{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:JA3DTKHIOAOBJTT6JBFHYAWVIJ","short_pith_number":"pith:JA3DTKHI","schema_version":"1.0","canonical_sha256":"483639a8e8701c14ce7e484a7c02d54271ecaa6acdd10e3c4841921a0ffd4da1","source":{"kind":"arxiv","id":"1512.04690","version":1},"attestation_state":"computed","paper":{"title":"Probing the innermost regions of AGN jets and their magnetic fields with RadioAstron. I. Imaging BL Lacertae at 21 microarcsecond resolution","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Alan P. Marscher, Andrei P. Lobanov, Gabriele Bruni, James M. Anderson, Jos\\'e L. G\\'omez, Kirill V. Sokolovsky, Mikhail M. Lisakov, Nikolay S. Kardashev, Pablo Galindo, Svetlana G. Jorstad, Uwe Bach, Yosuke Mizuno, Yuri Y. Kovalev","submitted_at":"2015-12-15T09:33:08Z","abstract_excerpt":"We present the first polarimetric space VLBI imaging observations at 22 GHz. BL Lacertae was observed in 2013 November 10 with the RadioAstron space VLBI mission, including a ground array of 15 radio telescopes. The instrumental polarization of the space radio telescope is found to be within 9%, demonstrating the polarimetric imaging capabilities of RadioAstron at 22 GHz. Ground-space fringes were obtained up to a projected baseline distance of 7.9 Earth's diameters in length, allowing us to image the jet in BL Lacertae with a maximum angular resolution of 21 $\\mu$as, the highest achieved to d"},"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":"1512.04690","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2015-12-15T09:33:08Z","cross_cats_sorted":[],"title_canon_sha256":"b72605d92827aef14ab288ce223185a7047a6bc882b376e6b5bea2b8c8a78df4","abstract_canon_sha256":"e847ff3e2ad8e05d6e6dfc09fe4559d513670c5df0dd52abc45b0ee6d92aca14"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:22:00.065105Z","signature_b64":"9eWSfmWEA5pyphDYk9ePBlWDN1wtqJYFiidHb9vIE1iZczf7Hs1XG5exNA9CQd8kahoWh/lu1Ko7+nqmNwVPDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"483639a8e8701c14ce7e484a7c02d54271ecaa6acdd10e3c4841921a0ffd4da1","last_reissued_at":"2026-05-18T01:22:00.064653Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:22:00.064653Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Probing the innermost regions of AGN jets and their magnetic fields with RadioAstron. I. Imaging BL Lacertae at 21 microarcsecond resolution","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Alan P. Marscher, Andrei P. Lobanov, Gabriele Bruni, James M. Anderson, Jos\\'e L. G\\'omez, Kirill V. Sokolovsky, Mikhail M. Lisakov, Nikolay S. Kardashev, Pablo Galindo, Svetlana G. Jorstad, Uwe Bach, Yosuke Mizuno, Yuri Y. Kovalev","submitted_at":"2015-12-15T09:33:08Z","abstract_excerpt":"We present the first polarimetric space VLBI imaging observations at 22 GHz. BL Lacertae was observed in 2013 November 10 with the RadioAstron space VLBI mission, including a ground array of 15 radio telescopes. The instrumental polarization of the space radio telescope is found to be within 9%, demonstrating the polarimetric imaging capabilities of RadioAstron at 22 GHz. Ground-space fringes were obtained up to a projected baseline distance of 7.9 Earth's diameters in length, allowing us to image the jet in BL Lacertae with a maximum angular resolution of 21 $\\mu$as, the highest achieved to d"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1512.04690","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":"1512.04690","created_at":"2026-05-18T01:22:00.064723+00:00"},{"alias_kind":"arxiv_version","alias_value":"1512.04690v1","created_at":"2026-05-18T01:22:00.064723+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1512.04690","created_at":"2026-05-18T01:22:00.064723+00:00"},{"alias_kind":"pith_short_12","alias_value":"JA3DTKHIOAOB","created_at":"2026-05-18T12:29:27.538025+00:00"},{"alias_kind":"pith_short_16","alias_value":"JA3DTKHIOAOBJTT6","created_at":"2026-05-18T12:29:27.538025+00:00"},{"alias_kind":"pith_short_8","alias_value":"JA3DTKHI","created_at":"2026-05-18T12:29:27.538025+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/JA3DTKHIOAOBJTT6JBFHYAWVIJ","json":"https://pith.science/pith/JA3DTKHIOAOBJTT6JBFHYAWVIJ.json","graph_json":"https://pith.science/api/pith-number/JA3DTKHIOAOBJTT6JBFHYAWVIJ/graph.json","events_json":"https://pith.science/api/pith-number/JA3DTKHIOAOBJTT6JBFHYAWVIJ/events.json","paper":"https://pith.science/paper/JA3DTKHI"},"agent_actions":{"view_html":"https://pith.science/pith/JA3DTKHIOAOBJTT6JBFHYAWVIJ","download_json":"https://pith.science/pith/JA3DTKHIOAOBJTT6JBFHYAWVIJ.json","view_paper":"https://pith.science/paper/JA3DTKHI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1512.04690&json=true","fetch_graph":"https://pith.science/api/pith-number/JA3DTKHIOAOBJTT6JBFHYAWVIJ/graph.json","fetch_events":"https://pith.science/api/pith-number/JA3DTKHIOAOBJTT6JBFHYAWVIJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JA3DTKHIOAOBJTT6JBFHYAWVIJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JA3DTKHIOAOBJTT6JBFHYAWVIJ/action/storage_attestation","attest_author":"https://pith.science/pith/JA3DTKHIOAOBJTT6JBFHYAWVIJ/action/author_attestation","sign_citation":"https://pith.science/pith/JA3DTKHIOAOBJTT6JBFHYAWVIJ/action/citation_signature","submit_replication":"https://pith.science/pith/JA3DTKHIOAOBJTT6JBFHYAWVIJ/action/replication_record"}},"created_at":"2026-05-18T01:22:00.064723+00:00","updated_at":"2026-05-18T01:22:00.064723+00:00"}