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Paper Citation Record · LEDGER

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion

As of 20 August 2026, this Paper Citation Record lists 91 of 91 outbound references and 1 inbound Pith citation observation for arXiv:2605.15261.

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

pith.paper-citation-record.v1
2605.15261 v1

Coverage vector

measured 91 of 91 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-05-19T16:10:46.102334Z

measured 92 of 92 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-20T06:33:59.587034+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-09T14:56:45.760028Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-09T15:06:18.226837Z

Reference resolution

91 of 91 outbound references displayed

  • verified exact51
  • verified fuzzy20
  • unresolved19
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  • malformed identifier0
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External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 326d253f-3a21-4b16-994a-deb1a21d1ecc · outbound

This paper cites an unresolved cited work.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Unresolved cited work

Reference 1

Resolution
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Source-reported events for the cited work

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Observation 0f7e5484-3b03-41e0-9680-14ae00bd2eea · outbound

This paper cites an unresolved cited work.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Unresolved cited work

Reference 2

Resolution
unresolved
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Source-reported events for the cited work

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Observation 4412ca58-0ea0-4de8-984a-4ef268d21744 · outbound

This paper cites Weinberg,A New Light Boson?,Phys.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Weinberg,A New Light Boson?,Phys

Reference 3

Resolution
verified fuzzy
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Source-reported events for the cited work

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Observation d5f2dfbf-6d20-44e7-9e5c-20e0b34735e0 · outbound

This paper cites Wilczek,Problem of Strong P and T Invariance in the Presence of Instantons,Phys.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Wilczek,Problem of Strong P and T Invariance in the Presence of Instantons,Phys

Reference 4

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation 0f6a526b-9d13-485b-b269-8cab4d4a88e3 · outbound

This paper cites an unresolved cited work.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Unresolved cited work

Reference 5

Resolution
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation c5a7bd9f-4495-4ae9-95e4-5f97a8261c30 · outbound

This paper cites an unresolved cited work.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Unresolved cited work

Reference 6

Resolution
unresolved
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation ba027ee8-cea5-453e-9ceb-f0bab8cbdb9a · outbound

This paper cites an unresolved cited work.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Unresolved cited work

Reference 7

Resolution
unresolved
raw_fallback, observed 2026-05-19T16:13:08.238760Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation 579f8cf8-7b63-4891-a4c0-27606414e4e8 · outbound

This paper cites an unresolved cited work.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Unresolved cited work

Reference 8

Resolution
unresolved
raw_fallback, observed 2026-05-19T16:13:08.255633Z

Source-reported events for the cited work

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Observation 9e5d2af9-989b-4a49-be38-3a0ae7667c8c · outbound

This paper cites The landscape of QCD axion models.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion The landscape of QCD axion models

Reference 9

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:12:38.964141Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation 1ec3f23c-1d55-430c-b3d2-18263484d36f · outbound

This paper cites Preskill, M.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Preskill, M

Reference 10

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation 5e0842c5-7d23-4eaa-b917-ddaf4f2aea5c · outbound

This paper cites an unresolved cited work.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Unresolved cited work

Reference 11

Resolution
unresolved
raw_fallback, observed 2026-05-19T16:13:08.250164Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation e18c61c6-ae1f-4a6b-a9db-00fa24aa82cc · outbound

This paper cites Dine and W.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Dine and W

Reference 12

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation 6c570d7c-b614-46d0-8626-d641ae5aff81 · outbound

This paper cites Cosmology of axion dark matter.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Cosmology of axion dark matter

Reference 13

Resolution
verified exact
arxiv_id, observed 2026-05-19T16:12:38.961479Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation 14a40aa2-821f-4a39-a345-b62b2fa1454d · outbound

This paper cites Axions In String Theory.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Axions In String Theory

Reference 14

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:12:38.969645Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation c9a7e316-919c-4bfe-a399-9f2d94fa742b · outbound

This paper cites String Axiverse.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion String Axiverse

Reference 15

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:12:38.955536Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation c112b368-80ee-4b7c-a9cd-c40e574aef79 · outbound

This paper cites The type IIB string axiverse and its low-energy phenomenology.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion The type IIB string axiverse and its low-energy phenomenology

Reference 16

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:12:38.958264Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation 054b52c2-4690-4b3c-8536-9524ad1c17e1 · outbound

