{"as_of":"2026-08-17T01:00:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:ff5417acce04452338e21e47396c4859dc8e8ecfc02f208ad8632b0f077f324c","coverage":[{"denominator":63,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":63,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T17:09:57.793407Z","state":"measured"},{"denominator":63,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":63,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2412.09306/citation-record","integrity":"/paper/2412.09306/integrity","json":"/paper/2412.09306/citation-record.json","paper":"/paper/2412.09306"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.806224Z","title":"1 and Table I)","venue":null,"work_id":"1e255b0a-191e-4d50-ae45-9bbed59d9b68","year":null},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.499453Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:3e18d8a384716d785ed8b0faca6c240456e40a8e3417c95ebbfc22ff73529323","observation_id":"f13ef6b1-3857-4993-840c-844b2cbdc1d0","resolution":{"observed_at":"2026-08-11T17:09:58.810995Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.820704Z","title":null,"venue":null,"work_id":"5590b125-9fa5-4099-a30f-d1911059eaaa","year":null},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.493517Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:70636de6f925426676095c0e0e63ac56b7f82a228cd0431012693d274ec76b67","observation_id":"b7a25ab2-2778-4080-b77a-a7e460634310","resolution":{"observed_at":"2026-08-11T17:09:58.825340Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.790452Z","title":"2 and Table II), ¯λ is varied between [0.1, 1.0]","venue":null,"work_id":"fdcb1efa-fcb3-4756-b64b-5962d137c683","year":null},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.504500Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:34924a8ce8ee1c7f12e18e97e079eccd4af647fa2570312e54dbb8d65c6ab2ee","observation_id":"6b9ea781-5470-4270-b645-c0d8f0ae2ee5","resolution":{"observed_at":"2026-08-11T17:09:58.795290Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.774750Z","title":"3 and Table III), we explore the effect of vary- ing Beff within the range [60, 90] MeV/fm 3","venue":null,"work_id":"cec2c5f7-6dc0-4f89-8d74-5010830741ac","year":null},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.509498Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:5a46fbc0c8f156a6f760f169d6b394b964103fd57efe5d3011854e8bfc3469dc","observation_id":"adf38113-d974-41bf-86c0-81bf00ea304e","resolution":{"observed_at":"2026-08-11T17:09:58.780128Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.759131Z","title":"Furthermore, we gather the data for maximum compact- ness in Table III depending on the parameters and is found to be 0.297","venue":null,"work_id":"0f49b768-58ee-4cca-b382-cd071c607654","year":null},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.514410Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:577de2202c7604246455393f273b125e86fc23634aec81974c25a8767aeb83d4","observation_id":"f1f2d02b-3c8d-47c4-8d27-9ffa6cb21b15","resolution":{"observed_at":"2026-08-11T17:09:58.764382Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.00363","last_updated":"2024-08-22T03:42:16Z","snapshot_observed_at":"2026-08-16T14:05:00.459263Z","submitted_at":"2024-03-30T13:32:23Z","title":"Recent progresses in strange quark stars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.00363","snapshot_observed_at":"2026-08-11T17:09:57.520150Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.520150Z"},"links":{"cited_paper":"/paper/2404.00363","citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:4d814efa01f7080afcd03e39bab1d4cb7ddb63e6970a4ca743454eeb094e20ae","observation_id":"26667353-bee8-4f43-bce5-0e6941c5f8b2","resolution":{"observed_at":"2026-08-11T17:09:57.520150Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.743434Z","title":null,"venue":null,"work_id":"b2722b42-9c3b-47d3-905e-f5e578b094fd","year":2024},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.525862Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:6f3d5bb3a6a56ec7c09dadb426285122351487f7da20bc91267aa8ecf5387fe4","observation_id":"8cae38cf-d381-4d9c-ae6e-222122b53de2","resolution":{"observed_at":"2026-08-11T17:09:58.748526Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.09875","last_updated":"2024-04-15T15:47:01Z","snapshot_observed_at":"2026-08-16T14:00:47.204623Z","submitted_at":"2024-04-15T15:47:01Z","title":"The NICER data and a $\\sigma$-field dependent stiffness of the hadronic equation of