Paper Citation Record · LEDGER

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields

As of 14 August 2026, this Paper Citation Record lists 87 of 87 outbound references and 3 inbound Pith citation observations for arXiv:1908.05275.

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

pith.paper-citation-record.v1
1908.05275 v1

Coverage vector

measured 87 of 87 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-14T13:24:12.578909Z

measured 90 of 90 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T12:39:17.826727Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T02:57:34.984925Z

Reference resolution

87 of 87 outbound references displayed

verified exact5
verified fuzzy23
unresolved58
parse uncertain1
malformed identifier0
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External citation measurements

No source-named external measurement is stored.

Outbound references

Observation c569cea8-44e4-4886-bb9b-1aa5515e2363 · outbound

This paper cites Our particle model assumption is.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Our particle model assumption is

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.235820Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f321830d-2378-4afa-acd7-56bcf99c7271 · outbound

This paper cites and since we are working in the ballistic limit we are assuming.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields and since we are working in the ballistic limit we are assuming

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.240658Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 035a160b-7555-4f21-8a6d-efe6273bcdcb · outbound

This paper cites We expand to 2nd order in ∆z/RL (2nd Born approximation) to obtain the leading-order contribution to ISM spin- down and obtain our spin-down bound.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields We expand to 2nd order in ∆z/RL (2nd Born approximation) to obtain the leading-order contribution to ISM spin- down and obtain our spin-down bound

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.244750Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 590ea93b-a1e5-4e71-af74-954c2ef9905d · outbound

This paper cites an unresolved cited work.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Unresolved cited work

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.248961Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 615be730-8756-4d0d-b24d-eec4e6b85982 · outbound

This paper cites an unresolved cited work.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Unresolved cited work

Reference 5

Resolution: parse uncertain; no resolver link, observed 2026-08-14T13:24:12.252651Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0d5f304d-942a-46ea-9c97-504238fa5891 · outbound

This paper cites magnetic plasma waves move slowly compared to typical qDM velocities (see [17] which reviews ISM plasma dynamics); and some are more dubious and might be made diﬀerently.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields magnetic plasma waves move slowly compared to typical qDM velocities (see [17] which reviews ISM plasma dynamics); and some are more dubious and might be made diﬀerently

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.256526Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ebbc0ea7-492f-47b9-a5e0-4950bc239925 · outbound

This paper cites an unresolved cited work.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Unresolved cited work

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.260608Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f497c1d9-5eff-4ea0-91d2-1c7f877583cf · outbound

This paper cites an unresolved cited work.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Unresolved cited work

Reference 8

Resolution: unresolved; raw_fallback, observed 2026-08-14T13:24:13.483708Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation f35c0b70-483d-4feb-8e4f-ea74633e2eee · outbound

This paper cites To derive a numerical bound on q/m we also assume.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields To derive a numerical bound on q/m we also assume

Reference 9

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T13:24:13.472734Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation e5db0671-ff25-4305-907a-98fb8b1de3e6 · outbound

This paper cites an unresolved cited work.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Unresolved cited work

Reference 10

Resolution: unresolved; raw_fallback, observed 2026-08-14T13:24:13.461760Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 33440827-e642-4de3-b1cc-986d77345edf · outbound

This paper cites an unresolved cited work.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Unresolved cited work

Reference 11

Resolution: unresolved; raw_fallback, observed 2026-08-14T13:24:13.450508Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation a6db9f4b-239a-499a-8fdc-5a4908ee7b61 · outbound

This paper cites an unresolved cited work.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Unresolved cited work

Reference 12

Resolution: unresolved; raw_fallback, observed 2026-08-14T13:24:13.439257Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 4edfbbb2-99db-4e13-8de0-90d5eb5c34fe · outbound

This paper cites an unresolved cited work.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Unresolved cited work

Reference 13

Resolution: unresolved; raw_fallback, observed 2026-08-14T13:24:13.426372Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation b95d579e-4ce9-409f-a369-b878816e5692 · outbound

