{"as_of":"2026-08-13T15:11:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:6e0f40d60a59b8fa354eb496869e9cd38ab134c46f583ebcb7e2a9889c55582e","coverage":[{"denominator":111,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-04T22:14:30.404829Z","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":"2026-08-13T06:32:02.005865+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/2509.07470/citation-record","integrity":"/paper/2509.07470/integrity","json":"/paper/2509.07470/citation-record.json","paper":"/paper/2509.07470"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T22:14:21.485522Z","title":null,"venue":null,"work_id":null,"year":1978},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:21.485522Z"},"links":{"citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:85eeaf4846a65768954bcd5712958d075213fe56e1619924af2a319c198f694d","observation_id":"03b74d13-2f99-43b7-bf21-fc9f5ef149fa","resolution":{"observed_at":"2026-08-04T22:14:21.485522Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.03097","last_updated":"2018-04-09T16:51:59Z","snapshot_observed_at":"2026-07-06T06:32:29.028840Z","submitted_at":"2018-04-09T16:51:59Z","title":"The Connection between Galaxies and their Dark Matter Halos","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.03097","snapshot_observed_at":"2026-08-04T22:14:21.563305Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:21.563305Z"},"links":{"cited_paper":"/paper/1804.03097","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:ad73e9d0bf193a4e1315e4d7b88080dd807d4c16ba3dbd4808bcad8dc145a3de","observation_id":"db5a70b6-7b55-4ece-83a3-59ff9a913b80","resolution":{"observed_at":"2026-08-04T22:14:21.563305Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0203004","last_updated":"2002-12-06T01:44:56Z","snapshot_observed_at":"2026-07-07T00:25:18.276338Z","submitted_at":"2002-03-01T02:39:08Z","title":"The Structural Evolution of Substructure","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0203004","snapshot_observed_at":"2026-08-04T22:14:21.627315Z","title":"Hayashi, J","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:21.627315Z"},"links":{"cited_paper":"/paper/astro-ph/0203004","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:1b6b5d0dac9ceb513d193c65755b79f3ac05cf70eb11b6b1f3ac97f105acd870","observation_id":"eac3844d-5401-4d55-8483-8cfe57f1598d","resolution":{"observed_at":"2026-08-04T22:14:21.627315Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0002308","last_updated":"2000-02-17T09:18:50Z","snapshot_observed_at":"2026-08-08T22:16:18.582778Z","submitted_at":"2000-02-16T17:38:33Z","title":"Collisional versus Collisionless Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0002308","snapshot_observed_at":"2026-08-04T22:14:21.701783Z","title":"Moore, S","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:21.701783Z"},"links":{"cited_paper":"/paper/astro-ph/0002308","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:949fcb14c0374f8e480f2a4952af484a3f6306a2730c0f6023f7f394e5db3098","observation_id":"578d5b3e-113a-47ab-84d2-bf92ec14994c","resolution":{"observed_at":"2026-08-04T22:14:21.701783Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1203.3695","last_updated":"2012-03-16T13:08:31Z","snapshot_observed_at":"2026-08-12T16:19:33.257992Z","submitted_at":"2012-03-16T13:08:31Z","title":"SubHaloes going Notts: The SubHalo-Finder Comparison Project","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1203.3695","snapshot_observed_at":"2026-08-04T22:14:21.767556Z","title":"Onions, A","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:21.767556Z"},"links":{"cited_paper":"/paper/1203.3695","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:57b8bc33e9c90c93c0158ebc68ff04d5afcc917a23ee8a6070b27cb2b7780a53","observation_id":"9ffc3405-4b18-48c7-b798-e9d2b37121d3","resolution":{"observed_at":"2026-08-04T22:14:21.767556Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.10926","last_updated":"2026-05-11T17:50:24Z","snapshot_observed_at":"2026-08-03T01:48:29.894230Z","submitted_at":"2023-08-21T18:00:00Z","title":"Symfind: Addressing the Fragility of Subhalo Finders and Revealing the Durability of Subhalos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.10926","snapshot_observed_at":"2026-08-04T22:14:21.827145Z","title":"Mansfield, E","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:21.827145Z"},"links":{"cited_paper":"/paper/2308.10926","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:453c2c0409a63dd6204d4b6903b1b30a1f883b3870b4a35788e5d6fb2eb189a3","observation_id":"a52ed224-9226-49c5-8096-caef38512302","resolution":{"observed_at":"2026-08-04T22:14:21.827145Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.22742","last_updated":"2025-08-13T10:04:32Z","snapshot_observed_at":"2026-08-13T05:31:09.239830Z","submitted_at":"2025-05-28T18:03:23Z","title":"Survivors and Zombies: The Quenching and Disruption of Satellites around Milky Way Analogs","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.22742","snapshot_observed_at":"2026-08-04T22:14:21.922039Z","title":"Pathak, C","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:21.922039Z"},"links":{"cited_paper":"/paper/2505.22742","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:e87b33b34e1edcecf019a95ae457948f9b77a499e4e4ed99062ef79567942387","observation_id":"68624a0d-2bb2-453f-86fd-43d391d817fa","resolution":{"observed_at":"2026-08-04T22:14:21.922039Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1103.0007","last_updated":"2011-05-13T15:41:38Z","snapshot_observed_at":"2026-08-07T08:29:50.029418Z","submitted_at":"2011-02-28T21:00:02Z","title":"Too big to fail? The puzzling darkness of massive Milky Way subhaloes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1103.0007","snapshot_observed_at":"2026-08-04T22:14:22.019468Z","title":"Boylan-Kolchin, J","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:22.019468Z"},"links":{"cited_paper":"/paper/1103.0007","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:7266eb8997d99e338ab87f224e8489ede6582aa5c04c029da43fc577fab1a13b","observation_id":"fc8986d1-9ecf-407b-9183-cd52cd8ae5ac","resolution":{"observed_at":"2026-08-04T22:14:22.019468Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0810.2100","last_updated":"2008-10-14T07:33:25Z","snapshot_observed_at":"2026-08-08T05:43:20.065908Z","submitted_at":"2008-10-13T16:05:47Z","title":"High-Resolution Rotation Curves and Galaxy Mass Models from THINGS","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0810.2100","snapshot_observed_at":"2026-08-04T22:14:22.087366Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:22.087366Z"},"links":{"cited_paper":"/paper/0810.2100","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:2f53d457fcb72a8e71d2fc426431cd338b469613d37b891edaef7795c68a506a","observation_id":"2f82ecf1-4d34-4567-80f6-7821dea5b263","resolution":{"observed_at":"2026-08-04T22:14:22.087366Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1011.2777","last_updated":"2011-04-15T14:58:26Z","snapshot_observed_at":"2026-07-06T02:19:05.048681Z","submitted_at":"2010-11-11T21:23:46Z","title":"The central slope of dark matter cores in dwarf galaxies: Simulations vs. THINGS","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1011.2777","snapshot_observed_at":"2026-08-04T22:14:22.190322Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:22.190322Z"},"links":{"cited_paper":"/paper/1011.2777","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:cb864dd96642d1f06c3c48e7c2dab88d2fa0dafd020d3e05dca8e5f9d99c67fe","observation_id":"fe04f7a7-65d7-490e-abe7-26b4027495a1","resolution":{"observed_at":"2026-08-04T22:14:22.190322Z","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":"2026-08-04T22:14:22.286576Z","title":"Moore, Evidence against dissipation-less dark matter from observations of galaxy haloes, Nature370(1994) 629","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:22.286576Z"},"links":{"citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:04140b1641ca52df92ae626fbfaa5ed1a94d14337cc70074c6a6b0b71ef39ed0","observation_id":"cb2bc591-b2ce-404f-85d6-8e7379a7e6e2","resolution":{"observed_at":"2026-08-04T22:14:22.286576Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9402004","last_updated":"1994-02-02T02:03:31Z","snapshot_observed_at":"2026-08-07T14:13:27.662655Z","submitted_at":"1994-02-02T02:03:31Z","title":"Observational and Theoretical Constraints on Singular Dark Matter Halos","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9402004","snapshot_observed_at":"2026-08-04T22:14:22.408004Z","title":null,"venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:22.408004Z"},"links":{"cited_paper":"/paper/astro-ph/9402004","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:18ee79940c48527cc70a6b8b02c3288aca2fce0dc57700f17ec864690b3a184a","observation_id":"ae7cd930-7137-45ed-8d17-c3dae928bc75","resolution":{"observed_at":"2026-08-04T22:14:22.408004Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.14151","last_updated":"2022-09-28T15:01:54Z","snapshot_observed_at":"2026-08-13T14:17:40.231126Z","submitted_at":"2022-09-28T15:01:54Z","title":"Review of solutions to the Cusp-core problem of the $\\Lambda$CDM Model","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.14151","snapshot_observed_at":"2026-08-04T22:14:22.594758Z","title":"Del Popolo and