{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:GKLIYZOYGSWDHXRWTSXXFEC3NF","short_pith_number":"pith:GKLIYZOY","schema_version":"1.0","canonical_sha256":"32968c65d834ac33de369caf72905b6968bd336c234fc2c4f3e82a9907b0f66c","source":{"kind":"arxiv","id":"1605.02708","version":1},"attestation_state":"computed","paper":{"title":"$Extrasolar~Storms$: Pressure-dependent Changes In Light Curve Phase In Brown Dwarfs From Simultaneous $Hubble$ and $Spitzer$ Observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"Adam J. Burgasser, Adam P. Showman, D\\'aniel Apai, Davin Flateau, Esther Buenzli, \\'Etienne Artigau, Hao Yang, Jacqueline Radigan, Mark S. Marley, Patrick J. Lowrance, Stanimir Metchev, Theodora Karalidi","submitted_at":"2016-05-09T19:33:30Z","abstract_excerpt":"We present $Spitzer$/IRAC Ch1 and Ch2 monitoring of six brown dwarfs during 8 different epochs over the course of 20 months. For four brown dwarfs, we also obtained simulataneous $HST$/WFC3 G141 Grism spectra during two epochs and derived light curves in five narrow-band filters. Probing different pressure levels in the atmospheres, the multi-wavelength light curves of our six targets all exhibit variations, and the shape of the light curves evolves over the timescale of a rotation period, ranging from 1.4 h to 13 h. We compare the shapes of the light curves and estimate the phase shifts betwe"},"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":"1605.02708","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2016-05-09T19:33:30Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"ab99df59aae403d48c15d515876dbafe1653b9fee13e17a7fd96d4ef685c4aa7","abstract_canon_sha256":"66637b18261816e50c4b131a2b5c1d376e74f904322b711c51880b9166cbc5f9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:10:47.752733Z","signature_b64":"uG5HwA/nnpyTcTXmP0dQFC3KlWYqAtMphyOGiSwpg/SEXB4T75qtmoB9qpAq0HaYujbjo1oXWfr6VV4ddt3iBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"32968c65d834ac33de369caf72905b6968bd336c234fc2c4f3e82a9907b0f66c","last_reissued_at":"2026-05-18T01:10:47.752174Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:10:47.752174Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"$Extrasolar~Storms$: Pressure-dependent Changes In Light Curve Phase In Brown Dwarfs From Simultaneous $Hubble$ and $Spitzer$ Observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"Adam J. Burgasser, Adam P. Showman, D\\'aniel Apai, Davin Flateau, Esther Buenzli, \\'Etienne Artigau, Hao Yang, Jacqueline Radigan, Mark S. Marley, Patrick J. Lowrance, Stanimir Metchev, Theodora Karalidi","submitted_at":"2016-05-09T19:33:30Z","abstract_excerpt":"We present $Spitzer$/IRAC Ch1 and Ch2 monitoring of six brown dwarfs during 8 different epochs over the course of 20 months. For four brown dwarfs, we also obtained simulataneous $HST$/WFC3 G141 Grism spectra during two epochs and derived light curves in five narrow-band filters. Probing different pressure levels in the atmospheres, the multi-wavelength light curves of our six targets all exhibit variations, and the shape of the light curves evolves over the timescale of a rotation period, ranging from 1.4 h to 13 h. We compare the shapes of the light curves and estimate the phase shifts betwe"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1605.02708","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":"1605.02708","created_at":"2026-05-18T01:10:47.752246+00:00"},{"alias_kind":"arxiv_version","alias_value":"1605.02708v1","created_at":"2026-05-18T01:10:47.752246+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1605.02708","created_at":"2026-05-18T01:10:47.752246+00:00"},{"alias_kind":"pith_short_12","alias_value":"GKLIYZOYGSWD","created_at":"2026-05-18T12:30:19.053100+00:00"},{"alias_kind":"pith_short_16","alias_value":"GKLIYZOYGSWDHXRW","created_at":"2026-05-18T12:30:19.053100+00:00"},{"alias_kind":"pith_short_8","alias_value":"GKLIYZOY","created_at":"2026-05-18T12:30:19.053100+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/GKLIYZOYGSWDHXRWTSXXFEC3NF","json":"https://pith.science/pith/GKLIYZOYGSWDHXRWTSXXFEC3NF.json","graph_json":"https://pith.science/api/pith-number/GKLIYZOYGSWDHXRWTSXXFEC3NF/graph.json","events_json":"https://pith.science/api/pith-number/GKLIYZOYGSWDHXRWTSXXFEC3NF/events.json","paper":"https://pith.science/paper/GKLIYZOY"},"agent_actions":{"view_html":"https://pith.science/pith/GKLIYZOYGSWDHXRWTSXXFEC3NF","download_json":"https://pith.science/pith/GKLIYZOYGSWDHXRWTSXXFEC3NF.json","view_paper":"https://pith.science/paper/GKLIYZOY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1605.02708&json=true","fetch_graph":"https://pith.science/api/pith-number/GKLIYZOYGSWDHXRWTSXXFEC3NF/graph.json","fetch_events":"https://pith.science/api/pith-number/GKLIYZOYGSWDHXRWTSXXFEC3NF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GKLIYZOYGSWDHXRWTSXXFEC3NF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GKLIYZOYGSWDHXRWTSXXFEC3NF/action/storage_attestation","attest_author":"https://pith.science/pith/GKLIYZOYGSWDHXRWTSXXFEC3NF/action/author_attestation","sign_citation":"https://pith.science/pith/GKLIYZOYGSWDHXRWTSXXFEC3NF/action/citation_signature","submit_replication":"https://pith.science/pith/GKLIYZOYGSWDHXRWTSXXFEC3NF/action/replication_record"}},"created_at":"2026-05-18T01:10:47.752246+00:00","updated_at":"2026-05-18T01:10:47.752246+00:00"}