state","version":1},"cited_work":{"arxiv_id":"2404.09875","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.09875","snapshot_observed_at":"2026-08-11T17:09:57.891640Z","title":"The NICER data and a $\\sigma$-field dependent stiffness of the hadronic equation of state","venue":"nucl-th","work_id":"12bc61e6-ca8e-4a7c-a586-1c04b667982f","year":2024},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.530582Z"},"links":{"cited_paper":"/paper/2404.09875","citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:59bc983cc070e4ffe8edfa61c3e3fb73a65e64290a98aa63ac789f0cb7c3eafe","observation_id":"5e37227e-592c-48b9-a31a-ae6504d0f233","resolution":{"observed_at":"2026-08-11T17:09:57.897545Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.729284Z","title":null,"venue":null,"work_id":"eff2cb62-9eb3-4d71-8b71-2168ca871aef","year":2024},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.536149Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:74e352871383454972d9f42e0043634255308ee787a9f3ffe267072e733afb78","observation_id":"04dc19b5-b7c6-4df3-a6c5-8c238c8bb894","resolution":{"observed_at":"2026-08-11T17:09:58.733712Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2402.18912","last_updated":"2024-06-21T09:38:16Z","snapshot_observed_at":"2026-08-16T14:14:16.120505Z","submitted_at":"2024-02-29T07:10:39Z","title":"Hadron-quark phase transition in the neutron star with vector MIT bag model and Korea-IBS-Daegu-SKKU functional","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.18912","snapshot_observed_at":"2026-08-11T17:09:57.540706Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.540706Z"},"links":{"cited_paper":"/paper/2402.18912","citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:a27ac5306594ad9e7adbef50498b99b2c6d76d3e9574bd85940cd650355c7eb5","observation_id":"941234ae-2151-425b-b909-a8a925fbf1e5","resolution":{"observed_at":"2026-08-11T17:09:57.540706Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.08835","last_updated":"2024-12-31T03:36:57Z","snapshot_observed_at":"2026-08-16T14:18:49.017129Z","submitted_at":"2024-02-13T22:42:58Z","title":"Fast Pulsars, Neutron Stars, and Astrophysical Strange Quark Matter Objects","version":3},"cited_work":{"arxiv_id":"2402.08835","doi":null,"metadata_source":"pith","pith_arxiv_id":"2402.08835","snapshot_observed_at":"2026-08-11T17:09:57.855166Z","title":"Fast Pulsars, Neutron Stars, and Astrophysical Strange Quark Matter Objects","venue":"astro-ph.HE","work_id":"d0fac248-e8d6-4332-b2c0-7a3933c8746a","year":2024},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.545472Z"},"links":{"cited_paper":"/paper/2402.08835","citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:7e9ed3fe26be31e33b59184cb37f25af967603e9f2372e1248948cd7447dc48d","observation_id":"2c22cbff-6570-4ba3-a1c6-e3628cfc3625","resolution":{"observed_at":"2026-08-11T17:09:57.860186Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.709327Z","title":"Tangphati, A","venue":null,"work_id":"c36c8d21-372e-42ce-91af-fa4e0338a20c","year":2024},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.550519Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:61bc3f03537e6ef39644af8389ca49ee86831ae991b767ac67674d1d924043b2","observation_id":"ac21d77c-d38b-4e71-913c-2d123c44a2c3","resolution":{"observed_at":"2026-08-11T17:09:58.714432Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.693081Z","title":null,"venue":null,"work_id":"5ce24783-8e5f-4787-aaff-d47d0aa7b71c","year":2018},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.555220Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:e0c26147621f36e57e40eebd7089ba8ac5c773a35426d0f5c1168733ec7657ee","observation_id":"830c7d46-0fc6-4a99-ba7c-31c1ef3b8cd3","resolution":{"observed_at":"2026-08-11T17:09:58.698134Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.678592Z","title":"Feroci et al","venue":null,"work_id":"3004639e-6d19-4960-8198-3e6fc2972b76","year":2012},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.560250Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:9a76cd85fb7cdab57219ecc9c67016af4a045870c6459e79b19ea2e0cda1803f","observation_id":"5f5bc63e-c3c6-4410-a018-70b3f9117ced","resolution":{"observed_at":"2026-08-11T17:09:58.683213Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.664051Z","title":"Darabi, H","venue":null,"work_id":"acbf3adf-72ff-4759-b14e-eeaf922d1043","year":2018},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.565197Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:37ed2afefb92d11c4c3856555a8db2ae6065b65a33a4c1345799a557f1d3bec4","observation