Variable gravitational potential of Milky Way analogues in HESTIA suite | Paper Citation Record

Observation ce3a76ab-6000-4914-b8e1-afa027b08b51 · outbound

This paper cites The spikes in cℓ at 30 and 50 kpc are caused by a less massive satellite (2 × 1010 M⊙) reaching these distances.

Variable gravitational potential of Milky Way analogues in HESTIA suite The spikes in cℓ at 30 and 50 kpc are caused by a less massive satellite (2 × 1010 M⊙) reaching these distances

Reference 1

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T04:27:09.215128Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 8dcba05d-f415-40dc-8d2e-300966243e04 · outbound

This paper cites an unresolved cited work.

Variable gravitational potential of Milky Way analogues in HESTIA suite Unresolved cited work

Reference 2

Resolution: unresolved; raw_fallback, observed 2026-08-11T04:27:09.202075Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 2b714b2b-3811-4692-a3cf-a9b1abd46e25 · outbound

This paper cites an unresolved cited work.

Variable gravitational potential of Milky Way analogues in HESTIA suite Unresolved cited work

Reference 3

Resolution: unresolved; raw_fallback, observed 2026-08-11T04:27:09.190201Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 23e669db-cb93-4c5d-a913-df291a68a9bc · outbound

This paper cites Great Circle tidal streams: evidence for a nearly spherical massive dark halo around the Milky Way.

Variable gravitational potential of Milky Way analogues in HESTIA suite Great Circle tidal streams: evidence for a nearly spherical massive dark halo around the Milky Way

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-11T04:27:08.345601Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 787ad1b1-610f-4e2e-93ee-6ee75314eda0 · outbound

This paper cites Is the dark halo of our Galaxy spherical?.

Variable gravitational potential of Milky Way analogues in HESTIA suite Is the dark halo of our Galaxy spherical?

Reference 5

Resolution: verified exact; local_arxiv, observed 2026-08-11T04:27:09.086582Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 3cf3599b-21ef-460f-a6c4-484d02660cf6 · outbound

This paper cites A 2MASS All-Sky View of the Sagittarius Dwarf Galaxy: IV. Modeling the Sagittarius Tidal Tails.

Variable gravitational potential of Milky Way analogues in HESTIA suite A 2MASS All-Sky View of the Sagittarius Dwarf Galaxy: IV. Modeling the Sagittarius Tidal Tails

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-11T04:27:08.354854Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2cc4d97e-5476-4497-b8bb-465a26a77591 · outbound

This paper cites The Sagittarius Dwarf Galaxy: a Model for Evolution in a Triaxial Milky Way Halo.

Variable gravitational potential of Milky Way analogues in HESTIA suite The Sagittarius Dwarf Galaxy: a Model for Evolution in a Triaxial Milky Way Halo

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-11T04:27:08.359706Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f24621a5-5dd4-4833-8715-869ed82afafd · outbound

This paper cites Constraining the Milky Way potential with a 6-D phase-space map of the GD-1 stellar stream.

Variable gravitational potential of Milky Way analogues in HESTIA suite Constraining the Milky Way potential with a 6-D phase-space map of the GD-1 stellar stream

Reference 8

Resolution: malformed identifier; no resolver link, observed 2026-08-11T04:27:08.364223Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9919c208-bc5b-4f82-89f8-d24f836e48a9 · outbound

This paper cites Globular Cluster Streams as Galactic High-Precision Scales - The Poster Child Palomar 5.

Variable gravitational potential of Milky Way analogues in HESTIA suite Globular Cluster Streams as Galactic High-Precision Scales - The Poster Child Palomar 5

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-11T04:27:08.368907Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 33f72d39-90a9-4a54-b994-8c53fcc98cfe · outbound

This paper cites Constraining the Milky Way Halo Potential with the GD-1 stellar stream.

Variable gravitational potential of Milky Way analogues in HESTIA suite Constraining the Milky Way Halo Potential with the GD-1 stellar stream

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-11T04:27:08.373718Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5a9d142c-0e68-44a7-9fe8-71fcef43b8cd · outbound

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

Variable gravitational potential of Milky Way analogues in HESTIA suite Uncertainties associated with the backward integration of dwarf satellites using simple parametric potentials

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-11T04:27:08.378325Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 538a5971-274b-494c-976f-2cc7c19aca98 · outbound

This paper cites Measuring the Milky Way mass distribution in the presence of the LMC.

