{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2014:VELE24YSNFZ5KZ3SWBCKMCOI6T","short_pith_number":"pith:VELE24YS","canonical_record":{"source":{"id":"1410.6488","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-10-23T20:01:03Z","cross_cats_sorted":[],"title_canon_sha256":"3d5043ffa82f82fe61892716d7cf130cd77f9939cf489812ec50f50f7775d959","abstract_canon_sha256":"32b47a913e7c07790b54a259c15e4aa655dc07613518d6fe320f6b7ed17443e1"},"schema_version":"1.0"},"canonical_sha256":"a9164d73126973d56772b044a609c8f4c4b4ce827f3af3116341a213d91b085c","source":{"kind":"arxiv","id":"1410.6488","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1410.6488","created_at":"2026-05-18T01:41:40Z"},{"alias_kind":"arxiv_version","alias_value":"1410.6488v1","created_at":"2026-05-18T01:41:40Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1410.6488","created_at":"2026-05-18T01:41:40Z"},{"alias_kind":"pith_short_12","alias_value":"VELE24YSNFZ5","created_at":"2026-05-18T12:28:52Z"},{"alias_kind":"pith_short_16","alias_value":"VELE24YSNFZ5KZ3S","created_at":"2026-05-18T12:28:52Z"},{"alias_kind":"pith_short_8","alias_value":"VELE24YS","created_at":"2026-05-18T12:28:52Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2014:VELE24YSNFZ5KZ3SWBCKMCOI6T","target":"record","payload":{"canonical_record":{"source":{"id":"1410.6488","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-10-23T20:01:03Z","cross_cats_sorted":[],"title_canon_sha256":"3d5043ffa82f82fe61892716d7cf130cd77f9939cf489812ec50f50f7775d959","abstract_canon_sha256":"32b47a913e7c07790b54a259c15e4aa655dc07613518d6fe320f6b7ed17443e1"},"schema_version":"1.0"},"canonical_sha256":"a9164d73126973d56772b044a609c8f4c4b4ce827f3af3116341a213d91b085c","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:40.344286Z","signature_b64":"q6Xc0yCrwvYps9ZMGDNsIR1Wt4iH1CP642dUhKzBlEAYc5pSTZDZ03weA8TKBl2qruCpqnL2Q0sUtULwM87TCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a9164d73126973d56772b044a609c8f4c4b4ce827f3af3116341a213d91b085c","last_reissued_at":"2026-05-18T01:41:40.343555Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:40.343555Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1410.6488","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":"2026-05-18T01:41:40Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"d7E9RvboCqEI7ww0xByhwi0HlEGLxWcx8cV9jDyLL3NZHOEb2JVICOqwRNI1ojGt6qRcBvMGaGogJmpXB3zjCQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T01:09:26.055515Z"},"content_sha256":"6fbc67142b5d5c446136cf7fa698f7972c89b1d01d7a7c20b8e51c3205c97c22","schema_version":"1.0","event_id":"sha256:6fbc67142b5d5c446136cf7fa698f7972c89b1d01d7a7c20b8e51c3205c97c22"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2014:VELE24YSNFZ5KZ3SWBCKMCOI6T","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"The Near-Ultraviolet Luminosity Function of Young, Early M-Type Dwarf Stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Andrea Buccino, Andrew W. Mann, Christoph Baranec, David James, Eric Gaidos, Megan Ansdell, Nicholas M. Law, Pablo Mauas, Reed Riddle, Romina Petrucci, Sebastien Lepine","submitted_at":"2014-10-23T20:01:03Z","abstract_excerpt":"Planets orbiting within the close-in habitable zones of M dwarf stars will be exposed to elevated high-energy radiation driven by strong magneto-hydrodynamic dynamos during stellar youth. Near-ultraviolet (NUV) irradiation can erode and alter the chemistry of planetary atmospheres, and a quantitative description of the evolution of NUV emission from M dwarfs is needed when modeling these effects. We investigated the NUV luminosity evolution of early M-type dwarfs by cross-correlating the Lepine & Gaidos (2011) catalog of bright M dwarfs with the GALEX catalog of NUV (1771-2831A) sources. Of th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1410.6488","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":"2026-05-18T01:41:40Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"fiO9fNfWDc1GTc2xXOvE6g84tbsK59G2O0way+09w9SO8+GXvpeIYFOJmXXeR65fWwMdh6fE372FyPZN1oqqAg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T01:09:26.056097Z"},"content_sha256":"c7571c401f9845fd1dddd3397eb07c29b49b17cedeb6cded25a0269434568d8b","schema_version":"1.0","event_id":"sha256:c7571c401f9845fd1dddd3397eb07c29b49b17cedeb6cded25a0269434568d8b"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/VELE24YSNFZ5KZ3SWBCKMCOI6T/bundle.json","state_url":"https://pith.science/pith/VELE24YSNFZ5KZ3SWBCKMCOI6T/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/VELE24YSNFZ5KZ3SWBCKMCOI6T/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":"2026-05-26T01:09:26Z","links":{"resolver":"https://pith.science/pith/VELE24YSNFZ5KZ3SWBCKMCOI6T","bundle":"https://pith.science/pith/VELE24YSNFZ5KZ3SWBCKMCOI6T/bundle.json","state":"https://pith.science/pith/VELE24YSNFZ5KZ3SWBCKMCOI6T/state.json","well_known_bundle":"https://pith.science/.well-known/pith/VELE24YSNFZ5KZ3SWBCKMCOI6T/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2014:VELE24YSNFZ5KZ3SWBCKMCOI6T","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":"32b47a913e7c07790b54a259c15e4aa655dc07613518d6fe320f6b7ed17443e1","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-10-23T20:01:03Z","title_canon_sha256":"3d5043ffa82f82fe61892716d7cf130cd77f9939cf489812ec50f50f7775d959"},"schema_version":"1.0","source":{"id":"1410.6488","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1410.6488","created_at":"2026-05-18T01:41:40Z"},{"alias_kind":"arxiv_version","alias_value":"1410.6488v1","created_at":"2026-05-18T01:41:40Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1410.6488","created_at":"2026-05-18T01:41:40Z"},{"alias_kind":"pith_short_12","alias_value":"VELE24YSNFZ5","created_at":"2026-05-18T12:28:52Z"},{"alias_kind":"pith_short_16","alias_value":"VELE24YSNFZ5KZ3S","created_at":"2026-05-18T12:28:52Z"},{"alias_kind":"pith_short_8","alias_value":"VELE24YS","created_at":"2026-05-18T12:28:52Z"}],"graph_snapshots":[{"event_id":"sha256:c7571c401f9845fd1dddd3397eb07c29b49b17cedeb6cded25a0269434568d8b","target":"graph","created_at":"2026-05-18T01:41:40Z","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":"Planets orbiting within the close-in habitable zones of M dwarf stars will be exposed to elevated high-energy radiation driven by strong magneto-hydrodynamic dynamos during stellar youth. Near-ultraviolet (NUV) irradiation can erode and alter the chemistry of planetary atmospheres, and a quantitative description of the evolution of NUV emission from M dwarfs is needed when modeling these effects. We investigated the NUV luminosity evolution of early M-type dwarfs by cross-correlating the Lepine & Gaidos (2011) catalog of bright M dwarfs with the GALEX catalog of NUV (1771-2831A) sources. Of th","authors_text":"Andrea Buccino, Andrew W. Mann, Christoph Baranec, David James, Eric Gaidos, Megan Ansdell, Nicholas M. Law, Pablo Mauas, Reed Riddle, Romina Petrucci, Sebastien Lepine","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-10-23T20:01:03Z","title":"The Near-Ultraviolet Luminosity Function of Young, Early M-Type Dwarf Stars"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1410.6488","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":"sha256:6fbc67142b5d5c446136cf7fa698f7972c89b1d01d7a7c20b8e51c3205c97c22","target":"record","created_at":"2026-05-18T01:41:40Z","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":"32b47a913e7c07790b54a259c15e4aa655dc07613518d6fe320f6b7ed17443e1","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-10-23T20:01:03Z","title_canon_sha256":"3d5043ffa82f82fe61892716d7cf130cd77f9939cf489812ec50f50f7775d959"},"schema_version":"1.0","source":{"id":"1410.6488","kind":"arxiv","version":1}},"canonical_sha256":"a9164d73126973d56772b044a609c8f4c4b4ce827f3af3116341a213d91b085c","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"a9164d73126973d56772b044a609c8f4c4b4ce827f3af3116341a213d91b085c","first_computed_at":"2026-05-18T01:41:40.343555Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:41:40.343555Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"q6Xc0yCrwvYps9ZMGDNsIR1Wt4iH1CP642dUhKzBlEAYc5pSTZDZ03weA8TKBl2qruCpqnL2Q0sUtULwM87TCw==","signature_status":"signed_v1","signed_at":"2026-05-18T01:41:40.344286Z","signed_message":"canonical_sha256_bytes"},"source_id":"1410.6488","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:6fbc67142b5d5c446136cf7fa698f7972c89b1d01d7a7c20b8e51c3205c97c22","sha256:c7571c401f9845fd1dddd3397eb07c29b49b17cedeb6cded25a0269434568d8b"],"state_sha256":"6b248823586961e4339de7e5fd593459f40bd7d845456c1b2cb5ea6e4189ce8b"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"k1Jf2+dhFU1XC1XnY1izYAlEYuwzZyXgDAwlkB+SOF/WG8wZ+KGxWzSUErzovkrZmVbRiT4FV+LJS/0+rZ2hBQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-26T01:09:26.059234Z","bundle_sha256":"677f20f6704fb1c6dfd9db6de8fba8958f4b02046a7013217e3e9d9ddf591735"}}