{"as_of":"2026-08-13T09:27:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:1627302a17f936d3fd703c7f032afae2fcb7a3a411a6cdff5bda2e34494d84c7","coverage":[{"denominator":42,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":42,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T17:25:03.244943Z","state":"measured"},{"denominator":44,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":44,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-13T06:32:02.005865+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T22:21:35.112001Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"arxiv_reference","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":0,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.12629","snapshot_observed_at":"2026-08-11T22:21:35.112001Z","title":"Garuda, J","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.03547","last_updated":"2025-09-09T12:55:02Z","snapshot_observed_at":"2026-08-12T15:55:20.553754Z","submitted_at":"2024-12-04T18:45:30Z","title":"Learning from galactic rotation curves: a neural network approach","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-11T22:21:35.112001Z"},"links":{"cited_paper":"/paper/2411.12629","citing_paper":"/paper/2412.03547"},"observation_digest":"sha256:2d22fb1f8c179b197ab5918a650da2a9a8a5e1b00a38e9d571478edf5109135a","observation_id":"8885b588-3006-4432-b5e7-40608d9afc28","resolution":{"observed_at":"2026-08-11T22:21:35.112001Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"cited_work":{"arxiv_id":"2411.12629","doi":"10.48550/arxiv.2411.12629","metadata_source":"arxiv_reference","pith_arxiv_id":"2411.12629","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"arXiv (Cornell University)","work_id":"f8dc8686-4398-4d30-8764-4f023faee433","year":null},"citing_paper":{"arxiv_id":"2606.12938","last_updated":"2026-06-11T06:02:29Z","snapshot_observed_at":"2026-07-06T23:51:45.306189Z","submitted_at":"2026-06-11T06:02:29Z","title":"Cluster Mass Inference from Galaxy Kinematics","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-06-27T06:16:37.393826Z"},"links":{"cited_paper":"/paper/2411.12629","citing_paper":"/paper/2606.12938"},"observation_digest":"sha256:b3c8eb6ace02059a9adb1a8e56a6d384ebcab36d1ecd30323de33f4c6f7eb13d","observation_id":"92a6b3cf-576c-4bd9-8f18-3c0170dbf641","resolution":{"observed_at":"2026-06-27T07:30:41.906832Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2411.12629/citation-record","integrity":"/paper/2411.12629/integrity","json":"/paper/2411.12629/citation-record.json","paper":"/paper/2411.12629"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T17:25:03.967308Z","title":"Painting galaxies into dark matter haloes using machine learning","venue":null,"work_id":"6df83bab-29c5-41a4-9854-7fb4a6354194","year":2018},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.038950Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:4477c0a6792e2310212cd49a1692555982995b8edc749961ce4550d9a2b85a81","observation_id":"2fc9d975-5061-44b8-819d-0fd4d5c2b54b","resolution":{"observed_at":"2026-08-12T17:25:03.972672Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.950593Z","title":"The Sunyaev–Zel’dovich effect","venue":null,"work_id":"a51c502e-327b-4319-adcb-5b51ce84a32f","year":1999},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.044433Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:ed6755f591d9fce6099b6d91333717ed788dee814c9f36324a77aa7278032904","observation_id":"9e925d27-f367-4fd0-8b9b-95640a1ea7ee","resolution":{"observed_at":"2026-08-12T17:25:03.956385Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.932768Z","title":null,"venue":null,"work_id":"543a199f-71dc-4ee3-8ca7-753bc8086cb7","year":2015},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.049915Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:4d62932955f69c269b90bab9f2a25e963cf1d9fbf4017ac3fdd048108272f0f4","observation_id":"9278c98e-b0c9-4eef-bae9-2a86690fda10","resolution":{"observed_at":"2026-08-12T17:25:03.937895Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.916764Z","title":"Bullock and Michael Boylan-Kolchin","venue":null,"work_id":"1c70f4fb-fbbc-4ed1-a08f-f5a08a4d2c51","year":2017},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.054910Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:1a8172a2f153de6245875904ad8fbd847417d5de1cd197dcd844766dbe4f9c89","observation_id":"2058dbc6-d832-466d-bc35-60d62d4b90ac","resolution":{"observed_at":"2026-08-12T17:25:03.921714Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.900179Z","title":null,"venue":null,"work_id":"d349c3a1-d514-45ff-9c6c-10b26ce2c540","year":2023},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.059877Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:23ee2a8d1147961dc3c3d87a446b182a30c745dd051d650bbbb36f3eaee6b3f3","observation_id":"4b893934-8cac-4781-9f26-883bce9fdb8c","resolution":{"observed_at":"2026-08-12T17:25:03.905773Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.883868Z","title":"Cluster- GCN: