Paper Citation Record · LEDGER

Can the neutrinos from TXS 0506+056 have a coronal origin?

As of 18 August 2026, this Paper Citation Record lists 67 of 67 outbound references and 2 inbound Pith citation observations for arXiv:2502.01738.

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

pith.paper-citation-record.v1
2502.01738 v2

Coverage vector

measured 67 of 67 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-09T14:44:29.426656Z

measured 69 of 69 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-14T16:57:50.370612Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-19T07:52:09.457260Z

Reference resolution

67 of 67 outbound references displayed

verified exact5
verified fuzzy1
unresolved61
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 39f616fa-dd81-4092-92dc-a588de585d2e · outbound

This paper cites G., et al.

Can the neutrinos from TXS 0506+056 have a coronal origin? G., et al

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:28.986413Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9fc957e9-6079-4a9f-ba6c-64194ac2836e · outbound

This paper cites G., Ackermann , M., Adams , J., et al.

Can the neutrinos from TXS 0506+056 have a coronal origin? G., Ackermann , M., Adams , J., et al

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:28.992186Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a40ee6e0-92ec-401f-b007-8bbc90fb5706 · outbound

This paper cites 2022, Science, 378, 538, 10.1126/science.abg3395.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2022, Science, 378, 538, 10.1126/science.abg3395

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.003437Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 43fbded6-9731-4619-89bd-dbab64783684 · outbound

This paper cites A., et al.

Can the neutrinos from TXS 0506+056 have a coronal origin? A., et al

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.009414Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ff150002-41aa-4f82-b89a-b6ca2097b313 · outbound

This paper cites A., Aniello , T., Ansoldi , S., et al.

Can the neutrinos from TXS 0506+056 have a coronal origin? A., Aniello , T., Ansoldi , S., et al

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.014923Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2b158986-0954-4ddf-ba68-3ad495f482cd · outbound

This paper cites A., Arcaro , C., et al.

Can the neutrinos from TXS 0506+056 have a coronal origin? A., Arcaro , C., et al

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.020786Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ee2a8171-6ead-4dd1-b125-286ee7f29c81 · outbound

This paper cites 2019, , 628, A135, 10.1051/0004-6361/201935874.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2019, , 628, A135, 10.1051/0004-6361/201935874

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.026364Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a35c6bff-9684-48c5-945e-b48b92ad42f9 · outbound

This paper cites an unresolved cited work.

Can the neutrinos from TXS 0506+056 have a coronal origin? Unresolved cited work

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.030934Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b32a1736-47c3-4f3c-a731-76e59ad667ad · outbound

This paper cites S., & Ginzburg , V.

Can the neutrinos from TXS 0506+056 have a coronal origin? S., & Ginzburg , V

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.037971Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9b140d80-4c3d-42c1-af30-2f6d50e70e2a · outbound

This paper cites M., Bentz , M.

Can the neutrinos from TXS 0506+056 have a coronal origin? M., Bentz , M

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.051353Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 16d26a57-1b7f-4f2f-ad96-c43c84434bd1 · outbound

This paper cites 2019, , 483, L12, 10.1093/mnrasl/sly210.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2019, , 483, L12, 10.1093/mnrasl/sly210

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.065393Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2249582b-deec-4350-841c-c9b2eec7bbe7 · outbound

This paper cites High-Energy Radiation and Ion Acceleration in Three-dimensional Relativistic Magnetic Reconnection with Strong Synchrotron Cooling.

Can the neutrinos from TXS 0506+056 have a coronal origin? High-Energy Radiation and Ion Acceleration in Three-dimensional Relativistic Magnetic Reconnection with Strong Synchrotron Cooling

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.072941Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4233e7fa-ae5b-4606-9f94-88458112da80 · outbound

This paper cites 2019, , 886, 122, 10.3847/1538-4357/ab4c33.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2019, , 886, 122, 10.3847/1538-4357/ab4c33

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.083270Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4e917e19-79b8-4b8b-9bd2-f5d2284de9c8 · outbound

This paper cites an unresolved cited work.

Can the neutrinos from TXS 0506+056 have a coronal origin? Unresolved cited work

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.101693Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8d046bfd-cb3c-43f5-986b-e038af98ea84 · outbound

This paper cites an unresolved cited work.

