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We study the temporal and spectral profile of these Orphan $\\gamma$-ray flares in detail from three $\\gamma-ray$ bright blazars, 3C 273, PKS 1510-089 and 3C 279 and also their simultaneous broadband emissions. We find that the variability timescales of the Orphan $\\gamma$-ray flares were $(0.96\\pm0.28)$ days, $(3.12\\pm2.40)$ hr and $(2.16\\pm0.72)$ hr, for 3C 273, PKS 15"},"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":"2012.10291","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2020-12-18T15:15:02Z","cross_cats_sorted":[],"title_canon_sha256":"aaaec9a94c291288ded73e8f917577a747e9b390fe354da41bc91249f203bb0b","abstract_canon_sha256":"18c50141dd2684fb878539d9094df46289902d97e5a3f2ee043f68fa545bc7cf"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:00:37.405383Z","signature_b64":"qFurnxCyeggze2jkRIDfcUIGyliafXs74WarDDI2IY/0vh/xnPweWEMG7ImGYlazt62S8i3ZCFjwkSzX6nB0Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e8dd3be5d3da40b6151eb273428af4caf360934c7cffd38719ebc1708c27a32b","last_reissued_at":"2026-07-05T02:00:37.405014Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:00:37.405014Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Broadband Modelling of Orphan Gamma Ray Flares","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"D. 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