AxisBenchTechniquesRaman spectrum analysis
RamanRaman spectroscopy
Raman spectrum analysis with open library matching.
Remove the background, measure bands and match against 36,062 Raman spectra from Open Specy, RRUFF and the Raman Open Database, with every setting saved beside the result.
- Band position
- Raman shift, cm⁻¹
- Band intensity
- on the recorded signal basis
- Excitation wavelength
- nm, when converting
- Region area
- per declared region
- Library candidate
- name, source entry
- Similarity score
- cosine or Pearson
Each value is saved with the processing settings and library version that produced it.
- Reference spectra
- 36,062 open Raman spectra
- Sources
- Open Specy, RRUFF, ROD
- Files
- CSV, TXT, TSV, Excel, JCAMP-DX
- Price
- Free plan, no credit card
01 · What it computes
From raw spectrum to ranked candidates.
Every transform is a named, parameterised step. Settings save as presets and run across a batch of spectra.
Raman shift
Convert between wavelength and Raman shift with your excitation wavelength, or keep the axis as imported.
Background and smoothing
AsLS, linear or rubberband baseline for the fluorescence background, with an optional baseline region. Savitzky–Golay, moving-average or Gaussian smoothing.
Normalisation
Vector, max or SNV normalisation, recorded with the result so spectra compare on the same basis.
Band table
Bands are detected by prominence, distance and a maximum count. Each row records the axis unit and the signal it was found on.
Band areas
Integrate the regions you declare, one line each with low and high limits and a label, and see which bands fall inside each region.
Library matching
Cosine or Pearson similarity across the full library, with a candidate count and minimum score. Templates for general Raman and polymorph screening.
02 · Reference library
The whole library, searched on every match.
Every reference is hosted on our servers and compared on every run, not a demo subset. The library is identical on Free, Pro, Lab and Enterprise.
- Raman
- 36,062
- Raman spectra
- Open Specy, RRUFF, ROD
How a spectrum match is made
- Your processed spectrum goes in.
Smoothing, baseline and normalisation come from the settings you chose, and they are saved with the match.
- The whole library is compared.
Your spectrum is compared curve against curve with all 36,062 Raman references, then peak overlap is checked for the shortlist.
- Candidates come with their scores.
Each candidate shows its similarity score and its spectrum beside yours. Candidates are evidence for your interpretation, not a verdict.
- Sources stay attached.
Every record keeps its source and attribution in your export, and relevant papers retrieved from OpenAlex sit next to the result.
Where the reference spectra come from
Record counts are from the catalog published on 28 September 2026. Each source keeps its own license, and attribution travels with every matched record and exported report.
03 · Files and limits
What goes in, and what it does not claim.
Supported files
- CSV, TXT, TSV and ExcelColumns are mapped to the spectral axis and signal at import, and quality warnings show before anything is computed.
- JCAMP-DXSingle-spectrum
.jdx,.dxand.jcampfiles with one##XYDATAblock. Multi-block, NTUPLES and peak-table JCAMP files are not supported.
Limits
- Candidates, not verdictsA high similarity score is evidence for your interpretation, not an identification.
- Shift conversion needs the laserConverting between wavelength and Raman shift requires the excitation wavelength.
- JCAMP-DX scopeOne spectrum per file, as uncompressed
##XYDATA. - ExportsTables as CSV or XLSX, figures as PNG and reports as DOCX or PDF. The whole project downloads as a file you can reopen later.
Other techniques in the same project
DSC, TGA, DTA, FTIR, Raman and XRD data live side by side in one AxisBench project. Full multi-technique reports come with Pro.
Match your next Raman spectrum.
The Free plan includes every technique and the full reference libraries, with 10 analyses a month (up to 3 a day). Pro removes the limits.