{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:M4YV3OI4B42FEGSS5HSKBZONEP","short_pith_number":"pith:M4YV3OI4","schema_version":"1.0","canonical_sha256":"67315db91c0f34521a52e9e4a0e5cd23fceeb40d741dc2fed2095d3445f7bf5c","source":{"kind":"arxiv","id":"1504.05589","version":2},"attestation_state":"computed","paper":{"title":"Physical conditions of the interstellar medium in star-forming galaxies at z~1.5","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Chun Ly, Kazuhiro Shimasaku, Kentaro Motohara, Masao Hayashi, Matthew A. Malkan, Nobunari Kashikawa, Ryosuke Goto, Tohru Nagao, Yoshiaki Naito","submitted_at":"2015-04-21T20:01:34Z","abstract_excerpt":"We present results from Subaru/FMOS near-infrared (NIR) spectroscopy of 118 star-forming galaxies at $z\\sim1.5$ in the Subaru Deep Field. These galaxies are selected as [OII]$\\lambda$3727 emitters at $z\\approx$ 1.47 and 1.62 from narrow-band imaging. We detect H$\\alpha$ emission line in 115 galaxies, [OIII]$\\lambda$5007 emission line in 45 galaxies, and H$\\beta$, [NII]$\\lambda$6584, and [SII]$\\lambda\\lambda$6716,6731 in 13, 16, and 6 galaxies, respectively. Including the [OII] emission line, we use the six strong nebular emission lines in the individual and composite rest-frame optical spectra"},"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":"1504.05589","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-04-21T20:01:34Z","cross_cats_sorted":[],"title_canon_sha256":"8571aae1e279abaf04825caaba55da8589e4b3f3e658c405c3f93fbb29991699","abstract_canon_sha256":"ec655e7fdd879156dab65e509ca39a1904a3ba4eab64e659cab5f205f9e1d1e7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:30:24.701039Z","signature_b64":"w1dyC45/qjNIUhMMsWHGvHfPOtjI34kkPUw9MnBgQqo9VFE5jRb2DS0MfSHNXFlbfVgdZk3OV+oqpHsE+0UxCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"67315db91c0f34521a52e9e4a0e5cd23fceeb40d741dc2fed2095d3445f7bf5c","last_reissued_at":"2026-05-18T01:30:24.700380Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:30:24.700380Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Physical conditions of the interstellar medium in star-forming galaxies at z~1.5","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Chun Ly, Kazuhiro Shimasaku, Kentaro Motohara, Masao Hayashi, Matthew A. Malkan, Nobunari Kashikawa, Ryosuke Goto, Tohru Nagao, Yoshiaki Naito","submitted_at":"2015-04-21T20:01:34Z","abstract_excerpt":"We present results from Subaru/FMOS near-infrared (NIR) spectroscopy of 118 star-forming galaxies at $z\\sim1.5$ in the Subaru Deep Field. These galaxies are selected as [OII]$\\lambda$3727 emitters at $z\\approx$ 1.47 and 1.62 from narrow-band imaging. We detect H$\\alpha$ emission line in 115 galaxies, [OIII]$\\lambda$5007 emission line in 45 galaxies, and H$\\beta$, [NII]$\\lambda$6584, and [SII]$\\lambda\\lambda$6716,6731 in 13, 16, and 6 galaxies, respectively. Including the [OII] emission line, we use the six strong nebular emission lines in the individual and composite rest-frame optical spectra"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1504.05589","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":"1504.05589","created_at":"2026-05-18T01:30:24.700484+00:00"},{"alias_kind":"arxiv_version","alias_value":"1504.05589v2","created_at":"2026-05-18T01:30:24.700484+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1504.05589","created_at":"2026-05-18T01:30:24.700484+00:00"},{"alias_kind":"pith_short_12","alias_value":"M4YV3OI4B42F","created_at":"2026-05-18T12:29:32.376354+00:00"},{"alias_kind":"pith_short_16","alias_value":"M4YV3OI4B42FEGSS","created_at":"2026-05-18T12:29:32.376354+00:00"},{"alias_kind":"pith_short_8","alias_value":"M4YV3OI4","created_at":"2026-05-18T12:29:32.376354+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/M4YV3OI4B42FEGSS5HSKBZONEP","json":"https://pith.science/pith/M4YV3OI4B42FEGSS5HSKBZONEP.json","graph_json":"https://pith.science/api/pith-number/M4YV3OI4B42FEGSS5HSKBZONEP/graph.json","events_json":"https://pith.science/api/pith-number/M4YV3OI4B42FEGSS5HSKBZONEP/events.json","paper":"https://pith.science/paper/M4YV3OI4"},"agent_actions":{"view_html":"https://pith.science/pith/M4YV3OI4B42FEGSS5HSKBZONEP","download_json":"https://pith.science/pith/M4YV3OI4B42FEGSS5HSKBZONEP.json","view_paper":"https://pith.science/paper/M4YV3OI4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1504.05589&json=true","fetch_graph":"https://pith.science/api/pith-number/M4YV3OI4B42FEGSS5HSKBZONEP/graph.json","fetch_events":"https://pith.science/api/pith-number/M4YV3OI4B42FEGSS5HSKBZONEP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/M4YV3OI4B42FEGSS5HSKBZONEP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/M4YV3OI4B42FEGSS5HSKBZONEP/action/storage_attestation","attest_author":"https://pith.science/pith/M4YV3OI4B42FEGSS5HSKBZONEP/action/author_attestation","sign_citation":"https://pith.science/pith/M4YV3OI4B42FEGSS5HSKBZONEP/action/citation_signature","submit_replication":"https://pith.science/pith/M4YV3OI4B42FEGSS5HSKBZONEP/action/replication_record"}},"created_at":"2026-05-18T01:30:24.700484+00:00","updated_at":"2026-05-18T01:30:24.700484+00:00"}