This paper cites The Kreuzer-Skarke Axiverse.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion The Kreuzer-Skarke Axiverse

Reference 17

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:12:38.966822Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation 5458b956-f703-4ef4-b6d1-6bcbdb1d3fbe · outbound

This paper cites On String Theory Expectations for Photon Couplings to Axion-Like Particles.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion On String Theory Expectations for Photon Couplings to Axion-Like Particles

Reference 18

Resolution
verified exact
arxiv_id, observed 2026-05-19T16:12:39.067542Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation 2bbc269d-5ffa-415b-a0b0-7ab0cb05a74d · outbound

This paper cites PQ Axiverse.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion PQ Axiverse

Reference 19

Resolution
verified exact
arxiv_id, observed 2026-05-19T16:12:39.098444Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:90eb8c820e5024413d33953f2f8614b55a8b4a51944586646f20eb3e5cbd4f90

Observation 4fd72713-e157-47f7-b302-231dda62a02e · outbound

This paper cites Glimmers from the Axiverse.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Glimmers from the Axiverse

Reference 20

Resolution
verified exact
arxiv_id, observed 2026-05-19T16:12:39.092432Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation 4d353cb0-0f00-497f-a2e5-4da78dd04999 · outbound

This paper cites Sikivie,Experimental Tests of the Invisible Axion, Phys.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Sikivie,Experimental Tests of the Invisible Axion, Phys

Reference 21

Resolution
verified fuzzy
raw_fallback, observed 2026-05-19T16:13:08.236281Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation c8984281-b81e-4df4-aba9-4597711e4aea · outbound

This paper cites Raffelt and L.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Raffelt and L

Reference 22

Resolution
verified fuzzy
raw_fallback, observed 2026-05-19T16:13:08.226997Z

Source-reported events for the cited work

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Observation 435d84c3-896b-4944-b9b0-01eb2e38b3bc · outbound

This paper cites Experimental Searches for the Axion and Axion-like Particles.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Experimental Searches for the Axion and Axion-like Particles

Reference 23

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:12:39.095368Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation 5771bf1b-42b6-4b00-9ab4-de807728ec00 · outbound

This paper cites New experimental approaches in the search for axion-like particles.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion New experimental approaches in the search for axion-like particles

Reference 24

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:12:39.086129Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation 55fcd958-c708-4fd2-92cc-ca1655ce1481 · outbound

This paper cites Invisible Axion Search Methods.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Invisible Axion Search Methods

Reference 25

Resolution
verified exact
arxiv_id, observed 2026-05-19T16:12:39.089197Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation acff03fb-65b1-4277-a928-4d0c0bcb0402 · outbound

This paper cites New Technologies for Axion and Dark Photon Searches.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion New Technologies for Axion and Dark Photon Searches

Reference 26

Resolution
verified exact
arxiv_id, observed 2026-05-19T16:12:38.975621Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:ab1bd90cdc74ac4846fb38f15f7e5b2a0bcb7c53d0820370f54984c2e0cef7a1

Observation 16229f67-9c4f-4ce9-b94d-805f8bfb886e · outbound

This paper cites Searching for the QCD Dark Matter Axion.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Searching for the QCD Dark Matter Axion

Reference 27

Resolution
verified exact
arxiv_id, observed 2026-05-19T16:12:38.978541Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation c2cefdfd-1321-4861-b0a0-389a3595f8c1 · outbound

This paper cites an unresolved cited work.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Unresolved cited work

Reference 28

Resolution
unresolved
raw_fallback, observed 2026-05-19T16:13:08.240381Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:31a5f57fa01f54c6a1df61f107c3e3ef0d3f250d3d93c22ee8073aedac842566

Observation 7a714629-3d0d-4178-83c0-fd0153ba9af8 · outbound

This paper cites Turbulent axion-photon conversions in the Milky-Way.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Turbulent axion-photon conversions in the Milky-Way

Reference 29

Resolution
verified exact
arxiv_id, observed 2026-05-19T16:12:39.083275Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation ddfa0156-cd97-4257-a413-8dfa90491c79 · outbound

This paper cites Manzari, Y.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Manzari, Y

Reference 30

Resolution
verified exact
arxiv_id, observed 2026-05-19T16:12:38.980948Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:e6e40ef31d57360de532e475d079b4cbc0eb9dce9854ecde5bb990f325b8e54c

