{"as_of":"2026-08-16T20:47:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:4ba826954107ae643350fbe94cf942fea430cab34b68bd8d9c3b60fe6c7fac79","coverage":[{"denominator":295,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-02T02:59:16.937509Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2607.14066/citation-record","integrity":"/paper/2607.14066/integrity","json":"/paper/2607.14066/citation-record.json","paper":"/paper/2607.14066"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0303057","last_updated":"2003-03-03T22:30:17Z","snapshot_observed_at":"2026-08-08T23:52:12.399544Z","submitted_at":"2003-03-03T22:30:17Z","title":"Mg isotopic ratios in giant stars of the globular cluster NGC 6752","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0303057","snapshot_observed_at":"2026-08-02T02:59:09.617678Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:09.617678Z"},"links":{"cited_paper":"/paper/astro-ph/0303057","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:5052de2fb71453f50e2512d186c17eb8fc42b779b7fa8812bf64988f52178f3e","observation_id":"6f11e2a1-4b1c-464e-94ea-d0c22e5d2319","resolution":{"observed_at":"2026-08-02T02:59:09.617678Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1403.0819","last_updated":"2014-03-04T15:45:01Z","snapshot_observed_at":"2026-08-15T18:04:57.184902Z","submitted_at":"2014-03-04T15:45:01Z","title":"Heavy elements in Globular Clusters: the role of AGB stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1403.0819","snapshot_observed_at":"2026-08-02T02:59:09.674113Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:09.674113Z"},"links":{"cited_paper":"/paper/1403.0819","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:3a90d825a37ee9023a473f2085df21c41250be984ee5ea7dc78daa52daa94906","observation_id":"90e957a0-f123-4922-9c23-d7c3e85b2e30","resolution":{"observed_at":"2026-08-02T02:59:09.674113Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1409.1227","last_updated":"2014-09-03T20:00:07Z","snapshot_observed_at":"2026-08-14T23:20:51.658392Z","submitted_at":"2014-09-03T20:00:07Z","title":"The s-Process Enrichment of the Globular Clusters M4 and M22","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1409.1227","snapshot_observed_at":"2026-08-02T02:59:09.774643Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:09.774643Z"},"links":{"cited_paper":"/paper/1409.1227","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:cb3e2c4c03759fe28201f1cbbe14b10d8e2bb57c80a715832a39e17b32a57c3f","observation_id":"13324c92-5e6c-4557-b677-cfc81c587679","resolution":{"observed_at":"2026-08-02T02:59:09.774643Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1307.4486","last_updated":"2013-07-17T02:27:11Z","snapshot_observed_at":"2026-08-15T00:10:07.424875Z","submitted_at":"2013-07-17T02:27:11Z","title":"High Precision Differential Abundance Measurements in Globular Clusters: Chemical Inhomogeneities in NGC 6752","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.4486","snapshot_observed_at":"2026-08-02T02:59:09.946180Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:09.946180Z"},"links":{"cited_paper":"/paper/1307.4486","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:953779b9dccb8f0a917c8b146a5b16ad761d60260c02f02e8101b2350a6dc8e6","observation_id":"2249a488-27f0-4ebb-987e-953a4ee9360a","resolution":{"observed_at":"2026-08-02T02:59:09.946180Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0905.4058","last_updated":"2009-05-25T19:28:00Z","snapshot_observed_at":"2026-08-15T05:47:41.579299Z","submitted_at":"2009-05-25T19:28:00Z","title":"A double stellar generation in the Globular Cluster NGC6656 (M 22). Two stellar groups with different iron and s-process element abundance","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0905.4058","snapshot_observed_at":"2026-08-02T02:59:10.039291Z","title":"Two stellar groups with different iron and s-process element abundances","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:10.039291Z"},"links":{"cited_paper":"/paper/0905.4058","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:a78288df3fd917de2bf20f7676c3273aa204974eb7cecb30bb808e3a6513026e","observation_id":"aa042bd4-c78a-4f05-869c-a718a9cd21a0","resolution":{"observed_at":"2026-08-02T02:59:10.039291Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1105.1523","last_updated":"2011-05-08T14:20:51Z","snapshot_observed_at":"2026-08-15T04:47:24.566928Z","submitted_at":"2011-05-08T14:20:51Z","title":"The two metallicity groups of the globular cluster M22: a chemical perspective","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1105.1523","snapshot_observed_at":"2026-08-02T02:59:10.144193Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:10.144193Z"},"links":{"cited_paper":"/paper/1105.1523","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:8fb3e5e3232488a838755a9f219d2e3d0453dc1eb2d9c9c27669902a9f5e4d83","observation_id":"4e7e820a-6ad4-4ca3-b879-70bd92dfbf5c","resolution":{"observed_at":"2026-08-02T02:59:10.144193Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:10.230745Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:10.230745Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:bab90445929eb35bd3b9107f3cbbbe7b06716c8538d9f3237722d00acf846859","observation_id":"b8f42cd3-ec8e-43cf-b6e4-57a344bd6ba1","resolution":{"observed_at":"2026-08-02T02:59:10.230745Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1708.06853","last_updated":"2018-01-17T02:00:46Z","snapshot_observed_at":"2026-08-15T09:53:48.742917Z","submitted_at":"2017-08-22T23:46:20Z","title":"Metallicity Fluctuation Statistics in the Interstellar Medium and Young Stars. I. Variance and Correlation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1708.06853","snapshot_observed_at":"2026-08-02T02:59:10.302109Z","title":"Variance and correlation","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:10.302109Z"},"links":{"cited_paper":"/paper/1708.06853","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:f8fa728bb971c9b1308a3f5aa55bd17c1d3fe90e2697a04d1e70be7275bfde7d","observation_id":"92da58ec-56e2-4664-a47a-92d1a0562d7e","resolution":{"observed_at":"2026-08-02T02:59:10.302109Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.10173","last_updated":"2018-10-24T03:53:46Z","snapshot_observed_at":"2026-08-16T17:17:39.595081Z","submitted_at":"2018-10-24T03:53:46Z","title":"SLUG IV: A Novel Forward-Modelling Method to Derive the Demographics of Star Clusters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.10173","snapshot_observed_at":"2026-08-02T02:59:10.405339Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:10.405339Z"},"links":{"cited_paper":"/paper/1810.10173","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:8eba17b06a6149c78042a2b07f8ac256d19f78945c5c60ecad5844697f273f89","observation_id":"aff0de83-606c-4c94-bc7e-bbe81c96e9bb","resolution":{"observed_at":"2026-08-02T02:59:10.405339Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.05408","last_updated":"2015-06-18T20:18:55Z","snapshot_observed_at":"2026-08-14T22:59:29.811980Z","submitted_at":"2015-02-18T21:00:15Z","title":"SLUG -- Stochastically Lighting Up Galaxies. III: A Suite of Tools for Simulated Photometry, Spectroscopy, and Bayesian Inference with Stochastic Stellar Populations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.05408","snapshot_observed_at":"2026-08-02T02:59:10.498523Z","title":"A suite of tools for simulated photometry, spectroscopy, and Bayesian inference with stochastic stellar