AxisBenchTechniquesFTIR spectrum analysis
FTIRInfrared spectroscopy
FTIR spectrum analysis with open library matching.
Correct the baseline, build the band table and match your spectrum against 20,762 infrared spectra from Open Specy and RRUFF. Every step is a named setting saved with the result.
- Band position
- cm⁻¹
- Band intensity
- on the recorded signal basis
- Signal basis
- %T, absorbance, normalised
- 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
- 20,762 open infrared spectra
- Sources
- Open Specy, RRUFF
- 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.
Axis and absorbance
Wavenumber in cm⁻¹, or wavelength in µm or nm, converted on request. Transmittance converts to absorbance with A = −log₁₀ T.
Smoothing and baseline
Savitzky–Golay, moving-average or Gaussian smoothing. AsLS, linear or rubberband baseline, with an optional baseline region.
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 FTIR and functional-group 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.
- FTIR
- 20,762
- infrared spectra
- Open Specy, RRUFF
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 20,762 FTIR 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.
- No invented assignmentsThe band table records what was detected. It does not label bands with functional groups on its own.
- 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 FTIR 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.