{"as_of":"2026-08-07T19:14:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a5599ba021327562162fd5ba1f099e7a8314a51c8f4a98bd8d7d849c23723c2d","coverage":[{"denominator":163,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T00:14:16.695826Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+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/2608.02730/citation-record","integrity":"/paper/2608.02730/integrity","json":"/paper/2608.02730/citation-record.json","paper":"/paper/2608.02730"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:04.796301Z","title":"Frontiers in Astronomy and Space Sciences , keywords =","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:04.796301Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:2e8a63fe7789fceaf70c448ccc5885b024a9ced16930e52cc8a94217ea045b6e","observation_id":"b62ae471-2732-4a7e-a708-ad681f6766a9","resolution":{"observed_at":"2026-08-07T00:14:04.796301Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1402.7073","last_updated":"2014-04-29T14:14:50Z","snapshot_observed_at":"2026-08-04T03:39:32.769738Z","submitted_at":"2014-02-27T21:00:01Z","title":"Cold dark matter haloes in the Planck era: evolution of structural parameters for Einasto and NFW profiles","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1402.7073","snapshot_observed_at":"2026-08-07T00:14:04.901531Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:04.901531Z"},"links":{"cited_paper":"/paper/1402.7073","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:8dee70c32fe700281616e3f701fdc28326096116bd3f98d2f55e95576927e120","observation_id":"b61316ef-e7a6-48c3-9b78-0f91b13a7743","resolution":{"observed_at":"2026-08-07T00:14:04.901531Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1712.05833","last_updated":"2018-07-17T09:24:11Z","snapshot_observed_at":"2026-07-06T06:14:38.280461Z","submitted_at":"2017-12-15T20:58:42Z","title":"The extended Planetary Nebula Spectrograph (ePN.S) early-type galaxy survey. The kinematic diversity of stellar halos and the relation between halo transition scale and stellar mass","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1712.05833","snapshot_observed_at":"2026-08-07T00:14:05.500531Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:05.500531Z"},"links":{"cited_paper":"/paper/1712.05833","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:669dd99609cd1770be2c5d1de989e28539d10f60d3ef6d426a77708e92824b05","observation_id":"8a4296a0-c7f2-4ec2-bc19-a47fea1d2851","resolution":{"observed_at":"2026-08-07T00:14:05.500531Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.4606","last_updated":"2011-11-20T05:01:44Z","snapshot_observed_at":"2026-08-02T02:50:47.625459Z","submitted_at":"2011-11-20T05:01:44Z","title":"The Carnegie-Irvine Galaxy Survey. II. Isophotal Analysis","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.4606","snapshot_observed_at":"2026-08-07T00:14:05.985712Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:05.985712Z"},"links":{"cited_paper":"/paper/1111.4606","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:9a2dc4817598c02a14f18e12c7cb183ad92eacf85135a102e137b07ada9f5644","observation_id":"26cd2a20-c213-475a-90cf-522f82717fd1","resolution":{"observed_at":"2026-08-07T00:14:05.985712Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0709.0585","last_updated":"2007-09-05T07:40:11Z","snapshot_observed_at":"2026-08-07T05:07:18.377330Z","submitted_at":"2007-09-05T07:40:11Z","title":"The Black Hole Mass and Extreme Orbital Structure in NGC1399","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0709.0585","snapshot_observed_at":"2026-08-07T00:14:06.110316Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:06.110316Z"},"links":{"cited_paper":"/paper/0709.0585","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:1d458ccd4717bff5be6e039085b73adfc904ec0c7472b8065666f5232e656244","observation_id":"26be34b4-eedb-4a05-9868-86429c652f33","resolution":{"observed_at":"2026-08-07T00:14:06.110316Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.12551","last_updated":"2018-07-17T14:59:15Z","snapshot_observed_at":"2026-07-06T06:42:18.699391Z","submitted_at":"2018-05-31T16:42:49Z","title":"The stellar population and initial mass function of NGC 1399 with MUSE","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.12551","snapshot_observed_at":"2026-08-07T00:14:06.255994Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:06.255994Z"},"links":{"cited_paper":"/paper/1805.12551","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:62ba21ab2610223998d0a876320d62df0175c4e61cf7cd49a97b018e8014f7b3","observation_id":"ce577ace-e570-473e-985d-d4fc15254e60","resolution":{"observed_at":"2026-08-07T00:14:06.255994Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.12338","last_updated":"2023-10-18T21:32:12Z","snapshot_observed_at":"2026-07-06T16:35:19.728025Z","submitted_at":"2023-10-18T21:32:12Z","title":"Total mass slopes and enclosed mass constrained by globular cluster system dynamics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.12338","snapshot_observed_at":"2026-08-07T00:14:06.357424Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:06.357424Z"},"links":{"cited_paper":"/paper/2310.12338","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:ac66467a6589626af009af74328c246c0d96c9bf571ac3de80ee9565611a0ae0","observation_id":"511c19bf-22bd-4e6e-8b5b-c632118d1d7a","resolution":{"observed_at":"2026-08-07T00:14:06.357424Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.13109","last_updated":"2024-03-19T19:15:59Z","snapshot_observed_at":"2026-08-04T16:32:23.042658Z","submitted_at":"2024-03-19T19:15:59Z","title":"Shapes of dark matter haloes with discrete globular cluster dynamics: The example of NGC 5128 (Centaurus A)","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.13109","snapshot_observed_at":"2026-08-07T00:14:06.490082Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:06.490082Z"},"links":{"cited_paper":"/paper/2403.13109","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:2fb8a7b508d14e9e44c62fdf5381472a8dba59f0efef247d424346c09fad03bd","observation_id":"3841da72-2771-43da-86d3-8bcf8256b044","resolution":{"observed_at":"2026-08-07T00:14:06.490082Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0901.1138","last_updated":"2009-01-08T21:20:40Z","snapshot_observed_at":"2026-07-06T01:49:41.701885Z","submitted_at":"2009-01-08T21:20:40Z","title":"The ACS Fornax Cluster Survey. V. Measurement and Recalibration of Surface Brightness Fluctuations and a Precise Value of the Fornax--Virgo Relative Distance","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0901.1138","snapshot_observed_at":"2026-08-07T00:14:06.651018Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:06.651018Z"},"links":{"cited_paper":"/paper/0901.1138","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:ebb071a78e3779276c7c29a8f80fa83622fa8862adb5210c4207bd3ef0b006c2","observation_id":"3c0bc2c6-e902-4136-9165-5b5eb69ae568","resolution":{"observed_at":"2026-08-07T00:14:06.651018Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:06.785502Z","title":"Soviet Astronomy Letters , year = 1979, month = jan, volume =","venue":null,"work_id":null,"year":1979},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:06.785502Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:2d10e9b5f7d779256d9ec0199d3521523f1b80aea074539ba5cf3ba370630a1b","observation_id":"d4a214db-0d87-4a42-9d1b-905587a70689","resolution":{"observed_at":"2026-08-07T00:14:06.785502Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:06.899602Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:06.899602Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:6981f8ceb361e28407a22ebf2abe1cab0aeb0e6808fc8860d4a99f8ea40bfe17","observation_id":"15630c21-aa0e-4c4c-9109-43f49cbfa425","resolution":{"observed_at":"2026-08-07T00:14:06.899602Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.03325","last_updated":"2015-04-13T20:00:46Z","snapshot_observed_at":"2026-07-06T04:14:53.101856Z","submitted_at":"2015-04-13T20:00:46Z","title":"The SLUGGS Survey: Multi-population dynamical modelling of the elliptical galaxy NGC 1407 from stars and globular