Observation 00d317fd-5a30-4e05-84b1-03c3ae1dba84 · outbound

This paper cites Axion-photon conversion in transient compact stars: Systematics, constraints, and opportunities.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Axion-photon conversion in transient compact stars: Systematics, constraints, and opportunities

Reference 31

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:12:39.101552Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:80fd85200691bbf2efa37903fdfbf082055764be1d7e8d351c57fdab75e7f787

Observation e6d517e0-88ae-4ed4-9f2d-f49f02c07fd2 · outbound

This paper cites Stripped-Envelope Supernovae for QCD Axion Detection.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Stripped-Envelope Supernovae for QCD Axion Detection

Reference 32

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:12:39.104180Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:c170da2b608eed36ea220342a20680b0db82d0c4501f31c5ca46637f490bc55e

Observation d8ca3166-bffd-4036-acc7-3526de0b4a3f · outbound

This paper cites van Bibber, P.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion van Bibber, P

Reference 33

Resolution
verified fuzzy
raw_fallback, observed 2026-05-19T16:13:08.249808Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:b5bf3a3a94ff3e6d3270ad8df054b5e06e1cd18594fd0d78021399f48f815ce6

Observation ea4bfe38-9db4-4cdf-8d5e-f9e66a2220d3 · outbound

This paper cites Van Bibber, N.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Van Bibber, N

Reference 34

Resolution
verified fuzzy
raw_fallback, observed 2026-05-19T16:13:08.209685Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:98be1844232fe505c663b5da6bd01afe4fd2dc782dfaf60ec8289830d9c5c9b5

Observation 2e6881b1-044d-4365-87a2-4682e348f270 · outbound

This paper cites Search for Axions in Magnetic White Dwarf Polarization at Lick and Keck Observatories.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Search for Axions in Magnetic White Dwarf Polarization at Lick and Keck Observatories

Reference 35

Resolution
verified exact
arxiv_id, observed 2026-05-19T16:12:39.050737Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation b76f6fcd-2eee-4914-b3ef-b711b9133616 · outbound

This paper cites Panagia,Distance to SN 1987A and the LMC, in: New Views of the Magellanic Clouds, Proc.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Panagia,Distance to SN 1987A and the LMC, in: New Views of the Magellanic Clouds, Proc

Reference 36

Resolution
verified fuzzy
raw_fallback, observed 2026-05-19T16:13:08.234719Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:d70bc8b35ff8ad59bcccddedeeab3f93621cbd4bb5f8be2c29267ae19000b99f

Observation a7f0c47f-5121-4af5-84ff-1f85d0393ade · outbound

This paper cites A Geometric Determination of the Distance to SN 1987A and the LMC.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion A Geometric Determination of the Distance to SN 1987A and the LMC

Reference 37

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:12:39.056646Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:c7063e67049cbb29083a90f812355e51dde7069abffab8ca9fd3206c5ed79aea

Observation f2299d70-1409-4fb8-b9a8-7822cb2d941f · outbound

This paper cites A distance to the Large Magellanic Cloud that is precise to one per cent.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion A distance to the Large Magellanic Cloud that is precise to one per cent

Reference 38

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:12:39.061673Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:b2e3d781d8713efaad7e6f42278bd32e1e6e44b0c805776093e81c95f29db1fa

Observation d4559310-4444-4ec1-adce-954397c82338 · outbound

This paper cites an unresolved cited work.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Unresolved cited work

Reference 39

Resolution
unresolved
raw_fallback, observed 2026-05-19T16:13:08.246018Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:7aea8aafe2b9ac42c1d451629eb16ccb8f2b0daf0fff05f8b00e0427c8eb0900

Observation 25142803-2db2-4c7f-9f54-85268a96de64 · outbound

This paper cites an unresolved cited work.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Unresolved cited work

Reference 40

Resolution
unresolved
raw_fallback, observed 2026-05-19T16:13:08.244268Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:e3fa36c94462734733d9850cda99f37dbad0678efa8580935b27656bf199935b

Observation 6e6472b2-d1ba-4c41-85ef-472901634e17 · outbound

This paper cites an unresolved cited work.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Unresolved cited work

Reference 41

Resolution
unresolved
raw_fallback, observed 2026-05-19T16:13:08.229092Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:b4256b26b54c82e03007e23ec69cdc95b756c0e0e942c8b4acea7f4925e1c9af

