{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:4BNTIFH23ZBM5TXR7ZXVYQZ6T2","short_pith_number":"pith:4BNTIFH2","schema_version":"1.0","canonical_sha256":"e05b3414fade42cecef1fe6f5c433e9eadec0c522cef5cb1e9873673855fef95","source":{"kind":"arxiv","id":"2405.13183","version":1},"attestation_state":"computed","paper":{"title":"Spectrum and polarization of the Galactic center radio transient ASKAP J173608.2-321635 from THOR-GC and VLITE","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.GA","authors_text":"Ashley Barnes, Henrik Beuther, James Urquhart, Jeroen M. Stil, Karl M. Menten, Kierra J. Weatherhead, Kristina E. Nyland, Loren Anderson, Mattia C. Sormani, Michael Rugel, Paul Goldsmith, Sergio A. Dzib, Tracy E. Clarke, Wendy M. Peters","submitted_at":"2024-05-21T20:25:19Z","abstract_excerpt":"The radio transient ASKAP J173608.2-321735, at the position (l,b)= (356.0872,-0.0390), was serendipitously observed by The HI/OH/Recombination Line Survey of the Galactic Center (THOR-GC) at three epochs in March 2020, April 2020 and February 2021. The source was detected only on 2020 April 11 with flux density 20.6 +/- 1.1 mJy at 1.23 GHz and in-band spectral index alpha = -3.1 +/- 0.2. The commensal VLA Low-band Ionsophere and Transient Experiment (VLITE) simultaneously detected the source at 339 MHz with a flux density 122.6 +/- 20.4 mJy, indicating a spectral break below 1 GHz. The rotatio"},"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":"2405.13183","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2024-05-21T20:25:19Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"04ba7dc9cb37b6e0e1fb0e153f3857ccbceefc7d683e7377268500937b82894c","abstract_canon_sha256":"60c4e2cb8b8b557130256dd63abded042a47ab7767b5aac31bf0219a2b3ead73"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:21:59.364083Z","signature_b64":"CKd3bgHWO9sMNp+U6Gn+e8/AdTNke03MV5Jo/EJFMAV5P9vZ6EwykUSTJw06WrGUTIBcXGObuRqMaPbuXu0fCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e05b3414fade42cecef1fe6f5c433e9eadec0c522cef5cb1e9873673855fef95","last_reissued_at":"2026-07-05T08:21:59.363577Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:21:59.363577Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Spectrum and polarization of the Galactic center radio transient ASKAP J173608.2-321635 from THOR-GC and VLITE","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.GA","authors_text":"Ashley Barnes, Henrik Beuther, James Urquhart, Jeroen M. Stil, Karl M. Menten, Kierra J. Weatherhead, Kristina E. Nyland, Loren Anderson, Mattia C. Sormani, Michael Rugel, Paul Goldsmith, Sergio A. Dzib, Tracy E. Clarke, Wendy M. Peters","submitted_at":"2024-05-21T20:25:19Z","abstract_excerpt":"The radio transient ASKAP J173608.2-321735, at the position (l,b)= (356.0872,-0.0390), was serendipitously observed by The HI/OH/Recombination Line Survey of the Galactic Center (THOR-GC) at three epochs in March 2020, April 2020 and February 2021. The source was detected only on 2020 April 11 with flux density 20.6 +/- 1.1 mJy at 1.23 GHz and in-band spectral index alpha = -3.1 +/- 0.2. The commensal VLA Low-band Ionsophere and Transient Experiment (VLITE) simultaneously detected the source at 339 MHz with a flux density 122.6 +/- 20.4 mJy, indicating a spectral break below 1 GHz. The rotatio"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2405.13183","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/2405.13183/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":"2405.13183","created_at":"2026-07-05T08:21:59.363641+00:00"},{"alias_kind":"arxiv_version","alias_value":"2405.13183v1","created_at":"2026-07-05T08:21:59.363641+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2405.13183","created_at":"2026-07-05T08:21:59.363641+00:00"},{"alias_kind":"pith_short_12","alias_value":"4BNTIFH23ZBM","created_at":"2026-07-05T08:21:59.363641+00:00"},{"alias_kind":"pith_short_16","alias_value":"4BNTIFH23ZBM5TXR","created_at":"2026-07-05T08:21:59.363641+00:00"},{"alias_kind":"pith_short_8","alias_value":"4BNTIFH2","created_at":"2026-07-05T08:21:59.363641+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.30518","citing_title":"Regime-Aware Peer Specialization for Robust RAG under Heterogeneous Knowledge Conflicts","ref_index":41,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/4BNTIFH23ZBM5TXR7ZXVYQZ6T2","json":"https://pith.science/pith/4BNTIFH23ZBM5TXR7ZXVYQZ6T2.json","graph_json":"https://pith.science/api/pith-number/4BNTIFH23ZBM5TXR7ZXVYQZ6T2/graph.json","events_json":"https://pith.science/api/pith-number/4BNTIFH23ZBM5TXR7ZXVYQZ6T2/events.json","paper":"https://pith.science/paper/4BNTIFH2"},"agent_actions":{"view_html":"https://pith.science/pith/4BNTIFH23ZBM5TXR7ZXVYQZ6T2","download_json":"https://pith.science/pith/4BNTIFH23ZBM5TXR7ZXVYQZ6T2.json","view_paper":"https://pith.science/paper/4BNTIFH2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2405.13183&json=true","fetch_graph":"https://pith.science/api/pith-number/4BNTIFH23ZBM5TXR7ZXVYQZ6T2/graph.json","fetch_events":"https://pith.science/api/pith-number/4BNTIFH23ZBM5TXR7ZXVYQZ6T2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4BNTIFH23ZBM5TXR7ZXVYQZ6T2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4BNTIFH23ZBM5TXR7ZXVYQZ6T2/action/storage_attestation","attest_author":"https://pith.science/pith/4BNTIFH23ZBM5TXR7ZXVYQZ6T2/action/author_attestation","sign_citation":"https://pith.science/pith/4BNTIFH23ZBM5TXR7ZXVYQZ6T2/action/citation_signature","submit_replication":"https://pith.science/pith/4BNTIFH23ZBM5TXR7ZXVYQZ6T2/action/replication_record"}},"created_at":"2026-07-05T08:21:59.363641+00:00","updated_at":"2026-07-05T08:21:59.363641+00:00"}