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Paper Citation Record · LEDGER

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations

As of 15 August 2026, this Paper Citation Record lists 74 of 74 outbound references and 0 inbound Pith citation observations for arXiv:1908.09844.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
1908.09844 v1

Coverage vector

measured 74 of 74 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-14T11:05:14.782461Z

measured 74 of 74 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: cited_works

Reference resolution

74 of 74 outbound references displayed

  • verified exact10
  • verified fuzzy2
  • unresolved61
  • parse uncertain0
  • malformed identifier1
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External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 5097f71b-9b61-40ae-9279-f4817b12cb75 · outbound

This paper cites write newline.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations write newline

Reference 1

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Observation 12cd8413-2a02-49af-9ba3-88bdd28285b3 · outbound

This paper cites A., 2018, @doi [ ] 10.1093/mnras/sty1169 , https://ui.adsabs.harvard.edu/\#abs/2018MNRAS.478.3410A 478, 3410.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations A., 2018, @doi [ ] 10.1093/mnras/sty1169 , https://ui.adsabs.harvard.edu/\#abs/2018MNRAS.478.3410A 478, 3410

Reference 2

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Observation 40e40955-1f50-46a1-8e1d-7fd99d5e9e0e · outbound

This paper cites M., 2006, @doi [Reports on Progress in Physics] 10.1088/0034-4885/69/12/R02 , https://ui.adsabs.harvard.edu/\#abs/2006RPPh...69.3101B 69, 3101.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations M., 2006, @doi [Reports on Progress in Physics] 10.1088/0034-4885/69/12/R02 , https://ui.adsabs.harvard.edu/\#abs/2006RPPh...69.3101B 69, 3101

Reference 4

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Observation 42c244db-e080-4266-b496-da04ebc20fce · outbound

This paper cites S., Wechsler R.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations S., Wechsler R

Reference 5

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Observation 784c105e-f498-46cb-b408-6c5cf65b8905 · outbound

This paper cites UniverseMachine: The Correlation between Galaxy Growth and Dark Matter Halo Assembly from z=0-10.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations UniverseMachine: The Correlation between Galaxy Growth and Dark Matter Halo Assembly from z=0-10

Reference 6

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Observation c2b4c76b-05c1-47a6-8295-c3debc835959 · outbound

This paper cites J., 2010, @doi [ ] 10.1016/j.physrep.2010.06.001 , https://ui.adsabs.harvard.edu/\#abs/2010PhR...495...33B 495, 33.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations J., 2010, @doi [ ] 10.1016/j.physrep.2010.06.001 , https://ui.adsabs.harvard.edu/\#abs/2010PhR...495...33B 495, 33

Reference 7

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Observation 2a8bd790-5a51-4263-9378-1c848f0d066e · outbound

This paper cites S., Dekel A., Kolatt T.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations S., Dekel A., Kolatt T

Reference 12

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Observation b49d2418-10df-4948-90a2-5fcb505dac1d · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 13

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Observation 54d54255-f3f6-4636-a5ce-5155ecf69ef4 · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 14

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Observation f98a3130-50af-49a4-8a12-f7e8fef0af07 · outbound

This paper cites A., et al., 2018, @doi [ ] 10.1093/mnras/sty1131 , https://ui.adsabs.harvard.edu/\#abs/2018MNRAS.479....2C 479, 2.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations A., et al., 2018, @doi [ ] 10.1093/mnras/sty1131 , https://ui.adsabs.harvard.edu/\#abs/2018MNRAS.479....2C 479, 2

Reference 15

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Observation 413f9961-bf8a-484b-b691-88899f3b0af1 · outbound

This paper cites J., et al., 2016, @doi [ ] 10.3847/0067-0049/222/2/22 , https://ui.adsabs.harvard.edu/\#abs/2016ApJS..222...22C 222, 22.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations J., et al., 2016, @doi [ ] 10.3847/0067-0049/222/2/22 , https://ui.adsabs.harvard.edu/\#abs/2016ApJS..222...22C 222, 22

Reference 16

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Observation a09b0394-7967-4adf-bfa8-167a9de795a4 · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 17

