{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:SICCD3JKZ4VG65VAUNLHXRRSDH","short_pith_number":"pith:SICCD3JK","schema_version":"1.0","canonical_sha256":"920421ed2acf2a6f76a0a3567bc63219f572aa80d844bdf6fa0f7ac707883fb7","source":{"kind":"arxiv","id":"1305.0262","version":3},"attestation_state":"computed","paper":{"title":"On-sky characterisation of the VISTA NB118 narrow-band filters at 1.19 micron","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.GA"],"primary_cat":"astro-ph.IM","authors_text":"B. Milvang-Jensen, D. Sobral, H. Joy McCracken, J. Hjorth, J. P. U. Fynbo, J. S. Dunlop, J. Zabl, K. K. Nilsson, L. Tasca, O. Le Fevre, P. Moller, W. Freudling","submitted_at":"2013-05-01T20:00:01Z","abstract_excerpt":"Observations of the high redshift Universe through narrow-band filters have proven very successful in the last decade. The 4-meter VISTA telescope, equipped with the wide-field camera VIRCAM, offers a major step forward in wide-field near-infrared imaging, and in order to utilise VISTA's large field-of-view and sensitivity, the Dark Cosmology Centre provided a set of 16 narrow-band filters for VIRCAM. These NB118 filters are centered at a wavelength near 1.19 micron in a region with few airglow emission lines. The filters allow the detection of Halpha emitters at z = 0.8, Hbeta and [OIII] emit"},"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":"1305.0262","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2013-05-01T20:00:01Z","cross_cats_sorted":["astro-ph.CO","astro-ph.GA"],"title_canon_sha256":"3b65026ac8351d5c16321f411bfcad8c636d4bd3af9de5622d5dc90468d52ca6","abstract_canon_sha256":"952cb7ec683a83e0f17d45cbbd60aabe5473b5e0b5f41c195c664912fcaf9628"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:06:22.064827Z","signature_b64":"6ApDzbtXjAyGMl1G4otX0ELzP0+u/tmnVGfyHvgmC+r7zo6DU4VswhN4nTouB8k03uK+UCjliFDASNloCKO3AQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"920421ed2acf2a6f76a0a3567bc63219f572aa80d844bdf6fa0f7ac707883fb7","last_reissued_at":"2026-05-18T03:06:22.064286Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:06:22.064286Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On-sky characterisation of the VISTA NB118 narrow-band filters at 1.19 micron","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.GA"],"primary_cat":"astro-ph.IM","authors_text":"B. Milvang-Jensen, D. Sobral, H. Joy McCracken, J. Hjorth, J. P. U. Fynbo, J. S. Dunlop, J. Zabl, K. K. Nilsson, L. Tasca, O. Le Fevre, P. Moller, W. Freudling","submitted_at":"2013-05-01T20:00:01Z","abstract_excerpt":"Observations of the high redshift Universe through narrow-band filters have proven very successful in the last decade. The 4-meter VISTA telescope, equipped with the wide-field camera VIRCAM, offers a major step forward in wide-field near-infrared imaging, and in order to utilise VISTA's large field-of-view and sensitivity, the Dark Cosmology Centre provided a set of 16 narrow-band filters for VIRCAM. These NB118 filters are centered at a wavelength near 1.19 micron in a region with few airglow emission lines. The filters allow the detection of Halpha emitters at z = 0.8, Hbeta and [OIII] emit"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1305.0262","kind":"arxiv","version":3},"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":"1305.0262","created_at":"2026-05-18T03:06:22.064376+00:00"},{"alias_kind":"arxiv_version","alias_value":"1305.0262v3","created_at":"2026-05-18T03:06:22.064376+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1305.0262","created_at":"2026-05-18T03:06:22.064376+00:00"},{"alias_kind":"pith_short_12","alias_value":"SICCD3JKZ4VG","created_at":"2026-05-18T12:27:59.945178+00:00"},{"alias_kind":"pith_short_16","alias_value":"SICCD3JKZ4VG65VA","created_at":"2026-05-18T12:27:59.945178+00:00"},{"alias_kind":"pith_short_8","alias_value":"SICCD3JK","created_at":"2026-05-18T12:27:59.945178+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/SICCD3JKZ4VG65VAUNLHXRRSDH","json":"https://pith.science/pith/SICCD3JKZ4VG65VAUNLHXRRSDH.json","graph_json":"https://pith.science/api/pith-number/SICCD3JKZ4VG65VAUNLHXRRSDH/graph.json","events_json":"https://pith.science/api/pith-number/SICCD3JKZ4VG65VAUNLHXRRSDH/events.json","paper":"https://pith.science/paper/SICCD3JK"},"agent_actions":{"view_html":"https://pith.science/pith/SICCD3JKZ4VG65VAUNLHXRRSDH","download_json":"https://pith.science/pith/SICCD3JKZ4VG65VAUNLHXRRSDH.json","view_paper":"https://pith.science/paper/SICCD3JK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1305.0262&json=true","fetch_graph":"https://pith.science/api/pith-number/SICCD3JKZ4VG65VAUNLHXRRSDH/graph.json","fetch_events":"https://pith.science/api/pith-number/SICCD3JKZ4VG65VAUNLHXRRSDH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SICCD3JKZ4VG65VAUNLHXRRSDH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SICCD3JKZ4VG65VAUNLHXRRSDH/action/storage_attestation","attest_author":"https://pith.science/pith/SICCD3JKZ4VG65VAUNLHXRRSDH/action/author_attestation","sign_citation":"https://pith.science/pith/SICCD3JKZ4VG65VAUNLHXRRSDH/action/citation_signature","submit_replication":"https://pith.science/pith/SICCD3JKZ4VG65VAUNLHXRRSDH/action/replication_record"}},"created_at":"2026-05-18T03:06:22.064376+00:00","updated_at":"2026-05-18T03:06:22.064376+00:00"}