Paper Citation Record · LEDGER

Evidences of low-diffusion bubbles around Galactic pulsars

As of 23 August 2026, this Paper Citation Record lists 50 of 50 outbound references and 3 inbound Pith citation observations for arXiv:1908.03216.

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

pith.paper-citation-record.v1
1908.03216 v2

Coverage vector

measured 50 of 50 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-14T14:28:20.331878Z

measured 53 of 53 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-23T06:30:58.430688+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T04:55:36.246734Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-18T23:02:52.402876Z

Reference resolution

50 of 50 outbound references displayed

verified exact6
verified fuzzy2
unresolved37
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malformed identifier3
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External citation measurements

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Outbound references

Observation 23f941b6-d301-4f43-81b4-b27aa749c704 · outbound

This paper cites an unresolved cited work.

Evidences of low-diffusion bubbles around Galactic pulsars Unresolved cited work

Reference 1

Resolution: malformed identifier; raw_fallback, observed 2026-08-14T14:28:21.364761Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 9a7dd593-bc44-4539-801a-6d1dde078c1e · outbound

This paper cites Milagro Observations of Multi-TeV Emission from Galactic Sources in the Fermi Bright Source List.

Evidences of low-diffusion bubbles around Galactic pulsars Milagro Observations of Multi-TeV Emission from Galactic Sources in the Fermi Bright Source List

Reference 2

Resolution: verified exact; local_arxiv, observed 2026-08-14T14:28:21.269999Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation eb8682fc-e8df-46e2-9be2-4ab01e154a82 · outbound

This paper cites Detection of a $\gamma$-ray halo around Geminga with the Fermi-LAT and implications for the positron flux.

Evidences of low-diffusion bubbles around Galactic pulsars Detection of a $\gamma$-ray halo around Geminga with the Fermi-LAT and implications for the positron flux

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.084488Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ef025239-7a7b-41fd-868d-9d672ac23a71 · outbound

This paper cites Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth.

Evidences of low-diffusion bubbles around Galactic pulsars Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.071504Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3cddd9e1-95a5-4af6-ab9d-88d9065f1283 · outbound

This paper cites Measurement of separate cosmic-ray electron and positron spectra with the Fermi Large Area Telescope.

Evidences of low-diffusion bubbles around Galactic pulsars Measurement of separate cosmic-ray electron and positron spectra with the Fermi Large Area Telescope

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.096218Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation efb65e0d-767e-4925-b750-935137de2bde · outbound

This paper cites Aguilar, L.

Evidences of low-diffusion bubbles around Galactic pulsars Aguilar, L

Reference 6

Resolution: malformed identifier; raw_fallback, observed 2026-08-14T14:28:21.466478Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 734c20bc-d61c-41d7-ad4e-25c9161cb9e8 · outbound

This paper cites The cosmic-ray positron energy spectrum measured by PAMELA.

Evidences of low-diffusion bubbles around Galactic pulsars The cosmic-ray positron energy spectrum measured by PAMELA

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.090285Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 72bd3f4b-4314-4eeb-80d5-de7ea8a8e559 · outbound

This paper cites Theoretical uncertainties in extracting cosmic-ray diffusion parameters: the boron-to-carbon ratio.

Evidences of low-diffusion bubbles around Galactic pulsars Theoretical uncertainties in extracting cosmic-ray diffusion parameters: the boron-to-carbon ratio

Reference 8

Resolution: verified exact; local_arxiv, observed 2026-08-14T14:28:21.167231Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 56ddf347-b041-4140-a728-70ce46cb110f · outbound

This paper cites Cosmic-ray transport from AMS-02 B/C data: benchmark models and interpretation.

Evidences of low-diffusion bubbles around Galactic pulsars Cosmic-ray transport from AMS-02 B/C data: benchmark models and interpretation

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.121540Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bfdf05c7-a407-4a6e-814d-4846814116d4 · outbound

This paper cites AMS-02 Antiprotons Reloaded.

Evidences of low-diffusion bubbles around Galactic pulsars AMS-02 Antiprotons Reloaded

Reference 10

Resolution: verified exact; local_arxiv, observed 2026-08-14T14:28:21.192397Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 23283c0e-9e1e-44e2-8afe-f611ab7410d2 · outbound

This paper cites On the TeV Halo Fraction in gamma-ray bright Pulsar Wind Nebulae.

Evidences of low-diffusion bubbles around Galactic pulsars On the TeV Halo Fraction in gamma-ray bright Pulsar Wind Nebulae

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.134086Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7fc97350-6189-4f90-84f8-e6a713f2c118 · outbound

This paper cites The H.E.S.S. Galactic plane survey.

