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Liszt","submitted_at":"2009-05-04T17:49:53Z","abstract_excerpt":"The field just West of the galactic supernova remnant W28\n  (l=6.4\\degr, b=-0.2\\degr) harbors 3 of 5 newly-discovered 1720 OH maser spots and two recently-discovered candidate supernova candidates (one of which is a $\\gamma$-ray source), as well as several compact and classical HII regions. Here, we analyze a datacube of CO J=1-0 emission having 1\\arcmin and 1 \\kms resolution, made with on-the-fly mapping over the region $5\\degr \\le l \\le 6\\degr, -1\\degr \\le b \\le 0.5\\degr$}. {Extended and often very bright CO emission was detected at the velocities of the 1720 MHz OH masers and around the sup"},"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":"0905.0438","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2009-05-04T17:49:53Z","cross_cats_sorted":[],"title_canon_sha256":"e6aa325f1144487a4034b54e0c5159029802b5d95042bff99c35f675e60a5c5a","abstract_canon_sha256":"e929dfc1d7364e3ef6543fbe492062367a6e8eead002aaccee876b26f7d08abc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:13:47.779762Z","signature_b64":"GI4+dsmEXcIQ16MiAx1bjUR3TJjUVfJBTjNMtdLagytJvGzDs+PPuJb4jF/kTrJ90Actj1SPstrasCLu3BTeDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f087723035d686700f2d798f5903cbf2973fdecbdf9bb4758a72253b8e5f6155","last_reissued_at":"2026-05-18T02:13:47.779199Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:13:47.779199Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"CO J=1-0 observations of molecular gas interacting with galactic supernova remnants G5.4-1.2, G5.55+0.32 and G5.71-0.08","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"H. 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Here, we analyze a datacube of CO J=1-0 emission having 1\\arcmin and 1 \\kms resolution, made with on-the-fly mapping over the region $5\\degr \\le l \\le 6\\degr, -1\\degr \\le b \\le 0.5\\degr$}. {Extended and often very bright CO emission was detected at the velocities of the 1720 MHz OH masers and around the sup"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0905.0438","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":"0905.0438","created_at":"2026-05-18T02:13:47.779285+00:00"},{"alias_kind":"arxiv_version","alias_value":"0905.0438v1","created_at":"2026-05-18T02:13:47.779285+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0905.0438","created_at":"2026-05-18T02:13:47.779285+00:00"},{"alias_kind":"pith_short_12","alias_value":"6CDXEMBV22DH","created_at":"2026-05-18T12:25:58.837520+00:00"},{"alias_kind":"pith_short_16","alias_value":"6CDXEMBV22DHADZN","created_at":"2026-05-18T12:25:58.837520+00:00"},{"alias_kind":"pith_short_8","alias_value":"6CDXEMBV","created_at":"2026-05-18T12:25:58.837520+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/6CDXEMBV22DHADZNPGHVSA6L6K","json":"https://pith.science/pith/6CDXEMBV22DHADZNPGHVSA6L6K.json","graph_json":"https://pith.science/api/pith-number/6CDXEMBV22DHADZNPGHVSA6L6K/graph.json","events_json":"https://pith.science/api/pith-number/6CDXEMBV22DHADZNPGHVSA6L6K/events.json","paper":"https://pith.science/paper/6CDXEMBV"},"agent_actions":{"view_html":"https://pith.science/pith/6CDXEMBV22DHADZNPGHVSA6L6K","download_json":"https://pith.science/pith/6CDXEMBV22DHADZNPGHVSA6L6K.json","view_paper":"https://pith.science/paper/6CDXEMBV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0905.0438&json=true","fetch_graph":"https://pith.science/api/pith-number/6CDXEMBV22DHADZNPGHVSA6L6K/graph.json","fetch_events":"https://pith.science/api/pith-number/6CDXEMBV22DHADZNPGHVSA6L6K/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6CDXEMBV22DHADZNPGHVSA6L6K/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6CDXEMBV22DHADZNPGHVSA6L6K/action/storage_attestation","attest_author":"https://pith.science/pith/6CDXEMBV22DHADZNPGHVSA6L6K/action/author_attestation","sign_citation":"https://pith.science/pith/6CDXEMBV22DHADZNPGHVSA6L6K/action/citation_signature","submit_replication":"https://pith.science/pith/6CDXEMBV22DHADZNPGHVSA6L6K/action/replication_record"}},"created_at":"2026-05-18T02:13:47.779285+00:00","updated_at":"2026-05-18T02:13:47.779285+00:00"}