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Observation adb6dce5-6bc3-4219-bdd4-87d924151c50 · outbound

This paper cites F., 2016, @doi [ ] 10.1093/mnras/stw1862 , https://ui.adsabs.harvard.edu/\#abs/2016MNRAS.462.3265D 462, 3265.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations F., 2016, @doi [ ] 10.1093/mnras/stw1862 , https://ui.adsabs.harvard.edu/\#abs/2016MNRAS.462.3265D 462, 3265

Reference 19

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Observation 427a16b6-1bad-4e56-ab26-9736e648461f · outbound

This paper cites Simba: Cosmological Simulations with Black Hole Growth and Feedback.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Simba: Cosmological Simulations with Black Hole Growth and Feedback

Reference 20

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Observation fa7cd7f7-e3d5-442a-9c71-b570a3c7ff18 · outbound

This paper cites S., White S.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations S., White S

Reference 21

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Observation 14a0319e-9870-4f8d-a4de-942ad825c38c · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 22

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Observation 133b65a6-a4c8-47ad-817e-d32e226f7369 · outbound

This paper cites R., Schaye J., Kay S.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations R., Schaye J., Kay S

Reference 23

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Observation a9ebaaed-42c9-4f49-86ae-5cd0a2eb2a8e · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 24

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Observation 0037d779-e4a1-40a2-bf4c-7a06595044dd · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 25

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Observation d8f76b7c-cbef-4aa8-bb99-d399436bc9cb · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 26

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Observation a063cd22-a5ed-40a0-b630-d81a1f715ce9 · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 27

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verified exact
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No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

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Observation 734e3c8e-99ab-4de4-b0ec-89c7ae4aa991 · outbound

This paper cites A., Barnes D.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations A., Barnes D

Reference 28

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Observation 16794d62-921b-4442-ad0f-4048dc677011 · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 29

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Observation be8a4edc-e01b-4ff3-a353-6b027d5d56fc · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 30

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Reference 31

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Reference 32

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Observation 32803412-fa27-43d5-b674-bfdbbf2d1f76 · outbound

This paper cites H., Hernquist L., 1996, @doi [ ] 10.1086/192305 , https://ui.adsabs.harvard.edu/\#abs/1996ApJS..105...19K 105, 19.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations H., Hernquist L., 1996, @doi [ ] 10.1086/192305 , https://ui.adsabs.harvard.edu/\#abs/1996ApJS..105...19K 105, 19

Reference 33

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Observation 61584113-0278-4436-9df7-7cc7a9b1fb0a · outbound

This paper cites V., Khokhlov A.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations V., Khokhlov A

Reference 34

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Observation 9f8c04eb-fa8b-4e75-bf4e-96556adbf312 · outbound

This paper cites A., Trujillo-Gomez S., Primack J., 2011, @doi [ ] 10.1088/0004-637X/740/2/102 , https://ui.adsabs.harvard.edu/abs/2011ApJ...740..102K 740, 102.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations A., Trujillo-Gomez S., Primack J., 2011, @doi [ ] 10.1088/0004-637X/740/2/102 , https://ui.adsabs.harvard.edu/abs/2011ApJ...740..102K 740, 102

Reference 35

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Observation 9c1c912e-b7d4-4664-83ee-021c02ed80ea · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 36

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Observation 8846a78a-8830-4bd4-9418-08cf81d42df4 · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 37

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unresolved
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Observation cd96e698-eb3a-4c8a-9ba9-1cb542bc0fa4 · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 38

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unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 7e7ecf2b-f9a2-4d90-9c0c-13872a2b428d · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 39

Resolution
verified exact
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

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Observation 525b4bbf-67a8-4ee4-a271-2a85584139ef · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 41

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unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.573534Z digest=sha256:2ca965836c5c4303b18a0112e2448ca300abf1de849fc341c217b66ae7f87a52

Observation 24cecfe2-deae-42d8-845c-c817faa21f8f · outbound

This paper cites P., Naab T., White S.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations P., Naab T., White S