This paper cites an unresolved cited work.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Unresolved cited work

Reference 14

Resolution: unresolved; raw_fallback, observed 2026-08-14T13:24:13.413886Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation c0843e21-9fbc-4db0-8c9f-200ecf20ccdc · outbound

This paper cites an unresolved cited work.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Unresolved cited work

Reference 15

Resolution: unresolved; raw_fallback, observed 2026-08-14T13:24:13.399317Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation a80c435a-bed0-4572-b13c-63f500ad8ee1 · outbound

This paper cites We assume that initially f+ = f− = f0, but f will evolve away from this as the qDM particles travel through the magnetic ﬁeld.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields We assume that initially f+ = f− = f0, but f will evolve away from this as the qDM particles travel through the magnetic ﬁeld

Reference 16

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T13:24:13.385596Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation e7138ad2-df8b-4259-9c1b-ffeb7363fb24 · outbound

This paper cites For slight deﬂections, the time it takes to traverse the ISM of thickness ∆ z is∼ ∆z/v wherev &V is the particle’s speed.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields For slight deﬂections, the time it takes to traverse the ISM of thickness ∆ z is∼ ∆z/v wherev &V is the particle’s speed

Reference 17

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T13:24:13.374834Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 38b568bb-54b5-47f3-86c3-6f611336d6b9 · outbound

This paper cites For notational simplicity we suppress the⃗ x0 dependence in most formulae as we are considering only a small region of the disk.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields For notational simplicity we suppress the⃗ x0 dependence in most formulae as we are considering only a small region of the disk

Reference 18

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T13:24:13.363874Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 07100b87-8a72-4551-9c90-9af9efd485ff · outbound

This paper cites an unresolved cited work.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Unresolved cited work

Reference 19

Resolution: unresolved; raw_fallback, observed 2026-08-14T13:24:13.352907Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 32ef5580-6096-4bbd-92fa-862f734dce08 · outbound

This paper cites an unresolved cited work.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Unresolved cited work

Reference 20

Resolution: unresolved; raw_fallback, observed 2026-08-14T13:24:13.342981Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 98f2cde6-b10c-4b6c-b023-1f33a14e617d · outbound

This paper cites an unresolved cited work.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Unresolved cited work

Reference 21

Resolution: unresolved; raw_fallback, observed 2026-08-14T13:24:13.332532Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation def1a807-8a72-45e8-a82e-85bce210b6f2 · outbound

This paper cites an unresolved cited work.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Unresolved cited work

Reference 22

Resolution: unresolved; raw_fallback, observed 2026-08-14T13:24:13.322901Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 7c448c4a-a9ac-40a8-a271-3c509d58de00 · outbound

This paper cites voltages.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields voltages

Reference 23

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T13:24:13.313161Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 7f36c250-c479-4f16-850a-5fb0d76f1bd3 · outbound

This paper cites One expects the vz→ 0 trajectories to already be co-rotating with the ISM and ∆ ⃗ p→ 0 so the assumption that the distribution is not signiﬁcantly modiﬁed is in error.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields One expects the vz→ 0 trajectories to already be co-rotating with the ISM and ∆ ⃗ p→ 0 so the assumption that the distribution is not signiﬁcantly modiﬁed is in error

Reference 24

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T13:24:13.303425Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation c07cfb92-28e9-46a6-8c8c-534453a6cbb8 · outbound

This paper cites (44) where σ is the 1-D velocity dispersion.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields (44) where σ is the 1-D velocity dispersion

Reference 25

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T13:24:13.291766Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 59d1a278-6094-4221-8d5d-aef479e191cb · outbound

This paper cites We fully expect τsd to ﬂuctuate within a galaxy and over the history of a galaxy.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields We fully expect τsd to ﬂuctuate within a galaxy and over the history of a galaxy