Evidences of low-diffusion bubbles around Galactic pulsars The H.E.S.S. Galactic plane survey

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.139262Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5aeee53b-cc85-4ffe-b6ff-f4c853f182bd · outbound

This paper cites HAWC Observations Strongly Favor Pulsar Interpretations of the Cosmic-Ray Positron Excess.

Evidences of low-diffusion bubbles around Galactic pulsars HAWC Observations Strongly Favor Pulsar Interpretations of the Cosmic-Ray Positron Excess

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.127343Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 41a49673-4631-47c6-8142-f3942be90344 · outbound

This paper cites Positron flux and gamma-ray emission from Geminga pulsar and pulsar wind nebula.

Evidences of low-diffusion bubbles around Galactic pulsars Positron flux and gamma-ray emission from Geminga pulsar and pulsar wind nebula

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.150835Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation dd3e2db4-6bcc-4508-86ff-0eedac6ed2bd · outbound

This paper cites Two-zone diffusion of electrons and positrons from Geminga explains the positron anomaly.

Evidences of low-diffusion bubbles around Galactic pulsars Two-zone diffusion of electrons and positrons from Geminga explains the positron anomaly

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.156179Z

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Unavailable: canonical work link unavailable.

Observation 783ab2de-4054-4316-93ad-19308232d607 · outbound

This paper cites GeV observations of the extended pulsar wind nebulae constrain the pulsar interpretations of the cosmic-ray positron excess.

Evidences of low-diffusion bubbles around Galactic pulsars GeV observations of the extended pulsar wind nebulae constrain the pulsar interpretations of the cosmic-ray positron excess

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.145548Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a3aaf374-09f0-4bd3-9017-90d87685f8aa · outbound

This paper cites In the present study, we argue that the most promising energy range for searching for ICS halos is above 100 GeV, where IACTs, and HAWC and Milagro operate.

Evidences of low-diffusion bubbles around Galactic pulsars In the present study, we argue that the most promising energy range for searching for ICS halos is above 100 GeV, where IACTs, and HAWC and Milagro operate

Reference 17

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T14:28:21.501469Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation c02e5aef-5d73-4fca-9865-dfe2b04b13c8 · outbound

This paper cites Science with the Cherenkov Telescope Array.

Evidences of low-diffusion bubbles around Galactic pulsars Science with the Cherenkov Telescope Array

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.172417Z

Source-reported events for the cited work

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Observation e1b53dc9-192a-4ca9-8251-a7b78a087431 · outbound

This paper cites The 2HWC HAWC Observatory Gamma Ray Catalog.

Evidences of low-diffusion bubbles around Galactic pulsars The 2HWC HAWC Observatory Gamma Ray Catalog

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.161241Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3014cd56-fc2a-44d1-9e7c-e695730331c9 · outbound

This paper cites Hobbs, D.

Evidences of low-diffusion bubbles around Galactic pulsars Hobbs, D

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.166438Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7eb22484-5023-4c63-9217-cf8e41c4722c · outbound

This paper cites The theory of pulsar wind nebulae.

Evidences of low-diffusion bubbles around Galactic pulsars The theory of pulsar wind nebulae

Reference 21

Resolution: metadata mismatch; local_arxiv, observed 2026-08-14T14:28:20.845194Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation c1723b38-ba62-48a3-8336-7b44bb7ecf7a · outbound

This paper cites The ATNF Pulsar Catalogue.

Evidences of low-diffusion bubbles around Galactic pulsars The ATNF Pulsar Catalogue

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.177637Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 274692e5-97a8-4258-81e9-67b2e8b6b371 · outbound

This paper cites an unresolved cited work.

Evidences of low-diffusion bubbles around Galactic pulsars Unresolved cited work

Reference 23

Resolution: unresolved; raw_fallback, observed 2026-08-14T14:28:21.449256Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation e59fdb3f-599f-4fe8-92a7-492c26982216 · outbound

This paper cites A Dynamical Model for the Evolution of a Pulsar Wind Nebula inside a Non-Radiative Supernova Remnant.

Evidences of low-diffusion bubbles around Galactic pulsars A Dynamical Model for the Evolution of a Pulsar Wind Nebula inside a Non-Radiative Supernova Remnant

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.204020Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 96e4bbee-69bf-4c51-81da-d5206a0b758c · outbound

This paper cites The Evolution and Structure of Pulsar Wind Nebulae.

Evidences of low-diffusion bubbles around Galactic pulsars The Evolution and Structure of Pulsar Wind Nebulae

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.192427Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation af771e4c-db16-4552-b448-5a29a3f80163 · outbound

This paper cites an unresolved cited work.

Evidences of low-diffusion bubbles around Galactic pulsars Unresolved cited work

Reference 26

Resolution: unresolved; raw_fallback, observed 2026-08-14T14:28:21.430691Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 97ad3377-fb7f-43c0-ae61-f9b2af105caf · outbound

This paper cites TeV Gamma Rays from Geminga and the Origin of the GeV Positron Excess.