Observation 6069bd13-c87a-406b-aeeb-83848c7a03f6 · outbound

This paper cites an unresolved cited work.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Unresolved cited work

Reference 42

Resolution
unresolved
raw_fallback, observed 2026-05-19T16:13:08.232844Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:c02634ef6b26c5204b88883544c630e17aae094d3444da585c201a9c55035026

Observation 3b424f31-d9c3-469e-a214-dee0456f82b8 · outbound

This paper cites Koshiba,Observational neutrino astrophysics,Phys.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Koshiba,Observational neutrino astrophysics,Phys

Reference 43

Resolution
verified fuzzy
raw_fallback, observed 2026-05-19T16:13:08.236604Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:0d6a5d6cc2860c4d7c907c5c3d2668fe03ce3bdbc8f4f07a7b32ba86138e8465

Observation 911748cf-5ef3-4725-9801-60cc75d9e272 · outbound

This paper cites Supernova Simulations Confront SN 1987A Neutrinos.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Supernova Simulations Confront SN 1987A Neutrinos

Reference 44

Resolution
verified exact
arxiv_id, observed 2026-05-19T16:12:39.109303Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:6696c5a748c944871bc9375416618ec81f583ef8c460080acd725d55e8bc01a6

Observation 41340c53-0f9a-48a1-a7e1-782a97e9291f · outbound

This paper cites an unresolved cited work.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Unresolved cited work

Reference 45

Resolution
unresolved
raw_fallback, observed 2026-05-19T16:13:08.234155Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:bf8f8c984409ee639b80ab8cefb9e8e5c66adb79d307e0891ecd43219f51e302

Observation 89f90377-fd68-43cd-afef-6ef880f25464 · outbound

This paper cites G., Janka, H.-T., & Fiorillo, D.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion G., Janka, H.-T., & Fiorillo, D

Reference 46

Resolution
verified exact
arxiv_id, observed 2026-05-19T16:12:38.992166Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:2fd06408a293c93a8e095f6478271e136d5efc5cd063b0027f12145dafffe8f4

Observation 1b88ba9a-741a-4548-8228-b87efaba92ab · outbound

This paper cites Arzaet al., The COSMIC WISPers White Paper: The physics case for Weakly Interacting Slim Particles, arXiv:2603.03433 [hep-ph] (2026).

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Arzaet al., The COSMIC WISPers White Paper: The physics case for Weakly Interacting Slim Particles, arXiv:2603.03433 [hep-ph] (2026)

Reference 47

Resolution
verified exact
arxiv_id, observed 2026-05-19T16:12:39.027775Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:df60bbcad22cf7b6f4646992375d7c06ae59b6bf872963123c133fecb53208ea

Observation d7640080-8584-4acb-9298-76eb2dd0a913 · outbound

This paper cites Mayle, J.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Mayle, J

Reference 48

Resolution
verified fuzzy
raw_fallback, observed 2026-05-19T16:13:08.257174Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:247dc06a328dfaceaf861c3aeac5622e7ddf7c2fc16692d4c5bfae68df3930a8

Observation b451800b-b1d9-4abb-aa8c-4fb7851ed91f · outbound

This paper cites an unresolved cited work.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Unresolved cited work

Reference 49

Resolution
unresolved
raw_fallback, observed 2026-05-19T16:13:08.232362Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:fac351fee300dace44a86a46b59b75eafd30d406f1812c833c3c435d717a19d0

Observation 8b80bcc1-ab09-4d69-84ba-011da8f31ce5 · outbound

This paper cites Burrows, M.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Burrows, M

Reference 50

Resolution
verified fuzzy
raw_fallback, observed 2026-05-19T16:13:08.242320Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:de68e5a4877ef1a571d6f71658a03e4227ded6a0e14045a0dcea3031e4ed4d2c

Observation 9ae3995c-40cb-4696-bd4f-0054203d949c · outbound

This paper cites Mayle, J.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Mayle, J

Reference 51

Resolution
verified fuzzy
raw_fallback, observed 2026-05-19T16:13:08.214233Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:7a541b7f107a34146ba167319b449c7829e277e30f1fe382c5d51d6e822da2f0

Observation f65c2ac8-6c59-4be6-b4dc-299f55a7c8ca · outbound

This paper cites Burrows, M.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Burrows, M

