{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:3CHHNS7SERXZFRWYIBZVSMUSLA","short_pith_number":"pith:3CHHNS7S","schema_version":"1.0","canonical_sha256":"d88e76cbf2246f92c6d84073593292583f860036f168a4fc3ef3e25e5d6739a0","source":{"kind":"arxiv","id":"1507.05631","version":1},"attestation_state":"computed","paper":{"title":"The ARCONS Pipeline: Data Reduction for MKID Arrays","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"A. B. Walter, B. A. Mazin, C. Stoughton, D. Marsden, J. C. van Eyken, K. O'Brien, M. J. Strader, N. K. Rice, P. Szypryt, S. R. Meeker, Y. Lin","submitted_at":"2015-07-20T20:01:48Z","abstract_excerpt":"The Array Camera for Optical to Near-IR Spectrophotometry, or ARCONS, is a camera based on Microwave Kinetic Inductance Detectors (MKIDs), a new technology that has the potential for broad application in astronomy. Using an array of MKIDs, the instrument is able to produce time-resolved imaging and low-resolution spectroscopy constructed from detections of individual photons. The arrival time and energy of each photon are recorded in a manner similar to X-ray calorimetry, but at higher photon fluxes. The technique works over a very large wavelength range, is free from fundamental read noise an"},"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":"1507.05631","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2015-07-20T20:01:48Z","cross_cats_sorted":[],"title_canon_sha256":"d27d062ca640845924f2fa7bd95b2add62cdee92998d327cac78c0522bd86324","abstract_canon_sha256":"8b84423f23ca8c01f47bcc5f7bc87e1f46cb85469a6b24c40c2d769fa71656d4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:35:44.489677Z","signature_b64":"MYhY/ljRHthyGf7+9LcBZIFDCbb0V41mWA2xiX8Di6hiiQroa4OFe4IR5McGLZmXA8LF2vzNmdbmDTtlNd5eCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d88e76cbf2246f92c6d84073593292583f860036f168a4fc3ef3e25e5d6739a0","last_reissued_at":"2026-05-18T01:35:44.489261Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:35:44.489261Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The ARCONS Pipeline: Data Reduction for MKID Arrays","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"A. B. Walter, B. A. Mazin, C. Stoughton, D. Marsden, J. C. van Eyken, K. O'Brien, M. J. Strader, N. K. Rice, P. Szypryt, S. R. Meeker, Y. Lin","submitted_at":"2015-07-20T20:01:48Z","abstract_excerpt":"The Array Camera for Optical to Near-IR Spectrophotometry, or ARCONS, is a camera based on Microwave Kinetic Inductance Detectors (MKIDs), a new technology that has the potential for broad application in astronomy. Using an array of MKIDs, the instrument is able to produce time-resolved imaging and low-resolution spectroscopy constructed from detections of individual photons. The arrival time and energy of each photon are recorded in a manner similar to X-ray calorimetry, but at higher photon fluxes. The technique works over a very large wavelength range, is free from fundamental read noise an"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1507.05631","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":"1507.05631","created_at":"2026-05-18T01:35:44.489325+00:00"},{"alias_kind":"arxiv_version","alias_value":"1507.05631v1","created_at":"2026-05-18T01:35:44.489325+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1507.05631","created_at":"2026-05-18T01:35:44.489325+00:00"},{"alias_kind":"pith_short_12","alias_value":"3CHHNS7SERXZ","created_at":"2026-05-18T12:29:02.477457+00:00"},{"alias_kind":"pith_short_16","alias_value":"3CHHNS7SERXZFRWY","created_at":"2026-05-18T12:29:02.477457+00:00"},{"alias_kind":"pith_short_8","alias_value":"3CHHNS7S","created_at":"2026-05-18T12:29:02.477457+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/3CHHNS7SERXZFRWYIBZVSMUSLA","json":"https://pith.science/pith/3CHHNS7SERXZFRWYIBZVSMUSLA.json","graph_json":"https://pith.science/api/pith-number/3CHHNS7SERXZFRWYIBZVSMUSLA/graph.json","events_json":"https://pith.science/api/pith-number/3CHHNS7SERXZFRWYIBZVSMUSLA/events.json","paper":"https://pith.science/paper/3CHHNS7S"},"agent_actions":{"view_html":"https://pith.science/pith/3CHHNS7SERXZFRWYIBZVSMUSLA","download_json":"https://pith.science/pith/3CHHNS7SERXZFRWYIBZVSMUSLA.json","view_paper":"https://pith.science/paper/3CHHNS7S","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1507.05631&json=true","fetch_graph":"https://pith.science/api/pith-number/3CHHNS7SERXZFRWYIBZVSMUSLA/graph.json","fetch_events":"https://pith.science/api/pith-number/3CHHNS7SERXZFRWYIBZVSMUSLA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3CHHNS7SERXZFRWYIBZVSMUSLA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3CHHNS7SERXZFRWYIBZVSMUSLA/action/storage_attestation","attest_author":"https://pith.science/pith/3CHHNS7SERXZFRWYIBZVSMUSLA/action/author_attestation","sign_citation":"https://pith.science/pith/3CHHNS7SERXZFRWYIBZVSMUSLA/action/citation_signature","submit_replication":"https://pith.science/pith/3CHHNS7SERXZFRWYIBZVSMUSLA/action/replication_record"}},"created_at":"2026-05-18T01:35:44.489325+00:00","updated_at":"2026-05-18T01:35:44.489325+00:00"}