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Paper Citation Record · LEDGER

Evidences of low-diffusion bubbles around Galactic pulsars

As of 15 August 2026, this Paper Citation Record lists 50 of 50 outbound references and 1 inbound Pith citation observation 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 51 of 51 standing notices

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

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-05-18T23:02:15.483780Z

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

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  • verified fuzzy2
  • unresolved37
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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

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

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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

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local_arxiv, observed 2026-08-14T14:28:21.269999Z

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

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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

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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

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source=pdf_text observed=2026-08-14T14:28:20.071504Z digest=sha256:746f65bd3ca414736f91e02896df68591c127f6e4a6d8cb4ede59fe7535a4043

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

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source=pdf_text observed=2026-08-14T14:28:20.096218Z digest=sha256:be8fc69464cf28a831a8005db0c8bc6a25967944da753d2f0eb1835bad70a75f

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

This paper cites Aguilar, L.

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

Reference 6

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

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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

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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

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local_arxiv, observed 2026-08-14T14:28:21.167231Z

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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

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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

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local_arxiv, observed 2026-08-14T14:28:21.192397Z

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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

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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

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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

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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

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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

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source=pdf_text observed=2026-08-14T14:28:20.156179Z digest=sha256:b1b6b0766a45aabd91e3f965cb66b2fc8ea5cd1459e7268d1188b29a133ba6e2

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

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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

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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

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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

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

This paper cites Hobbs, D.

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

Reference 20

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source=pdf_text observed=2026-08-14T14:28:20.166438Z digest=sha256:af8c4a1d44fb689f88d14b137a0b6b6e5b2b5ced9c7d18debe1b29af55f632d0

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

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local_arxiv, observed 2026-08-14T14:28:20.845194Z

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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

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source=pdf_text observed=2026-08-14T14:28:20.177637Z digest=sha256:2e50ca52b8fe3467cb1594da455470d24c8606ac5acbfccfd7b265d5dcfd657e

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

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

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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

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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

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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

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

source=pdf_text observed=2026-08-14T14:28:20.198837Z digest=sha256:3a30c97ec60923a2575e7d76f1ce21764fb1809de42ca85edd28035071aad5bc

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

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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

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

source=pdf_text observed=2026-08-14T14:28:20.209196Z digest=sha256:0182001f267e589f795659d16ef652e89b1e8370efe0ca738d436a5efc1dafb1

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

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

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

source=pdf_text observed=2026-08-14T14:28:20.214143Z digest=sha256:178425c74a522361f9a26a249b3a616c15c5a46cdee4d3434aa10c6f6b9dde58

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

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

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source=pdf_text observed=2026-08-14T14:28:20.236329Z digest=sha256:f6c092f3b20a59a470b96dec28d328558a9d83a6902b1f7e81be1f6c9e4c62fb

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

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

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

source=pdf_text observed=2026-08-14T14:28:20.224557Z digest=sha256:dcb64150551f536bc605a838ec905c58ae0a3fbf33f6f67b98ab15f53138b756

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

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local_arxiv, observed 2026-08-14T14:28:20.723185Z

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

source=pdf_text observed=2026-08-14T14:28:20.229685Z digest=sha256:325b3e5bebec46ea57410d7a378ea303d816e24bb62f4655ad92d78f4a5dfb61

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

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

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source=pdf_text observed=2026-08-14T14:28:20.252670Z digest=sha256:1fc3b8edbeb2cb2524e41ced4b197203e73be772d013415d5a5bb2089c915bf5

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

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source=pdf_text observed=2026-08-14T14:28:20.242065Z digest=sha256:03d290f6a8044de7d3b785e5cd20520a68c994be76d9cc198cae8b88abbeff21

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

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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 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-14T14:28:20.247393Z digest=sha256:c85665ef7fd0deb711d6f2c18ba9cd790538104d686ad20158bce688f98399fa

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

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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T14:28:20.267675Z digest=sha256:9a329781186696c8e2d3aabcd7940c060a4deeb2faccf25b9fc59b5690c2b0d0

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 2026-08-14T06:32:32.682623+00:00.

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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.

source=pdf_text observed=2026-08-14T14:28:20.262695Z digest=sha256:aee8e083b183b7dc3b129e4628b999a672b1e1951d516a8ca3468a193d7dab22

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.

source=pdf_text observed=2026-08-14T14:28:20.286052Z digest=sha256:81c251d4699a3f6ddac1cde1a8fcb8d61b6a9f70d59c440cb1e1f33203fab706

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.

source=pdf_text observed=2026-08-14T14:28:20.274405Z digest=sha256:b6d819572a59e1c5a766de33deb509da5cfe0f5e5ced030ab3d14cafad31687b

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.

source=pdf_text observed=2026-08-14T14:28:20.280091Z digest=sha256:dee094f9c75ceb0ec41e4d2a14133e9440b4d94e4236475fc4771da88e48502a

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.

source=pdf_text observed=2026-08-14T14:28:20.303629Z digest=sha256:b823e8a5182d29590c949dfdb4812106ffb1de44779aaff6821bf594475a1772

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.

source=pdf_text observed=2026-08-14T14:28:20.291817Z digest=sha256:ded35c9fce1dc0cd2d235ac23680e6bf0c0fb7358e6a98aa2f62a2178cafde78

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.

source=pdf_text observed=2026-08-14T14:28:20.297399Z digest=sha256:9b7e46b6978804c1503e1bc6a094076b6f327d19bb8724845a9ede3d63aec532

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.

source=pdf_text observed=2026-08-14T14:28:20.321177Z digest=sha256:ca57a179ddddfaaf975fed00cce1784e22a8c15b856e9813c250f45444ad64db

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.

source=pdf_text observed=2026-08-14T14:28:20.309663Z digest=sha256:e62c06c4cdba3acb4d8d38d1af7f7c64617610e94ceae8df5997c39eafc821ad

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 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-14T14:28:20.315641Z digest=sha256:419b390101a18e3b406ee20ec5e64879ccedee088de1be37495a72c3222d32a8

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.

source=pdf_text observed=2026-08-14T14:28:20.326589Z digest=sha256:1c2decf8479420979b94f84c23d357e049dd79c6435cf13cdd8daf5d4a4e6b64

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.

source=pdf_text observed=2026-08-14T14:28:20.331878Z digest=sha256:92ded2a8a232e3153d139220589ba0f6531911f4e54f6dead367f23cf12cc47a

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 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-14T14:28:20.065809Z digest=sha256:b17794c5ffb10082ff95f582bc210b85b2a8ab92aec85297b860b93f005b99a5

Pith citing papers

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 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-05-18T23:02:15.483780Z digest=sha256:df37b7ccaaa336fbcd7449c655feb088e8543883190635e467e077bed9befa54