{"as_of":"2026-08-08T10:18:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:ebfac1ac61561d342112667e9c2e6e1504ae779c434bfbb5bd60d3ab2e6e0798","coverage":[{"denominator":176,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T13:18:31.963641Z","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":"2026-08-08T06:32:00.761636+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/2505.22302/citation-record","integrity":"/paper/2505.22302/integrity","json":"/paper/2505.22302/citation-record.json","paper":"/paper/2505.22302"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T13:18:23.329047Z","title":"write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:23.329047Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:1f618a5b41f0db023458a8196fbde46d00477e0133f7c109219562cd77437035","observation_id":"42c4ce36-e85a-459e-836e-7e59bb79e6ca","resolution":{"observed_at":"2026-08-07T13:18:23.329047Z","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":"2026-08-07T13:18:23.381734Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:23.381734Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:4f83965a34bd7a84aa5ff2d1ceb1af37321df0740d4894b0afc633a51d5aab3f","observation_id":"52fecd0e-b87b-4086-b2da-a703612b3601","resolution":{"observed_at":"2026-08-07T13:18:23.381734Z","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":"2026-08-07T13:18:23.462286Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:23.462286Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:1df0c0b8306ee187d82abe641f40dba0a7abaf3a795e11dcdd79573e4c633f3e","observation_id":"b2bd1883-027b-4cc4-942e-4b5c61a9a5c6","resolution":{"observed_at":"2026-08-07T13:18:23.462286Z","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":"2026-08-07T13:18:23.568855Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:23.568855Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:fd569aa179268abf63260648d1480e9701dd7d1928862f32e7e0fb22afec971f","observation_id":"8baf78a9-cadb-4c63-a091-ec5afa3097e6","resolution":{"observed_at":"2026-08-07T13:18:23.568855Z","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":"2026-08-07T13:18:23.679165Z","title":"P., et al., 2013, @doi [ ] 10.1093/mnras/stt860 , https://ui.adsabs.harvard.edu/abs/2013MNRAS.433.1951A 433, 1951","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:23.679165Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:5a85580d0a8a04700a568269dc149e11a751b0fa51b27be1c7fa62b9977e24d4","observation_id":"995392ec-67b8-40ef-8f44-ff15ef6495e7","resolution":{"observed_at":"2026-08-07T13:18:23.679165Z","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":"2026-08-07T13:18:23.759112Z","title":"M., Banerjee D","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:23.759112Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:ea63d5cdb0686602f7e8e485e5af39d2017a6b29fb71a103c07330529bf1c919","observation_id":"235754cf-dd81-4f48-8ab1-61dab3fca18a","resolution":{"observed_at":"2026-08-07T13:18:23.759112Z","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":"2026-08-07T13:18:23.858408Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:23.858408Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:82ba845f9fe9bf7e0fbe8752d83c40d55cbfb915dd03276e2cb159632d71949b","observation_id":"4e24f308-5d8b-4be7-98df-851332b05383","resolution":{"observed_at":"2026-08-07T13:18:23.858408Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9709094","last_updated":"1997-09-10T17:53:07Z","snapshot_observed_at":"2026-08-06T02:42:17.687721Z","submitted_at":"1997-09-10T17:53:07Z","title":"Thermonuclear Burning on Rapidly Accreting Neutron Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9709094","snapshot_observed_at":"2026-08-07T13:18:23.950273Z","title":"515, The Many Faces of Neutron Stars","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:23.950273Z"},"links":{"cited_paper":"/paper/astro-ph/9709094","citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:dfddc27535eb15e412888328eac3d46ede2f4ff3ae5394cb9423796ed80235d6","observation_id":"a549bda5-14c5-4704-9488-16b1674623c9","resolution":{"observed_at":"2026-08-07T13:18:23.950273Z","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":"2026-08-07T13:18:24.014395Z","title":"I., Dunina-Barkovskaya N","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:24.014395Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:9e7f821cd355393f4f2abd2c7ed14d793f98ba7c2e4f33e9930549afea1eca6d","observation_id":"219bc58b-b411-4845-ba1c-aad4dadc07a3","resolution":{"observed_at":"2026-08-07T13:18:24.014395Z","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":"2026-08-07T13:18:24.159348Z","title":"F., et al., 2016, @doi [ ] 10.3847/0004-637X/818/2/145 , https://ui.adsabs.harvard.edu/abs/2016ApJ...818..145B 818, 145","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:24.159348Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:c2baf8ecb1c7dea115ce66e9bf8777c8d831fbf1c8eec192772595836255cd6c","observation_id":"fbf7c68d-0e34-4c1d-9bcb-446de190851b","resolution":{"observed_at":"2026-08-07T13:18:24.159348Z","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":"2026-08-07T13:18:24.264650Z","title":"E., Garc \\' a