FTS to MAP Converter

Export FTS to MAP — simple online conversion

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Bulk Conversion

Handle many FTS to MAP conversions at once. Upload a batch, start the process, and download all results — no repeated uploading.

Quick Results

FTS to MAP conversion is fast — upload, process, and download typically wraps up in under a minute for standard images.

Cross-Platform

The converter works on Windows, macOS, Linux, iOS, and Android. Convert FTS to MAP from whichever device you have at hand.

How to convert FTS to MAP

1

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

2

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

3

Let the file convert and you can download your map 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
MAP is an internal raster image format used by ImageMagick, the open-source image processing suite first released by John Cristy at DuPont on August 1, 1990. MAP files store indexed-color (color-mapped) images in ImageMagick's native representation: a color palette (the map) followed by pixel data where each pixel is an index into that palette rather than a direct RGB value. The format provides a compact representation for images with a limited number of distinct colors — each pixel requires only enough bits to index the palette (typically 8 bits for up to 256 colors), compared to the 24 or 32 bits per pixel required by full-color formats. MAP serves primarily as an intermediate format within ImageMagick's processing pipeline, useful when performing operations that benefit from or require palettized representation: color quantization (reducing an image to a specific number of colors), palette manipulation, GIF preparation, and indexed-color analysis. The format is invoked through ImageMagick's standard I/O syntax and can be piped between processing stages without disk overhead. One advantage is direct access to ImageMagick's color quantization and palette management capabilities: MAP format output makes the palette structure explicit and manipulable, enabling workflows where specific palette operations (reordering, remapping, merging) need to be performed between processing steps. The format's integration into the ImageMagick processing ecosystem is another practical strength — any of ImageMagick's extensive image manipulation operations can consume or produce MAP format data, making it a natural intermediate for color-reduction pipelines that ultimately target GIF, PNG with palette, or other indexed-color formats.
Initial release: 1990

Frequently Asked Questions

Why convert FTS to MAP?

Most people lack software for FTS. Converting to MAP ensures your astronomical images are viewable everywhere — from phones to desktops.

What programs open MAP?

Any modern image viewer opens MAP — Windows Photos, macOS Preview, GIMP, Photoshop, and web browsers all support it.

How long does the conversion take?

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

Is the output quality comparable?

The conversion extracts the best possible quality from your FTS data. The MAP output reflects the format's capabilities accurately.

Can I convert multiple FTS images at once?

Yes — upload several FTS images in one session and convert them all to MAP simultaneously. Batch processing saves significant time.

Do I need FTS software installed?

No — the converter processes FTS entirely in the cloud. You do not need any astronomy and scientific research software on your device to convert.