{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:XX35VSZKROSV6LAAUVHLVHVVPR","short_pith_number":"pith:XX35VSZK","schema_version":"1.0","canonical_sha256":"bdf7dacb2a8ba55f2c00a54eba9eb57c52d175bb93648db47e65923738f2bb59","source":{"kind":"arxiv","id":"1312.1891","version":1},"attestation_state":"computed","paper":{"title":"Exploring the early dust-obscured phase of galaxy formation with blind mid-/far-IR spectroscopic surveys","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A. Bressan, A. Lapi, C. Gruppioni, G. de Zotti, L. Danese, L. Spinoglio, M. Bonato, M. Negrello, Z.-Y. Cai","submitted_at":"2013-12-06T15:28:11Z","abstract_excerpt":"While continuum imaging data at far-infrared to sub-millimeter wavelengths have provided tight constraints on the population properties of dusty star forming galaxies up to high redshifts, future space missions like the Space Infra-Red Telescope for Cosmology and Astrophysics (SPICA) and ground based facilities like the Cerro Chajnantor Atacama Telescope (CCAT) will allow detailed investigations of their physical properties via their mid-/far-infrared line emission. We present updated predictions for the number counts and the redshift distributions of star forming galaxies spectroscopically de"},"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":"1312.1891","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2013-12-06T15:28:11Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"7531499c8f47c01dc355eb1fd9f6091bfd787be604ab3a33c681bf97b81c9e7e","abstract_canon_sha256":"74931cf6a07e8cd8ba891422f89172a561c1a1b2c0b9b02ee589892a4e9be3a2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:45:57.839119Z","signature_b64":"yKEyKsl2BFENQUCuKaHGhsq2dyARomodG5KYf9sytVBvLRR79DVQZyaMHmiCshP/fCX5/Rb25gG4WHXRTxIqBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bdf7dacb2a8ba55f2c00a54eba9eb57c52d175bb93648db47e65923738f2bb59","last_reissued_at":"2026-05-18T01:45:57.838569Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:45:57.838569Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Exploring the early dust-obscured phase of galaxy formation with blind mid-/far-IR spectroscopic surveys","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A. Bressan, A. Lapi, C. Gruppioni, G. de Zotti, L. Danese, L. Spinoglio, M. Bonato, M. Negrello, Z.-Y. Cai","submitted_at":"2013-12-06T15:28:11Z","abstract_excerpt":"While continuum imaging data at far-infrared to sub-millimeter wavelengths have provided tight constraints on the population properties of dusty star forming galaxies up to high redshifts, future space missions like the Space Infra-Red Telescope for Cosmology and Astrophysics (SPICA) and ground based facilities like the Cerro Chajnantor Atacama Telescope (CCAT) will allow detailed investigations of their physical properties via their mid-/far-infrared line emission. We present updated predictions for the number counts and the redshift distributions of star forming galaxies spectroscopically de"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1312.1891","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":"1312.1891","created_at":"2026-05-18T01:45:57.838671+00:00"},{"alias_kind":"arxiv_version","alias_value":"1312.1891v1","created_at":"2026-05-18T01:45:57.838671+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1312.1891","created_at":"2026-05-18T01:45:57.838671+00:00"},{"alias_kind":"pith_short_12","alias_value":"XX35VSZKROSV","created_at":"2026-05-18T12:28:06.772260+00:00"},{"alias_kind":"pith_short_16","alias_value":"XX35VSZKROSV6LAA","created_at":"2026-05-18T12:28:06.772260+00:00"},{"alias_kind":"pith_short_8","alias_value":"XX35VSZK","created_at":"2026-05-18T12:28:06.772260+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/XX35VSZKROSV6LAAUVHLVHVVPR","json":"https://pith.science/pith/XX35VSZKROSV6LAAUVHLVHVVPR.json","graph_json":"https://pith.science/api/pith-number/XX35VSZKROSV6LAAUVHLVHVVPR/graph.json","events_json":"https://pith.science/api/pith-number/XX35VSZKROSV6LAAUVHLVHVVPR/events.json","paper":"https://pith.science/paper/XX35VSZK"},"agent_actions":{"view_html":"https://pith.science/pith/XX35VSZKROSV6LAAUVHLVHVVPR","download_json":"https://pith.science/pith/XX35VSZKROSV6LAAUVHLVHVVPR.json","view_paper":"https://pith.science/paper/XX35VSZK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1312.1891&json=true","fetch_graph":"https://pith.science/api/pith-number/XX35VSZKROSV6LAAUVHLVHVVPR/graph.json","fetch_events":"https://pith.science/api/pith-number/XX35VSZKROSV6LAAUVHLVHVVPR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XX35VSZKROSV6LAAUVHLVHVVPR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XX35VSZKROSV6LAAUVHLVHVVPR/action/storage_attestation","attest_author":"https://pith.science/pith/XX35VSZKROSV6LAAUVHLVHVVPR/action/author_attestation","sign_citation":"https://pith.science/pith/XX35VSZKROSV6LAAUVHLVHVVPR/action/citation_signature","submit_replication":"https://pith.science/pith/XX35VSZKROSV6LAAUVHLVHVVPR/action/replication_record"}},"created_at":"2026-05-18T01:45:57.838671+00:00","updated_at":"2026-05-18T01:45:57.838671+00:00"}