L","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:24.264650Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:18287a6cd10dddbd1efcbccf1657c946ca2c60adbbef06f6f8929f79a4724b90","observation_id":"af397586-6b48-43a2-a185-eadb9f72b24e","resolution":{"observed_at":"2026-08-07T13:18:24.264650Z","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":"2026-08-07T13:18:24.367982Z","title":null,"venue":null,"work_id":null,"year":1992},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:24.367982Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:2d1e2d0539b96522c68afc021b6ffe5e34ca46ac9af177d7a766d54745c2c06a","observation_id":"aa3c1f73-b717-4ff4-945b-de17634ffe96","resolution":{"observed_at":"2026-08-07T13:18:24.367982Z","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":"2026-08-07T13:18:24.440773Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:24.440773Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:4e727471a0cd35d00282967b1c50cf73443564adfc737dc259abdb24b00a7380","observation_id":"812b64e8-f7f2-4658-b9d6-fe2b1370eeeb","resolution":{"observed_at":"2026-08-07T13:18:24.440773Z","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":"2026-08-07T13:18:24.486488Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:24.486488Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:278a961fd16e7241d651fc1d82ce6e100675aa46b2106d519d48e521091e29ba","observation_id":"83a8580b-296d-4c0c-b6d0-174018dae80d","resolution":{"observed_at":"2026-08-07T13:18:24.486488Z","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":"2026-08-07T13:18:24.571606Z","title":"L., Galloway D","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:24.571606Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:c16b0204b29269a7c7466f21348d4a6ae1a3130eb3eb6341db0baeba594e24a6","observation_id":"d79cdc8f-8ca9-413b-95ad-51a939cd0eed","resolution":{"observed_at":"2026-08-07T13:18:24.571606Z","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":"2026-08-07T13:18:24.702627Z","title":"H., 1998, @doi [ ] 10.1038/28561 , https://ui.adsabs.harvard.edu/abs/1998Natur.394..346C 394, 346","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:24.702627Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:89a43fe4de641bea8b8bf764b9d878c4c05ab3d2eccf1dfa5df0b38805a3a395","observation_id":"f6895984-d7c4-4091-a597-d6198463ce09","resolution":{"observed_at":"2026-08-07T13:18:24.702627Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-08-07T13:18:24.862687Z","title":null,"venue":null,"work_id":null,"year":1933},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:24.862687Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:977959dec2deb1965ce9da3fb007bbb332984948de294ba530bdb6804455210f","observation_id":"95b96444-d4bc-4511-9c40-e549c6b3beb7","resolution":{"observed_at":"2026-08-07T13:18:24.862687Z","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":"2026-08-07T13:18:24.935624Z","title":"D., Shen K","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:24.935624Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:1ea7ec2ec955ccfdff7a54840379b4cc62296f7c6e7fd2bac64e6bb41305e647","observation_id":"39bc9eac-57db-4fc5-a424-18123f2be5cf","resolution":{"observed_at":"2026-08-07T13:18:24.935624Z","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":"2026-08-07T13:18:25.005418Z","title":"R., Wood K","venue":null,"work_id":null,"year":1984},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:25.005418Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:b0dd345925ce3b9188b7927b0a2acb843e3e23d8588f459444c37230f6ec3754","observation_id":"f6cba3ed-a102-4c4c-9711-aa5b33d9d65c","resolution":{"observed_at":"2026-08-07T13:18:25.005418Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0003454","last_updated":"2000-03-30T12:50:58Z","snapshot_observed_at":"2026-07-07T00:10:39.970994Z","submitted_at":"2000-03-30T12:50:58Z","title":"The longest thermonuclear X-ray burst ever observed? (A BeppoSAX Wide Field Camera observation of 4U 1735-44)","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0003454","snapshot_observed_at":"2026-08-07T13:18:25.053079Z","title":null,"venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:25.053079Z"},"links":{"cited_paper":"/paper/astro-ph/0003454","citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:78978d9f184c393f4304df18c93b3369a98a4c73d61dd9f84b714b0004d5552d","observation_id":"5c2ac009-a206-4f61-849c-30ff96e51fe9","resolution":{"observed_at":"2026-08-07T13:18:25.053079Z","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":"2026-08-07T13:18:25.114440Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:25.114440Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:27b7bd16c2d00a96d78d098abf8e3ccd9280debdbe131beb89084863ae4a2c1a","observation_id":"a785c065-9e43-44fc-bfb6-c1851d281f47","resolution":{"observed_at":"2026-08-07T13:18:25.114440Z","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":"2026-08-07T13:18:25.208086Z","title":"P., Crampton D., Hutchings J","venue":null,"work_id":null,"year":1979},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:25.208086Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:23086725b4df103a9bc8612d33f2513e53d5281ba21220bbfefe417412395fe6","observation_id":"9a319b6e-9674-49ee-997b-6957ce096ca4","resolution":{"observed_at":"2026-08-07T13:18:25.208086Z","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":"2026-08-07T13:18:25.345092Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:25.345092Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:cf6d871c0f640f1966e95ea5b322947c7b20955c64e60d88cdeb42113d8aa582","observation_id":"610b09f2-aaa8-45e1-87b2-d5da51a6feea","resolution":{"observed_at":"2026-08-07T13:18:25.345092Z","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":"2026-08-07T13:18:25.422465Z","title":null,"venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:25.422465Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:71bc485007402e27845e7bfd516e1ffae1d305394193a85f99346fb26012b3b3","observation_id":"20a9ba63-3981-41c8-a5ba-f0724b44a613","resolution":{"observed_at":"2026-08-07T13:18:25.422465Z","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":"2026-08-07T13:18:25.526830Z","title":null,"venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:25.526830Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:8c949cc488134b61dde3ba1eb4dbb926886ca33b6a1d52efa8d6995f50a82045","observation_id":"6e3f2b31-cda2-4000-8e06-68191d900e89","resolution":{"observed_at":"2026-08-07T13:18:25.526830Z","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":"2026-08-07T13:18:25.656604Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:25.656604Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:f214b861085acbc9cb6716e20ccf5c9ed4a065a42972a58ca4ca37e1c2fcbbb7","observation_id":"249279ed-f0b1-473e-b727-d2be74fe6408","resolution":{"observed_at":"2026-08-07T13:18:25.656604Z","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":"2026-08-07T13:18:25.795274Z","title":"J., Henze