M","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:22.594758Z"},"links":{"cited_paper":"/paper/2209.14151","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:50d58187866fac6fd8228189faedc51cd4f5930feaac62f9ba279fa394ccb374","observation_id":"89b872a5-589f-403f-8d29-09bf92b3d1cb","resolution":{"observed_at":"2026-08-04T22:14:22.594758Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.01437","last_updated":"2015-07-09T00:02:11Z","snapshot_observed_at":"2026-07-06T04:14:13.016827Z","submitted_at":"2015-04-06T23:11:21Z","title":"The unexpected diversity of dwarf galaxy rotation curves","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.01437","snapshot_observed_at":"2026-08-04T22:14:22.777631Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:22.777631Z"},"links":{"cited_paper":"/paper/1504.01437","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:59e515becd51dfb397b8c68cbfdd90454e560c722243c1a3a80983877410431e","observation_id":"ca97d847-2911-481a-b2f7-3848b69ae602","resolution":{"observed_at":"2026-08-04T22:14:22.777631Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1207.0007","last_updated":"2012-12-04T13:48:05Z","snapshot_observed_at":"2026-07-06T02:50:58.658876Z","submitted_at":"2012-06-29T20:00:04Z","title":"Baryons Matter: Why Luminous Satellite Galaxies Have Reduced Central Masses","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1207.0007","snapshot_observed_at":"2026-08-04T22:14:22.965038Z","title":"Zolotov, A","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:22.965038Z"},"links":{"cited_paper":"/paper/1207.0007","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:417aa6c844a1d102377fc955c143f0b552b355a180546283083e238cf1704d10","observation_id":"1eb5c3c3-5a40-4be1-8634-95e97c5fed72","resolution":{"observed_at":"2026-08-04T22:14:22.965038Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1404.3674","last_updated":"2014-04-11T19:00:10Z","snapshot_observed_at":"2026-07-06T03:41:10.318277Z","submitted_at":"2014-04-11T19:00:10Z","title":"A unified solution to the small scale problems of the $\\Lambda$CDM model","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1404.3674","snapshot_observed_at":"2026-08-04T22:14:23.145267Z","title":"Del Popolo, J","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:23.145267Z"},"links":{"cited_paper":"/paper/1404.3674","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:6aaf50742969d9d3c2ca9d8f6c421bb17460b6079a65487d2a20c2daf370f0ae","observation_id":"cba7e913-65dd-41be-b66f-9610fd1b732c","resolution":{"observed_at":"2026-08-04T22:14:23.145267Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0605672","last_updated":"2006-05-26T17:19:44Z","snapshot_observed_at":"2026-08-08T06:26:15.857516Z","submitted_at":"2006-05-26T17:19:44Z","title":"Cosmological puzzle resolved by stellar feedback in high redshift galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0605672","snapshot_observed_at":"2026-08-04T22:14:23.289477Z","title":"Mashchenko, H","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:23.289477Z"},"links":{"cited_paper":"/paper/astro-ph/0605672","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:0a122c3ecb6ae1c97a2e66f64afb65d757ec83a5b164fff791f4607d1b39ca9a","observation_id":"a3a546e4-55bd-4db7-a201-fe71eab4c0a1","resolution":{"observed_at":"2026-08-04T22:14:23.289477Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0711.4803","last_updated":"2007-11-29T19:31:38Z","snapshot_observed_at":"2026-07-06T01:35:50.241998Z","submitted_at":"2007-11-29T19:31:38Z","title":"Stellar Feedback in Dwarf Galaxy Formation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0711.4803","snapshot_observed_at":"2026-08-04T22:14:23.414113Z","title":"Mashchenko, J","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:23.414113Z"},"links":{"cited_paper":"/paper/0711.4803","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:7b0b49451d65ce797b63ebf518a54eb31dc8a7805928efcfe9db57455256a572","observation_id":"f1e252cc-9f1a-4203-a140-c531078acd95","resolution":{"observed_at":"2026-08-04T22:14:23.414113Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1002.3376","last_updated":"2010-05-28T18:02:56Z","snapshot_observed_at":"2026-08-13T01:59:53.490881Z","submitted_at":"2010-02-17T21:05:20Z","title":"The impact of dark matter cusps and cores on the satellite galaxy population around spiral galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1002.3376","snapshot_observed_at":"2026-08-04T22:14:23.560010Z","title":"Peñarrubia, A","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:23.560010Z"},"links":{"cited_paper":"/paper/1002.3376","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:c761e8de17e7020f022f6e59756620f58299e3f87f2f34aea9614a234930c8eb","observation_id":"b665a9e1-c774-430e-a704-4ca876d28313","resolution":{"observed_at":"2026-08-04T22:14:23.560010Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.01131","last_updated":"2022-12-26T07:06:25Z","snapshot_observed_at":"2026-08-13T14:13:54.730002Z","submitted_at":"2022-10-03T18:00:01Z","title":"Dark matter halo cores and the tidal survival of Milky Way satellites","version":2},"cited_work":{"arxiv_id":"2210.01131","doi":null,"metadata_source":"pith","pith_arxiv_id":"2210.01131","snapshot_observed_at":"2026-08-04T22:14:35.718237Z","title":"Dark matter halo cores and the tidal survival of Milky Way satellites","venue":"astro-ph.GA","work_id":"4f2929f3-1a4d-42f1-bb4e-7273f59c6323","year":2022},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:23.683397Z"},"links":{"cited_paper":"/paper/2210.01131","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:b259414b001f53062ae8f3cecd0a2ad7139385c31ad1be7978fa23a9bfa2ccb0","observation_id":"d636b2aa-456a-4c35-b190-9a981090ff21","resolution":{"observed_at":"2026-08-04T22:14:35.804491Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2505.01620","last_updated":"2026-07-29T17:18:14Z","snapshot_observed_at":"2026-08-13T13:50:17.204195Z","submitted_at":"2025-05-02T22:54:28Z","title":"Mass-morphology relation of TNG50 galaxies","version":2},"cited_work":{"arxiv_id":"2505.01620","doi":null,"metadata_source":"pith","pith_arxiv_id":"2505.01620","snapshot_observed_at":"2026-08-04T22:14:35.578339Z","title":"Mass-morphology relation of TNG50 galaxies","venue":"astro-ph.GA","work_id":"d9be5304-74d3-45e8-95ad-935deb6d5b5d","year":2025},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:23.817048Z"},"links":{"cited_paper":"/paper/2505.01620","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:024980e67aeede936120582143fb05dc51f38b3abc93379886bb2d3b58227534","observation_id":"654cf985-278e-417d-945c-4ad2dccbff63","resolution":{"observed_at":"2026-08-04T22:14:35.626194Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9912166","last_updated":"2006-03-04T15:00:49Z","snapshot_observed_at":"2026-08-12T20:00:16.927727Z","submitted_at":"1999-12-08T15:34:35Z","title":"Formation of Disk Galaxies: Warm Dark Matter and the Angular Momentum problem","version":2},"cited_work":{"arxiv_id":"astro-ph/9912166","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/9912166","snapshot_observed_at":"2026-08-04T22:14:35.398961Z","title":"Formation of Disk Galaxies: Warm Dark Matter and the Angular Momentum problem","venue":"astro-ph","work_id":"da3657a7-f077-4dc6-82d9-8a03788ae01b","year":1999},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:23.918904Z"},"links":{"cited_paper":"/paper/astro-ph/9912166","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:bbc46c149870ff8867ad074a737bfc730da071efb5edecf40e88f99335334f55","observation_id":"75400ff7-3b22-4994-b6f4-38160d11ec47","resolution":{"observed_at":"2026-08-04T22:14:35.458428Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0002495","last_updated":"2000-02-26T20:50:00Z","snapshot_observed_at":"2026-07-07T00:10:15.760445Z","submitted_at":"2000-02-26T20:50:00Z","title":"Fluid Dark Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0002495","snapshot_observed_at":"2026-08-04T22:14:24.012158Z","title":null,"venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:24.012158Z"},"links":{"cited_paper":"/paper/astro-ph/0002495","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:06b51ddb17ec81a1807623ac67dbb190dbea96800c31ef931186b9c13bd5ea60","observation_id":"2fb65082-9e5d-48e0-bbe9-5d6761c51a4a","resolution":{"observed_at":"2026-08-04T22:14:24.012158Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0003018","last_updated":"2000-03-02T04:58:24Z","snapshot_observed_at":"2026-07-07T00:10:15.760445Z","submitted_at":"2000-03-02T04:58:24Z","title":"Repulsive Dark Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0003018","snapshot_observed_at":"2026-08-04T22:14:24.116122Z","title":"Goodman, Repulsive dark matter,na5(2000) 103 [astro-ph/0003018]","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:24.116122Z"},"links":{"cited_paper":"/paper/astro-ph/0003018","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:ce8044651940f836ca2de2f75ad5cd096ef793a76f32d0230a099e58e9b3b398","observation_id":"fe25c309-c009-48c9-a277-afeeeb3f93a9","resolution":{"observed_at":"2026-08-04T22:14:24.116122Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0003365","last_updated":"2000-03-26T22:50:24Z","snapshot_observed_at":"2026-07-07T00:10:35.167895Z","submitted_at":"2000-03-24T00:29:30Z","title":"Cold and Fuzzy Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0003365","snapshot_observed_at":"2026-08-04T22:14:24.202941Z","title":null,"venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:24.202941Z"},"links":{"cited_paper":"/paper/astro-ph/0003365","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:012d4a2f03660fb0cf4b6164a632e1c84cbcd9f1f2357321b85a956756371511","observation_id":"9560a45f-492c-4bb6-9f22-bc081f20353d","resolution":{"observed_at":"2026-08-04T22:14:24.202941Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0005206","last_updated":"2000-10-12T18:38:57Z","snapshot_observed_at":"2026-07-07T00:11:13.294340Z","submitted_at":"2000-05-09T20:11:53Z","title":"Decaying