Reference 26

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T13:24:13.281093Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation dac624ca-8124-44aa-8492-3e1e4f809f51 · outbound

This paper cites A rough estimate of when spin-up can occur is when Rρ qdm≤ Σism.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields A rough estimate of when spin-up can occur is when Rρ qdm≤ Σism

Reference 27

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T13:24:13.270507Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 47ea1d53-829c-4586-be0a-8bb32bbfe8fb · outbound

This paper cites Here we suppose that these evolutionary eﬀects can be modeled as if the current conﬁguration has been constant over an interval of duration Tism.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Here we suppose that these evolutionary eﬀects can be modeled as if the current conﬁguration has been constant over an interval of duration Tism

Reference 28

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T13:24:13.258874Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 1a171c2e-ffd8-4379-8542-90a02f40bcec · outbound

This paper cites an unresolved cited work.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Unresolved cited work

Reference 29

Resolution: unresolved; raw_fallback, observed 2026-08-14T13:24:13.248106Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 1dfba9b2-26d5-4b02-bfb1-77da98ecd130 · outbound

This paper cites brown dwarfs and atomic hydrogen.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields brown dwarfs and atomic hydrogen

Reference 30

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T13:24:13.237358Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation ff216c16-0a18-4f7e-9ca3-c95b9e7f9635 · outbound

This paper cites In this case, the pitch angle, ψ, is the angle between the spiral arms and the circular orbits.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields In this case, the pitch angle, ψ, is the angle between the spiral arms and the circular orbits

Reference 31

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T13:24:13.226452Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 90cb0e84-0332-46c5-bfaa-d05ab1c29935 · outbound

This paper cites Measured RM maps are signiﬁcantly more complicated than a dipole pattern.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Measured RM maps are signiﬁcantly more complicated than a dipole pattern

Reference 32

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T13:24:13.215395Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation aeb3ad13-2416-488b-931f-36f8a0aa6cb8 · outbound

This paper cites freeze-in.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields freeze-in

Reference 33

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T13:24:13.204112Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 819950cf-dd2f-4ee9-ad20-747287b8da87 · outbound

This paper cites Rotation Curves of Spiral Galaxies.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Rotation Curves of Spiral Galaxies

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.371325Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4388fac0-a641-4fe5-9b88-1a4da95903c4 · outbound

This paper cites The dark matter of gravitational lensing.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields The dark matter of gravitational lensing

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.375741Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 864a8023-307b-4ee0-ae61-28a288235872 · outbound

This paper cites Planck 2018 results. VI. Cosmological parameters.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Planck 2018 results. VI. Cosmological parameters

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.379643Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f4531679-af2b-4f4c-8cf9-71844f7693f8 · outbound

This paper cites Cosmological Structure Formation.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Cosmological Structure Formation

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.383595Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a90bf7e2-558f-4b84-ad97-dc6335403cfc · outbound

This paper cites A History of Dark Matter.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields A History of Dark Matter

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.387420Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5a964784-23d0-472b-a911-46eee6cb623b · outbound

This paper cites Updated Bounds on Milli-Charged Particles.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Updated Bounds on Milli-Charged Particles

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.391841Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0219074f-ccd8-4739-9b41-f84e2198237e · outbound

This paper cites WIMPZILLAS!.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields WIMPZILLAS!

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.396309Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f4f19131-bbe6-4633-8b08-26b16156d459 · outbound

This paper cites freeze-in.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields freeze-in

Reference 42

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T13:24:13.192469Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 24069934-528c-441a-b4a7-9516ec6d2846 · outbound

This paper cites The Interstellar Environment of our Galaxy.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields The Interstellar Environment of our Galaxy

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.401335Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 70dc3d2d-79f6-41b1-981a-7f930723193c · outbound

This paper cites Sterile Neutrinos as Dark Matter.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Sterile Neutrinos as Dark Matter

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.405679Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 316d0e56-bf1a-4669-82eb-9634d68d9fba · outbound

