{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2015:X4LTB7R2IZNRLMCZWU2EJVUMZ5","short_pith_number":"pith:X4LTB7R2","canonical_record":{"source":{"id":"1510.01944","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-10-07T13:56:19Z","cross_cats_sorted":[],"title_canon_sha256":"4fa377fb9987f32eaac70d623148371c9fb3573899d159771e64ca6d0271fccd","abstract_canon_sha256":"e4476f541a9fa44ca5520042ab84c960a081709860a0a8ea7a5b356a151554b5"},"schema_version":"1.0"},"canonical_sha256":"bf1730fe3a465b15b059b53444d68ccf647622fabc23fd2185c2e502de262018","source":{"kind":"arxiv","id":"1510.01944","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1510.01944","created_at":"2026-05-18T01:30:50Z"},{"alias_kind":"arxiv_version","alias_value":"1510.01944v1","created_at":"2026-05-18T01:30:50Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1510.01944","created_at":"2026-05-18T01:30:50Z"},{"alias_kind":"pith_short_12","alias_value":"X4LTB7R2IZNR","created_at":"2026-05-18T12:29:47Z"},{"alias_kind":"pith_short_16","alias_value":"X4LTB7R2IZNRLMCZ","created_at":"2026-05-18T12:29:47Z"},{"alias_kind":"pith_short_8","alias_value":"X4LTB7R2","created_at":"2026-05-18T12:29:47Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2015:X4LTB7R2IZNRLMCZWU2EJVUMZ5","target":"record","payload":{"canonical_record":{"source":{"id":"1510.01944","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-10-07T13:56:19Z","cross_cats_sorted":[],"title_canon_sha256":"4fa377fb9987f32eaac70d623148371c9fb3573899d159771e64ca6d0271fccd","abstract_canon_sha256":"e4476f541a9fa44ca5520042ab84c960a081709860a0a8ea7a5b356a151554b5"},"schema_version":"1.0"},"canonical_sha256":"bf1730fe3a465b15b059b53444d68ccf647622fabc23fd2185c2e502de262018","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:30:50.031296Z","signature_b64":"tnziurq6HHdaMQ0PJPXBF65ijdgVtUpKD2awdGqzGcOhSozFrDYqPcKC3Jc7i2DtuL/I5VEmwDuPJ45rgBgsDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bf1730fe3a465b15b059b53444d68ccf647622fabc23fd2185c2e502de262018","last_reissued_at":"2026-05-18T01:30:50.030703Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:30:50.030703Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1510.01944","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":"2026-05-18T01:30:50Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"8BSEEYeT282tvL9pBWEXpfJ3EvR+E9dfwDQq01grnRmDgEyEwBvdpb4/4ONrQ2HCXKn4JZnjFG1FNySVsKicCQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-01T05:24:38.578915Z"},"content_sha256":"8712bd9997fd8aa873f7366595fff632b8973e98e1620eb01c630189d15ac85b","schema_version":"1.0","event_id":"sha256:8712bd9997fd8aa873f7366595fff632b8973e98e1620eb01c630189d15ac85b"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2015:X4LTB7R2IZNRLMCZWU2EJVUMZ5","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"The super star cluster driven feedback in ESO338-IG04 and Haro 11","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Angela Adamo, Arjan Bik, G\\\"oran \\\"Ostlin, Jens Melinder, Matthew Hayes, Philippe Amram, Veronica Menacho","submitted_at":"2015-10-07T13:56:19Z","abstract_excerpt":"The stellar content of young massive star clusters emit large amounts of Lyman continuum photons and inject momentum into the inter stellar medium (ISM) by the strong stellar winds of the most massive stars in the cluster. When the most massive stars explode as supernovae, large amounts of mechanical energy are injected in the ISM. A detailed study of the ISM around these massive cluster provides insights on the effect of cluster feedback. We present high quality integral field spectroscopy taken with VLT/MUSE of two starburst galaxies: ESO 338-IG04 and Haro 11. Both galaxies contain a signifi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1510.01944","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":"2026-05-18T01:30:50Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"7bAGLBKZ9hDL+r1Cwia7jiOKzHK2PonwW6DIPkAVyUGTO8xFwnTHSjI+IJT1A6z288AQ9in/ogs+LGN/PWrQCg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-01T05:24:38.579655Z"},"content_sha256":"440fde9e2c910433a56efb8cce41a42443b82a8dd4f1cc4525902b46a8abee53","schema_version":"1.0","event_id":"sha256:440fde9e2c910433a56efb8cce41a42443b82a8dd4f1cc4525902b46a8abee53"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/X4LTB7R2IZNRLMCZWU2EJVUMZ5/bundle.json","state_url":"https://pith.science/pith