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Xfig at a glance
Xfig
Xfig began in 1985 and accumulated decades of maintenance and export tooling, which made the .fig format a durable bridge between interactive diagram editing on Unix systems and downstream conversion to PostScript, PDF, and other outputs.
FITS at a glance
FITS
FITS became a durable scientific standard because observatories, spacecraft, and analysis tools needed a stable interchange format that outlived individual instruments and software stacks.
Format comparison
| Feature | Xfig | FITS |
|---|---|---|
| File type | Vector | Image |
| Extensions |
|
|
| MIME type |
|
|
| Compression / quality | scalable | depends |
| File size characteristics | small | medium |
| Compatibility | moderate | broad |
| Editability | high | moderate |
| Created year | 1985 | 1981 |
| Inventor | Supoj Sutanthavibul | NASA / astronomical data community |
| Status | legacy | active |
| Transparency | Not supported | Not supported |
| Animation | Not supported | Not supported |
| Primary use cases |
|
|
| Common software |
|
|
| Archival suitability | good | moderate |
| Metadata handling | moderate | moderate |
| Delivery profile | strong | strong |
| Workflow fit | design | delivery |
| Layer support | Not supported | Not supported |
| Vector scaling | Supported | Not supported |
When to use each format
When to use Xfig
- illustration
- diagramming
- brand asset delivery
- Preserves object-level editability for technical diagrams.
When to use FITS
- capture ingest
- editing
- web or print delivery
- Strong fit for scientific metadata-rich imaging.
FAQs
Why convert Xfig to FITS?
Choose FITS as target when preserving scientific image data, observation metadata, or instrument-derived captures for astronomy and research workflows.
What changes when converting Xfig to FITS?
Convert to FITS when preserving scientific image data, observation metadata, or instrument-derived captures for astronomy and research workflows. It is the right target when measurement context matters as much as the picture itself.
What should I review after converting Xfig to FITS?
After conversion, review these destination checks: Open converted output in astronomy tools and verify behavior on real samples; Compare output against the expected depends quality profile; Not designed as a mainstream consumer image format.
How can I keep quality stable in Xfig to FITS conversion?
Run representative samples, keep settings deterministic, and monitor these risks: Validation needs domain-aware tools, not just generic viewers; Not designed as a mainstream consumer image format; Validate destination compatibility before large-batch conversion.