{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:W5A372MVEIMGALUACYYHCSUTKY","short_pith_number":"pith:W5A372MV","schema_version":"1.0","canonical_sha256":"b741bfe9952218602e801630714a93562060a4ef223a8801cb2271f0260651b7","source":{"kind":"arxiv","id":"2505.09148","version":2},"attestation_state":"computed","paper":{"title":"VAST-MeMeS: Characterising non-thermal radio emission from magnetic massive stars using the Australian SKA Pathfinder","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Andrew Zic, Barnali Das, Gregory Sivakoff, Joshua Pritchard, Kovi Rose, Laura N. Driessen, Matt E. Shultz, Tara Murphy, Yuanming Wang, Yu Wing Joshua Lee","submitted_at":"2025-05-14T05:10:03Z","abstract_excerpt":"Magnetic massive stars are stars of spectral types O, B and A that harbour $\\sim$ kG strength (mostly dipolar) surface magnetic fields. Their non-thermal radio emission has been demonstrated to be an important magnetospheric probe, provided the emission is fully characterised. A necessary step for that is to build a statistically significant sample of radio-bright magnetic massive stars. In this paper, we present the `VAST project to study Magnetic Massive Stars' or VAST-MeMeS that aims to achieve that by taking advantage of survey data acquired with the Australian SKA Pathfinder telescope. VA"},"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":"2505.09148","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2025-05-14T05:10:03Z","cross_cats_sorted":[],"title_canon_sha256":"c5c1fac0e1e78a668105e19094298d708ab581754ac9107ff839bdf939809d10","abstract_canon_sha256":"b67b8b6db9744167202cf9195c20c3e9da0cb341934f8bd8d384f83e29382590"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T12:02:46.119989Z","signature_b64":"C153BlQa9nErzUBJCVka9id620ezfWeEH0CS1SnyIxNFpf0LDjw2uFeQbJTagGsuIEEPwLiDloiuOa+EiHgYAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b741bfe9952218602e801630714a93562060a4ef223a8801cb2271f0260651b7","last_reissued_at":"2026-07-05T12:02:46.119484Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T12:02:46.119484Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"VAST-MeMeS: Characterising non-thermal radio emission from magnetic massive stars using the Australian SKA Pathfinder","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Andrew Zic, Barnali Das, Gregory Sivakoff, Joshua Pritchard, Kovi Rose, Laura N. Driessen, Matt E. Shultz, Tara Murphy, Yuanming Wang, Yu Wing Joshua Lee","submitted_at":"2025-05-14T05:10:03Z","abstract_excerpt":"Magnetic massive stars are stars of spectral types O, B and A that harbour $\\sim$ kG strength (mostly dipolar) surface magnetic fields. Their non-thermal radio emission has been demonstrated to be an important magnetospheric probe, provided the emission is fully characterised. A necessary step for that is to build a statistically significant sample of radio-bright magnetic massive stars. In this paper, we present the `VAST project to study Magnetic Massive Stars' or VAST-MeMeS that aims to achieve that by taking advantage of survey data acquired with the Australian SKA Pathfinder telescope. VA"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2505.09148","kind":"arxiv","version":2},"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/2505.09148/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":"2505.09148","created_at":"2026-07-05T12:02:46.119543+00:00"},{"alias_kind":"arxiv_version","alias_value":"2505.09148v2","created_at":"2026-07-05T12:02:46.119543+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2505.09148","created_at":"2026-07-05T12:02:46.119543+00:00"},{"alias_kind":"pith_short_12","alias_value":"W5A372MVEIMG","created_at":"2026-07-05T12:02:46.119543+00:00"},{"alias_kind":"pith_short_16","alias_value":"W5A372MVEIMGALUA","created_at":"2026-07-05T12:02:46.119543+00:00"},{"alias_kind":"pith_short_8","alias_value":"W5A372MV","created_at":"2026-07-05T12:02:46.119543+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.23768","citing_title":"GMRT Survey of Radio Emission from Magnetic Massive Stars -- I: Emission from Single Stars at sub-GHz Frequencies","ref_index":167,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/W5A372MVEIMGALUACYYHCSUTKY","json":"https://pith.science/pith/W5A372MVEIMGALUACYYHCSUTKY.json","graph_json":"https://pith.science/api/pith-number/W5A372MVEIMGALUACYYHCSUTKY/graph.json","events_json":"https://pith.science/api/pith-number/W5A372MVEIMGALUACYYHCSUTKY/events.json","paper":"https://pith.science/paper/W5A372MV"},"agent_actions":{"view_html":"https://pith.science/pith/W5A372MVEIMGALUACYYHCSUTKY","download_json":"https://pith.science/pith/W5A372MVEIMGALUACYYHCSUTKY.json","view_paper":"https://pith.science/paper/W5A372MV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2505.09148&json=true","fetch_graph":"https://pith.science/api/pith-number/W5A372MVEIMGALUACYYHCSUTKY/graph.json","fetch_events":"https://pith.science/api/pith-number/W5A372MVEIMGALUACYYHCSUTKY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/W5A372MVEIMGALUACYYHCSUTKY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/W5A372MVEIMGALUACYYHCSUTKY/action/storage_attestation","attest_author":"https://pith.science/pith/W5A372MVEIMGALUACYYHCSUTKY/action/author_attestation","sign_citation":"https://pith.science/pith/W5A372MVEIMGALUACYYHCSUTKY/action/citation_signature","submit_replication":"https://pith.science/pith/W5A372MVEIMGALUACYYHCSUTKY/action/replication_record"}},"created_at":"2026-07-05T12:02:46.119543+00:00","updated_at":"2026-07-05T12:02:46.119543+00:00"}