Cold Dark Matter Model and Small-Scale Power","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0005206","snapshot_observed_at":"2026-08-04T22:14:24.333510Z","title":"Cen,Decaying Cold Dark Matter Model and Small-Scale Power,Astrophys","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:24.333510Z"},"links":{"cited_paper":"/paper/astro-ph/0005206","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:66efd5acfeee5c137b954418283703089cb7d4053712dd6003b49954b497171e","observation_id":"51c41c37-61cb-4609-b2ea-bf50759baf6c","resolution":{"observed_at":"2026-08-04T22:14:24.333510Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0005210","last_updated":"2000-08-29T19:52:09Z","snapshot_observed_at":"2026-08-07T14:39:57.091122Z","submitted_at":"2000-05-10T20:27:37Z","title":"Annihilating Cold Dark Matter","version":2},"cited_work":{"arxiv_id":"astro-ph/0005210","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0005210","snapshot_observed_at":"2026-08-04T22:14:35.194239Z","title":"Annihilating Cold Dark Matter","venue":"astro-ph","work_id":"70feb33a-5220-465a-b576-4122c3060fc7","year":2000},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:24.462713Z"},"links":{"cited_paper":"/paper/astro-ph/0005210","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:4f4224a1f9b48aefef1bc418e12eb1ca5b116d930dacd164af762c0f7cdeca84","observation_id":"5a7ea83e-2531-4f13-8c95-0082a8c45a71","resolution":{"observed_at":"2026-08-04T22:14:35.255860Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9909386","last_updated":"2000-02-28T15:13:46Z","snapshot_observed_at":"2026-08-06T18:45:17.409953Z","submitted_at":"1999-09-23T00:12:32Z","title":"Observational evidence for self-interacting cold dark matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9909386","snapshot_observed_at":"2026-08-04T22:14:24.555151Z","title":null,"venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:24.555151Z"},"links":{"cited_paper":"/paper/astro-ph/9909386","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:379d01d0f1cf3b28447a19cbb1a7f398b55b700c8d47ad32d678887877d151da","observation_id":"10ab2f2b-3c31-4fcb-94a9-049b274d9d24","resolution":{"observed_at":"2026-08-04T22:14:24.555151Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0304292","last_updated":"2003-07-27T20:10:36Z","snapshot_observed_at":"2026-07-07T00:32:43.377098Z","submitted_at":"2003-04-15T21:17:52Z","title":"Halo Substructure And The Power Spectrum","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0304292","snapshot_observed_at":"2026-08-04T22:14:24.648553Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:24.648553Z"},"links":{"cited_paper":"/paper/astro-ph/0304292","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:53c05e0dca515133714d48a8d7925a4f4da5991b28b4c1fb7d05db36de04194f","observation_id":"3de3978b-f07c-4fbe-b139-25c252c9b9df","resolution":{"observed_at":"2026-08-04T22:14:24.648553Z","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":"2026-08-04T22:14:24.781108Z","title":"Milgrom,A modification of the Newtonian dynamics - Implications for galaxies., Astrophys","venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:24.781108Z"},"links":{"citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:e7532dbdd390b395bd75d22e57370d5b9655401100d5d354d9aa978c5f2ff8a6","observation_id":"ca817071-4076-4345-8796-a36510fcbe3d","resolution":{"observed_at":"2026-08-04T22:14:24.781108Z","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":"2026-08-04T22:14:24.868804Z","title":"Milgrom, A modification of the Newtonian dynamics as a possible alternative to the hidden mass hypothesis., Astrophys","venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:24.868804Z"},"links":{"citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:9b35f2ae147d0873a26dd02fb2b04d6f327ea351c83758f857965b58d6aa5b51","observation_id":"a6824610-1e56-4b82-9f71-ff08f5502b60","resolution":{"observed_at":"2026-08-04T22:14:24.868804Z","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":"2026-08-04T22:14:24.960897Z","title":null,"venue":null,"work_id":null,"year":1970},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:24.960897Z"},"links":{"citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:316477cf78c06f35a05511005f3b95fffbc2ec2a35af2c1f7317c94e9ec46472","observation_id":"f3a81669-4b36-4f3c-8a26-45e11d52dee5","resolution":{"observed_at":"2026-08-04T22:14:24.960897Z","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":"2026-08-04T22:14:25.079884Z","title":null,"venue":null,"work_id":null,"year":1980},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:25.079884Z"},"links":{"citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:5aecd41cbcebcdb1deda70cff5eacad6f949855a22a16e972245116af8d60f22","observation_id":"632fd5dd-a96d-43b6-a7e7-f2dbf2788c3e","resolution":{"observed_at":"2026-08-04T22:14:25.079884Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0812.1205","last_updated":"2009-05-21T19:41:47Z","snapshot_observed_at":"2026-08-03T09:06:19.016196Z","submitted_at":"2008-12-05T19:39:54Z","title":"Dark torsion as the cosmic speed-up","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0812.1205","snapshot_observed_at":"2026-08-04T22:14:25.166192Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:25.166192Z"},"links":{"cited_paper":"/paper/0812.1205","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:aca736dffd1f795e236100d072b6ed7cc4a573c29a8ca8c84897f3a1ee51e951","observation_id":"355ed526-14a5-4026-904d-f8cdbad3dbee","resolution":{"observed_at":"2026-08-04T22:14:25.166192Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1010.2215","last_updated":"2010-12-20T16:49:16Z","snapshot_observed_at":"2026-07-06T02:16:45.493056Z","submitted_at":"2010-10-11T20:02:15Z","title":"f(T) gravity mimicking dynamical dark energy. Background and perturbation analysis","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1010.2215","snapshot_observed_at":"2026-08-04T22:14:25.225660Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:25.225660Z"},"links":{"cited_paper":"/paper/1010.2215","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:81c32fc797fe5b16431f08d9b20084b440fedac648cf248ebbd84ed30322a1d4","observation_id":"f1976d3b-c1c7-4a2c-815c-033717b4fa94","resolution":{"observed_at":"2026-08-04T22:14:25.225660Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0103102","last_updated":"2001-03-09T10:25:29Z","snapshot_observed_at":"2026-07-07T00:17:00.753523Z","submitted_at":"2001-03-07T04:32:43Z","title":"Mass Density Profiles of LSB Galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0103102","snapshot_observed_at":"2026-08-04T22:14:25.284731Z","title":null,"venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:25.284731Z"},"links":{"cited_paper":"/paper/astro-ph/0103102","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:76b3bb4b2fd3be9e38d9a987a9c342240d73921ec2d9c37cf0a606b6cff62906","observation_id":"28d99e4e-dd95-4adc-9e03-f21a1a25e69a","resolution":{"observed_at":"2026-08-04T22:14:25.284731Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0212102","last_updated":"2002-12-05T11:55:36Z","snapshot_observed_at":"2026-07-07T00:30:05.972335Z","submitted_at":"2002-12-04T15:27:30Z","title":"Simulating Observations of Dark Matter Dominated Galaxies: Towards the Optimal Halo Profile","version":2},"cited_work":{"arxiv_id":"astro-ph/0212102","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0212102","snapshot_observed_at":"2026-08-04T22:14:34.961749Z","title":"Simulating Observations of Dark Matter Dominated Galaxies: Towards the Optimal Halo Profile","venue":"astro-ph","work_id":"14ca8ff3-5baa-4ff1-97cb-cea63d6dfb86","year":2002},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:25.394350Z"},"links":{"cited_paper":"/paper/astro-ph/0212102","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:3e292abc9f779c77c27c4b58639588c815f5eef247c9c2377c6a7fba297f7129","observation_id":"bbed94c7-fc65-4b16-81ca-2ad7cbaa0eb1","resolution":{"observed_at":"2026-08-04T22:14:35.021477Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0201544","last_updated":"2003-01-14T11:58:33Z","snapshot_observed_at":"2026-07-07T00:24:50.595459Z","submitted_at":"2002-01-31T18:35:28Z","title":"The Inner Structure of LambdaCDM Halos I: A Numerical Convergence Study","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0201544","snapshot_observed_at":"2026-08-04T22:14:25.440785Z","title":"Power, J","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:25.440785Z"},"links":{"cited_paper":"/paper/astro-ph/0201544","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:15402d7751c1296fb08edf6080e7537d92c8c5d15720887bf3d405ed33c9b42b","observation_id":"7cb44542-01f3-4fd9-8ace-16f32cee3a8b","resolution":{"observed_at":"2026-08-04T22:14:25.440785Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1306.0898","last_updated":"2013-10-07T18:43:52Z","snapshot_observed_at":"2026-07-06T03:15:05.518065Z","submitted_at":"2013-06-04T20:00:01Z","title":"The dependence of dark matter profiles on the stellar to halo mass ratio: a prediction for cusps vs cores","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1306.0898","snapshot_observed_at":"2026-08-04T22:14:25.482998Z","title":"Di