Variable gravitational potential of Milky Way analogues in HESTIA suite Measuring the Milky Way mass distribution in the presence of the LMC

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-11T04:27:08.382393Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a2709d0e-c1fe-4a03-9684-b70ec71f5e3b · outbound

This paper cites $S^5$: Probing the Milky Way and Magellanic Clouds potentials with the 6-D map of the Orphan-Chenab stream.

Variable gravitational potential of Milky Way analogues in HESTIA suite $S^5$: Probing the Milky Way and Magellanic Clouds potentials with the 6-D map of the Orphan-Chenab stream

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-11T04:27:08.386518Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a6be3e80-1d5f-4697-9750-0d1653069acb · outbound

This paper cites Hunting for the Dark Matter Wake Induced by the Large Magellanic Cloud.

Variable gravitational potential of Milky Way analogues in HESTIA suite Hunting for the Dark Matter Wake Induced by the Large Magellanic Cloud

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-11T04:27:08.390833Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c15daf9a-8c3d-41b5-bdc7-263198455548 · outbound

This paper cites Quantifying the Stellar Halo's Response to the LMC's Infall with Spherical Harmonics.

Variable gravitational potential of Milky Way analogues in HESTIA suite Quantifying the Stellar Halo's Response to the LMC's Infall with Spherical Harmonics

Reference 15

Resolution: malformed identifier; no resolver link, observed 2026-08-11T04:27:08.395358Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 75d1a3ea-e168-4e44-be13-72e5dcca117b · outbound

This paper cites Erkal, V.

Variable gravitational potential of Milky Way analogues in HESTIA suite Erkal, V

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-11T04:27:08.399725Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b8d4ed65-ce30-4e55-bbf9-7a89589f7d32 · outbound

This paper cites Reflex motion in the Milky Way stellar halo resulting from the Large Magellanic Cloud infall.

Variable gravitational potential of Milky Way analogues in HESTIA suite Reflex motion in the Milky Way stellar halo resulting from the Large Magellanic Cloud infall

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-11T04:27:08.403700Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4cf70b22-a7b1-4211-940e-f9f871f0bb91 · outbound

This paper cites an unresolved cited work.

Variable gravitational potential of Milky Way analogues in HESTIA suite Unresolved cited work

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-11T04:27:08.407629Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fbf62318-9272-4b95-ae57-23be910d8fae · outbound

This paper cites Quantifying the impact of the Large Magellanic Cloud on the structure of the Milky Way's dark matter halo using Basis Function Expansions.

Variable gravitational potential of Milky Way analogues in HESTIA suite Quantifying the impact of the Large Magellanic Cloud on the structure of the Milky Way's dark matter halo using Basis Function Expansions

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-11T04:27:08.411958Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7a0681af-0607-4a76-9872-54bb59f3126c · outbound

This paper cites The effect of the LMC on the Milky Way system.

Variable gravitational potential of Milky Way analogues in HESTIA suite The effect of the LMC on the Milky Way system

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-11T04:27:08.415914Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 09b28d79-2a3d-4cfd-8645-77f1f5054128 · outbound

This paper cites Dear Magellanic Clouds, welcome back!.

Variable gravitational potential of Milky Way analogues in HESTIA suite Dear Magellanic Clouds, welcome back!

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-11T04:27:08.419963Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e9ef1a2d-0afe-4c3b-a379-06a5b9e231fb · outbound

This paper cites The LMC impact on the kinematics of the Milky Way satellites: clues from the running solar apex.

Variable gravitational potential of Milky Way analogues in HESTIA suite The LMC impact on the kinematics of the Milky Way satellites: clues from the running solar apex

Reference 22

Resolution: verified exact; local_arxiv, observed 2026-08-11T04:27:08.909656Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 3c901b3b-8d0f-4a1a-955d-8311a5ceec71 · outbound

This paper cites It is not necessarily connected with the rotation of particles constituting a halo.

Variable gravitational potential of Milky Way analogues in HESTIA suite It is not necessarily connected with the rotation of particles constituting a halo

Reference 23

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T04:27:09.177462Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 5ca24704-d100-4419-babf-9e20dd58daf7 · outbound

This paper cites Dubinski, Cosmological Tidal Shear, ApJ401 (1992).

Variable gravitational potential of Milky Way analogues in HESTIA suite Dubinski, Cosmological Tidal Shear, ApJ401 (1992)

Reference 24

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T04:27:09.163915Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation e32bd703-a2ae-48d5-82ef-9763f0aa8632 · outbound

This paper cites Figure Rotation of Cosmological Dark Matter Halos.

Variable gravitational potential of Milky Way analogues in HESTIA suite Figure Rotation of Cosmological Dark Matter Halos

Reference 25

Resolution: verified exact; local_arxiv, observed 2026-08-11T04:27:08.894400Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation acb9e0d3-0bfb-42af-a4f5-764018bcc851 · outbound

This paper cites Figure rotation of dark halos in CDM simulations.