This paper cites Freeze-In Production of FIMP Dark Matter.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Freeze-In Production of FIMP Dark Matter

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.409803Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 28f1bc5f-10c4-4b78-a49a-8a0e5e94b478 · outbound

This paper cites The Four Basic Ways of Creating Dark Matter Through a Portal.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields The Four Basic Ways of Creating Dark Matter Through a Portal

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.413622Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 204b45f3-e551-45d8-8fcc-21d25c353c27 · outbound

This paper cites Making dark matter out of light: freeze-in from plasma effects.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Making dark matter out of light: freeze-in from plasma effects

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.417460Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 909f37f4-922c-44d2-bdaf-8fec336d985b · outbound

This paper cites On the local dark matter density.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields On the local dark matter density

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.421218Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 36258e80-8d5b-4b6c-ae14-04537be50933 · outbound

This paper cites A simple model for the evolution of disc galaxies: The Milky Way.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields A simple model for the evolution of disc galaxies: The Milky Way

Reference 49

Resolution: verified exact; local_arxiv, observed 2026-08-14T13:24:12.851244Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation ccc3ba94-1c39-4092-b1af-ce1f4107e818 · outbound

This paper cites Low-frequency Faraday rotation measures towards pulsars using LOFAR: probing the 3-D Galactic halo magnetic field.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Low-frequency Faraday rotation measures towards pulsars using LOFAR: probing the 3-D Galactic halo magnetic field

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.429178Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3b1447ac-8433-448e-9c95-48b799850c9f · outbound

This paper cites Pakmor, F.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Pakmor, F

Reference 51

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T13:24:13.181108Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation daa0e0c5-abf7-4a24-904c-7e904499ab34 · outbound

This paper cites an unresolved cited work.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Unresolved cited work

Reference 52

Resolution: unresolved; raw_fallback, observed 2026-08-14T13:24:13.171941Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 5a63753d-d58c-4d84-a0ca-da0968c7e6a4 · outbound

This paper cites Krall and A.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Krall and A

Reference 53

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T13:24:13.162092Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 2cbe143f-abeb-4add-98d0-bbfd36f046c3 · outbound

This paper cites Bland-Hawthorn and O.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Bland-Hawthorn and O

Reference 54

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T13:24:13.151847Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 4cd50ebc-4944-46f3-adf1-cb66a34271de · outbound

This paper cites Jungman, M.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Jungman, M

Reference 55

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T13:24:13.141503Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 8d731629-7bda-4b00-b688-bae69b84207a · outbound

This paper cites an unresolved cited work.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Unresolved cited work

Reference 56

Resolution: unresolved; raw_fallback, observed 2026-08-14T13:24:13.130074Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation a2a9bc57-cfd5-49c2-8481-168c2b5bb839 · outbound

This paper cites The Local Dark Matter Density.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields The Local Dark Matter Density

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.455284Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8bc5bed7-7d3e-4c96-ba01-5005e29cb20b · outbound

This paper cites an unresolved cited work.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Unresolved cited work

Reference 58

Resolution: unresolved; raw_fallback, observed 2026-08-14T13:24:13.117727Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 9dedd07e-bd4c-4d8f-a955-9fde11262333 · outbound

This paper cites an unresolved cited work.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Unresolved cited work

Reference 59

Resolution: unresolved; raw_fallback, observed 2026-08-14T13:24:13.106671Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation d0615a3e-1943-46f7-8f5a-9bdbee795745 · outbound

This paper cites Constraining a Thin Dark Matter Disk with Gaia.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Constraining a Thin Dark Matter Disk with Gaia

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.466262Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation df640e95-b19a-48fc-8cd3-65f6ba312387 · outbound

This paper cites an unresolved cited work.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Unresolved cited work

Reference 61

Resolution: unresolved; raw_fallback, observed 2026-08-14T13:24:13.095759Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 684506bc-e5b1-45b1-bcea-e84c12d0184f · outbound

