{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2001:T2CQ44WO2FA3463M7MUGIL4472","short_pith_number":"pith:T2CQ44WO","schema_version":"1.0","canonical_sha256":"9e850e72ced141be7b6cfb28642f9cfeaef7216741353e455e7fb2ced5e13fd1","source":{"kind":"arxiv","id":"astro-ph/0110007","version":2},"attestation_state":"computed","paper":{"title":"Strategies for prompt searches for GRB afterglows: the discovery of the GRB 001011 optical/near-infrared counterpart using colour-colour selection","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Fruchter, A.J. Castro-Tirado, B.L. Jensen, C. Kouveliotou, C. Wolf, E. Palazzi, E. Pian, E. Rol, E. van den Heuvel, F. Frontera, G. Mallen-Ornelas, H. Pedersen, I. Salamanca, J. Afonso, J. Gorosabel, J. Greiner, J. Hjorth, J.U. Fynbo, L. Christensen, L. Kaper, M.A. Treyer, M.I. Andersen, N. Masetti, N. Tanvir, P. Moller, P.M. Vreeswijk, R.A.M.J. Wijers, S. Klose","submitted_at":"2001-09-29T17:25:47Z","abstract_excerpt":"We report the discovery of the optical and near-infrared counterparts to GRB 001011. The GRB 001011 error box determined by Beppo-SAX was simultaneously imaged in the near-infrared by the 3.58-m New Technology Telescope and in the optical by the 1.54-m Danish Telescope ~8 hr after the gamma-ray event. Here we implement the colour-colour discrimination technique proposed by Rhoads (2001) and extend it using near-IR data as well. We present the results provided by an automatic colour-colour discrimination pipe-line developed to discern the different populations of objects present in the GRB 0010"},"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/0110007","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2001-09-29T17:25:47Z","cross_cats_sorted":[],"title_canon_sha256":"b029df35b46ba4b9b90b4c442c5d3a1ce6c168cfdaa39f485f65397aed1d1fb0","abstract_canon_sha256":"ca9eaf093b41a5ae2d85a455641d3ab3135abb1fe9f154a110e579ec82d341bd"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T14:11:31.679168Z","signature_b64":"S/NHjo50Gz4AvUg8/UXHo/gsL+x15O6rt9M7ZmiWuVQRWDp/oxkvtqmx3EF3u9xh6eN5tt3D/mnGTYyH1NOnDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9e850e72ced141be7b6cfb28642f9cfeaef7216741353e455e7fb2ced5e13fd1","last_reissued_at":"2026-07-04T14:11:31.678663Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T14:11:31.678663Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Strategies for prompt searches for GRB afterglows: the discovery of the GRB 001011 optical/near-infrared counterpart using colour-colour selection","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Fruchter, A.J. Castro-Tirado, B.L. Jensen, C. Kouveliotou, C. Wolf, E. Palazzi, E. Pian, E. Rol, E. van den Heuvel, F. Frontera, G. Mallen-Ornelas, H. Pedersen, I. Salamanca, J. Afonso, J. Gorosabel, J. Greiner, J. Hjorth, J.U. Fynbo, L. Christensen, L. Kaper, M.A. Treyer, M.I. Andersen, N. Masetti, N. Tanvir, P. Moller, P.M. Vreeswijk, R.A.M.J. Wijers, S. Klose","submitted_at":"2001-09-29T17:25:47Z","abstract_excerpt":"We report the discovery of the optical and near-infrared counterparts to GRB 001011. The GRB 001011 error box determined by Beppo-SAX was simultaneously imaged in the near-infrared by the 3.58-m New Technology Telescope and in the optical by the 1.54-m Danish Telescope ~8 hr after the gamma-ray event. Here we implement the colour-colour discrimination technique proposed by Rhoads (2001) and extend it using near-IR data as well. We present the results provided by an automatic colour-colour discrimination pipe-line developed to discern the different populations of objects present in the GRB 0010"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0110007","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0110007/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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/0110007","created_at":"2026-07-04T14:11:31.678717+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0110007v2","created_at":"2026-07-04T14:11:31.678717+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0110007","created_at":"2026-07-04T14:11:31.678717+00:00"},{"alias_kind":"pith_short_12","alias_value":"T2CQ44WO2FA3","created_at":"2026-07-04T14:11:31.678717+00:00"},{"alias_kind":"pith_short_16","alias_value":"T2CQ44WO2FA3463M","created_at":"2026-07-04T14:11:31.678717+00:00"},{"alias_kind":"pith_short_8","alias_value":"T2CQ44WO","created_at":"2026-07-04T14:11:31.678717+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/T2CQ44WO2FA3463M7MUGIL4472","json":"https://pith.science/pith/T2CQ44WO2FA3463M7MUGIL4472.json","graph_json":"https://pith.science/api/pith-number/T2CQ44WO2FA3463M7MUGIL4472/graph.json","events_json":"https://pith.science/api/pith-number/T2CQ44WO2FA3463M7MUGIL4472/events.json","paper":"https://pith.science/paper/T2CQ44WO"},"agent_actions":{"view_html":"https://pith.science/pith/T2CQ44WO2FA3463M7MUGIL4472","download_json":"https://pith.science/pith/T2CQ44WO2FA3463M7MUGIL4472.json","view_paper":"https://pith.science/paper/T2CQ44WO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0110007&json=true","fetch_graph":"https://pith.science/api/pith-number/T2CQ44WO2FA3463M7MUGIL4472/graph.json","fetch_events":"https://pith.science/api/pith-number/T2CQ44WO2FA3463M7MUGIL4472/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/T2CQ44WO2FA3463M7MUGIL4472/action/timestamp_anchor","attest_storage":"https://pith.science/pith/T2CQ44WO2FA3463M7MUGIL4472/action/storage_attestation","attest_author":"https://pith.science/pith/T2CQ44WO2FA3463M7MUGIL4472/action/author_attestation","sign_citation":"https://pith.science/pith/T2CQ44WO2FA3463M7MUGIL4472/action/citation_signature","submit_replication":"https://pith.science/pith/T2CQ44WO2FA3463M7MUGIL4472/action/replication_record"}},"created_at":"2026-07-04T14:11:31.678717+00:00","updated_at":"2026-07-04T14:11:31.678717+00:00"}