_id":"77ffe712-f1a8-41e4-a069-11bbf90b40c2","resolution":{"observed_at":"2026-08-11T17:09:58.668798Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.648532Z","title":null,"venue":null,"work_id":"0406347d-25b0-4550-918d-b6f568a67a78","year":2015},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.570148Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:8228a525a8bcf7c2deef387d75c7214527d46fb6ff240df0a42f9bac293b44e6","observation_id":"3c84f827-d456-43c3-bcb0-b1269eb22023","resolution":{"observed_at":"2026-08-11T17:09:58.653491Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.634186Z","title":"Heydarzade, H","venue":null,"work_id":"f59971b6-87d2-48d3-b36b-5dd021d3b392","year":2017},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.574540Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:6d58629bfb948edf069aa2d2b5e51bd4af16989b3706ce47638d2377c4acd910","observation_id":"26002485-d479-4867-b9fb-334291d39bdb","resolution":{"observed_at":"2026-08-11T17:09:58.638768Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.619229Z","title":null,"venue":null,"work_id":"a90ad0b9-7ed1-4eaa-a004-c59f2df7d4bf","year":2012},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.579830Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:e3c39e1e0e2f5bd152fafe77df2e30a9e1e5bf73acccc9c08b037f3814be65ab","observation_id":"4548f313-e58a-41be-be58-4fa33ae4124f","resolution":{"observed_at":"2026-08-11T17:09:58.624079Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.604465Z","title":"¨Ovg ¨un, ˙I","venue":null,"work_id":"398b9bb3-2448-45f7-9916-fd1512c6ed2f","year":2020},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.584529Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:5757c963fc7b56b22a97893051084431fb58f2d9bae55611738b0aa5dd928c43","observation_id":"79bf9b67-02cf-4707-b4a0-65df2726012f","resolution":{"observed_at":"2026-08-11T17:09:58.609146Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.588392Z","title":null,"venue":null,"work_id":"5918a32b-c365-434a-931e-080bf0a88506","year":2019},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.589304Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:6e07a767c625ab473542f7524419dc494ffee0b27313b1225283cdd28a28f001","observation_id":"c957295c-65f8-4a67-8393-13c932ae8de4","resolution":{"observed_at":"2026-08-11T17:09:58.593791Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.573947Z","title":"Annala, C","venue":null,"work_id":"0163860f-f649-4625-8e50-b13e05c92438","year":2018},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.594643Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:919af7ea83763a9c95efe189784379a2732aaec6e18794f4c7bc91b01e26df61","observation_id":"2a3a4ab5-23e4-456a-a8f5-52f3633683e1","resolution":{"observed_at":"2026-08-11T17:09:58.578664Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.559124Z","title":"Kurkela, E","venue":null,"work_id":"7be6bd17-f7a0-4280-a375-050235c62b49","year":2014},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.599617Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:2cab9920c2fadb44c42b4e422837f3a2f6e0bf4ac7dd1fc9033cb6e833758371","observation_id":"80910270-c9f1-4767-91e7-2c22da2b8d7e","resolution":{"observed_at":"2026-08-11T17:09:58.563735Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.543786Z","title":"Mariani, M","venue":null,"work_id":"a8d1a755-3449-4334-93a9-296382f59c9a","year":2019},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.604307Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:f300ef0dacc5279a7185c0c03254465398875d09a886ce3135318a192721ade1","observation_id":"731c2880-aeb1-404f-836c-3baeae513ee9","resolution":{"observed_at":"2026-08-11T17:09:58.548629Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.528462Z","title":"Freedman and L","venue":null,"work_id":"74943951-2880-49f5-a75b-ae27e354fc59","year":1978},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.608969Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:ffc6d1d38a52154260f4a3e48589698a38c85d6a0e0bc12bc6d023d5e83ebad2","observation_id":"31f931df-08bd-4e96-9002-02c01e81532f","resolution":{"observed_at":"2026-08-11T17:09:58.533582Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.511913Z","title":"Hasenfratz and J","venue":null,"work_id":"4e898af9-beea-47a6-92e9-9ff90ab1e7bd","year":1978},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.613193Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:23b192a1859777b72dc244f5088545fd54715128b7b9144a4256194968aae553","observation_id":"ee755d11-7a5c-42fd-9331-6ff1520808e2","resolution":{"observed_at":"2026-08-11T17:09:58.517218Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.495731Z","title":"Baym