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.578109Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.578109Z digest=sha256:54c0b112487da9551f169726ac74ed873f6b71af36121f44fea61bf94534badf

Observation 15cfca00-7563-413a-983f-05eef067064d · outbound

This paper cites P., et al., 2018, @doi [ ] 10.1093/mnras/sty618 , https://ui.adsabs.harvard.edu/\#abs/2018MNRAS.477.1206N 477, 1206.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations P., et al., 2018, @doi [ ] 10.1093/mnras/sty618 , https://ui.adsabs.harvard.edu/\#abs/2018MNRAS.477.1206N 477, 1206

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.583599Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.583599Z digest=sha256:19f655784ce82641894df5ae3b3cd46cea39ab5fc3e66062a123ba442391a62b

Observation b18a6b4b-9c77-444c-a1e3-f966f5d85e95 · outbound

This paper cites F., Frenk C.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations F., Frenk C

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.587766Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.587766Z digest=sha256:cbb0c309c1fe4eb9bb0aceaa718d39ff8b5b2b767a46c03d90ca98b0995d717d

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.592243Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.592243Z digest=sha256:1e121555f25964a78b09b46ea0d86ec557cb435046c7e59a19bf10582a848de7

Observation a3aa76ac-9e0e-4faf-9ebc-029a9b9c8940 · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.597107Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.597107Z digest=sha256:eaddc45d109f661e41f0b491a03166b81e9b3e2ae1ef69dde42a3b296a6690d4

Observation 0fc18c1f-26bc-4485-9693-e491c9f31ea1 · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.602582Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.602582Z digest=sha256:e8499490315923a7635bb57956440450f4e3a4f607062e0d4ecbfdfe72e689af

Observation 0a993a85-77ea-4070-8caf-7d262a90b71f · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 48

Resolution
verified exact
arxiv_id_nonexistent, observed 2026-08-14T11:05:15.590413Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T11:05:14.607318Z digest=sha256:6a787910b79287e84e20a32553f5a9c3ea04754af546f9719296b04860f50ab4

Observation c2e18ee0-35a2-4c40-a5a6-a933f838a50f · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.611866Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.611866Z digest=sha256:0bec5725e93af74ebb03d27dd1aa4107126e43fce8cb63f3262de9ef94671746

Observation b6e40d7f-7cad-4bca-b19b-b58de47126c8 · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.617019Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.617019Z digest=sha256:7551f8b433e2828aef615d9964804583cfa4f69440677542eb33909cff8dd605

Observation addc7b8c-896f-4256-b9ec-4c03e0b35583 · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.621902Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.621902Z digest=sha256:f8c254fa7077677de05e72e7d4a340e3db52d8c85a3e2cffce1181cdf3e030af

Observation f8750ed0-98c7-42ec-b35b-e221b9cc845f · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.626377Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.626377Z digest=sha256:b78cadcd4d91f87361d0d67e04a327a7aba432d1e193955c7cb9b7c97282543d

Observation ea56c805-6b80-4ca8-87a4-89da58ff033d · outbound

This paper cites A., Simonneau E., Betancort-Rijo J., Patiri S., Gottl \"o ber S., Sanchez-Conde M.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations A., Simonneau E., Betancort-Rijo J., Patiri S., Gottl \"o ber S., Sanchez-Conde M

Reference 53

Resolution
verified exact
doi, observed 2026-08-14T11:05:14.988502Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T11:05:14.631111Z digest=sha256:08553600022278c3d7290899fc7e0cff17ad945f67c549e0fcbd7ec3990088b7

Observation 7f33686e-c21a-4e0b-8088-521cd4431792 · outbound

This paper cites A., Cuesta A.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations A., Cuesta A

Reference 54

Resolution
verified exact
arxiv_id_nonexistent, observed 2026-08-14T11:05:16.013822Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T11:05:14.635575Z digest=sha256:317056c6261dabf6e9887ab4af3f75028ee21c12b58368a5df8abad58701e5d9

Observation cbded979-088f-47b5-9d85-d8a1c3950b53 · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.639817Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.639817Z digest=sha256:081603539faf801b5a15fcfbd9492d861cd3bddd0b8f2a77b41df6bfcce4a834

