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The thermal fits have kT$\\approx$4 keV, the Raymond-Smith iron abundance is $0.4^{+0.7}_{-0.3}$ Solar, the power-law fit has $\\alpha$=1.6$\\pm$0.1, and all fits have $N_H$ consistent with the Galactic column. The source is centered on M32 to an accuracy of 9$''$, and unresolved at 27$''$ FWHM ($\\sim$90 pc). M32 is x-ray variable b"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"astro-ph/9603100","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"1996-03-19T00:54:22Z","cross_cats_sorted":[],"title_canon_sha256":"aa3190c35daf7d2480a45723004057527841fbdc39667917cd74344e04c2c48d","abstract_canon_sha256":"3f70cc3034bc45a514df3e5b8ff6801415d983c5c7f8300ecc240def5494777a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:07:41.060276Z","signature_b64":"NDFq7oeIP6L9qFKvsBWiYILoOSrWGhKn4Oz+3CPK3IGy8wrQjfRVsihZ5sqBY8omMD3jNMnmP7FYD19JiW3kDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"78cd5db785b096d7a65e299639aaf59c699220c87ed9be0edb8a50e0176faa92","last_reissued_at":"2026-05-18T01:07:41.059889Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:07:41.059889Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"X-Ray Emission from M32: X-Ray Binaries or a micro-AGN?","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Astronomy, David S. 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