{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:XVFLSGRYDCGL35V5USNH3GQU4O","short_pith_number":"pith:XVFLSGRY","schema_version":"1.0","canonical_sha256":"bd4ab91a38188cbdf6bda49a7d9a14e3a8707aa08434a8ba2dab218d55b86d45","source":{"kind":"arxiv","id":"1902.10833","version":1},"attestation_state":"computed","paper":{"title":"Combining timing characteristics with physical broadband spectral modelling of black hole X-ray binary GX~339$-$4","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Chiara Ceccobello, David van Eijnatten, Dimitris Kantzas, Lucy Heil, Matteo Lucchini, Patrick Crumley, Riley M. T. Connors, Sera Markoff, Victoria Grinberg","submitted_at":"2019-02-27T23:40:18Z","abstract_excerpt":"GX~339$-$4 is a black hole X-ray binary that is a key focus of accretion studies since it goes into outburst roughly every two-to-three years. Tracking of its radio, IR and X-ray flux during multiple outbursts reveals tight broadband correlations. The radio emission originates in a compact, self-absorbed jet, however the origin of the X-ray emission is still debated: jet base or corona? We fit 20 quasi-simultaneous radio, IR, optical and X-ray observations of GX~339$-$4 covering three separate outbursts in 2005, 2007, 2010--2011, with a composite corona + jet model, where inverse Compton emiss"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1902.10833","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2019-02-27T23:40:18Z","cross_cats_sorted":[],"title_canon_sha256":"f02daab36c966abe67fbb9b7419d05ca65872d9fd89e73e9b759e8576ebccecb","abstract_canon_sha256":"850a1ccda363b2f36373dc4111a49970f5a651dcd8547d5b51b856e7c461fbfa"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:51:29.798234Z","signature_b64":"nGg/VcnE5A81C/0coFBZS2XRSLqkndqsD9/4dgqKtGMeNfwLYQ1vfi9f7wu3X4OjwrPtYBSePfnwhJpe27f7BA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bd4ab91a38188cbdf6bda49a7d9a14e3a8707aa08434a8ba2dab218d55b86d45","last_reissued_at":"2026-05-17T23:51:29.797756Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:51:29.797756Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Combining timing characteristics with physical broadband spectral modelling of black hole X-ray binary GX~339$-$4","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Chiara Ceccobello, David van Eijnatten, Dimitris Kantzas, Lucy Heil, Matteo Lucchini, Patrick Crumley, Riley M. T. Connors, Sera Markoff, Victoria Grinberg","submitted_at":"2019-02-27T23:40:18Z","abstract_excerpt":"GX~339$-$4 is a black hole X-ray binary that is a key focus of accretion studies since it goes into outburst roughly every two-to-three years. Tracking of its radio, IR and X-ray flux during multiple outbursts reveals tight broadband correlations. The radio emission originates in a compact, self-absorbed jet, however the origin of the X-ray emission is still debated: jet base or corona? We fit 20 quasi-simultaneous radio, IR, optical and X-ray observations of GX~339$-$4 covering three separate outbursts in 2005, 2007, 2010--2011, with a composite corona + jet model, where inverse Compton emiss"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1902.10833","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":"1902.10833","created_at":"2026-05-17T23:51:29.797822+00:00"},{"alias_kind":"arxiv_version","alias_value":"1902.10833v1","created_at":"2026-05-17T23:51:29.797822+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1902.10833","created_at":"2026-05-17T23:51:29.797822+00:00"},{"alias_kind":"pith_short_12","alias_value":"XVFLSGRYDCGL","created_at":"2026-05-18T12:33:33.725879+00:00"},{"alias_kind":"pith_short_16","alias_value":"XVFLSGRYDCGL35V5","created_at":"2026-05-18T12:33:33.725879+00:00"},{"alias_kind":"pith_short_8","alias_value":"XVFLSGRY","created_at":"2026-05-18T12:33:33.725879+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/XVFLSGRYDCGL35V5USNH3GQU4O","json":"https://pith.science/pith/XVFLSGRYDCGL35V5USNH3GQU4O.json","graph_json":"https://pith.science/api/pith-number/XVFLSGRYDCGL35V5USNH3GQU4O/graph.json","events_json":"https://pith.science/api/pith-number/XVFLSGRYDCGL35V5USNH3GQU4O/events.json","paper":"https://pith.science/paper/XVFLSGRY"},"agent_actions":{"view_html":"https://pith.science/pith/XVFLSGRYDCGL35V5USNH3GQU4O","download_json":"https://pith.science/pith/XVFLSGRYDCGL35V5USNH3GQU4O.json","view_paper":"https://pith.science/paper/XVFLSGRY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1902.10833&json=true","fetch_graph":"https://pith.science/api/pith-number/XVFLSGRYDCGL35V5USNH3GQU4O/graph.json","fetch_events":"https://pith.science/api/pith-number/XVFLSGRYDCGL35V5USNH3GQU4O/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XVFLSGRYDCGL35V5USNH3GQU4O/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XVFLSGRYDCGL35V5USNH3GQU4O/action/storage_attestation","attest_author":"https://pith.science/pith/XVFLSGRYDCGL35V5USNH3GQU4O/action/author_attestation","sign_citation":"https://pith.science/pith/XVFLSGRYDCGL35V5USNH3GQU4O/action/citation_signature","submit_replication":"https://pith.science/pith/XVFLSGRYDCGL35V5USNH3GQU4O/action/replication_record"}},"created_at":"2026-05-17T23:51:29.797822+00:00","updated_at":"2026-05-17T23:51:29.797822+00:00"}