{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2017:DUK7XRPPS5FPZROSYZXUHF6B7K","short_pith_number":"pith:DUK7XRPP","canonical_record":{"source":{"id":"1711.02111","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-11-06T19:01:00Z","cross_cats_sorted":[],"title_canon_sha256":"1a16a1a82042ca8f750b61297d635b9691e3703662a16aea2cd92b6a6c962be2","abstract_canon_sha256":"c4a7e9a6ccbba97487af01e37af6e8b15cbd61cb977e1920f1880b5cec6bd2bf"},"schema_version":"1.0"},"canonical_sha256":"1d15fbc5ef974afcc5d2c66f4397c1fa9c1cd18c77cc33c6406e4406861af156","source":{"kind":"arxiv","id":"1711.02111","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1711.02111","created_at":"2026-05-18T00:20:05Z"},{"alias_kind":"arxiv_version","alias_value":"1711.02111v2","created_at":"2026-05-18T00:20:05Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.02111","created_at":"2026-05-18T00:20:05Z"},{"alias_kind":"pith_short_12","alias_value":"DUK7XRPPS5FP","created_at":"2026-05-18T12:31:12Z"},{"alias_kind":"pith_short_16","alias_value":"DUK7XRPPS5FPZROS","created_at":"2026-05-18T12:31:12Z"},{"alias_kind":"pith_short_8","alias_value":"DUK7XRPP","created_at":"2026-05-18T12:31:12Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2017:DUK7XRPPS5FPZROSYZXUHF6B7K","target":"record","payload":{"canonical_record":{"source":{"id":"1711.02111","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-11-06T19:01:00Z","cross_cats_sorted":[],"title_canon_sha256":"1a16a1a82042ca8f750b61297d635b9691e3703662a16aea2cd92b6a6c962be2","abstract_canon_sha256":"c4a7e9a6ccbba97487af01e37af6e8b15cbd61cb977e1920f1880b5cec6bd2bf"},"schema_version":"1.0"},"canonical_sha256":"1d15fbc5ef974afcc5d2c66f4397c1fa9c1cd18c77cc33c6406e4406861af156","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:20:05.855721Z","signature_b64":"7nzo6H7ptofg9qaJmrGjRfZX1YQKUM32uorA3We/LcEgNesgyCS5nWFeTWT9wPtPwni7ZDgLhljf3+v1zwCYBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1d15fbc5ef974afcc5d2c66f4397c1fa9c1cd18c77cc33c6406e4406861af156","last_reissued_at":"2026-05-18T00:20:05.855143Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:20:05.855143Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1711.02111","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:20:05Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"2X4Oltde6nLdHXklEdIrQ2NoDPaUyxLgLpaMv83cYh1GMTCXvwt5wcY9zeoC50U80pBRCisdAMYp1m4Dfy58Aw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-18T18:51:08.169408Z"},"content_sha256":"45741e4a96278d38b86e2bf33aba728b43d053eccc50f455d2f727205423e143","schema_version":"1.0","event_id":"sha256:45741e4a96278d38b86e2bf33aba728b43d053eccc50f455d2f727205423e143"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2017:DUK7XRPPS5FPZROSYZXUHF6B7K","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"The KMOS$^\\mathrm{3D}$ Survey: rotating compact star forming galaxies and the decomposition of integrated line widths","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Beifiori, A. Galametz, D. Lutz, D. Rosario, D. Wilman, E. J. Nelson, E. Wisnioski, G. Brammer, H. \\\"Ubler, I. Momcheva, J. Chan, J. T. Mendel, K. Tadaki, L. J. Tacconi, M. Fabricius, M. Fossati, N. M. F\\\"orster Schreiber, P. G. van Dokkum, P. Lang, R. Bender, R. Genzel, R. I. Davies, R. L. Davies, R. Saglia, S. Belli, S. Wuyts","submitted_at":"2017-11-06T19:01:00Z","abstract_excerpt":"Using integral field spectroscopy we investigate the kinematic properties of 35 massive centrally-dense and compact star-forming galaxies (${\\log{\\overline{M}_*}}=11.1$, $\\log{(\\Sigma_\\mathrm{1kpc})}>9.5$, $\\log{(M_\\ast/r_e^{1.5})}>10.3$) at $z\\sim0.7-3.7$ within the KMOS$^\\mathrm{3D}$survey. We spatially resolve 23 compact star-forming galaxies (SFGs) and find that the majority are dominated by rotational motions with velocities ranging from {$95-500$ km s$^{-1}$}. The range of rotation velocities is reflected in a similar range of integrated H$\\alpha$ linewidths, $75-400$ km s$^{-1}$, consis"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.02111","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:20:05Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"ozlHPnAOFEWaVltMf1oJTfyzY5bxN8gEHt9miXoEsodQDiqPgYHPb42NEVpv3m/Ir/y8OpcgGUpMcISyH3X0BQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-18T18:51:08.170025Z"},"content_sha256":"192b396c3b53fb18d321caf22d3ea231f2ad98577cbc2c55598f418998d8dd95","schema_version":"1.0","event_id":"sha256:192b396c3b53fb18d321caf22d3ea231f2ad98577cbc2c55598f418998d8dd95"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/DUK7XRPPS5FPZROSYZXUHF6B7K/bundle.json","state_url":"https://pith.science/pith/DUK7XRPPS5FPZROSYZXUHF6B7K/