{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2005:MNBBCDDDLL25VGVPNGOTAANWNA","short_pith_number":"pith:MNBBCDDD","schema_version":"1.0","canonical_sha256":"6342110c635af5da9aaf699d3001b6680afd84c9082ccbf2361d407164ef5316","source":{"kind":"arxiv","id":"astro-ph/0507413","version":1},"attestation_state":"computed","paper":{"title":"The Swift Ultra-Violet/Optical Telescope","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. A. Breeveld, B. K. Hancock, H. E. Huckle, H. Kawakami, J. A. Nousek, J. C. Soto, J. Stock, K. O. Mason, K. Smith, L. Ahr, M. D. Still, M. Ivanushkina, M. J. Carter, M. K. McLelland, M. S. Pryzby, P. J. Smith, P. S. Broos, P. T. Boyd, P. W. A. Roming, R. E. Bingham, R. Killough, S. D. Hunsberger, S. T. Holland, T. E. Kennedy, T. S. Koch","submitted_at":"2005-07-18T17:43:22Z","abstract_excerpt":"The UV/Optical Telescope (UVOT) is one of three instruments flying aboard the Swift Gamma-ray Observatory. It is designed to capture the early (approximately 1 minute) UV and optical photons from the afterglow of gamma-ray bursts in the 170-600 nm band as well as long term observations of these afterglows. This is accomplished through the use of UV and optical broadband filters and grisms. The UVOT has a modified Ritchey-Chretien design with micro-channel plate intensified charged-coupled device detectors that record the arrival time of individual photons and provide sub-arcsecond positioning "},"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":"astro-ph/0507413","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2005-07-18T17:43:22Z","cross_cats_sorted":[],"title_canon_sha256":"04d4f25ea89f8bdfe1a7b7f5356e41a7fbb5577c034c05cb668d48b0d75691c4","abstract_canon_sha256":"46ad6d955e2dff1506d7dcbef81d102988263a4db4d3d28d00ab871ae7901eb0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:18:14.341605Z","signature_b64":"27vSavgw0a2ReBym5zftjztOYbi8aII7B2UVRjuqHGA7FkNSgUL2xFLv/HCRVBZWxcXMQGfhwrIoMU8vh4PZDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6342110c635af5da9aaf699d3001b6680afd84c9082ccbf2361d407164ef5316","last_reissued_at":"2026-05-18T04:18:14.340999Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:18:14.340999Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Swift Ultra-Violet/Optical Telescope","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. A. Breeveld, B. K. Hancock, H. E. Huckle, H. Kawakami, J. A. Nousek, J. C. Soto, J. Stock, K. O. Mason, K. Smith, L. Ahr, M. D. Still, M. Ivanushkina, M. J. Carter, M. K. McLelland, M. S. Pryzby, P. J. Smith, P. S. Broos, P. T. Boyd, P. W. A. Roming, R. E. Bingham, R. Killough, S. D. Hunsberger, S. T. Holland, T. E. Kennedy, T. S. Koch","submitted_at":"2005-07-18T17:43:22Z","abstract_excerpt":"The UV/Optical Telescope (UVOT) is one of three instruments flying aboard the Swift Gamma-ray Observatory. It is designed to capture the early (approximately 1 minute) UV and optical photons from the afterglow of gamma-ray bursts in the 170-600 nm band as well as long term observations of these afterglows. This is accomplished through the use of UV and optical broadband filters and grisms. The UVOT has a modified Ritchey-Chretien design with micro-channel plate intensified charged-coupled device detectors that record the arrival time of individual photons and provide sub-arcsecond positioning "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0507413","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":"astro-ph/0507413","created_at":"2026-05-18T04:18:14.341113+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0507413v1","created_at":"2026-05-18T04:18:14.341113+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0507413","created_at":"2026-05-18T04:18:14.341113+00:00"},{"alias_kind":"pith_short_12","alias_value":"MNBBCDDDLL25","created_at":"2026-05-18T12:25:53.335082+00:00"},{"alias_kind":"pith_short_16","alias_value":"MNBBCDDDLL25VGVP","created_at":"2026-05-18T12:25:53.335082+00:00"},{"alias_kind":"pith_short_8","alias_value":"MNBBCDDD","created_at":"2026-05-18T12:25:53.335082+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":17,"internal_anchor_count":5,"sample":[{"citing_arxiv_id":"2412.20091","citing_title":"Gamma-Ray Burst Light Curve Reconstruction: A Comparative Machine and Deep Learning