populations","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:10.498523Z"},"links":{"cited_paper":"/paper/1502.05408","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:3aade6ee705731faa2e104dba1fdb29aeac9e02e03ed6a438de49c208e1bf981","observation_id":"7e9c7ec9-f9e5-441e-9bc9-b5b3e1a305fa","resolution":{"observed_at":"2026-08-02T02:59:10.498523Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1403.4605","last_updated":"2014-08-18T08:35:12Z","snapshot_observed_at":"2026-08-14T23:40:49.701673Z","submitted_at":"2014-03-18T20:00:20Z","title":"SLUG - Stochastically Lighting Up Galaxies. II: Quantifying the Effects of Stochasticity on Star Formation Rate Indicators","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1403.4605","snapshot_observed_at":"2026-08-02T02:59:10.572108Z","title":"Quantifying the effects of stochasticity on star formation rate indicators","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:10.572108Z"},"links":{"cited_paper":"/paper/1403.4605","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:481185ed1397537cacebb4f3bac0628c3c3685c3f3fa60e200d3fd6616c77bb3","observation_id":"54393d75-4828-4c05-9bba-5e44a2818055","resolution":{"observed_at":"2026-08-02T02:59:10.572108Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1106.3072","last_updated":"2011-06-15T20:00:03Z","snapshot_observed_at":"2026-08-15T04:43:48.578618Z","submitted_at":"2011-06-15T20:00:03Z","title":"SLUG - Stochastically Lighting Up Galaxies I: Methods and Validating Tests","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1106.3072","snapshot_observed_at":"2026-08-02T02:59:10.706998Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:10.706998Z"},"links":{"cited_paper":"/paper/1106.3072","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:e9d26b5d4b7db488b254374eb5bf86078e2ed97543366b42807ec6a74771e8dd","observation_id":"44f67439-fc42-4ae2-8bee-b393cd0c9089","resolution":{"observed_at":"2026-08-02T02:59:10.706998Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1108.3868","last_updated":"2011-08-18T22:30:03Z","snapshot_observed_at":"2026-08-15T04:37:52.194187Z","submitted_at":"2011-08-18T22:30:03Z","title":"Characterizing the Heavy Elements in Globular Cluster M22 and an Empirical s-process Abundance Distribution Derived from the Two Stellar Groups","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1108.3868","snapshot_observed_at":"2026-08-02T02:59:10.770850Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:10.770850Z"},"links":{"cited_paper":"/paper/1108.3868","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:29179df15c974f4c444bf1900f1c013a197ca3e742878dcc7c17f7270759ba35","observation_id":"fc4614e0-3f81-4f54-945f-121fcfcb9942","resolution":{"observed_at":"2026-08-02T02:59:10.770850Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:10.830907Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:10.830907Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:bf6d834c14aea346295e04055bce7157b7d0ca148def902a342b6dca9c564720","observation_id":"a691faf4-b558-4918-9cc3-8a9c763b4721","resolution":{"observed_at":"2026-08-02T02:59:10.830907Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1202.0797","last_updated":"2012-02-03T18:52:44Z","snapshot_observed_at":"2026-08-15T04:20:20.083236Z","submitted_at":"2012-02-03T18:52:44Z","title":"CNO and F abundances in the globular cluster M22 (NGC 6656)","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1202.0797","snapshot_observed_at":"2026-08-02T02:59:10.895829Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:10.895829Z"},"links":{"cited_paper":"/paper/1202.0797","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:1164e03d861fe540ffe3a1149ae1ea1b0eb9a83226a5f205e92def4af10a80b1","observation_id":"396ca83f-8cba-4632-8f23-f681f53aad74","resolution":{"observed_at":"2026-08-02T02:59:10.895829Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.04643","last_updated":"2016-02-13T11:19:23Z","snapshot_observed_at":"2026-08-14T22:27:39.622145Z","submitted_at":"2015-10-15T17:45:30Z","title":"Core-Collapse Supernovae from 9 to 120 Solar Masses Based on Neutrino-powered Explosions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.04643","snapshot_observed_at":"2026-08-02T02:59:10.963423Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:10.963423Z"},"links":{"cited_paper":"/paper/1510.04643","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:0998ea10753233a5133d3ac1f384a30ccda4ec4810b9492461230f1554234039","observation_id":"4b4adba9-325e-4fad-90a5-fd1c87a20f10","resolution":{"observed_at":"2026-08-02T02:59:10.963423Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1310.2614","last_updated":"2013-10-09T20:00:58Z","snapshot_observed_at":"2026-08-14T23:59:33.189735Z","submitted_at":"2013-10-09T20:00:58Z","title":"Super and Massive AGB Stars: II - Nucleosynthesis and Yields - Z=0.02, 0.008 and 0.004","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1310.2614","snapshot_observed_at":"2026-08-02T02:59:11.020461Z","title":"Nucleosynthesis and yields - Z = 0.02, 0.008 and 0.004","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:11.020461Z"},"links":{"cited_paper":"/paper/1310.2614","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:0d9ca23590169d45870b475a2a24acf05b2c56b84bc24219c0d3ca8bd17ad768","observation_id":"2a8f3acb-a027-434b-bab8-abb51d202238","resolution":{"observed_at":"2026-08-02T02:59:11.020461Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1604.02178","last_updated":"2016-04-07T21:13:49Z","snapshot_observed_at":"2026-08-14T22:02:35.911874Z","submitted_at":"2016-04-07T21:13:49Z","title":"Stellar yields from metal-rich asymptotic giant branch models","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1604.02178","snapshot_observed_at":"2026-08-02T02:59:11.136106Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:11.136106Z"},"links":{"cited_paper":"/paper/1604.02178","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:a5fd9684e54bbb610fa76a72e63d7dde491ebd4627b516d15966a369da9af335","observation_id":"a25782a8-9a67-4734-84ba-9d71d2e197d0","resolution":{"observed_at":"2026-08-02T02:59:11.136106Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1911.02598","last_updated":"2019-11-06T19:14:50Z","snapshot_observed_at":"2026-08-13T23:00:22.488749Z","submitted_at":"2019-11-06T19:14:50Z","title":"The Impact of Starbursts on Element Abundance Ratios","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.02598","snapshot_observed_at":"2026-08-02T02:59:11.194988Z","title":", keywords =","venue":null,"work_id":null,"year":1911},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:11.194988Z"},"links":{"cited_paper":"/paper/1911.02598","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:dbc4209ffca37ec64653624dcbee25e78d4565c3dd1417c810fae1d2637fa190","observation_id":"e57d4fbb-9f27-4adc-98f0-b6b2fab0bd3f","resolution":{"observed_at":"2026-08-02T02:59:11.194988Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:11.251790Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:11.251790Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:7267e132669d2c5bd082587b7d0846b3eb0dd940798577b7b5667d0fc9b6533d","observation_id":"9ac88525-4a50-413b-a2e6-51b6d6662c99","resolution":{"observed_at":"2026-08-02T02:59:11.251790Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.05063","last_updated":"2021-10-25T15:42:15Z","snapshot_observed_at":"2026-08-10T22:12:50.404873Z","submitted_at":"2020-09-10T18:01:08Z","title":"The Similarity of Abundance Ratio Trends and Nucleosynthetic Patterns in the Milky Way Disk and Bulge","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.05063","snapshot_observed_at":"2026-08-02T02:59:11.312743Z","title":", keywords =","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:11.312743Z"},"links":{"cited_paper":"/paper/2009.05063","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:5000281fd3acd2be868ab4e7d07318d6a67b00c2ed491e476ac6cf61af51c5d4","observation_id":"f798e3d7-2e29-4a3b-b724-d2d1e7995609","resolution":{"observed_at":"2026-08-02T02:59:11.312743Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.06113","last_updated":"2019-10-08T17:14:48Z","snapshot_observed_at":"2026-08-16T00:08:59.411605Z","submitted_at":"2019-08-16T18:02:47Z","title":"Abundance ratios in GALAH DR2 and their implications for nucleosynthesis","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.06113","snapshot_observed_at":"2026-08-02T02:59:11.380174Z","title":", keywords =","venue":null,"work_id":null,"year":1908},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:11.380174Z"},"links":{"cited_paper":"/paper/1908.06113","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:f098b5b750144758eb8ae26ae17268d6884e3f1300f99f593b9bc193d87ba125","observation_id":"f2687e6b-32e3-48fe-b738-18533555cc14","resolution":{"observed_at":"2026-08-02T02:59:11.380174Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.04660","last_updated":"2020-08-11T12:25:00Z","snapshot_observed_at":"2026-08-14T00:17:17.252362Z","submitted_at":"2020-08-11T12:25:00Z","title":"The Origin of Elements from Carbon to Uranium","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.04660","snapshot_observed_at":"2026-08-02T02:59:11.444284Z","title":", keywords =","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:11.444284Z"},"links":{"cited_paper":"/paper/2008.04660","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:a19f76164faa4c53a8c44690fed613e551e64e32ca210fe9ad3acfc942ac5f99","observation_id":"774c1b3d-0fb3-4cb3-b13c-ddba56a8ddc6","resolution":{"observed_at":"2026-08-02T02:59:11.444284Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:11.515580Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:11.515580Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:270d4cb0fc36ef6879623743b0976b35b36e5009bda8bc89371602d8c00ee054","observation_id":"afe1003a-2c5c-4928-a260-01ad01048d76","resolution":{"observed_at":"2026-08-02T02:59:11.515580Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.12325","last_updated":"2018-10-29T18:03:08Z","snapshot_observed_at":"2026-08-14T18:07:35.849264Z","submitted_at":"2018-10-29T18:03:08Z","title":"Chemical Cartography with APOGEE: Multi-element abundance ratios","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.12325","snapshot_observed_at":"2026-08-02T02:59:11.565775Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:11.565775Z"},"links":{"cited_paper":"/paper/1810.12325","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:b841a74b89b44f50ca739cddc3a8cd96406822426681b14fad160929cbc58988","observation_id":"126ea780-c49b-43bd-bb32-82e2e6a9d019","resolution":{"observed_at":"2026-08-02T02:59:11.565775Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:11.619000Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:11.619000Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:371db4544ef63052d5cc97c83f93eebe34a916218bf2b03160302af1b5cb417b","observation_id":"cacd3718-01a2-4104-9fed-bc82d5e99d08","resolution":{"observed_at":"2026-08-02T02:59:11.619000Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.04695","last_updated":"2020-01-03T22:20:10Z","snapshot_observed_at":"2026-08-16T05:37:22.175423Z","submitted_at":"2019-09-10T18:18:43Z","title":"Simulating Metal Mixing of Both Common and Rare Enrichment Sources in a Low Mass Dwarf Galaxy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.04695","snapshot_observed_at":"2026-08-02T02:59:11.680590Z","title":", keywords =","venue":null,"work_id":null,"year":1909},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:11.680590Z"},"links":{"cited_paper":"/paper/1909.04695","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:0b9ad961f8a005356d763c8fd0cbaf96f6b59701cea888dbf94e713d259161c3","observation_id":"a096d366-9a84-465d-9110-6a872ffbc84d","resolution":{"observed_at":"2026-08-02T02:59:11.680590Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.01712","last_updated":"2018-07-04T18:00:03Z","snapshot_observed_at":"2026-08-14T18:55:40.794746Z","submitted_at":"2018-07-04T18:00:03Z","title":"Mixing of metals during star cluster formation: statistics and implications for chemical tagging","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.01712","snapshot_observed_at":"2026-08-02T02:59:11.751812Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:11.751812Z"},"links":{"cited_paper":"/paper/1807.01712","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:90b2060dabe02e6bf10fc377f0505da701f0bf7ce59497068caa277bf9eecb9b","observation_id":"2fadc088-7f0f-41a7-92ee-89520bebf426","resolution":{"observed_at":"2026-08-02T02:59:11.751812Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.07311","last_updated":"2021-02-25T13:04:40Z","snapshot_observed_at":"2026-08-16T19:13:27.840220Z","submitted_at":"2020-10-14T18:00:04Z","title":"LYRA I: Simulating the multi-phase ISM of a dwarf galaxy with variable energy supernovae from individual stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.07311","snapshot_observed_at":"2026-08-02T02:59:11.813906Z","title":"Simulating the multiphase ISM of a dwarf galaxy with variable energy supernovae from individual stars","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:11.813906Z"},"links":{"cited_paper":"/paper/2010.07311","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:2013afc1c54ffc77924a242b143e54ef7b0a4b2430e9414be98c41a129362697","observation_id":"693ebb9d-4ce6-4922-86a7-5ce2a9382010","resolution":{"observed_at":"2026-08-02T02:59:11.813906Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1501.05459","last_updated":"2015-01-22T11:06:25Z","snapshot_observed_at":"2026-08-16T14:41:32.427557Z","submitted_at":"2015-01-22T11:06:25Z","title":"Dust-regulated galaxy formation and evolution:A new chemodynamical model with live dust particles","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1501.05459","snapshot_observed_at":"2026-08-02T02:59:11.880027Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:11.880027Z"},"links":{"cited_paper":"/paper/1501.05459","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:fc649010e02ac3255b08769eb60308323950813307920867dbd6b6d7205569be","observation_id":"2e8b402b-217c-432d-a764-6a6ebee5d20e","resolution":{"observed_at":"2026-08-02T02:59:11.880027Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:11.928747Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:11.928747Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:788c3e4a10e16780fb027c2e3a9c575e45d51dd366d28dd140370c77d4581b2e","observation_id":"e20f7fef-f3c6-4bd9-86ae-4eaa0af1bba3","resolution":{"observed_at":"2026-08-02T02:59:11.928747Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.14807","last_updated":"2021-04-30T07:43:11Z","snapshot_observed_at":"2026-08-16T18:27:58.255250Z","submitted_at":"2021-04-30T07:43:11Z","title":"Detection of metallicity correlations in 100 nearby galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.14807","snapshot_observed_at":"2026-08-02T02:59:12.042786Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:12.042786Z"},"links":{"cited_paper":"/paper/2104.14807","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:46fec234283242a208d1230148c502ffbede77ba2f99f6486b91ad83e8def97d","observation_id":"c90ef93a-2cda-48b1-97d7-131805a955f1","resolution":{"observed_at":"2026-08-02T02:59:12.042786Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.02342","last_updated":"2020-09-04T18:03:06Z","snapshot_observed_at":"2026-08-14T06:48:55.635044Z","submitted_at":"2020-09-04T18:03:06Z","title":"Measuring