Cintio, C","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:25.482998Z"},"links":{"cited_paper":"/paper/1306.0898","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:35a68394944a73ffd388ce70d3754db3f66b422c225f46cf6321aa69b21e270a","observation_id":"621b7e36-76a6-4943-aee0-34f5c9a23239","resolution":{"observed_at":"2026-08-04T22:14:25.482998Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1507.03590","last_updated":"2019-05-06T11:53:11Z","snapshot_observed_at":"2026-07-06T04:23:42.810602Z","submitted_at":"2015-07-13T20:00:32Z","title":"NIHAO IV: Core creation and destruction in dark matter density profiles across cosmic time","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1507.03590","snapshot_observed_at":"2026-08-04T22:14:25.538993Z","title":"Tollet, A","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:25.538993Z"},"links":{"cited_paper":"/paper/1507.03590","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:4a9d23be0283d31adee1d52c3b2c0ce9bfc7ebf8c6accaf68b704e2d834cb8de","observation_id":"de6d4c86-fd25-49b8-9f01-15fa576ac21d","resolution":{"observed_at":"2026-08-04T22:14:25.538993Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1507.02282","last_updated":"2015-09-23T22:17:45Z","snapshot_observed_at":"2026-07-06T04:23:14.183048Z","submitted_at":"2015-07-08T20:00:38Z","title":"The Impact of Baryonic Physics on the Structure of Dark Matter Halos: the View from the FIRE Cosmological Simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1507.02282","snapshot_observed_at":"2026-08-04T22:14:25.601787Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:25.601787Z"},"links":{"cited_paper":"/paper/1507.02282","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:33aac3656b21bc41d05499a1ea433bbf617aeb7f7b587108cd76a811bf51b92b","observation_id":"5cb0de0c-0d2e-4f1f-924d-4c00a9d0b3d5","resolution":{"observed_at":"2026-08-04T22:14:25.601787Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.13055","last_updated":"2024-01-08T17:56:25Z","snapshot_observed_at":"2026-08-13T05:45:07.676147Z","submitted_at":"2023-10-19T18:00:03Z","title":"The formation of cores in galaxies across cosmic time -- the existence of cores is not in tension with the LCDM paradigm","version":2},"cited_work":{"arxiv_id":"2310.13055","doi":null,"metadata_source":"pith","pith_arxiv_id":"2310.13055","snapshot_observed_at":"2026-08-04T22:14:34.733928Z","title":"The formation of cores in galaxies across cosmic time -- the existence of cores is not in tension with the LCDM paradigm","venue":"astro-ph.GA","work_id":"0df2882e-225a-49fe-b827-50557342e4a2","year":2023},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:25.649425Z"},"links":{"cited_paper":"/paper/2310.13055","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:0b32e68f8f66e217414190b5fff80197a9a8bafe4171419d9cd2ae181200b86b","observation_id":"4a26859c-969f-46f0-80be-83c6b9d7eadb","resolution":{"observed_at":"2026-08-04T22:14:34.798807Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1508.04143","last_updated":"2016-05-05T08:25:22Z","snapshot_observed_at":"2026-07-06T04:26:57.065710Z","submitted_at":"2015-08-17T20:07:34Z","title":"Dark matter cores all the way down","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1508.04143","snapshot_observed_at":"2026-08-04T22:14:25.688607Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:25.688607Z"},"links":{"cited_paper":"/paper/1508.04143","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:179afa51d5484888f0eab5e30eb6ebefbb9b264762683563fedf680b16794c2a","observation_id":"f5256d46-2f29-468b-8351-2ce16c8ce3c2","resolution":{"observed_at":"2026-08-04T22:14:25.688607Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.03635","last_updated":"2019-05-30T15:38:59Z","snapshot_observed_at":"2026-08-12T07:48:59.365239Z","submitted_at":"2018-10-08T18:01:20Z","title":"No cores in dark matter-dominated dwarf galaxies with bursty star formation histories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.03635","snapshot_observed_at":"2026-08-04T22:14:25.783154Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:25.783154Z"},"links":{"cited_paper":"/paper/1810.03635","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:e87c17957fef336503e21614a7522e56f72d14429202fd6a103445df9334b996","observation_id":"a0d5adfd-f79d-417c-80db-d110d5261681","resolution":{"observed_at":"2026-08-04T22:14:25.783154Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.12437","last_updated":"2019-07-05T19:01:04Z","snapshot_observed_at":"2026-08-06T22:24:54.189449Z","submitted_at":"2018-11-29T19:14:48Z","title":"Subhalo destruction in the Apostle and Auriga simulations","version":2},"cited_work":{"arxiv_id":"1811.12437","doi":null,"metadata_source":"pith","pith_arxiv_id":"1811.12437","snapshot_observed_at":"2026-08-04T22:14:34.543616Z","title":"Subhalo destruction in the Apostle and Auriga simulations","venue":"astro-ph.GA","work_id":"b114668f-ed98-4dd6-a479-448b03d084a7","year":2018},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:25.828427Z"},"links":{"cited_paper":"/paper/1811.12437","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:b22471d95477617c7a7dc188be2616682e43a17f1cc5580075af572b0d734d34","observation_id":"55aef8c6-0b85-4cb8-82c8-05b861d715ef","resolution":{"observed_at":"2026-08-04T22:14:34.615127Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2004.06008","last_updated":"2022-09-14T12:58:00Z","snapshot_observed_at":"2026-08-05T07:11:48.584526Z","submitted_at":"2020-04-13T15:32:00Z","title":"Cosmological simulations of the same spiral galaxy: the impact of baryonic physics","version":2},"cited_work":{"arxiv_id":"2004.06008","doi":null,"metadata_source":"pith","pith_arxiv_id":"2004.06008","snapshot_observed_at":"2026-08-04T22:14:34.462451Z","title":"Cosmological simulations of the same spiral galaxy: the impact of baryonic physics","venue":"astro-ph.GA","work_id":"fe4eaaf2-87e9-4aa5-a168-b0b1c8aa774e","year":2020},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:25.888776Z"},"links":{"cited_paper":"/paper/2004.06008","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:4566ace02fc3714e024dd1bf8b12b67e1072a51cd03d6ef53eff6e59e7d24a0c","observation_id":"2258ce61-a2c8-4970-a48b-92c77fef6a17","resolution":{"observed_at":"2026-08-04T22:14:34.506778Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0806.4381","last_updated":"2008-10-08T21:39:55Z","snapshot_observed_at":"2026-07-06T01:41:35.334177Z","submitted_at":"2008-06-26T23:54:33Z","title":"Hundreds of Milky Way Satellites? Luminosity Bias in the Satellite Luminosity Function","version":2},"cited_work":{"arxiv_id":"0806.4381","doi":null,"metadata_source":"pith","pith_arxiv_id":"0806.4381","snapshot_observed_at":"2026-08-04T22:14:34.336448Z","title":"Hundreds of Milky Way Satellites? Luminosity Bias in the Satellite Luminosity Function","venue":"astro-ph","work_id":"0689057b-9483-42b0-b88f-122a4b1ca311","year":2008},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:25.957391Z"},"links":{"cited_paper":"/paper/0806.4381","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:e6b1658ea85b8988ebaacb17bae82612a034aba61e4537427f4cc80c6e8f2613","observation_id":"4f7052ff-28dc-47ce-8440-a2a182c8e9a7","resolution":{"observed_at":"2026-08-04T22:14:34.389406Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1204.1562","last_updated":"2012-05-05T00:11:37Z","snapshot_observed_at":"2026-07-06T02:45:53.370955Z","submitted_at":"2012-04-06T20:54:59Z","title":"The observed properties of dwarf galaxies in and around the Local Group","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1204.1562","snapshot_observed_at":"2026-08-04T22:14:26.030796Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:26.030796Z"},"links":{"cited_paper":"/paper/1204.1562","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:466db027c09950783563c5c68097027c839e1fc4be31d2a493832e6255c1cee5","observation_id":"d8fe9d9c-5280-413f-9c85-5b7e7cc52331","resolution":{"observed_at":"2026-08-04T22:14:26.030796Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1607.06479","last_updated":"2016-07-21T20:04:33Z","snapshot_observed_at":"2026-08-04T22:23:59.172058Z","submitted_at":"2016-07-21T20:04:33Z","title":"The cold dark matter content of Galactic dwarf spheroidals: no cores, no failures, no problem","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1607.06479","snapshot_observed_at":"2026-08-04T22:14:26.109625Z","title":"Fattahi, J","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:26.109625Z"},"links":{"cited_paper":"/paper/1607.06479","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:a884b40dc0145d4f7e223f98815167aee948cd2b00b9838c226f4db7dedf2289","observation_id":"69ebc8bf-8f2a-4925-813d-acda47bd23d9","resolution":{"observed_at":"2026-08-04T22:14:26.109625Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.10578","last_updated":"2021-06-28T10:19:06Z","snapshot_observed_at":"2026-08-05T04:50:56.950269Z","submitted_at":"2020-09-22T14:39:37Z","title":"Introducing the NewHorizon simulation: Galaxy properties with resolved internal dynamics across cosmic time","version":4},"cited_work":{"arxiv_id":"2009.10578","doi":null,"metadata_source":"pith","pith_arxiv_id":"2009.10578","snapshot_observed_at":"2026-08-04T22:14:34.286970Z","title":"Introducing the NewHorizon simulation: Galaxy properties with resolved internal dynamics across cosmic time","venue":"astro-ph.GA","work_id":"37aa766b-8533-4453-9c04-186605b3666b","year":2020},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:26.146015Z"},"links":{"cited_paper":"/paper/2009.10578","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:6d949fddcbc273e419e05d52148c9a3538413b10647be4920da4564a50641e95","observation_id":"2ab6ed86-4695-47a1-8d3c-ab924b822c7d","resolution":{"observed_at":"2026-08-04T22:14:34.308141Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1610.01159","last_updated":"2017-01-11T11:57:37Z","snapshot_observed_at":"2026-08-10T00:14:26.690521Z","submitted_at":"2016-10-04T20:00:01Z","title":"The