Convert anything, at global scale.
200+ formats and automation APIs that feels instant.
CONVERT
From
To
Drop files or choose a source
Upload multiple files at once, mix formats, and fine-tune every conversion with format-aware settings.
Max 2GB per file · Drag & drop ready · Mixed file types welcome
CSV at a glance
CSV
CSV predates modern API and analytics stacks, and RFC 4180 mostly documents common practice rather than imposing one rich canonical semantics layer.
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 | CSV | FITS |
|---|---|---|
| File type | Not available | Not available |
| Extensions |
|
|
| MIME type |
|
|
| Compression / quality | Not available | Not available |
| File size characteristics | Not available | Not available |
| Compatibility | Not available | Not available |
| Editability | Not available | Not available |
| Created year | Not available | Not available |
| Inventor | Not available | Not available |
| Status | Not available | Not available |
| Primary use cases |
|
|
| Common software |
|
|
| Archival suitability | Not available | Not available |
| Metadata handling | Not available | Not available |
| Delivery profile | Not available | Not available |
| Workflow fit | Not available | Not available |
| Vector scaling | Not available | Not available |
When to use each format
When to use CSV
- analysis
- reporting
- business-data exchange
- Almost every spreadsheet and data tool can read it.
When to use FITS
- capture ingest
- editing
- web or print delivery
- Strong fit for scientific metadata-rich imaging.
FAQs
Why convert CSV 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 CSV 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 CSV 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 CSV 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.