fits op• Data kinds: any → any
• Call: import fullseye as fs; fs.ledger.astro_fits_write(image, *, header) (to call the implementation directly, import fileio; fileio.astro_fits_write(image, *, header); from the registry, opsfileio.get("astro_fits_write"))
• GPU: none (CPU reference implementation only)
Write a 2-D/3-D astronomical image and basic WCS as primary-HDU FITS bytes.
> The detailed description below is the original text — the summary and the headings are translated.
header は FITS の基本 WCS キー(CTYPE*, CRPIX*, CRVAL*, CDELT*, PC*_*, CD*_*, CUNIT* など)だけを持つ辞書。構造キーは配列から作り、int8/uint16/uint32/uint64 は FITS 4.0 の標準の BZERO 規約で保存する。呼び出し例:
payload = astro_fits_write(image, header={"CTYPE1": "RA---TAN"})。
• Sample-data catalog (download URLs / licences) — 2-D uses skimage.data (BSD/public domain) plus synthetic images; 3-D lists download URLs for real data sources (Stanford, PDS, …).
• Operator provenance and references — the sources of the research/methods this op family came from.
• The canonical algorithm (author, year) and its uses are named in the family usage guide above.
• fileio_scientific_roundtrip — py -3.11 examples/fileio_scientific_roundtrip.py
any as input)table_write_csv · table_read_csv · mesh_write_ply · mesh_read_ply · mesh_write_stl · mesh_read_stl · mesh_write_obj · mesh_read_obj
fits)*Provenance: fileio.py — FILEIO operator registry. This per-op note is generated by tools/opdocs.py md (do not hand-edit).*
© 2026 Kazufumi Furuse — Fullseye operator documentation. Licensed under Apache-2.0.