clusters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.03325","snapshot_observed_at":"2026-08-07T00:14:07.040135Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:07.040135Z"},"links":{"cited_paper":"/paper/1504.03325","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:ddb917d0f896c72be78f561332a2fc4d5ca976db224904b0f72ae8e20f228af5","observation_id":"bc04732a-2ff6-4240-9c2e-e6f98493bb8c","resolution":{"observed_at":"2026-08-07T00:14:07.040135Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-08-07T00:14:07.180251Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:07.180251Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:7929e446ce28d87f00917b576b582ba428b42c8fc65498c7b81cda94974114d9","observation_id":"e0f49f31-1dda-4bd4-8ccb-791f3aa22e2b","resolution":{"observed_at":"2026-08-07T00:14:07.180251Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:07.506536Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:07.506536Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:91edbde56670d498ea9bd8693090d909fbafca5da9a255f0266704fec7e2a514","observation_id":"b19160dc-e3ef-471a-accb-fe0df7461a90","resolution":{"observed_at":"2026-08-07T00:14:07.506536Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0106005","last_updated":"2001-05-31T23:13:07Z","snapshot_observed_at":"2026-07-31T10:29:21.351082Z","submitted_at":"2001-05-31T23:13:07Z","title":"Dynamics of the Globular Cluster System Associated with M87 (NGC 4486). II. Analysis","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0106005","snapshot_observed_at":"2026-08-07T00:14:07.688476Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:07.688476Z"},"links":{"cited_paper":"/paper/astro-ph/0106005","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:d5707e456b35f1b0664581e97a8238e87eba6865a566faa8b3a920d6f6a419a4","observation_id":"5db74687-c19a-4f28-9e98-0da695e6dda9","resolution":{"observed_at":"2026-08-07T00:14:07.688476Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.04018","last_updated":"2016-05-31T12:31:32Z","snapshot_observed_at":"2026-07-06T04:45:59.479347Z","submitted_at":"2016-02-12T11:32:06Z","title":"The kinematics of globular clusters systems in the outer halos of the Aquarius simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.04018","snapshot_observed_at":"2026-08-07T00:14:07.802360Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:07.802360Z"},"links":{"cited_paper":"/paper/1602.04018","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:80d7687fd38e3710af7db92c9bc958c3ab768fa2c9fd01f9a444e5142948dff3","observation_id":"5c0b1879-e7a4-477c-98c7-1026f04ff2b2","resolution":{"observed_at":"2026-08-07T00:14:07.802360Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0109342","last_updated":"2001-09-20T14:22:48Z","snapshot_observed_at":"2026-07-07T00:21:37.649124Z","submitted_at":"2001-09-20T14:22:48Z","title":"Deep ROSAT-HRI observations of the NGC 1399/NGC 1404 region: morphology and structure of the X-ray halo","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0109342","snapshot_observed_at":"2026-08-07T00:14:08.113029Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:08.113029Z"},"links":{"cited_paper":"/paper/astro-ph/0109342","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:26b1714267b2b784330e9dd79c28cd96274f54ab7dbd7766cf3ca2f56204917c","observation_id":"02693ae5-9c27-45f5-ad0a-65dbf89a5cce","resolution":{"observed_at":"2026-08-07T00:14:08.113029Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.09922","last_updated":"2017-08-16T14:29:11Z","snapshot_observed_at":"2026-08-01T16:18:26.000248Z","submitted_at":"2016-11-29T22:26:47Z","title":"Density profile of dark matter haloes and galaxies in the Horizon-AGN simulation: the impact of AGN feedback","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.09922","snapshot_observed_at":"2026-08-07T00:14:08.285392Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:08.285392Z"},"links":{"cited_paper":"/paper/1611.09922","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:3c630e92fa951f00f8e2c65651d1429d106e07a42b5f08c4db947e85bbd49b7b","observation_id":"c2b38091-acc2-4943-9fae-07a214a2108d","resolution":{"observed_at":"2026-08-07T00:14:08.285392Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:08.430558Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:08.430558Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:6aa81fe9a31039978b3944b7d2d484aef473c7324ff3ef4f705c94e0f91afad4","observation_id":"7d2fa02e-14ca-45ad-a102-7626e70648e2","resolution":{"observed_at":"2026-08-07T00:14:08.430558Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0309465","last_updated":"2003-12-02T20:26:13Z","snapshot_observed_at":"2026-08-01T16:35:40.702970Z","submitted_at":"2003-09-17T07:32:36Z","title":"The Dark Matter Distribution in the Central Regions of Galaxy Clusters: Implications for CDM","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0309465","snapshot_observed_at":"2026-08-07T00:14:08.589266Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:08.589266Z"},"links":{"cited_paper":"/paper/astro-ph/0309465","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:e426b50c235347f01b54201de0f21e8ca3f0f20c11dbd7048f9843b14bfd4a22","observation_id":"c5d9f684-f5dc-435f-8727-2c53551118df","resolution":{"observed_at":"2026-08-07T00:14:08.589266Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0710.1069","last_updated":"2007-10-04T18:36:38Z","snapshot_observed_at":"2026-07-06T01:30:44.394035Z","submitted_at":"2007-10-04T18:36:38Z","title":"Separating baryons and dark matter in cluster cores: a full 2-D lensing and dynamic analysis of Abell 383 and MS2137-23","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0710.1069","snapshot_observed_at":"2026-08-07T00:14:08.774741Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:08.774741Z"},"links":{"cited_paper":"/paper/0710.1069","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:8a3e992c3bbee6222bf141adeb0c8f6fee66b61436b8c4b78f5e8f9e26776514","observation_id":"c063cbc9-0ae2-4682-bc5e-3ddf5be60e2b","resolution":{"observed_at":"2026-08-07T00:14:08.774741Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1209.1392","last_updated":"2013-02-26T05:52:15Z","snapshot_observed_at":"2026-07-06T02:55:09.130398Z","submitted_at":"2012-09-06T20:00:02Z","title":"The Density Profiles of Massive, Relaxed Galaxy Clusters. II. Separating Luminous and Dark Matter in Cluster Cores","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1209.1392","snapshot_observed_at":"2026-08-07T00:14:08.923389Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:08.923389Z"},"links":{"cited_paper":"/paper/1209.1392","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:a237611442df869548c97aef85275b7cf3285ec89b1fa712c9f9cd986799d67d","observation_id":"65cbd970-e060-49b9-babb-5bf32fb78640","resolution":{"observed_at":"2026-08-07T00:14:08.923389Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ab609d","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:23.279777Z","title":"Walker and Mario Mateo and Edward W","venue":null,"work_id":"fbeb0019-250a-4bbd-a4e7-c6fd98f14ecd","year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:09.085077Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:459b6c580d35cce82aaa324aad35e6be4a5318742f78a700fbc680389d7e5f30","observation_id":"3bc0cdc4-8713-4bdf-9a78-fee4a27b4a5b","resolution":{"observed_at":"2026-08-07T00:14:23.364285Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-07T00:14:09.212262Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:09.212262Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:9122ee73a0bf7dc296e9da97a3bf1ba9f54829e811c14f3fa66fc6a2323d8868","observation_id":"132267f2-88ad-4342-903e-be4eca2afb03","resolution":{"observed_at":"2026-08-07T00:14:09.212262Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:09.340299Z","title":", keywords =","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:09.340299Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:912020f7bbc2e1d5dd862d211d2672a824bdef0cad233ce3b8248ab1790cf148","observation_id":"79cf9583-7b9a-4fc7-a412-0b46866eb6ea","resolution":{"observed_at":"2026-08-07T00:14:09.340299Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1407.4730","last_updated":"2015-01-20T19:51:44Z","snapshot_observed_at":"2026-07-06T03:49:19.093285Z","submitted_at":"2014-07-17T16:28:26Z","title":"A