FTS to RGBA Converter

Render FTS content as RGBA — instant conversion

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Visual Fidelity

Your FTS imagery is carefully converted to RGBA with maximum quality retention. No unnecessary degradation during the transformation process.

Server-Side Engine

Conversion runs entirely in the cloud. Even complex FTS data is processed on powerful servers, keeping your device responsive and fast.

Effortless Conversion

Upload your FTS, pick RGBA, and click Convert — the entire process takes just a few clicks with no technical expertise required.

How to convert FTS to RGBA

1

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

2

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

3

Let the file convert and you can download your rgba 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
RGBA is a raw (headerless) image format that extends the RGB color model with a fourth channel for alpha transparency. Each pixel is stored as four consecutive sample values — red, green, blue, and alpha — written sequentially in scanline order with no container structure, headers, or compression. The alpha channel specifies opacity for each pixel independently: a maximum value means fully opaque, zero means fully transparent, and intermediate values produce semi-transparency. Like its three-channel counterpart, RGBA files require the image dimensions and bit depth to be specified externally since the raw data stream contains no metadata. The format supports 8-bit (four bytes per pixel, 32-bit total), 16-bit, and floating-point channel depths. In compositing workflows, the alpha channel enables layering operations where foreground elements are blended over backgrounds according to their per-pixel opacity — the mathematical foundation for all modern image compositing, described by Porter and Duff in their seminal 1984 paper on digital compositing. One advantage is direct framebuffer compatibility: modern GPU hardware natively processes 32-bit RGBA pixels, so raw RGBA data can be uploaded to texture memory or written from render targets without any format conversion, critical for real-time graphics applications and game engines. The format's simplicity in representing transparent images provides another practical benefit — scientific visualization, medical imaging, and overlay rendering can produce raw RGBA output that any downstream tool can consume without needing a common container format. RGBA files are handled by ImageMagick, FFmpeg, and various graphics and compositing tools.
Initial release: 1990

Frequently Asked Questions

Why convert FTS to RGBA?

SGI format with full alpha channel support — converting FTS to RGBA gives your astronomical images broader reach and easier sharing across standard platforms.

What programs open RGBA?

Most image viewers and editors handle RGBA — Photoshop, GIMP, IrfanView, and built-in viewers on Windows, macOS, and Linux.

How long does the conversion take?

Most FTS to RGBA conversions finish within seconds. Larger or more complex images may take slightly longer depending on the data size.

Is batch FTS to RGBA conversion supported?

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

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.

Does the conversion preserve quality?

The converter retains maximum fidelity during the FTS to RGBA transformation. Any differences stem from the output format's own characteristics.