/X4LTB7R2IZNRLMCZWU2EJVUMZ5/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/X4LTB7R2IZNRLMCZWU2EJVUMZ5/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":"2026-06-01T05:24:38Z","links":{"resolver":"https://pith.science/pith/X4LTB7R2IZNRLMCZWU2EJVUMZ5","bundle":"https://pith.science/pith/X4LTB7R2IZNRLMCZWU2EJVUMZ5/bundle.json","state":"https://pith.science/pith/X4LTB7R2IZNRLMCZWU2EJVUMZ5/state.json","well_known_bundle":"https://pith.science/.well-known/pith/X4LTB7R2IZNRLMCZWU2EJVUMZ5/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2015:X4LTB7R2IZNRLMCZWU2EJVUMZ5","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":"e4476f541a9fa44ca5520042ab84c960a081709860a0a8ea7a5b356a151554b5","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-10-07T13:56:19Z","title_canon_sha256":"4fa377fb9987f32eaac70d623148371c9fb3573899d159771e64ca6d0271fccd"},"schema_version":"1.0","source":{"id":"1510.01944","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1510.01944","created_at":"2026-05-18T01:30:50Z"},{"alias_kind":"arxiv_version","alias_value":"1510.01944v1","created_at":"2026-05-18T01:30:50Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1510.01944","created_at":"2026-05-18T01:30:50Z"},{"alias_kind":"pith_short_12","alias_value":"X4LTB7R2IZNR","created_at":"2026-05-18T12:29:47Z"},{"alias_kind":"pith_short_16","alias_value":"X4LTB7R2IZNRLMCZ","created_at":"2026-05-18T12:29:47Z"},{"alias_kind":"pith_short_8","alias_value":"X4LTB7R2","created_at":"2026-05-18T12:29:47Z"}],"graph_snapshots":[{"event_id":"sha256:440fde9e2c910433a56efb8cce41a42443b82a8dd4f1cc4525902b46a8abee53","target":"graph","created_at":"2026-05-18T01:30:50Z","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":"The stellar content of young massive star clusters emit large amounts of Lyman continuum photons and inject momentum into the inter stellar medium (ISM) by the strong stellar winds of the most massive stars in the cluster. When the most massive stars explode as supernovae, large amounts of mechanical energy are injected in the ISM. A detailed study of the ISM around these massive cluster provides insights on the effect of cluster feedback. We present high quality integral field spectroscopy taken with VLT/MUSE of two starburst galaxies: ESO 338-IG04 and Haro 11. Both galaxies contain a signifi","authors_text":"Angela Adamo, Arjan Bik, G\\\"oran \\\"Ostlin, Jens Melinder, Matthew Hayes, Philippe Amram, Veronica Menacho","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-10-07T13:56:19Z","title":"The super star cluster driven feedback in ESO338-IG04 and Haro 11"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1510.01944","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":"sha256:8712bd9997fd8aa873f7366595fff632b8973e98e1620eb01c630189d15ac85b","target":"record","created_at":"2026-05-18T01:30:50Z","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":"e4476f541a9fa44ca5520042ab84c960a081709860a0a8ea7a5b356a151554b5","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-10-07T13:56:19Z","title_canon_sha256":"4fa377fb9987f32eaac70d623148371c9fb3573899d159771e64ca6d0271fccd"},"schema_version":"1.0","source":{"id":"1510.01944","kind":"arxiv","version":1}},"canonical_sha256":"bf1730fe3a465b15b059b53444d68ccf647622fabc23fd2185c2e502de262018","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"bf1730fe3a465b15b059b53444d68ccf647622fabc23fd2185c2e502de262018","first_computed_at":"2026-05-18T01:30:50.030703Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:30:50.030703Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"tnziurq6HHdaMQ0PJPXBF65ijdgVtUpKD2awdGqzGcOhSozFrDYqPcKC3Jc7i2DtuL/I5VEmwDuPJ45rgBgsDw==","signature_status":"signed_v1","signed_at":"2026-05-18T01:30:50.031296Z","signed_message":"canonical_sha256_bytes"},"source_id":"1510.01944","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:8712bd9997fd8aa873f7366595fff632b8973e98e1620eb01c630189d15ac85b","sha256:440fde9e2c910433a56efb8cce41a42443b82a8dd4f1cc4525902b46a8abee53"],"state_sha256":"5c42d56c91e7bf57af727f5eb12308d71234a8bea3bcbe073829aaeb3e07b30d"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"fGSsBCFAfR5Oyx3Mvm54eGFjFhSx+lxKpK5i8WadAsL/rRhDprd4svVyu5vIoEEGWgc1cyUdv2vvEfIommoTCA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-01T05:24:38.584396Z","bundle_sha256":"f182e526c45070d6b1d06e07cb87d59a005550d68dbbef18e4c021d28aaf8b72"}}