Reference 52

Resolution
verified fuzzy
raw_fallback, observed 2026-05-19T16:13:08.255354Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:2eaf62d006e08300aac3673e79b69580685a40c031d6f4c85995ba3e11bcb43d

Observation 4c298ec8-3d8b-448b-96e0-22b1a035aa66 · outbound

This paper cites Astrophysical Axion Bounds.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Astrophysical Axion Bounds

Reference 53

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:12:39.022912Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:2934be42800a9d213766c25d9cd4b1352873408f5c2d77017f2b0a4249d56ec4

Observation a3a28043-8bec-45ff-9392-59cf032ce2c2 · outbound

This paper cites Improved axion emissivity from a supernova via nucleon-nucleon bremsstrahlung.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Improved axion emissivity from a supernova via nucleon-nucleon bremsstrahlung

Reference 54

Resolution
verified exact
arxiv_id, observed 2026-05-19T16:12:39.125379Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:0637124b924e28deb8943abe43c55bc26b327440fbb67ef0c0b27060639ec25a

Observation 5cc9fa0b-62eb-441f-87ce-3fefd305e349 · outbound

This paper cites Forrest, E.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Forrest, E

Reference 55

Resolution
verified fuzzy
raw_fallback, observed 2026-05-19T16:13:08.222636Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:ebef708d9127d43e89159634514f28ef0c5ba9bef40cd9ebd724759110ab43a2

Observation db4b6645-e949-4347-b7fa-4a35341efd30 · outbound

This paper cites an unresolved cited work.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Unresolved cited work

Reference 56

Resolution
unresolved
raw_fallback, observed 2026-05-19T16:13:08.253520Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:d9dad06385b8270692b854914d606436dd3e091361d712250aae214b970a39b1

Observation 67715d8a-1c40-4245-9470-9f5fee7986f5 · outbound

This paper cites an unresolved cited work.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Unresolved cited work

Reference 57

Resolution
unresolved
raw_fallback, observed 2026-05-19T16:13:08.238381Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:dd5be4566de8aba03b837042791f471786858a4fe9635199944f26517d0256ab

Observation c9db9acc-0671-46fa-9825-7776b0fe8695 · outbound

This paper cites Oberauer, C.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Oberauer, C

Reference 58

Resolution
verified fuzzy
raw_fallback, observed 2026-05-19T16:13:08.210036Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:39d4ea96cdbc5eb2f62dc75b1c5afe1e298859abf30b243962270b08c911e3f4

Observation 87be702d-4839-47b1-9fdb-e2cea4c041c3 · outbound

This paper cites SN 1987A Gamma-Ray Limits on the Conversion of Pseudoscalars.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion SN 1987A Gamma-Ray Limits on the Conversion of Pseudoscalars

Reference 59

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:12:39.073857Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:363502245703f0712ac3edf56601f66161ab3dd8371323bf6115bbccfc4ec1ff

Observation 39ffc27b-ea4c-4621-ae88-3afd36becba3 · outbound

This paper cites Gamma Rays from SN1987A due to Pseudoscalar Conversion.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Gamma Rays from SN1987A due to Pseudoscalar Conversion

Reference 60

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:12:39.045464Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:271733208d0560e7784097237a70bff766e59ab1ddf44909708657cb916d8301

Observation 6d514f5d-a0bc-4fbf-9771-4782160af501 · outbound

This paper cites Revisiting the SN1987A gamma-ray limit on ultralight axion-like particles.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Revisiting the SN1987A gamma-ray limit on ultralight axion-like particles

Reference 61

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:12:38.995488Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:7ccd885f7d86a913a041eb7b13cb662c9de0fbbfddc1604419fc25732bfefe81

Observation 8c79c6c6-7eaf-40b6-aa20-35d88acb3d23 · outbound

This paper cites Updated constraints on axion-like particles from temporal information in supernova SN1987A gamma-ray data.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Updated constraints on axion-like particles from temporal information in supernova SN1987A gamma-ray data

Reference 62

Resolution
verified exact
arxiv_id, observed 2026-05-19T16:12:38.986250Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:67553e933fb277a1bed4786184fcc60fe3f7e9d0eb6aab2c6bfee05b1075a38c