Observation 39559766-2868-4f33-8022-e99bdaf4aaf1 · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.644398Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.644398Z digest=sha256:88f4396471dad420dfe73ad63623baeed38815e4e68d1e33c92f4d6f65f9cc44

Observation 55669b70-a4d1-4914-b920-d0ef90a93ccd · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.649052Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.649052Z digest=sha256:ec24d77051639010968cbe55ed68d415eaaba97bb6a8cca7138575b6b384c1cd

Observation a296bf7d-5162-4138-98d9-0c517f3fb4c2 · outbound

This paper cites R., Avila-Reese V., Faber S.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations R., Avila-Reese V., Faber S

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.653626Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.653626Z digest=sha256:d538e2f08d60ddf2f8d0691a16499ddebabb70a1d5a901ae7daf37ced18d2f94

Observation 27576723-aa58-4502-a852-102c3c6a3749 · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.658130Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.658130Z digest=sha256:0e7627a9472c6f53c7d9773f77646f49451a4280e4b1cdc622303b75edfa2851

Observation 9d4e6cf0-663a-46b9-9c8f-04df3b9f76b6 · outbound

This paper cites S., Crain R.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations S., Crain R

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.662845Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.662845Z digest=sha256:50147c9561f3065c6f96df112b3ea6fbb4761714b9bdb59f4289fb5744c83c23

Observation fbd8a6eb-d195-46d1-8293-f4587131c58e · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 61

Resolution
verified exact
arxiv_id_nonexistent, observed 2026-08-14T11:05:15.959402Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T11:05:14.667373Z digest=sha256:4a2fa716bbf82c90ac66844b6e117b1a5c80621ea74335298e3c09a0e1b2ae3f

Observation e00653d6-bed4-424c-91dd-42ad2c29ce1a · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.672220Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.672220Z digest=sha256:e62b3f753642d50114d819ba94391a7496650e7d0e1a79efd0aab26a56410cb5

Observation 757b14d8-5bc3-403f-821b-36f4f2140808 · outbound

This paper cites A., 2012, @doi [Research in Astronomy and Astrophysics] 10.1088/1674-4527/12/8/004 , https://ui.adsabs.harvard.edu/\#abs/2012RAA....12..917S 12, 917.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations A., 2012, @doi [Research in Astronomy and Astrophysics] 10.1088/1674-4527/12/8/004 , https://ui.adsabs.harvard.edu/\#abs/2012RAA....12..917S 12, 917

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.677275Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.677275Z digest=sha256:4b2cb6f6cead12655a79c0574d3a074337b20bb32cefbe6db5d24bb44ecacb57

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.682011Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.682011Z digest=sha256:0c261bae19447bed7e5f950d2ea4dbf7a1b292d3afce7310437cde6d1a0c8b39

Observation 06de5b09-e083-4e5d-b9dd-0bf8e33172db · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 68

Resolution
verified exact
arxiv_id_nonexistent, observed 2026-08-14T11:05:15.850629Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T11:05:14.700369Z digest=sha256:cdf3a5dbfff741e1d09f6bfb56b465b0d1c0cc9f2fd5608a8d7e65b6a816912b

Observation a18d5031-670e-4ea3-af88-646e919c9d6c · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.704614Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.704614Z digest=sha256:293c904de584ec3326ec7614192a1320c6d0e5ddaac31eee9b26b6a0d7a40fa6

Observation 65c29821-6f79-4ee0-aaad-c49f8dc46f70 · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 70

Resolution
verified exact
arxiv_id_nonexistent, observed 2026-08-14T11:05:15.537457Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T11:05:14.708960Z digest=sha256:a28cdf8cc4499df04f6e1c809a2e170406ce9e06db0028fd494b4febd9398d53

Observation 210895b7-b852-403d-bce2-b9a6e7bfc4dd · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 71

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.713175Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.713175Z digest=sha256:e8566052cc2fdd634ad7050124fb81ddb00b5d601474b64048c9811f465f02d9