universal model for halo concentrations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1407.4730","snapshot_observed_at":"2026-08-07T00:14:09.456961Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:09.456961Z"},"links":{"cited_paper":"/paper/1407.4730","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:5a9350786a6b4a194b352b6c3f8c34a5e21de2c25795115c216bffa808457e67","observation_id":"064f0b93-7938-48ec-8352-3be1e181cd5a","resolution":{"observed_at":"2026-08-07T00:14:09.456961Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1409.8617","last_updated":"2015-05-25T09:49:21Z","snapshot_observed_at":"2026-08-04T02:03:52.228774Z","submitted_at":"2014-09-30T16:24:57Z","title":"Baryon effects on the internal structure of LCDM halos in the EAGLE simulations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1409.8617","snapshot_observed_at":"2026-08-07T00:14:09.534113Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:09.534113Z"},"links":{"cited_paper":"/paper/1409.8617","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:8ce5fe0c6a8082029fd44f7f4321bb79b3ebe40fb925923b59144f40d2303325","observation_id":"2be5c641-e420-41d9-984d-fbec80274299","resolution":{"observed_at":"2026-08-07T00:14:09.534113Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.08282","last_updated":"2021-01-20T19:00:10Z","snapshot_observed_at":"2026-07-06T10:34:09.630357Z","submitted_at":"2021-01-20T19:00:10Z","title":"What to expect when using globular clusters as tracers of the total mass distribution in Milky Way-mass galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.08282","snapshot_observed_at":"2026-08-07T00:14:09.632599Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:09.632599Z"},"links":{"cited_paper":"/paper/2101.08282","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:0d591114a6811ce1b257c26f4104d393f2e4e443712e62465516a7ace15ff9f2","observation_id":"8f490a3d-45af-4ae4-b347-0d7bb896450e","resolution":{"observed_at":"2026-08-07T00:14:09.632599Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.08997","last_updated":"2022-08-18T18:00:01Z","snapshot_observed_at":"2026-07-06T13:43:17.139333Z","submitted_at":"2022-08-18T18:00:01Z","title":"New Velocity Measurements of NGC 5128 Globular Clusters out to 130 kpc: Outer Halo Kinematics, Substructure and Dynamics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.08997","snapshot_observed_at":"2026-08-07T00:14:09.757615Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:09.757615Z"},"links":{"cited_paper":"/paper/2208.08997","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:d74d40d9989d94f7e073efb4aec71c46adec2038166c5c20a770606e0f30c5a7","observation_id":"8b75e226-f038-4e00-8fc8-97bbf6041231","resolution":{"observed_at":"2026-08-07T00:14:09.757615Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1038/379427a0","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:23.143343Z","title":", year = 1996, month = feb, volume =","venue":null,"work_id":"d228d4cc-dccd-4544-8272-c61a2aff9c3e","year":1996},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:09.893713Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:d90c9ea81b6c6a25020369173da8ab64d64f596e0bd58ec1bd53669fb55612c0","observation_id":"30448eea-cb94-4025-8720-b840b0960a19","resolution":{"observed_at":"2026-08-07T00:14:23.189731Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1809.02134","last_updated":"2018-09-06T18:00:00Z","snapshot_observed_at":"2026-07-06T06:59:38.852251Z","submitted_at":"2018-09-06T18:00:00Z","title":"The Recent Growth History of the Fornax Cluster Derived from Simultaneous Sloshing and Gas Stripping: Simulating the Infall of NGC 1404","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.02134","snapshot_observed_at":"2026-08-07T00:14:10.026706Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:10.026706Z"},"links":{"cited_paper":"/paper/1809.02134","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:05a73f9ac73de385c8e5a6654a9287142c3550bf68bd1b50abcd8d87879f5308","observation_id":"9b5846e3-e998-4130-81bd-cb96aadc418b","resolution":{"observed_at":"2026-08-07T00:14:10.026706Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0711.4077","last_updated":"2007-11-26T18:55:10Z","snapshot_observed_at":"2026-07-06T01:32:53.743235Z","submitted_at":"2007-11-26T18:55:10Z","title":"The dark matter halo of NGC 1399 - CDM or MOND?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0711.4077","snapshot_observed_at":"2026-08-07T00:14:10.136648Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:10.136648Z"},"links":{"cited_paper":"/paper/0711.4077","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:0c4d42759378df1c5103b841483f2511d41b7e2a1e33b3e01eba4599e2c744f3","observation_id":"ab006580-9cba-4b69-b332-cf14da5f9e2f","resolution":{"observed_at":"2026-08-07T00:14:10.136648Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:10.255854Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:10.255854Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:c9e09c7dc61022ca03caf22891d4d92c6b9c66970d2cda103ec9f755b3941c55","observation_id":"4e6cf733-5ea4-4d52-9d31-8ecd62e029ea","resolution":{"observed_at":"2026-08-07T00:14:10.255854Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:10.368630Z","title":"Monthly Notices of the Royal Astronomical Society , author =","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:10.368630Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:8b492d14991be5f508a42cc9bfa96c70d4ba0a77c204d3b4243cf35d5246a8c9","observation_id":"71ce3c19-e9b4-4f5c-9720-0f066bb7622e","resolution":{"observed_at":"2026-08-07T00:14:10.368630Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:10.482686Z","title":"Monthly Notices of the Royal Astronomical Society , author =","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:10.482686Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:43401de203da5633c5cb1266ee53d071492dccdf33b303fa1d2a7cf8a9fdfa87","observation_id":"992a7750-1f05-4c56-adb1-b29e9760bd1b","resolution":{"observed_at":"2026-08-07T00:14:10.482686Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:10.672440Z","title":"The faint light in groups and clusters of galaxies , url =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:10.672440Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:9f94f8de7647b23e9975dc8f8af97c13bef71e55c7e7ea94da0a1d42bcd57ebb","observation_id":"6f193e43-105a-4212-8a92-fe540cbd2de8","resolution":{"observed_at":"2026-08-07T00:14:10.672440Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:10.818289Z","title":"Monthly Notices of the Royal Astronomical Society , author =","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:10.818289Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:bd70c0b82b40448d39094d7d894bae15f07b043a6ae9b46cd84cb3cb77238ca2","observation_id":"8e88aa6a-5307-4c71-b8bc-a02d132b0997","resolution":{"observed_at":"2026-08-07T00:14:10.818289Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:10.931058Z","title":"Journal of the Royal Statistical Society: Series D (The Statistician) , author =","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:10.931058Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:f0d390222835a604880e142a32f3ebd545237738f1c17ce18d506efebca04d49","observation_id":"e01bb6b0-3418-4e26-9919-b93d09bb9985","resolution":{"observed_at":"2026-08-07T00:14:10.931058Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:11.034825Z","title":", year = 1993, month = nov, volume =","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:11.034825Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:5129a23a01c27db7056341f79a2da24b6f3a9288be99ce76a0e8f3e35eb0af5d","observation_id":"d6c32250-b62a-448e-ba0d-488327b02b6e","resolution":{"observed_at":"2026-08-07T00:14:11.034825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:11.107201Z","title":"Boletin de la Asociacion Argentina de Astronomia La Plata Argentina , year = 1963, month = feb, volume =","venue":null,"work_id":null,"year":1963},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:11.107201Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:ecc03b90e4be2312be3d8f7e35de3193edf7bf06d6a2255563df56283fa7846e","observation_id":"2547bb92-1d4e-4062-b0e7-d0504e95fafc","resolution":{"observed_at":"2026-08-07T00:14:11.107201Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.08695","last_updated":"2021-09-30T10:35:33Z","snapshot_observed_at":"2026-08-06T05:53:20.946463Z","submitted_at":"2021-09-17T18:00:08Z","title":"The Fornax Cluster VLT Spectroscopic Survey IV -- Cold kinematical substructures in the Fornax core from COSTA","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2109.08695","snapshot_observed_at":"2026-08-07T00:14:11.249099Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:11.249099Z"},"links":{"cited_paper":"/paper/2109.08695","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:8cdbeb29b290024e47ceeedacb6d65fae9fe8c8cb7bf1a171972a0f11511f53f","observation_id":"1b7cb1ef-1501-4ed2-87f2-10e48d49ee58","resolution":{"observed_at":"2026-08-07T00:14:11.249099Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9812033","last_updated":"1998-12-02T00:14:55Z","snapshot_observed_at":"2026-07-07T01:23:18.957958Z","submitted_at":"1998-12-02T00:14:55Z","title":"Galaxy Disruption as the Origin of Intracluster Light in the Coma Cluster","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9812033","snapshot_observed_at":"2026-08-07T00:14:11.369449Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:11.369449Z"},"links":{"cited_paper":"/paper/astro-ph/9812033","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:1294a9f523e5c05b560a279e826418f51e3b6e7a1b0db7852175efb9dcc123fe","observation_id":"458a323a-0e3f-4f49-8eee-6864953224c7","resolution":{"observed_at":"2026-08-07T00:14:11.369449Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.2070","last_updated":"2014-08-26T11:07:26Z","snapshot_observed_at":"2026-07-06T03:43:12.725828Z","submitted_at":"2014-05-08T20:00:01Z","title":"Intra-Cluster Light at the Frontier: Abell 2744","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.2070","snapshot_observed_at":"2026-08-07T00:14:11.475307Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:11.475307Z"},"links":{"cited_paper":"/paper/1405.2070","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:f0dc338406abec4bd4d70d7772939ca87c858fc469a3d24caf737fef46db22db","observation_id":"d0f3dd56-9acf-4417-9ef7-a92ab1ef4bf7","resolution":{"observed_at":"2026-08-07T00:14:11.475307Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.01050","last_updated":"2018-12-03T19:34:39Z","snapshot_observed_at":"2026-07-06T07:18:49.521593Z","submitted_at":"2018-12-03T19:34:39Z","title":"The Fornax Deep Survey with VST. V. Exploring the faintest regions of the bright early-type galaxies inside the virial radius","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1812.01050","snapshot_observed_at":"2026-08-07T00:14:11.558798Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:11.558798Z"},"links":{"cited_paper":"/paper/1812.01050","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:a6c0c4b1e29bffd6830b88059389845c75ea76466535633e021756788ff1b2f2","observation_id":"59816cc0-66b6-4f02-a7db-1f2f823a2f30","resolution":{"observed_at":"2026-08-07T00:14:11.558798Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.08544","last_updated":"2020-11-25T19:02:31Z","snapshot_observed_at":"2026-07-06T08:16:13.373890Z","submitted_at":"2019-08-22T18:00:02Z","title":"Structure of Brightest Cluster Galaxies and Intracluster Light","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.08544","snapshot_observed_at":"2026-08-07T00:14:11.645543Z","title":", keywords =","venue":null,"work_id":null,"year":1908},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:11.645543Z"},"links":{"cited_paper":"/paper/1908.08544","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:f461fd3669c7297c0c1f6092fad2ae176ec592252242c76254ee1f066f0f9691","observation_id":"14f0b5d7-993a-4f3f-bd72-1a9dcbc4c623","resolution":{"observed_at":"2026-08-07T00:14:11.645543Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.03360","last_updated":"2022-06-03T11:50:28Z","snapshot_observed_at":"2026-08-06T02:16:45.596816Z","submitted_at":"2022-03-07T13:09:31Z","title":"Machine Learning to identify ICL and BCG in simulated galaxy clusters","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.03360","snapshot_observed_at":"2026-08-07T00:14:11.784001Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:11.784001Z"},"links":{"cited_paper":"/paper/2203.03360","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:fb9d69583834cb2e8d3dd5539fbf7c7dd32a030c2a81cf75ddf592808c3f251a","observation_id":"88d6c895-28dc-4ddc-9ce9-ce9bf9b5f5ab","resolution":{"observed_at":"2026-08-07T00:14:11.784001Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0903.1636","last_updated":"2009-06-16T08:02:42Z","snapshot_observed_at":"2026-08-06T20:20:36.473420Z","submitted_at":"2009-03-09T20:00:36Z","title":"Minor mergers and the size evolution of elliptical galaxies","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0903.1636","snapshot_observed_at":"2026-08-07T00:14:11.934449Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:11.934449Z"},"links":{"cited_paper":"/paper/0903.1636","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:9113cbece004e20f847955a673da73ca349211738353a44d5423a93ede67ba24","observation_id":"f6c78bc7-fe94-4b49-9332-67ad3f1959a6","resolution":{"observed_at":"2026-08-07T00:14:11.934449Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1010.1381","last_updated":"2010-12-07T18:52:02Z","snapshot_observed_at":"2026-08-04T19:37:39.533757Z","submitted_at":"2010-10-07T09:59:00Z","title":"The Two Phases of Galaxy Formation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1010.1381","snapshot_observed_at":"2026-08-07T00:14:12.069549Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:12.069549Z"},"links":{"cited_paper":"/paper/1010.1381","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:42d64fe6c82a29ba5fc0ab93e9a85cb6242645828df3a64c65fc5ec8cf6b3226","observation_id":"7fca8d22-da69-474c-8a0b-3a6e3988a22f","resolution":{"observed_at":"2026-08-07T00:14:12.069549Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1009.5992","last_updated":"2010-09-29T20:00:03Z","snapshot_observed_at":"2026-07-06T02:16:05.048610Z","submitted_at":"2010-09-29T20:00:03Z","title":"A Substantial Population of Low Mass Stars in Luminous Elliptical Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1009.5992","snapshot_observed_at":"2026-08-07T00:14:12.164184Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:12.164184Z"},"links":{"cited_paper":"/paper/1009.5992","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:7cf259ef501ccebedfcd277a7ffe266cd4bdf6b79ad61853aa4555b20bafc2e9","observation_id":"0b83f7ee-b60d-4204-bd04-050ad23cc690","resolution":{"observed_at":"2026-08-07T00:14:12.164184Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1205.5289","last_updated":"2012-06-27T08:43:03Z","snapshot_observed_at":"2026-07-06T02:48:40.122616Z","submitted_at":"2012-05-23T20:58:54Z","title":"A tale of two tails and an off-centered envelope: diffuse light around the cD galaxy NGC 3311 in the Hydra I cluster","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1205.5289","snapshot_observed_at":"2026-08-07T00:14:12.235265Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:12.235265Z"},"links":{"cited_paper":"/paper/1205.5289","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:4f8505eefb2a6b930a12e0b1706e00635548d69375a2884134bd083f102df0cc","observation_id":"6ee5a8ac-62a9-4ebd-85d6-b41f8629d0d7","resolution":{"observed_at":"2026-08-07T00:14:12.235265Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:12.338592Z","title":"Astronomy & Astrophysics , author =","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:12.338592Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:1bc23287cf836e806a8946d5df95c85f48f2907b1473475bcb273818dc5521a3","observation_id":"1c6ad444-3008-49c4-bba6-45a6f25293cc","resolution":{"observed_at":"2026-08-07T00:14:12.338592Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0401175","last_updated":"2004-01-10T14:50:04Z","snapshot_observed_at":"2026-07-07T00:39:37.044390Z","submitted_at":"2004-01-10T14:50:04Z","title":"The Globular Cluster System of NGC 1399. II. Kinematics of a Large Sample of Globular