{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:UD6FQOGNICWX7453BHEJUKZZ5Q","short_pith_number":"pith:UD6FQOGN","schema_version":"1.0","canonical_sha256":"a0fc5838cd40ad7ff3bb09c89a2b39ec0ac1b9b42b5e5628eadbce784d2f1315","source":{"kind":"arxiv","id":"1707.01937","version":1},"attestation_state":"computed","paper":{"title":"Simultaneous Monitoring of X-ray and Radio Variability in Sagittarius A*","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Bill Cotton, Casey J. Law, Craig O. Heinke, Daniel M. Capellupo, Daryl Haggard, Farhad Yusef-Zadeh, Fred Baganoff, Gabriele Ponti, Geoffrey C. Bower, Heino Falcke, Jason Dexter, Joey Neilsen, Nanda Rea, Nathalie Degenaar, Nicolas Choux, P. Chris Fragile, Sera Markoff","submitted_at":"2017-07-06T18:53:00Z","abstract_excerpt":"Monitoring of Sagittarius A* from X-ray to radio wavelengths has revealed structured variability --- including X-ray flares --- but it is challenging to establish correlations between them. Most studies have focused on variability in the X-ray and infrared, where variations are often simultaneous, and because long time series at sub-millimeter and radio wavelengths are limited. Previous work on sub-mm and radio variability hints at a lag between X-ray flares and their candidate sub-millimeter or radio counterparts, with the long wavelength data lagging the X-ray. However, there is only one pub"},"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":"1707.01937","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-07-06T18:53:00Z","cross_cats_sorted":[],"title_canon_sha256":"95133637dda7d8e93dbaa115bd254c4390e0d63a6e9dd05a232172ca9b897155","abstract_canon_sha256":"d54b378f9c40194e5a785f12a9cbb77cb593dba0a881660ce7111374124c2be1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:37:01.297221Z","signature_b64":"8s9y9uYKm1vkVcSW/0gim7ufI5/ge1fjUG1PKLdTGvx2KefToVEpJSin2B3/vULVacQa5C7XNOaBU8pCWmfYCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a0fc5838cd40ad7ff3bb09c89a2b39ec0ac1b9b42b5e5628eadbce784d2f1315","last_reissued_at":"2026-05-18T00:37:01.296711Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:37:01.296711Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Simultaneous Monitoring of X-ray and Radio Variability in Sagittarius A*","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Bill Cotton, Casey J. Law, Craig O. Heinke, Daniel M. Capellupo, Daryl Haggard, Farhad Yusef-Zadeh, Fred Baganoff, Gabriele Ponti, Geoffrey C. Bower, Heino Falcke, Jason Dexter, Joey Neilsen, Nanda Rea, Nathalie Degenaar, Nicolas Choux, P. Chris Fragile, Sera Markoff","submitted_at":"2017-07-06T18:53:00Z","abstract_excerpt":"Monitoring of Sagittarius A* from X-ray to radio wavelengths has revealed structured variability --- including X-ray flares --- but it is challenging to establish correlations between them. Most studies have focused on variability in the X-ray and infrared, where variations are often simultaneous, and because long time series at sub-millimeter and radio wavelengths are limited. Previous work on sub-mm and radio variability hints at a lag between X-ray flares and their candidate sub-millimeter or radio counterparts, with the long wavelength data lagging the X-ray. However, there is only one pub"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1707.01937","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":""},"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":"1707.01937","created_at":"2026-05-18T00:37:01.296799+00:00"},{"alias_kind":"arxiv_version","alias_value":"1707.01937v1","created_at":"2026-05-18T00:37:01.296799+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1707.01937","created_at":"2026-05-18T00:37:01.296799+00:00"},{"alias_kind":"pith_short_12","alias_value":"UD6FQOGNICWX","created_at":"2026-05-18T12:31:46.661854+00:00"},{"alias_kind":"pith_short_16","alias_value":"UD6FQOGNICWX7453","created_at":"2026-05-18T12:31:46.661854+00:00"},{"alias_kind":"pith_short_8","alias_value":"UD6FQOGN","created_at":"2026-05-18T12:31:46.661854+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/UD6FQOGNICWX7453BHEJUKZZ5Q","json":"https://pith.science/pith/UD6FQOGNICWX7453BHEJUKZZ5Q.json","graph_json":"https://pith.science/api/pith-number/UD6FQOGNICWX7453BHEJUKZZ5Q/graph.json","events_json":"https://pith.science/api/pith-number/UD6FQOGNICWX7453BHEJUKZZ5Q/events.json","paper":"https://pith.science/paper/UD6FQOGN"},"agent_actions":{"view_html":"https://pith.science/pith/UD6FQOGNICWX7453BHEJUKZZ5Q","download_json":"https://pith.science/pith/UD6FQOGNICWX7453BHEJUKZZ5Q.json","view_paper":"https://pith.science/paper/UD6FQOGN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1707.01937&json=true","fetch_graph":"https://pith.science/api/pith-number/UD6FQOGNICWX7453BHEJUKZZ5Q/graph.json","fetch_events":"https://pith.science/api/pith-number/UD6FQOGNICWX7453BHEJUKZZ5Q/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UD6FQOGNICWX7453BHEJUKZZ5Q/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UD6FQOGNICWX7453BHEJUKZZ5Q/action/storage_attestation","attest_author":"https://pith.science/pith/UD6FQOGNICWX7453BHEJUKZZ5Q/action/author_attestation","sign_citation":"https://pith.science/pith/UD6FQOGNICWX7453BHEJUKZZ5Q/action/citation_signature","submit_replication":"https://pith.science/pith/UD6FQOGNICWX7453BHEJUKZZ5Q/action/replication_record"}},"created_at":"2026-05-18T00:37:01.296799+00:00","updated_at":"2026-05-18T00:37:01.296799+00:00"}