{"as_of":"2026-08-23T05:47:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:c074261d0a2319c1acd1dbf5b2424cf7760ea8362b7f232ee4101a1f2beff444","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":12,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":12,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-22T06:32:14.747728+00:00","state":"measured"},{"denominator":12,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":12,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T23:13:10.642301Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-06-29T01:22:56.356974Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1205.3030","last_updated":"2012-06-13T09:18:47Z","snapshot_observed_at":"2026-08-15T04:09:57.294777Z","submitted_at":"2012-05-14T14:00:20Z","title":"Rapid growth of gas-giant cores by pebble accretion","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1205.3030","snapshot_observed_at":"2026-08-11T23:13:10.642301Z","title":"Astronomy & Astrophysics 544, A32","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.02785","last_updated":"2024-12-03T19:26:19Z","snapshot_observed_at":"2026-08-13T00:29:58.769038Z","submitted_at":"2024-12-03T19:26:19Z","title":"Accretion of Uranus and Neptune: confronting different giant impact scenarios","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-11T23:13:10.642301Z"},"links":{"cited_paper":"/paper/1205.3030","citing_paper":"/paper/2412.02785"},"observation_digest":"sha256:38558ced94934067ce8bc422c2138894149b1c14beac9977bdb3628fd477a786","observation_id":"814ef0bc-8c7f-4120-b416-d158e89759f9","resolution":{"observed_at":"2026-08-11T23:13:10.642301Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1205.3030","last_updated":"2012-06-13T09:18:47Z","snapshot_observed_at":"2026-08-15T04:09:57.294777Z","submitted_at":"2012-05-14T14:00:20Z","title":"Rapid growth of gas-giant cores by pebble accretion","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1205.3030","snapshot_observed_at":"2026-08-11T21:00:08.570176Z","title":"ApJ 864, no","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2412.05099","last_updated":"2024-12-06T14:55:59Z","snapshot_observed_at":"2026-08-13T12:20:55.897665Z","submitted_at":"2024-12-06T14:55:59Z","title":"C/O ratios in self-gravitating protoplanetary discs with dust evolution","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-11T21:00:08.570176Z"},"links":{"cited_paper":"/paper/1205.3030","citing_paper":"/paper/2412.05099"},"observation_digest":"sha256:912be19cc5ec024eea7ec9680b7f33f35b892eb7918a92b65808cc251f0037a3","observation_id":"4fb8360f-4ba1-4ab6-84d2-192dbe1398aa","resolution":{"observed_at":"2026-08-11T21:00:08.570176Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1205.3030","last_updated":"2012-06-13T09:18:47Z","snapshot_observed_at":"2026-08-15T04:09:57.294777Z","submitted_at":"2012-05-14T14:00:20Z","title":"Rapid growth of gas-giant cores by pebble accretion","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1205.3030","snapshot_observed_at":"2026-08-11T10:51:27.448007Z","title":"Lambrechts and A","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2412.16278","last_updated":"2024-12-20T19:00:00Z","snapshot_observed_at":"2026-08-15T06:20:17.317894Z","submitted_at":"2024-12-20T19:00:00Z","title":"Correlation between planet formation rate and gas surface density: an analog of Kennicutt Schmidt law for planet