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The Galactic background emission was modeled by a 2-temperature thermal component, which is typical for Galactic diffuse emission.\n  We detected significant diffuse excess emission ab"},"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":"1002.0711","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2010-02-03T11:41:04Z","cross_cats_sorted":[],"title_canon_sha256":"a95a22abd32ac3553a5a884a84b3ee8cfdaa8d96d44d7975c86d4b4854021850","abstract_canon_sha256":"5a9dcbbc3d41f57f446c4cb89c23853ff765d83c7e72f984f91efaa8af9852c7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:09:20.409862Z","signature_b64":"Gmyg455MWWF2PDSGLillI9sJC6+f7FmPMOjIyoDT/vHudtwxF9l0JzS68Gl4dY2UY8uZgwScRxnWlLq5XWohDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ae57a564904f8821137cc83f722086807a3aa4740cccb6be08cc3366e30e5aa7","last_reissued_at":"2026-05-18T02:09:20.408889Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:09:20.408889Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Chandra detection of diffuse X-ray emission from the globular cluster Terzan 5","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A.-C. 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