{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2010:F4BML23MIJAXSOJK4N5TVOIGMS","short_pith_number":"pith:F4BML23M","canonical_record":{"source":{"id":"1009.1642","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-09-08T20:22:57Z","cross_cats_sorted":[],"title_canon_sha256":"8d5e104df58a554be0ca9b34212e7a2a2744c3cb7ebcf74e4726a6f807ccebb6","abstract_canon_sha256":"c0f2125d8b446d73029e7a0be41bde22ad58dbca3b10e1071c49ce5071787c67"},"schema_version":"1.0"},"canonical_sha256":"2f02c5eb6c424179392ae37b3ab90664ba11d175ff93179bc3dc68e79749a0fc","source":{"kind":"arxiv","id":"1009.1642","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1009.1642","created_at":"2026-05-18T02:05:32Z"},{"alias_kind":"arxiv_version","alias_value":"1009.1642v1","created_at":"2026-05-18T02:05:32Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1009.1642","created_at":"2026-05-18T02:05:32Z"},{"alias_kind":"pith_short_12","alias_value":"F4BML23MIJAX","created_at":"2026-05-18T12:26:06Z"},{"alias_kind":"pith_short_16","alias_value":"F4BML23MIJAXSOJK","created_at":"2026-05-18T12:26:06Z"},{"alias_kind":"pith_short_8","alias_value":"F4BML23M","created_at":"2026-05-18T12:26:06Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2010:F4BML23MIJAXSOJK4N5TVOIGMS","target":"record","payload":{"canonical_record":{"source":{"id":"1009.1642","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-09-08T20:22:57Z","cross_cats_sorted":[],"title_canon_sha256":"8d5e104df58a554be0ca9b34212e7a2a2744c3cb7ebcf74e4726a6f807ccebb6","abstract_canon_sha256":"c0f2125d8b446d73029e7a0be41bde22ad58dbca3b10e1071c49ce5071787c67"},"schema_version":"1.0"},"canonical_sha256":"2f02c5eb6c424179392ae37b3ab90664ba11d175ff93179bc3dc68e79749a0fc","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:05:32.988668Z","signature_b64":"lKNb6Bwb71QkeDBfbXlF2JHAbG2P8cgoI8F1D+LtnH9MB+z/16PFn4ca8jGlQLJ4JP3ZwIAktUQCRjm9GbutDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2f02c5eb6c424179392ae37b3ab90664ba11d175ff93179bc3dc68e79749a0fc","last_reissued_at":"2026-05-18T02:05:32.987889Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:05:32.987889Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1009.1642","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":"2026-05-18T02:05:32Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"MGjETo2x3WvThwI4rD/Rq3ztkwR9dOawKnD0A0a/t1CrGYWEcgo6d3jmTpL9osVQCFb2GhLiNrgO2Xtz9mviCg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-28T00:02:11.737582Z"},"content_sha256":"aba31743fb59d9bee5f1add9bfbdae38de63c5c61b1a591da2e9025994d30612","schema_version":"1.0","event_id":"sha256:aba31743fb59d9bee5f1add9bfbdae38de63c5c61b1a591da2e9025994d30612"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2010:F4BML23MIJAXSOJK4N5TVOIGMS","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Diffuse Far-UV Line Emission from the Low-Redshift Lyman Break Galaxy Analog KISSR242","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Claus Leitherer (STScI), James C. Green (CASA/University of Colorado), Kevin France, Nicholas Nell","submitted_at":"2010-09-08T20:22:57Z","abstract_excerpt":"We present new ultraviolet (UV) observations of the luminous compact blue galaxy KISSR242, obtained with the HST-COS. We identify multiple resolved sub-arcsecond near-UV sources within the COS aperture. The far-UV spectroscopic data show strong outflow absorption lines, consistent with feedback processes related to an episode of massive star-formation. OI, CII, and SiII--SiIV are observed with a mean outflow velocity v_{out} = -60 km/s. We also detect faint fine-structure emission lines of singly ionized silicon for the first time in a low-redshift starburst galaxy. These emissions have been s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1009.1642","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":"2026-05-18T02:05:32Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"s21kNOEA4H7Ka4a7PhUN3enL5oWaT91J95+rJHlt6LnOljJtapZ7PYM00joTNh3JaoWf1AluqVSso8EiFaeZAg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-28T00:02:11.738328Z"},"content_sha256":"6b02765b38b0a143f05cd1a8be9d08a3d855cf17e582448f0a137d9e5e950a7a","schema_version":"1.0","event_id":"sha256:6b02765b38b0a143f05cd1a8be9d08a3d855cf17e582448f0a137d9e5e950a7a"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/F4BML23MIJAXSOJK4N5TVOIGMS/bundle.json","state_url":"https://pith.science/pith/F4BML23MIJAXSOJK4N5TVOIGMS/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/F4BML23MIJAXSOJK4N5TVOIGMS/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":"2026-05-28T00:02:11Z","links":{"resolver":"https://pith.science/pith/F4BML23MIJAXSOJK4N5TVOIGMS","bundle":"https://pith.science/pith/F4BML23MIJAXSOJK4N5TVOIGMS/bundle.json","state":"https://pith.science/pith/F4BML23MIJAXSOJK4N5TVOIGMS/state.json","well_known_bundle":"https://pith.science/.well-known/pith/F4BML23MIJAXSOJK4N5TVOIGMS/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2010:F4BML23MIJAXSOJK4N5TVOIGMS","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":"c0f2125d8b446d73029e7a0be41bde22ad58dbca3b10e1071c49ce5071787c67","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-09-08T20:22:57Z","title_canon_sha256":"8d5e104df58a554be0ca9b34212e7a2a2744c3cb7ebcf74e4726a6f807ccebb6"},"schema_version":"1.0","source":{"id":"1009.1642","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1009.1642","created_at":"2026-05-18T02:05:32Z"},{"alias_kind":"arxiv_version","alias_value":"1009.1642v1","created_at":"2026-05-18T02:05:32Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1009.1642","created_at":"2026-05-18T02:05:32Z"},{"alias_kind":"pith_short_12","alias_value":"F4BML23MIJAX","created_at":"2026-05-18T12:26:06Z"},{"alias_kind":"pith_short_16","alias_value":"F4BML23MIJAXSOJK","created_at":"2026-05-18T12:26:06Z"},{"alias_kind":"pith_short_8","alias_value":"F4BML23M","created_at":"2026-05-18T12:26:06Z"}],"graph_snapshots":[{"event_id":"sha256:6b02765b38b0a143f05cd1a8be9d08a3d855cf17e582448f0a137d9e5e950a7a","target":"graph","created_at":"2026-05-18T02:05:32Z","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":"We present new ultraviolet (UV) observations of the luminous compact blue galaxy KISSR242, obtained with the HST-COS. We identify multiple resolved sub-arcsecond near-UV sources within the COS aperture. The far-UV spectroscopic data show strong outflow absorption lines, consistent with feedback processes related to an episode of massive star-formation. OI, CII, and SiII--SiIV are observed with a mean outflow velocity v_{out} = -60 km/s. We also detect faint fine-structure emission lines of singly ionized silicon for the first time in a low-redshift starburst galaxy. These emissions have been s","authors_text":"Claus Leitherer (STScI), James C. Green (CASA/University of Colorado), Kevin France, Nicholas Nell","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-09-08T20:22:57Z","title":"Diffuse Far-UV Line Emission from the Low-Redshift Lyman Break Galaxy Analog KISSR242"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1009.1642","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:aba31743fb59d9bee5f1add9bfbdae38de63c5c61b1a591da2e9025994d30612","target":"record","created_at":"2026-05-18T02:05:32Z","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":"c0f2125d8b446d73029e7a0be41bde22ad58dbca3b10e1071c49ce5071787c67","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-09-08T20:22:57Z","title_canon_sha256":"8d5e104df58a554be0ca9b34212e7a2a2744c3cb7ebcf74e4726a6f807ccebb6"},"schema_version":"1.0","source":{"id":"1009.1642","kind":"arxiv","version":1}},"canonical_sha256":"2f02c5eb6c424179392ae37b3ab90664ba11d175ff93179bc3dc68e79749a0fc","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"2f02c5eb6c424179392ae37b3ab90664ba11d175ff93179bc3dc68e79749a0fc","first_computed_at":"2026-05-18T02:05:32.987889Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:05:32.987889Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"lKNb6Bwb71QkeDBfbXlF2JHAbG2P8cgoI8F1D+LtnH9MB+z/16PFn4ca8jGlQLJ4JP3ZwIAktUQCRjm9GbutDA==","signature_status":"signed_v1","signed_at":"2026-05-18T02:05:32.988668Z","signed_message":"canonical_sha256_bytes"},"source_id":"1009.1642","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:aba31743fb59d9bee5f1add9bfbdae38de63c5c61b1a591da2e9025994d30612","sha256:6b02765b38b0a143f05cd1a8be9d08a3d855cf17e582448f0a137d9e5e950a7a"],"state_sha256":"5df8bad147956f4770c89991f4af97c5fe35212088881a30232f2186f8e5e295"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"AXlh7C8Yun9GqQ3DBDKa6uYARhEe2I3YJrzNlKXdLTgIWsQJGJeku0KbUJXgdXS8jsQTcQ8SlJpcoO3sIKt8DA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-28T00:02:11.741762Z","bundle_sha256":"1191d382d5d4cd9a904162f9eadd81505b46ea69b4713bd62c7ce3bdf7ebd2a7"}}