{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1995:M7JROWDDCMRUAE2GZWQV6B6AGO","short_pith_number":"pith:M7JROWDD","schema_version":"1.0","canonical_sha256":"67d31758631323401346cda15f07c033840d922c9f5cde6f6130246ef6eb684a","source":{"kind":"arxiv","id":"astro-ph/9512135","version":1},"attestation_state":"computed","paper":{"title":"Radio observations of the $\\gamma$-ray blazar 0528+134","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"E. B. Waltman, F. D. Ghigo, H. P. Reuter, H. Ungerechts, K. J. Johnston, K. Standke, M. Pohl, P. Reich, R. L. Fiedler, R. Schlickeiser, S. Britzen, T.P. Krichbaum, W. Reich","submitted_at":"1995-12-20T08:50:23Z","abstract_excerpt":"We report multifrequency observations of the $\\gamma$-ray blazar 0528+134 with the Effelsberg 100-m telescope, the IRAM 30-m telescope, and the NRL Green Bank Interferometer. 0528+134 underwent a major radio and mm outburst in 1993 a few month after a very strong outburst in high energy $\\gamma$-rays. A similar behaviour is indicated for the weaker $\\gamma$-ray outburst in May 1991 and the mm activity in the beginning of 1992. This result fits nicely to the general finding that blazars are bright in $\\gamma$-rays preferrentially at the beginning of a radio outburst. 0528+134 was observed with "},"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/9512135","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"1995-12-20T08:50:23Z","cross_cats_sorted":[],"title_canon_sha256":"684d87504792d2bd76a460bad235410cd72bc2054039ca15b041ffa7b2532945","abstract_canon_sha256":"9863508023376dcb023f8bcc8d2520fbab431ad5d301460383068ba65c274f59"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T14:14:40.179738Z","signature_b64":"PgdttatY1Li3PJm5QerQYMbIme45XCYkj6VExIEOL/BFrctwIy/AiDC0JZB0sYfqrGQyAuHhK5qXsRQLhIJGDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"67d31758631323401346cda15f07c033840d922c9f5cde6f6130246ef6eb684a","last_reissued_at":"2026-07-04T14:14:40.179229Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T14:14:40.179229Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Radio observations of the $\\gamma$-ray blazar 0528+134","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"E. B. Waltman, F. D. Ghigo, H. P. Reuter, H. Ungerechts, K. J. Johnston, K. Standke, M. Pohl, P. Reich, R. L. Fiedler, R. Schlickeiser, S. Britzen, T.P. Krichbaum, W. Reich","submitted_at":"1995-12-20T08:50:23Z","abstract_excerpt":"We report multifrequency observations of the $\\gamma$-ray blazar 0528+134 with the Effelsberg 100-m telescope, the IRAM 30-m telescope, and the NRL Green Bank Interferometer. 0528+134 underwent a major radio and mm outburst in 1993 a few month after a very strong outburst in high energy $\\gamma$-rays. A similar behaviour is indicated for the weaker $\\gamma$-ray outburst in May 1991 and the mm activity in the beginning of 1992. This result fits nicely to the general finding that blazars are bright in $\\gamma$-rays preferrentially at the beginning of a radio outburst. 0528+134 was observed with "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/9512135","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/9512135/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/9512135","created_at":"2026-07-04T14:14:40.179287+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/9512135v1","created_at":"2026-07-04T14:14:40.179287+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/9512135","created_at":"2026-07-04T14:14:40.179287+00:00"},{"alias_kind":"pith_short_12","alias_value":"M7JROWDDCMRU","created_at":"2026-07-04T14:14:40.179287+00:00"},{"alias_kind":"pith_short_16","alias_value":"M7JROWDDCMRUAE2G","created_at":"2026-07-04T14:14:40.179287+00:00"},{"alias_kind":"pith_short_8","alias_value":"M7JROWDD","created_at":"2026-07-04T14:14:40.179287+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/M7JROWDDCMRUAE2GZWQV6B6AGO","json":"https://pith.science/pith/M7JROWDDCMRUAE2GZWQV6B6AGO.json","graph_json":"https://pith.science/api/pith-number/M7JROWDDCMRUAE2GZWQV6B6AGO/graph.json","events_json":"https://pith.science/api/pith-number/M7JROWDDCMRUAE2GZWQV6B6AGO/events.json","paper":"https://pith.science/paper/M7JROWDD"},"agent_actions":{"view_html":"https://pith.science/pith/M7JROWDDCMRUAE2GZWQV6B6AGO","download_json":"https://pith.science/pith/M7JROWDDCMRUAE2GZWQV6B6AGO.json","view_paper":"https://pith.science/paper/M7JROWDD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/9512135&json=true","fetch_graph":"https://pith.science/api/pith-number/M7JROWDDCMRUAE2GZWQV6B6AGO/graph.json","fetch_events":"https://pith.science/api/pith-number/M7JROWDDCMRUAE2GZWQV6B6AGO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/M7JROWDDCMRUAE2GZWQV6B6AGO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/M7JROWDDCMRUAE2GZWQV6B6AGO/action/storage_attestation","attest_author":"https://pith.science/pith/M7JROWDDCMRUAE2GZWQV6B6AGO/action/author_attestation","sign_citation":"https://pith.science/pith/M7JROWDDCMRUAE2GZWQV6B6AGO/action/citation_signature","submit_replication":"https://pith.science/pith/M7JROWDDCMRUAE2GZWQV6B6AGO/action/replication_record"}},"created_at":"2026-07-04T14:14:40.179287+00:00","updated_at":"2026-07-04T14:14:40.179287+00:00"}