M., 2020, @doi [Advances in Space Research] 10.1016/j.asr.2019.09.044 , https://ui.adsabs.harvard.edu/abs/2020AdSpR..66.1147D 66, 1147","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:25.795274Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:6d5d2c9d7fa4d7ed8e2183e004c0f1857f57e83b5e86370eb1f5de714f1a943b","observation_id":"9e4fb0e3-c19d-4fde-9b76-d59a80e024ab","resolution":{"observed_at":"2026-08-07T13:18:25.795274Z","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":"2026-08-07T13:18:25.962251Z","title":"J., et al., 2016, @doi [ ] 10.3847/1538-4357/833/2/149 , https://ui.adsabs.harvard.edu/abs/2016ApJ...833..149D 833, 149","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:25.962251Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:c88ef3af2b9eff98d058f07c6cdf9b95a8272500b5966f7df5ce7be25279da35","observation_id":"7d954b81-7f8f-4192-ad2c-1f3e19a269be","resolution":{"observed_at":"2026-08-07T13:18:25.962251Z","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":"2026-08-07T13:18:26.084030Z","title":"J., et al., 2017, @doi [ ] 10.3847/1538-4357/aa9062 , https://ui.adsabs.harvard.edu/abs/2017ApJ...849...96D 849, 96","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:26.084030Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:0ce962639f2aff9ac331f273a7476275739f1ffba7dfdb1c097d6255e7b80c0c","observation_id":"6ef51fb8-0393-4756-9b98-642e7937825c","resolution":{"observed_at":"2026-08-07T13:18:26.084030Z","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":"2026-08-07T13:18:26.185748Z","title":"J., et al., 2019, @doi [ ] 10.1038/s41586-018-0825-4 , https://ui.adsabs.harvard.edu/abs/2019Natur.565..460D 565, 460","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:26.185748Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:fc934e8f4d1ee6c82510e5a5dd7e64d7f03959e22bec3b8340dd5a44be0bc22f","observation_id":"f22594ee-acec-4429-9996-71278f91d0d3","resolution":{"observed_at":"2026-08-07T13:18:26.185748Z","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":"2026-08-07T13:18:26.255642Z","title":"J., Kuin N","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:26.255642Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:2d13fddfda61cacb976e043ab4717ee69a452b89cb4c3ea3fc2da351fbb302e4","observation_id":"3c697b68-1c7e-4522-9a3d-f83088da44cf","resolution":{"observed_at":"2026-08-07T13:18:26.255642Z","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":"2026-08-07T13:18:26.332341Z","title":null,"venue":null,"work_id":null,"year":1973},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:26.332341Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:09267717f03eb1e131db06468c15f5d7d7c6f85c9f480c7f22f8e211ab095dbb","observation_id":"e4e97040-5826-4596-acc0-10b1e6ef614e","resolution":{"observed_at":"2026-08-07T13:18:26.332341Z","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":"2026-08-07T13:18:26.417658Z","title":"C., Heinke C","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:26.417658Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:8a780764eab7769c1e9224f80a7300a235c5ca7833d35b1449d2b3a3e9a52db8","observation_id":"e57aa999-5fcf-416b-a674-3f2b9ba71419","resolution":{"observed_at":"2026-08-07T13:18:26.417658Z","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":"2026-08-07T13:18:26.482677Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:26.482677Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:2f1a2cead2312b5a87181380b60906e307419b20241950b2c9c59fc9907a19a0","observation_id":"384da627-608f-49bb-9be8-5b6d228f3941","resolution":{"observed_at":"2026-08-07T13:18:26.482677Z","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":"2026-08-07T13:18:26.548419Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:26.548419Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:35de66a852871c52a83e44aa08d09ce6dd45dec36cca6ccb3ada2fbc7db26c5d","observation_id":"3a080a9b-d5e1-4e01-b850-cab0dad31e10","resolution":{"observed_at":"2026-08-07T13:18:26.548419Z","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":"2026-08-07T13:18:26.642696Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:26.642696Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:ec9995ac661102216439987b67e304e0636f9fb07686ca5b1d18d1cd2713a068","observation_id":"1260ce34-62a3-435b-b5f2-1199c0a484af","resolution":{"observed_at":"2026-08-07T13:18:26.642696Z","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":"2026-08-07T13:18:26.764687Z","title":"Y., Hanawa T., Miyaji S., 1981, @doi [ ] 10.1086/159034 , 247, 267","venue":null,"work_id":null,"year":1981},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:26.764687Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:0902295008328998a035b8abeb4281964490e709a80c7f906a0a0b2844bdd83c","observation_id":"ad6ac952-ae8a-4f10-b110-84ed76328358","resolution":{"observed_at":"2026-08-07T13:18:26.764687Z","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":"2026-08-07T13:18:26.930428Z","title":"K., Cumming A., 2006, @doi [ ] 10.1086/507598 , 652, 