Observation fdd5e467-4c49-4876-85a4-c7fa251cb5e5 · outbound

This paper cites Signatures of axion-like particles in the spectra of TeV gamma-ray sources.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Signatures of axion-like particles in the spectra of TeV gamma-ray sources

Reference 63

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:12:38.998573Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:606eca0a0d60dc1c0c5617b636d1918d3735713c0320b7c3adc81545d8f221ae

Observation ca056b90-fc71-44dd-8764-3ed8c5531a49 · outbound

This paper cites On detecting oscillations of gamma rays into axion-like particles in turbulent and coherent magnetic fields.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion On detecting oscillations of gamma rays into axion-like particles in turbulent and coherent magnetic fields

Reference 64

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:12:39.010347Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:794f9df13c762c0e92823a5938dfe7578be193796c165eba7e10cd3e96f595b8

Observation 24b4b4b0-c483-42f5-b827-5599825b66c6 · outbound

This paper cites The Fourier formalism for relativistic axion-photon conversion, with astrophysical applications.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion The Fourier formalism for relativistic axion-photon conversion, with astrophysical applications

Reference 65

Resolution
verified exact
arxiv_id, observed 2026-05-19T16:12:39.122823Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:c30abd6f952d7a8bd076dd9024b21cd891209526d1888a932ee101d46d3a8c26

Observation 9e08b82e-31ae-4241-b6a4-9e160a7ede6f · outbound

This paper cites Magnetohydrodynamics predicts heavy-tailed distributions of axion-photon conversion.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Magnetohydrodynamics predicts heavy-tailed distributions of axion-photon conversion

Reference 66

Resolution
verified exact
arxiv_id, observed 2026-05-19T16:12:39.019672Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:094008052dd917896130f0f83a7723b9f8eeffbd757c601d3ae39395156f3517

Observation 94575b54-ef25-4af9-baff-c740ec234fde · outbound

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

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion The Coherent Magnetic Field of the Milky Way

Reference 67

Resolution
verified exact
arxiv_id, observed 2026-05-19T16:12:39.035875Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:08e5d577fde6316022b56f5423f8ea0dfe3a63806912b16f0b8943d20985887b

Observation 2da0c6f4-5c06-4323-a0e3-138080a47073 · outbound

This paper cites The Galactic Magnetic Field.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion The Galactic Magnetic Field

Reference 68

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:12:39.031832Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:8d986dc95c09bca27863a57c22924044ccead984d5e1ccd009ccb47439eafce5

Observation 591405e3-9a61-4bcd-8ad1-299672c94910 · outbound

This paper cites Loops and spurs: The angular power spectrum of the Galactic synchrotron background.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Loops and spurs: The angular power spectrum of the Galactic synchrotron background

Reference 69

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:12:38.989007Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:074c5491e92537d07b6b0d9f4099f16b2ce063aeb5ff6da6a6a7d1841b1854d4

Observation 18f41cf9-6eab-4c41-bdd9-dec4a802a07d · outbound

This paper cites New constraints on modelling the random magnetic field of the MW.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion New constraints on modelling the random magnetic field of the MW

Reference 70

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:12:39.040708Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:a9a8f6a426a25e6b85d92e08235a9d52e6afbecb898c2f248a32f2e8f9f15774

Observation f3e585fd-13b4-48d8-84c5-c37d4960ad24 · outbound

This paper cites The outer scale of turbulence in the magneto-ionized Galactic interstellar medium.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion The outer scale of turbulence in the magneto-ionized Galactic interstellar medium

Reference 71

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:12:39.106851Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:ccd72399c1431cfc6bd3f5d325892914c75e2d6ff1cab09e0deb7297d4a69190

Observation f50b17ad-6e94-47e7-8e41-34d56614dc7f · outbound

This paper cites The coherent magnetic field of the Milky Way halo, Local Bubble and Fan Region.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion The coherent magnetic field of the Milky Way halo, Local Bubble and Fan Region

Reference 72

Resolution
verified exact
arxiv_id, observed 2026-05-19T16:12:39.111866Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:ac99cd5e8633b5b6813e0260cf09f7fee6ca2213ea2eb5d250794276ad4e5ec1

Observation 2f855b54-a1f1-4f3e-aa2f-f09438f2bf20 · outbound

This paper cites The Galactic Magnetic Field and UHECR Deflections.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion The Galactic Magnetic Field and UHECR Deflections