Observation b14b5c23-745f-493c-9f5e-e95aea36cff8 · outbound

This paper cites Springer International Publishing, pp 21--36.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Springer International Publishing, pp 21--36

Reference 73

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T11:05:16.045544Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T11:05:14.723128Z digest=sha256:5ec97e011dcb9252a61abb66a4902f94289e4b6396ffacecb8ab7efb99bae942

Observation a01dfd27-5523-4f73-802c-ac08ac7a1d56 · outbound

This paper cites R., Pontzen A., Anderson L., Bellovary J., 2017, @doi [ ] 10.1093/mnras/stx1160 , https://ui.adsabs.harvard.edu/\#abs/2017MNRAS.470.1121T 470, 1121.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations R., Pontzen A., Anderson L., Bellovary J., 2017, @doi [ ] 10.1093/mnras/stx1160 , https://ui.adsabs.harvard.edu/\#abs/2017MNRAS.470.1121T 470, 1121

Reference 74

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.727934Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.727934Z digest=sha256:ae16dc8ef7b48018dbc62fc615d298a6b2f1d03d942806de3e91c639729abc3c

Observation 526a5931-b3e2-4d25-a70f-d5381c5c09a1 · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.733062Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.733062Z digest=sha256:b64aff8ad6611e16c70170b795cd9a5f62554e1104c3e5113ce6f9d2f31de380

Observation e5855732-c317-429d-91cd-6a3b24134228 · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.737852Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.737852Z digest=sha256:bd47bf04ea100439855232352ea56ff8c0d0a74b2f4af3dd3966c22402c82f02

Observation 6b7af301-5724-4ac7-a23e-e4a2b2a9c580 · outbound

This paper cites A., Iliev I.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations A., Iliev I

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.742842Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.742842Z digest=sha256:7eb8609791684d057d99d9966a0eef907cc7d73be9287dd1b39186d431337090

Observation c15a8e2a-1f09-40f0-92fd-985de119404d · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 78

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.748372Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.748372Z digest=sha256:32c9cf1da5dc345041ca0f2d3e6d3a529d2e5a5217c74c4d84d271cca84cc599

Observation cf819197-7f42-4920-8090-85fdc05bd5cc · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.753626Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.753626Z digest=sha256:9894e284eb08a3470721ab8d1a7dd15aa2d94857eea52f4066a7a0f5aafadf27

Observation cd51db46-d288-4702-8519-a02b7d024b88 · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.758524Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.758524Z digest=sha256:89475c87c1c869da49586cf37013d4fedbdb8514043f4e7ddd77ef782efc218f

Observation f7aaed85-3657-4503-aa11-919dc4ad2ecd · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 81

Resolution
verified exact
doi, observed 2026-08-14T11:05:14.820051Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T11:05:14.763278Z digest=sha256:91ca514b21bc43bc67bbad4611d8a6243b4093883a4f299881147d1b16f14c31

Observation 519bb7dd-039c-444e-9d66-7ba201dcd00f · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 82

Resolution
verified exact
arxiv_id_nonexistent, observed 2026-08-14T11:05:15.498696Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T11:05:14.767881Z digest=sha256:c9212402d2c179e0a045378fcf5e8bb9a6a8526bb8ee6f49236e593766d84192

Observation f4dcf606-c651-48db-a036-5bd26545b20e · outbound

This paper cites an unresolved cited work.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations Unresolved cited work

Reference 83

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.772721Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.772721Z digest=sha256:95509122d34bfdef49d805c83b9617b744346218defc7280a30831c2e45d1aff

Reference 84

Resolution
unresolved
no resolver link, observed 2026-08-14T11:05:14.777170Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:05:14.777170Z digest=sha256:5c6bf1dfd1fb1357d3e0c8d000f8e372c9314b002589863935c0953055e34e25

Observation 91091a36-60cb-4966-8299-ba8cc205b906 · outbound

This paper cites write newline.

Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations write newline

Reference 85

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T11:05:16.029831Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T11:05:14.782461Z digest=sha256:3f1061e1005a97adac5520b516d46e6a864c41c51636dbcd64e8185f2f51935c

Pith citing papers

No inbound Pith citation observations are available.