the mixing scale of the ISM within nearby spiral galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.02342","snapshot_observed_at":"2026-08-02T02:59:12.111170Z","title":", keywords =","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:12.111170Z"},"links":{"cited_paper":"/paper/2009.02342","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:e55488c9604e049b4b68132c7769bf846188a3c4c1445b4e0076226af4956712","observation_id":"016d027f-e71a-4d4e-b5ba-9e5f679ec613","resolution":{"observed_at":"2026-08-02T02:59:12.111170Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.07190","last_updated":"2019-10-16T06:51:14Z","snapshot_observed_at":"2026-08-15T11:40:08.852962Z","submitted_at":"2019-10-16T06:51:14Z","title":"Mapping metallicity variations across nearby galaxy disks","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.07190","snapshot_observed_at":"2026-08-02T02:59:12.202604Z","title":", keywords =","venue":null,"work_id":null,"year":1910},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:12.202604Z"},"links":{"cited_paper":"/paper/1910.07190","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:d8d7b727fad4f1e6a8df205ec1a66ede2993e2f5c2dc922a162e430ff8cd8ee6","observation_id":"704796e0-fade-439c-9d83-eec19dc1c4a0","resolution":{"observed_at":"2026-08-02T02:59:12.202604Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2102.06220","last_updated":"2021-08-19T16:55:29Z","snapshot_observed_at":"2026-08-16T18:46:07.773722Z","submitted_at":"2021-02-11T19:01:23Z","title":"3-D gas-phase elemental abundances across the formation histories of Milky Way-mass galaxies in the FIRE simulations: initial conditions for chemical tagging","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2102.06220","snapshot_observed_at":"2026-08-02T02:59:12.299380Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:12.299380Z"},"links":{"cited_paper":"/paper/2102.06220","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:d8623dd520bdb9bf09d507524d83b18ddbe88766cd9c6019708b9eed62cf57b2","observation_id":"48bd829b-06df-4326-81d7-0b59eb112b70","resolution":{"observed_at":"2026-08-02T02:59:12.299380Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.05019","last_updated":"2020-05-07T07:23:25Z","snapshot_observed_at":"2026-08-16T05:52:11.293620Z","submitted_at":"2019-08-14T08:56:33Z","title":"Numerical convergence of hydrodynamical simulations of galaxy formation: the abundance and internal structure of galaxies and their cold dark matter haloes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.05019","snapshot_observed_at":"2026-08-02T02:59:12.367693Z","title":", keywords =","venue":null,"work_id":null,"year":1908},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:12.367693Z"},"links":{"cited_paper":"/paper/1908.05019","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:c6cf8fb679a8e3974861dc00d695eaf5f5b0d804457ba4649ad5fb057e688219","observation_id":"81c2b8f0-2529-432e-9031-6eb78cf4c38e","resolution":{"observed_at":"2026-08-02T02:59:12.367693Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1408.4130","last_updated":"2014-08-18T20:00:24Z","snapshot_observed_at":"2026-08-14T23:22:46.580260Z","submitted_at":"2014-08-18T20:00:24Z","title":"The Solar Twin Planet Search. I. Fundamental parameters of the stellar sample","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1408.4130","snapshot_observed_at":"2026-08-02T02:59:12.429574Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:12.429574Z"},"links":{"cited_paper":"/paper/1408.4130","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:8bfe235d33935270eeebb7883b4eb3eb569f85268dc19a55404be6db7faeb2a5","observation_id":"eedf6d23-b3c1-49a9-b2f8-e7635b748836","resolution":{"observed_at":"2026-08-02T02:59:12.429574Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:12.534341Z","title":", year = 1973, month = sep, volume =","venue":null,"work_id":null,"year":1973},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:12.534341Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:a520f4d76ebe16fcd9fb8e40b5d806968fb5ad1785cde51ace8dc780c446d30b","observation_id":"77a30296-e11d-4a0a-9cdd-caf941234610","resolution":{"observed_at":"2026-08-02T02:59:12.534341Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.00058","last_updated":"2016-01-30T02:07:13Z","snapshot_observed_at":"2026-08-14T22:12:26.876905Z","submitted_at":"2016-01-30T02:07:13Z","title":"The chemical composition of red giants in 47 Tucanae. II. Magnesium isotopes and pollution scenarios","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.00058","snapshot_observed_at":"2026-08-02T02:59:12.597833Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:12.597833Z"},"links":{"cited_paper":"/paper/1602.00058","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:9a6f009c8b931daed3aa35c6ea5c9f809b8aa07c5a76533829f0befce61aa92e","observation_id":"8caac9db-2448-4942-b9f0-09994109beb4","resolution":{"observed_at":"2026-08-02T02:59:12.597833Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.04218","last_updated":"2017-06-13T18:32:48Z","snapshot_observed_at":"2026-08-14T20:54:16.829178Z","submitted_at":"2017-06-13T18:32:48Z","title":"An investigation of the formation and line properties of MgH in 3D hydrodynamical model stellar atmospheres","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.04218","snapshot_observed_at":"2026-08-02T02:59:12.663741Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:12.663741Z"},"links":{"cited_paper":"/paper/1706.04218","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:0498de5cc99a6cf7c90951fb2a7b494bc5f5ed33de04c877df2ee2a790e4faf9","observation_id":"73d45408-1610-4f55-b905-204e2817845e","resolution":{"observed_at":"2026-08-02T02:59:12.663741Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1304.0523","last_updated":"2013-04-02T03:50:24Z","snapshot_observed_at":"2026-08-15T00:22:58.679166Z","submitted_at":"2013-04-02T03:50:24Z","title":"Magnesium Isotope Ratios in omega Centauri Red Giants","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1304.0523","snapshot_observed_at":"2026-08-02T02:59:12.746138Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:12.746138Z"},"links":{"cited_paper":"/paper/1304.0523","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:9da3d8946f37324ed943d17e46db9e20a612185e07a50a8a0417e2ddaca39c5f","observation_id":"c1c09363-dfd5-4250-a601-8fe48861d68a","resolution":{"observed_at":"2026-08-02T02:59:12.746138Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0811.2932","last_updated":"2008-11-18T15:37:28Z","snapshot_observed_at":"2026-08-15T10:01:45.882423Z","submitted_at":"2008-11-18T15:37:28Z","title":"DAOSPEC: an automatic code for measuring equivalent widths in high-resolution stellar spectra","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0811.2932","snapshot_observed_at":"2026-08-02T02:59:12.816053Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:12.816053Z"},"links":{"cited_paper":"/paper/0811.2932","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:9679e2969518057f449901d6f9cf16e1492abed8d7b4d99f11b58b3e6de22af4","observation_id":"f3dea8dd-4bf3-4109-b3c4-8d460073d24d","resolution":{"observed_at":"2026-08-02T02:59:12.816053Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0312054","last_updated":"2003-12-02T02:58:15Z","snapshot_observed_at":"2026-08-14T09:09:21.835136Z","submitted_at":"2003-12-02T02:58:15Z","title":"Magnesium isotope ratios in Hyades stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0312054","snapshot_observed_at":"2026-08-02T02:59:12.876199Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:12.876199Z"},"links":{"cited_paper":"/paper/astro-ph/0312054","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:f4c82487d518b284374e99413beb05b49aca858d8a816bb97aee040d1993ed29","observation_id":"4f321cfc-eeaa-45b0-be33-e1f8bf73e872","resolution":{"observed_at":"2026-08-02T02:59:12.876199Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:12.945222Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:12.945222Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:2ad8bc2e241ea29f14005ba5ab7dc41680115abe162df24e296f8a3db34b1ff9","observation_id":"9fc66abe-99db-4fe0-930b-dd06150c7448","resolution":{"observed_at":"2026-08-02T02:59:12.945222Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.16355","last_updated":"2020-06-29T20:18:48Z","snapshot_observed_at":"2026-07-06T09:33:50.133351Z","submitted_at":"2020-06-29T20:18:48Z","title":"Gaia and Hubble unveil the kinematics of stellar populations in the Type II globular clusters {\\omega} Centauri and M 22","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.16355","snapshot_observed_at":"2026-08-02T02:59:13.004665Z","title":", keywords =","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:13.004665Z"},"links":{"cited_paper":"/paper/2006.16355","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:f6ada07ebcf601b609488bc84e36881e1636c5b468ea4ae86f7423f047ff799b","observation_id":"0d542cff-6f8a-4dda-8d62-064f409f2f13","resolution":{"observed_at":"2026-08-02T02:59:13.004665Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0909.5265","last_updated":"2009-09-29T04:32:43Z","snapshot_observed_at":"2026-08-15T05:37:59.811469Z","submitted_at":"2009-09-29T04:32:43Z","title":"M22: A [Fe/H] Abundance Range Revealed","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0909.5265","snapshot_observed_at":"2026-08-02T02:59:13.107488Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:13.107488Z"},"links":{"cited_paper":"/paper/0909.5265","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:84a937faaf937b84c82069f545be04c19fbd730d6a56dde720f21ef96c0cc208","observation_id":"5f6ece31-37fe-4530-b7e6-ccff80e65820","resolution":{"observed_at":"2026-08-02T02:59:13.107488Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:13.176868Z","title":"Star Clusters , year = 1980, editor =","venue":null,"work_id":null,"year":1980},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:13.176868Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:76d94a4588de5473f30b30b4a3602b68b94a608efe05e86575c0bdc509c4b151","observation_id":"8f81cfe0-d3b0-4540-a25b-ad3d4b7a0933","resolution":{"observed_at":"2026-08-02T02:59:13.176868Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:13.290063Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:13.290063Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:bd69be46cb9377680101bad5238166cdadf0a0300178d55bf8a5aa21b4583846","observation_id":"740ed60a-8fba-40cc-9416-10cd7d25d6d0","resolution":{"observed_at":"2026-08-02T02:59:13.290063Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:13.358625Z","title":", year = 1977, month = apr, volume =","venue":null,"work_id":null,"year":1977},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:13.358625Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:c3b59f6e93457f6945025b62aaf4a4256cd34ba3e0f6cece7804d7368ba2f911","observation_id":"345502b6-de14-4b4a-b7b0-0c56cef9165f","resolution":{"observed_at":"2026-08-02T02:59:13.358625Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:13.453871Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:13.453871Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:d9892ca20925eb04696e5d6626c7f213fb7d4e492b62e36a7428c2c47feba05d","observation_id":"ccbcbbd0-0741-419d-ab02-60e69ff22702","resolution":{"observed_at":"2026-08-02T02:59:13.453871Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:13.552511Z","title":", year = 1975, month = oct, volume =","venue":null,"work_id":null,"year":1975},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:13.552511Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:fe5afc88550aae0f47c62647cef93204b91ccb64f37088263ff357013154d024","observation_id":"b58dc729-1fb2-4ce2-84a1-5f1d07f5c119","resolution":{"observed_at":"2026-08-02T02:59:13.552511Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:13.626732Z","title":", year = 1975, month = oct, volume =","venue":null,"work_id":null,"year":1975},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:13.626732Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:db6a758e214489c53d2d7487907c9ba2f77cc4b0b13f10082ea42e53099dc71a","observation_id":"321d8b7b-a611-4cbe-9240-ef45a7fd0f77","resolution":{"observed_at":"2026-08-02T02:59:13.626732Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:13.680978Z","title":"The anomalous giant branch of omega Centauri","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:13.680978Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:e40b16b67ed028225b8a3b2c40280fd0174e7bbdaeb300a514c279b2d6e71824","observation_id":"349cc734-5622-4ef4-ac50-50012a856357","resolution":{"observed_at":"2026-08-02T02:59:13.680978Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:13.748953Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:13.748953Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:ab0acd3cd5824dbbbaccafee28e0e7bd5e79071b56cc17b86b7bc3343b0120cd","observation_id":"d923c155-2bde-4367-ad92-1cb0d719dfd0","resolution":{"observed_at":"2026-08-02T02:59:13.748953Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:13.817876Z","title":", year = 1976, month = oct, volume =","venue":null,"work_id":null,"year":1976},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:13.817876Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:32a821db3dc2a21f673b3df8b5598c19d95d1e4102c10a8c7bb2377df43f8812","observation_id":"d3f73296-bc8a-41c8-8348-9ffb278659f0","resolution":{"observed_at":"2026-08-02T02:59:13.817876Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:13.908390Z","title":", year = 1976, month = apr, volume =","venue":null,"work_id":null,"year":1976},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:13.908390Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:657014185d2ca740c0b8f91e62e715389b0f21879c8bb498967b82cb41715183","observation_id":"240e5111-0183-4a39-a39b-767df61a8fcc","resolution":{"observed_at":"2026-08-02T02:59:13.908390Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:13.977137Z","title":"The Observatory , year = 1962, month = oct, volume =","venue":null,"work_id":null,"year":1962},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:13.977137Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:a87c072c0abb373d455967352ef736a759548268a4fd447ec0e181c23055e3be","observation_id":"a4beac47-3ee4-4ef5-94ef-c3656eb9726e","resolution":{"observed_at":"2026-08-02T02:59:13.977137Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:14.024812Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:14.024812Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:57c83c52f9e7c8f5944769bf7d76a657cdd628f9f87751dfc1dba3291ff571c6","observation_id":"e1af541f-6c9e-472f-83ac-6c160a58bb8a","resolution":{"observed_at":"2026-08-02T02:59:14.024812Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:14.093177Z","title":"Royal Observatory Annals , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:14.093177Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:fbb1639ba6cded848e3ce0a763497034545298fa57e1331119ae294f7ff8bb03","observation_id":"a7bc4b44-5b0b-474b-8d71-c97d226b459f","resolution":{"observed_at":"2026-08-02T02:59:14.093177Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:14.150170Z","title":null,"venue":null,"work_id":null,"year":1973},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:14.150170Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:129d6ebdee5c0dc51f4e4dae22ca705c0e574bce43cd3afef1dd1e26d9b8f305","observation_id":"14e70941-c745-4d6a-bc82-f880bc56af3d","resolution":{"observed_at":"2026-08-02T02:59:14.150170Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:14.206815Z","title":null,"venue":null,"work_id":null,"year":1976},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:14.206815Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:a8749b2412db967ebd7265ab51a2d754c539b9f5e080ec2ab540cfac77edf887","observation_id":"6b280bcb-3366-4a7a-b1bc-0beacea30e5d","resolution":{"observed_at":"2026-08-02T02:59:14.206815Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:14.304122Z","title":", keywords =","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:14.304122Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:2e177ffb38b846a5f27fd0471ef23457fce9bce0bfca6d3dacd9f1c3233f2c7b","observation_id":"cce8c2d4-f9b3-4586-b98f-70c21b3c7f53","resolution":{"observed_at":"2026-08-02T02:59:14.304122Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:14.376816Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:14.376816Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:86eba7b9306cc73ed7e2e184d237011e65981e4ad1d02939395866d5eb09fd90","observation_id":"23a34b35-92ef-43d7-b292-476af6535795","resolution":{"observed_at":"2026-08-02T02:59:14.376816Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:14.433787Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:14.433787Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:ba230df37a97efea33b8731a22685bc276ee7ccb0ee73a2d85ee2bf2a928d82c","observation_id":"15df9115-9689-4260-9f04-d2527bac86ab","resolution":{"observed_at":"2026-08-02T02:59:14.433787Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:14.496327Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:14.496327Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:5fc407b427cb733e516f2635fcbdd5d4f0201dcea7fd536fbc66db64ad83a7b9","observation_id":"666f285b-1200-4c8f-9d95-aa81a8e30f93","resolution":{"observed_at":"2026-08-02T02:59:14.496327Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:14.564997Z","title":"Vistas in Astronomy , year = 1956, month = jan, volume =","venue":null,"work_id":null,"year":1956},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:14.564997Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:95c842feb0e51adc6d1c609ce729f7390e11ba34ebf190bd8fd141c01823320c","observation_id":"2134b772-8a11-42ea-bbab-0835bea1dad1","resolution":{"observed_at":"2026-08-02T02:59:14.564997Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:14.623759Z","title":", year = 1961, month = mar, volume =","venue":null,"work_id":null,"year":1961},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:14.623759Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:af29caf9e255e716a51a96b7f7cf2a5733e354591c4378e9f1faa840baed9723","observation_id":"c18fb6ff-f1d7-4155-ae99-c0b39d322037","resolution":{"observed_at":"2026-08-02T02:59:14.623759Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1305.6025","last_updated":"2013-05-26T14:10:33Z","snapshot_observed_at":"2026-08-15T00:16:35.453490Z","submitted_at":"2013-05-26T14:10:33Z","title":"Rotating Globular Clusters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1305.6025","snapshot_observed_at":"2026-08-02T02:59:14.722915Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:14.722915Z"},"links":{"cited_paper":"/paper/1305.6025","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:15e2105812a2c819e2ce17d3a1dd6ccb5bc896db688b929700f935cc4d603b90","observation_id":"9747b434-24b2-489e-bc27-45d17a92d992","resolution":{"observed_at":"2026-08-02T02:59:14.722915Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.02580","last_updated":"2018-08-30T09:05:01Z","snapshot_observed_at":"2026-08-14T19:06:33.360913Z","submitted_at":"2018-06-07T09:31:32Z","title":"The internal rotation of globular clusters revealed by Gaia DR2","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.02580","snapshot_observed_at":"2026-08-02T02:59:14.782428Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:14.782428Z"},"links":{"cited_paper":"/paper/1806.02580","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:45a2af97d0cfec0edc54b6e42147f0238b2546e84ee04262f6db1b2ef9864d2a","observation_id":"b12f02b8-bbc4-460f-a65d-d5c965adf19d","resolution":{"observed_at":"2026-08-02T02:59:14.782428Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.07257","last_updated":"2017-10-19T17:26:33Z","snapshot_observed_at":"2026-08-14T20:22:06.459361Z","submitted_at":"2017-10-19T17:26:33Z","title":"A stellar census in globular clusters with MUSE: The contribution of rotation to cluster dynamics studied with 200 000 stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.07257","snapshot_observed_at":"2026-08-02T02:59:14.849227Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:14.849227Z"},"links":{"cited_paper":"/paper/1710.07257","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:7c13db4ead6df14e86f1df2d7f0620ee02c55edbb02449a17476c21feeba90ac","observation_id":"9dc24020-ea28-4b28-944e-a39f41594186","resolution":{"observed_at":"2026-08-02T02:59:14.849227Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.09908","last_updated":"2019-11-22T03:57:00Z","snapshot_observed_at":"2026-08-14T16:27:32.210486Z","submitted_at":"2019-05-23T20:29:03Z","title":"Three-Component Kinematics of Multiple Stellar Populations in Globular Clusters with Gaia and VLT","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.09908","snapshot_observed_at":"2026-08-02T02:59:14.937710Z","title":", keywords =","venue":null,"work_id":null,"year":1905},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:14.937710Z"},"links":{"cited_paper":"/paper/1905.09908","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:a45aa23d8b8edc9daa79a826699f100b51dfd5ca8cf24ff3e96c31a7745f3542","observation_id":"cf9f0fa8-97b1-42b5-b42c-29cfbb5149f5","resolution":{"observed_at":"2026-08-02T02:59:14.937710Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.07438","last_updated":"2015-02-26T05:09:45Z","snapshot_observed_at":"2026-08-14T22:58:35.432893Z","submitted_at":"2015-02-26T05:09:45Z","title":"Iron and s-elements abundance variations in NGC5286: comparison with anomalous globular clusters and Milky Way satellites","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.07438","snapshot_observed_at":"2026-08-02T02:59:14.981095Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:14.981095Z"},"links":{"cited_paper":"/paper/1502.07438","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:a7f3ef6dc5b6c3ff17df9e0ba4e41d1cedbd4afcdfb551122c7ad6741c0dac52","observation_id":"f9d2d235-d869-486a-9274-85ae1976c4a2","resolution":{"observed_at":"2026-08-02T02:59:14.981095Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0711.1394","last_updated":"2007-11-09T01:20:36Z","snapshot_observed_at":"2026-08-15T10:28:05.513671Z","submitted_at":"2007-11-09T01:20:36Z","title":"An abundance analysis of bright giants in the globular cluster NGC 1851","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0711.1394","snapshot_observed_at":"2026-08-02T02:59:15.074542Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:15.074542Z"},"links":{"cited_paper":"/paper/0711.1394","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:c7fed1afc3ddfa8fc9486623552a5a113ea036b8eff9d0023481cf82a61491d2","observation_id":"b4770122-4077-49e9-88dd-98fca5f91ec8","resolution":{"observed_at":"2026-08-02T02:59:15.074542Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1404.6873","last_updated":"2014-04-28T06:06:17Z","snapshot_observed_at":"2026-08-14T23:36:08.634059Z","submitted_at":"2014-04-28T06:06:17Z","title":"Iron