and S","venue":null,"work_id":"e16b06fc-368e-4ad7-9b81-2e35d87f7fc5","year":1976},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.617597Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:d256d677d1ab2049ca91af3d70d6775efdf11b33d29c5ac8fcea8cb19967aa25","observation_id":"f57af858-1352-4267-a8bf-ab2fb4f6ac47","resolution":{"observed_at":"2026-08-11T17:09:58.501293Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.481032Z","title":"Reya, Phys","venue":null,"work_id":"639f7a9e-a534-44ce-9cfd-ad2218d2dee9","year":1981},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.622182Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:382514f66431cdf7ff38df06c91ed2b30bdb3a75eefa4ef819a6dc396b07381b","observation_id":"c3789314-f42f-47a5-a9e2-203997930777","resolution":{"observed_at":"2026-08-11T17:09:58.485511Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.465343Z","title":"Gross, E","venue":null,"work_id":"73cffbde-e379-4cfb-90bf-f185d1e1e0d4","year":2023},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.626940Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:6f7076839dbdb89e115ef897504266ed6c15b28aec38d664229bfbef4b32417c","observation_id":"774f7b29-45e0-41d3-a589-d9244593b8ce","resolution":{"observed_at":"2026-08-11T17:09:58.470424Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.450380Z","title":"Buballa, Phys","venue":null,"work_id":"a25c596f-c792-4b3b-9384-27965e82f11f","year":2005},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.631500Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:10219edd027101a15a62af14644c3a9481535255690aa697b4359fe8d49ab770","observation_id":"9ec0d7f0-46f5-4359-8c31-c763d0c91ab2","resolution":{"observed_at":"2026-08-11T17:09:58.455151Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:57.635853Z","title":null,"venue":null,"work_id":null,"year":1975},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.635853Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:95f09b6589cd7986d8a4eecce008f81e3c8a30d9ba3422687126c3b8485ebd46","observation_id":"87c4b108-1db1-4ccf-a666-a3e39b7a2894","resolution":{"observed_at":"2026-08-11T17:09:57.635853Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.423388Z","title":"Annala, T","venue":null,"work_id":"f74e6c3c-fac7-4753-9963-e6690dedba47","year":2020},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.640238Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:c3d70f20aa969daaa046b731f16075abbd3366f44ae1aa7280fb83c1dff861bd","observation_id":"992ea619-840b-4a0a-a989-57a056b62d8a","resolution":{"observed_at":"2026-08-11T17:09:58.428357Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.406205Z","title":"Weissenborn, I","venue":null,"work_id":"de72c7ac-1304-45f1-b056-dbd6a978f22a","year":2011},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.645471Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:22e04c212a9a804428915553b9d0abf9191fbe32f8c599147e03184f75af55f2","observation_id":"8debb9aa-20e9-4862-82bf-6bb74d741e3a","resolution":{"observed_at":"2026-08-11T17:09:58.411147Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.388109Z","title":null,"venue":null,"work_id":"7742e8cb-eeba-4045-a478-5b225a878d43","year":2021},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.650607Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:ca9bc3e9e6b5f019c14d12f05274597c185a96732ea2ee9bae70963d98af06c9","observation_id":"bb4be0e2-8c48-4550-bde8-ea7452758460","resolution":{"observed_at":"2026-08-11T17:09:58.393548Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.371247Z","title":"McLerran and R","venue":null,"work_id":"b88457db-bd53-41e7-a7c7-7ec4a78c2958","year":2007},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.655393Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:9f027f1e09a0c775545b5a161f537696d880a7a1e79df689affc22dbca965ff9","observation_id":"8cd9ee5a-b2cb-44d8-89d5-521506251fbd","resolution":{"observed_at":"2026-08-11T17:09:58.376230Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.355583Z","title":null,"venue":null,"work_id":"0aeb6057-670e-4606-9db0-29e16be77702","year":2023},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.659946Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:4069769da5b719dca06bf62e9520a14766128b8aca1edff78d0182dc8fb20375","observation_id":"167f68e0-2222-4d29-9c5e-b8009f7d5cad","resolution":{"observed_at":"2026-08-11T17:09:58.360371Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.337620Z","title":null,"venue":null,"work_id":"dc158e51-a6f1-428c-bfec-15fa9d192514","year":2024},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.664229Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:58c88f407ebbc56226d027cb02409d04b3b5e3fa2e8a16ec79f9e94c6eebde0c","observation_id":"11ee75b4-f0dd-42f4-9115-3a73437783dd","resolution":{"observed_at":"2026-08-11T17:09:58.343635Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.316932Z","title":"Shankaranarayanan