{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2007:VYMVQ2RK6YXTAUWHCUBPLZZZKG","short_pith_number":"pith:VYMVQ2RK","schema_version":"1.0","canonical_sha256":"ae19586a2af62f3052c71502f5e73951b9f83505c97930569cfe2908f73e8bd4","source":{"kind":"arxiv","id":"0710.3383","version":1},"attestation_state":"computed","paper":{"title":"Simultaneous Multi-Wavelength Observations of Magnetic Activity in Ultracool Dwarfs. II. Mixed Trends in VB10 and LSR1835+32 and the Possible Role of Rotation","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"C.M. Johns-Krull, E. Berger (Princeton/OCIW), E. Martin, G. Basri, J.E. Gizis, J. Liebert, M.S. Giampapa, N. Phan-Bao, R.E. Rutledge, T.A. Fleming, W.H. Sherry","submitted_at":"2007-10-17T20:03:27Z","abstract_excerpt":"[Abridged] As part of our on-going investigation of magnetic activity in ultracool dwarfs we present simultaneous radio, X-ray, UV, and optical observations of LSR1835+32 (M8.5), and simultaneous X-ray and UV observations of VB10 (M8), both with a duration of about 9 hours. LSR1835+32 exhibits persistent radio emission and H-alpha variability on timescales of ~0.5-2 hr. The detected UV flux is consistent with photospheric emission, and no X-ray emission is detected to a deep limit of L_X/L_bol<10^-5.7. The H-alpha and radio emission are temporally uncorrelated, and the ratio of radio to X-ray "},"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":"0710.3383","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2007-10-17T20:03:27Z","cross_cats_sorted":[],"title_canon_sha256":"84f0b153fadaab796f5aeaddbc3141ddcbe024a0e8917bc460e3db414e722900","abstract_canon_sha256":"646fd3e72851d4aee93cab4a3cc8b7ade1d4c026dd0b08b4309f702776a14e10"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T17:06:18.366247Z","signature_b64":"bZEN/b3SCQP+AATn3xVWG7gH3vSh4ovGsMaZbWGP0cLztOUc2/+t2ULphHfw2ivKEmAqzZRXzHdjcqZdR2VjCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ae19586a2af62f3052c71502f5e73951b9f83505c97930569cfe2908f73e8bd4","last_reissued_at":"2026-07-04T17:06:18.365832Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T17:06:18.365832Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Simultaneous Multi-Wavelength Observations of Magnetic Activity in Ultracool Dwarfs. II. Mixed Trends in VB10 and LSR1835+32 and the Possible Role of Rotation","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"C.M. Johns-Krull, E. Berger (Princeton/OCIW), E. Martin, G. Basri, J.E. Gizis, J. Liebert, M.S. Giampapa, N. Phan-Bao, R.E. Rutledge, T.A. Fleming, W.H. Sherry","submitted_at":"2007-10-17T20:03:27Z","abstract_excerpt":"[Abridged] As part of our on-going investigation of magnetic activity in ultracool dwarfs we present simultaneous radio, X-ray, UV, and optical observations of LSR1835+32 (M8.5), and simultaneous X-ray and UV observations of VB10 (M8), both with a duration of about 9 hours. LSR1835+32 exhibits persistent radio emission and H-alpha variability on timescales of ~0.5-2 hr. The detected UV flux is consistent with photospheric emission, and no X-ray emission is detected to a deep limit of L_X/L_bol<10^-5.7. The H-alpha and radio emission are temporally uncorrelated, and the ratio of radio to X-ray "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0710.3383","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/0710.3383/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":"0710.3383","created_at":"2026-07-04T17:06:18.365888+00:00"},{"alias_kind":"arxiv_version","alias_value":"0710.3383v1","created_at":"2026-07-04T17:06:18.365888+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0710.3383","created_at":"2026-07-04T17:06:18.365888+00:00"},{"alias_kind":"pith_short_12","alias_value":"VYMVQ2RK6YXT","created_at":"2026-07-04T17:06:18.365888+00:00"},{"alias_kind":"pith_short_16","alias_value":"VYMVQ2RK6YXTAUWH","created_at":"2026-07-04T17:06:18.365888+00:00"},{"alias_kind":"pith_short_8","alias_value":"VYMVQ2RK","created_at":"2026-07-04T17:06:18.365888+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2606.04144","citing_title":"Characterizing Transiting Exoplanet Atmospheres in the 2030s with the Hubble Space Telescope","ref_index":97,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/VYMVQ2RK6YXTAUWHCUBPLZZZKG","json":"https://pith.science/pith/VYMVQ2RK6YXTAUWHCUBPLZZZKG.json","graph_json":"https://pith.science/api/pith-number/VYMVQ2RK6YXTAUWHCUBPLZZZKG/graph.json","events_json":"https://pith.science/api/pith-number/VYMVQ2RK6YXTAUWHCUBPLZZZKG/events.json","paper":"https://pith.science/paper/VYMVQ2RK"},"agent_actions":{"view_html":"https://pith.science/pith/VYMVQ2RK6YXTAUWHCUBPLZZZKG","download_json":"https://pith.science/pith/VYMVQ2RK6YXTAUWHCUBPLZZZKG.json","view_paper":"https://pith.science/paper/VYMVQ2RK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0710.3383&json=true","fetch_graph":"https://pith.science/api/pith-number/VYMVQ2RK6YXTAUWHCUBPLZZZKG/graph.json","fetch_events":"https://pith.science/api/pith-number/VYMVQ2RK6YXTAUWHCUBPLZZZKG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VYMVQ2RK6YXTAUWHCUBPLZZZKG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VYMVQ2RK6YXTAUWHCUBPLZZZKG/action/storage_attestation","attest_author":"https://pith.science/pith/VYMVQ2RK6YXTAUWHCUBPLZZZKG/action/author_attestation","sign_citation":"https://pith.science/pith/VYMVQ2RK6YXTAUWHCUBPLZZZKG/action/citation_signature","submit_replication":"https://pith.science/pith/VYMVQ2RK6YXTAUWHCUBPLZZZKG/action/replication_record"}},"created_at":"2026-07-04T17:06:18.365888+00:00","updated_at":"2026-07-04T17:06:18.365888+00:00"}