{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:75QQZWKRXGFPI4ELLWYINGRYNF","short_pith_number":"pith:75QQZWKR","schema_version":"1.0","canonical_sha256":"ff610cd951b98af4708b5db0869a386964d870f45a0efeee2b2d439c5ecb407e","source":{"kind":"arxiv","id":"1603.00824","version":1},"attestation_state":"computed","paper":{"title":"Low frequency radio observations of SN 2011dh and the evolution of its post-shock plasma properties","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"2), 3), 4) ((1) Tata Institute of Fundamental Research, Alak Ray (1, Bangalore, Cambridge, Computation, Harvard Smithsonian Center for Astrophysics, Harvard University, Homi Bhabha Road, India. (2) Department of Physics, India. (3) Institute for Theory, Indian Institute of Science, Mumbai, Naveen Yadav (1, Sayan Chakraborti (3, USA), USA. (4) Society of Fellows","submitted_at":"2016-03-02T18:49:55Z","abstract_excerpt":"We present late time, low frequency observations of SN 2011dh made using the Giant Metrewave Radio Telescope (GMRT). Our observations at $325\\ \\rm MHz$, $610\\ \\rm MHz$ and $1280\\ \\rm MHz$ conducted between $93-421\\ \\rm days$ after the explosion supplement the millimeter and centimeter wave observations conducted between $4-15 \\ \\rm days$ after explosion using the Combined Array for Research in Millimeter-wave Astronomy (CARMA) and extensive radio observations ($ 1.0-36.5\\ \\rm GHz$) conducted between $16-93\\ \\rm days$ after explosion using Jansky Very Large Array (JVLA). We fit a synchrotron se"},"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":"1603.00824","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-03-02T18:49:55Z","cross_cats_sorted":[],"title_canon_sha256":"df075cd02cfdf7503bf2cc0a030a616369dddaa95fe25088239c2e1fc769428a","abstract_canon_sha256":"f90c67ce1b2c8044903b8d5be03befd5272f2625a2f8ca34c33bbab9142ce648"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:18:36.938366Z","signature_b64":"LnQaF36AAM6QRpA0kwVTARspFtlobNOPB6r3y8pQp98NTcjSa1fYrTyAsWV74unwpPIS254sOQWd/v9I0C+ZDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ff610cd951b98af4708b5db0869a386964d870f45a0efeee2b2d439c5ecb407e","last_reissued_at":"2026-05-18T01:18:36.937923Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:18:36.937923Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Low frequency radio observations of SN 2011dh and the evolution of its post-shock plasma properties","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"2), 3), 4) ((1) Tata Institute of Fundamental Research, Alak Ray (1, Bangalore, Cambridge, Computation, Harvard Smithsonian Center for Astrophysics, Harvard University, Homi Bhabha Road, India. (2) Department of Physics, India. (3) Institute for Theory, Indian Institute of Science, Mumbai, Naveen Yadav (1, Sayan Chakraborti (3, USA), USA. (4) Society of Fellows","submitted_at":"2016-03-02T18:49:55Z","abstract_excerpt":"We present late time, low frequency observations of SN 2011dh made using the Giant Metrewave Radio Telescope (GMRT). Our observations at $325\\ \\rm MHz$, $610\\ \\rm MHz$ and $1280\\ \\rm MHz$ conducted between $93-421\\ \\rm days$ after the explosion supplement the millimeter and centimeter wave observations conducted between $4-15 \\ \\rm days$ after explosion using the Combined Array for Research in Millimeter-wave Astronomy (CARMA) and extensive radio observations ($ 1.0-36.5\\ \\rm GHz$) conducted between $16-93\\ \\rm days$ after explosion using Jansky Very Large Array (JVLA). We fit a synchrotron se"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1603.00824","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":"1603.00824","created_at":"2026-05-18T01:18:36.937988+00:00"},{"alias_kind":"arxiv_version","alias_value":"1603.00824v1","created_at":"2026-05-18T01:18:36.937988+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1603.00824","created_at":"2026-05-18T01:18:36.937988+00:00"},{"alias_kind":"pith_short_12","alias_value":"75QQZWKRXGFP","created_at":"2026-05-18T12:30:04.600751+00:00"},{"alias_kind":"pith_short_16","alias_value":"75QQZWKRXGFPI4EL","created_at":"2026-05-18T12:30:04.600751+00:00"},{"alias_kind":"pith_short_8","alias_value":"75QQZWKR","created_at":"2026-05-18T12:30:04.600751+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/75QQZWKRXGFPI4ELLWYINGRYNF","json":"https://pith.science/pith/75QQZWKRXGFPI4ELLWYINGRYNF.json","graph_json":"https://pith.science/api/pith-number/75QQZWKRXGFPI4ELLWYINGRYNF/graph.json","events_json":"https://pith.science/api/pith-number/75QQZWKRXGFPI4ELLWYINGRYNF/events.json","paper":"https://pith.science/paper/75QQZWKR"},"agent_actions":{"view_html":"https://pith.science/pith/75QQZWKRXGFPI4ELLWYINGRYNF","download_json":"https://pith.science/pith/75QQZWKRXGFPI4ELLWYINGRYNF.json","view_paper":"https://pith.science/paper/75QQZWKR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1603.00824&json=true","fetch_graph":"https://pith.science/api/pith-number/75QQZWKRXGFPI4ELLWYINGRYNF/graph.json","fetch_events":"https://pith.science/api/pith-number/75QQZWKRXGFPI4ELLWYINGRYNF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/75QQZWKRXGFPI4ELLWYINGRYNF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/75QQZWKRXGFPI4ELLWYINGRYNF/action/storage_attestation","attest_author":"https://pith.science/pith/75QQZWKRXGFPI4ELLWYINGRYNF/action/author_attestation","sign_citation":"https://pith.science/pith/75QQZWKRXGFPI4ELLWYINGRYNF/action/citation_signature","submit_replication":"https://pith.science/pith/75QQZWKRXGFPI4ELLWYINGRYNF/action/replication_record"}},"created_at":"2026-05-18T01:18:36.937988+00:00","updated_at":"2026-05-18T01:18:36.937988+00:00"}