Reference 73

Resolution
verified exact
arxiv_id, observed 2026-05-19T16:12:39.114572Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:7d5c425cd0588b1cb61644bf636b9ed2deac7192b5792132c510a65a40653113

Observation 5d5b5b39-5fbe-4a49-828f-29d0a4f8cc65 · outbound

This paper cites Magnetic Field Structure of the Large Magellanic Cloud from Faraday Rotation Measures of Diffuse Polarized Emission.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Magnetic Field Structure of the Large Magellanic Cloud from Faraday Rotation Measures of Diffuse Polarized Emission

Reference 74

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:12:39.076802Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:8ca32fd3df91109d936648c0c9f1a8fe77259c9a409c9543eb099d48ddf8934b

Observation 05a7e8ee-0211-4cf8-b2bc-f165b095fa2a · outbound

This paper cites The magnetic field of the Large Magellanic Cloud revealed through Faraday rotation.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion The magnetic field of the Large Magellanic Cloud revealed through Faraday rotation

Reference 75

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:12:39.070764Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:28ad61a6789c40b64cd7acdf4063bc2fee9e7b5bd2c4f67e5fae62e3214c8c38

Observation fbb2bd2e-5690-478c-a6f4-490be5842749 · outbound

This paper cites an unresolved cited work.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Unresolved cited work

Reference 76

Resolution
unresolved
raw_fallback, observed 2026-05-19T16:13:08.220648Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:f607b638f739b0fc121f87bdc8d0595da11e035a2a41502301cc284ef25e0a68

Observation b7a80a4b-3996-4d84-843c-ae5dbfa4bb0b · outbound

This paper cites It includes bounds ong ap ×g aγ when varying the assumed CL, bounds ong aγ alone, a discussion on dissipation scale for the turbulence and its structure function.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion It includes bounds ong ap ×g aγ when varying the assumed CL, bounds ong aγ alone, a discussion on dissipation scale for the turbulence and its structure function

Reference 77

Resolution
verified fuzzy
raw_fallback, observed 2026-05-19T16:13:08.216917Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:3478ab575114aa2fed070afa77c55fa5bb6eb2e772bee14194b2ec507f144071

Observation 857a36fb-2077-4ae3-a913-182fd8c1d8a2 · outbound

This paper cites an unresolved cited work.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Unresolved cited work

Reference 78

Resolution
unresolved
raw_fallback, observed 2026-05-19T16:13:08.251624Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:6fef33e3296f0c2ff5527931234035c18b1699943efff8d8a703ba0137ef18c6

Observation a9bac5c3-06e8-4976-b9a1-7c586fa5ace4 · outbound

This paper cites Goldreich and S.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Goldreich and S

Reference 79

Resolution
verified fuzzy
raw_fallback, observed 2026-05-19T16:13:08.230660Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:093673007c117e171975dacd52794e94d6827b5b135a58d10cb277f845b95405

Observation 7ab7ded2-c5e8-4df9-85b0-87b01351ca69 · outbound

This paper cites Rotation measure structure functions with higher-order stencils as a probe of small-scale magnetic fluctuations and its application to the Small and Large Magellanic Clouds.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Rotation measure structure functions with higher-order stencils as a probe of small-scale magnetic fluctuations and its application to the Small and Large Magellanic Clouds

Reference 80

Resolution
verified exact
arxiv_id, observed 2026-05-19T16:12:39.012858Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:e61827e51342dda0a897a89bc42ef5149ca06e97616e7406850f6f42134ec189

Observation 4d89e590-bf9c-472b-aca8-a66be921d7b7 · outbound

This paper cites Depth estimation of the Large and Small Magellanic Clouds.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Depth estimation of the Large and Small Magellanic Clouds

Reference 81

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:12:39.015471Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:a1017f154e0f68891aefc2781e2a1be079a01db8ceef5ef07f454167c3ca75bf

Observation ffb85ab5-7c48-4040-9eae-fffe3e928be6 · outbound

This paper cites Reynoso-Cordova, D.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Reynoso-Cordova, D

Reference 82

Resolution
verified exact
arxiv_id, observed 2026-05-19T16:12:39.003335Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:4791a7a9d3f4e31d6af63ea9f6f1670232f77bae984ee750376a9b5159897611