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/DUK7XRPPS5FPZROSYZXUHF6B7K/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":"2026-05-18T18:51:08Z","links":{"resolver":"https://pith.science/pith/DUK7XRPPS5FPZROSYZXUHF6B7K","bundle":"https://pith.science/pith/DUK7XRPPS5FPZROSYZXUHF6B7K/bundle.json","state":"https://pith.science/pith/DUK7XRPPS5FPZROSYZXUHF6B7K/state.json","well_known_bundle":"https://pith.science/.well-known/pith/DUK7XRPPS5FPZROSYZXUHF6B7K/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2017:DUK7XRPPS5FPZROSYZXUHF6B7K","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":"c4a7e9a6ccbba97487af01e37af6e8b15cbd61cb977e1920f1880b5cec6bd2bf","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-11-06T19:01:00Z","title_canon_sha256":"1a16a1a82042ca8f750b61297d635b9691e3703662a16aea2cd92b6a6c962be2"},"schema_version":"1.0","source":{"id":"1711.02111","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1711.02111","created_at":"2026-05-18T00:20:05Z"},{"alias_kind":"arxiv_version","alias_value":"1711.02111v2","created_at":"2026-05-18T00:20:05Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.02111","created_at":"2026-05-18T00:20:05Z"},{"alias_kind":"pith_short_12","alias_value":"DUK7XRPPS5FP","created_at":"2026-05-18T12:31:12Z"},{"alias_kind":"pith_short_16","alias_value":"DUK7XRPPS5FPZROS","created_at":"2026-05-18T12:31:12Z"},{"alias_kind":"pith_short_8","alias_value":"DUK7XRPP","created_at":"2026-05-18T12:31:12Z"}],"graph_snapshots":[{"event_id":"sha256:192b396c3b53fb18d321caf22d3ea231f2ad98577cbc2c55598f418998d8dd95","target":"graph","created_at":"2026-05-18T00:20:05Z","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":"Using integral field spectroscopy we investigate the kinematic properties of 35 massive centrally-dense and compact star-forming galaxies (${\\log{\\overline{M}_*}}=11.1$, $\\log{(\\Sigma_\\mathrm{1kpc})}>9.5$, $\\log{(M_\\ast/r_e^{1.5})}>10.3$) at $z\\sim0.7-3.7$ within the KMOS$^\\mathrm{3D}$survey. We spatially resolve 23 compact star-forming galaxies (SFGs) and find that the majority are dominated by rotational motions with velocities ranging from {$95-500$ km s$^{-1}$}. The range of rotation velocities is reflected in a similar range of integrated H$\\alpha$ linewidths, $75-400$ km s$^{-1}$, consis","authors_text":"A. Beifiori, A. Galametz, D. Lutz, D. Rosario, D. Wilman, E. J. Nelson, E. Wisnioski, G. Brammer, H. \\\"Ubler, I. Momcheva, J. Chan, J. T. Mendel, K. Tadaki, L. J. Tacconi, M. Fabricius, M. Fossati, N. M. F\\\"orster Schreiber, P. G. van Dokkum, P. Lang, R. Bender, R. Genzel, R. I. Davies, R. L. Davies, R. Saglia, S. Belli, S. Wuyts","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-11-06T19:01:00Z","title":"The KMOS$^\\mathrm{3D}$ Survey: rotating compact star forming galaxies and the decomposition of integrated line widths"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.02111","kind":"arxiv","version":2},"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":"sha256:45741e4a96278d38b86e2bf33aba728b43d053eccc50f455d2f727205423e143","target":"record","created_at":"2026-05-18T00:20:05Z","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":"c4a7e9a6ccbba97487af01e37af6e8b15cbd61cb977e1920f1880b5cec6bd2bf","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-11-06T19:01:00Z","title_canon_sha256":"1a16a1a82042ca8f750b61297d635b9691e3703662a16aea2cd92b6a6c962be2"},"schema_version":"1.0","source":{"id":"1711.02111","kind":"arxiv","version":2}},"canonical_sha256":"1d15fbc5ef974afcc5d2c66f4397c1fa9c1cd18c77cc33c6406e4406861af156","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"1d15fbc5ef974afcc5d2c66f4397c1fa9c1cd18c77cc33c6406e4406861af156","first_computed_at":"2026-05-18T00:20:05.855143Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:20:05.855143Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"7nzo6H7ptofg9qaJmrGjRfZX1YQKUM32uorA3We/LcEgNesgyCS5nWFeTWT9wPtPwni7ZDgLhljf3+v1zwCYBQ==","signature_status":"signed_v1","signed_at":"2026-05-18T00:20:05.855721Z","signed_message":"canonical_sha256_bytes"},"source_id":"1711.02111","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:45741e4a96278d38b86e2bf33aba728b43d053eccc50f455d2f727205423e143","sha256:192b396c3b53fb18d321caf22d3ea231f2ad98577cbc2c55598f418998d8dd95"],"state_sha256":"fff52a45758e0cd4358c799294d1de75cfe8ca11e2000b8ffd9ee3ee77d304e3"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"13MFnCxHLHGUONJhObRQbWU7asTmGR/DPGzLpSePNiKRf2USlS6Uz1aS3ZacLCMKG1gUuf/5cS0fpoGfufcSDQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-18T18:51:08.172068Z","bundle_sha256":"bbe535aee43213d94adebf7b75ecc5d77b400feec7c2a34996c11223d90593ea"}}