{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:KAUF5WVIWJ7BXLDV7U7XKDCTUB","short_pith_number":"pith:KAUF5WVI","schema_version":"1.0","canonical_sha256":"50285edaa8b27e1bac75fd3f750c53a05fd405b2a4693c6168eac58341f35c16","source":{"kind":"arxiv","id":"1403.7974","version":1},"attestation_state":"computed","paper":{"title":"Probing obscured, high redshift galaxies using deep P-band continuum imaging with GMRT","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Alain Omont, Alexandre Beelen, C. H. Ishwara-Chandra, Sandeep Sirothia, Veeresh Singh, Yogesh Wadadekar","submitted_at":"2014-03-31T12:50:05Z","abstract_excerpt":"We have carried out a deep (150 micro Jy rms) P-band, continuum imaging survey of about 40 square degrees of sky in the XMM-LSS, Lockman Hole and ELAIS-N1 fields with the GMRT. Our deep radio data, combined with deep archival observations in the X-ray (XMM/Chandra), optical (SDSS, CFHTLS), near-infrared (UKIDSS, VISTA/VIDEO), mid-infrared (Spitzer/SWIRE, Spitzer/SERVS) and far-infrared (Spitzer/SWIRE, Herschel/HerMES) will enable us to obtain an accurate census of star-forming and active galaxies out to z~2. This panchromatic coverage enables accurate determination of photometric redshifts and"},"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":"1403.7974","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-03-31T12:50:05Z","cross_cats_sorted":[],"title_canon_sha256":"e6e70c907ee55495d5b6ec5811bdada7d07610ba8a3aae81371e74f234628599","abstract_canon_sha256":"6ddd14a98b3d361f5d77080162c42963a8eed0a730d57b6569ef415a650b85e3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:55:12.046070Z","signature_b64":"F7D/m0ZXfCJVsaXlE6PN4IE8kQy9bLOE5TVvCOQauqsEI284EKhSSsG6rouXiwngQRza5+52oob8FaMxzv04Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"50285edaa8b27e1bac75fd3f750c53a05fd405b2a4693c6168eac58341f35c16","last_reissued_at":"2026-05-18T02:55:12.045699Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:55:12.045699Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Probing obscured, high redshift galaxies using deep P-band continuum imaging with GMRT","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Alain Omont, Alexandre Beelen, C. H. Ishwara-Chandra, Sandeep Sirothia, Veeresh Singh, Yogesh Wadadekar","submitted_at":"2014-03-31T12:50:05Z","abstract_excerpt":"We have carried out a deep (150 micro Jy rms) P-band, continuum imaging survey of about 40 square degrees of sky in the XMM-LSS, Lockman Hole and ELAIS-N1 fields with the GMRT. Our deep radio data, combined with deep archival observations in the X-ray (XMM/Chandra), optical (SDSS, CFHTLS), near-infrared (UKIDSS, VISTA/VIDEO), mid-infrared (Spitzer/SWIRE, Spitzer/SERVS) and far-infrared (Spitzer/SWIRE, Herschel/HerMES) will enable us to obtain an accurate census of star-forming and active galaxies out to z~2. This panchromatic coverage enables accurate determination of photometric redshifts and"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1403.7974","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":"1403.7974","created_at":"2026-05-18T02:55:12.045755+00:00"},{"alias_kind":"arxiv_version","alias_value":"1403.7974v1","created_at":"2026-05-18T02:55:12.045755+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1403.7974","created_at":"2026-05-18T02:55:12.045755+00:00"},{"alias_kind":"pith_short_12","alias_value":"KAUF5WVIWJ7B","created_at":"2026-05-18T12:28:35.611951+00:00"},{"alias_kind":"pith_short_16","alias_value":"KAUF5WVIWJ7BXLDV","created_at":"2026-05-18T12:28:35.611951+00:00"},{"alias_kind":"pith_short_8","alias_value":"KAUF5WVI","created_at":"2026-05-18T12:28:35.611951+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/KAUF5WVIWJ7BXLDV7U7XKDCTUB","json":"https://pith.science/pith/KAUF5WVIWJ7BXLDV7U7XKDCTUB.json","graph_json":"https://pith.science/api/pith-number/KAUF5WVIWJ7BXLDV7U7XKDCTUB/graph.json","events_json":"https://pith.science/api/pith-number/KAUF5WVIWJ7BXLDV7U7XKDCTUB/events.json","paper":"https://pith.science/paper/KAUF5WVI"},"agent_actions":{"view_html":"https://pith.science/pith/KAUF5WVIWJ7BXLDV7U7XKDCTUB","download_json":"https://pith.science/pith/KAUF5WVIWJ7BXLDV7U7XKDCTUB.json","view_paper":"https://pith.science/paper/KAUF5WVI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1403.7974&json=true","fetch_graph":"https://pith.science/api/pith-number/KAUF5WVIWJ7BXLDV7U7XKDCTUB/graph.json","fetch_events":"https://pith.science/api/pith-number/KAUF5WVIWJ7BXLDV7U7XKDCTUB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KAUF5WVIWJ7BXLDV7U7XKDCTUB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KAUF5WVIWJ7BXLDV7U7XKDCTUB/action/storage_attestation","attest_author":"https://pith.science/pith/KAUF5WVIWJ7BXLDV7U7XKDCTUB/action/author_attestation","sign_citation":"https://pith.science/pith/KAUF5WVIWJ7BXLDV7U7XKDCTUB/action/citation_signature","submit_replication":"https://pith.science/pith/KAUF5WVIWJ7BXLDV7U7XKDCTUB/action/replication_record"}},"created_at":"2026-05-18T02:55:12.045755+00:00","updated_at":"2026-05-18T02:55:12.045755+00:00"}