Auriga Project: the properties and formation mechanisms of disc galaxies across cosmic time","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.01159","snapshot_observed_at":"2026-08-04T22:14:26.214376Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:26.214376Z"},"links":{"cited_paper":"/paper/1610.01159","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:927f7b334786411146eb7c7f1078b13671a7b56b584178dafb47964d1b264cfc","observation_id":"4a0f07db-fecf-4662-8707-ce37971de69b","resolution":{"observed_at":"2026-08-04T22:14:26.214376Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.06189","last_updated":"2023-03-30T16:53:09Z","snapshot_observed_at":"2026-08-13T13:04:04.269311Z","submitted_at":"2023-01-15T21:00:13Z","title":"Cosmological simulations of the same spiral galaxy: connecting the dark matter distribution of the host halo with the subgrid baryonic physics","version":2},"cited_work":{"arxiv_id":"2301.06189","doi":null,"metadata_source":"pith","pith_arxiv_id":"2301.06189","snapshot_observed_at":"2026-08-04T22:14:34.193675Z","title":"Cosmological simulations of the same spiral galaxy: connecting the dark matter distribution of the host halo with the subgrid baryonic physics","venue":"astro-ph.CO","work_id":"1a0b103c-8f4d-4f67-bfa1-99afc9495af6","year":2023},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:26.284339Z"},"links":{"cited_paper":"/paper/2301.06189","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:584ec60f7d68d26ed09bdf0b7c4f8d0ffe22fb970f76b897ff3df0487fc0457a","observation_id":"fc813ea5-7017-47e3-bcd1-606e9329f4e3","resolution":{"observed_at":"2026-08-04T22:14:34.232846Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1602.05957","last_updated":"2016-08-08T19:54:37Z","snapshot_observed_at":"2026-08-08T11:03:42.984154Z","submitted_at":"2016-02-18T21:00:02Z","title":"Reconciling dwarf galaxies with LCDM cosmology: Simulating a realistic population of satellites around a Milky Way-mass galaxy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.05957","snapshot_observed_at":"2026-08-04T22:14:26.335029Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:26.335029Z"},"links":{"cited_paper":"/paper/1602.05957","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:c3d3596ec9685c1731e19ed279ae4f30c88437b073c20b9ac20679505e8bde66","observation_id":"2ae33934-bbfb-4034-bfaf-3c75236570ce","resolution":{"observed_at":"2026-08-04T22:14:26.335029Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0111367","last_updated":"2001-11-19T18:11:54Z","snapshot_observed_at":"2026-07-07T00:23:16.895347Z","submitted_at":"2001-11-19T18:11:54Z","title":"Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0111367","snapshot_observed_at":"2026-08-04T22:14:26.376812Z","title":"Teyssier, Cosmological hydrodynamics with adaptive mesh refinement: a new high resolution code called ramses, Astron","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:26.376812Z"},"links":{"cited_paper":"/paper/astro-ph/0111367","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:a7e6049208ab67ff9621aaf0dd8ee1c5e43f8249755cfa325436df70b8b93667","observation_id":"c61627ae-b7ee-4a1d-945e-9882ae53e971","resolution":{"observed_at":"2026-08-04T22:14:26.376812Z","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":"2026-08-04T22:14:26.449232Z","title":"MUSIC: MUlti-Scale Initial Conditions","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:26.449232Z"},"links":{"citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:d7ce189c6a02105f2d9f4b238c88a713d237e04430cb8b44a65f34eac140c95c","observation_id":"642a7e18-cae7-44ea-a4c6-93ab08e0548e","resolution":{"observed_at":"2026-08-04T22:14:26.449232Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.4318","last_updated":"2014-12-05T16:27:42Z","snapshot_observed_at":"2026-08-12T21:30:37.431160Z","submitted_at":"2014-05-16T21:51:56Z","title":"Baryonic and dark matter distribution in cosmological simulations of spiral galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.4318","snapshot_observed_at":"2026-08-04T22:14:26.484332Z","title":"Mollitor, E","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:26.484332Z"},"links":{"cited_paper":"/paper/1405.4318","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:d13a939ce7448c1e93a2f37ac795c769ce9bc469cb5c873a6b2d27178af7ca37","observation_id":"de14d708-2ad6-4e7d-bbc3-5f4aff2ee1ff","resolution":{"observed_at":"2026-08-04T22:14:26.484332Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1305.5360","last_updated":"2013-11-06T16:53:32Z","snapshot_observed_at":"2026-08-10T16:31:15.617168Z","submitted_at":"2013-05-23T09:38:01Z","title":"The formation of disc galaxies in high resolution moving-mesh cosmological simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1305.5360","snapshot_observed_at":"2026-08-04T22:14:26.547975Z","title":"Marinacci, R","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:26.547975Z"},"links":{"cited_paper":"/paper/1305.5360","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:e82fd8c558c4d617107144ceded898208ce665c633a54a02ff2f7ce0c478e382","observation_id":"a2d81ae1-b8d3-449e-893b-8b044c735afc","resolution":{"observed_at":"2026-08-04T22:14:26.547975Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9712213","last_updated":"1997-12-16T22:26:49Z","snapshot_observed_at":"2026-07-07T01:19:21.427941Z","submitted_at":"1997-12-16T22:26:49Z","title":"The Global Schmidt Law in Star Forming Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9712213","snapshot_observed_at":"2026-08-04T22:14:26.618389Z","title":"Kennicutt, Robert C.,The Global Schmidt Law in Star-forming Galaxies,Astrophys","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:26.618389Z"},"links":{"cited_paper":"/paper/astro-ph/9712213","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:02939ecbebfafbe0f06d7161a63e3db1450476b7bd03ae5160fc936dd038c3f1","observation_id":"c844e802-068e-46d6-ab74-6890c0856d44","resolution":{"observed_at":"2026-08-04T22:14:26.618389Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1206.4895","last_updated":"2012-12-24T10:16:48Z","snapshot_observed_at":"2026-07-06T02:50:23.656476Z","submitted_at":"2012-06-21T14:27:33Z","title":"Cusp-core transformations in dwarf galaxies: observational predictions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1206.4895","snapshot_observed_at":"2026-08-04T22:14:26.681388Z","title":"Teyssier, A","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:26.681388Z"},"links":{"cited_paper":"/paper/1206.4895","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:38f13f4c79c4d7435efc76dc31bd9b7ca61a270a99b418d641dda834d8544abf","observation_id":"000fd476-5fb0-40a0-ba6c-20656acc7678","resolution":{"observed_at":"2026-08-04T22:14:26.681388Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1209.2856","last_updated":"2012-11-07T03:31:00Z","snapshot_observed_at":"2026-08-13T02:58:31.867984Z","submitted_at":"2012-09-13T11:28:41Z","title":"The Star Formation Rate of Turbulent Magnetized Clouds: Comparing Theory, Simulations, and Observations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1209.2856","snapshot_observed_at":"2026-08-04T22:14:26.766341Z","title":"Federrath and R","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:26.766341Z"},"links":{"cited_paper":"/paper/1209.2856","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:a0a92d86834c8133964da1096065ca22f186aae2d4dc239c91539c2be0afe088","observation_id":"2774d003-0ee6-484b-a7e9-e43e8f5985f2","resolution":{"observed_at":"2026-08-04T22:14:26.766341Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0505177","last_updated":"2005-05-09T20:32:18Z","snapshot_observed_at":"2026-07-07T00:50:30.468086Z","submitted_at":"2005-05-09T20:32:18Z","title":"A General Theory of Turbulence-Regulated Star Formation, From Spirals to ULIRGs","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0505177","snapshot_observed_at":"2026-08-04T22:14:26.832649Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:26.832649Z"},"links":{"cited_paper":"/paper/astro-ph/0505177","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:44b2d552f60935c3f40f3cba87ddec36e5390e0cdac6df5a3c2a8e2f9906c857","observation_id":"53bb8b88-bd3c-4351-a985-d8f0de4a373d","resolution":{"observed_at":"2026-08-04T22:14:26.832649Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1501.05655","last_updated":"2015-06-03T08:57:42Z","snapshot_observed_at":"2026-08-07T13:44:43.250317Z","submitted_at":"2015-01-22T21:00:12Z","title":"Towards simulating star formation in turbulent high-z galaxies with mechanical supernova feedback","version":2},"cited_work":{"arxiv_id":"1501.05655","doi":null,"metadata_source":"pith","pith_arxiv_id":"1501.05655","snapshot_observed_at":"2026-08-04T22:14:34.038205Z","title":"Towards simulating star formation in turbulent high-z galaxies with mechanical supernova feedback","venue":"astro-ph.GA","work_id":"7548e167-75a8-40b5-add0-53e8d95abec9","year":2015},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:26.905956Z"},"links":{"cited_paper":"/paper/1501.05655","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:31cdb4b76709ed2e4f96a1d8f565b9b103bf94f4d88b37a66492e40f792a3f77","observation_id":"7415da3b-8413-4cb3-a50b-288e63f9190a","resolution":{"observed_at":"2026-08-04T22:14:34.055757Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1410.1629","last_updated":"2014-10-07T07:18:24Z","snapshot_observed_at":"2026-07-06T03:56:37.580059Z","submitted_at":"2014-10-07T07:18:24Z","title":"SKIRT: