{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:HED4XWMZD36B7OJTJXP2TC4EOK","short_pith_number":"pith:HED4XWMZ","schema_version":"1.0","canonical_sha256":"3907cbd9991efc1fb9334ddfa98b84728167a1a9868490bdda634ee7c3d8b1e1","source":{"kind":"arxiv","id":"1505.00265","version":2},"attestation_state":"computed","paper":{"title":"Band-9 ALMA observations of the [NII] 122 micron line and FIR continuum in two high-z galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Carl Ferkinhoff, Drew Brisbin, Edith Falgarone, Gordon J. Stacey, Kartik Sheth, Steve Hailey-Dunsheath, Thomas Nikola","submitted_at":"2015-05-01T20:00:28Z","abstract_excerpt":"We present Atacama Large Millimeter Array (ALMA) observations of two high-redshift systems (SMMJ02399-0136 and the Cloverleaf QSO) in their rest-frame 122 micron continuum (~650 GHz or ~450 micron on-sky) and [NII] 122 micron line emission. The continuum observations with a synthesized beam of ~0.25\" resolve both sources and recover the expected flux. The Cloverleaf is resolved into a partial Einstein ring, while the SMMJ02399-0136 is unambiguously separated into two components; an AGN associated point source and an extend region at the location of a previously identified dusty starburst. We d"},"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":"1505.00265","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-05-01T20:00:28Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"902508a03637bf743305a1646c04f53a3006282e5d50a690f9fa9a7f7e281d0e","abstract_canon_sha256":"bc32120970e4f2f6b3c093aad3c24887756aa8a464ac0d530cb8bcbcaadf9024"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:17:00.096738Z","signature_b64":"+lR4Ma4HespGorAWyPqWm/M3zUWNst2j+T5ST2e4DQmgKePYHbCxjurjnlmUJ3oPkBsqh4c2xzsEYT9aleMlDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3907cbd9991efc1fb9334ddfa98b84728167a1a9868490bdda634ee7c3d8b1e1","last_reissued_at":"2026-05-18T02:17:00.096259Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:17:00.096259Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Band-9 ALMA observations of the [NII] 122 micron line and FIR continuum in two high-z galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Carl Ferkinhoff, Drew Brisbin, Edith Falgarone, Gordon J. Stacey, Kartik Sheth, Steve Hailey-Dunsheath, Thomas Nikola","submitted_at":"2015-05-01T20:00:28Z","abstract_excerpt":"We present Atacama Large Millimeter Array (ALMA) observations of two high-redshift systems (SMMJ02399-0136 and the Cloverleaf QSO) in their rest-frame 122 micron continuum (~650 GHz or ~450 micron on-sky) and [NII] 122 micron line emission. The continuum observations with a synthesized beam of ~0.25\" resolve both sources and recover the expected flux. The Cloverleaf is resolved into a partial Einstein ring, while the SMMJ02399-0136 is unambiguously separated into two components; an AGN associated point source and an extend region at the location of a previously identified dusty starburst. We d"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1505.00265","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":""},"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":"1505.00265","created_at":"2026-05-18T02:17:00.096335+00:00"},{"alias_kind":"arxiv_version","alias_value":"1505.00265v2","created_at":"2026-05-18T02:17:00.096335+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1505.00265","created_at":"2026-05-18T02:17:00.096335+00:00"},{"alias_kind":"pith_short_12","alias_value":"HED4XWMZD36B","created_at":"2026-05-18T12:29:25.134429+00:00"},{"alias_kind":"pith_short_16","alias_value":"HED4XWMZD36B7OJT","created_at":"2026-05-18T12:29:25.134429+00:00"},{"alias_kind":"pith_short_8","alias_value":"HED4XWMZ","created_at":"2026-05-18T12:29:25.134429+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1908.05504","citing_title":"Theoretical ISM pressure and electron density diagnostics for local and high-redshift galaxies","ref_index":40,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/HED4XWMZD36B7OJTJXP2TC4EOK","json":"https://pith.science/pith/HED4XWMZD36B7OJTJXP2TC4EOK.json","graph_json":"https://pith.science/api/pith-number/HED4XWMZD36B7OJTJXP2TC4EOK/graph.json","events_json":"https://pith.science/api/pith-number/HED4XWMZD36B7OJTJXP2TC4EOK/events.json","paper":"https://pith.science/paper/HED4XWMZ"},"agent_actions":{"view_html":"https://pith.science/pith/HED4XWMZD36B7OJTJXP2TC4EOK","download_json":"https://pith.science/pith/HED4XWMZD36B7OJTJXP2TC4EOK.json","view_paper":"https://pith.science/paper/HED4XWMZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1505.00265&json=true","fetch_graph":"https://pith.science/api/pith-number/HED4XWMZD36B7OJTJXP2TC4EOK/graph.json","fetch_events":"https://pith.science/api/pith-number/HED4XWMZD36B7OJTJXP2TC4EOK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HED4XWMZD36B7OJTJXP2TC4EOK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HED4XWMZD36B7OJTJXP2TC4EOK/action/storage_attestation","attest_author":"https://pith.science/pith/HED4XWMZD36B7OJTJXP2TC4EOK/action/author_attestation","sign_citation":"https://pith.science/pith/HED4XWMZD36B7OJTJXP2TC4EOK/action/citation_signature","submit_replication":"https://pith.science/pith/HED4XWMZD36B7OJTJXP2TC4EOK/action/replication_record"}},"created_at":"2026-05-18T02:17:00.096335+00:00","updated_at":"2026-05-18T02:17:00.096335+00:00"}