks (e.g., from KEGG) and need
Use when you have an untargeted metabolomics feature table (m/z and retention
Use when after assigning hierarchical KEGG identifiers to a metabolomics
Use when when you have abundance-normalized FT-ICR MS peak data with
Use when you have extracted parallel feature streams from a CNN backbone
Use when when you have experimental MS/MS spectra and want to discover
Use when you have a Galaxy Master branch installation (or specific commit
Use when after deploying Galaxy-M tool files and XML wrappers into a
Use when you have a working R package that performs established preprocessing,
Use when when integrating a multi-backend metadata enrichment package
Use when you have access to a computation-times table or performance
Use when after fitting candidate GAM splines with B-spline basis functions
Use when when processing untargeted LC-MS data with SLAW and observing
Use when when merging multiple draft metabolic models (in JSON, XML,
Use when after peak detection on a composite mass track has identified
Use when after peak detection on mass track segments using find_peaks,
Use when after you have accumulated experimental MS data from ≥2 LC gradient
Use when after collecting observed separation efficiency scores at sampled
Use when you have vendor-format GC-CI-MS raw data from a stable isotope
Use when you have a combined EI mass spectral library (MSP format) lacking