Variable gravitational potential of Milky Way analogues in HESTIA suite Figure rotation of dark halos in CDM simulations

Reference 26

Resolution: verified exact; local_arxiv, observed 2026-08-11T04:27:08.877643Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 7d9604c7-e726-41eb-89cb-d7d7fe1a52a6 · outbound

This paper cites Response of dark matter halos to condensation of baryons: cosmological simulations and improved adiabatic contraction model.

Variable gravitational potential of Milky Way analogues in HESTIA suite Response of dark matter halos to condensation of baryons: cosmological simulations and improved adiabatic contraction model

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-11T04:27:08.443245Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a5c57ad9-4248-4b26-aad2-a5a5cd349fb7 · outbound

This paper cites The Effect of Gas Cooling on the Shapes of Dark Matter Halos.

Variable gravitational potential of Milky Way analogues in HESTIA suite The Effect of Gas Cooling on the Shapes of Dark Matter Halos

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-11T04:27:08.447376Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e8b36b01-09c0-4870-a3bf-e3edb2238a6f · outbound

This paper cites Gustafsson, M.

Variable gravitational potential of Milky Way analogues in HESTIA suite Gustafsson, M

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-11T04:27:08.451408Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 12c4fa08-fb5d-47f9-8370-877f9efb541a · outbound

This paper cites an unresolved cited work.

Variable gravitational potential of Milky Way analogues in HESTIA suite Unresolved cited work

Reference 30

Resolution: unresolved; raw_fallback, observed 2026-08-11T04:27:09.151989Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 13904a07-10b8-4146-9288-abf41cde23ea · outbound

This paper cites Efficient and accurate force replay in cosmological-baryonic simulations.

Variable gravitational potential of Milky Way analogues in HESTIA suite Efficient and accurate force replay in cosmological-baryonic simulations

Reference 31

Resolution: verified exact; local_arxiv, observed 2026-08-11T04:27:08.805933Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 8202e76d-a99a-45f6-982f-17b1306b93da · outbound

This paper cites an unresolved cited work.

Variable gravitational potential of Milky Way analogues in HESTIA suite Unresolved cited work

Reference 32

Resolution: unresolved; raw_fallback, observed 2026-08-11T04:27:09.138687Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 77744307-802e-420f-a855-2eb379201a52 · outbound

This paper cites Agama reference documentation.

Variable gravitational potential of Milky Way analogues in HESTIA suite Agama reference documentation

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-11T04:27:08.488942Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 35fdaab9-1397-4552-afb9-a03219160310 · outbound

This paper cites an unresolved cited work.

Variable gravitational potential of Milky Way analogues in HESTIA suite Unresolved cited work

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-11T04:27:08.471594Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 34fb46e3-8d1c-4488-bdd4-a5db4e862446 · outbound

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

Variable gravitational potential of Milky Way analogues in HESTIA suite On the stability of tidal streams in action space

Reference 35

Resolution: malformed identifier; no resolver link, observed 2026-08-11T04:27:08.475749Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e4c0a1af-d7bb-4998-9fbd-30dc9c3efd68 · outbound

This paper cites Cosmicflows-2: The Data.

Variable gravitational potential of Milky Way analogues in HESTIA suite Cosmicflows-2: The Data

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-11T04:27:08.501736Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7c48cf4d-4a38-4b81-8b72-f797d6ffb40b · outbound

This paper cites an unresolved cited work.

Variable gravitational potential of Milky Way analogues in HESTIA suite Unresolved cited work

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-11T04:27:08.484953Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 75cfb036-bb8e-438f-8288-175f9909f230 · outbound

This paper cites Planes of satellite galaxies and the cosmic web.

Variable gravitational potential of Milky Way analogues in HESTIA suite Planes of satellite galaxies and the cosmic web

Reference 38

Resolution: malformed identifier; local_arxiv, observed 2026-08-11T04:27:08.756361Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 36ce403c-18c0-437e-af35-d695633c7cd8 · outbound

This paper cites Constrained Simulations of the Real Universe: the Local Supercluster.

Variable gravitational potential of Milky Way analogues in HESTIA suite Constrained Simulations of the Real Universe: the Local Supercluster

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-11T04:27:08.493102Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a73d809f-1307-4445-a2f3-c9eadbd00282 · outbound

This paper cites an unresolved cited work.

