{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:ZBZOXUOON7OWP672WDNSNAMNMW","short_pith_number":"pith:ZBZOXUOO","schema_version":"1.0","canonical_sha256":"c872ebd1ce6fdd67fbfab0db26818d65ab289dea9c95f2b096a04cb6dfcbfc38","source":{"kind":"arxiv","id":"1705.10927","version":1},"attestation_state":"computed","paper":{"title":"Galactic Supernova Remnant Candidates Discovered by THOR","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Alyssa A. Goodman, E. Churchwell, F. Bigiel, H. Beuther, H. Linz, J.D. Soler, J.M. Stil, J. Ott, J.S. Urquhart, K.M. Menten, L. D. Anderson, M. Heyer, M. Rugel, N. Roy, R.S. Klessen, S. Bihr, S.C.O. Glover, S.N. Longmore, Th. Henning, Y. Wang","submitted_at":"2017-05-31T02:58:12Z","abstract_excerpt":"There is a considerable deficiency in the number of known supernova remnants (SNRs) in the Galaxy compared to that expected. Searches for extended low-surface brightness radio sources may find new Galactic SNRs, but confusion with the much larger population of HII regions makes identifying such features challenging. SNRs can, however, be separated from HII regions using their significantly lower mid-infrared (MIR) to radio continuum intensity ratios. We use the combination of high-resolution 1-2 GHz continuum data from The HI, OH, Recombination line survey of the Milky Way (THOR) and lower-res"},"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":"1705.10927","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-05-31T02:58:12Z","cross_cats_sorted":[],"title_canon_sha256":"7bf6f7ad825589761bb7aa8e1b496d95d4d2c64ac3ada770c351cc386e40847e","abstract_canon_sha256":"0d27d3dd98ef4a60d38991eb9a78012b8a6da98018897e9f5a79521f99e0cd8e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:35:31.366719Z","signature_b64":"qUIlgdfx6JxdpwfVCezJtlL7YQzWuJfNeD0GtN3/IvsflaNg/PVn73y73DeAeRH2m0wSV4ZjPFiBFq+VVe25Cg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c872ebd1ce6fdd67fbfab0db26818d65ab289dea9c95f2b096a04cb6dfcbfc38","last_reissued_at":"2026-05-18T00:35:31.366205Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:35:31.366205Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Galactic Supernova Remnant Candidates Discovered by THOR","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Alyssa A. Goodman, E. Churchwell, F. Bigiel, H. Beuther, H. Linz, J.D. Soler, J.M. Stil, J. Ott, J.S. Urquhart, K.M. Menten, L. D. Anderson, M. Heyer, M. Rugel, N. Roy, R.S. Klessen, S. Bihr, S.C.O. Glover, S.N. Longmore, Th. Henning, Y. Wang","submitted_at":"2017-05-31T02:58:12Z","abstract_excerpt":"There is a considerable deficiency in the number of known supernova remnants (SNRs) in the Galaxy compared to that expected. Searches for extended low-surface brightness radio sources may find new Galactic SNRs, but confusion with the much larger population of HII regions makes identifying such features challenging. SNRs can, however, be separated from HII regions using their significantly lower mid-infrared (MIR) to radio continuum intensity ratios. We use the combination of high-resolution 1-2 GHz continuum data from The HI, OH, Recombination line survey of the Milky Way (THOR) and lower-res"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.10927","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":"1705.10927","created_at":"2026-05-18T00:35:31.366294+00:00"},{"alias_kind":"arxiv_version","alias_value":"1705.10927v1","created_at":"2026-05-18T00:35:31.366294+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1705.10927","created_at":"2026-05-18T00:35:31.366294+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZBZOXUOON7OW","created_at":"2026-05-18T12:31:59.375834+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZBZOXUOON7OWP672","created_at":"2026-05-18T12:31:59.375834+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZBZOXUOO","created_at":"2026-05-18T12:31:59.375834+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/ZBZOXUOON7OWP672WDNSNAMNMW","json":"https://pith.science/pith/ZBZOXUOON7OWP672WDNSNAMNMW.json","graph_json":"https://pith.science/api/pith-number/ZBZOXUOON7OWP672WDNSNAMNMW/graph.json","events_json":"https://pith.science/api/pith-number/ZBZOXUOON7OWP672WDNSNAMNMW/events.json","paper":"https://pith.science/paper/ZBZOXUOO"},"agent_actions":{"view_html":"https://pith.science/pith/ZBZOXUOON7OWP672WDNSNAMNMW","download_json":"https://pith.science/pith/ZBZOXUOON7OWP672WDNSNAMNMW.json","view_paper":"https://pith.science/paper/ZBZOXUOO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1705.10927&json=true","fetch_graph":"https://pith.science/api/pith-number/ZBZOXUOON7OWP672WDNSNAMNMW/graph.json","fetch_events":"https://pith.science/api/pith-number/ZBZOXUOON7OWP672WDNSNAMNMW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZBZOXUOON7OWP672WDNSNAMNMW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZBZOXUOON7OWP672WDNSNAMNMW/action/storage_attestation","attest_author":"https://pith.science/pith/ZBZOXUOON7OWP672WDNSNAMNMW/action/author_attestation","sign_citation":"https://pith.science/pith/ZBZOXUOON7OWP672WDNSNAMNMW/action/citation_signature","submit_replication":"https://pith.science/pith/ZBZOXUOON7OWP672WDNSNAMNMW/action/replication_record"}},"created_at":"2026-05-18T00:35:31.366294+00:00","updated_at":"2026-05-18T00:35:31.366294+00:00"}