and J","venue":null,"work_id":"0ed370de-aae0-46f4-95e1-89d25dd7b613","year":2022},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.668456Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:45bc023e360a2fbe2c05a9e46d332696dab93d37dbeb2bd266ab90aa1b608b1f","observation_id":"2ea5ef20-ffeb-461c-99d3-933dcb438b5b","resolution":{"observed_at":"2026-08-11T17:09:58.322547Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.299399Z","title":null,"venue":null,"work_id":"7a9653c7-e489-4099-a356-cba817389fb4","year":2017},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.672664Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:87b355c30dd55cb0a3cb0d091f26931ea7dcf25f5f4d6750a8e7333cf646a7cc","observation_id":"f5c7163a-d7ca-4b2d-9f33-58bd2399d3e3","resolution":{"observed_at":"2026-08-11T17:09:58.305454Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.265706Z","title":"Cardoso and P","venue":null,"work_id":"53e02db8-cbf0-4f29-af1e-c2cd3b520039","year":2019},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.681227Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:761d3222cecc5154c8ecf2fc0ba57c8daca11681c9f8652625725f913aaf8ca4","observation_id":"e148f281-d3f4-4e63-9f36-d05a8a980e16","resolution":{"observed_at":"2026-08-11T17:09:58.270383Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.246475Z","title":"Baiotti and L","venue":null,"work_id":"fca2cc70-5eee-4c51-a95c-f06bdaf940d6","year":2017},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.685944Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:20a714540a354b30905258754262377094a7f6a8cd00aac359ef8ed7a73da8f7","observation_id":"42593cdb-9c54-4c04-b004-d290c56acb61","resolution":{"observed_at":"2026-08-11T17:09:58.254158Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:57.690345Z","title":"Sakalli and S","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.690345Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:5f99456a547c923712adfb81e2e85f01974e669e2bc185f9b626fb40f3fa80d1","observation_id":"bff0702d-63bd-40df-b940-40ddd90874ec","resolution":{"observed_at":"2026-08-11T17:09:57.690345Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.215585Z","title":null,"venue":null,"work_id":"348f73a1-4bdd-48e8-9af4-a84f860e4e06","year":2024},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.694619Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:22e4672f615385cd5cd5bea574fb5903aec1053a10c5f8e52a6aba4bd3f8f99a","observation_id":"cd4a7c5b-3517-4c61-a546-be2037180a36","resolution":{"observed_at":"2026-08-11T17:09:58.221462Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.197360Z","title":"Wu and C","venue":null,"work_id":"613a53d5-5b48-494f-a5ba-ea24091c030e","year":2020},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.699308Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:66d7517bd328305f6a75f22b62d156555935d4a6b33a667e3bf7bbb38d9bd7a6","observation_id":"c09af6e3-bcd1-4a44-a0f1-527e7fcde61c","resolution":{"observed_at":"2026-08-11T17:09:58.203941Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.180238Z","title":null,"venue":null,"work_id":"c532d937-03fd-40f9-b0e3-b5b11de3aa49","year":2022},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.703729Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:552eebd23daaaad93c4bda43a16bbcc9c909645341cca599bc1c6a964749715a","observation_id":"79c689df-c2b2-4b49-97ba-fa60b4109a67","resolution":{"observed_at":"2026-08-11T17:09:58.185969Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.164731Z","title":null,"venue":null,"work_id":"69e26acc-c8c6-4a2d-b352-a32f0615c45e","year":2023},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.708194Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:8f8ebab1443bc4fd785e99aaa750b4f13afcda8b906ef47f7180c89505e3088a","observation_id":"74844d19-6598-4ef5-8216-71e5e2cfe6eb","resolution":{"observed_at":"2026-08-11T17:09:58.169676Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.01970","last_updated":"2024-12-01T14:01:51Z","snapshot_observed_at":"2026-08-16T14:04:17.505741Z","submitted_at":"2024-04-02T14:14:04Z","title":"Anisotropic