{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:EIAUHKZ2AVNVCVIESZKOIQ5GZO","short_pith_number":"pith:EIAUHKZ2","schema_version":"1.0","canonical_sha256":"220143ab3a055b5155049654e443a6cbaf3532b2a51069d5db27bfd1a82433cb","source":{"kind":"arxiv","id":"1508.02294","version":1},"attestation_state":"computed","paper":{"title":"The Mid-Infrared Instrument for the James Webb Space Telescope I: Introduction","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Alistair Glasse, C. Waelkens, E. G. van Dishoeck, G. H. Rieke, G. S. Wright, H.-U. Norgaard-Nielsen, J. Bouwman, K. D. Gordon, K. Justtanont, L. Colina, Manual Guedel, M. E. Meixner, M. E. Ressler, P.-O. Lagage, T. Boeker, Th. Henning, T. P. Greene, T. P. Ray","submitted_at":"2015-08-10T15:46:11Z","abstract_excerpt":"MIRI (the Mid-Infrared Instrument for the James Webb Space Telescope (JWST)) operates from 5 to 28.5 microns and combines over this range: 1.) unprecedented sensitivity levels; 2.) sub-arcsec angular resolution; 3.) freedom from atmospheric interference; 4.) the inherent stability of observing in space; and 5.) a suite of versatile capabilities including imaging, low and medium resolution spectroscopy (with an integral field unit), and coronagraphy. We illustrate the potential uses of this unique combination of capabilities with various science examples: 1.) imaging exoplanets; 2.) transit and"},"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":"1508.02294","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2015-08-10T15:46:11Z","cross_cats_sorted":[],"title_canon_sha256":"99bf45330c3623e88b8459ff392b9c233b15309a2c34f26100d0d62f2be742eb","abstract_canon_sha256":"856952e95b80ed1d5f43105b5dbb54d6be20c16f787ed68081e7fd6204870e71"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:35:06.430757Z","signature_b64":"gRKXg0Gx53Ld9G0lLnHv3mHABPfDtIaz/jZZsQfWnakYALcIZbf4TIkpoHKUk57FXxn+IFIDmLSIj2Ecg48jBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"220143ab3a055b5155049654e443a6cbaf3532b2a51069d5db27bfd1a82433cb","last_reissued_at":"2026-05-18T01:35:06.430061Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:35:06.430061Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Mid-Infrared Instrument for the James Webb Space Telescope I: Introduction","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Alistair Glasse, C. Waelkens, E. G. van Dishoeck, G. H. Rieke, G. S. Wright, H.-U. Norgaard-Nielsen, J. Bouwman, K. D. Gordon, K. Justtanont, L. Colina, Manual Guedel, M. E. Meixner, M. E. Ressler, P.-O. Lagage, T. Boeker, Th. Henning, T. P. Greene, T. P. Ray","submitted_at":"2015-08-10T15:46:11Z","abstract_excerpt":"MIRI (the Mid-Infrared Instrument for the James Webb Space Telescope (JWST)) operates from 5 to 28.5 microns and combines over this range: 1.) unprecedented sensitivity levels; 2.) sub-arcsec angular resolution; 3.) freedom from atmospheric interference; 4.) the inherent stability of observing in space; and 5.) a suite of versatile capabilities including imaging, low and medium resolution spectroscopy (with an integral field unit), and coronagraphy. We illustrate the potential uses of this unique combination of capabilities with various science examples: 1.) imaging exoplanets; 2.) transit and"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1508.02294","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":"1508.02294","created_at":"2026-05-18T01:35:06.430179+00:00"},{"alias_kind":"arxiv_version","alias_value":"1508.02294v1","created_at":"2026-05-18T01:35:06.430179+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1508.02294","created_at":"2026-05-18T01:35:06.430179+00:00"},{"alias_kind":"pith_short_12","alias_value":"EIAUHKZ2AVNV","created_at":"2026-05-18T12:29:19.899920+00:00"},{"alias_kind":"pith_short_16","alias_value":"EIAUHKZ2AVNVCVIE","created_at":"2026-05-18T12:29:19.899920+00:00"},{"alias_kind":"pith_short_8","alias_value":"EIAUHKZ2","created_at":"2026-05-18T12:29:19.899920+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/EIAUHKZ2AVNVCVIESZKOIQ5GZO","json":"https://pith.science/pith/EIAUHKZ2AVNVCVIESZKOIQ5GZO.json","graph_json":"https://pith.science/api/pith-number/EIAUHKZ2AVNVCVIESZKOIQ5GZO/graph.json","events_json":"https://pith.science/api/pith-number/EIAUHKZ2AVNVCVIESZKOIQ5GZO/events.json","paper":"https://pith.science/paper/EIAUHKZ2"},"agent_actions":{"view_html":"https://pith.science/pith/EIAUHKZ2AVNVCVIESZKOIQ5GZO","download_json":"https://pith.science/pith/EIAUHKZ2AVNVCVIESZKOIQ5GZO.json","view_paper":"https://pith.science/paper/EIAUHKZ2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1508.02294&json=true","fetch_graph":"https://pith.science/api/pith-number/EIAUHKZ2AVNVCVIESZKOIQ5GZO/graph.json","fetch_events":"https://pith.science/api/pith-number/EIAUHKZ2AVNVCVIESZKOIQ5GZO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EIAUHKZ2AVNVCVIESZKOIQ5GZO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EIAUHKZ2AVNVCVIESZKOIQ5GZO/action/storage_attestation","attest_author":"https://pith.science/pith/EIAUHKZ2AVNVCVIESZKOIQ5GZO/action/author_attestation","sign_citation":"https://pith.science/pith/EIAUHKZ2AVNVCVIESZKOIQ5GZO/action/citation_signature","submit_replication":"https://pith.science/pith/EIAUHKZ2AVNVCVIESZKOIQ5GZO/action/replication_record"}},"created_at":"2026-05-18T01:35:06.430179+00:00","updated_at":"2026-05-18T01:35:06.430179+00:00"}