559","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:26.930428Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:cb63a4c9405221bff7544a7d336ba10a3ecbfe5259d57a53284b13a850f65cf5","observation_id":"3636d9e3-ab65-436e-8187-1c8b52517e08","resolution":{"observed_at":"2026-08-07T13:18:26.930428Z","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":"2026-08-07T13:18:27.137092Z","title":"K., Cumming A., Kuulkers E., Bildsten L., Chakrabarty D., Rothschild R","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:27.137092Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:dafe0fafeabb4842652c83a979134526ac9e34ac751702ccacd6dedd76852440","observation_id":"c6bdae8b-55be-4265-a41b-21d388642b85","resolution":{"observed_at":"2026-08-07T13:18:27.137092Z","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":"2026-08-07T13:18:27.232348Z","title":"K., Muno M","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:27.232348Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:9b5a760264d19c71c5093d8877cac8450567df907b82b871fdc0a2e403643a86","observation_id":"f0e1d520-9b65-47e9-aceb-34cb2c013d5a","resolution":{"observed_at":"2026-08-07T13:18:27.232348Z","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":"2026-08-07T13:18:27.305222Z","title":"K., et al., 2018, @doi [ ] 10.3847/2041-8213/aabd32 , https://ui.adsabs.harvard.edu/abs/2018ApJ...857L..24G 857, L24","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:27.305222Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:b960676a379d86558ae1428ee6e82bf5493f5f2ac9ec8f30414a36bad71b45b5","observation_id":"7734b444-39a3-4643-a5dd-bb20fa70829c","resolution":{"observed_at":"2026-08-07T13:18:27.305222Z","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":"2026-08-07T13:18:27.364533Z","title":"K., et al., 2020, @doi [ ] 10.3847/1538-4365/ab9f2e , https://ui.adsabs.harvard.edu/abs/2020ApJS..249...32G 249, 32","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:27.364533Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:c035acc76b9570b1e59a6d3ada17c5da44929a8800dd591e59321eee801e016f","observation_id":"01c800de-0ea5-4694-940a-14f21bb72603","resolution":{"observed_at":"2026-08-07T13:18:27.364533Z","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":"2026-08-07T13:18:27.415248Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:27.415248Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:daf9d61ab18ff9e5b0a2fb8733a46075756ff031a42a435c4db9582552f9408e","observation_id":"278a550a-db5d-4235-8da9-57f8eb9951cd","resolution":{"observed_at":"2026-08-07T13:18:27.415248Z","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":"2026-08-07T13:18:27.472171Z","title":"M., Balman S ., Blair W","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:27.472171Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:8fe910bd19489c55e66fd5d492145359778f64489943c7d82b84a4ca8df869dd","observation_id":"702e8df1-e1c9-4adb-884e-6dd88741a2db","resolution":{"observed_at":"2026-08-07T13:18:27.472171Z","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":"2026-08-07T13:18:27.547380Z","title":"J., Galloway D","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:27.547380Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:ccdc7d315b197fb5cea75148ee5e6eff22c241666923a1afc859239e000e4fb3","observation_id":"b60aa036-4d98-4235-b4b6-c2e320c90fdb","resolution":{"observed_at":"2026-08-07T13:18:27.547380Z","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":"2026-08-07T13:18:27.742462Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:27.742462Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:a35dbcecf0c78df41085a612e8fb051710d21c3a7559dd6dd3b751e53ac028af","observation_id":"3c9a4fbb-af45-439f-8d69-cdde9443c38e","resolution":{"observed_at":"2026-08-07T13:18:27.742462Z","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":"2026-08-07T13:18:27.936829Z","title":null,"venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:27.936829Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:dbc20d5b01b656762b8d7f075295e335bca78e133d4e40d5e77ef456718e0e5a","observation_id":"a5c1d8d1-f553-4ac8-8697-56d1eaa77da1","resolution":{"observed_at":"2026-08-07T13:18:27.936829Z","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":"2026-08-07T13:18:27.998124Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:27.998124Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:dde188df9971e57980563e8766c851e67946ef9cd74f9a2f4ae2aaebe00277ee","observation_id":"1761ae71-878a-45aa-bf92-135d8303004d","resolution":{"observed_at":"2026-08-07T13:18:27.998124Z","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":"2026-08-07T13:18:28.066159Z","title":null,"venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:28.066159Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:d10dd8972f09535af465c9ee3883cc7b7d9b2e79dde3930861de75ad7fb20a74","observation_id":"54ee1c1b-743c-441b-a59d-20d704b23ef3","resolution":{"observed_at":"2026-08-07T13:18:28.066159Z","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":"2026-08-07T13:18:28.130574Z","title":"L., 1990, , 227, 431","venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:28.130574Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:cd6a0eb5a0c9b0c496cdfcad930aeb0433df2ad9eae45ade283043548a7c053c","observation_id":"46c7a0e6-5d4c-455d-97ec-5c76735b090b","resolution":{"observed_at":"2026-08-07T13:18:28.130574Z","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":"2026-08-07T13:18:28.186400Z","title":"L., 2003, @doi [ ] 10.1051/0004-6361:20030708 , 404, L33","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:28.186400Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:7f573c4bdb96fdab9533e8e7b74f521dd55bb0d7fcb3edbb3c0f12fe1cf90eb5","observation_id":"50ec3004-f8c2-4119-9f85-04a8f1557c47","resolution":{"observed_at":"2026-08-07T13:18:28.186400Z","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":"2026-08-07T13:18:28.241545Z","title":"E., 