Paper Citation Record · LEDGER

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations

As of 7 August 2026, this Paper Citation Record lists 39 of 39 outbound references and 0 inbound Pith citation observations for arXiv:2506.13813.

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

pith.paper-citation-record.v1
2506.13813 v1

Coverage vector

measured 39 of 39 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-07T00:51:08.120436Z

measured 39 of 39 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

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measured 0 of 1 external citation measurements

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Source: cited_works

Reference resolution

39 of 39 outbound references displayed

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External citation measurements

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Outbound references

Observation 9e49bc91-fb9c-4a99-8541-a6cd4d23d2ab · outbound

This paper cites The Gaia mission.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations The Gaia mission

Reference 1

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Observation 4677eb5a-9e72-4673-a48c-652fe35c5fed · outbound

This paper cites Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-07T00:51:07.842890Z

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Observation d71bf4e3-f008-4a9f-83ad-f2a6d8121286 · outbound

This paper cites Gaia Data Release 2. Summary of the contents and survey properties.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations Gaia Data Release 2. Summary of the contents and survey properties

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-07T00:51:07.848169Z

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Observation fa739650-a9b9-4414-b674-8f73425dacea · outbound

This paper cites Gaia Early Data Release 3: Summary of the contents and survey properties.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations Gaia Early Data Release 3: Summary of the contents and survey properties

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-07T00:51:07.853561Z

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Observation 0be5b889-e063-4948-81c4-9f54c7fe2706 · outbound

This paper cites Gaia Data Release 3: Summary of the content and survey properties.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations Gaia Data Release 3: Summary of the content and survey properties

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-07T00:51:07.859590Z

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Observation c97e9791-977e-4e9a-8aa6-088b3211b070 · outbound

This paper cites A dwarf satellite galaxy in Sagittarius.Nature1994,370, 194–196.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations A dwarf satellite galaxy in Sagittarius.Nature1994,370, 194–196

Reference 6

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Observation 7721fa8b-71c1-42ff-a51f-a6bbd332eb8b · outbound

This paper cites Sagittarius: The Nearest Dwarf Galaxy.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations Sagittarius: The Nearest Dwarf Galaxy

Reference 7

Resolution: verified exact; local_arxiv, observed 2026-08-07T00:51:09.981155Z

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Observation 751383d4-962f-4276-8d86-54bb4bed01fb · outbound

This paper cites Detection of massive tidal tails around the globular cluster Pal 5 with SDSS commissioning data.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations Detection of massive tidal tails around the globular cluster Pal 5 with SDSS commissioning data

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-07T00:51:07.878592Z

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Observation 277587b4-22f7-418a-aba6-1d331635adf5 · outbound

This paper cites A Matched-Filter Analysis of the Tidal Tails of the Globular Cluster Palomar 5.The Astronomical Journal2002, 124, 349–363.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations A Matched-Filter Analysis of the Tidal Tails of the Globular Cluster Palomar 5.The Astronomical Journal2002, 124, 349–363

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-07T00:51:07.884542Z

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Observation 86d87a54-8aea-4b90-9719-4dba72c40c96 · outbound

This paper cites Streams, substructures and the early history of the Milky Way.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations Streams, substructures and the early history of the Milky Way

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-07T00:51:07.892789Z

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Observation 1c8a79a6-1997-425f-b7ce-e6b4632f838d · outbound

This paper cites galstreams: A Library of Milky Way Stellar Stream Footprints and Tracks.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations galstreams: A Library of Milky Way Stellar Stream Footprints and Tracks

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-07T00:51:07.898888Z

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Observation bc36000a-460b-4b55-b912-c1fc6e9030b2 · outbound

This paper cites Charting the Galactic acceleration field II. A global mass model of the Milky Way from the STREAMFINDER Atlas of Stellar Streams detected in Gaia DR3.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations Charting the Galactic acceleration field II. A global mass model of the Milky Way from the STREAMFINDER Atlas of Stellar Streams detected in Gaia DR3

Reference 12

Resolution: malformed identifier; no resolver link, observed 2026-08-07T00:51:07.905550Z

Source-reported events for the cited work

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Observation fe369c9a-8929-4815-9367-2b8ff1539fbd · outbound

This paper cites Stellar Streams in the Gaia Era.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations Stellar Streams in the Gaia Era

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-07T00:51:07.910636Z

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Unavailable: canonical work link unavailable.

