{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2016:SCZMXNKLM722ZVUN5A2H3AQQWP","short_pith_number":"pith:SCZMXNKL","canonical_record":{"source":{"id":"1610.04541","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-10-14T17:16:00Z","cross_cats_sorted":[],"title_canon_sha256":"d5f10eacb5a6cb033ee2b5c904e15f7515ff09dc6a46b569a6f142da184b36cd","abstract_canon_sha256":"e696b4d8746fab4f04907f96f223a14ef2e4ece41e49180921efe22ae81b5ba9"},"schema_version":"1.0"},"canonical_sha256":"90b2cbb54b67f5acd68de8347d8210b3c8645dcf9690179418f78b3aa36064c6","source":{"kind":"arxiv","id":"1610.04541","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1610.04541","created_at":"2026-05-18T00:53:07Z"},{"alias_kind":"arxiv_version","alias_value":"1610.04541v1","created_at":"2026-05-18T00:53:07Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1610.04541","created_at":"2026-05-18T00:53:07Z"},{"alias_kind":"pith_short_12","alias_value":"SCZMXNKLM722","created_at":"2026-05-18T12:30:44Z"},{"alias_kind":"pith_short_16","alias_value":"SCZMXNKLM722ZVUN","created_at":"2026-05-18T12:30:44Z"},{"alias_kind":"pith_short_8","alias_value":"SCZMXNKL","created_at":"2026-05-18T12:30:44Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2016:SCZMXNKLM722ZVUN5A2H3AQQWP","target":"record","payload":{"canonical_record":{"source":{"id":"1610.04541","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-10-14T17:16:00Z","cross_cats_sorted":[],"title_canon_sha256":"d5f10eacb5a6cb033ee2b5c904e15f7515ff09dc6a46b569a6f142da184b36cd","abstract_canon_sha256":"e696b4d8746fab4f04907f96f223a14ef2e4ece41e49180921efe22ae81b5ba9"},"schema_version":"1.0"},"canonical_sha256":"90b2cbb54b67f5acd68de8347d8210b3c8645dcf9690179418f78b3aa36064c6","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:53:07.178678Z","signature_b64":"yIYr2zILj+7w5T0djiL2EvPYI90WsmXlxO76q7LNauwW7+zEquU1mQ2jabyUr4qwhJ8cRXsr8CX7kq856TxjAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"90b2cbb54b67f5acd68de8347d8210b3c8645dcf9690179418f78b3aa36064c6","last_reissued_at":"2026-05-18T00:53:07.178232Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:53:07.178232Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1610.04541","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:53:07Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"aSwbi5+3uQciiS0Vv2HTECnmx6F6frm+PsDPQEdeRQQHE3ysdUSoC73cnrAQdutcEr5K5PIUOEBv3zhA3B31Aw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T18:44:34.666501Z"},"content_sha256":"a9229dff0e30320145a475390e14e8c92c016802562959254554cccea6e1702e","schema_version":"1.0","event_id":"sha256:a9229dff0e30320145a475390e14e8c92c016802562959254554cccea6e1702e"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2016:SCZMXNKLM722ZVUN5A2H3AQQWP","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"LAMOST Observations of Flaring M Dwarfs in the Kepler Field","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A.-L. Luo, H.-Y. Chang, J.-N. Fu, L.-C. Huang, W.-H. Ip, Y.-F Wang, Y.-H. Hou, Y.-H. Song, Y. Zhang, Z.-H Cao","submitted_at":"2016-10-14T17:16:00Z","abstract_excerpt":"A sample of the LAMOST spectra of the early type M0-M3 dwarfs is compared with the Kepler observations. It is found that M dwarfs with strong chromospheric emission in $H_{\\alpha}$ have large flare activity in general. The rotational periods derived from the Kepler measurements have close correlations with the sizes of the flares, the power-law distribution index and the equivalent widths of the $H_{\\alpha}$ emission. A clear trend exists for higher magnetic activities being detected in faster rotating M dwarfs (rotation periods $<$ 20 day)."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1610.04541","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:53:07Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Ygyiun+Fjar1a32+4qHpT4AYXrxMbTjBoKSypg9IZiFEP46y1NJKrxLKVvRFxSYqufRXzYI4eaohaiu4tMGDCg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T18:44:34.666871Z"},"content_sha256":"5f98345601bebc626a5873c3dceb537bc1b155e4095473d5232b9a4ce5b66c03","schema_version":"1.0","event_id":"sha256:5f98345601bebc626a5873c3dceb537bc1b155e4095473d5232b9a4ce5b66c03"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/SCZMXNKLM722ZVUN5A2H3AQQWP/bundle.json","state_url":"https://pith.science/pith/SCZMXNKLM722ZVUN