an Advanced Dust Radiative Transfer Code with a User-Friendly Architecture","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1410.1629","snapshot_observed_at":"2026-08-04T22:14:26.969024Z","title":"Camps and M","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:26.969024Z"},"links":{"cited_paper":"/paper/1410.1629","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:6c96d0a6bb6ece852f5c19b7f2eac6186eb7728c69ec146c2d74f811be50d281","observation_id":"cc52009b-d7da-414a-9c9c-d319cd851751","resolution":{"observed_at":"2026-08-04T22:14:26.969024Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0809.0898","last_updated":"2008-09-05T16:59:22Z","snapshot_observed_at":"2026-08-03T18:37:12.576030Z","submitted_at":"2008-09-05T16:59:22Z","title":"The Aquarius Project: the subhalos of galactic halos","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0809.0898","snapshot_observed_at":"2026-08-04T22:14:27.033314Z","title":"Springel, J","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:27.033314Z"},"links":{"cited_paper":"/paper/0809.0898","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:42fe1278272d6b78d9dee5e7318fbca3e6eccf9693e35d9db50e78f4714dbb7f","observation_id":"86d29167-c0e4-411d-bd52-3508f65ecded","resolution":{"observed_at":"2026-08-04T22:14:27.033314Z","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":"2026-08-04T22:14:27.144679Z","title":"Binney and S","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:27.144679Z"},"links":{"citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:bf07ef7b3fa1159dbce4dae2a05553466f44099fbe6c126b0f19c5ca995b0f0b","observation_id":"58151c09-1ad0-418a-84b3-2edb3a977ce6","resolution":{"observed_at":"2026-08-04T22:14:27.144679Z","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":"2026-08-04T22:14:27.180562Z","title":null,"venue":null,"work_id":null,"year":1982},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:27.180562Z"},"links":{"citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:0c921081ecb60f634a47135f1219840a40d458cc274b9e38b17ba08f473baa00","observation_id":"81bed3bd-68af-46bc-9469-37216a9fafd7","resolution":{"observed_at":"2026-08-04T22:14:27.180562Z","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":"2026-08-04T22:14:27.251065Z","title":"Davis, G","venue":null,"work_id":null,"year":1985},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:27.251065Z"},"links":{"citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:d61082a55cb5895a15dfcc2eae5a0fea2779f4aef49ba48eea231947925dba11","observation_id":"d92785e8-93d8-41bf-8978-e851f342eda9","resolution":{"observed_at":"2026-08-04T22:14:27.251065Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0812.0288","last_updated":"2008-12-01T13:26:24Z","snapshot_observed_at":"2026-08-01T12:18:54.648437Z","submitted_at":"2008-12-01T13:26:24Z","title":"Phase-space structures II: Hierarchical Structure Finder","version":1},"cited_work":{"arxiv_id":"0812.0288","doi":null,"metadata_source":"pith","pith_arxiv_id":"0812.0288","snapshot_observed_at":"2026-08-04T22:14:33.900008Z","title":"Phase-space structures II: Hierarchical Structure Finder","venue":"astro-ph","work_id":"833314b4-6024-4149-85e4-e2133db952a8","year":2008},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:27.319497Z"},"links":{"cited_paper":"/paper/0812.0288","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:1f786536007986c9d76dc8bff92e3c166cd5ac31bb12055701255a36f46ebce8","observation_id":"ad090297-c332-487a-ab04-0a5404391f4e","resolution":{"observed_at":"2026-08-04T22:14:33.946678Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T22:14:27.385338Z","title":"Rockstar: Phase-space halo finder","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:27.385338Z"},"links":{"citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:6e2ff3e50702af772926a76116e24ff5f4135b446055dc6ed456b2e9f4d3c677","observation_id":"00edd97e-8028-4936-99af-3031492107e2","resolution":{"observed_at":"2026-08-04T22:14:27.385338Z","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":"2506.09146","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T22:14:33.779094Z","title":"Vladimir, C","venue":null,"work_id":"86f0477e-22e2-4e1d-a194-e3fcf07e49c8","year":2025},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:27.459771Z"},"links":{"citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:04a5711ca45d9bb91fcbd780e854a3c9c8c5e2435d32ab445452c6feaada015a","observation_id":"98074558-1f8f-48dd-8db3-de67b9de5930","resolution":{"observed_at":"2026-08-04T22:14:33.820945Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0012055","last_updated":"2000-12-03T14:33:15Z","snapshot_observed_at":"2026-07-07T00:14:26.519053Z","submitted_at":"2000-12-03T14:33:15Z","title":"Populating a cluster of galaxies - I. Results at z=0","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0012055","snapshot_observed_at":"2026-08-04T22:14:27.518794Z","title":"Springel, S","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:27.518794Z"},"links":{"cited_paper":"/paper/astro-ph/0012055","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:de9a23be2604927eed5ab3f002a885b8021a6f8b1d141a2eba02347f6d6267e8","observation_id":"b23ccbe1-41eb-4405-9fd1-b44599621dfe","resolution":{"observed_at":"2026-08-04T22:14:27.518794Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1006.2882","last_updated":"2010-08-31T08:26:49Z","snapshot_observed_at":"2026-07-06T02:11:47.161439Z","submitted_at":"2010-06-15T04:09:19Z","title":"The statistics of the subhalo abundance of dark matter haloes","version":3},"cited_work":{"arxiv_id":"1006.2882","doi":null,"metadata_source":"pith","pith_arxiv_id":"1006.2882","snapshot_observed_at":"2026-08-04T22:14:33.680911Z","title":"The statistics of the subhalo abundance of dark matter haloes","venue":"astro-ph.CO","work_id":"1288bdf5-13e5-4a69-9e81-16567390b87f","year":2010},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:27.603294Z"},"links":{"cited_paper":"/paper/1006.2882","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:df486955cf74f3aac2b3e388a13345fbf72e02190f09ce5d66b4e4ee5eeb4d89","observation_id":"ad727685-d549-42c5-b58a-5b62ec3725ff","resolution":{"observed_at":"2026-08-04T22:14:33.727896Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1805.00484","last_updated":"2018-09-25T13:41:12Z","snapshot_observed_at":"2026-08-09T06:57:56.413944Z","submitted_at":"2018-05-01T18:00:02Z","title":"Systematics in virial mass estimators for pressure-supported systems","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.00484","snapshot_observed_at":"2026-08-04T22:14:27.678621Z","title":"Errani, J","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:27.678621Z"},"links":{"cited_paper":"/paper/1805.00484","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:2752fd659fb572686abcdb7e5c64b1e217db8164d92d42892171fb7163772e7c","observation_id":"2c2caa32-2ce2-4b32-a99a-99a97af7379a","resolution":{"observed_at":"2026-08-04T22:14:27.678621Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.03303","last_updated":"2020-04-16T18:00:06Z","snapshot_observed_at":"2026-08-09T11:28:18.255882Z","submitted_at":"2019-12-06T19:01:07Z","title":"Milky Way Satellite Census. II. Galaxy--Halo Connection Constraints Including the Impact of the Large Magellanic Cloud","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.03303","snapshot_observed_at":"2026-08-04T22:14:27.721044Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:27.721044Z"},"links":{"cited_paper":"/paper/1912.03303","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:b7b0fb9bcbd4cb0aec45ebc29128e4ad0c5a2e86a461a57f1746abd2f540ed58","observation_id":"1a9f96b8-e0cd-4460-81bd-95fda80059f3","resolution":{"observed_at":"2026-08-04T22:14:27.721044Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1207.6105","last_updated":"2013-05-29T18:24:59Z","snapshot_observed_at":"2026-08-13T01:48:59.393961Z","submitted_at":"2012-07-25T20:00:00Z","title":"The Average Star Formation Histories of Galaxies in Dark Matter Halos from z=0-8","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1207.6105","snapshot_observed_at":"2026-08-04T22:14:27.835363Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:27.835363Z"},"links":{"cited_paper":"/paper/1207.6105","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:a5a36490b3f599b988947e71087c21fc4a760a95036ddacb06c10b48ed19f279","observation_id":"e6b3d842-3b63-4e8f-afa9-e78cbd4dcff0","resolution":{"observed_at":"2026-08-04T22:14:27.835363Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0903.4682","last_updated":"2009-12-14T13:02:56Z","snapshot_observed_at":"2026-08-03T03:30:07.203110Z","submitted_at":"2009-03-27T17:38:32Z","title":"Constraints on the relationship between stellar mass and halo mass at low and high redshift","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0903.4682","snapshot_observed_at":"2026-08-04T22:14:27.870335Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:27.870335Z"},"links":{"cited_paper":"/paper/0903.4682","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:7519b10974253b8bc96af0c2715dfd2ed93dfb6070dae81f6b3aca2c9d865568","observation_id":"332795c8-b2f5-4436-972d-ca8d07520403","resolution":{"observed_at":"2026-08-04T22:14:27.870335Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.14233","last_updated":"2023-08-13T09:09:00Z","snapshot_observed_at":"2026-08-13T13:57:15.321517Z","submitted_at":"2022-10-25T18:00:00Z","title":"ELVES IV: The Satellite Stellar-to-Halo Mass Relation Beyond the