Observation 11a51e9c-f703-488e-b44e-16f0f7ba6aaf · outbound

This paper cites Probing protoneutron stars with gamma-ray axionscopes.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Probing protoneutron stars with gamma-ray axionscopes

Reference 83

Resolution
verified exact
arxiv_id, observed 2026-05-19T16:12:39.128245Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:4b58cf7867a526eff99286500d0eefe0793a94193537cec2f347cd2c7df7d238

Observation 1c415b8e-ce86-47a7-806b-9320aec28cba · outbound

This paper cites Leading Axion-Photon Sensitivity with NuSTAR Observations of M82 and M87.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Leading Axion-Photon Sensitivity with NuSTAR Observations of M82 and M87

Reference 84

Resolution
verified exact
arxiv_id, observed 2026-05-19T16:12:38.983574Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:a0e7b9f6da881ec67dafb4124795d39c5a552864dbf53ebe8e8404b90fc93cc8

Observation ef00d028-1284-41c6-a9e5-0e8d7e6aae99 · outbound

This paper cites NuSTAR bounds on radiatively decaying particles from M82.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion NuSTAR bounds on radiatively decaying particles from M82

Reference 85

Resolution
verified exact
arxiv_id, observed 2026-05-19T16:12:38.972790Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:ed8c67b4076ceee1274c91e79aef1e86f8c1de5b1ff4526af434c9ee88e0ca61

Observation c67a6e77-3c07-43b5-8754-e94eb590fac9 · outbound

This paper cites Probing the Axion-Electron Coupling with NuSTAR Observations of Galaxies.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Probing the Axion-Electron Coupling with NuSTAR Observations of Galaxies

Reference 86

Resolution
verified exact
arxiv_id, observed 2026-05-19T16:12:39.080355Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:282341f4d42d1d1200f0b6f05e2c215204ea0f0d4c46d116f6f1542772b5dc4d

Observation 6bf7b411-23ba-4a98-9edf-d7744456ed83 · outbound

This paper cites Ruz et al.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Ruz et al

Reference 87

Resolution
metadata mismatch
arxiv_id, observed 2026-05-19T16:12:39.120190Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:314c75297ec7e0684a3b8e637e58d103224390080c0faf72bab0e3b94b4be963

Observation 21a06701-f471-4cc5-9d7e-3249f264dc99 · outbound

This paper cites Novel Constraints on Axions Produced in Pulsar Polar-Cap Cascades.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Novel Constraints on Axions Produced in Pulsar Polar-Cap Cascades

Reference 88

Resolution
verified exact
arxiv_id, observed 2026-05-19T16:12:39.117257Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:bc7ed629b79344d001c1fb060fe73f64b2d9245a6b7552e13d08e85521c221ed

Observation 9a1088a2-f790-4275-856a-384deef3c008 · outbound

This paper cites an unresolved cited work.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Unresolved cited work

Reference 89

Resolution
unresolved
raw_fallback, observed 2026-05-19T16:13:08.258947Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:4f75384a454b762238e4dd43a3be7802b9d5ba92a3bef916761f0db9637b9ae0

Observation d7726ecb-9dd3-45b5-906b-7bf4f052251e · outbound

This paper cites Padmanabhan,Theoretical Astrophysics.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion Padmanabhan,Theoretical Astrophysics

Reference 90

Resolution
verified fuzzy
raw_fallback, observed 2026-05-19T16:13:08.206082Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:57495cf0f417c24006033e50111f3076972afc62b162544de8a730b13d9f6a22

Observation 05d0ae9f-e599-4704-a47d-79551cfed283 · outbound

This paper cites pinched.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion pinched

Reference 91

Resolution
verified fuzzy
raw_fallback, observed 2026-05-19T16:13:08.247975Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:a58644644bb61195375cc6977fb941f2c005d3b290af862a3e7904a92a23fa42

Pith citing papers

Observation 81f8f72d-0436-47d2-abce-d75d333b7367 · inbound

Reappraisal of the Constraints on Heavy Axion-like Particles from Gamma-Ray Bursts cites this paper.

Reappraisal of the Constraints on Heavy Axion-like Particles from Gamma-Ray Bursts Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion

Reference 24

Resolution
verified exact
local_arxiv, observed 2026-07-09T15:06:18.228091Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-07-09T14:56:45.760028Z digest=sha256:66350b1964d720e4994c7fc6687edef39a80b4a4ef7d81846a6f6e256e76e347