5A2H3AQQWP/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/SCZMXNKLM722ZVUN5A2H3AQQWP/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-05-25T18:44:34Z","links":{"resolver":"https://pith.science/pith/SCZMXNKLM722ZVUN5A2H3AQQWP","bundle":"https://pith.science/pith/SCZMXNKLM722ZVUN5A2H3AQQWP/bundle.json","state":"https://pith.science/pith/SCZMXNKLM722ZVUN5A2H3AQQWP/state.json","well_known_bundle":"https://pith.science/.well-known/pith/SCZMXNKLM722ZVUN5A2H3AQQWP/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2016:SCZMXNKLM722ZVUN5A2H3AQQWP","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"e696b4d8746fab4f04907f96f223a14ef2e4ece41e49180921efe22ae81b5ba9","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-10-14T17:16:00Z","title_canon_sha256":"d5f10eacb5a6cb033ee2b5c904e15f7515ff09dc6a46b569a6f142da184b36cd"},"schema_version":"1.0","source":{"id":"1610.04541","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1610.04541","created_at":"2026-05-18T00:53:07Z"},{"alias_kind":"arxiv_version","alias_value":"1610.04541v1","created_at":"2026-05-18T00:53:07Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1610.04541","created_at":"2026-05-18T00:53:07Z"},{"alias_kind":"pith_short_12","alias_value":"SCZMXNKLM722","created_at":"2026-05-18T12:30:44Z"},{"alias_kind":"pith_short_16","alias_value":"SCZMXNKLM722ZVUN","created_at":"2026-05-18T12:30:44Z"},{"alias_kind":"pith_short_8","alias_value":"SCZMXNKL","created_at":"2026-05-18T12:30:44Z"}],"graph_snapshots":[{"event_id":"sha256:5f98345601bebc626a5873c3dceb537bc1b155e4095473d5232b9a4ce5b66c03","target":"graph","created_at":"2026-05-18T00:53:07Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"A sample of the LAMOST spectra of the early type M0-M3 dwarfs is compared with the Kepler observations. It is found that M dwarfs with strong chromospheric emission in $H_{\\alpha}$ have large flare activity in general. The rotational periods derived from the Kepler measurements have close correlations with the sizes of the flares, the power-law distribution index and the equivalent widths of the $H_{\\alpha}$ emission. A clear trend exists for higher magnetic activities being detected in faster rotating M dwarfs (rotation periods $<$ 20 day).","authors_text":"A.-L. Luo, H.-Y. Chang, J.-N. Fu, L.-C. Huang, W.-H. Ip, Y.-F Wang, Y.-H. Hou, Y.-H. Song, Y. Zhang, Z.-H Cao","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-10-14T17:16:00Z","title":"LAMOST Observations of Flaring M Dwarfs in the Kepler Field"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1610.04541","kind":"arxiv","version":1},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:a9229dff0e30320145a475390e14e8c92c016802562959254554cccea6e1702e","target":"record","created_at":"2026-05-18T00:53:07Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"e696b4d8746fab4f04907f96f223a14ef2e4ece41e49180921efe22ae81b5ba9","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-10-14T17:16:00Z","title_canon_sha256":"d5f10eacb5a6cb033ee2b5c904e15f7515ff09dc6a46b569a6f142da184b36cd"},"schema_version":"1.0","source":{"id":"1610.04541","kind":"arxiv","version":1}},"canonical_sha256":"90b2cbb54b67f5acd68de8347d8210b3c8645dcf9690179418f78b3aa36064c6","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"90b2cbb54b67f5acd68de8347d8210b3c8645dcf9690179418f78b3aa36064c6","first_computed_at":"2026-05-18T00:53:07.178232Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:53:07.178232Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"yIYr2zILj+7w5T0djiL2EvPYI90WsmXlxO76q7LNauwW7+zEquU1mQ2jabyUr4qwhJ8cRXsr8CX7kq856TxjAA==","signature_status":"signed_v1","signed_at":"2026-05-18T00:53:07.178678Z","signed_message":"canonical_sha256_bytes"},"source_id":"1610.04541","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:a9229dff0e30320145a475390e14e8c92c016802562959254554cccea6e1702e","sha256:5f98345601bebc626a5873c3dceb537bc1b155e4095473d5232b9a4ce5b66c03"],"state_sha256":"9361f42399636acbec900bb10b90eb9e81b3bdc58b100a4e943c82386a2954ea"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"LTt2VxFzLUz/7u33KaK13FgL50cPaMrqsa/kUyIDObCL+zSLjC91sEAQBCUG9firVR2DEUv2Z68jw3hgCC7+Dg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-25T18:44:34.669295Z","bundle_sha256":"2739231a7fd579ea6c19af23cd7b8fdd1b39227336213177c91ec6dfe2000310"}}