Milky-Way","version":2},"cited_work":{"arxiv_id":"2210.14233","doi":null,"metadata_source":"pith","pith_arxiv_id":"2210.14233","snapshot_observed_at":"2026-08-04T22:14:33.528853Z","title":"ELVES IV: The Satellite Stellar-to-Halo Mass Relation Beyond the Milky-Way","venue":"astro-ph.GA","work_id":"42dbc776-f999-4546-9151-bdb229da200b","year":2022},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:27.953938Z"},"links":{"cited_paper":"/paper/2210.14233","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:cf66add837e81cef171c51b98c9005cacdc47901c3894655c2cd566dad36074f","observation_id":"f412e671-912f-44e4-a155-4a0a85261459","resolution":{"observed_at":"2026-08-04T22:14:33.588452Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1204.0804","last_updated":"2012-07-03T17:34:31Z","snapshot_observed_at":"2026-07-06T02:45:42.930237Z","submitted_at":"2012-04-03T20:30:49Z","title":"The stellar-subhalo mass relation of satellite galaxies","version":2},"cited_work":{"arxiv_id":"1204.0804","doi":null,"metadata_source":"pith","pith_arxiv_id":"1204.0804","snapshot_observed_at":"2026-08-04T22:14:33.403477Z","title":"The stellar-subhalo mass relation of satellite galaxies","venue":"astro-ph.CO","work_id":"a9462ff2-5d08-4cae-bf91-fbb76dd84857","year":2012},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:28.009081Z"},"links":{"cited_paper":"/paper/1204.0804","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:f03c83f09101030372b8e1b664f581f0e78a268d6f22c02387c667dfdd9ce876","observation_id":"b3a3fbc1-15ef-41c2-b9b5-d5aab842701b","resolution":{"observed_at":"2026-08-04T22:14:33.470874Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2008.11207","last_updated":"2020-11-17T23:22:59Z","snapshot_observed_at":"2026-08-06T08:59:10.939216Z","submitted_at":"2020-08-25T18:00:02Z","title":"Ultra-faint dwarfs in a Milky Way context: Introducing the Mint Condition DC Justice League Simulations","version":2},"cited_work":{"arxiv_id":"2008.11207","doi":null,"metadata_source":"pith","pith_arxiv_id":"2008.11207","snapshot_observed_at":"2026-08-04T22:14:33.285981Z","title":"Ultra-faint dwarfs in a Milky Way context: Introducing the Mint Condition DC Justice League Simulations","venue":"astro-ph.GA","work_id":"8d4ac425-42df-4ed8-bfce-136a47618f46","year":2020},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:28.069243Z"},"links":{"cited_paper":"/paper/2008.11207","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:b1f995051e382c50e262c647fc529c375be3e0c4cdeeb3afeeff1588c538e3c8","observation_id":"d378c763-36c1-4336-b25f-6c6cd6877d2e","resolution":{"observed_at":"2026-08-04T22:14:33.327792Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0703337","last_updated":"2008-05-13T22:49:06Z","snapshot_observed_at":"2026-08-02T10:33:01.185048Z","submitted_at":"2007-03-14T05:08:43Z","title":"Formation and evolution of galaxy dark matter halos and their substructure","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0703337","snapshot_observed_at":"2026-08-04T22:14:28.072325Z","title":"Diemand, M","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:28.072325Z"},"links":{"cited_paper":"/paper/astro-ph/0703337","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:84de30d7a64f823b05cd629576f7777c1c37c1ee0a3498acb2a85d0f5e0b609a","observation_id":"903362c7-3df9-445c-890d-a646e3c67864","resolution":{"observed_at":"2026-08-04T22:14:28.072325Z","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":"2026-08-04T22:14:28.144367Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:28.144367Z"},"links":{"citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:1d908782384da0df036217f20481af7946303c68e1f4400fbba96023de3c6c07","observation_id":"413931b7-e8da-444e-a267-a01c8c738e8b","resolution":{"observed_at":"2026-08-04T22:14:28.144367Z","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":"2026-08-04T22:14:28.219287Z","title":null,"venue":null,"work_id":null,"year":1974},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:28.219287Z"},"links":{"citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:5d381e73e2c94a08c76d2173becac6c3e456e6e4775351c2efb826151adef8b0","observation_id":"a8c9c723-171f-454b-80f8-8e18377e1938","resolution":{"observed_at":"2026-08-04T22:14:28.219287Z","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":"2026-08-04T22:14:28.385503Z","title":null,"venue":null,"work_id":null,"year":1991},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:28.385503Z"},"links":{"citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:61141ba9f15d411b71608b4bd98852ebf4d7e3fdc5b0e230851a92a213c042a5","observation_id":"e2befb3f-88e0-496d-9cd3-612adaf2503e","resolution":{"observed_at":"2026-08-04T22:14:28.385503Z","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":"2026-08-04T22:14:28.533334Z","title":"Lacey and S","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:28.533334Z"},"links":{"citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:d061bc3263745631b958d0d29587a7a8c8be0ee4f3a9be7996b04378070e2c90","observation_id":"0bed5b44-9575-49a1-90b6-f3066ccb827b","resolution":{"observed_at":"2026-08-04T22:14:28.533334Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9712222","last_updated":"1997-12-17T17:25:40Z","snapshot_observed_at":"2026-08-02T14:06:03.104840Z","submitted_at":"1997-12-17T17:25:40Z","title":"Survival of Substructure within Dark Matter Haloes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9712222","snapshot_observed_at":"2026-08-04T22:14:28.712988Z","title":"Tormen, A","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:28.712988Z"},"links":{"cited_paper":"/paper/astro-ph/9712222","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:67087d20791a65df10c1c496ccfdad06b4ce4f60164946d739903daab6b294ec","observation_id":"0a6bd736-bd62-40ed-9a98-2f969b64cf13","resolution":{"observed_at":"2026-08-04T22:14:28.712988Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0611454","last_updated":"2006-11-14T22:02:33Z","snapshot_observed_at":"2026-08-11T20:35:21.439509Z","submitted_at":"2006-11-14T22:02:33Z","title":"The Excursion Set Theory of Halo Mass Functions, Halo Clustering, and Halo Growth","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0611454","snapshot_observed_at":"2026-08-04T22:14:28.901726Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:28.901726Z"},"links":{"cited_paper":"/paper/astro-ph/0611454","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:3308579187a54e1308f7ae2dfc4712ee30081163c54dce9796d154c9052f9c99","observation_id":"08a16614-81da-48e4-8ca6-b8845ea614a0","resolution":{"observed_at":"2026-08-04T22:14:28.901726Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9802268","last_updated":"1999-07-26T10:32:24Z","snapshot_observed_at":"2026-07-07T01:20:01.459011Z","submitted_at":"1998-02-20T14:32:23Z","title":"Semi-Analytic Modelling of Galaxy Formation: The Local Universe","version":3},"cited_work":{"arxiv_id":"astro-ph/9802268","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/9802268","snapshot_observed_at":"2026-08-04T22:14:33.142479Z","title":"Semi-Analytic Modelling of Galaxy Formation: The Local Universe","venue":"astro-ph","work_id":"b90ca4aa-48eb-4364-aecc-3d74d55e787f","year":1998},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:28.988194Z"},"links":{"cited_paper":"/paper/astro-ph/9802268","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:765a13620b48a25804f877138806ca3fa7d39585fd695dd757c07dbd771921a9","observation_id":"68bb0bf4-0433-4d26-ac6e-5bd6857f9a6f","resolution":{"observed_at":"2026-08-04T22:14:33.202674Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2506.09152","last_updated":"2025-06-10T18:05:44Z","snapshot_observed_at":"2026-08-07T04:53:44.943632Z","submitted_at":"2025-06-10T18:05:44Z","title":"Born to be Starless: Revisiting the Missing Satellite Problem","version":1},"cited_work":{"arxiv_id":"2506.09152","doi":null,"metadata_source":"pith","pith_arxiv_id":"2506.09152","snapshot_observed_at":"2026-08-04T22:14:33.001231Z","title":"Born to be Starless: Revisiting the Missing Satellite Problem","venue":"astro-ph.GA","work_id":"231e759e-913a-42dc-9582-712fb78baf84","year":2025},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:29.144252Z"},"links":{"cited_paper":"/paper/2506.09152","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:f1d3fc5e4cf7689395cb2d3eaabdc49bee67f7d09757d0adeba2433f60b2b1be","observation_id":"c912e1f9-0c4c-4025-93e1-79f070655b86","resolution":{"observed_at":"2026-08-04T22:14:33.073349Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0911.2237","last_updated":"2009-11-11T23:13:22Z","snapshot_observed_at":"2026-07-06T01:59:45.730024Z","submitted_at":"2009-11-11T23:13:22Z","title":"At the heart of the matter: the origin of bulgeless dwarf galaxies and Dark Matter cores","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0911.2237","snapshot_observed_at":"2026-08-04T22:14:29.192073Z","title":"Governato et al., At the heart of the matter: the origin of bulgeless dwarf galaxies and Dark Matter cores, Nature463(2010) 203 [0911.2237]","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:29.192073Z"},"links":{"cited_paper":"/paper/0911.2237","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:db04807cd81a51afaec807778ea36166a698f1adc0eb9c6a4fe4c63f6c0f7d9f","observation_id":"f3486b0d-d68c-426c-9568-e46aa41ae6c3","resolution":{"observed_at":"2026-08-04T22:14:29.192073Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1106.0499","last_updated":"2012-01-20T15:06:09Z","snapshot_observed_at":"2026-08-10T07:57:44.982227Z","submitted_at":"2011-06-02T20:00:07Z","title":"How supernova feedback turns dark matter cusps into