Observation b50b8e61-f3c2-401e-b1c1-8657916180d4 · outbound

This paper cites On $N$-body simulations of globular cluster stream.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations On $N$-body simulations of globular cluster stream

Reference 14

Resolution: verified exact; local_arxiv, observed 2026-08-07T00:51:09.694737Z

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Observation 09612d15-1b1d-42af-96cc-e78d3e577f90 · outbound

This paper cites Milky Way Mass and Potential Recovery Using Tidal Streams in a Realistic Halo.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations Milky Way Mass and Potential Recovery Using Tidal Streams in a Realistic Halo

Reference 15

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Observation cbb47b21-f821-4be6-9210-8820cd471350 · outbound

This paper cites galpy: A Python Library for Galactic Dynamics.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations galpy: A Python Library for Galactic Dynamics

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-07T00:51:07.927496Z

Source-reported events for the cited work

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Observation 01f2e119-1654-43a4-aae5-eed52d61dbe4 · outbound

This paper cites The mass distribution and gravitational potential of the Milky Way.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations The mass distribution and gravitational potential of the Milky Way

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-07T00:51:07.936179Z

Source-reported events for the cited work

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Observation 284450f9-3e0a-4208-8d1a-1367a4639d1c · outbound

This paper cites Gala: A Python package for galactic dynamics.The Journal of Open Source Software2017,2, 388.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations Gala: A Python package for galactic dynamics.The Journal of Open Source Software2017,2, 388

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-07T00:51:07.941781Z

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Observation 5e222111-88e3-41b9-80ca-7b5f63cfa3ef · outbound

This paper cites Uncertainties associated with the backward integration of dwarf satellites using simple parametric potentials.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations Uncertainties associated with the backward integration of dwarf satellites using simple parametric potentials

Reference 19

Resolution: verified exact; local_arxiv, observed 2026-08-07T00:51:09.479159Z

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Observation af06e7f0-98a6-4fab-b6bd-bea33b7657d0 · outbound

This paper cites Modeling the orbital histories of satellites of Milky Way-mass galaxies: testing static host potentials against cosmological simulations.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations Modeling the orbital histories of satellites of Milky Way-mass galaxies: testing static host potentials against cosmological simulations

Reference 20

Resolution: verified exact; local_arxiv, observed 2026-08-07T00:51:09.353480Z

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Observation a039aa78-5793-45e1-baac-ea9d3f48f3d7 · outbound

This paper cites The last breath of the Sagittarius dSph.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations The last breath of the Sagittarius dSph

Reference 21

Resolution: verified exact; local_arxiv, observed 2026-08-07T00:51:09.215889Z

Source-reported events for the cited work

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Observation 2f20edef-29a1-4e2d-a975-49d6016c3406 · outbound

This paper cites Tango for three: Sagittarius, LMC, and the Milky Way.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations Tango for three: Sagittarius, LMC, and the Milky Way

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-07T00:51:07.984449Z

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Observation e0d23389-1724-4250-8b62-6a40a94b38ee · outbound

This paper cites And yet it moves: The dangers of artificially fixing the Milky Way center of mass in the presence of a massive Large Magellanic Cloud.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations And yet it moves: The dangers of artificially fixing the Milky Way center of mass in the presence of a massive Large Magellanic Cloud

Reference 23

Resolution: verified exact; local_arxiv, observed 2026-08-07T00:51:09.054973Z

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Observation 26473351-3a2e-4f09-9fd7-45e323dbed09 · outbound

This paper cites Reconstructing the Last Major Merger of the Milky Way with the H3 Survey.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations Reconstructing the Last Major Merger of the Milky Way with the H3 Survey

Reference 24

Resolution: verified exact; local_arxiv, observed 2026-08-07T00:51:08.915763Z

Source-reported events for the cited work

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Observation a29e7eb7-0006-490e-ad29-1edf2ed57a70 · outbound

This paper cites Gaps and length asymmetry in the stellar stream Palomar 5 as effects of Galactic bar rotation.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations Gaps and length asymmetry in the stellar stream Palomar 5 as effects of Galactic bar rotation

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-07T00:51:08.004540Z

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Observation f37833a8-aad9-49cd-b6ad-2da6abbbe92e · outbound

