{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:IRW2DQRHSRLSJHJOT4FW3S2IVM","short_pith_number":"pith:IRW2DQRH","schema_version":"1.0","canonical_sha256":"446da1c2279457249d2e9f0b6dcb48ab00c47ce1eca2798437fae30974ca7134","source":{"kind":"arxiv","id":"1309.4491","version":1},"attestation_state":"computed","paper":{"title":"Bayesian Matching for X-ray and Infrared Sources in the MYStIX Project","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Eric D. Feigelson, Patrick S. Broos, Tim Naylor","submitted_at":"2013-09-17T22:16:25Z","abstract_excerpt":"Identifying the infrared counterparts of X-ray sources in Galactic Plane fields such as those of the MYStIX project presents particular difficulties due to the high density of infrared sources. This high stellar density makes it inevitable that a large fraction of X-ray positions will have a faint field star close to them, which standard matching techniques may incorrectly take to be the counterpart. Instead we use the infrared data to create a model of both the field star and counterpart magnitude distributions, which we then combine with a Bayesian technique to yield a probability that any s"},"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":"1309.4491","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2013-09-17T22:16:25Z","cross_cats_sorted":[],"title_canon_sha256":"efd293a5ecf24144c9d5366ffdff7313e7aea4f6dc7398608f61ae61c22fcf94","abstract_canon_sha256":"24ab379299b7eca74174759322423a08e2a9f939f17788e4c1a07c1d931a3de0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:47:36.143963Z","signature_b64":"tO19uAxlXgHI/V8OLSr1c0nHfQFd/GsUrDFpwBxl0z8mB/8LyASgqhWI8gDbI4bX5N9m9KycNj2fJJ+bJ8jaBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"446da1c2279457249d2e9f0b6dcb48ab00c47ce1eca2798437fae30974ca7134","last_reissued_at":"2026-05-18T01:47:36.143297Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:47:36.143297Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Bayesian Matching for X-ray and Infrared Sources in the MYStIX Project","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Eric D. Feigelson, Patrick S. Broos, Tim Naylor","submitted_at":"2013-09-17T22:16:25Z","abstract_excerpt":"Identifying the infrared counterparts of X-ray sources in Galactic Plane fields such as those of the MYStIX project presents particular difficulties due to the high density of infrared sources. This high stellar density makes it inevitable that a large fraction of X-ray positions will have a faint field star close to them, which standard matching techniques may incorrectly take to be the counterpart. Instead we use the infrared data to create a model of both the field star and counterpart magnitude distributions, which we then combine with a Bayesian technique to yield a probability that any s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1309.4491","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":"1309.4491","created_at":"2026-05-18T01:47:36.143429+00:00"},{"alias_kind":"arxiv_version","alias_value":"1309.4491v1","created_at":"2026-05-18T01:47:36.143429+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1309.4491","created_at":"2026-05-18T01:47:36.143429+00:00"},{"alias_kind":"pith_short_12","alias_value":"IRW2DQRHSRLS","created_at":"2026-05-18T12:27:49.015174+00:00"},{"alias_kind":"pith_short_16","alias_value":"IRW2DQRHSRLSJHJO","created_at":"2026-05-18T12:27:49.015174+00:00"},{"alias_kind":"pith_short_8","alias_value":"IRW2DQRH","created_at":"2026-05-18T12:27:49.015174+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/IRW2DQRHSRLSJHJOT4FW3S2IVM","json":"https://pith.science/pith/IRW2DQRHSRLSJHJOT4FW3S2IVM.json","graph_json":"https://pith.science/api/pith-number/IRW2DQRHSRLSJHJOT4FW3S2IVM/graph.json","events_json":"https://pith.science/api/pith-number/IRW2DQRHSRLSJHJOT4FW3S2IVM/events.json","paper":"https://pith.science/paper/IRW2DQRH"},"agent_actions":{"view_html":"https://pith.science/pith/IRW2DQRHSRLSJHJOT4FW3S2IVM","download_json":"https://pith.science/pith/IRW2DQRHSRLSJHJOT4FW3S2IVM.json","view_paper":"https://pith.science/paper/IRW2DQRH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1309.4491&json=true","fetch_graph":"https://pith.science/api/pith-number/IRW2DQRHSRLSJHJOT4FW3S2IVM/graph.json","fetch_events":"https://pith.science/api/pith-number/IRW2DQRHSRLSJHJOT4FW3S2IVM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IRW2DQRHSRLSJHJOT4FW3S2IVM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IRW2DQRHSRLSJHJOT4FW3S2IVM/action/storage_attestation","attest_author":"https://pith.science/pith/IRW2DQRHSRLSJHJOT4FW3S2IVM/action/author_attestation","sign_citation":"https://pith.science/pith/IRW2DQRHSRLSJHJOT4FW3S2IVM/action/citation_signature","submit_replication":"https://pith.science/pith/IRW2DQRHSRLSJHJOT4FW3S2IVM/action/replication_record"}},"created_at":"2026-05-18T01:47:36.143429+00:00","updated_at":"2026-05-18T01:47:36.143429+00:00"}