{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2009:LRW7JQJTOGKOLAU7N3TF5HOWN7","short_pith_number":"pith:LRW7JQJT","schema_version":"1.0","canonical_sha256":"5c6df4c1337194e5829f6ee65e9dd66ffb9b80a7f6196d8a48112fb8892bb0af","source":{"kind":"arxiv","id":"0908.3819","version":2},"attestation_state":"computed","paper":{"title":"Upper Limits on X-ray Emission from Two Rotating Radio Transients","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Possenti, D. Chakrabarty, D. L. Kaplan, F. Camilo, M. A. McLaughlin, P. Esposito, P. O. Slane, S. Chatterjee","submitted_at":"2009-08-26T13:30:05Z","abstract_excerpt":"X-ray emission from the enigmatic Rotating RAdio Transients (RRATs) offers a vital clue to understanding these objects and how they relate to the greater neutron star population. An X-ray counterpart to J1819-1458 is known, and its properties are similar to those of other middle-aged (0.1 Myr) neutron stars. We have searched for X-ray emission with Chandra/ACIS at the positions of two RRATs with arcsecond (or better) localisation, J0847-4316 and J1846-0257. Despite deep searches (especially for J1847-0257) we did not detect any emission with 0.3-8 keV count-rate limits of 1 counts/ks and 0.068"},"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":"0908.3819","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2009-08-26T13:30:05Z","cross_cats_sorted":[],"title_canon_sha256":"01262072f2c929a763269dff3363c593227b08890172c7c10160102b7d52e517","abstract_canon_sha256":"9ea8acbc4921568a4662d488ddfbd3849e79d092501ed3bf0915cbd7130e3cde"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:12:22.716690Z","signature_b64":"x+sSJos90MpsXQqOFp0zy4p6zjGPDByqeuTxKWX2r4R3ymyEFVlCRiInK1HFgXO1tpcZ8i7+4LivOfWd4o5WDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5c6df4c1337194e5829f6ee65e9dd66ffb9b80a7f6196d8a48112fb8892bb0af","last_reissued_at":"2026-05-18T02:12:22.715922Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:12:22.715922Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Upper Limits on X-ray Emission from Two Rotating Radio Transients","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Possenti, D. Chakrabarty, D. L. Kaplan, F. Camilo, M. A. McLaughlin, P. Esposito, P. O. Slane, S. Chatterjee","submitted_at":"2009-08-26T13:30:05Z","abstract_excerpt":"X-ray emission from the enigmatic Rotating RAdio Transients (RRATs) offers a vital clue to understanding these objects and how they relate to the greater neutron star population. An X-ray counterpart to J1819-1458 is known, and its properties are similar to those of other middle-aged (0.1 Myr) neutron stars. We have searched for X-ray emission with Chandra/ACIS at the positions of two RRATs with arcsecond (or better) localisation, J0847-4316 and J1846-0257. Despite deep searches (especially for J1847-0257) we did not detect any emission with 0.3-8 keV count-rate limits of 1 counts/ks and 0.068"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0908.3819","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":"0908.3819","created_at":"2026-05-18T02:12:22.716041+00:00"},{"alias_kind":"arxiv_version","alias_value":"0908.3819v2","created_at":"2026-05-18T02:12:22.716041+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0908.3819","created_at":"2026-05-18T02:12:22.716041+00:00"},{"alias_kind":"pith_short_12","alias_value":"LRW7JQJTOGKO","created_at":"2026-05-18T12:26:00.592388+00:00"},{"alias_kind":"pith_short_16","alias_value":"LRW7JQJTOGKOLAU7","created_at":"2026-05-18T12:26:00.592388+00:00"},{"alias_kind":"pith_short_8","alias_value":"LRW7JQJT","created_at":"2026-05-18T12:26:00.592388+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/LRW7JQJTOGKOLAU7N3TF5HOWN7","json":"https://pith.science/pith/LRW7JQJTOGKOLAU7N3TF5HOWN7.json","graph_json":"https://pith.science/api/pith-number/LRW7JQJTOGKOLAU7N3TF5HOWN7/graph.json","events_json":"https://pith.science/api/pith-number/LRW7JQJTOGKOLAU7N3TF5HOWN7/events.json","paper":"https://pith.science/paper/LRW7JQJT"},"agent_actions":{"view_html":"https://pith.science/pith/LRW7JQJTOGKOLAU7N3TF5HOWN7","download_json":"https://pith.science/pith/LRW7JQJTOGKOLAU7N3TF5HOWN7.json","view_paper":"https://pith.science/paper/LRW7JQJT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0908.3819&json=true","fetch_graph":"https://pith.science/api/pith-number/LRW7JQJTOGKOLAU7N3TF5HOWN7/graph.json","fetch_events":"https://pith.science/api/pith-number/LRW7JQJTOGKOLAU7N3TF5HOWN7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LRW7JQJTOGKOLAU7N3TF5HOWN7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LRW7JQJTOGKOLAU7N3TF5HOWN7/action/storage_attestation","attest_author":"https://pith.science/pith/LRW7JQJTOGKOLAU7N3TF5HOWN7/action/author_attestation","sign_citation":"https://pith.science/pith/LRW7JQJTOGKOLAU7N3TF5HOWN7/action/citation_signature","submit_replication":"https://pith.science/pith/LRW7JQJTOGKOLAU7N3TF5HOWN7/action/replication_record"}},"created_at":"2026-05-18T02:12:22.716041+00:00","updated_at":"2026-05-18T02:12:22.716041+00:00"}