An Efficient Algorithm for Training Deep and Large Graph Convolutional Networks","venue":null,"work_id":"0ac4fb2b-01f4-4281-a6fa-aa78a216716d","year":2019},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.066191Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:22bd8147f48072befee096b7f695b7a3266e662cb2aadd7f3e85ad203758c418","observation_id":"2acbb200-39f9-4490-9eba-add1865c9ec5","resolution":{"observed_at":"2026-08-12T17:25:03.889225Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.868685Z","title":"´Ciprijanovi´c, D","venue":null,"work_id":"5ece7dd6-700b-46d4-985f-7c3741af6248","year":2021},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.072376Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:e878e1eeb9b24518213f92d881191265c8b22ec1639ffd01228c1b9d470b7635","observation_id":"1be582d8-baf7-4e69-936d-e747c31d475c","resolution":{"observed_at":"2026-08-12T17:25:03.873599Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.852165Z","title":"Gonzalez, Maxim Markevitch, Scott W","venue":null,"work_id":"a1fd0a18-a8ce-42b4-9fd3-e4ceae8cce95","year":2006},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.077070Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:86bc7f462a62da17f463cd9ed3e82c9345ab6e7880043003d03b2a6a67c310c8","observation_id":"ad62d8e0-1691-4880-acfa-441a7a364ddf","resolution":{"observed_at":"2026-08-12T17:25:03.857269Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.836256Z","title":"Large Synoptic Survey Telescope: Dark Energy Science Collaboration, November 2012","venue":null,"work_id":"09ac0b78-918e-4948-9b6b-0ced5ec4e3e0","year":2012},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.081675Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:70c93024c46d9f7cfff65cc0b6381bb72b36659d58eea5f14919838da0f8fbb7","observation_id":"c04b0268-79e6-4768-a226-cde48569f529","resolution":{"observed_at":"2026-08-12T17:25:03.841419Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.820135Z","title":"Discovering Symbolic Models from Deep Learning with Inductive Biases, 2020","venue":null,"work_id":"dccc4bd2-21fd-4f77-ad54-8496a9f26f6f","year":2020},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.086202Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:263cd494a3ed683939c9ef1bed4a6d8c9648c50f56906c058dbae10c6afd742a","observation_id":"2e8bc97e-14d8-452e-b08b-afb15153e31d","resolution":{"observed_at":"2026-08-12T17:25:03.825193Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.802887Z","title":"Fast Graph Representation Learning with PyTorch Geomet- ric, 2019","venue":null,"work_id":"d8541f05-31b8-4b72-8990-253fcbaadcb0","year":2019},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.090800Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:08a9ec5f5027f5cc674e6c1543e8d90ce3778b978ae05c657dc363ef81ad072a","observation_id":"da75136d-53e2-43df-8d7e-c356cdb0c657","resolution":{"observed_at":"2026-08-12T17:25:03.808690Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.786950Z","title":"Gaussian Error Linear Units (GELUs), 2016","venue":null,"work_id":"b6750e0a-375b-4e1a-96d6-703dd2ce7351","year":2016},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.095319Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:a006c1e4d0e25ec6f48fca6f2f499e0e0cf66cbb1f2e27f574599f0a7ea5d5f7","observation_id":"5664f005-f41c-4a80-86c0-be080492e155","resolution":{"observed_at":"2026-08-12T17:25:03.791799Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.770345Z","title":"Benchmarks and explanations for deep learning estimates of X-ray galaxy cluster masses","venue":null,"work_id":"be7d3d65-e994-4652-9014-1eb708683ccd","year":2023},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.100466Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:19a235c56f3ab21d7f7c3e5cb1174cf53a58fe3afc46bc4986c73a6960e0ed51","observation_id":"fb5e1074-4458-475b-b2d1-d92c0861d6b2","resolution":{"observed_at":"2026-08-12T17:25:03.775708Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.752783Z","title":"Random decision