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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 2026-08-15T06:32:42.880941+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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T14:28:20.059071Z digest=sha256:a2a78da75a0f9b7776116b736f4b03027005ca84ee4cc5e78672715d3ad65262

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 2026-08-15T06:32:42.880941+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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source=pdf_text observed=2026-08-14T14:28:20.084488Z digest=sha256:d3c615970fa9896ca5d18bc66f1d07f7f3fd4e0e3bf815f79d467ec4a252eb98

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:c9da51a8b781a839ba5486df0abf02da0809dd1c3f847d268fe9ef71685709e4

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 2026-08-15T06:32:42.880941+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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No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

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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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source=pdf_text observed=2026-08-14T14:28:20.121540Z digest=sha256:d1e0c27c19107bcf752ea4126e318635d6208e62321b1ae1d02dec9529e8dad4

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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source=pdf_text observed=2026-08-14T14:28:20.134086Z digest=sha256:752ed6d2f72e52452a20e95e2c769cc5fb7f8f36e901cca329ff039dda6ebac4

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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source=pdf_text observed=2026-08-14T14:28:20.127343Z digest=sha256:bc6102b1eaff1da59b38f102774cbe0803ad06590f2e9bfaa61ddd49b1a9a788

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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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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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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T14:28:20.182680Z digest=sha256:f06515188ff9c12dd7d44b6ec0168f5bd06d86e8a105d9c253f816987a7dcd62

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T14:28:20.198837Z digest=sha256:8280b606b715518b5997b2ca8c68319546488ef5ae40d1baf3ed5bc5fed36b16

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

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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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raw_fallback, observed 2026-08-14T14:28:21.414159Z

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No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T14:28:20.209196Z digest=sha256:07afee2e0cea84a43beb234aa0fbed3e352384ba78abee37aced84cfb6e935f9

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

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T14:28:20.214143Z digest=sha256:8582e12fd2e6c61d140c3d3e1ff3b5113d0c5bc8f29207339c6ea6d035d0957f

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

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T14:28:20.224557Z digest=sha256:9e818655cd850e1a10e4f987e96c625f572cf580b37d08d680dbca75ac9fba72

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

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No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T14:28:20.229685Z digest=sha256:dfcc9425754fa7ec6bd6f8463d420ad455d657ac3745feccf41c51913c81e2d4

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

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Unavailable: canonical work link unavailable.

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T14:28:20.247393Z digest=sha256:50956d7f524182ef45787d3906528b7d0bd0d94970ca57eb2029945faf7e2687

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T14:28:20.267675Z digest=sha256:fc6b4e74c916a90dfd938dcf515fb9e3031ae31b36422c46049bd30407da40c3

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T14:28:20.257626Z digest=sha256:4fae6378c6f2d9c608ad710eebd72c0a289bcad63de36767a113bfc1384a25f5

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=sha256:2db62ceaec7e04a67c6b027034649ac29cb29bbbf1225913e684b15728a9840c

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T14:28:20.315641Z digest=sha256:45db9b87cd336f48df3a99e3e67b290be6d1d68f4dfc8150cb56de3ecaef3969

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=sha256:5a7f7abb8ccb5b0e1e8d08f94780c9908be248eb3371eff81b71a5d7c0ff3e42

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T14:28:20.065809Z digest=sha256:703c3a60661fa6793c47ef0737b6379c12eb9a7a53ef362159488681f0662ec0

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-05-18T23:02:15.483780Z digest=sha256:c1bbb649c5dfc84a79653b4bc458c25af46bd8f87019c7701f49ea9839c30128