Download and install the latest version of Filestar.
Right click on one or more Cal file(s) on your desktop and select Convert with Filestar.
Type convert to fits in the search box.
Press Convert.
Or let an AI agent do it: filestarcli -i photo.cal -c "convert to fits" (how).
Documents - File Explorer─☐✕
This PC › Documents
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.calContract.cal
.xlsxBudget.xlsx
.pdfReport.pdf
.pngLogo.png
Filestar*Help✕
Drop files here to get started
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Let your AI agent convert CAL to FITS
Claude Code, Codex, Cursor and other agents can do this on your computer with Filestar. Your files stay on your machine.
Install Filestar and add it to your agents:
npm install -g filestar
filestarcli agent install
Then ask your agent:
“Convert the CAL files in my Downloads folder to FITS”
Or run it yourself:
filestarcli -i photo.cal -c "convert to fits"
Runs on your computer, so your files stay on it. Works on Windows, macOS and Linux. 50 free conversions with the npm install, no account needed.
Can my AI agent convert CAL to FITS?
Yes. Install the Filestar CLI with npm install -g filestar and your agent can run filestarcli -i photo.cal -c "convert to fits" on your computer, so your files stay on it.
The CALS raster file format, commonly known by the extension ".cal" or ".cals," is a bitmap file format designed primarily for the storage and interchange of digital images, especially in the field of computer-aided design (CAD) and engineering. Developed by the United States Department of Defense, it was intended to standardize the exchange of graphics data for electronic publishing of technical manuals. This format supports monochrome (1-bit) images and is distinguished by its efficient compression methods for reducing file sizes, facilitating easier storage and transmission. Despite its specific initial use case, the CALS raster format has found application in various industries for the archiving and sharing of high-resolution, scanned documents.
The Flexible Image Transport System (FITS) file format is a digital file format used primarily in astronomy for storing, transmitting, and analyzing scientific images and data. Developed in the late 1970s, FITS was designed to provide a standard for the interchange of astronomical data, facilitating the sharing and analysis of data among astronomers and researchers worldwide.