Can the neutrinos from TXS 0506+056 have a coronal origin? Unresolved cited work

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.111528Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1f9489c0-bfd0-4783-9ac8-423707eb72f4 · outbound

This paper cites 2019, Nature Astronomy, 3, 88, 10.1038/s41550-018-0610-1.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2019, Nature Astronomy, 3, 88, 10.1038/s41550-018-0610-1

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.118612Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c28de1ce-09dd-4ae2-b80f-9efbf27292f5 · outbound

This paper cites 2013, Radiative Processes in High Energy Astrophysics , Vol.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2013, Radiative Processes in High Energy Astrophysics , Vol

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.127649Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d5dbf5c5-329c-416e-a2a8-8d41b244b558 · outbound

This paper cites 2013, , 431, 1914, 10.1093/mnras/stt305.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2013, , 431, 1914, 10.1093/mnras/stt305

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.135010Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 872b6e25-5003-43ea-a982-d2ccd081d83a · outbound

This paper cites M., Sironi , L., & Philippov , A.

Can the neutrinos from TXS 0506+056 have a coronal origin? M., Sironi , L., & Philippov , A

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.140323Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e91da344-7a9d-4620-a235-5859c551a5e2 · outbound

This paper cites 1991, , 380, L51, 10.1086/186171.

Can the neutrinos from TXS 0506+056 have a coronal origin? 1991, , 380, L51, 10.1086/186171

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.145487Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 39134d5d-014a-41a7-88a7-f1cf19a99608 · outbound

This paper cites 1993, , 413, 507, 10.1086/173020.

Can the neutrinos from TXS 0506+056 have a coronal origin? 1993, , 413, 507, 10.1086/173020

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.151028Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 151b66de-07c1-4c2c-9882-6f0b070e2232 · outbound

This paper cites 2013, Science, 342, 1242856, 10.1126/science.1242856.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2013, Science, 342, 1242856, 10.1126/science.1242856

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.156291Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 607d7b76-6eec-4d4b-ab26-48cd52327150 · outbound

This paper cites G., Ackermann , M., et al.

Can the neutrinos from TXS 0506+056 have a coronal origin? G., Ackermann , M., et al

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.161516Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6439ab24-56f7-4fc4-9f64-06350e71048f · outbound

This paper cites 2018 b , Science, 361, 147, 10.1126/science.aat2890.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2018 b , Science, 361, 147, 10.1126/science.aat2890

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.166790Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4b4699dc-2f5c-44cb-b84d-91e21e680458 · outbound

This paper cites 2020, , 891, L33, 10.3847/2041-8213/ab7661.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2020, , 891, L33, 10.3847/2041-8213/ab7661

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.171055Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 12650e88-4ddb-4699-82b2-bdf8c7880475 · outbound

This paper cites Neutrino and pair creation in reconnection-powered coronae of accreting black holes.

Can the neutrinos from TXS 0506+056 have a coronal origin? Neutrino and pair creation in reconnection-powered coronae of accreting black holes

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.175595Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2ab31240-84c3-4f89-9318-73a5aba964e6 · outbound

This paper cites 2018, Astrophys.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2018, Astrophys

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.180440Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b0cbfe76-9b95-409b-a899-5d6a25d70562 · outbound

This paper cites An NGC 1068-Informed Understanding of Neutrino Emission of the Active Galactic Nucleus TXS 0506+056.

Can the neutrinos from TXS 0506+056 have a coronal origin? An NGC 1068-Informed Understanding of Neutrino Emission of the Active Galactic Nucleus TXS 0506+056

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.184771Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5421ea24-06e3-4021-a519-afa0ba5e2acd · outbound

This paper cites S., & Toma, K.

Can the neutrinos from TXS 0506+056 have a coronal origin? S., & Toma, K

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.190089Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b21123e4-d7a2-4b61-b9f1-ead7d7b134b2 · outbound

This paper cites 2024, Astrophys.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2024, Astrophys

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.195251Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b3670a57-0fdc-4a43-b97f-a649eab5ce4e · outbound

This paper cites Neutrinos from stochastic acceleration in black hole environments.

