{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:OX3FK557UZ2SEI4IIWODZXNF6H","short_pith_number":"pith:OX3FK557","schema_version":"1.0","canonical_sha256":"75f65577bfa675222388459c3cdda5f1d512c986d210855ee77b99d30c261761","source":{"kind":"arxiv","id":"1012.5827","version":1},"attestation_state":"computed","paper":{"title":"The Cosmic Origins Spectrograph: On-Orbit Instrument Performance","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"A. Aloisi, C. Biagetti, C. Froning, C. Keyes, C. Oliveira, C. Proffitt, D. Ebbets, D. Lennon, D. Massa, D. Sahnow, D. Soderblom, E. Burgh, E. Wilkinson, G. Hartig, J. Andrews, J. Bacinski, J. Green, J. McPhate, K. France, O. Siegmund, P. Ghavamian, P. Goudfrooij, R. Diaz, R. Kimble, R. Osten, S. B\\'eland, S. Friedman, S. Niemi, S. Osterman, S.Penton, T. Ake, T. Delker, T. Smith, W. Dixon","submitted_at":"2010-12-28T19:46:09Z","abstract_excerpt":"The Cosmic Origins Spectrograph (COS) was installed in the Hubble Space Telescope in May, 2009 as part of Servicing Mission 4 to provide high sensitivity, medium and low resolution spectroscopy at far- and near-ultraviolet wavelengths (FUV, NUV). COS is the most sensitive FUV/NUV spectrograph flown to date, spanning the wavelength range from 900{\\AA} to 3200{\\AA} with peak effective area approaching 3000 cm^2. This paper describes instrument design, the results of the Servicing Mission Orbital Verification (SMOV), and the ongoing performance monitoring program."},"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":"1012.5827","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2010-12-28T19:46:09Z","cross_cats_sorted":[],"title_canon_sha256":"2b4aea86a51caf281a05a3f3c7c054cb6ae97973fdd3bc8f9cae5ba05888caff","abstract_canon_sha256":"ef33957c2ca3865c26ee51253525b8c26dad70b649dca62a785070318bd75059"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:04:17.058696Z","signature_b64":"6nK7uP0qf5QxTKWl6/HLDWG3BqIyab1Y3XddrI41JcKngJedWHMxR8szpc0hjIM57FUOHn7Ln9gO7UL+pWTkBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"75f65577bfa675222388459c3cdda5f1d512c986d210855ee77b99d30c261761","last_reissued_at":"2026-05-18T02:04:17.057928Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:04:17.057928Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Cosmic Origins Spectrograph: On-Orbit Instrument Performance","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"A. Aloisi, C. Biagetti, C. Froning, C. Keyes, C. Oliveira, C. Proffitt, D. Ebbets, D. Lennon, D. Massa, D. Sahnow, D. Soderblom, E. Burgh, E. Wilkinson, G. Hartig, J. Andrews, J. Bacinski, J. Green, J. McPhate, K. France, O. Siegmund, P. Ghavamian, P. Goudfrooij, R. Diaz, R. Kimble, R. Osten, S. B\\'eland, S. Friedman, S. Niemi, S. Osterman, S.Penton, T. Ake, T. Delker, T. Smith, W. Dixon","submitted_at":"2010-12-28T19:46:09Z","abstract_excerpt":"The Cosmic Origins Spectrograph (COS) was installed in the Hubble Space Telescope in May, 2009 as part of Servicing Mission 4 to provide high sensitivity, medium and low resolution spectroscopy at far- and near-ultraviolet wavelengths (FUV, NUV). COS is the most sensitive FUV/NUV spectrograph flown to date, spanning the wavelength range from 900{\\AA} to 3200{\\AA} with peak effective area approaching 3000 cm^2. This paper describes instrument design, the results of the Servicing Mission Orbital Verification (SMOV), and the ongoing performance monitoring program."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1012.5827","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":"1012.5827","created_at":"2026-05-18T02:04:17.058063+00:00"},{"alias_kind":"arxiv_version","alias_value":"1012.5827v1","created_at":"2026-05-18T02:04:17.058063+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1012.5827","created_at":"2026-05-18T02:04:17.058063+00:00"},{"alias_kind":"pith_short_12","alias_value":"OX3FK557UZ2S","created_at":"2026-05-18T12:26:12.377268+00:00"},{"alias_kind":"pith_short_16","alias_value":"OX3FK557UZ2SEI4I","created_at":"2026-05-18T12:26:12.377268+00:00"},{"alias_kind":"pith_short_8","alias_value":"OX3FK557","created_at":"2026-05-18T12:26:12.377268+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/OX3FK557UZ2SEI4IIWODZXNF6H","json":"https://pith.science/pith/OX3FK557UZ2SEI4IIWODZXNF6H.json","graph_json":"https://pith.science/api/pith-number/OX3FK557UZ2SEI4IIWODZXNF6H/graph.json","events_json":"https://pith.science/api/pith-number/OX3FK557UZ2SEI4IIWODZXNF6H/events.json","paper":"https://pith.science/paper/OX3FK557"},"agent_actions":{"view_html":"https://pith.science/pith/OX3FK557UZ2SEI4IIWODZXNF6H","download_json":"https://pith.science/pith/OX3FK557UZ2SEI4IIWODZXNF6H.json","view_paper":"https://pith.science/paper/OX3FK557","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1012.5827&json=true","fetch_graph":"https://pith.science/api/pith-number/OX3FK557UZ2SEI4IIWODZXNF6H/graph.json","fetch_events":"https://pith.science/api/pith-number/OX3FK557UZ2SEI4IIWODZXNF6H/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OX3FK557UZ2SEI4IIWODZXNF6H/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OX3FK557UZ2SEI4IIWODZXNF6H/action/storage_attestation","attest_author":"https://pith.science/pith/OX3FK557UZ2SEI4IIWODZXNF6H/action/author_attestation","sign_citation":"https://pith.science/pith/OX3FK557UZ2SEI4IIWODZXNF6H/action/citation_signature","submit_replication":"https://pith.science/pith/OX3FK557UZ2SEI4IIWODZXNF6H/action/replication_record"}},"created_at":"2026-05-18T02:04:17.058063+00:00","updated_at":"2026-05-18T02:04:17.058063+00:00"}