Evidences of low-diffusion bubbles around Galactic pulsars TeV Gamma Rays from Geminga and the Origin of the GeV Positron Excess

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.219267Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 91dbab4c-bd78-48f1-9578-a8e4d4c231b2 · outbound

This paper cites van der Swaluw, A.

Evidences of low-diffusion bubbles around Galactic pulsars van der Swaluw, A

Reference 28

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T14:28:21.414159Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 804981c2-770a-42ba-8fa4-384f9a1e2055 · outbound

This paper cites an unresolved cited work.

Evidences of low-diffusion bubbles around Galactic pulsars Unresolved cited work

Reference 29

Resolution: unresolved; raw_fallback, observed 2026-08-14T14:28:21.397433Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation bcdb2467-914d-4f30-b63b-7fdd81817c01 · outbound

This paper cites Lessons from HAWC PWNe observations: the diffusion constant is not a constant; Pulsars remain the likeliest sources of the anomalous positron fraction; Cosmic rays are trapped for long periods of time in pockets of inefficient diffusion.

Evidences of low-diffusion bubbles around Galactic pulsars Lessons from HAWC PWNe observations: the diffusion constant is not a constant; Pulsars remain the likeliest sources of the anomalous positron fraction; Cosmic rays are trapped for long periods of time in pockets of inefficient diffusion

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.236329Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1c8312b8-a330-4854-83ef-7b96d5ff1a1d · outbound

This paper cites A Cosmic Ray Positron Anisotropy due to Two Middle-Aged, Nearby Pulsars?.

Evidences of low-diffusion bubbles around Galactic pulsars A Cosmic Ray Positron Anisotropy due to Two Middle-Aged, Nearby Pulsars?

Reference 31

Resolution: verified exact; local_arxiv, observed 2026-08-14T14:28:20.751500Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation f8cd7633-fa04-45ab-87bb-219e770b8357 · outbound

This paper cites Modeling of the Radio Emission from the Vela Supernova Remnant.

Evidences of low-diffusion bubbles around Galactic pulsars Modeling of the Radio Emission from the Vela Supernova Remnant

Reference 32

Resolution: verified exact; local_arxiv, observed 2026-08-14T14:28:20.723185Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 7dc01b6d-f5b3-473c-81f1-83e0ff1e24f8 · outbound

This paper cites Geminga's puzzling pulsar wind nebula.

Evidences of low-diffusion bubbles around Galactic pulsars Geminga's puzzling pulsar wind nebula

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.252670Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 721e379d-cb51-45a0-8d39-0c4d010fd020 · outbound

This paper cites Self-Generated Cosmic-Ray Confinement in TeV Halos: Implications for TeV Gamma-Ray Emission and the Positron Excess.

Evidences of low-diffusion bubbles around Galactic pulsars Self-Generated Cosmic-Ray Confinement in TeV Halos: Implications for TeV Gamma-Ray Emission and the Positron Excess

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.242065Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bb3e9e8d-f0ef-4c04-b2d3-24b3a6150d33 · outbound

This paper cites Pulsar Wind Nebulae.

Evidences of low-diffusion bubbles around Galactic pulsars Pulsar Wind Nebulae

Reference 35

Resolution: metadata mismatch; local_arxiv, observed 2026-08-14T14:28:20.657560Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation e08ce13e-5cb8-4870-a58a-59a920818b83 · outbound

This paper cites Galactic electrons and positrons at the Earth:new estimate of the primary and secondary fluxes.

Evidences of low-diffusion bubbles around Galactic pulsars Galactic electrons and positrons at the Earth:new estimate of the primary and secondary fluxes

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.267675Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 909e3ce5-1ca6-490d-9c0d-39a8fa4d2ffb · outbound

This paper cites an unresolved cited work.

Evidences of low-diffusion bubbles around Galactic pulsars Unresolved cited work

Reference 37

Resolution: unresolved; raw_fallback, observed 2026-08-14T14:28:21.381494Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 91960dc8-9fd9-412c-aef7-40aba7ded6df · outbound

This paper cites PPPC 4 DM ID: A Poor Particle Physicist Cookbook for Dark Matter Indirect Detection.

Evidences of low-diffusion bubbles around Galactic pulsars PPPC 4 DM ID: A Poor Particle Physicist Cookbook for Dark Matter Indirect Detection

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.262695Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 61499b60-bec2-4608-ab2b-56c438cb5e47 · outbound

This paper cites A radiation transfer model for the Milky-Way: I. Radiation fields and application to High Energy Astrophysics.