formation","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-11T10:51:27.448007Z"},"links":{"cited_paper":"/paper/1205.3030","citing_paper":"/paper/2412.16278"},"observation_digest":"sha256:debf66373257d521307386f13326e00ba6f7fbe3c39c395a1d9af68db9909092","observation_id":"d8d0fec3-5a96-46db-90bd-4e74df3c7774","resolution":{"observed_at":"2026-08-11T10:51:27.448007Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1205.3030","last_updated":"2012-06-13T09:18:47Z","snapshot_observed_at":"2026-08-15T04:09:57.294777Z","submitted_at":"2012-05-14T14:00:20Z","title":"Rapid growth of gas-giant cores by pebble accretion","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1205.3030","snapshot_observed_at":"2026-08-06T20:49:14.611265Z","title":"Astronomy & Astrophysics 544, A32","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.01826","last_updated":"2025-07-02T15:41:34Z","snapshot_observed_at":"2026-08-19T04:33:47.022340Z","submitted_at":"2025-07-02T15:41:34Z","title":"Dynamical origin of Theia, the last giant impactor on Earth","version":1},"reference_index":2012,"source":"pdf_text","source_observed_at":"2026-08-06T20:49:14.611265Z"},"links":{"cited_paper":"/paper/1205.3030","citing_paper":"/paper/2507.01826"},"observation_digest":"sha256:e2d410acdf53a1781a54b4996c4097fbdc4488b7a5bafd8586d0eb536c964583","observation_id":"dafdaf03-302d-4a09-9f52-7f8d02288c7a","resolution":{"observed_at":"2026-08-06T20:49:14.611265Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1205.3030","last_updated":"2012-06-13T09:18:47Z","snapshot_observed_at":"2026-08-15T04:09:57.294777Z","submitted_at":"2012-05-14T14:00:20Z","title":"Rapid growth of gas-giant cores by pebble accretion","version":2},"cited_work":{"arxiv_id":"1205.3030","doi":null,"metadata_source":"pith","pith_arxiv_id":"1205.3030","snapshot_observed_at":"2026-06-29T01:22:56.356974Z","title":"Rapid growth of gas-giant cores by pebble accretion","venue":"astro-ph.EP","work_id":"9d7c33c9-d91a-410a-9d95-b47dbf27d054","year":2012},"citing_paper":{"arxiv_id":"2510.17955","last_updated":"2026-04-16T18:34:05Z","snapshot_observed_at":"2026-08-03T04:06:26.356878Z","submitted_at":"2025-10-20T18:00:00Z","title":"Sub-Snowline Formation of Gas-Giant Planets in Binary Systems","version":3},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1205.3030","citing_paper":"/paper/2510.17955"},"observation_digest":"sha256:e040722713b87962c327b8d8f678b1dda8e882e81ddd6fdfd0e3dbea82111e4f","observation_id":"ab56f502-4553-4086-9650-af75be483e49","resolution":{"observed_at":"2026-05-18T05:45:55.867724Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1205.3030","last_updated":"2012-06-13T09:18:47Z","snapshot_observed_at":"2026-08-15T04:09:57.294777Z","submitted_at":"2012-05-14T14:00:20Z","title":"Rapid growth of gas-giant cores by pebble accretion","version":2},"cited_work":{"arxiv_id":"1205.3030","doi":null,"metadata_source":"pith","pith_arxiv_id":"1205.3030","snapshot_observed_at":"2026-06-29T01:22:56.356974Z","title":"Rapid growth of gas-giant cores by pebble accretion","venue":"astro-ph.EP","work_id":"9d7c33c9-d91a-410a-9d95-b47dbf27d054","year":2012},"citing_paper":{"arxiv_id":"2605.18950","last_updated":"2026-05-18T18:00:02Z","snapshot_observed_at":"2026-08-15T06:40:25.015722Z","submitted_at":"2026-05-18T18:00:02Z","title":"Planetary formation tracks on the Hertzsprung-Russell diagram: Visualising the processes of giant planet growth","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1205.3030","citing_paper":"/paper/2605.18950"},"observation_digest":"sha256:71f1d4622be962e5c0f9212a543dd134e781e367434f8a5b64dbe5f3ced5f010","observation_id":"1789b524-b2cc-4bd7-bd39-255c28ad39eb","resolution":{"observed_at":"2026-05-20T07:53:08.411587Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1205.3030","last_updated":"2012-06-13T09:18:47Z","snapshot_observed_at":"2026-08-15T04:09:57.294777Z","submitted_at":"2012-05-14T14:00:20Z","title":"Rapid