{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:LM2R37GUWZKFOIRQCTFBR2DRCU","short_pith_number":"pith:LM2R37GU","schema_version":"1.0","canonical_sha256":"5b351dfcd4b65457223014ca18e87115325c3c91db26806021a8924d30cc851b","source":{"kind":"arxiv","id":"1305.6985","version":2},"attestation_state":"computed","paper":{"title":"Multi-Color Transit Photometry of GJ 1214b through BJHKs-Bands and a Long-Term Monitoring of the Stellar Variability of GJ 1214","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"Akihiko Fukui, Amnart Sukom, Daisuke Kuroda, Hideyuki Izumiura, Hiroshi Ohnuki, Kenji Kurosaki, Kenshi Yanagisawa, Kiyoe Kawauchi, Masahiro Ikoma, Masahiro Onitsuka, Masayuki Kuzuhara, Michitoshi Yoshida, Motohide Tamura, Nobuyuki Kawai, Norio Narita, Takahiro Nagayama, Takuya Suenaga, Teruyuki Hirano, Yasuhiro H. Takahashi, Yasunori Hori, Yasushi Nakajima, Yui Kawashima","submitted_at":"2013-05-30T01:28:55Z","abstract_excerpt":"We present 5 new transit light curves of GJ 1214b taken in BJHKs-bands. Two transits were observed in B-band using the Suprime-Cam and the FOCAS instruments onboard the Subaru 8.2m telescope, and one transit was done in JHKs-bands simultaneously with the SIRIUS camera on the IRSF 1.4m telescope. MCMC analyses show that the planet-to-star radius ratios are, Rp/Rs = 0.11651 \\pm 0.00065 (B-band, Subaru/Suprime-Cam), Rp/Rs = 0.11601 \\pm 0.00117 (B-band, Subaru/FOCAS), Rp/Rs = 0.11654 \\pm 0.00080 (J-band, IRSF/SIRIUS), Rp/Rs = 0.11550 ^{+0.00142}_{-0.00153} (H-band, IRSF/SIRIUS), and Rp/Rs = 0.1154"},"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":"1305.6985","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2013-05-30T01:28:55Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"c6942c1a001e975c4649c2056b2d633c3f0605582dd61aceba0bef518a1eeecb","abstract_canon_sha256":"0ee1b8c3b4b835f9cd2b6a1bc8ef3c0972feebfcb60b1c687b8d36a3d240611e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:49:39.930107Z","signature_b64":"ny+7XdZPgScCOhSr3ZGBsWWpCUKPX1HqPLhKRfrlP0baiG4jaPl6PVnOEBHVW+6oPyQUp3nTXLNs02/G6zZVCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5b351dfcd4b65457223014ca18e87115325c3c91db26806021a8924d30cc851b","last_reissued_at":"2026-05-18T01:49:39.929514Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:49:39.929514Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Multi-Color Transit Photometry of GJ 1214b through BJHKs-Bands and a Long-Term Monitoring of the Stellar Variability of GJ 1214","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"Akihiko Fukui, Amnart Sukom, Daisuke Kuroda, Hideyuki Izumiura, Hiroshi Ohnuki, Kenji Kurosaki, Kenshi Yanagisawa, Kiyoe Kawauchi, Masahiro Ikoma, Masahiro Onitsuka, Masayuki Kuzuhara, Michitoshi Yoshida, Motohide Tamura, Nobuyuki Kawai, Norio Narita, Takahiro Nagayama, Takuya Suenaga, Teruyuki Hirano, Yasuhiro H. Takahashi, Yasunori Hori, Yasushi Nakajima, Yui Kawashima","submitted_at":"2013-05-30T01:28:55Z","abstract_excerpt":"We present 5 new transit light curves of GJ 1214b taken in BJHKs-bands. Two transits were observed in B-band using the Suprime-Cam and the FOCAS instruments onboard the Subaru 8.2m telescope, and one transit was done in JHKs-bands simultaneously with the SIRIUS camera on the IRSF 1.4m telescope. MCMC analyses show that the planet-to-star radius ratios are, Rp/Rs = 0.11651 \\pm 0.00065 (B-band, Subaru/Suprime-Cam), Rp/Rs = 0.11601 \\pm 0.00117 (B-band, Subaru/FOCAS), Rp/Rs = 0.11654 \\pm 0.00080 (J-band, IRSF/SIRIUS), Rp/Rs = 0.11550 ^{+0.00142}_{-0.00153} (H-band, IRSF/SIRIUS), and Rp/Rs = 0.1154"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1305.6985","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":"1305.6985","created_at":"2026-05-18T01:49:39.929601+00:00"},{"alias_kind":"arxiv_version","alias_value":"1305.6985v2","created_at":"2026-05-18T01:49:39.929601+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1305.6985","created_at":"2026-05-18T01:49:39.929601+00:00"},{"alias_kind":"pith_short_12","alias_value":"LM2R37GUWZKF","created_at":"2026-05-18T12:27:51.066281+00:00"},{"alias_kind":"pith_short_16","alias_value":"LM2R37GUWZKFOIRQ","created_at":"2026-05-18T12:27:51.066281+00:00"},{"alias_kind":"pith_short_8","alias_value":"LM2R37GU","created_at":"2026-05-18T12:27:51.066281+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/LM2R37GUWZKFOIRQCTFBR2DRCU","json":"https://pith.science/pith/LM2R37GUWZKFOIRQCTFBR2DRCU.json","graph_json":"https://pith.science/api/pith-number/LM2R37GUWZKFOIRQCTFBR2DRCU/graph.json","events_json":"https://pith.science/api/pith-number/LM2R37GUWZKFOIRQCTFBR2DRCU/events.json","paper":"https://pith.science/paper/LM2R37GU"},"agent_actions":{"view_html":"https://pith.science/pith/LM2R37GUWZKFOIRQCTFBR2DRCU","download_json":"https://pith.science/pith/LM2R37GUWZKFOIRQCTFBR2DRCU.json","view_paper":"https://pith.science/paper/LM2R37GU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1305.6985&json=true","fetch_graph":"https://pith.science/api/pith-number/LM2R37GUWZKFOIRQCTFBR2DRCU/graph.json","fetch_events":"https://pith.science/api/pith-number/LM2R37GUWZKFOIRQCTFBR2DRCU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LM2R37GUWZKFOIRQCTFBR2DRCU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LM2R37GUWZKFOIRQCTFBR2DRCU/action/storage_attestation","attest_author":"https://pith.science/pith/LM2R37GUWZKFOIRQCTFBR2DRCU/action/author_attestation","sign_citation":"https://pith.science/pith/LM2R37GUWZKFOIRQCTFBR2DRCU/action/citation_signature","submit_replication":"https://pith.science/pith/LM2R37GUWZKFOIRQCTFBR2DRCU/action/replication_record"}},"created_at":"2026-05-18T01:49:39.929601+00:00","updated_at":"2026-05-18T01:49:39.929601+00:00"}