This paper cites an unresolved cited work.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Unresolved cited work

Reference 62

Resolution: unresolved; raw_fallback, observed 2026-08-14T13:24:13.085703Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation aceccefa-d1ff-4888-b8f8-6d019d01a6ee · outbound

This paper cites An improved map of the Galactic Faraday sky.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields An improved map of the Galactic Faraday sky

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.476923Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1860f90e-38ea-4b2e-8c82-75fd0533b759 · outbound

This paper cites Han, Annual Review of Astronomy and Astrophysics 55, 111 (2017).

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Han, Annual Review of Astronomy and Astrophysics 55, 111 (2017)

Reference 64

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T13:24:13.074758Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 8e5bbb7d-5f9e-43ea-910a-7efb4b44787b · outbound

This paper cites an unresolved cited work.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Unresolved cited work

Reference 65

Resolution: unresolved; raw_fallback, observed 2026-08-14T13:24:13.062991Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 8cd04374-5f13-4457-863d-fff7ff813e3f · outbound

This paper cites The Magnetic Field of the Milky Way Galaxy.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields The Magnetic Field of the Milky Way Galaxy

Reference 66

Resolution: verified exact; local_arxiv, observed 2026-08-14T13:24:12.793218Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 45d484d0-8682-4107-8ffd-2f8a0a9d30ce · outbound

This paper cites Search for Millicharged Particles at SLAC.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Search for Millicharged Particles at SLAC

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.495687Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 46f39c17-d338-48bd-b08a-e7867ff104a0 · outbound

This paper cites Dark Radiation constraints on minicharged particles in models with a hidden photon.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Dark Radiation constraints on minicharged particles in models with a hidden photon

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.503868Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1aa9f807-65ea-46c2-a69f-011781709382 · outbound

This paper cites Tighter Limits on Dark Matter Explanations of the Anomalous EDGES 21cm Signal.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Tighter Limits on Dark Matter Explanations of the Anomalous EDGES 21cm Signal

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.507911Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bbbd7afd-dedb-4a34-a0aa-c391d32770da · outbound

This paper cites Turning off the Lights: How Dark is Dark Matter?.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Turning off the Lights: How Dark is Dark Matter?

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.511603Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b194c33d-b17f-4089-8acb-24198a39ce5a · outbound

This paper cites First Direct Detection Limits on sub-GeV Dark Matter from XENON10.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields First Direct Detection Limits on sub-GeV Dark Matter from XENON10

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.514953Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8e674cd6-ed0b-4779-ad13-412e2046521b · outbound

This paper cites New Constraints and Prospects for sub-GeV Dark Matter Scattering off Electrons in Xenon.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields New Constraints and Prospects for sub-GeV Dark Matter Scattering off Electrons in Xenon

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.518540Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e0ecc83a-9bd8-4d8d-9926-85e2c99fcc53 · outbound

This paper cites Direct Detection is testing Freeze-in.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Direct Detection is testing Freeze-in

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.522375Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c83c1d45-11b1-4098-8b8d-c258254e822f · outbound

This paper cites CHAMP Cosmic Rays.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields CHAMP Cosmic Rays

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.526496Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 70acb61c-8b51-4ec1-b613-cbc646054895 · outbound

This paper cites US Cosmic Visions: New Ideas in Dark Matter 2017: Community Report.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields US Cosmic Visions: New Ideas in Dark Matter 2017: Community Report

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.530235Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 55e59c3c-bf07-4d25-b93c-a14019371c83 · outbound

This paper cites Bowman, A.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Bowman, A

Reference 77

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T13:24:13.052269Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation b3f8a464-0eb5-4d86-a2ee-435bcacc6428 · outbound

This paper cites Barkana, Nature 555, 71 (2018).