Variable gravitational potential of Milky Way analogues in HESTIA suite Unresolved cited work

Reference 40

Resolution: verified exact; doi, observed 2026-08-11T04:27:08.587086Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation ae7fe06b-3140-4f18-8f96-9aa762f6ffa0 · outbound

This paper cites The Hestia project: simulations of the Local Group.

Variable gravitational potential of Milky Way analogues in HESTIA suite The Hestia project: simulations of the Local Group

Reference 41

Resolution: malformed identifier; no resolver link, observed 2026-08-11T04:27:08.524149Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ce791213-2c22-48d4-b920-fb3556513db7 · outbound

This paper cites The Laniakea supercluster of galaxies.

Variable gravitational potential of Milky Way analogues in HESTIA suite The Laniakea supercluster of galaxies

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-11T04:27:08.505871Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 56de0742-025a-4d68-afe8-3857918687e3 · outbound

This paper cites Ahf: Amiga's Halo Finder.

Variable gravitational potential of Milky Way analogues in HESTIA suite Ahf: Amiga's Halo Finder

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-11T04:27:08.531974Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 17157e80-fe8f-4823-9849-9f477779bd88 · outbound

This paper cites The preferred direction of infalling satellite galaxies in the Local Group.

Variable gravitational potential of Milky Way analogues in HESTIA suite The preferred direction of infalling satellite galaxies in the Local Group

Reference 44

Resolution: verified exact; local_arxiv, observed 2026-08-11T04:27:08.739068Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation bc093af3-00f4-4ca5-a19a-52d2322dd3cc · outbound

This paper cites The VPOS: a vast polar structure of satellite galaxies, globular clusters and streams around the Milky Way.

Variable gravitational potential of Milky Way analogues in HESTIA suite The VPOS: a vast polar structure of satellite galaxies, globular clusters and streams around the Milky Way

Reference 46

Resolution: verified exact; local_arxiv, observed 2026-08-11T04:27:08.687948Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation a5ce5d5c-d49c-4e5b-8728-b0fa4468000d · outbound

This paper cites an unresolved cited work.

Variable gravitational potential of Milky Way analogues in HESTIA suite Unresolved cited work

Reference 47

Resolution: unresolved; raw_fallback, observed 2026-08-11T04:27:09.125484Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation dd8f7023-43ff-42bf-a963-8e57a1bc4852 · outbound

This paper cites The Axial Zone of Avoidance in the Globular Cluster System and the Distance to the Galactic Center.

Variable gravitational potential of Milky Way analogues in HESTIA suite The Axial Zone of Avoidance in the Globular Cluster System and the Distance to the Galactic Center

Reference 48

Resolution: verified exact; local_arxiv, observed 2026-08-11T04:27:08.655580Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation de625fd4-9751-49fc-bdc9-628ba830d762 · outbound

This paper cites Arakelyan, S.

Variable gravitational potential of Milky Way analogues in HESTIA suite Arakelyan, S

Reference 49

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T04:27:09.112765Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation bf340ac6-86c6-4092-8dc9-6f7e47cd21ad · outbound

This paper cites The great disk of Milky-Way satellites and cosmological sub-structures.

Variable gravitational potential of Milky Way analogues in HESTIA suite The great disk of Milky-Way satellites and cosmological sub-structures

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-11T04:27:08.539988Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 23f5d941-f814-4967-a866-8a39bfceb1ce · outbound

This paper cites Spatial Distribution of Globular Clusters in the Galaxy.

Variable gravitational potential of Milky Way analogues in HESTIA suite Spatial Distribution of Globular Clusters in the Galaxy

Reference 52

Resolution: verified exact; local_arxiv, observed 2026-08-11T04:27:08.671866Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation d98edaf0-d8dc-4a65-b4a4-0022bad59ae5 · outbound

This paper cites The Causes of Halo Shape Changes Induced by Cooling Baryons: Disks Versus Substructures.

Variable gravitational potential of Milky Way analogues in HESTIA suite The Causes of Halo Shape Changes Induced by Cooling Baryons: Disks Versus Substructures

Reference 1088

Resolution: unresolved; no resolver link, observed 2026-08-11T04:27:08.459192Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fb5bf049-d065-4e9b-a7f7-5d39f36cebc4 · outbound

This paper cites Impact of baryon physics on dark matter structures: a detailed simulation study of halo density profiles.

Variable gravitational potential of Milky Way analogues in HESTIA suite Impact of baryon physics on dark matter structures: a detailed simulation study of halo density profiles

Reference 2178

Resolution: verified exact; local_arxiv, observed 2026-08-11T04:27:08.832454Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Coverage vector

Reference resolution

Outbound references

Pith citing papers