forests","venue":null,"work_id":"6fc46c3b-5099-4f4b-bb23-2b6fa94432e7","year":1995},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.105274Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:29bd83fd30355c6d0d29776ca5cce4f4405d0f3a07ab6d28e3feb1d60628a8ac","observation_id":"19e4a15c-077d-4b1e-8cd3-f6c783e2af65","resolution":{"observed_at":"2026-08-12T17:25:03.758217Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.734892Z","title":null,"venue":null,"work_id":"f8b913e8-9159-40b4-8d24-308c55b831d5","year":2020},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.110378Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:5b2b40c2f51794a97c57bbc2fd6aa6cb6b1e5404c53a70d63aa6fd23cba3be9b","observation_id":"da8b40b5-82ab-411b-a28e-7bc52b7fe062","resolution":{"observed_at":"2026-08-12T17:25:03.740335Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.718039Z","title":"Kamdar, Matthew J","venue":null,"work_id":"509f1b00-9a52-4eeb-8892-532689fbf545","year":2016},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.115239Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:9cd432810b4953d6681fd919dfce896cbad84edff82f26d398dbac2489eafce2","observation_id":"964fa108-7cfd-47ba-a760-54fe63e48c75","resolution":{"observed_at":"2026-08-12T17:25:03.723187Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.702411Z","title":"Kouw and Marco Loog","venue":null,"work_id":"0443d409-64cb-4569-bab9-c8fb22d6abef","year":2019},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.120256Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:09d99b23711fb1747fe2977480542503a25b937b54e9c6c9e9e9f0c2f526c5b3","observation_id":"16d1d3c9-bc65-4481-8e25-613c13379741","resolution":{"observed_at":"2026-08-12T17:25:03.707220Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.687109Z","title":"Larson, John F","venue":null,"work_id":"098d5ca3-07de-4965-b1e6-5584aff7ae0f","year":2024},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.125146Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:8bb00ad61717bcbc90d3ccf566175ac079134f01f6eadbbffa668a8acb7b3c9c","observation_id":"0ecc6e17-c30b-46b5-b065-ba50a6b09263","resolution":{"observed_at":"2026-08-12T17:25:03.691775Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.129913Z","title":"Decoupled Weight Decay Regularization, January 2019","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.129913Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:9d95d213028367b93c9c57cd21d087c7a3cf1f003fe0655578f3b95ab905a1c0","observation_id":"1ffac219-e325-4699-8dd7-6b2f5e41ae98","resolution":{"observed_at":"2026-08-12T17:25:03.129913Z","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":"2026-08-12T17:25:03.661091Z","title":null,"venue":null,"work_id":"c9da4596-c2cb-4d33-b3d8-3067a80b9e53","year":2017},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.135141Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:cd13e7d61bc6d9686351fb095615838019dd6622ba1e533b0b42785f5d34dd7f","observation_id":"fa9ae16d-4b94-4f97-8ee1-80b42aeb2bd8","resolution":{"observed_at":"2026-08-12T17:25:03.665733Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.645040Z","title":"Lovell, Stephen M","venue":null,"work_id":"e76702ab-7a0e-4502-9796-509458fdf666","year":2022},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.140050Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:5e62c3f0e30a3ea85b10a4586631084b92a211402f1d2e47e20991aec1a71e39","observation_id":"4f4596e2-a208-4f02-893c-c6392b0e4f3d","resolution":{"observed_at":"2026-08-12T17:25:03.650250Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.625895Z","title":"Marriage, Viviana Acquaviva, Peter A","venue":null,"work_id":"96413bd2-b93f-4fb5-9769-feb2c648987a","year":2008},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.145018Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:0b09ca8d8ef565aefcaa9e8f8e2494e1b05f2ff86e6013b873d2391bc88ec80a","observation_id":"b7414e26-a6aa-4093-b2ef-be35c3981f55","resolution":{"observed_at":"2026-08-12T17:25:03.632008Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.608443Z","title":"GalaxyNet: Connecting galaxies and dark matter haloes with deep neural networks and reinforcement learning in large volumes","venue":null,"work_id":"0cbb4a6c-8c84-41d6-99d8-4a85011ef82b","year":2021},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.149821Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:9548dc2be0b2768182ea45039fd44fb6e0e20b2395dc0328411a793e22cf9a73","observation_id":"6324fc67-c41c-4ed2-aa0e-4aff9319ed1b","resolution":{"observed_at":"2026-08-12T17:25:03.613889Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.591307Z","title":"Introducing the TNG-Cluster simulation: Overview and the physical properties of the gaseous intracluster