Paper Citation Record · LEDGER

Jets are the most robust observable ingredient of common envelope evolution

As of 12 August 2026, this Paper Citation Record lists 21 of 21 outbound references and 1 inbound Pith citation observation for arXiv:2412.04017.

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

pith.paper-citation-record.v1
2412.04017 v2

Coverage vector

measured 21 of 21 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-11T21:56:45.217408Z

measured 22 of 22 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T18:09:40.428855Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-11T18:09:45.243970Z

Reference resolution

21 of 21 outbound references displayed

verified exact4
verified fuzzy1
unresolved11
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External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 9ac41750-97c0-42f0-88c9-daa5ebf4c56c · outbound

This paper cites 2015, MNRAS, 453, 2115, doi: 10.1093/mnras/ stv1666 Akashi, M., & Soker, N.

Jets are the most robust observable ingredient of common envelope evolution 2015, MNRAS, 453, 2115, doi: 10.1093/mnras/ stv1666 Akashi, M., & Soker, N

Reference 1

Resolution: malformed identifier; no resolver link, observed 2026-08-11T21:56:45.126242Z

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Observation 36a4844f-39f6-4818-aac3-0373f332ca65 · outbound

This paper cites Variability of Central Stars of Planetary Nebulae with the Zwicky Transient Facility. I. Methods, Short-Timescale Variables, Binary Candidates, and the Unusual Nucleus of WeSb 1.

Jets are the most robust observable ingredient of common envelope evolution Variability of Central Stars of Planetary Nebulae with the Zwicky Transient Facility. I. Methods, Short-Timescale Variables, Binary Candidates, and the Unusual Nucleus of WeSb 1

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-11T21:56:45.139696Z

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Observation f5f19812-265e-46d3-81b5-6e046aa921a7 · outbound

This paper cites an unresolved cited work.

Jets are the most robust observable ingredient of common envelope evolution Unresolved cited work

Reference 5

Resolution: verified exact; raw_fallback, observed 2026-08-11T21:56:45.759025Z

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

Observation 95eeead5-2405-4da3-931b-194952dd137a · outbound

This paper cites Journey to the center of the common envelope evolution. Inner dynamics of the post-dynamical inspiral.

Jets are the most robust observable ingredient of common envelope evolution Journey to the center of the common envelope evolution. Inner dynamics of the post-dynamical inspiral

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-11T21:56:45.152045Z

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Observation 64b2a2f2-7f30-4ff0-8fed-01e625fe6c84 · outbound

This paper cites A., Cazzoli, S., Rechy-Garc ´ıa, J.

Jets are the most robust observable ingredient of common envelope evolution A., Cazzoli, S., Rechy-Garc ´ıa, J

Reference 8

Resolution: malformed identifier; no resolver link, observed 2026-08-11T21:56:45.156174Z

Source-reported events for the cited work

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Observation f6548239-4983-4275-9c3e-7773afd2ca99 · outbound

This paper cites A., Imai, H., & Orosz, G.

Jets are the most robust observable ingredient of common envelope evolution A., Imai, H., & Orosz, G

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-11T21:56:45.130997Z

Source-reported events for the cited work

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Observation 18fb58dd-16cd-4e8f-871d-1baeb11e5a33 · outbound

This paper cites 2020, MNRAS, 497, 3166, doi:.

Jets are the most robust observable ingredient of common envelope evolution 2020, MNRAS, 497, 3166, doi:

Reference 11

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T21:56:45.782853Z

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Observation 00aa19ce-0965-48bd-9987-c3a05d7a843e · outbound

This paper cites Post-common-envelope planetary nebulae.

Jets are the most robust observable ingredient of common envelope evolution Post-common-envelope planetary nebulae

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-11T21:56:45.171199Z

Source-reported events for the cited work

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Observation adf3dfd2-9655-409b-ae67-d27f26e053d8 · outbound

This paper cites 2010, MNRAS, 408, 2312, doi: 10.1111/j.1365-2966.

Jets are the most robust observable ingredient of common envelope evolution 2010, MNRAS, 408, 2312, doi: 10.1111/j.1365-2966

Reference 14

Resolution: verified exact; raw_fallback, observed 2026-08-11T21:56:45.592991Z

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

Observation fb0d5cbe-ee97-4af2-8f11-f88b60c65d5a · outbound

This paper cites Successful Common Envelope Ejection and Binary Neutron Star Formation in 3D Hydrodynamics.

Jets are the most robust observable ingredient of common envelope evolution Successful Common Envelope Ejection and Binary Neutron Star Formation in 3D Hydrodynamics

Reference 15

Resolution: malformed identifier; no resolver link, observed 2026-08-11T21:56:45.182188Z

Source-reported events for the cited work

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Observation 9bd6ef99-1159-42fa-8bb4-3608a0d01af8 · outbound

This paper cites Halving spaces and lower bounds in real enumerative geometry.