2007, @doi [ ] 10.1086/517491 , https://ui.adsabs.harvard.edu/abs/2007ApJ...665.1311H 665, 1311","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:28.241545Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:f486a5601f98d143947badcef585091c8bebdc832834a3302a3455ead8b80390","observation_id":"13186893-1cac-4465-af81-4dbcdf56c1c5","resolution":{"observed_at":"2026-08-07T13:18:28.241545Z","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":"2026-08-07T13:18:28.293712Z","title":"O., Zheng J., Maccarone T","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:28.293712Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:04aa708b707d9c87af2d3fd2940c54da4ff50e2811224edecebd7de4859dc9bb","observation_id":"f809b9d6-7eaa-4e31-8d70-1dcc7c7cb826","resolution":{"observed_at":"2026-08-07T13:18:28.293712Z","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":"2026-08-07T13:18:28.319344Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:28.319344Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:3b24559c42f04d8b6f2eba29d625e107f68ad23595b99adcc1c0dea7aaea31a7","observation_id":"6470ce19-3347-4859-927e-3f31065a7cb7","resolution":{"observed_at":"2026-08-07T13:18:28.319344Z","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":"2026-08-07T13:18:28.390887Z","title":"A., Rogers F","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:28.390887Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:9afaf200ef0ed8e7be0ad476b786353156da04890b50dee1459913d18d55d72d","observation_id":"9f51e76a-2f52-49b1-a7a3-65d6a035dc03","resolution":{"observed_at":"2026-08-07T13:18:28.390887Z","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":"2026-08-07T13:18:28.456271Z","title":"A., Linares M., Connaughton V., Beklen E., Camero-Arranz A., Finger M","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:28.456271Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:1258c5e99c3a806ffe6875e4145969f9b4398cdc7984dbd3e2cb165481782443","observation_id":"a87eeb87-8690-439c-99ab-0d2e4f60b22d","resolution":{"observed_at":"2026-08-07T13:18:28.456271Z","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":"2026-08-07T13:18:28.524212Z","title":"CRC Press","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:28.524212Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:797266df9ec7dcc086444f3ca049f589419c9cdaa20410a843d5a216649edf0a","observation_id":"dbdc3666-5c38-4bbe-8248-d1eebcda8797","resolution":{"observed_at":"2026-08-07T13:18:28.524212Z","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":"2026-08-07T13:18:28.589062Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:28.589062Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:e12c9939dd8f44df47dc7acd058bf35396912167d5744e8467b92762e7a191d5","observation_id":"32dc36ca-43b3-4573-94cc-08f10baa8046","resolution":{"observed_at":"2026-08-07T13:18:28.589062Z","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":"2026-08-07T13:18:28.660081Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:28.660081Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:be51d0b901ba7b005d6dd2460e8d7cdffa30e47d1e8040e84f7c02e1df82caed","observation_id":"fbffb6ea-00f0-40aa-83d4-23ac51208f7e","resolution":{"observed_at":"2026-08-07T13:18:28.660081Z","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":"2026-08-07T13:18:28.732424Z","title":"N., 2008, in Bode M","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:28.732424Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:6ddd2a8ac99dd10bc760856157d426c7de09bd6a9804ddd3ef5663827f73aa18","observation_id":"ff8fde75-a81d-4081-946b-001bc0aa565a","resolution":{"observed_at":"2026-08-07T13:18:28.732424Z","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":"2026-08-07T13:18:28.774228Z","title":"M., Psaltis D., Chakrabarty D., 2001, @doi [ ] 10.1086/324225 , 560, L59","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:28.774228Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:e0546ea034262aa5ebc6bfaae39ea3b220300ee8059c5df725a154eda9122691","observation_id":"43b52314-9691-4cdc-9aef-484d79792b98","resolution":{"observed_at":"2026-08-07T13:18:28.774228Z","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":"2026-08-07T13:18:28.819111Z","title":null,"venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:28.819111Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:d0d82ff37bc4adde4674e1d2debd51b986cc004f61038d1a2f9fcc5de2e3491f","observation_id":"8ff9577c-05e1-4813-a9bb-cbe8424c417e","resolution":{"observed_at":"2026-08-07T13:18:28.819111Z","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":"2026-08-07T13:18:28.883317Z","title":"J., Holt S","venue":null,"work_id":null,"year":1976},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:28.883317Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:19ed3ea88a084d507800343126547a1a7e98fd9c7ec7e41e6e0f34050a6b8bfd","observation_id":"6ddf3d77-36c5-4a46-8aaf-c9439e4d4fb5","resolution":{"observed_at":"2026-08-07T13:18:28.883317Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0005453","last_updated":"2000-05-23T13:37:11Z","snapshot_observed_at":"2026-07-07T00:11:27.453055Z","submitted_at":"2000-05-23T13:37:11Z","title":"Discovery of 1RXS J171824.2-402934 as an X-ray burster","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0005453","snapshot_observed_at":"2026-08-07T13:18:28.978209Z","title":"G., in't Zand