medium","venue":null,"work_id":"f9e87d4c-a43b-4299-8476-79f3601064d8","year":2024},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.154678Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:f42e04552d1b3b1edce53d73639c4e2dc875975f0fdf58338988450e55f1e9ea","observation_id":"ed67a3e9-d1b9-4480-ba58-0313058f1302","resolution":{"observed_at":"2026-08-12T17:25:03.596617Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.575261Z","title":"The IllustrisTNG simulations: Public data release","venue":null,"work_id":"d357de0f-a522-447d-a223-3a89e2577b9f","year":2019},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.159322Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:bfa6ddf656e123c16bbe66c765d39d65c5ed8f7c3f15a5213b2c9cc14b524d68","observation_id":"09052eb4-cd4c-4485-ab07-f9c1c46a467e","resolution":{"observed_at":"2026-08-12T17:25:03.580180Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.559598Z","title":"Ntampaka, J","venue":null,"work_id":"c73319d7-53fa-4fe3-96dc-50074a3a17ba","year":2019},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.164114Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:c195b02f68f70c0f9978b60adf4cf591efb11789de8845976085a74a86228a32","observation_id":"132df8bb-1674-482c-a0e1-5216bc21ebb2","resolution":{"observed_at":"2026-08-12T17:25:03.564578Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.541426Z","title":"Scikit-learn: Machine Learning in Python","venue":null,"work_id":"816424ec-34ec-4ee5-8a18-a5f381ed5767","year":2011},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.168935Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:8cb1b47723b2712ac45f4fe9de11ce814a2c48459f8d4a01ec2b0d88e3e33f51","observation_id":"97201b74-856c-463e-ab50-d3dd11a3e43e","resolution":{"observed_at":"2026-08-12T17:25:03.547941Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.524753Z","title":null,"venue":null,"work_id":"3c509bd2-c290-417b-bf67-c510afedfe57","year":1984},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.173942Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:bfbb37dea02cdbd839bca6dd042a37288b60e132c7b2ecf763511748fe46ab69","observation_id":"d1092f1c-e511-4c52-ab5c-01b51a6555c8","resolution":{"observed_at":"2026-08-12T17:25:03.529971Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.508585Z","title":null,"venue":null,"work_id":"e65e1730-5bbb-4bb3-b7ee-3c66e0638a68","year":2015},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.178517Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:c040f2498a8134f77e6dc54658edb2874ea179dbb870d650eb0cccd5d305676e","observation_id":"8587e2da-cf5d-498c-aa65-4399a828fc4f","resolution":{"observed_at":"2026-08-12T17:25:03.513827Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.491731Z","title":null,"venue":null,"work_id":"63842454-1f04-491b-b2ca-c55148119b0b","year":2014},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.183747Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:008689a8df3e5bf959feb0b6071d70d34c860bae8f882f3546e0844b85e78489","observation_id":"bf9e36b4-6687-4e6d-a77f-07e57680a5ae","resolution":{"observed_at":"2026-08-12T17:25:03.496607Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.476802Z","title":"Sampaio-Santos, Y","venue":null,"work_id":"eb01a05c-f129-4c5d-b49c-4f03f3b02d3a","year":2021},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.188473Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:892ae43e63d1078cbee3da2d85f8e5a767a6284a29b648994efd3c10107a96c7","observation_id":"dcceaeb1-32de-48dd-9020-6f303257109d","resolution":{"observed_at":"2026-08-12T17:25:03.481529Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.458968Z","title":"Scarselli, M","venue":null,"work_id":"08978b55-af30-42f2-b8e3-16c97b8de3ea","year":2009},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.193746Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:94d57ef10a927e60e18087dcfe956892bedecd36e507d260641d333a2a7ae758","observation_id":"d6d4d864-2119-4e47-9d33-3ec9788fd57f","resolution":{"observed_at":"2026-08-12T17:25:03.464481Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.441593Z","title":"Helly, Joey Braspenning, Willem Elbers, Ian G","venue":null,"work_id":"4813cd7e-f9f6-414b-bcaa-f87dc111b335","year":2023},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.198838Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:d02bcf0f71f7a9e2879356182a708c991aa9d8eb05d4e3d4dbad63edcfdc2303","observation_id":"78376602-37ef-4061-bb18-e0c020c345f8","resolution":{"observed_at":"2026-08-12T17:25:03.447162Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.425843Z","title":"Spergel, N","venue":null,"work_id":"81fb2b91-8954-474b-a7c1-7e13b5783b7b","year":2015},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.204140Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:1ef60257c2280dbaa97f2c06a56a83ad68aafad4da533312f791558758d2903f","observation_id":"86d8455b-9643-464b-975c-410fb64c8afe","resolution":{"observed_at":"2026-08-12T17:25:03.430694Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.408510Z","title":null,"venue":null,"work_id":"e85fd421-fccf-45d6-a137-3020b7873397","year":2001},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.209023Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:be9336d2b8aca5de7c150e12e4f7e2325377c8fea4c8235ae526b95c66398e2c","observation_id":"64051196-9c7a-47ae-90b1-724e8c4c71e2","resolution":{"observed_at":"2026-08-12T17:25:03.413518Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.391863Z","title":"Return