growth of gas-giant cores by pebble accretion","version":2},"cited_work":{"arxiv_id":"1205.3030","doi":null,"metadata_source":"pith","pith_arxiv_id":"1205.3030","snapshot_observed_at":"2026-06-29T01:22:56.356974Z","title":"Rapid growth of gas-giant cores by pebble accretion","venue":"astro-ph.EP","work_id":"9d7c33c9-d91a-410a-9d95-b47dbf27d054","year":2012},"citing_paper":{"arxiv_id":"2606.27476","last_updated":"2026-06-25T18:56:07Z","snapshot_observed_at":"2026-08-16T06:47:59.239267Z","submitted_at":"2026-06-25T18:56:07Z","title":"Chemical Divergence and Water Depletion: Gas Properties of Evolved Upper Scorpius Disks Revealed by JWST/MIRI","version":1},"reference_index":252,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1205.3030","citing_paper":"/paper/2606.27476"},"observation_digest":"sha256:b8078afc7f06ec74ce762609933d2f64326551ee1761c2966993bdc4b11defca","observation_id":"eeba47cf-750e-4253-9a42-09ba6b8da2d6","resolution":{"observed_at":"2026-06-29T01:12:55.712794Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1205.3030","last_updated":"2012-06-13T09:18:47Z","snapshot_observed_at":"2026-08-15T04:09:57.294777Z","submitted_at":"2012-05-14T14:00:20Z","title":"Rapid growth of gas-giant cores by pebble accretion","version":2},"cited_work":{"arxiv_id":"1205.3030","doi":null,"metadata_source":"pith","pith_arxiv_id":"1205.3030","snapshot_observed_at":"2026-06-29T01:22:56.356974Z","title":"Rapid growth of gas-giant cores by pebble accretion","venue":"astro-ph.EP","work_id":"9d7c33c9-d91a-410a-9d95-b47dbf27d054","year":2012},"citing_paper":{"arxiv_id":"2606.27477","last_updated":"2026-06-25T18:56:07Z","snapshot_observed_at":"2026-08-04T12:41:17.185796Z","submitted_at":"2026-06-25T18:56:07Z","title":"From Young to Older Disks: JWST/MIRI Evidence for Fading Molecular Emission and Hints for Elevated C/O in Upper Scorpius","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1205.3030","citing_paper":"/paper/2606.27477"},"observation_digest":"sha256:fa0c16828909a966415c1d127c384be1606774f35aa082c71e477a93521f0095","observation_id":"9eb53295-dc34-43fb-b50c-cf1b7ddc26c0","resolution":{"observed_at":"2026-06-29T01:22:56.358408Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1205.3030","last_updated":"2012-06-13T09:18:47Z","snapshot_observed_at":"2026-08-15T04:09:57.294777Z","submitted_at":"2012-05-14T14:00:20Z","title":"Rapid growth of gas-giant cores by pebble accretion","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1205.3030","snapshot_observed_at":"2026-08-01T13:29:13.802618Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19118","last_updated":"2026-07-21T14:04:46Z","snapshot_observed_at":"2026-08-13T09:02:40.861465Z","submitted_at":"2026-07-21T14:04:46Z","title":"Dynamical formation of long-period exoplanets systems in evolving binary stars","version":1},"reference_index":112,"source":"arxiv_source","source_observed_at":"2026-08-01T13:29:13.802618Z"},"links":{"cited_paper":"/paper/1205.3030","citing_paper":"/paper/2607.19118"},"observation_digest":"sha256:7f47bf3db45f18ccda1b9706c2d7d616a5b55178ed2921eafd8851c8dce7fef6","observation_id":"ac16165a-ea82-449b-82d6-aa25bdfe6096","resolution":{"observed_at":"2026-08-01T13:29:13.802618Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1205.3030","last_updated":"2012-06-13T09:18:47Z","snapshot_observed_at":"2026-08-15T04:09:57.294777Z","submitted_at":"2012-05-14T14:00:20Z","title":"Rapid