{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:SZYQZJ6UY5OC63Y33UUIHSIDCX","short_pith_number":"pith:SZYQZJ6U","schema_version":"1.0","canonical_sha256":"96710ca7d4c75c2f6f1bdd2883c90315e49f49a9f2dd404dfe09c00c975e606f","source":{"kind":"arxiv","id":"1412.6363","version":2},"attestation_state":"computed","paper":{"title":"Multiwaveband photometry of the irradiated brown dwarf WD0137-349B","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Ch. Helling, G. Wynn, J.J. Fortney, K.A. Lawrie, M.R. Burleigh, M.S. Marley, P.B. Rimmer, P.F.L. Maxted, S.L. Casewell, S.P. Littlefair","submitted_at":"2014-12-19T14:57:27Z","abstract_excerpt":"WD0137-349 is a white dwarf-brown dwarf binary system in a 116 minute orbit. We present radial velocity observations and multiwaveband photometry from V, R and I in the optical, to J, H and Ks in the near-IR and [3.6], [4.5], [5.8] and [8.0] microns in the mid-IR. The photometry and lightcurves show variability in all wavebands, with the amplitude peaking at [4.5] microns, where the system is also brightest. Fluxes and brightness temperatures were computed for the heated and unheated atmosphere of the brown dwarf (WD0137-349B) using synthetic spectra of the white dwarf using model atmosphere s"},"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":"1412.6363","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-12-19T14:57:27Z","cross_cats_sorted":[],"title_canon_sha256":"3ed6e6d631a6d681e3374c9117cbdce97f63308fc5467bf62d8fd4990917cb9c","abstract_canon_sha256":"f1b66c3414d4a44d08ef176ca7773c4220140a39a98e06ed4374f34d0295edb0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:16.482240Z","signature_b64":"1/eZwUOd1a5CKrtG2ofPcJFHIaZMp9XPPgAFmDtdM9VpVBYEGfQgxT2C7dAlBVQwKwfWvFfETQwOS4MHtsBLDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"96710ca7d4c75c2f6f1bdd2883c90315e49f49a9f2dd404dfe09c00c975e606f","last_reissued_at":"2026-05-18T01:41:16.481827Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:16.481827Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Multiwaveband photometry of the irradiated brown dwarf WD0137-349B","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Ch. Helling, G. Wynn, J.J. Fortney, K.A. Lawrie, M.R. Burleigh, M.S. Marley, P.B. Rimmer, P.F.L. Maxted, S.L. Casewell, S.P. Littlefair","submitted_at":"2014-12-19T14:57:27Z","abstract_excerpt":"WD0137-349 is a white dwarf-brown dwarf binary system in a 116 minute orbit. We present radial velocity observations and multiwaveband photometry from V, R and I in the optical, to J, H and Ks in the near-IR and [3.6], [4.5], [5.8] and [8.0] microns in the mid-IR. The photometry and lightcurves show variability in all wavebands, with the amplitude peaking at [4.5] microns, where the system is also brightest. Fluxes and brightness temperatures were computed for the heated and unheated atmosphere of the brown dwarf (WD0137-349B) using synthetic spectra of the white dwarf using model atmosphere s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1412.6363","kind":"arxiv","version":2},"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":"1412.6363","created_at":"2026-05-18T01:41:16.481883+00:00"},{"alias_kind":"arxiv_version","alias_value":"1412.6363v2","created_at":"2026-05-18T01:41:16.481883+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1412.6363","created_at":"2026-05-18T01:41:16.481883+00:00"},{"alias_kind":"pith_short_12","alias_value":"SZYQZJ6UY5OC","created_at":"2026-05-18T12:28:49.207871+00:00"},{"alias_kind":"pith_short_16","alias_value":"SZYQZJ6UY5OC63Y3","created_at":"2026-05-18T12:28:49.207871+00:00"},{"alias_kind":"pith_short_8","alias_value":"SZYQZJ6U","created_at":"2026-05-18T12:28:49.207871+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/SZYQZJ6UY5OC63Y33UUIHSIDCX","json":"https://pith.science/pith/SZYQZJ6UY5OC63Y33UUIHSIDCX.json","graph_json":"https://pith.science/api/pith-number/SZYQZJ6UY5OC63Y33UUIHSIDCX/graph.json","events_json":"https://pith.science/api/pith-number/SZYQZJ6UY5OC63Y33UUIHSIDCX/events.json","paper":"https://pith.science/paper/SZYQZJ6U"},"agent_actions":{"view_html":"https://pith.science/pith/SZYQZJ6UY5OC63Y33UUIHSIDCX","download_json":"https://pith.science/pith/SZYQZJ6UY5OC63Y33UUIHSIDCX.json","view_paper":"https://pith.science/paper/SZYQZJ6U","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1412.6363&json=true","fetch_graph":"https://pith.science/api/pith-number/SZYQZJ6UY5OC63Y33UUIHSIDCX/graph.json","fetch_events":"https://pith.science/api/pith-number/SZYQZJ6UY5OC63Y33UUIHSIDCX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SZYQZJ6UY5OC63Y33UUIHSIDCX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SZYQZJ6UY5OC63Y33UUIHSIDCX/action/storage_attestation","attest_author":"https://pith.science/pith/SZYQZJ6UY5OC63Y33UUIHSIDCX/action/author_attestation","sign_citation":"https://pith.science/pith/SZYQZJ6UY5OC63Y33UUIHSIDCX/action/citation_signature","submit_replication":"https://pith.science/pith/SZYQZJ6UY5OC63Y33UUIHSIDCX/action/replication_record"}},"created_at":"2026-05-18T01:41:16.481883+00:00","updated_at":"2026-05-18T01:41:16.481883+00:00"}