Convert Shimadzu XRD .raw files to .xy

Open binary Shimadzu XRD .raw files without the Shimadzu software and get .xy, .xye, CSV, Excel or XRDML.

Opens: RAW (Bruker v1–v4), RAW (Rigaku), RAW (Shimadzu), BRML, XRDML, RAS, RASX, RD/SD, UDF, UXD, GSA/FXYE, XY
Saves: .xy, .xye, CSV, XLSX, XRDML, PNG

Convert

Diffraction data files
Choose files… or drop them here
.raw, .brml, .xrdml, .ras, .rasx, .asc, .dat, .rd, .sd, .udf, .uxd, .gsa, .gsas, .gss, .fxye, .xra, .xy, .xye, .txt, .csv, .zip · up to 200 MB each, 200 files max
    Add more files

    Bruker .raw (versions 1–4) or .brml, PANalytical .xrdml, Rigaku .raw/.ras/.rasx/.asc/.dat, Shimadzu .raw, Philips .rd/.sd/.udf, Bruker .uxd, GSAS .gsa/.fxye or .xy/.xye text. Several files or a .zip can be combined into one table.

    Options

    Convert 2θ with the wavelength stored in the file (Kα1).

    Counts per second divide by the counting time per step stored in the file.

    More options

    Only for text files that hold a single column of intensities: the 2θ of the first point. Leave empty otherwise.

    Only for single-column intensity files: the angle between two points, for example 0.02.

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

    Your files are deleted after processing.

    Shimadzu's XRD software saves powder diffraction measurements as binary .raw files, which other programs rarely open. This page reads them and writes the pattern as a plain .xy file (2θ and intensity), plus .xye, CSV, Excel and XRDML, without any Shimadzu software.

    How to convert Shimadzu RAW to XY

    1. Upload the .raw file; several files or a ZIP of a folder work too. Shimadzu, Bruker and Rigaku .raw files are told apart by their content, so nothing needs to be chosen.
    2. Pick the intensity: Counts as stored in the file, or Counts per second (the counts divided by the counting time per step).
    3. Download the .xy for plotting or phase identification, or the .xye for Rietveld refinement.

    What is read

    • The pattern: every point, at the angles of the scan (start, end and step as stored).
    • X-ray source: the anode and the wavelength recorded in the file (Cu Kα1, 1.5406 Å, in a copper-tube file), so d-spacing, Q and Cu-equivalent 2θ use the right value.
    • Measurement conditions: tube voltage and current, scan mode, scan speed, time per step and the divergence, scatter and receiving slits.
    • Sample and date: the sample name and the measurement date.

    The preview lists all of this, and the Excel workbook has it on a metadata sheet. The XRDML download keeps the original 2θ positions, counts and counting time for HighScore, GSAS-II or Profex.

    Counts and counts per second

    The file stores counts per step. Counts per second divides them by the time per step; Normalised scales the strongest point to 100 for overlaying patterns.

    Good to know

    • Shimadzu support is new. The angles come from the start, end and step in the file and are checked against the number of points, and the conditions are shown as stored, but no Shimadzu text export of the same measurement has been available yet to compare the counts with.
    • Files with more than one range, or laid out differently from the files we have seen, are reported as not supported instead of being guessed at. Export them as text in the Shimadzu software; a two-column table of angles and intensities converts here too.
    • A file that was cut off while copying is reported as incomplete; copy it from the instrument PC again.

    Bruker's .raw files are covered by Bruker RAW to XY, Rigaku's by Rigaku RAW to XY. To plot against d-spacing or compare with Cu reference patterns, see 2θ to d-spacing.

    More about what this tool reads and writes: XRD Pattern Converter (RAW, BRML, XRDML, RAS).