J","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:28.978209Z"},"links":{"cited_paper":"/paper/astro-ph/0005453","citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:44ffdad37d64f842d30b44e391f3cb69036723db36623b1cae0cc6f5bbccf2e6","observation_id":"2f70305f-0902-44c6-9a8a-fed623004558","resolution":{"observed_at":"2026-08-07T13:18:28.978209Z","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":"2026-08-07T13:18:29.048046Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:29.048046Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:fcd3a2b7bca6c4c4d8aa58c45e2cd630220f524e3da4d1f8365030280d1d4468","observation_id":"b27aff62-a65b-47f3-a4a3-163ee1876a96","resolution":{"observed_at":"2026-08-07T13:18:29.048046Z","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":"2026-08-07T13:18:29.128734Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:29.128734Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:e84e8d843d30a265da64f8715b5972351876f92b7304c1976dea90049c60b7a7","observation_id":"0bed98bc-d349-442b-af01-98b4fa4b9a72","resolution":{"observed_at":"2026-08-07T13:18:29.128734Z","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":"2026-08-07T13:18:29.218063Z","title":"K., Zand J","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:29.218063Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:932938987704488121feb26eb709066998edc573c0f09376f91b0b8f364411bf","observation_id":"6462fb64-93e1-4613-a85a-4fa5924e4cdd","resolution":{"observed_at":"2026-08-07T13:18:29.218063Z","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":"2026-08-07T13:18:29.291674Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:29.291674Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:15bca001c9967ac039c5e40b361f2cdce2d345344de8bacddbb9bd08bfaabc72","observation_id":"89a5eb3f-113d-451a-bc5f-dcb4f1a153be","resolution":{"observed_at":"2026-08-07T13:18:29.291674Z","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":"2026-08-07T13:18:29.366014Z","title":null,"venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:29.366014Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:8e24f39a2acfd65b0083c08f449b6da1d62b9e8459c2bbd263bb3397916ee9a0","observation_id":"c709e971-4a12-4b92-8430-92e662e5c50a","resolution":{"observed_at":"2026-08-07T13:18:29.366014Z","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":"2026-08-07T13:18:29.458023Z","title":"R., in't Zand J","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:29.458023Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:0f2d837014e7385501094e6874600e92e2fc5b3c5ca0f1e03b9a2bab2996e769","observation_id":"4a983f71-5ca1-4537-8ca7-43d2dcc79840","resolution":{"observed_at":"2026-08-07T13:18:29.458023Z","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":"2026-08-07T13:18:29.553975Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:29.553975Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:053830397fa99dc78edf79ae7d7d211df4dc4dac768a672096feda34e7093d20","observation_id":"8e921d8f-e3b9-4740-b82d-a9839f89f436","resolution":{"observed_at":"2026-08-07T13:18:29.553975Z","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":"2026-08-07T13:18:29.645738Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:29.645738Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:acd1947cef37e334c5f48af36fd0a79ec2f4f29babf83000b09b01b9229805b0","observation_id":"32dec55b-dfe5-40c8-bb25-43b35f658b38","resolution":{"observed_at":"2026-08-07T13:18:29.645738Z","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":"2026-08-07T13:18:29.717864Z","title":null,"venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:29.717864Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:753195332cff04874ea8fec03d09f9697b3c40b9579d577a2916d38417e7898b","observation_id":"ef0c64d7-4f52-46ed-bcfb-f2f7d56a652c","resolution":{"observed_at":"2026-08-07T13:18:29.717864Z","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":"2026-08-07T13:18:29.809524Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:29.809524Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:4713b416d9af2754c3048f57b9c8ded4679c534b2e0e804f90439c6891f97c1e","observation_id":"ffe574b9-eff7-4908-895a-a28217217348","resolution":{"observed_at":"2026-08-07T13:18:29.809524Z","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":"2026-08-07T13:18:29.906799Z","title":null,"venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:29.906799Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:06320587153f9427580cf227e9eb65171db93d2774369dfac2eb061f54da4252","observation_id":"1958a823-50ec-4005-b431-dc2168ab6310","resolution":{"observed_at":"2026-08-07T13:18:29.906799Z","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":"2026-08-07T13:18:29.995824Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:29.995824Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:1725e4069f5ab3007f131ae5ba32f9dcd09925793ac22b28bb6d7ec849192477","observation_id":"9c0e1ef0-72a6-418e-8984-98c2f4b99e18","resolution":{"observed_at":"2026-08-07T13:18:29.995824Z","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":"2026-08-07T13:18:30.089433Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:30.089433Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:438a6563cc02b4d26fe97f0c91de3ac344b8ecea1ce912880214c039a34d34ee","observation_id":"6ae3dd54-e743-4408-add9-1fd4506bb4df","resolution":{"observed_at":"2026-08-07T13:18:30.089433Z","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":"2026-08-07T13:18:30.166570Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:30.166570Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:28cb13208fba3bcecfe046cb56957cb41c3003a591a1f6792badda9ee48bfebf","observation_id":"12cbcfa8-f4fb-4436-909d-f817d7c9ee7a","resolution":{"observed_at":"2026-08-07T13:18:30.166570Z","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":"2026-08-07T13:18:30.304930Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:30.304930Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:558cbad3d64247a8ae6cf7cc916b8b7b8ee5f69c13296dcec4309240947d31ce","observation_id":"693db32d-96bc-4ed2-a04c-54d121c805a9","resolution":{"observed_at":"2026-08-07T13:18:30.304930Z","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":"2026-08-07T13:18:30.394763Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:30.394763Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:b4b9ef27c9230370745a8bed79bdf6ddc78eb4a2f3496c7ab5e389f958c69653","observation_id":"b30fe587-153a-40e7-ba85-6a613492087c","resolution":{"observed_at":"2026-08-07T13:18:30.394763Z","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":"2026-08-07T13:18:30.462462Z","title":"P., 