of frustratingly easy domain adaptation","venue":null,"work_id":"5e4f1ccd-a003-4408-b3ca-ecbbda444896","year":2016},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.214279Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:6ca3cbd1e359acc855a0939ddd90d6c51705cd6873cf73288f85872109f92796","observation_id":"b83e0c64-d15d-4c50-acdc-ef42ee2b4bf0","resolution":{"observed_at":"2026-08-12T17:25:03.396781Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.375135Z","title":"Vegetti, S","venue":null,"work_id":"f5e6ab27-a5af-47fc-9cef-682d3fffa106","year":2024},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.219165Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:2729f159a257868760e35cda3e33a08ece4d6a1a0c0eeba373ce1898c58d9b79","observation_id":"27b7e06c-8b62-40c2-8b1e-5bc4adf7c426","resolution":{"observed_at":"2026-08-12T17:25:03.380351Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.357279Z","title":"Weaver, Sam E","venue":null,"work_id":"b3a8edad-b433-4c14-a6f7-cf1341ec5fc9","year":2024},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.224402Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:9d05bfb0b55d3614dae35406a55da805d6b5ec7f6bfa60b68b60d7f0addd22f1","observation_id":"37f58df1-1579-4693-9fed-0a1778eaf662","resolution":{"observed_at":"2026-08-12T17:25:03.362507Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.339468Z","title":"Wechsler and Jeremy L","venue":null,"work_id":"610ebed0-e177-47b7-ae75-83ac94f156a8","year":2018},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.229155Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:82cefa7bb1b635c5a9ae75bef3502aa16cad92b10aaf7364fd6ee9ed68f1b751","observation_id":"b020630d-82c3-485d-8d25-20359ed562b9","resolution":{"observed_at":"2026-08-12T17:25:03.344812Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.320904Z","title":"Wu and Christian Kragh Jespersen","venue":null,"work_id":"39c42340-3b3c-48c1-905d-bb158aee8b8e","year":2023},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.234235Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:8a0d49792d643d7a4776d723941cf441be9ea6f4e3dd9f73bb978bb1dfc6d12f","observation_id":"a4d7b4c1-bb24-45af-95a8-5f4436ece931","resolution":{"observed_at":"2026-08-12T17:25:03.327246Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.303214Z","title":"Wu, Christian Kragh Jespersen, and Risa H","venue":null,"work_id":"72a6bc04-5cab-445a-b8e3-d4a72b788206","year":2024},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.239260Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:9eb1aebb0538ee712038bd64c5d6d5b399b35383b8d55730909493e6d2fe8da7","observation_id":"f7679856-16a4-4250-a6da-010dbc5082f9","resolution":{"observed_at":"2026-08-12T17:25:03.308862Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T17:25:03.283371Z","title":"Galaxy cluster mass estimation with deep learning and hydrodynamical simulations","venue":null,"work_id":"609bc273-c273-46ad-b979-449e71abf231","year":2020},"citing_paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-12T17:25:03.244943Z"},"links":{"citing_paper":"/paper/2411.12629"},"observation_digest":"sha256:c1b563615152915098ad4e05fa41a17b8957cbcdcfdbc96f0666a284f473e23d","observation_id":"c8530d07-bba1-4972-a8b6-b1cce27c8b96","resolution":{"observed_at":"2026-08-12T17:25:03.290980Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2411.12629","last_updated":"2024-11-19T16:40:17Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-12T17:17:51.817500Z","submitted_at":"2024-11-19T16:40:17Z","title":"Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks"},"reference_resolution":{"displayed":42,"state_counts":{"malformed_identifier":1,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":9,"verified_exact":0,"verified_fuzzy":32},"total_outbound_references":42},"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":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 42 of 42 outbound references and 2 inbound Pith citation observations for arXiv:2411.12629."}