Evidences of low-diffusion bubbles around Galactic pulsars A radiation transfer model for the Milky-Way: I. Radiation fields and application to High Energy Astrophysics

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.286052Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation baa917c8-29c7-4c16-8773-02f19643768f · outbound

This paper cites Absorption of Very High Energy Gamma Rays in the Milky Way.

Evidences of low-diffusion bubbles around Galactic pulsars Absorption of Very High Energy Gamma Rays in the Milky Way

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.274405Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 379fdd9e-c1f8-4ae4-982f-ffd13d813638 · outbound

This paper cites Inverse Compton Emission from Galactic Supernova Remnants: Effect of the Interstellar Radiation Field.

Evidences of low-diffusion bubbles around Galactic pulsars Inverse Compton Emission from Galactic Supernova Remnants: Effect of the Interstellar Radiation Field

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.280091Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0e7c8b89-f515-4939-b52b-e07198b635bb · outbound

This paper cites The population of TeV pulsar wind nebulae in the H.E.S.S. Galactic Plane Survey.

Evidences of low-diffusion bubbles around Galactic pulsars The population of TeV pulsar wind nebulae in the H.E.S.S. Galactic Plane Survey

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.303629Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ad4c1ca9-7273-4013-9314-c857584ab1fb · outbound

This paper cites A statistical study of 233 pulsar proper motions.

Evidences of low-diffusion bubbles around Galactic pulsars A statistical study of 233 pulsar proper motions

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.291817Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8ac75bb8-53cc-4de6-ad06-b43cb1e43bd8 · outbound

This paper cites Fermi Large Area Telescope Third Source Catalog.

Evidences of low-diffusion bubbles around Galactic pulsars Fermi Large Area Telescope Third Source Catalog

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.297399Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 51f1aba4-a8d7-49bc-a827-1ed6c263da71 · outbound

This paper cites HAWC High Energy Upgrade with a Sparse Outrigger Array.

Evidences of low-diffusion bubbles around Galactic pulsars HAWC High Energy Upgrade with a Sparse Outrigger Array

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.321177Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3949751c-50fa-47ab-b778-1703d5409da0 · outbound

This paper cites The Cherenkov Telescope Array.

Evidences of low-diffusion bubbles around Galactic pulsars The Cherenkov Telescope Array

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.309663Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f04f4111-9d0f-469b-b399-1d67374f0031 · outbound

This paper cites On the potential of Cherenkov Telescope Arrays and KM3 Neutrino Telescopes for the detection of extended sources.

Evidences of low-diffusion bubbles around Galactic pulsars On the potential of Cherenkov Telescope Arrays and KM3 Neutrino Telescopes for the detection of extended sources

Reference 47

Resolution: verified exact; local_arxiv, observed 2026-08-14T14:28:20.441385Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation c5e3204c-b54b-4269-8ca5-7398e5f07447 · outbound

This paper cites Positrons from pulsar winds.

Evidences of low-diffusion bubbles around Galactic pulsars Positrons from pulsar winds

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.326589Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e267b427-d62d-413f-8f38-ab2243147b63 · outbound

This paper cites Time-dependent modeling of TeV-detected, young pulsar wind nebulae.

Evidences of low-diffusion bubbles around Galactic pulsars Time-dependent modeling of TeV-detected, young pulsar wind nebulae

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-14T14:28:20.331878Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8f05699b-0c35-4462-9533-ada7dfad00e7 · outbound

This paper cites If this factor is considered in their calculation, many of their sources would have a e± density comparable to the one of the ISM.

Evidences of low-diffusion bubbles around Galactic pulsars If this factor is considered in their calculation, many of their sources would have a e± density comparable to the one of the ISM

Reference 105

Resolution: malformed identifier; raw_fallback, observed 2026-08-14T14:28:21.482806Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Pith citing papers

Observation 044495ee-a65d-4f1c-bc59-e97552866234 · inbound

Extended TeV Halos May Commonly Exist around Middle-Aged Pulsars cites this paper.

Extended TeV Halos May Commonly Exist around Middle-Aged Pulsars Evidences of low-diffusion bubbles around Galactic pulsars

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-16T04:54:30.234519Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b8b9061b-e125-4653-90e5-c79d010d80f7 · inbound

Absence of TeV halos around millisecond pulsars cites this paper.

Absence of TeV halos around millisecond pulsars Evidences of low-diffusion bubbles around Galactic pulsars

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-16T04:55:36.246734Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b052fbfa-8363-4512-bc4c-4121ea89dd5a · inbound

PHECT: A lightweight computation tool for pulsar halo emission cites this paper.

PHECT: A lightweight computation tool for pulsar halo emission Evidences of low-diffusion bubbles around Galactic pulsars

Reference 24

Resolution: verified exact; arxiv_id, observed 2026-05-18T23:02:52.406064Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.