This paper cites On the stability of tidal streams in action space.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations On the stability of tidal streams in action space

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-07T00:51:08.010235Z

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Observation a5b168d9-e02f-480f-89e0-fc1a1836f07b · outbound

This paper cites Generation of mock tidal streams.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations Generation of mock tidal streams

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-07T00:51:08.015630Z

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Observation ca1b5b68-7fae-4084-a39f-88536bf7e32f · outbound

This paper cites An analytical model for spherical galaxies and bulges.Astrophys.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations An analytical model for spherical galaxies and bulges.Astrophys

Reference 28

Resolution: malformed identifier; no resolver link, observed 2026-08-07T00:51:08.020920Z

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Observation b51d128b-7154-45ad-bc9f-42a5eb692ee3 · outbound

This paper cites Three-dimensional models for the distribution of mass in galaxies.Publ.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations Three-dimensional models for the distribution of mass in galaxies.Publ

Reference 29

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T00:51:10.293787Z

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Observation 53d5c1a3-f3e3-42c9-94e2-41f6aa9ddcf7 · outbound

This paper cites Simple and accurate modelling of the gravitational potential produced by thick and thin exponential disks.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations Simple and accurate modelling of the gravitational potential produced by thick and thin exponential disks

Reference 30

Resolution: verified exact; local_arxiv, observed 2026-08-07T00:51:08.714124Z

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Observation f2741146-c447-473e-9778-a7d661676479 · outbound

This paper cites The fate of the gaseous disks of galaxies that fall into clusters.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations The fate of the gaseous disks of galaxies that fall into clusters

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-07T00:51:08.037975Z

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Observation b7c17596-82ae-461e-87ee-0ef69a8a4c19 · outbound

This paper cites On the problem of distribution in globular star clusters.Mon.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations On the problem of distribution in globular star clusters.Mon

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-07T00:51:08.047973Z

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Observation 8eb17b3f-52c3-4881-8eef-5e84a2a02610 · outbound

This paper cites The cosmological simulation code GADGET-2.Mon.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations The cosmological simulation code GADGET-2.Mon

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-07T00:51:08.056272Z

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Observation 9c916a36-46a7-4b40-94ac-d749486f3ff3 · outbound

This paper cites Simulating cosmic structure formation with the GADGET-4 code.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations Simulating cosmic structure formation with the GADGET-4 code

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-07T00:51:08.067963Z

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Observation 783e8e84-16d2-45a0-bcf8-a8fc6237e48b · outbound

This paper cites The Accuracy of Cross-Correlation Estimates of Quasar Emission-Line Region Sizes.Astrophys.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations The Accuracy of Cross-Correlation Estimates of Quasar Emission-Line Region Sizes.Astrophys

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-07T00:51:08.077641Z

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Observation 518d8cca-aac9-431a-a40b-64c13c7a2224 · outbound

This paper cites Cross-Correlation and Maximum Likelihood Analysis: A New Approach to Combine Cross-Correlation Functions.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations Cross-Correlation and Maximum Likelihood Analysis: A New Approach to Combine Cross-Correlation Functions

Reference 36

Resolution: verified exact; local_arxiv, observed 2026-08-07T00:51:08.439884Z

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Observation 5d58b3fc-b99d-471e-aa77-21ccd73590a2 · outbound

This paper cites The size distribution of galaxies in the Sloan Digital Sky Survey.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations The size distribution of galaxies in the Sloan Digital Sky Survey

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-07T00:51:08.097221Z

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Observation 9dec4b33-ba19-49d6-a3b9-61a98cf6fdbd · outbound

This paper cites Galaxy And Mass Assembly (GAMA): mass-size relations of z$<$0.1 galaxies subdivided by S\'ersic index, colour and morphology.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations Galaxy And Mass Assembly (GAMA): mass-size relations of z$<$0.1 galaxies subdivided by S\'ersic index, colour and morphology

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-07T00:51:08.109116Z

Source-reported events for the cited work

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Observation 55f64fce-f663-44b1-afd9-11adb153ff6e · outbound

This paper cites The stellar mass - physical effective radius relation for dwarf galaxies in low-density environments.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations The stellar mass - physical effective radius relation for dwarf galaxies in low-density environments

Reference 39

Resolution: verified exact; local_arxiv, observed 2026-08-07T00:51:08.292693Z

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No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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