Can the neutrinos from TXS 0506+056 have a coronal origin? Neutrinos from stochastic acceleration in black hole environments

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.200270Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 80060c8a-f39f-42d2-9926-b4e01536b2d8 · outbound

This paper cites 2019, , 99, 063008, 10.1103/PhysRevD.99.063008.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2019, , 99, 063008, 10.1103/PhysRevD.99.063008

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.205557Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 343c671b-2c3e-4cc9-85b3-eccf33ef5c30 · outbound

This paper cites 2010, , 512, A34, 10.1051/0004-6361/200913298.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2010, , 512, A34, 10.1051/0004-6361/200913298

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.210734Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 781eba5b-6520-41f5-b60b-3cde0a1b28d9 · outbound

This paper cites 2011, , 534, A110, 10.1051/0004-6361/201117175.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2011, , 534, A110, 10.1051/0004-6361/201117175

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.215652Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 03c79dba-efd8-4ec5-8552-d5b46ea75ff1 · outbound

This paper cites 2004 b , Mon.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2004 b , Mon

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.226535Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5160d6f6-526b-455c-a594-554a3986c495 · outbound

This paper cites 2024, Phys.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2024, Phys

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.231053Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fbd92f8a-9ed5-4848-9855-f366d43924ad · outbound

This paper cites J., & Dunlop , J.

Can the neutrinos from TXS 0506+056 have a coronal origin? J., & Dunlop , J

Reference 39

Resolution: verified exact; arxiv_id_nonexistent, observed 2026-08-09T14:44:51.534181Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation a44d3d80-baad-4860-8862-b482e4c1c295 · outbound

This paper cites an unresolved cited work.

Can the neutrinos from TXS 0506+056 have a coronal origin? Unresolved cited work

Reference 40

Resolution: verified exact; arxiv_id_nonexistent, observed 2026-08-09T14:44:51.491930Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 56378db5-805e-4cbc-a61c-e147e22ff78a · outbound

This paper cites 2022, Astrophys.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2022, Astrophys

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.245498Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 21e9b40e-fc16-46a5-8e36-728c7b320b8d · outbound

This paper cites S., & Meszaros, P.

Can the neutrinos from TXS 0506+056 have a coronal origin? S., & Meszaros, P

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.250041Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 19806b83-bb57-4987-8be5-473036425fa0 · outbound

This paper cites 2018, Astrophys.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2018, Astrophys

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.254504Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ee5a983c-2a95-400d-9153-facffdcc12fa · outbound

This paper cites 2019, Mon.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2019, Mon

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.259589Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7fe390e3-3f15-442e-ae01-03dae998f615 · outbound

This paper cites 2017, Astron.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2017, Astron

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.264220Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 960cf835-d46c-45a2-929f-215d25cdd395 · outbound

This paper cites 2018, , 854, L32, 10.3847/2041-8213/aaad5e.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2018, , 854, L32, 10.3847/2041-8213/aaad5e

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.268947Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 80241876-9097-4621-ab3a-58647a11e4e9 · outbound

This paper cites 2020, , 899, 113, 10.3847/1538-4357/aba8a0.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2020, , 899, 113, 10.3847/1538-4357/aba8a0

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.274786Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d79ca163-faf4-44ca-a01f-8c57adf69db1 · outbound

This paper cites 2020, , 891, 115, 10.3847/1538-4357/ab76d0.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2020, , 891, 115, 10.3847/1538-4357/ab76d0

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.284153Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 147ab1df-8d84-4dbf-ad3e-2d1466609e45 · outbound

This paper cites O., et al.

Can the neutrinos from TXS 0506+056 have a coronal origin? O., et al

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.288639Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f571d9a9-fb2e-465b-bca7-860c2009464c · outbound

This paper cites 2011, , 412, L123, 10.1111/j.1745-3933.2011.01019.x.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2011, , 412, L123, 10.1111/j.1745-3933.2011.01019.x

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.293210Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bc784655-3a7c-4534-a7ce-1ea39ac1f42b · outbound

This paper cites 2019, , 881, 46, 10.3847/1538-4357/ab2bff.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2019, , 881, 46, 10.3847/1538-4357/ab2bff

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.297867Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0862f194-ec46-4bb7-bebb-b3ac1ef3ee1e · outbound

This paper cites 2019, , 874, L29, 10.3847/2041-8213/ab1267.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2019, , 874, L29, 10.3847/2041-8213/ab1267

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.302783Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 88e57917-eb42-4500-bf0f-87abf21f3d7b · outbound

This paper cites 2024, , 689, A147, 10.1051/0004-6361/202450592.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2024, , 689, A147, 10.1051/0004-6361/202450592

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.307833Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 75a35152-b586-473f-84e3-cdb046271b59 · outbound

This paper cites J., Anderson , S.

Can the neutrinos from TXS 0506+056 have a coronal origin? J., Anderson , S

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.313074Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5b28767f-a2d7-486f-8bcc-1a0e183c4754 · outbound

This paper cites C., Brotherton , M.

Can the neutrinos from TXS 0506+056 have a coronal origin? C., Brotherton , M

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.318080Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9cb43b00-7763-46f8-800c-5c455c3b4f1b · outbound

This paper cites an unresolved cited work.