Clusters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0401175","snapshot_observed_at":"2026-08-07T00:14:12.773375Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:12.773375Z"},"links":{"cited_paper":"/paper/astro-ph/0401175","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:24e7a1fc515b9ce8b957159e2e5147da6ea5499c1807b0b512916a950cf97073","observation_id":"653e5199-b6cc-4714-915a-937ba904e33c","resolution":{"observed_at":"2026-08-07T00:14:12.773375Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.01884","last_updated":"2019-10-04T11:52:37Z","snapshot_observed_at":"2026-07-06T08:26:53.575779Z","submitted_at":"2019-10-04T11:52:37Z","title":"Astroinformatics based search for globular clusters in the Fornax Deep Survey","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.01884","snapshot_observed_at":"2026-08-07T00:14:12.950489Z","title":", keywords =","venue":null,"work_id":null,"year":1910},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:12.950489Z"},"links":{"cited_paper":"/paper/1910.01884","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:16f83115986e294c0337d64764ea2f9df5367b526e677d4721ce1948341a5974","observation_id":"c55dc784-cc7c-4ce4-b185-c0bb572c7644","resolution":{"observed_at":"2026-08-07T00:14:12.950489Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:13.060752Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:13.060752Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:14467409c0cd3a2778bed98f20f5374602f303d179053b7d1e73bd9c7eee5e6b","observation_id":"3765f2f5-6667-47fa-aa65-668993f7f0a1","resolution":{"observed_at":"2026-08-07T00:14:13.060752Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.06076","last_updated":"2016-02-19T08:47:18Z","snapshot_observed_at":"2026-08-05T00:18:42.951963Z","submitted_at":"2016-02-19T08:47:18Z","title":"The Extended Spatial Distribution of Globular Clusters in the Core of the Fornax Cluster","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.06076","snapshot_observed_at":"2026-08-07T00:14:13.150002Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:13.150002Z"},"links":{"cited_paper":"/paper/1602.06076","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:46dd670733493fba7561a30f594754e371d23ee4ff841b0bafccba3443d8f95b","observation_id":"30d9c31b-d6ac-4f3e-93d4-68c832e4e55b","resolution":{"observed_at":"2026-08-07T00:14:13.150002Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9504041","last_updated":"1995-04-12T15:15:01Z","snapshot_observed_at":"2026-08-03T08:52:14.570781Z","submitted_at":"1995-04-12T15:15:01Z","title":"The Structure of Dark Matter Haloes in Dwarf Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9504041","snapshot_observed_at":"2026-08-07T00:14:13.226809Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:13.226809Z"},"links":{"cited_paper":"/paper/astro-ph/9504041","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:94fb468248322dc9e3b47eedc822439e31b2d0dace7861c9807074c17b09236f","observation_id":"bc3c0f41-de97-4b10-9bed-56bd228b3e35","resolution":{"observed_at":"2026-08-07T00:14:13.226809Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9611107","last_updated":"1997-10-21T23:14:37Z","snapshot_observed_at":"2026-07-07T01:15:03.940917Z","submitted_at":"1996-11-13T22:59:55Z","title":"A Universal Density Profile from Hierarchical Clustering","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9611107","snapshot_observed_at":"2026-08-07T00:14:13.318791Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:13.318791Z"},"links":{"cited_paper":"/paper/astro-ph/9611107","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:b0c21d548b423ed788e8d69a47f75a6b3072ef0908fdba47b98d2623c5a49712","observation_id":"4ea8ffe7-c526-4c7b-a4b5-feca46e9a049","resolution":{"observed_at":"2026-08-07T00:14:13.318791Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1208.3522","last_updated":"2013-03-27T19:07:59Z","snapshot_observed_at":"2026-07-06T02:53:53.604023Z","submitted_at":"2012-08-17T02:59:35Z","title":"The Atlas3D project - XV. Benchmark for early-type galaxies scaling relations from 260 dynamical models: mass-to-light ratio, dark matter, Fundamental Plane and Mass Plane","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1208.3522","snapshot_observed_at":"2026-08-07T00:14:13.387949Z","title":"Benchmark for early-type galaxies scaling relations from 260 dynamical models: mass-to-light ratio, dark matter, Fundamental Plane and Mass Plane","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:13.387949Z"},"links":{"cited_paper":"/paper/1208.3522","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:9a7fb556c5960c329163e80d818624e34a28f66e64773c5af35331ab7c462ecf","observation_id":"640b96af-d6a5-4c47-9b54-1efd32e5ec88","resolution":{"observed_at":"2026-08-07T00:14:13.387949Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.11786","last_updated":"2023-06-20T18:00:01Z","snapshot_observed_at":"2026-07-06T15:44:46.456226Z","submitted_at":"2023-06-20T18:00:01Z","title":"Investigating the Dark Matter Halo of NGC 5128 using a Discrete Dynamical Model","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.11786","snapshot_observed_at":"2026-08-07T00:14:13.508435Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:13.508435Z"},"links":{"cited_paper":"/paper/2306.11786","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:f8c19108578d09c705e7ba85c574f7b7728b12c3efdd1971a7b6bc9af7f40cbc","observation_id":"26db2d48-0e10-4d6c-86b1-f8ba70581387","resolution":{"observed_at":"2026-08-07T00:14:13.508435Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.00812","last_updated":"2018-10-26T11:17:20Z","snapshot_observed_at":"2026-07-06T06:21:31.375147Z","submitted_at":"2018-02-02T19:00:00Z","title":"Globular cluster populations and the kinematical fingerprints of minor mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.00812","snapshot_observed_at":"2026-08-07T00:14:13.598033Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:13.598033Z"},"links":{"cited_paper":"/paper/1802.00812","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:dc3a59edf432af1cfa6cb0a4c4bda917fa2aa422df6f8fe994d1e76008e0fd85","observation_id":"061088b1-5195-440a-a61e-c8a9554203b2","resolution":{"observed_at":"2026-08-07T00:14:13.598033Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:13.684728Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:13.684728Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:c51071b3a23e44e28e32bcade2c5b241f93a5a7d3fbc8efd2782a1ceec6ef9f1","observation_id":"84e8d881-2a73-4d0d-902f-e5fc6cfb7e93","resolution":{"observed_at":"2026-08-07T00:14:13.684728Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1307.6212","last_updated":"2013-07-23T20:00:01Z","snapshot_observed_at":"2026-08-05T05:45:26.588200Z","submitted_at":"2013-07-23T20:00:01Z","title":"Astropy: A Community Python Package for Astronomy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.6212","snapshot_observed_at":"2026-08-07T00:14:13.766416Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:13.766416Z"},"links":{"cited_paper":"/paper/1307.6212","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:390298e80e2cdf7ed77333cc6d1980024e3666ee5042cef14f6bc0136b8e1c29","observation_id":"86ad5be0-df55-43f4-a8ee-0c9e679ff208","resolution":{"observed_at":"2026-08-07T00:14:13.766416Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.02634","last_updated":"2018-01-16T15:05:07Z","snapshot_observed_at":"2026-07-06T06:17:44.962713Z","submitted_at":"2018-01-08T19:00:08Z","title":"The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.02634","snapshot_observed_at":"2026-08-07T00:14:13.830430Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:13.830430Z"},"links":{"cited_paper":"/paper/1801.02634","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:4d24a1ad6942ad062e5513e39e1a8f54c158b926e3b73e19d62522314264f7dd","observation_id":"94869a30-0c8b-430d-99c8-415a818163b2","resolution":{"observed_at":"2026-08-07T00:14:13.830430Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:13.906022Z","title":"and Varoquaux, G","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:13.906022Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:c168fde16c24fcdda5bb892c79fb6bdb4ca29d09d4b512d88246e1e3c52a3dd1","observation_id":"5161374f-14f7-483a-9d9e-23d4cc2adbe3","resolution":{"observed_at":"2026-08-07T00:14:13.906022Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:13.989905Z","title":", keywords =","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:13.989905Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:6798dd0b25b989066bc4773f35b7e466d45d98058e72d67018ceb2c3d3de4039","observation_id":"27f77f4b-a8c9-4499-bfbe-f2ff0ee0336b","resolution":{"observed_at":"2026-08-07T00:14:13.989905Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:14.062119Z","title":"The case of NGC 1404 in the Fornax cluster","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:14.062119Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:de6aa308bedca3fe974b540e3bc2d3a0bc13ffc057853c3a8ab2afe6e8b30ddb","observation_id":"9f8e2e46-9168-401f-bbef-ac5f89e456ad","resolution":{"observed_at":"2026-08-07T00:14:14.062119Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0701378","last_updated":"2007-01-12T12:58:03Z","snapshot_observed_at":"2026-07-07T01:06:07.111737Z","submitted_at":"2007-01-12T12:58:03Z","title":"Globular clusters and dwarf galaxies in Fornax - I. Kinematics in the cluster core from multi-object spectroscopy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0701378","snapshot_observed_at":"2026-08-07T00:14:14.142810Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:14.142810Z"},"links":{"cited_paper":"/paper/astro-ph/0701378","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:a374e6610b2dc82c4e750c57aa0f6bbd06716d8c759037b883bb9f7a475435cb","observation_id":"f1d2f7d0-b7d5-4e88-bf6f-e66fbf2216d9","resolution":{"observed_at":"2026-08-07T00:14:14.142810Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:14.213388Z","title":"and Strader, Jay , title =","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:14.213388Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:abb1f22c5a0bb67b20159ace25a82670966346eb6cdb49625aa41ad9a6835e31","observation_id":"ecdb44e3-769f-40ab-9619-e1c8cf4bfcd7","resolution":{"observed_at":"2026-08-07T00:14:14.213388Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1507.01336","last_updated":"2015-07-10T08:01:34Z","snapshot_observed_at":"2026-07-06T04:22:56.796295Z","submitted_at":"2015-07-06T07:28:59Z","title":"VEGAS: A VST Early-type GAlaxy Survey. I. Presentation, wide-field surface photometry, and substructures in NGC 4472","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1507.01336","snapshot_observed_at":"2026-08-07T00:14:14.285037Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:14.285037Z"},"links":{"cited_paper":"/paper/1507.01336","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:839cc9a4566dfdbc6a861de687eee582d8efb39d653ca72aff0defc63db35508","observation_id":"90e059d9-ee8a-4b84-9fcf-e6b1ffae3a03","resolution":{"observed_at":"2026-08-07T00:14:14.285037Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:14.363267Z","title":"and D'Souza, Richard and Kauffmann, Guinevere and Wang, Jing and Boylan-Kolchin, Michael and Guo, Qi and Frenk, Carlos S","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:14.363267Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:3f9ab47f4d3e926bfc7f28e479082e3e997288e9dcb9cc1bba72b6fcd956de3e","observation_id":"ff38a1a6-633c-4e1f-b96f-1d3839b75694","resolution":{"observed_at":"2026-08-07T00:14:14.363267Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:14.445129Z","title":"Cleveland , title =","venue":null,"work_id":null,"year":1979},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:14.445129Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:3760483a140cc8039f7b64a2c2b2e76f990dff17aaee406e51e3aed737eb6e66","observation_id":"ce05c827-0fe4-48b9-a909-3e024dd2ee89","resolution":{"observed_at":"2026-08-07T00:14:14.445129Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:14.514800Z","title":"Cleveland and Susan J","venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:14.514800Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:338788f4be42e534e8bdadb054da36c346c26119d786836934193bdd0d3b26c4","observation_id":"af38ee75-d44e-4089-a12e-dd2010513c33","resolution":{"observed_at":"2026-08-07T00:14:14.514800Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1402.6090","last_updated":"2014-02-25T08:36:04Z","snapshot_observed_at":"2026-07-06T03:36:51.545768Z","submitted_at":"2014-02-25T08:36:04Z","title":"Globular clusters of NGC 3115 in the near-infrared. Demonstrating the correctness of two opposing scenarios","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1402.6090","snapshot_observed_at":"2026-08-07T00:14:14.592931Z","title":"Demonstrating the correctness of two opposing scenarios","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:14.592931Z"},"links":{"cited_paper":"/paper/1402.6090","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:afd39b77aa2c64b44591ee890e025ce707eb698d0bf5db18932d1f48df59e9f8","observation_id":"8661862c-fbae-4de2-9a3b-2d5f45f32e31","resolution":{"observed_at":"2026-08-07T00:14:14.592931Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.00750","last_updated":"2017-11-02T14:09:37Z","snapshot_observed_at":"2026-07-06T06:07:24.178032Z","submitted_at":"2017-11-02T14:09:37Z","title":"VEGAS-SSS II: Comparing the globular cluster systems in NGC3115 and NGC1399 using VEGAS and FDS survey data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.00750","snapshot_observed_at":"2026-08-07T00:14:14.679340Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:14.679340Z"},"links":{"cited_paper":"/paper/1711.00750","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:e51e22ad903b555b6035201545585dd3eed92bbeec3d6d53a2448553dc9eb2a9","observation_id":"156a850d-caf3-44c5-a936-85c9f22d0ebf","resolution":{"observed_at":"2026-08-07T00:14:14.679340Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.12085","last_updated":"2020-09-03T14:53:49Z","snapshot_observed_at":"2026-07-06T09:23:04.010956Z","submitted_at":"2020-05-25T12:59:37Z","title":"The Fornax Deep Survey with VST. IX. The catalog of sources in the FDS area, with an example study for globular clusters and background galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.12085","snapshot_observed_at":"2026-08-07T00:14:14.773302Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:14.773302Z"},"links":{"cited_paper":"/paper/2005.12085","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:848e6aa7556a3bc75b5408336745b6abcac560e65a31f4a2697be08f66cda6d2","observation_id":"f62efebe-a89d-42b2-9944-db06c94fd465","resolution":{"observed_at":"2026-08-07T00:14:14.773302Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:14.841116Z","title":", keywords =","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:14.841116Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:719f9d6dba9daf2147c2e44a37dd20a48eeddc28905aea318e977711c22f3505","observation_id":"9e4f5d94-f9e5-4449-9762-eb7e36fc3a18","resolution":{"observed_at":"2026-08-07T00:14:14.841116Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1209.0356","last_updated":"2013-09-03T18:12:36Z","snapshot_observed_at":"2026-07-06T02:54:51.696920Z","submitted_at":"2012-09-03T13:56:36Z","title":"Signatures of accretion events in the halos of early-type galaxies from comparing PNe and GCs kinematics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1209.0356","snapshot_observed_at":"2026-08-07T00:14:14.923065Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:14.923065Z"},"links":{"cited_paper":"/paper/1209.0356","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:fe0dcc44f1a98c96232e6d5c03a8a11d7116f2fa3a15083ccdf78d84fc2ecad4","observation_id":"079950aa-2d98-497f-97ed-6a34ac6f1315","resolution":{"observed_at":"2026-08-07T00:14:14.923065Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0312201","last_updated":"2003-12-08T12:34:33Z","snapshot_observed_at":"2026-07-07T00:38:54.734400Z","submitted_at":"2003-12-08T12:34:33Z","title":"Parametric Recovery of Line-of-Sight Velocity Distributions from Absorption-Line Spectra of Galaxies via Penalized