{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:ZRR4VFOPJERRGNBWFFIAJ2GRVX","short_pith_number":"pith:ZRR4VFOP","schema_version":"1.0","canonical_sha256":"cc63ca95cf4923133436295004e8d1add142604c868f180785c5d8b7b2e4b25f","source":{"kind":"arxiv","id":"1502.01345","version":2},"attestation_state":"computed","paper":{"title":"A Multiwavelength Study of the Relativistic Tidal Disruption Candidate Sw J2058+05 at Late Times","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Alexei V. Filippenko, Andrew J. Levan, Andrew S. Fruchter, Arne Rau, Assaf Horesh, Dheeraj R. Pasham (NASA/GSFC & JSI), Geoffrey C. Bower, Gregory C. Brown, Jochen Greiner, Kim L. Page, Klaas Wiersema, Nial R. Tanvir, Paul T. O'Brien, Rebekah A. Hounsell, S. Bradley Cenko (NASA/GSFC & JSI), Stephen Dolan","submitted_at":"2015-02-04T21:00:13Z","abstract_excerpt":"We report a multiwavelength (X-ray, ultraviolet/optical/infrared, radio) analysis of the relativistic tidal disruption event candidate Sw J2058+05 from 3 months to 3 yr post-discovery in order to study its properties and compare its behavior with that of Sw J1644+57. Our main results are as follows. (1) The long-term X-ray light curve of Sw J2058+05 shows a remarkably similar trend to that of Sw J1644+57. After a prolonged power-law decay, the X-ray flux drops off rapidly by a factor of $\\gtrsim 160$ within a span of $\\Delta$$t$/$t$ $\\le$ 0.95. Associating this sudden decline with the transiti"},"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":"1502.01345","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2015-02-04T21:00:13Z","cross_cats_sorted":[],"title_canon_sha256":"a7a8abd06709eb9f04ed8e5afa1c40da76cf9093eee380e5413cc85e295488e5","abstract_canon_sha256":"a661e86d3d16178d19054a805ec78aa369b11ed71a141c965f7d9a0646e3d052"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:23:04.286960Z","signature_b64":"DSZPhgE6noTDkw8DwfXxncdEc+Wewwgw18e+ua1CzBFm3ouWeI2CoF6smFBDsOc0RN4lYyC0yKAzUwZdfFKqCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cc63ca95cf4923133436295004e8d1add142604c868f180785c5d8b7b2e4b25f","last_reissued_at":"2026-05-18T01:23:04.286430Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:23:04.286430Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Multiwavelength Study of the Relativistic Tidal Disruption Candidate Sw J2058+05 at Late Times","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Alexei V. Filippenko, Andrew J. Levan, Andrew S. Fruchter, Arne Rau, Assaf Horesh, Dheeraj R. Pasham (NASA/GSFC & JSI), Geoffrey C. Bower, Gregory C. Brown, Jochen Greiner, Kim L. Page, Klaas Wiersema, Nial R. Tanvir, Paul T. O'Brien, Rebekah A. Hounsell, S. Bradley Cenko (NASA/GSFC & JSI), Stephen Dolan","submitted_at":"2015-02-04T21:00:13Z","abstract_excerpt":"We report a multiwavelength (X-ray, ultraviolet/optical/infrared, radio) analysis of the relativistic tidal disruption event candidate Sw J2058+05 from 3 months to 3 yr post-discovery in order to study its properties and compare its behavior with that of Sw J1644+57. Our main results are as follows. (1) The long-term X-ray light curve of Sw J2058+05 shows a remarkably similar trend to that of Sw J1644+57. After a prolonged power-law decay, the X-ray flux drops off rapidly by a factor of $\\gtrsim 160$ within a span of $\\Delta$$t$/$t$ $\\le$ 0.95. Associating this sudden decline with the transiti"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1502.01345","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"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":"1502.01345","created_at":"2026-05-18T01:23:04.286524+00:00"},{"alias_kind":"arxiv_version","alias_value":"1502.01345v2","created_at":"2026-05-18T01:23:04.286524+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1502.01345","created_at":"2026-05-18T01:23:04.286524+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZRR4VFOPJERR","created_at":"2026-05-18T12:29:52.810259+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZRR4VFOPJERRGNBW","created_at":"2026-05-18T12:29:52.810259+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZRR4VFOP","created_at":"2026-05-18T12:29:52.810259+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ZRR4VFOPJERRGNBWFFIAJ2GRVX","json":"https://pith.science/pith/ZRR4VFOPJERRGNBWFFIAJ2GRVX.json","graph_json":"https://pith.science/api/pith-number/ZRR4VFOPJERRGNBWFFIAJ2GRVX/graph.json","events_json":"https://pith.science/api/pith-number/ZRR4VFOPJERRGNBWFFIAJ2GRVX/events.json","paper":"https://pith.science/paper/ZRR4VFOP"},"agent_actions":{"view_html":"https://pith.science/pith/ZRR4VFOPJERRGNBWFFIAJ2GRVX","download_json":"https://pith.science/pith/ZRR4VFOPJERRGNBWFFIAJ2GRVX.json","view_paper":"https://pith.science/paper/ZRR4VFOP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1502.01345&json=true","fetch_graph":"https://pith.science/api/pith-number/ZRR4VFOPJERRGNBWFFIAJ2GRVX/graph.json","fetch_events":"https://pith.science/api/pith-number/ZRR4VFOPJERRGNBWFFIAJ2GRVX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZRR4VFOPJERRGNBWFFIAJ2GRVX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZRR4VFOPJERRGNBWFFIAJ2GRVX/action/storage_attestation","attest_author":"https://pith.science/pith/ZRR4VFOPJERRGNBWFFIAJ2GRVX/action/author_attestation","sign_citation":"https://pith.science/pith/ZRR4VFOPJERRGNBWFFIAJ2GRVX/action/citation_signature","submit_replication":"https://pith.science/pith/ZRR4VFOPJERRGNBWFFIAJ2GRVX/action/replication_record"}},"created_at":"2026-05-18T01:23:04.286524+00:00","updated_at":"2026-05-18T01:23:04.286524+00:00"}