{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:TGL2SIWWF4ZRCWUWG34WFELCL2","short_pith_number":"pith:TGL2SIWW","schema_version":"1.0","canonical_sha256":"9997a922d62f33115a9636f96291625e9869efcbe66fa8dbee07c93636fbe8ae","source":{"kind":"arxiv","id":"2302.00315","version":1},"attestation_state":"computed","paper":{"title":"Multi-wavelength study of NGC 1365: The obscured active nucleus and off-nuclear compact X-ray sources","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"Gulab Chand Dewangan, K .V. P. Latha, Prakash Tripathi, P. Shalima, Subhashree Swain","submitted_at":"2023-02-01T08:48:59Z","abstract_excerpt":"We present a multi-wavelength study of the active nucleus and the off-nuclear X-ray sources in the nearby spiral galaxy, NGC 1365 using three simultaneous UV/X-ray observations by AstroSat over a two months period and archival IR observations performed with Spitzer and Herschel. Utilising the data from the Soft X-ray Telescope (SXT) on-board AstroSat, we find spectral variability mainly caused by the variation in the X-ray column density, (N$_H$ $\\sim$ 10$^{22}$ - 10$^{23}$ cm$^{-2}$). With the accurate spatial resolution of the UVIT onboard AstroSat, we separate the intrinsic AGN flux from th"},"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":"2302.00315","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2023-02-01T08:48:59Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"9eb597734ef2f5055bb38333ee66c1defc992dcc38f67773f2eecc08726da7b0","abstract_canon_sha256":"b4b6a24a65f562ab55a644874529f1527d5f86770e4c9aa191c571661f35d2d0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:39:32.758878Z","signature_b64":"QaAl/4rtg9PiNZlX2sVb/6P4WVkse94kbWH9C0pKn+A5wOm8bNXGfxlsc9Jid2rSGMgiXtBZVTu2BDPYvUMKAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9997a922d62f33115a9636f96291625e9869efcbe66fa8dbee07c93636fbe8ae","last_reissued_at":"2026-07-05T05:39:32.758520Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:39:32.758520Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Multi-wavelength study of NGC 1365: The obscured active nucleus and off-nuclear compact X-ray sources","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"Gulab Chand Dewangan, K .V. P. Latha, Prakash Tripathi, P. Shalima, Subhashree Swain","submitted_at":"2023-02-01T08:48:59Z","abstract_excerpt":"We present a multi-wavelength study of the active nucleus and the off-nuclear X-ray sources in the nearby spiral galaxy, NGC 1365 using three simultaneous UV/X-ray observations by AstroSat over a two months period and archival IR observations performed with Spitzer and Herschel. Utilising the data from the Soft X-ray Telescope (SXT) on-board AstroSat, we find spectral variability mainly caused by the variation in the X-ray column density, (N$_H$ $\\sim$ 10$^{22}$ - 10$^{23}$ cm$^{-2}$). With the accurate spatial resolution of the UVIT onboard AstroSat, we separate the intrinsic AGN flux from th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2302.00315","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2302.00315/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"2302.00315","created_at":"2026-07-05T05:39:32.758576+00:00"},{"alias_kind":"arxiv_version","alias_value":"2302.00315v1","created_at":"2026-07-05T05:39:32.758576+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2302.00315","created_at":"2026-07-05T05:39:32.758576+00:00"},{"alias_kind":"pith_short_12","alias_value":"TGL2SIWWF4ZR","created_at":"2026-07-05T05:39:32.758576+00:00"},{"alias_kind":"pith_short_16","alias_value":"TGL2SIWWF4ZRCWUW","created_at":"2026-07-05T05:39:32.758576+00:00"},{"alias_kind":"pith_short_8","alias_value":"TGL2SIWW","created_at":"2026-07-05T05:39:32.758576+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2504.17436","citing_title":"Detection and Characterization of Quasi-Periodic Oscillations in Seyfert Galaxy NGC 4151","ref_index":1,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TGL2SIWWF4ZRCWUWG34WFELCL2","json":"https://pith.science/pith/TGL2SIWWF4ZRCWUWG34WFELCL2.json","graph_json":"https://pith.science/api/pith-number/TGL2SIWWF4ZRCWUWG34WFELCL2/graph.json","events_json":"https://pith.science/api/pith-number/TGL2SIWWF4ZRCWUWG34WFELCL2/events.json","paper":"https://pith.science/paper/TGL2SIWW"},"agent_actions":{"view_html":"https://pith.science/pith/TGL2SIWWF4ZRCWUWG34WFELCL2","download_json":"https://pith.science/pith/TGL2SIWWF4ZRCWUWG34WFELCL2.json","view_paper":"https://pith.science/paper/TGL2SIWW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2302.00315&json=true","fetch_graph":"https://pith.science/api/pith-number/TGL2SIWWF4ZRCWUWG34WFELCL2/graph.json","fetch_events":"https://pith.science/api/pith-number/TGL2SIWWF4ZRCWUWG34WFELCL2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TGL2SIWWF4ZRCWUWG34WFELCL2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TGL2SIWWF4ZRCWUWG34WFELCL2/action/storage_attestation","attest_author":"https://pith.science/pith/TGL2SIWWF4ZRCWUWG34WFELCL2/action/author_attestation","sign_citation":"https://pith.science/pith/TGL2SIWWF4ZRCWUWG34WFELCL2/action/citation_signature","submit_replication":"https://pith.science/pith/TGL2SIWWF4ZRCWUWG34WFELCL2/action/replication_record"}},"created_at":"2026-07-05T05:39:32.758576+00:00","updated_at":"2026-07-05T05:39:32.758576+00:00"}