Jets are the most robust observable ingredient of common envelope evolution Halving spaces and lower bounds in real enumerative geometry

Reference 16

Resolution: metadata mismatch; local_arxiv, observed 2026-08-11T21:56:45.507281Z

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 0c46d5a2-661c-42c7-a55a-6f104ec3aa12 · outbound

This paper cites A., Redman, M.

Jets are the most robust observable ingredient of common envelope evolution A., Redman, M

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-11T21:56:45.192109Z

Source-reported events for the cited work

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Observation ca24aea3-e3ea-4960-8457-6f72de147f90 · outbound

This paper cites The Evolution of Binaries Embedded Within Common Envelopes.

Jets are the most robust observable ingredient of common envelope evolution The Evolution of Binaries Embedded Within Common Envelopes

Reference 19

Resolution: malformed identifier; no resolver link, observed 2026-08-11T21:56:45.199350Z

Source-reported events for the cited work

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Observation 72da642d-ba85-4424-9d97-40fd7cfbdb51 · outbound

This paper cites High-Speed Outflows and Dusty Disks during the AGB to PN Transition: The PANORAMA survey.

Jets are the most robust observable ingredient of common envelope evolution High-Speed Outflows and Dusty Disks during the AGB to PN Transition: The PANORAMA survey

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-11T21:56:45.202509Z

Source-reported events for the cited work

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Observation 4ef63a67-3665-48c6-9649-b8e9a1ef0c34 · outbound

This paper cites From spherical stars to disk-like structures: 3D common-envelope evolution of massive binaries beyond inspiral.

Jets are the most robust observable ingredient of common envelope evolution From spherical stars to disk-like structures: 3D common-envelope evolution of massive binaries beyond inspiral

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-11T21:56:45.210106Z

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Observation 4533f4a3-b6f4-412b-9094-b0f685084117 · outbound

This paper cites C., & Nordhaus, J.

Jets are the most robust observable ingredient of common envelope evolution C., & Nordhaus, J

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-11T21:56:45.213931Z

Source-reported events for the cited work

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Observation 7fb0c2c4-711a-4411-b748-4ad0622019da · outbound

This paper cites 2020, MNRAS, 497, 2855, doi: 10.1093/mnras/staa2145.

Jets are the most robust observable ingredient of common envelope evolution 2020, MNRAS, 497, 2855, doi: 10.1093/mnras/staa2145

Reference 23

Resolution: verified exact; doi, observed 2026-08-11T21:56:45.247722Z

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Observation 5e865699-bc5d-4e22-bf59-156ae2ed2210 · outbound

This paper cites 2024, MNRAS, 532, 692, doi:10.

Jets are the most robust observable ingredient of common envelope evolution 2024, MNRAS, 532, 692, doi:10

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-11T21:56:45.206362Z

Source-reported events for the cited work

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Observation fb6344df-bb93-4af3-bf28-b3491434fc83 · outbound

This paper cites C., Frew, D.

Jets are the most robust observable ingredient of common envelope evolution C., Frew, D

Reference 319

Resolution: verified exact; doi, observed 2026-08-11T21:56:45.275848Z

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 dea8dc95-ee35-4693-a91e-4651e9a39e56 · outbound

This paper cites On the response of massive main sequence stars to mass accretion and outflow at high rates.

Jets are the most robust observable ingredient of common envelope evolution On the response of massive main sequence stars to mass accretion and outflow at high rates

Reference 778

Resolution: unresolved; no resolver link, observed 2026-08-11T21:56:45.135305Z

Source-reported events for the cited work

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Observation 60de5c3d-8480-4d11-96cf-682486b2e6cd · outbound

This paper cites 2024, MNRAS, 530, 3327, doi: 10.1093/mnras/stae1013 Estrella-Trujillo, D., Hern ´andez-Mart´ınez, L., Vel ´azquez, P.

Jets are the most robust observable ingredient of common envelope evolution 2024, MNRAS, 530, 3327, doi: 10.1093/mnras/stae1013 Estrella-Trujillo, D., Hern ´andez-Mart´ınez, L., Vel ´azquez, P

Reference 2277

Resolution: unresolved; no resolver link, observed 2026-08-11T21:56:45.148080Z

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Unavailable: canonical work link unavailable.

Pith citing papers

Observation 60e96441-16ff-4fd1-a9ab-3b30cb1957da · inbound

Hyperaccreting Magnetised Neutron Stars inside Rotating Massive Envelopes: Low-Power Jets and Precursor Flares cites this paper.

Hyperaccreting Magnetised Neutron Stars inside Rotating Massive Envelopes: Low-Power Jets and Precursor Flares Jets are the most robust observable ingredient of common envelope evolution

Reference 24

Resolution: verified exact; local_arxiv, observed 2026-08-11T18:09:45.248603Z

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.