FTS to IPL Converter

Turn FTS images into IPL format with ease online

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Privacy Protected

Uploaded FTS data is erased immediately after conversion. IPL results are purged within 24 hours — your content stays confidential.

Browser-Based Tool

No downloads or installations needed — open the converter in your browser and convert FTS to IPL instantly from anywhere.

Any Device Works

Run the FTS to IPL converter from any device — desktop, laptop, tablet, or phone. All you need is a web browser to get started.

How to convert FTS to IPL

1

Select files from Computer, Google Drive, Dropbox, URL or by dragging it on the page.

2

Choose ipl or any other format you need as a result (more than 200 formats supported)

3

Let the file convert and you can download your ipl file right afterwards

About formats

FTS is a file extension for the Flexible Image Transport System (FITS), the standard data format used in astronomy since 1981 when it was defined by Don Wells, Eric Greisen, and R.H. Harten at the National Radio Astronomy Observatory, and subsequently endorsed by the International Astronomical Union in 1982. FITS was designed from the outset as a self-describing archival format: each file begins with one or more 2880-byte header blocks containing ASCII keyword-value pairs that describe the data's dimensions, coordinate system, observation parameters, and provenance, followed by data blocks in a variety of numeric types — 8/16/32/64-bit integers and 32/64-bit IEEE floating-point values. FITS supports multi-dimensional arrays (images, data cubes, hypercubes), binary tables for catalog data, and ASCII tables, with multiple Header/Data Units (HDUs) that can coexist in a single file. The format handles specialized astronomical data: spectral cubes, radio interferometry visibilities, multi-extension mosaic images from CCD arrays, and time-series photometry. One advantage is scientific rigor: FITS mandates that all metadata needed to interpret the data physically — coordinate transformations (WCS), photometric calibration, telescope and instrument parameters — travels with the file, eliminating the metadata-loss problem that plagues general-purpose image formats in scientific contexts. The format's longevity and institutional backing is another strength — virtually every observatory, space telescope (Hubble, James Webb, Chandra), and astronomical software package (DS9, IRAF, Astropy) uses FITS as its primary data format.
Developer: NASA / IAU
Initial release: 1981
IPL (IPLab) is a scientific image format developed by Scanalytics (later acquired by BD Biosciences) for their IPLab scientific image analysis software, first released around 1988. The format was designed to store microscopy and scientific imaging data with the precision and metadata needed for quantitative analysis in biological and biomedical research. IPL files support multiple data types including 8-bit and 16-bit unsigned integers, 16-bit signed integers, and 32-bit floating-point pixel values, accommodating the wide dynamic ranges produced by fluorescence microscopes, CCD cameras, and other scientific imaging instruments. The format handles multi-dimensional datasets including Z-stacks (focal series through a specimen), time-lapse sequences, and multi-channel fluorescence acquisitions where each channel captures emission from a different fluorescent probe. IPL files include a header with image dimensions, data type, number of planes, spatial calibration (pixels-to-micrometers conversion), and acquisition metadata from the microscope system. One advantage is quantitative integrity: unlike photographic formats that apply gamma correction, compression, or color space transforms, IPL preserves the raw linear intensity values from the detector, ensuring that measurements of fluorescence intensity, optical density, or particle counts performed on the image data correspond directly to the physical quantities being measured. The format's role in the microscopy community is another practical consideration: IPLab was widely used in cell biology, neuroscience, and pathology labs throughout the 1990s and 2000s, and archived IPL datasets from published research remain scientifically valuable. IPL files can be read by ImageJ/FIJI, Bio-Formats, and ImageMagick.
Developer: Scanalytics
Initial release: 1988

Frequently Asked Questions

Why convert FTS to IPL?

Scientific microscopy storage — converting FTS to IPL gives your astronomical images broader reach and easier sharing across standard platforms.

What programs open IPL?

Open IPL with standard tools like Windows Photos, Preview on macOS, GIMP, Photoshop, or any web browser — no special software needed.

Does this work on mobile devices?

Yes — the converter runs in any web browser, so it works on phones, tablets, laptops, and desktops regardless of operating system.

Is the conversion instant?

Near-instant for typical images — the cloud-based processing handles FTS to IPL conversion quickly. Very large data may take a moment.

Is batch FTS to IPL conversion supported?

Absolutely — queue multiple FTS images and convert them all to IPL in a single session. No need to process one at a time.

What is the FTS format?

FTS is used in astronomy and scientific research. It stores telescope captures and observatory data — converting to IPL makes this data universally accessible.