quark stars in $f(R,L_m,T)$ gravity","version":3},"cited_work":{"arxiv_id":"2404.01970","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.01970","snapshot_observed_at":"2026-08-11T17:09:57.831646Z","title":"Anisotropic quark stars in $f(R,L_m,T)$ gravity","venue":"gr-qc","work_id":"c82b920d-0698-4a7b-83d9-f4bdf63c8f69","year":2024},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.713088Z"},"links":{"cited_paper":"/paper/2404.01970","citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:77ddbf1196b57957f0ddffcd6419c7a59b2d216749b1048c7224beea29d9ec28","observation_id":"9d3780c6-3ee0-4a64-b340-02bd60de67fe","resolution":{"observed_at":"2026-08-11T17:09:57.838775Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:57.723183Z","title":"Zhang and R","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.723183Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:80a36e11f8017f3a5874d82fc5074e2f7912ab74b1c8772226358662ec8e1241","observation_id":"0f2bcc04-9939-49d9-a3d7-5a421ee8ab81","resolution":{"observed_at":"2026-08-11T17:09:57.723183Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.122591Z","title":"Zhang, Phys","venue":null,"work_id":"9b342f5c-a075-41f4-87ef-b42306b4fb68","year":2021},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.727781Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:ee638f7f755df40ba79236a11873c569f95609bb8cb65e4f56b31800cb083041","observation_id":"f25aafad-6cc9-410b-8ba5-b31c62ad0a9f","resolution":{"observed_at":"2026-08-11T17:09:58.127800Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.106661Z","title":"Rastall, Phys","venue":null,"work_id":"914b1c00-2bc5-4942-af55-e39d422075ff","year":1972},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.732136Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:b2218a9ef74ca32570eab10ac7336614a28e0adc08aecc018077ab7ddcd38d8f","observation_id":"5d575792-a8b4-4597-be00-09ca8b361079","resolution":{"observed_at":"2026-08-11T17:09:58.111362Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.091147Z","title":"Rastall, Can","venue":null,"work_id":"f3495b5d-7ea1-4132-abd2-09f43e546029","year":1976},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.736688Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:a55f9ec3900f681ff19180308a9a6ffa9608d1bba001ec66ca4364bab4d4bf14","observation_id":"b9fa37ca-3141-4602-8ece-76527394470a","resolution":{"observed_at":"2026-08-11T17:09:58.095856Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.076473Z","title":"Velten, A","venue":null,"work_id":"9a34e256-26fd-4650-ba57-01e3ad5fff63","year":2016},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.740942Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:caf271675485f2535b114c36214378508ce7b1296849b6c1418e024bd479f478","observation_id":"620202f6-ce2b-4ad4-8862-25febaa83f9c","resolution":{"observed_at":"2026-08-11T17:09:58.081024Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.062056Z","title":"Maulana, and A","venue":null,"work_id":"37aa74fa-c838-488b-99ae-0c0df1cf14e1","year":2019},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.745032Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:5455271385d4a45f32103418132f38290663d37a655ed379bb64540362d48414","observation_id":"5488dacb-fa77-4fc1-8641-a2917788d9a6","resolution":{"observed_at":"2026-08-11T17:09:58.066442Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.281620Z","title":"Antoniadis, P","venue":null,"work_id":"c2f16a28-d884-449b-b79d-ea2d6c3ffcd2","year":2013},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.749143Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:9e88b45c6a21615e4552068b17e4bda3d7a1ad2408a4187b97bcb99f13682c12","observation_id":"f49ed337-e92c-44b5-839a-82ac2b9c0191","resolution":{"observed_at":"2026-08-11T17:09:58.287177Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.046934Z","title":"Fonseca, H","venue":null,"work_id":"e3e8dd02-2118-4e90-8207-948c60866c5a","year":2021},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.753332Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:80136608fee4e24a1ebaaecca3e07a00331b2810f5387cc5c3a4cb71b2951532","observation_id":"426918a2-9461-485e-b53a-02eadf3e335c","resolution":{"observed_at":"2026-08-11T17:09:58.051820Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.029172Z","title":null,"venue":null,"work_id":"388f6cd8-4c41-4629-8b4c-13938238be04","year":2022},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.757641Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:e92f62d5d6a7978f59b199d7ebf70a37e7683e0df0276580f641cc3394173d6c","observation_id":"ceac4efb-2045-4bf8-ad9a-8c85d783fe32","resolution":{"observed_at":"2026-08-11T17:09:58.035368Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.013439Z","title":"Abbott