Likelihood","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0312201","snapshot_observed_at":"2026-08-07T00:14:14.981479Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:14.981479Z"},"links":{"cited_paper":"/paper/astro-ph/0312201","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:e41d0adab6cdee7bad290425c26ad364dd1263c13c0981ba5d1ed4a0660ac95c","observation_id":"ef631b29-3ef0-408d-ac3a-8355d59ce5fc","resolution":{"observed_at":"2026-08-07T00:14:14.981479Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1607.08538","last_updated":"2016-11-18T14:37:36Z","snapshot_observed_at":"2026-07-06T05:05:16.748241Z","submitted_at":"2016-07-28T17:16:58Z","title":"Improving the full spectrum fitting method: accurate convolution with Gauss-Hermite functions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1607.08538","snapshot_observed_at":"2026-08-07T00:14:15.053631Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:15.053631Z"},"links":{"cited_paper":"/paper/1607.08538","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:02930dc2c084a8dbb84d56f95e2b29e93be26108f9aff3e81d596b8a251e6a1c","observation_id":"281c2121-ac23-492f-9495-d95449e5eef7","resolution":{"observed_at":"2026-08-07T00:14:15.053631Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1208.3523","last_updated":"2013-04-15T17:20:47Z","snapshot_observed_at":"2026-08-03T20:47:10.410884Z","submitted_at":"2012-08-17T02:59:48Z","title":"The Atlas3D project - XX. Mass-size and mass-sigma distributions of early-type galaxies: bulge fraction drives kinematics, mass-to-light ratio, molecular gas fraction and stellar initial mass function","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1208.3523","snapshot_observed_at":"2026-08-07T00:14:15.126622Z","title":"Mass-size and mass- distributions of early-type galaxies: bulge fraction drives kinematics, mass-to-light ratio, molecular gas fraction and stellar initial mass function","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:15.126622Z"},"links":{"cited_paper":"/paper/1208.3523","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:c20983343940a1b41f684c919923c842720c5d17eff8747cbd173c661e123b80","observation_id":"aba73cac-ad0e-4a64-876c-7b5c20f70f4e","resolution":{"observed_at":"2026-08-07T00:14:15.126622Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:15.210172Z","title":"and Haberland, Matt and Reddy, Tyler and Cournapeau, David and Burovski, Evgeni and Peterson, Pearu and Weckesser, Warren and Bright, Jonathan and","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:15.210172Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:6cebd3859b405591253075d1861a898c059ce9bcfeb62e3fa3f5296e08e44803","observation_id":"f474e959-f7f5-4f1e-ba42-d2343300ec93","resolution":{"observed_at":"2026-08-07T00:14:15.210172Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:15.276930Z","title":"Hogg and Dustin Lang and Jonathan Goodman , title =","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:15.276930Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:33915f13a86a03ae2013dc27f0da9cb630b79207737adeaee755d5aa2cced1a6","observation_id":"be0d772a-f7ff-4124-ad3f-2e4a97ffc7c4","resolution":{"observed_at":"2026-08-07T00:14:15.276930Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.09410","last_updated":"2020-05-19T13:08:50Z","snapshot_observed_at":"2026-07-06T09:21:39.131695Z","submitted_at":"2020-05-19T13:08:50Z","title":"A discrete chemo-dynamical model of M87's globular clusters: Kinematics extending to ~ 400 kpc","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.09410","snapshot_observed_at":"2026-08-07T00:14:15.347406Z","title":", keywords =","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:15.347406Z"},"links":{"cited_paper":"/paper/2005.09410","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:38cfed8c84fa85484f71fa9d4adf37d4eaddf97f06d71ffdad22f8b588b41b90","observation_id":"afafbf8f-375a-4ceb-90e7-3bf4a97d6999","resolution":{"observed_at":"2026-08-07T00:14:15.347406Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9804319","last_updated":"1998-04-29T23:08:31Z","snapshot_observed_at":"2026-07-07T01:20:40.325068Z","submitted_at":"1998-04-29T23:08:31Z","title":"The Formation of Giant Elliptical Galaxies and Their Globular Cluster Systems","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9804319","snapshot_observed_at":"2026-08-07T00:14:15.417486Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:15.417486Z"},"links":{"cited_paper":"/paper/astro-ph/9804319","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:f3c5ab7543cab2a6ecd822260766bcf47516afbb3c796d545ce42532339baa8f","observation_id":"02cc2844-5633-4c10-939f-1ebf88095db8","resolution":{"observed_at":"2026-08-07T00:14:15.417486Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.06396","last_updated":"2021-04-13T17:57:12Z","snapshot_observed_at":"2026-07-06T10:59:15.676279Z","submitted_at":"2021-04-13T17:57:12Z","title":"The SLUGGS survey: combining stars, globular clusters and planetary nebulae to understand the assembly history of early-type galaxies from their large radii kinematics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.06396","snapshot_observed_at":"2026-08-07T00:14:15.616822Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:15.616822Z"},"links":{"cited_paper":"/paper/2104.06396","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:d196eb38f2e24a7363a1aa69710b26db6b5d7a2b46756ab358024b0e71900cfe","observation_id":"38e398fb-4852-4bf9-b781-77e82b020f27","resolution":{"observed_at":"2026-08-07T00:14:15.616822Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:15.689705Z","title":"The merger origin of a fast- and a slow-rotating early-type galaxy revealed with deep optical imaging: first results","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:15.689705Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:d6154632b03206761e128f01473c9f5ac2da5d8e4888a3d0194dc63e63bce67a","observation_id":"ee9e4e4d-218c-4c7c-89d4-d7ef7ad1e137","resolution":{"observed_at":"2026-08-07T00:14:15.689705Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:15.757434Z","title":", keywords =","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:15.757434Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:816c0a8935c7dc61c7ff32b9a70bd55befc2c772cf866a007771f8f497023164","observation_id":"eb93199e-f7f1-4ad5-ad91-acfbe6484e52","resolution":{"observed_at":"2026-08-07T00:14:15.757434Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0703047","last_updated":"2007-03-02T18:03:09Z","snapshot_observed_at":"2026-08-06T01:43:25.194765Z","submitted_at":"2007-03-02T18:03:09Z","title":"The PN.S Elliptical Galaxy Survey: Data Reduction, Planetary Nebula Catalog, and Basic Dynamics for NGC 3379","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0703047","snapshot_observed_at":"2026-08-07T00:14:15.821971Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:15.821971Z"},"links":{"cited_paper":"/paper/astro-ph/0703047","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:0b404cc78925f85aa74caf98d4a401c5d34f65ccdb6833b28193562169a8105e","observation_id":"0127cd5d-2230-4895-8a77-67dfc3c19ae6","resolution":{"observed_at":"2026-08-07T00:14:15.821971Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0401218","last_updated":"2004-01-12T19:53:56Z","snapshot_observed_at":"2026-07-07T00:39:37.044390Z","submitted_at":"2004-01-12T19:53:56Z","title":"The Globular Cluster System of NGC 1399: III. VLT Spectroscopy and Database","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0401218","snapshot_observed_at":"2026-08-07T00:14:15.892848Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:15.892848Z"},"links":{"cited_paper":"/paper/astro-ph/0401218","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:a15ec00d07c1e51469f3cfad7c42406b2075ab52ea8feaf54bd2aabaa9dd1931","observation_id":"6de144a0-07db-4c46-995b-6a5da4fd6053","resolution":{"observed_at":"2026-08-07T00:14:15.892848Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0301223","last_updated":"2003-01-13T20:20:15Z","snapshot_observed_at":"2026-07-07T00:30:43.588193Z","submitted_at":"2003-01-13T20:20:15Z","title":"The Globular Cluster System of NGC 1399. I. A Wide-field Photometric