{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:SU6VZ4H3BFJPP7AO6TO3CIIOFG","short_pith_number":"pith:SU6VZ4H3","schema_version":"1.0","canonical_sha256":"953d5cf0fb0952f7fc0ef4ddb1210e298722869e2b1fbd21bc7d6d7d4af2cad0","source":{"kind":"arxiv","id":"2607.27730","version":1},"attestation_state":"computed","paper":{"title":"eRASSU J043115.8-711730: The first pulsating symbiotic super-soft X-ray source in the Magellanic Bridge","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Andrej Udalski, Chandreyee Maitra, David Buckley, David Kaltenbrunner, Frank Haberl, Itumenleng Monageng, Lee Townsend, Manami Sasaki, Mara Salvato, Philip Charles, Sara Saeedi, Tathagata Saha","submitted_at":"2026-07-30T06:11:53Z","abstract_excerpt":"The Magellanic Bridge stellar population is a relic of the tidal interaction between the Large and Small Magellanic Clouds. A comprehensive view of the evolution of the Bridge stellar population requires probing the compact remnants of stellar evolution, otherwise hidden at optical wavelengths. The all-sky survey conducted by the eROSITA instrument on-board the Spectrum Roentgen Gamma observatory has discovered a significant population of compact-object-powered systems in the Bridge using X-ray. The candidate super-soft source eRASSU J043115.8-711730 (hereafter J0431-71) was discovered as a pa"},"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":"2607.27730","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2026-07-30T06:11:53Z","cross_cats_sorted":[],"title_canon_sha256":"fb57f5bf7989fcdd888e63b6e0e4d6b28737fa6927b5f4b1c8e19f1bc865f0ca","abstract_canon_sha256":"6b1390614dff6edd6dca555306d8a69159746d83d080e8b605bf09e18ffa4fc7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"953d5cf0fb0952f7fc0ef4ddb1210e298722869e2b1fbd21bc7d6d7d4af2cad0","last_reissued_at":"2026-07-31T01:30:05.045109Z","signature_status":"unsigned_v0","first_computed_at":"2026-07-31T01:30:05.045109Z"},"graph_snapshot":{"paper":{"title":"eRASSU J043115.8-711730: The first pulsating symbiotic super-soft X-ray source in the Magellanic Bridge","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Andrej Udalski, Chandreyee Maitra, David Buckley, David Kaltenbrunner, Frank Haberl, Itumenleng Monageng, Lee Townsend, Manami Sasaki, Mara Salvato, Philip Charles, Sara Saeedi, Tathagata Saha","submitted_at":"2026-07-30T06:11:53Z","abstract_excerpt":"The Magellanic Bridge stellar population is a relic of the tidal interaction between the Large and Small Magellanic Clouds. A comprehensive view of the evolution of the Bridge stellar population requires probing the compact remnants of stellar evolution, otherwise hidden at optical wavelengths. The all-sky survey conducted by the eROSITA instrument on-board the Spectrum Roentgen Gamma observatory has discovered a significant population of compact-object-powered systems in the Bridge using X-ray. The candidate super-soft source eRASSU J043115.8-711730 (hereafter J0431-71) was discovered as a pa"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2607.27730","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/2607.27730/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":"2607.27730","created_at":"2026-07-31T01:30:05.049133+00:00"},{"alias_kind":"arxiv_version","alias_value":"2607.27730v1","created_at":"2026-07-31T01:30:05.049133+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2607.27730","created_at":"2026-07-31T01:30:05.049133+00:00"},{"alias_kind":"pith_short_12","alias_value":"SU6VZ4H3BFJP","created_at":"2026-07-31T01:30:05.049133+00:00"},{"alias_kind":"pith_short_16","alias_value":"SU6VZ4H3BFJPP7AO","created_at":"2026-07-31T01:30:05.049133+00:00"},{"alias_kind":"pith_short_8","alias_value":"SU6VZ4H3","created_at":"2026-07-31T01:30:05.049133+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/SU6VZ4H3BFJPP7AO6TO3CIIOFG","json":"https://pith.science/pith/SU6VZ4H3BFJPP7AO6TO3CIIOFG.json","graph_json":"https://pith.science/api/pith-number/SU6VZ4H3BFJPP7AO6TO3CIIOFG/graph.json","events_json":"https://pith.science/api/pith-number/SU6VZ4H3BFJPP7AO6TO3CIIOFG/events.json","paper":"https://pith.science/paper/SU6VZ4H3"},"agent_actions":{"view_html":"https://pith.science/pith/SU6VZ4H3BFJPP7AO6TO3CIIOFG","download_json":"https://pith.science/pith/SU6VZ4H3BFJPP7AO6TO3CIIOFG.json","view_paper":"https://pith.science/paper/SU6VZ4H3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2607.27730&json=true","fetch_graph":"https://pith.science/api/pith-number/SU6VZ4H3BFJPP7AO6TO3CIIOFG/graph.json","fetch_events":"https://pith.science/api/pith-number/SU6VZ4H3BFJPP7AO6TO3CIIOFG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SU6VZ4H3BFJPP7AO6TO3CIIOFG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SU6VZ4H3BFJPP7AO6TO3CIIOFG/action/storage_attestation","attest_author":"https://pith.science/pith/SU6VZ4H3BFJPP7AO6TO3CIIOFG/action/author_attestation","sign_citation":"https://pith.science/pith/SU6VZ4H3BFJPP7AO6TO3CIIOFG/action/citation_signature","submit_replication":"https://pith.science/pith/SU6VZ4H3BFJPP7AO6TO3CIIOFG/action/replication_record"}},"created_at":"2026-07-31T01:30:05.049133+00:00","updated_at":"2026-07-31T01:30:05.049133+00:00"}