2009, @doi [Landolt B \\\"o rnstein] 10.1007/978-3-540-88055-4_34 , https://ui.adsabs.harvard.edu/abs/2009LanB...4B..712L 4B, 712","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:30.462462Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:5ef00fa21aef0ab8228151dda5b24e4c44151b782f2ed86d5f9e97a9d4357543","observation_id":"28c27c26-0c53-4f66-baf1-2748c4d35e4f","resolution":{"observed_at":"2026-08-07T13:18:30.462462Z","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":"10.1086/309453","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T13:18:46.170226Z","title":"K., Rudy R","venue":null,"work_id":"8560896f-14bf-48ef-a273-0b95e952467f","year":2000},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:30.556246Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:357d3a1256f172970d9b458fc285d59c08b3f9f082c196e86eae0f76eb62a86d","observation_id":"7c186a7b-11c7-4fde-ac94-2208f0e99443","resolution":{"observed_at":"2026-08-07T13:18:46.232610Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T13:18:30.638805Z","title":"C., Altamirano D., Garc \\' a F., Lyu M., M \\'e ndez M., Combi J","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:30.638805Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:a0bb811a7f4a609177aaf216791aa78578f393cf7dedc16852ec557b8d406ff4","observation_id":"26c9b498-023a-42e0-929b-afcb8a0d4501","resolution":{"observed_at":"2026-08-07T13:18:30.638805Z","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":"2026-08-07T13:18:30.727661Z","title":"C., et al., 2023, @doi [ ] 10.1093/mnras/stad949 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.521.5616M 521, 5616","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:30.727661Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:527b62ab850595ccb461405ac814bd7245cb932858cfa534c2cb7b0c9230db7a","observation_id":"97769588-dd88-4ca1-82ec-071ecb442a2e","resolution":{"observed_at":"2026-08-07T13:18:30.727661Z","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":"10.1093/mnras/stad604","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T13:18:45.993742Z","title":null,"venue":null,"work_id":"f675a752-1b75-43a4-966a-b6be6ce99abd","year":2023},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:30.846095Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:bf0a3e6bd0c9b424b09ab004f07b319b68d4408b782ec74fdb6574dcb9ad01f3","observation_id":"8611384d-6602-4044-a31d-aea0d551aec9","resolution":{"observed_at":"2026-08-07T13:18:46.053146Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T13:18:30.924169Z","title":null,"venue":null,"work_id":null,"year":1971},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:30.924169Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:63226fe7e806063cb79e963358a253a305b8d0142d1b4897740dbb36f70e9a84","observation_id":"198c2eea-9cd1-43b4-b40e-63b20dce22f1","resolution":{"observed_at":"2026-08-07T13:18:30.924169Z","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":"2026-08-07T13:18:31.004674Z","title":null,"venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:31.004674Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:ab5cb9429011970d564417aad773434f6367d2a2ebdb7c5fede5f6f23d5cc7fc","observation_id":"4c542161-994a-47f0-9196-63193b6af9f8","resolution":{"observed_at":"2026-08-07T13:18:31.004674Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1305.3424","last_updated":"2013-05-15T10:37:10Z","snapshot_observed_at":"2026-07-06T03:13:25.964368Z","submitted_at":"2013-05-15T10:37:10Z","title":"Modelling the recurrent nova U Scorpii in quiescence","version":1},"cited_work":{"arxiv_id":"1305.3424","doi":"10.48550/arxiv.1305.3424","metadata_source":"pith","pith_arxiv_id":"1305.3424","snapshot_observed_at":"2026-08-07T18:16:16.850658Z","title":"Modelling the recurrent nova U Scorpii in quiescence","venue":"astro-ph.SR","work_id":"e4d7f506-f03f-460f-97bd-f62b3d404095","year":2013},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:31.123667Z"},"links":{"cited_paper":"/paper/1305.3424","citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:4732880a0ce3de472b3e6c9748cfd0f88ea404fd38c3c8496b0243f9d7d526a0","observation_id":"e2d5e4e2-fa01-48ce-95b5-51e6d09c5eb7","resolution":{"observed_at":"2026-08-07T13:18:45.891913Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1134/s106377371010004x","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T13:18:45.607102Z","title":"V., Revnivtsev M","venue":null,"work_id":"87122db0-97c8-4e1c-9e45-77a9da2f031a","year":2010},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:31.209092Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:4ad9b2b673ae47270b6c953b61a6ba2f06173895930ee497d5e0af037c87e180","observation_id":"4e3d1b14-dfeb-4423-b972-0b8c95d40d04","resolution":{"observed_at":"2026-08-07T13:18:45.659936Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T13:18:31.281151Z","title":"M., 2017, @doi [ ] 10.3847/1538-4357/aa87b6 , https://ui.adsabs.harvard.edu/abs/2017ApJ...847...99M 847, 99","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:31.281151Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:c6caee09cf843d0a020c035437089146fbe752d443fc6e0634e0cc0efbe907db","observation_id":"be2c1c86-8a10-4a60-812e-57794aadb71d","resolution":{"observed_at":"2026-08-07T13:18:31.281151Z","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":"2026-08-07T13:18:31.339266Z","title":"M., Udalski