Study","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0301223","snapshot_observed_at":"2026-08-07T00:14:15.962839Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:15.962839Z"},"links":{"cited_paper":"/paper/astro-ph/0301223","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:28edc991f1c39c833bd9bec90fa7f3b58fc851d2e00cba6f982c8806bb1c4afc","observation_id":"a7f5fe34-05a3-455b-a8f8-ae27ac47d5f1","resolution":{"observed_at":"2026-08-07T00:14:15.962839Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:16.021649Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:16.021649Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:204bdb9b0331b9182feb746ed76bc1a08d178b6ff65545cd58a0b3c2d55ee7a7","observation_id":"6edb996d-0360-4412-aed0-49ba9bc21b54","resolution":{"observed_at":"2026-08-07T00:14:16.021649Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0306026","last_updated":"2004-12-01T03:06:23Z","snapshot_observed_at":"2026-08-01T18:46:59.156750Z","submitted_at":"2003-06-02T06:33:08Z","title":"A class of compact dwarf galaxies from disruptive processes in galaxy clusters","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0306026","snapshot_observed_at":"2026-08-07T00:14:16.112012Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:16.112012Z"},"links":{"cited_paper":"/paper/astro-ph/0306026","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:f9d6a3f15a34d0c0442000f316b55bef952f4e6ece7c31363c534768f06bb686","observation_id":"9fd12de0-3b43-424a-9f5e-ef5166144d8a","resolution":{"observed_at":"2026-08-07T00:14:16.112012Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:16.180284Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:16.180284Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:7de048859575d5072dd9e6eb1d50c5bf357044e4934a35618e286897b3a478e1","observation_id":"7879181c-8e2d-42f7-84a8-7f7e675809d8","resolution":{"observed_at":"2026-08-07T00:14:16.180284Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1406.1397","last_updated":"2014-06-16T18:46:20Z","snapshot_observed_at":"2026-07-06T03:45:35.499800Z","submitted_at":"2014-06-05T14:22:03Z","title":"The colour-magnitude relation of Globular Clusters in Centaurus and Hydra - Constraints on star cluster self-enrichment with a link to massive Milky Way GCs","version":2},"cited_work":{"arxiv_id":"1406.1397","doi":null,"metadata_source":"pith","pith_arxiv_id":"1406.1397","snapshot_observed_at":"2026-08-07T00:14:32.110850Z","title":"The colour-magnitude relation of Globular Clusters in Centaurus and Hydra - Constraints on star cluster self-enrichment with a link to massive Milky Way GCs","venue":"astro-ph.GA","work_id":"e05809fd-030c-4e17-983a-6eceb41fa3ac","year":2014},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":101,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:16.249445Z"},"links":{"cited_paper":"/paper/1406.1397","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:2c82cbb59586d0a7f0b363539a1beb7d2793f3e14b4328bf8ebc5f9a7471247c","observation_id":"6199b4ef-b234-4682-9166-597ec6b2d7dd","resolution":{"observed_at":"2026-08-07T00:14:32.186727Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9702146","last_updated":"1997-02-17T19:08:34Z","snapshot_observed_at":"2026-07-07T01:15:55.239042Z","submitted_at":"1997-02-17T19:08:34Z","title":"On the Origin of Globular Cluster Systems in Elliptical and cD Galaxies","version":1},"cited_work":{"arxiv_id":"astro-ph/9702146","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/9702146","snapshot_observed_at":"2026-08-07T00:14:31.932131Z","title":"On the Origin of Globular Cluster Systems in Elliptical and cD Galaxies","venue":"astro-ph","work_id":"54ac1f1c-8af2-4fdc-9c12-881672436152","year":1997},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":102,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:16.330318Z"},"links":{"cited_paper":"/paper/astro-ph/9702146","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:1c7b4a55a1d020a66a74bd9e5800f0af770e10b27cc416a3b5a000d95c70b3b6","observation_id":"fea03ae2-9e35-4bd5-ac7e-142fc2341b76","resolution":{"observed_at":"2026-08-07T00:14:32.006321Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1807.02142","last_updated":"2018-07-05T18:35:10Z","snapshot_observed_at":"2026-07-06T06:48:36.957224Z","submitted_at":"2018-07-05T18:35:10Z","title":"Metallicity gradients in the globular cluster systems of early-type galaxies: In-situ and accreted components?","version":1},"cited_work":{"arxiv_id":"1807.02142","doi":null,"metadata_source":"pith","pith_arxiv_id":"1807.02142","snapshot_observed_at":"2026-08-07T00:14:31.733722Z","title":"Metallicity gradients in the globular cluster systems of early-type galaxies: In-situ and accreted components?","venue":"astro-ph.GA","work_id":"96b4c127-faf0-46a5-b571-8f95e0a28754","year":2018},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":103,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:16.398223Z"},"links":{"cited_paper":"/paper/1807.02142","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:ef498fd254aa2bb2fba94215679c5ada71e9990347e0f527452d467e45170322","observation_id":"95ca9bad-4b8c-47a5-9c13-502d6705e244","resolution":{"observed_at":"2026-08-07T00:14:31.814631Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1712.05410","last_updated":"2017-12-14T19:00:01Z","snapshot_observed_at":"2026-07-06T06:14:26.039309Z","submitted_at":"2017-12-14T19:00:01Z","title":"Intra-cluster Globular Clusters in a Simulated Galaxy Cluster","version":1},"cited_work":{"arxiv_id":"1712.05410","doi":null,"metadata_source":"pith","pith_arxiv_id":"1712.05410","snapshot_observed_at":"2026-08-07T00:14:31.596491Z","title":"Intra-cluster Globular Clusters in a Simulated Galaxy Cluster","venue":"astro-ph.GA","work_id":"58256716-38c7-4705-bb7d-3a22b866cafe","year":2017},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":104,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:16.465332Z"},"links":{"cited_paper":"/paper/1712.05410","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:499f2b2b98772d0db7c294226b2051c3292a868edf0fcfa02d1496c814f5bdfc","observation_id":"8a0ab588-4d7b-4d82-84ac-2994b8ba06be","resolution":{"observed_at":"2026-08-07T00:14:31.642035Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-07T00:14:16.560996Z","title":", keywords =","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":105,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:16.560996Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:53c62e7ec39ce5ffd35717df09ec1b950edd56b83fe596a9a54e9609a8bc504b","observation_id":"fe831e54-5882-4e06-8c9d-99c906b4edab","resolution":{"observed_at":"2026-08-07T00:14:16.560996Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1311.5411","last_updated":"2013-11-21T14:12:15Z","snapshot_observed_at":"2026-07-06T03:28:50.751448Z","submitted_at":"2013-11-21T14:12:15Z","title":"Automated data reduction workflows for astronomy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1311.5411","snapshot_observed_at":"2026-08-07T00:14:16.628979Z","title":"The ESO Reflex environment","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":106,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:16.628979Z"},"links":{"cited_paper":"/paper/1311.5411","citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:787d29cc2e8a1b2bf0f7b62840467fa6fa258bc53e56d70726ade304e5f39ed9","observation_id":"2aac36f2-cb14-46ac-8090-ea6e71849d74","resolution":{"observed_at":"2026-08-07T00:14:16.628979Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T00:14:16.695826Z","title":", keywords =","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc","version":1},"reference_index":107,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:16.695826Z"},"links":{"citing_paper":"/paper/2608.02730"},"observation_digest":"sha256:744d7e5cc61fce2de6a96b74d351fdd3e69aa5aa4a8f24b605f0a92649afa937","observation_id":"098d28f7-29e3-4f65-9910-0a22df7691a2","resolution":{"observed_at":"2026-08-07T00:14:16.695826Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2608.02730","last_updated":"2026-08-03T18:00:02Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-07T19:10:28.112453Z","submitted_at":"2026-08-03T18:00:02Z","title":"The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":1,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":93,"verified_exact":6,"verified_fuzzy":0},"total_outbound_references":163},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 100 of 163 outbound references and 0 inbound Pith citation observations for arXiv:2608.02730."}