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Barkana, Nature 555, 71 (2018)

Reference 78

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T13:24:13.040461Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation deb23aed-1551-4e8b-b0df-dec025c2d5d3 · outbound

This paper cites Constraining Baryon--Dark Matter Scattering with the Cosmic Dawn 21-cm Signal.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Constraining Baryon--Dark Matter Scattering with the Cosmic Dawn 21-cm Signal

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.541593Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a4beaa09-8c84-404b-9710-b847aa7cbbd4 · outbound

This paper cites The Effects of Dark Matter-Baryon Scattering on Redshifted 21 cm Signals.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields The Effects of Dark Matter-Baryon Scattering on Redshifted 21 cm Signals

Reference 80

Resolution: verified exact; local_arxiv, observed 2026-08-14T13:24:12.654498Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 13847ac6-9d59-4459-9549-3777dfcedd66 · outbound

This paper cites Heating of Baryons due to Scattering with Dark Matter During the Dark Ages.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Heating of Baryons due to Scattering with Dark Matter During the Dark Ages

Reference 81

Resolution: verified exact; local_arxiv, observed 2026-08-14T13:24:12.639358Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation bd989a71-e61d-4935-abed-dac4ca9b1221 · outbound

This paper cites Supernova 1987A Constraints on Sub-GeV Dark Sectors, Millicharged Particles, the QCD Axion, and an Axion-like Particle.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Supernova 1987A Constraints on Sub-GeV Dark Sectors, Millicharged Particles, the QCD Axion, and an Axion-like Particle

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.554748Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ba667dd8-8030-4bbb-bec4-50207d546d01 · outbound

This paper cites Make Dark Matter Charged Again.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Make Dark Matter Charged Again

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.558213Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4afe6536-9854-4423-971e-d35ff7370b2a · outbound

This paper cites A new constraint on millicharged dark matter from galaxy clusters.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields A new constraint on millicharged dark matter from galaxy clusters

Reference 84

Resolution: verified exact; local_arxiv, observed 2026-08-14T13:24:12.779105Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 6fda66dd-363a-428e-8053-fadffc530ef7 · outbound

This paper cites an unresolved cited work.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Unresolved cited work

Reference 85

Resolution: unresolved; raw_fallback, observed 2026-08-14T13:24:13.029207Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation aab3690e-0fc5-4b2c-b463-0043d848ff83 · outbound

This paper cites an unresolved cited work.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Unresolved cited work

Reference 86

Resolution: unresolved; raw_fallback, observed 2026-08-14T13:24:13.018826Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 91e18f4d-6a1d-497e-93bc-9e7aa9ffcf05 · outbound

This paper cites Holdom, Phys.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Holdom, Phys

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.571903Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2fd1ab34-b673-41b6-84e4-21602fb0fcac · outbound

This paper cites Heating up the Galaxy with Hidden Photons.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields Heating up the Galaxy with Hidden Photons

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-14T13:24:12.575201Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 86b71ab1-d909-4fa0-a6b3-0474cf1c0fa7 · outbound

This paper cites dark photon.

New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields dark photon

Reference 89

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T13:24:13.001444Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Pith citing papers

Observation e18bf480-9911-432e-8667-85fb33e04d9b · inbound

Direct Deflection of Particle Dark Matter cites this paper.

Direct Deflection of Particle Dark Matter New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-14T12:39:17.826727Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 420c52a3-ded1-4c7a-8ca5-d74108c599a7 · inbound

Vector dark matter with non-abelian kinetic mixing cites this paper.

Vector dark matter with non-abelian kinetic mixing New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-04T07:13:10.619250Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 90be331e-8e26-411c-bd60-a45de273a1ac · inbound

Constraints and Projections for Millicharged Dark Matter in the Sun with Water Cherenkov Neutrino Detectors cites this paper.

Constraints and Projections for Millicharged Dark Matter in the Sun with Water Cherenkov Neutrino Detectors New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields

Reference 39

Resolution: verified exact; arxiv_id, observed 2026-07-03T02:57:34.986465Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.