Analysis","ref_index":81,"is_internal_anchor":true},{"citing_arxiv_id":"2605.18958","citing_title":"Directly tracking the re-brightening of a supermassive black hole accretion disk","ref_index":39,"is_internal_anchor":true},{"citing_arxiv_id":"2512.10239","citing_title":"EP250827b/SN 2025wkm: An X-ray Flash-Supernova Powered by a Central Engine and Circumstellar Interaction","ref_index":199,"is_internal_anchor":true},{"citing_arxiv_id":"2602.05404","citing_title":"The Double-Burst Nature and Early Afterglow Evolution of Long GRB 110801A","ref_index":42,"is_internal_anchor":true},{"citing_arxiv_id":"2602.06407","citing_title":"Primordial Black Hole signatures from femtolensing and spectral fringe of Gamma Ray Bursts","ref_index":42,"is_internal_anchor":true},{"citing_arxiv_id":"2603.25331","citing_title":"Jet Power Estimates of FSRQs PKS 1441+25 and Ton 599 from Broadband SED Modeling","ref_index":42,"is_internal_anchor":false},{"citing_arxiv_id":"2603.28699","citing_title":"An Intertwined Short and Long GRB with 4-minute Separation","ref_index":28,"is_internal_anchor":false},{"citing_arxiv_id":"2605.10423","citing_title":"SAPLE: Swift Analysis Pipeline for Lightcurve Extraction","ref_index":20,"is_internal_anchor":false},{"citing_arxiv_id":"2604.13650","citing_title":"Prospects for GRB Afterglow Discovery with the Eric and Wendy Schmidt Observatory System","ref_index":97,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14343","citing_title":"GRB 210704A: A Luminous Fast Blue Transient in a GRB Afterglow at $z = 2.34$","ref_index":119,"is_internal_anchor":false},{"citing_arxiv_id":"2604.16093","citing_title":"JWST and Keck observations of the off-nuclear tidal disruption event TDE 2025abcr: An evolving reprocessing layer","ref_index":92,"is_internal_anchor":false},{"citing_arxiv_id":"2604.19435","citing_title":"SDSSJ110546.07+145202.4: The first long-duration radio changing-look NLS1 galaxy","ref_index":125,"is_internal_anchor":false},{"citing_arxiv_id":"2604.19674","citing_title":"Resolved UV-Optical HST Imaging and Spectral Energy Distribution Modeling of Nearby BAT Active Galactic Nuclei","ref_index":51,"is_internal_anchor":false},{"citing_arxiv_id":"2604.20480","citing_title":"The January 2010 flare of Mrk421: Insights from a stochastic acceleration model","ref_index":60,"is_internal_anchor":false},{"citing_arxiv_id":"2605.05303","citing_title":"Multi-wavelength outburst activity from EP J174942.2-384834: a very faint X-ray transient discovered by Einstein Probe","ref_index":123,"is_internal_anchor":false},{"citing_arxiv_id":"2605.05380","citing_title":"The Eye of Sauron in SN 2025ngs: a Short-plateau Cousin of SN 1998S with Evidence for a Ring-like Circumstellar Medium","ref_index":119,"is_internal_anchor":false},{"citing_arxiv_id":"2605.04818","citing_title":"AGILE detection of transient {\\gamma}-ray emission from the region of the supergiant fast X-ray transient source IGR J17354-3255","ref_index":76,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/MNBBCDDDLL25VGVPNGOTAANWNA","json":"https://pith.science/pith/MNBBCDDDLL25VGVPNGOTAANWNA.json","graph_json":"https://pith.science/api/pith-number/MNBBCDDDLL25VGVPNGOTAANWNA/graph.json","events_json":"https://pith.science/api/pith-number/MNBBCDDDLL25VGVPNGOTAANWNA/events.json","paper":"https://pith.science/paper/MNBBCDDD"},"agent_actions":{"view_html":"https://pith.science/pith/MNBBCDDDLL25VGVPNGOTAANWNA","download_json":"https://pith.science/pith/MNBBCDDDLL25VGVPNGOTAANWNA.json","view_paper":"https://pith.science/paper/MNBBCDDD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0507413&json=true","fetch_graph":"https://pith.science/api/pith-number/MNBBCDDDLL25VGVPNGOTAANWNA/graph.json","fetch_events":"https://pith.science/api/pith-number/MNBBCDDDLL25VGVPNGOTAANWNA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MNBBCDDDLL25VGVPNGOTAANWNA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MNBBCDDDLL25VGVPNGOTAANWNA/action/storage_attestation","attest_author":"https://pith.science/pith/MNBBCDDDLL25VGVPNGOTAANWNA/action/author_attestation","sign_citation":"https://pith.science/pith/MNBBCDDDLL25VGVPNGOTAANWNA/action/citation_signature","submit_replication":"https://pith.science/pith/MNBBCDDDLL25VGVPNGOTAANWNA/action/replication_record"}},"created_at":"2026-05-18T04:18:14.341113+00:00","updated_at":"2026-05-18T04:18:14.341113+00:00"}