{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:B7SX7EKY3XGC6R6FSHLORTMXZV","short_pith_number":"pith:B7SX7EKY","schema_version":"1.0","canonical_sha256":"0fe57f9158ddcc2f47c591d6e8cd97cd62870653e19115d3d136f3e6b60018c5","source":{"kind":"arxiv","id":"1210.0020","version":2},"attestation_state":"computed","paper":{"title":"Late Time Radio Emission from X-ray Selected Tidal Disruption Events","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"Brian D. Metzger (Princeton), Geoffrey C. Bower (UCB), Jeffrey M. Silverman, Joshua S. Bloom (UCB), S. Bradley Cenko","submitted_at":"2012-09-28T20:05:00Z","abstract_excerpt":"We present new observations with the Karl G. Jansky Very Large Array of seven X-ray-selected tidal disruption events (TDEs). The radio observations were carried out between 9 and 22 years after the initial X-ray discovery, and, thus, probe the late-time formation of relativistic jets and jet interactions with the interstellar medium in these systems. We detect a compact radio source in the nucleus of the galaxy IC 3599 and a compact radio source that is a possible counterpart to RX J1420.4+5334. We find no radio counterparts for five other sources with flux density upper limits between 51 and "},"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":"1210.0020","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2012-09-28T20:05:00Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"ddcacc2d95e04eef959f7948d56d16b3d183189cfaad62e89c655d6ea4447221","abstract_canon_sha256":"08c08ee3494c5d42212de56026aed219d5b4f8e2c8cb6cf0d0bbfd1574167d22"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:54:12.640876Z","signature_b64":"0DYRQAVpa7bCreHiQ6YAJobnWm5Iwz7ZrYfMQkj3dDhRFjBq2AT2xlTK/4p4UU48wxol8JljsCn40B9t0BAgAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0fe57f9158ddcc2f47c591d6e8cd97cd62870653e19115d3d136f3e6b60018c5","last_reissued_at":"2026-05-18T01:54:12.640428Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:54:12.640428Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Late Time Radio Emission from X-ray Selected Tidal Disruption Events","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"Brian D. Metzger (Princeton), Geoffrey C. Bower (UCB), Jeffrey M. Silverman, Joshua S. Bloom (UCB), S. Bradley Cenko","submitted_at":"2012-09-28T20:05:00Z","abstract_excerpt":"We present new observations with the Karl G. Jansky Very Large Array of seven X-ray-selected tidal disruption events (TDEs). The radio observations were carried out between 9 and 22 years after the initial X-ray discovery, and, thus, probe the late-time formation of relativistic jets and jet interactions with the interstellar medium in these systems. We detect a compact radio source in the nucleus of the galaxy IC 3599 and a compact radio source that is a possible counterpart to RX J1420.4+5334. We find no radio counterparts for five other sources with flux density upper limits between 51 and "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1210.0020","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":"1210.0020","created_at":"2026-05-18T01:54:12.640489+00:00"},{"alias_kind":"arxiv_version","alias_value":"1210.0020v2","created_at":"2026-05-18T01:54:12.640489+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1210.0020","created_at":"2026-05-18T01:54:12.640489+00:00"},{"alias_kind":"pith_short_12","alias_value":"B7SX7EKY3XGC","created_at":"2026-05-18T12:26:58.693483+00:00"},{"alias_kind":"pith_short_16","alias_value":"B7SX7EKY3XGC6R6F","created_at":"2026-05-18T12:26:58.693483+00:00"},{"alias_kind":"pith_short_8","alias_value":"B7SX7EKY","created_at":"2026-05-18T12:26:58.693483+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/B7SX7EKY3XGC6R6FSHLORTMXZV","json":"https://pith.science/pith/B7SX7EKY3XGC6R6FSHLORTMXZV.json","graph_json":"https://pith.science/api/pith-number/B7SX7EKY3XGC6R6FSHLORTMXZV/graph.json","events_json":"https://pith.science/api/pith-number/B7SX7EKY3XGC6R6FSHLORTMXZV/events.json","paper":"https://pith.science/paper/B7SX7EKY"},"agent_actions":{"view_html":"https://pith.science/pith/B7SX7EKY3XGC6R6FSHLORTMXZV","download_json":"https://pith.science/pith/B7SX7EKY3XGC6R6FSHLORTMXZV.json","view_paper":"https://pith.science/paper/B7SX7EKY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1210.0020&json=true","fetch_graph":"https://pith.science/api/pith-number/B7SX7EKY3XGC6R6FSHLORTMXZV/graph.json","fetch_events":"https://pith.science/api/pith-number/B7SX7EKY3XGC6R6FSHLORTMXZV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/B7SX7EKY3XGC6R6FSHLORTMXZV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/B7SX7EKY3XGC6R6FSHLORTMXZV/action/storage_attestation","attest_author":"https://pith.science/pith/B7SX7EKY3XGC6R6FSHLORTMXZV/action/author_attestation","sign_citation":"https://pith.science/pith/B7SX7EKY3XGC6R6FSHLORTMXZV/action/citation_signature","submit_replication":"https://pith.science/pith/B7SX7EKY3XGC6R6FSHLORTMXZV/action/replication_record"}},"created_at":"2026-05-18T01:54:12.640489+00:00","updated_at":"2026-05-18T01:54:12.640489+00:00"}