growth of gas-giant cores by pebble accretion","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1205.3030","snapshot_observed_at":"2026-08-01T10:41:57.450482Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.20158","last_updated":"2026-08-15T17:04:31Z","snapshot_observed_at":"2026-08-21T22:11:28.708991Z","submitted_at":"2026-07-22T13:55:07Z","title":"Dust and Gas Transport in Substructured Nonideal MHD Wind-Launching Disks with Embedded Planets","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-01T10:41:57.450482Z"},"links":{"cited_paper":"/paper/1205.3030","citing_paper":"/paper/2607.20158"},"observation_digest":"sha256:64a919a71314d5bcb444fc76553eead0325a3eb95e838e7c51e9d9bcb2ca6502","observation_id":"0f469801-b7fa-42b5-bd6c-dadb0c8efc6e","resolution":{"observed_at":"2026-08-01T10:41:57.450482Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1205.3030","last_updated":"2012-06-13T09:18:47Z","snapshot_observed_at":"2026-08-15T04:09:57.294777Z","submitted_at":"2012-05-14T14:00:20Z","title":"Rapid growth of gas-giant cores by pebble accretion","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1205.3030","snapshot_observed_at":"2026-08-03T04:44:10.007392Z","title":", keywords =","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.29558","last_updated":"2026-07-31T15:49:18Z","snapshot_observed_at":"2026-08-16T00:34:13.883275Z","submitted_at":"2026-07-31T15:49:18Z","title":"Warm Sub-Saturns Orbiting Single Stars Are Spin-Orbit Aligned","version":1},"reference_index":195,"source":"arxiv_source","source_observed_at":"2026-08-03T04:44:10.007392Z"},"links":{"cited_paper":"/paper/1205.3030","citing_paper":"/paper/2607.29558"},"observation_digest":"sha256:1189de2253978f7425035065e5ebcd71f97929b94cf7b20eedabc9ad72e83afd","observation_id":"cd86bcfe-7558-4fec-94bd-b7a5cc888a7a","resolution":{"observed_at":"2026-08-03T04:44:10.007392Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1205.3030","last_updated":"2012-06-13T09:18:47Z","snapshot_observed_at":"2026-08-15T04:09:57.294777Z","submitted_at":"2012-05-14T14:00:20Z","title":"Rapid growth of gas-giant cores by pebble accretion","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1205.3030","snapshot_observed_at":"2026-08-04T11:34:00.652909Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02204","last_updated":"2026-08-03T13:28:59Z","snapshot_observed_at":"2026-08-18T17:26:02.716585Z","submitted_at":"2026-08-03T13:28:59Z","title":"Accretion across scales: streamers, surface-layer transport, and rapid replenishment in young protoplanetary discs","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-04T11:34:00.652909Z"},"links":{"cited_paper":"/paper/1205.3030","citing_paper":"/paper/2608.02204"},"observation_digest":"sha256:b45339c32d87a739eda1af72c1ca5ab863b3c7c824099361933ea1812a8af181","observation_id":"2ded9d49-9f35-4cec-9996-94f978422a51","resolution":{"observed_at":"2026-08-04T11:34:00.652909Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1205.3030/citation-record","integrity":"/paper/1205.3030/integrity","json":"/paper/1205.3030/citation-record.json","paper":"/paper/1205.3030"},"outbound":[],"paper":{"arxiv_id":"1205.3030","last_updated":"2012-06-13T09:18:47Z","latest_version":2,"primary_category":"astro-ph.EP","snapshot_observed_at":"2026-08-15T04:09:57.294777Z","submitted_at":"2012-05-14T14:00:20Z","title":"Rapid growth of gas-giant cores by pebble accretion"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"thesis":"As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 12 inbound Pith citation observations for arXiv:1205.3030."}