et al","venue":null,"work_id":"5ceb40df-e2b3-4c12-a047-88be55a7b6a7","year":2020},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.761927Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:39cd7ad878763e60ee1272393db7bb079e61f4347b8d2be2f7d01b6864fde1a9","observation_id":"288a6e04-7343-400f-8293-6940183eb64b","resolution":{"observed_at":"2026-08-11T17:09:58.018738Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:58.149546Z","title":"Maulana and A","venue":null,"work_id":"4327521a-bd36-49d3-b254-daa6d43deb3f","year":2019},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.766230Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:47bcca3a832e6526f9c5a612cd2731527835c65cb18babc2b45bf103559154c4","observation_id":"1873d1a1-8c58-407e-999f-0109df29a7b2","resolution":{"observed_at":"2026-08-11T17:09:58.154205Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:57.997498Z","title":null,"venue":null,"work_id":"aed39903-5837-40b4-afc6-04772b4a9112","year":2006},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.771059Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:bfce1a8d2f67778694aec125d7395a41a7ddda0206a0c4a4dd949053884ff510","observation_id":"52cea8b1-84f3-4461-aa0a-bd316ff96606","resolution":{"observed_at":"2026-08-11T17:09:58.002433Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:57.982209Z","title":null,"venue":null,"work_id":"1b75d210-ca6c-4415-b805-67579baf9802","year":1965},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.775274Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:0856d1edb0678902fcc219f953ad0afe782431c9779e8c285204850e45c939ef","observation_id":"f002e768-bbd3-4f90-979b-89f437738126","resolution":{"observed_at":"2026-08-11T17:09:57.987026Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:57.967409Z","title":null,"venue":null,"work_id":"ef899994-6a00-4565-adc9-f31777d695bf","year":1971},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.780257Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:5156e59d0358ba5f939ba33265dfa0bddfa6e070e194dadfc594b35e16691dc7","observation_id":"a8a7897b-6a43-4180-9c07-91ae8b220470","resolution":{"observed_at":"2026-08-11T17:09:57.972174Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:57.785035Z","title":"Chandrasekhar, Astrophys","venue":null,"work_id":null,"year":1964},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.785035Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:1368e120387c6d1abbe2a3ff3572981cfe664dbc3cabc14b8f5bfabfd2a7c7d8","observation_id":"25232a8a-a53c-46ee-8c31-9c837caa3435","resolution":{"observed_at":"2026-08-11T17:09:57.785035Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:57.942313Z","title":null,"venue":null,"work_id":"17833ca5-b004-4c3f-9b93-cd8a186fe634","year":1983},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.789240Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:6716ffbeabbbdf474468f071e33d4cb150ef55150a815afdbeebd2a9973ee7ed","observation_id":"e41db332-690f-4941-9dfe-bf7bc5a86ad2","resolution":{"observed_at":"2026-08-11T17:09:57.947069Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T17:09:57.926074Z","title":null,"venue":null,"work_id":"eed368a7-47ff-4484-a17a-7f248bb6a7ef","year":2017},"citing_paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-11T17:09:57.793407Z"},"links":{"citing_paper":"/paper/2412.09306"},"observation_digest":"sha256:39cd7ef7864e447c0de8cf1486b23aee15881f623e96e77775a78804387bf121","observation_id":"3ce19783-68e7-4e4c-9fc2-1d24b2a947c6","resolution":{"observed_at":"2026-08-11T17:09:57.930749Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2412.09306","last_updated":"2024-12-12T14:23:28Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-16T08:19:37.013193Z","submitted_at":"2024-12-12T14:23:28Z","title":"Properties of interacting quark star in light of Rastall gravity"},"reference_resolution":{"displayed":63,"state_counts":{"malformed_identifier":2,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":26,"verified_exact":3,"verified_fuzzy":32},"total_outbound_references":63},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 17 August 2026, this Paper Citation Record lists 63 of 63 outbound references and 0 inbound Pith citation observations for arXiv:2412.09306."}