and neutron-capture element abundance variations in the globular cluster M2 (NGC 7089)","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1404.6873","snapshot_observed_at":"2026-08-02T02:59:15.137281Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:15.137281Z"},"links":{"cited_paper":"/paper/1404.6873","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:e2c09387232ee77f026de95cbca6e390b6b93348a33af188116a8da5e8114ebc","observation_id":"f07c5fbf-e214-45c0-8541-9b79dca2a6e9","resolution":{"observed_at":"2026-08-02T02:59:15.137281Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:15.196874Z","title":", keywords =","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:15.196874Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:dc605392dce741a4e64630abf7336e0f986c8dcaab412378ae9f785dc4dd228f","observation_id":"79363d77-e014-497f-b6a9-eece9184e2fc","resolution":{"observed_at":"2026-08-02T02:59:15.196874Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.08359","last_updated":"2018-06-30T00:01:21Z","snapshot_observed_at":"2026-08-15T13:07:06.122921Z","submitted_at":"2018-04-23T12:19:05Z","title":"A catalogue of masses, structural parameters and velocity dispersion profiles of 112 Milky Way globular clusters","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.08359","snapshot_observed_at":"2026-08-02T02:59:15.296757Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:15.296757Z"},"links":{"cited_paper":"/paper/1804.08359","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:aeb7fb33777b14767fd67288ed235a82fb2001ce8f387b264d03e55d1adf2d2a","observation_id":"489a5553-b3c5-4ef4-b507-fec5bfdca4f4","resolution":{"observed_at":"2026-08-02T02:59:15.296757Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1411.4886","last_updated":"2014-11-18T16:07:58Z","snapshot_observed_at":"2026-08-14T23:11:11.141207Z","submitted_at":"2014-11-18T16:07:58Z","title":"The Gaia-ESO Survey: Kinematics of seven Galactic globular clusters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1411.4886","snapshot_observed_at":"2026-08-02T02:59:15.356774Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:15.356774Z"},"links":{"cited_paper":"/paper/1411.4886","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:25008c65e85646e0e432036213f0bba4d7a0979dcb9ecfaa3a46c36282bcd65b","observation_id":"2673beca-dc62-4798-a9c7-4b60df7bc44f","resolution":{"observed_at":"2026-08-02T02:59:15.356774Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:15.429329Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:15.429329Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:5ae146d626c369f2b616a595837909306b9e7dcf315aa7e3c0bdf1e3fef92e07","observation_id":"8ac7cfe1-0e12-4e31-9220-064c16b7c040","resolution":{"observed_at":"2026-08-02T02:59:15.429329Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:15.501882Z","title":null,"venue":null,"work_id":null,"year":1922},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:15.501882Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:4e7be22b7d0624e53af9f37aeb503d8d36d6aa47e6c708dace1590e5f0d5e864","observation_id":"1e9de44a-ca39-424f-b94a-a137dd41b538","resolution":{"observed_at":"2026-08-02T02:59:15.501882Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:15.557160Z","title":", year = 1959, month = feb, volume =","venue":null,"work_id":null,"year":1959},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:15.557160Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:c96d671296fa2927c1479e69334c74a396729e1d95c86d834e5a5292b736e9fe","observation_id":"7bc5b370-bd5f-4296-9dbf-90991cc10748","resolution":{"observed_at":"2026-08-02T02:59:15.557160Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:15.627906Z","title":"Harvard College Observatory Bulletin , year = 1930, month = mar, volume =","venue":null,"work_id":null,"year":1930},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:15.627906Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:1ee67b33fb57482845553d5b8f61923a7e5f3915160c10f70091860b7379ddf9","observation_id":"0b85cb59-ec08-493c-9f60-ece3d7244877","resolution":{"observed_at":"2026-08-02T02:59:15.627906Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:15.701895Z","title":"Publications of the David Dunlap Observatory , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:15.701895Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:106c8e1270acfb55c4d6a5a887cbbad694f7880c5a2f5fcf62bc2a4d44306719","observation_id":"345bff81-0b8a-4bae-b45a-f70809ebaeac","resolution":{"observed_at":"2026-08-02T02:59:15.701895Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:15.754063Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:15.754063Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:5c7e2de4e76c126174b0d72764a78ed771c7f22367b3762e100346c8f93ecced","observation_id":"ecb2156b-25b9-437f-afb1-8d5e2b3bd6b9","resolution":{"observed_at":"2026-08-02T02:59:15.754063Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0912.0192","last_updated":"2009-12-01T15:59:38Z","snapshot_observed_at":"2026-08-15T05:32:35.541358Z","submitted_at":"2009-12-01T15:59:38Z","title":"The cluster Terzan 5 as a remnant of a primordial building block of the Galactic bulge","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0912.0192","snapshot_observed_at":"2026-08-02T02:59:15.813198Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:15.813198Z"},"links":{"cited_paper":"/paper/0912.0192","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:eb9c828414317e1e8d3e1e509f4a6909de025527d1c6db91058615b3745cbb56","observation_id":"94349cdb-d254-4194-9e8e-4924ff4c3b00","resolution":{"observed_at":"2026-08-02T02:59:15.813198Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1006.5866","last_updated":"2010-06-30T14:29:13Z","snapshot_observed_at":"2026-08-15T05:14:58.186628Z","submitted_at":"2010-06-30T14:29:13Z","title":"Detailed abundances of a large sample of giant stars in M 54 and in the Sagittarius nucleus","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1006.5866","snapshot_observed_at":"2026-08-02T02:59:15.865987Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:15.865987Z"},"links":{"cited_paper":"/paper/1006.5866","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:f7280b1c1d9aebec7dce3aeda85929ce90a62f8555f6a79728bc9f03f5c7f181","observation_id":"ad0e9288-4729-46c5-8362-8bc3366ffb41","resolution":{"observed_at":"2026-08-02T02:59:15.865987Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:15.962888Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:15.962888Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:46a37d8b4415c71fe68da025c06571e2746341e33e4bb3b56589cadcab8bf1a4","observation_id":"6557e8ff-a788-4eba-a8d7-b510dc793cc9","resolution":{"observed_at":"2026-08-02T02:59:15.962888Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.02042","last_updated":"2020-11-03T22:28:54Z","snapshot_observed_at":"2026-08-16T19:08:17.026380Z","submitted_at":"2020-11-03T22:28:54Z","title":"The Accreted Nuclear Clusters of the Milky Way","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.02042","snapshot_observed_at":"2026-08-02T02:59:16.038152Z","title":", keywords =","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:16.038152Z"},"links":{"cited_paper":"/paper/2011.02042","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:009bb7fe291989fbd4adc778a88d3f359e47f76c9e7444e2dd8f115cec222db8","observation_id":"e5e5d7e4-15db-4ea0-840f-2243a5d97bdf","resolution":{"observed_at":"2026-08-02T02:59:16.038152Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1507.01596","last_updated":"2015-07-06T20:00:48Z","snapshot_observed_at":"2026-08-14T22:41:33.115096Z","submitted_at":"2015-07-06T20:00:48Z","title":"A chemical trompe-l'\\oe{}il: no iron spread in the globular cluster M22","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1507.01596","snapshot_observed_at":"2026-08-02T02:59:16.098446Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:16.098446Z"},"links":{"cited_paper":"/paper/1507.01596","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:4af5431a6258b4f73081d412a99c2ae8c3fb8d6d536e5922224fdbc3f8af1c34","observation_id":"df922792-b482-47c4-9d1c-27756a48b277","resolution":{"observed_at":"2026-08-02T02:59:16.098446Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.04839","last_updated":"2020-04-29T08:24:15Z","snapshot_observed_at":"2026-08-03T03:22:40.408637Z","submitted_at":"2019-12-10T17:30:46Z","title":"Homogeneous Analysis of Globular Clusters from the APOGEE Survey with the BACCHUS Code. II. The Southern Clusters and Overview","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.04839","snapshot_observed_at":"2026-08-02T02:59:16.156289Z","title":"The Southern clusters and overview","venue":null,"work_id":null,"year":1912},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:16.156289Z"},"links":{"cited_paper":"/paper/1912.04839","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:2d550d7ebe62b2aeeedaf7580fd8b6222ad148c9f6274f51f68ea65d8d845fca","observation_id":"b21d0cd9-6599-4bea-a7b8-00df2cac0e7a","resolution":{"observed_at":"2026-08-02T02:59:16.156289Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:16.223785Z","title":"Spectral Evolution of Galaxies , year = 1986, publisher =","venue":null,"work_id":null,"year":1986},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:16.223785Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:6ee46cc3c8b7bff9dec2c4404c28459b1a48e8e295316336f6f4b986030e7507","observation_id":"5cc94ee4-0473-48b7-bfb8-6195d0143322","resolution":{"observed_at":"2026-08-02T02:59:16.223785Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.04824","last_updated":"2018-06-13T02:23:31Z","snapshot_observed_at":"2026-08-14T19:04:27.674738Z","submitted_at":"2018-06-13T02:23:31Z","title":"A new model for the multiple stellar populations within Terzan 5","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.04824","snapshot_observed_at":"2026-08-02T02:59:16.298395Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:16.298395Z"},"links":{"cited_paper":"/paper/1806.04824","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:ea766fac67115bf2b005943d9d924c60290f7978ac8b0df98e56d5a83a0f45ed","observation_id":"55ac212e-d473-4ef3-aace-6cedf3b59eda","resolution":{"observed_at":"2026-08-02T02:59:16.298395Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.02348","last_updated":"2021-01-07T03:19:06Z","snapshot_observed_at":"2026-08-16T18:53:49.253211Z","submitted_at":"2021-01-07T03:19:06Z","title":"Simulations of globular clusters within their parent galaxies: multiple stellar populations and internal kinematics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.02348","snapshot_observed_at":"2026-08-02T02:59:16.395453Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:16.395453Z"},"links":{"cited_paper":"/paper/2101.02348","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:01462ec8b57cbe4d8ad939b959978a777e051d098500be7559f605ac82319922","observation_id":"4020ca52-f81f-444e-846d-7be623f8dca4","resolution":{"observed_at":"2026-08-02T02:59:16.395453Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:16.467004Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:16.467004Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:b0ce86d4751c1a83261f6f6fea3ee240090b23f34edd237c5b440f778689367b","observation_id":"660a875a-0d33-473a-8040-0a429ca5f27c","resolution":{"observed_at":"2026-08-02T02:59:16.467004Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1712.01286","last_updated":"2017-12-04T19:00:01Z","snapshot_observed_at":"2026-08-15T18:30:18.376810Z","submitted_at":"2017-12-04T19:00:01Z","title":"Multiple Stellar Populations in Globular Clusters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1712.01286","snapshot_observed_at":"2026-08-02T02:59:16.543177Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:16.543177Z"},"links":{"cited_paper":"/paper/1712.01286","citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:79518316737bac0273de1fcf14820e6a9ccbe915b19a629eeadd76482e9b17fd","observation_id":"60036686-8c02-49f6-85fc-73655e888ee3","resolution":{"observed_at":"2026-08-02T02:59:16.543177Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:16.603581Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:16.603581Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:18bedbf06981dce3e13d4b8410562857cd1f79dde4ed4a2761ff4319620d1e51","observation_id":"433031ca-f82e-49ee-bffb-71ce7b21b1eb","resolution":{"observed_at":"2026-08-02T02:59:16.603581Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:16.670898Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:16.670898Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:7921292a7f3a7acae5043b8aae52527508846cf74aa735e81002e539d2b8876d","observation_id":"6ae73a22-5117-410c-80bf-0c22256de5b6","resolution":{"observed_at":"2026-08-02T02:59:16.670898Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:16.736493Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:16.736493Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:2132cbc8adab3cf00b00e3d70693dd9d29f1c6c6cb7a90e5df4728eaa84e3d8d","observation_id":"371305ca-55bf-43d3-935a-f93d1d693514","resolution":{"observed_at":"2026-08-02T02:59:16.736493Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:16.820580Z","title":", year = 1980, month = jan, volume =","venue":null,"work_id":null,"year":1980},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:16.820580Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:507bc59b139f44051f63978411ac466722c1d1ed98021dd0e513e8ac94831115","observation_id":"cf3771c0-6b99-487d-98f6-8d0a24764565","resolution":{"observed_at":"2026-08-02T02:59:16.820580Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:16.891310Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:16.891310Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:d21ded69258d442269bdd47861206860b0e6dbda2ce9e2ea7ad4fe000828380f","observation_id":"243d5b53-5586-4eec-a723-d1aa75d98856","resolution":{"observed_at":"2026-08-02T02:59:16.891310Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T02:59:16.937509Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios","version":1},"reference_index":101,"source":"arxiv_source","source_observed_at":"2026-08-02T02:59:16.937509Z"},"links":{"citing_paper":"/paper/2607.14066"},"observation_digest":"sha256:a522c3a59ae2d31ff9cfa422572ca5874b923a2d8087b631be54f2650345adb0","observation_id":"4aa744c6-bb0c-4a87-acf8-ffc79e56bbdb","resolution":{"observed_at":"2026-08-02T02:59:16.937509Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2607.14066","last_updated":"2026-07-15T17:36:45Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-12T08:16:33.224538Z","submitted_at":"2026-07-15T17:36:45Z","title":"The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":100,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":295},"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":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 100 of 295 outbound references and 0 inbound Pith citation observations for arXiv:2607.14066."}