cores","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1106.0499","snapshot_observed_at":"2026-08-04T22:14:29.314020Z","title":"Pontzen and F","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:29.314020Z"},"links":{"cited_paper":"/paper/1106.0499","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:ff1072fd686408633247d44337a254620f4c9111ca5dac7fa465cea89091bccf","observation_id":"8df69dc1-668c-4cd2-90d0-5a15567999a0","resolution":{"observed_at":"2026-08-04T22:14:29.314020Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1603.00526","last_updated":"2016-06-27T17:02:30Z","snapshot_observed_at":"2026-07-06T04:47:58.839044Z","submitted_at":"2016-03-02T00:02:46Z","title":"From cusps to cores: a stochastic model","version":2},"cited_work":{"arxiv_id":"1603.00526","doi":null,"metadata_source":"pith","pith_arxiv_id":"1603.00526","snapshot_observed_at":"2026-08-04T22:14:32.845767Z","title":"From cusps to cores: a stochastic model","venue":"astro-ph.GA","work_id":"1f67b709-1448-4e2b-b08e-29148a831e05","year":2016},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:29.430012Z"},"links":{"cited_paper":"/paper/1603.00526","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:0f0ff7c051ad3a5a9a9d840fad371def50ce8ae2ee0b2e2b0b29688f21ff6cb4","observation_id":"a6427724-b94e-4c61-b761-21dc2f2e93c8","resolution":{"observed_at":"2026-08-04T22:14:32.927406Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.11726","last_updated":"2019-11-22T17:34:30Z","snapshot_observed_at":"2026-07-06T08:10:34.301657Z","submitted_at":"2019-07-26T18:00:02Z","title":"A model for core formation in dark matter haloes and ultra diffuse galaxies by outflow episodes","version":2},"cited_work":{"arxiv_id":"1907.11726","doi":null,"metadata_source":"pith","pith_arxiv_id":"1907.11726","snapshot_observed_at":"2026-08-04T22:14:32.667952Z","title":"A model for core formation in dark matter haloes and ultra diffuse galaxies by outflow episodes","venue":"astro-ph.GA","work_id":"cd159a62-f4b0-4756-83f9-8ad1d2363acc","year":2019},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:29.546955Z"},"links":{"cited_paper":"/paper/1907.11726","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:82b0db861776f11340ab6e4a6f9db1d630d1474ac526e9a715c7bebee2f37580","observation_id":"f2e56460-4cf3-4b43-bb7a-a5369916bb31","resolution":{"observed_at":"2026-08-04T22:14:32.765825Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2206.07069","last_updated":"2023-04-07T15:08:51Z","snapshot_observed_at":"2026-07-06T13:20:47.902165Z","submitted_at":"2022-06-14T18:00:07Z","title":"The Response of Dark Matter Haloes to Gas Ejection: CuspCore II","version":2},"cited_work":{"arxiv_id":"2206.07069","doi":null,"metadata_source":"pith","pith_arxiv_id":"2206.07069","snapshot_observed_at":"2026-08-04T22:14:32.526004Z","title":"The Response of Dark Matter Haloes to Gas Ejection: CuspCore II","venue":"astro-ph.GA","work_id":"e8497b69-8ecb-4838-938c-07a422b7ad50","year":2022},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:29.668528Z"},"links":{"cited_paper":"/paper/2206.07069","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:3f19d9e725d4bd0136ea7d5f918a681d223e8f8045373e20af14b3998b0d50a3","observation_id":"78744331-672d-4ced-ae09-19bdfb64cb88","resolution":{"observed_at":"2026-08-04T22:14:32.598484Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1707.06264","last_updated":"2017-07-19T19:09:54Z","snapshot_observed_at":"2026-07-06T05:51:51.253539Z","submitted_at":"2017-07-19T19:09:54Z","title":"On stellar mass loss from galaxies in groups and clusters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.06264","snapshot_observed_at":"2026-08-04T22:14:29.791664Z","title":"Tollet, A","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:29.791664Z"},"links":{"cited_paper":"/paper/1707.06264","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:15cd3ff5a7db30f4c3ea706491c4a51f8bcc7ab471744b7cb5208924689ddf0e","observation_id":"27059334-741b-4433-b565-4a8c81d65e8f","resolution":{"observed_at":"2026-08-04T22:14:29.791664Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1608.01327","last_updated":"2016-11-22T13:53:01Z","snapshot_observed_at":"2026-08-10T08:42:25.843738Z","submitted_at":"2016-08-03T20:04:58Z","title":"NIHAO XI: Formation of Ultra-Diffuse Galaxies by outflows","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1608.01327","snapshot_observed_at":"2026-08-04T22:14:29.983425Z","title":"Di Cintio, C","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:29.983425Z"},"links":{"cited_paper":"/paper/1608.01327","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:6d5d55531318b25a315a2766d0eff611d91bbb289ef70171d5a34dcbadba3460","observation_id":"6b762974-dd71-4230-a79a-02a4b972e861","resolution":{"observed_at":"2026-08-04T22:14:29.983425Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.02281","last_updated":"2017-09-30T11:33:17Z","snapshot_observed_at":"2026-07-06T05:17:43.785682Z","submitted_at":"2016-11-07T21:00:00Z","title":"FIRE in the Field: Simulating the Threshold of Galaxy Formation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.02281","snapshot_observed_at":"2026-08-04T22:14:30.066826Z","title":"Fitts, M","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:30.066826Z"},"links":{"cited_paper":"/paper/1611.02281","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:a06e5b044979d0548711483e21bd10508872f73c2e514ca9fe361ba4759065e3","observation_id":"fb362a25-329c-4a2d-99b7-c6fe8ef4e8cb","resolution":{"observed_at":"2026-08-04T22:14:30.066826Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.01378","last_updated":"2021-06-02T18:00:02Z","snapshot_observed_at":"2026-08-07T17:57:15.013805Z","submitted_at":"2021-06-02T18:00:02Z","title":"Core Formation in High-z Massive Haloes: Heating by Post Compaction Satellites and Response to AGN Outflows","version":1},"cited_work":{"arxiv_id":"2106.01378","doi":null,"metadata_source":"pith","pith_arxiv_id":"2106.01378","snapshot_observed_at":"2026-08-04T22:14:32.281963Z","title":"Core Formation in High-z Massive Haloes: Heating by Post Compaction Satellites and Response to AGN Outflows","venue":"astro-ph.GA","work_id":"1ba52dc1-9b75-47fb-a8b6-dd4931306df6","year":2021},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:30.159630Z"},"links":{"cited_paper":"/paper/2106.01378","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:94e95c6b403c8563fa529a4015ae30817c2c8a80a818806f2f54e7d14e46e0ff","observation_id":"bca63428-90e5-4838-99cd-cbff47fda05f","resolution":{"observed_at":"2026-08-04T22:14:32.376027Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2209.08631","last_updated":"2023-02-20T17:51:20Z","snapshot_observed_at":"2026-08-13T14:24:20.209404Z","submitted_at":"2022-09-18T18:48:13Z","title":"Halo heating from fluctuating gas in a model dwarf","version":2},"cited_work":{"arxiv_id":"2209.08631","doi":null,"metadata_source":"pith","pith_arxiv_id":"2209.08631","snapshot_observed_at":"2026-08-04T22:14:32.131817Z","title":"Halo heating from fluctuating gas in a model dwarf","venue":"astro-ph.GA","work_id":"5ee1e2e0-fc49-4b26-ae0f-f2bff3581e47","year":2022},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:30.214029Z"},"links":{"cited_paper":"/paper/2209.08631","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:ffea5298492961064e0b7709af57b025b74d90cebfe6b534093fa5c8a335773d","observation_id":"07773c6b-7f4f-4b02-8262-f5af17a0a236","resolution":{"observed_at":"2026-08-04T22:14:32.209249Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1404.7144","last_updated":"2014-04-28T20:00:21Z","snapshot_observed_at":"2026-07-06T03:42:17.811981Z","submitted_at":"2014-04-28T20:00:21Z","title":"The Star Formation Histories of Local Group Dwarf Galaxies I. Hubble Space Telescope / Wide Field Planetary Camera 2 Observations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1404.7144","snapshot_observed_at":"2026-08-04T22:14:30.283625Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:30.283625Z"},"links":{"cited_paper":"/paper/1404.7144","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:49d556a8a40ab61d593d5a1d1284d6999536e7fc5ac905f44afd277f49a45536","observation_id":"a5db569e-ba68-4a4f-a12c-24d7aa0988d9","resolution":{"observed_at":"2026-08-04T22:14:30.283625Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.10607","last_updated":"2018-11-26T19:00:00Z","snapshot_observed_at":"2026-08-09T08:50:03.471370Z","submitted_at":"2018-11-26T19:00:00Z","title":"Formation of ultra-diffuse galaxies in the field and in galaxy groups","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.10607","snapshot_observed_at":"2026-08-04T22:14:30.404829Z","title":"Jiang, A","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","version":1},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-04T22:14:30.404829Z"},"links":{"cited_paper":"/paper/1811.10607","citing_paper":"/paper/2509.07470"},"observation_digest":"sha256:b20797461803a2b065d79bef15167ebe26d60818add492bbc5f5c5f55d2c2eb6","observation_id":"b62a2dda-a56c-4d7a-88b7-19198612d987","resolution":{"observed_at":"2026-08-04T22:14:30.404829Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2509.07470","last_updated":"2025-09-09T07:48:46Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-13T01:49:04.533641Z","submitted_at":"2025-09-09T07:48:46Z","title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":75,"verified_exact":25,"verified_fuzzy":0},"total_outbound_references":111},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 100 of 111 outbound references and 0 inbound Pith citation observations for arXiv:2509.07470."}