PAM to FTS Converter

Change PAM to FTS format — no installation required

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Simple Workflow

Upload PAM, choose FTS, download your file — three clear steps with no complicated settings or confusing interfaces.

Instant Results

Your PAM to FTS conversion is done within moments. The pipeline is optimized for speed and minimal wait times.

Secure Conversion

File privacy is guaranteed — PAM uploads are removed after conversion, and FTS results are deleted within 24 hours.

How to convert PAM to FTS

1

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

2

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

3

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

About formats

PAM (Portable Arbitrary Map) is a raster image format added to the Netpbm family around the year 2000 by Bryan Henderson, the maintainer of Netpbm, as a generalization that unifies and extends the original PBM, PGM, and PPM formats. Where the classic Netpbm formats each handle a specific image type (PBM for bilevel, PGM for grayscale, PPM for color), PAM provides a single format that can represent any combination of channels, bit depths, and image types through a flexible ASCII header. The PAM header uses keyword-value pairs: WIDTH, HEIGHT, DEPTH (number of channels), MAXVAL (maximum sample value, up to 65535), and TUPLTYPE (a string identifying the image type — BLACKANDWHITE, GRAYSCALE, RGB, GRAYSCALE_ALPHA, RGB_ALPHA, or custom types). After the header, pixel data is stored in binary, with each sample occupying one or two bytes depending on MAXVAL. PAM's key innovation over its predecessors is native alpha channel support: GRAYSCALE_ALPHA (2-channel) and RGB_ALPHA (4-channel) tupletypes provide transparency without requiring a separate mask file, something the original PBM/PGM/PPM formats could not express. One advantage is format unification: a single PAM-reading implementation handles monochrome, grayscale, color, and alpha-augmented images, eliminating the need for separate parsers for each Netpbm variant. The extensible TUPLTYPE mechanism provides another practical strength — custom channel configurations (multispectral, depth + color, or any application-specific arrangement) can be represented and labeled without modifying the format specification. PAM is supported by Netpbm tools, ImageMagick, GIMP, and programming libraries that process the Netpbm family.
Initial release: 2000
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

Frequently Asked Questions

Why convert PAM to FTS?

FTS offers scientific and astronomical data — giving your image broader compatibility and a format suited for modern workflows.

What programs open FTS files?

For FTS files, try SAOImage DS9, FITS Liberator, AstroImageJ. Cross-platform support means you can view them on any operating system.

Will I lose image quality converting PAM to FTS?

The conversion preserves the original quality of your PAM file. Any inherent quality limits in PAM carry over, but nothing additional is lost.

Can I convert multiple PAM files to FTS at once?

Absolutely — queue up multiple PAM files and the converter handles each one, producing FTS outputs for all of them.

Is the PAM to FTS conversion instant?

Conversion typically finishes in seconds. PAM files are lightweight, so the transformation to FTS is quick.

Do I need to create an account to convert?

No account is needed for standard conversions. Just upload your PAM file, pick FTS, and download the result.