Convert PerkinElmer .sp spectra to CSV (Beta)

Open PerkinElmer Spectrum .sp files (Spectrum One, Two, 100, Frontier) without the Spectrum software and export CSV, Excel or JCAMP-DX.

Opens: OPUS (.0, .1 …), SPA, SPG, SPC, WDF, SP, JWS
Saves: CSV, XLSX, JCAMP-DX

Convert

Spectrum files
Choose files… or drop them here
up to 200 MB each, 200 files max
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    Bruker OPUS (.0, .1, .2 …), Thermo OMNIC (.spa, .spg), GRAMS/Galactic (.spc), Renishaw WiRE (.wdf), PerkinElmer (.sp) or JASCO (.jws). Several files or a .zip can be combined into one table.

    Options

    OPUS files usually hold several blocks (absorbance, sample and background single channel, interferograms). Groups and maps always export every spectrum.

    Pick the comma version if your Excel uses a decimal comma (most of Europe).

    More options

    Columns: one x column and one column per spectrum. Rows: one spectrum per row (best for maps and chemometrics). Auto uses rows above 100 spectra.

    Convert between wavenumber and wavelength (not possible for Raman shift or time axes).

    Convert transmittance to absorbance (A = −log₁₀T) or back. Other spectrum types are left unchanged.

    Your files are deleted after processing.

    PerkinElmer's Spectrum software stores FTIR spectra as binary .sp files. If the instrument PC is the only place with Spectrum installed, or someone sent you .sp files, this page converts them to CSV, Excel or JCAMP-DX so you can open them anywhere.

    How to convert PerkinElmer .sp to CSV

    1. Upload the .sp file. Many files, or a ZIP of them, can go in at once.
    2. Keep the number format on decimal points, or switch to decimal commas with semicolons if your Excel expects that.
    3. If you need absorbance but measured in %T (or the reverse), set Y axis under More options.
    4. Download the CSV: Wavenumber (cm-1) in the first column, then the spectrum in its stored unit, for example Absorbance.

    What is read from the file

    Besides the data, a .sp file records the measurement setup, and all of it appears in the preview and on the workbook's metadata sheet:

    • sample name and creation date;
    • instrument model and serial number, for example a Frontier FT-IR/NIR, and the firmware;
    • number of scans, detector, source and beam splitter;
    • apodization, phase correction and beam type;
    • the accessory used, such as a Universal ATR;
    • y and x units, data interval, spectral range and number of points.

    That is often enough to answer "how was this measured?" months later without going back to the instrument.

    Which files work

    The reader handles the binary format written by Spectrum for instruments such as the Spectrum One, Spectrum Two, Spectrum 100/400 and Frontier, in absorbance and transmittance. Files were checked against PerkinElmer's own CSV exports (identical x values, y within the export's rounding) and against an independent open-source reader.

    Older text-header .SP files, for example from some older fluorescence instruments, use a different layout that this converter doesn't read yet (it tells you when it sees one); export them as CSV or JCAMP-DX from the instrument software instead.

    Tips

    • Spectra that PerkinElmer software saved as .spc or in Bruker's OPUS format are read too; see SPC to CSV.
    • Upload a series of .sp files together to line them up side by side in one table, ready for an overlay or an average in Excel.
    • The JCAMP-DX download is useful for spectral library software and carries the instrument details in its header.

    More about what this tool reads and writes: Spectrum File Converter (OPUS, OMNIC, SPC, WDF, SP, JWS).