A., 2021, @doi [ ] 10.1093/mnras/stab1058 , https://ui.adsabs.harvard.edu/abs/2021MNRAS.504.2122M 504, 2122","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:31.339266Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:421c341dc413de06ce169f460c28bce287008f68c7704adcf490af1371c5fb82","observation_id":"0a1cab22-ff7b-45c8-b2f7-6c5e78f201a9","resolution":{"observed_at":"2026-08-07T13:18:31.339266Z","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":"10.1051/0004-6361:20041846","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T13:18:45.440696Z","title":null,"venue":null,"work_id":"8911db82-64da-4589-901b-ac4230287bdb","year":2005},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:31.397616Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:dd58e4dbaa8c193bab4761e8ad26a79591637345bc2651c5554527b995e3d7bf","observation_id":"09bf6fdc-ee72-44cb-b8f1-5ad411545422","resolution":{"observed_at":"2026-08-07T13:18:45.503089Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.19709","last_updated":"2024-04-30T17:01:18Z","snapshot_observed_at":"2026-07-06T18:07:47.744531Z","submitted_at":"2024-04-30T17:01:18Z","title":"SRG/ART-XC discovery of SRGAJ144459.2-604207: a well-tempered bursting accreting millisecond X-ray pulsar","version":1},"cited_work":{"arxiv_id":"2404.19709","doi":"10.48550/arxiv.2404.19709","metadata_source":"pith","pith_arxiv_id":"2404.19709","snapshot_observed_at":"2026-08-07T18:16:16.850658Z","title":"SRG/ART-XC discovery of SRGAJ144459.2-604207: a well-tempered bursting accreting millisecond X-ray pulsar","venue":"astro-ph.HE","work_id":"2ad67f8a-5ed3-4024-bca7-f8d20b9323e7","year":2024},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:31.464478Z"},"links":{"cited_paper":"/paper/2404.19709","citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:5c6809a9e49ad8a2693ac0c4aeb7fbed5146d43f666849137a199129d683bba5","observation_id":"28f72663-550c-420d-92ca-44670ce74e9c","resolution":{"observed_at":"2026-08-07T13:18:45.367697Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T13:18:31.564508Z","title":"R., Kahn S","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:31.564508Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:ad43462a2f738a369bdaf560d46f856266a33d025e2e89a3597e96762e84e186","observation_id":"81a9c48b-8940-4d30-afc7-d563d991dedc","resolution":{"observed_at":"2026-08-07T13:18:31.564508Z","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":"2026-08-07T13:18:31.650277Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:31.650277Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:754acad6d18cd4d1c1197daac8c93a6516a520dcb15decc0dc8cdeb9e1d4f126","observation_id":"878484f5-e72b-49bf-a4d8-8284c967a1c5","resolution":{"observed_at":"2026-08-07T13:18:31.650277Z","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":"10.1086/379211","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T13:18:45.051351Z","title":"S., 2003, @doi [ ] 10.1086/379211 , https://ui.adsabs.harvard.edu/abs/2003ApJ...599..419N 599, 419","venue":null,"work_id":"350844ea-b8e3-46de-9d42-57624f8dece0","year":2003},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:31.708051Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:ed8cf4a66cb5f6e1264ced41d96f15d9049422e365e975e242bf64c8ae55fb6b","observation_id":"612e5ac7-386f-4c46-9538-72c4195a1b9a","resolution":{"observed_at":"2026-08-07T13:18:45.147138Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T13:18:31.787738Z","title":"G., Marsh T","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:31.787738Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:5152436be23b25565309729b0d99b9a7b95a5298f2c62e470af37c701b5b86bf","observation_id":"00262644-3b1c-4919-8bea-1ef8c97fd478","resolution":{"observed_at":"2026-08-07T13:18:31.787738Z","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":"2026-08-07T13:18:31.846882Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:31.846882Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:117995f9db39d9da614d34e03c899cdd1f2ba94442b552e1311b899aa192ae51","observation_id":"06de6283-b228-45fe-aa2a-7299b738c0d1","resolution":{"observed_at":"2026-08-07T13:18:31.846882Z","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":"2026-08-07T13:18:31.908973Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:31.908973Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:7730b7654bf1673d03d13e2452ecd3f9280fababf1b6ad7e7fc5195ecb032e8d","observation_id":"c2b0002e-72b9-44c5-bd01-d974f22d857c","resolution":{"observed_at":"2026-08-07T13:18:31.908973Z","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":"2026-08-07T13:18:31.963641Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-07T13:18:31.963641Z"},"links":{"citing_paper":"/paper/2505.22302"},"observation_digest":"sha256:868c2b3eeabfd91c4aff145b65a7962d9493599b86dcbfb3832f8426d0677c71","observation_id":"b2028609-7b39-4a70-8733-1bf47d6bd6df","resolution":{"observed_at":"2026-08-07T13:18:31.963641Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2505.22302","last_updated":"2025-05-28T12:38:43Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-07T13:08:16.674092Z","submitted_at":"2025-05-28T12:38:43Z","title":"Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":1,"metadata_mismatch":1,"parse_uncertain":0,"unresolved":92,"verified_exact":6,"verified_fuzzy":0},"total_outbound_references":176},"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":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 100 of 176 outbound references and 0 inbound Pith citation observations for arXiv:2505.22302."}