Can the neutrinos from TXS 0506+056 have a coronal origin? Unresolved cited work

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.323108Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6ee13b19-71ca-43c9-ba05-d154846950cd · outbound

This paper cites an unresolved cited work.

Can the neutrinos from TXS 0506+056 have a coronal origin? Unresolved cited work

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.328288Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6debeac1-90cd-4de3-8e70-7aa77558ba74 · outbound

This paper cites an unresolved cited work.

Can the neutrinos from TXS 0506+056 have a coronal origin? Unresolved cited work

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.333653Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7928d0c7-292e-4ea2-b3de-ac6d22476201 · outbound

This paper cites an unresolved cited work.

Can the neutrinos from TXS 0506+056 have a coronal origin? Unresolved cited work

Reference 60

Resolution: verified exact; doi, observed 2026-08-09T14:44:29.601261Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation cde1e64b-50a9-419d-9364-7544990498fd · outbound

This paper cites I., Petropoulou, M., Sironi, L., & Giannios, D.

Can the neutrinos from TXS 0506+056 have a coronal origin? I., Petropoulou, M., Sironi, L., & Giannios, D

Reference 61

Resolution: verified exact; doi, observed 2026-08-09T14:44:29.571082Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation dfec83c6-fddf-4610-9001-cec847fae3a1 · outbound

This paper cites A., & Titarchuk , L.

Can the neutrinos from TXS 0506+056 have a coronal origin? A., & Titarchuk , L

Reference 62

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T14:45:17.246557Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 16dd1dba-fbb2-41ac-a932-75e4047d3345 · outbound

This paper cites A., & Truemper , J.

Can the neutrinos from TXS 0506+056 have a coronal origin? A., & Truemper , J

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.353446Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5a1f966a-56cd-4d0e-b80b-bbc988df17a7 · outbound

This paper cites an unresolved cited work.

Can the neutrinos from TXS 0506+056 have a coronal origin? Unresolved cited work

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.358608Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 85f242cd-4593-459b-89ec-03f56dad5d07 · outbound

This paper cites R., & Uzdensky , D.

Can the neutrinos from TXS 0506+056 have a coronal origin? R., & Uzdensky , D

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.363378Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9abc4b8e-44eb-40bf-bb3b-0d69c10998de · outbound

This paper cites R., & Gallo, L.

Can the neutrinos from TXS 0506+056 have a coronal origin? R., & Gallo, L

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.373898Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0168a62d-e574-4b59-8fb8-492ae242f68c · outbound

This paper cites Could the neutrino emission of TXS 0506+056 come from the accretion flow of the supermassive black hole?.

Can the neutrinos from TXS 0506+056 have a coronal origin? Could the neutrino emission of TXS 0506+056 come from the accretion flow of the supermassive black hole?

Reference 68

Resolution: verified exact; local_arxiv, observed 2026-08-09T14:44:30.293315Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation f3649a25-5903-490f-8de8-d0cc2bfca7f8 · outbound

This paper cites 2021, Astrophys.

Can the neutrinos from TXS 0506+056 have a coronal origin? 2021, Astrophys

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.384790Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6e22153f-3211-4b9e-8b77-2f25dde515c8 · outbound

This paper cites The origin of power-law spectra in relativistic magnetic reconnection.

Can the neutrinos from TXS 0506+056 have a coronal origin? The origin of power-law spectra in relativistic magnetic reconnection

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.395604Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 81a0b921-4ada-4eae-ac04-ae743e1d744f · outbound

This paper cites The origin of power-law spectra in relativistic magnetic reconnection.

Can the neutrinos from TXS 0506+056 have a coronal origin? The origin of power-law spectra in relativistic magnetic reconnection

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-09T14:44:29.426656Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Pith citing papers

Observation 7f919b41-3ec7-4068-af6d-b8a4e485362e · inbound

3C403: a candidate neutrino-emitting radio galaxy cites this paper.

3C403: a candidate neutrino-emitting radio galaxy Can the neutrinos from TXS 0506+056 have a coronal origin?

Reference 18

Resolution: verified exact; arxiv_id, observed 2026-05-19T07:52:09.459089Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation c205a84d-bafd-448d-8443-3d5a0b126e07 · inbound

Active Galactic Nuclei as high-energy neutrino sources cites this paper.

Active Galactic Nuclei as high-energy neutrino sources Can the neutrinos from TXS 0506+056 have a coronal origin?

Reference 65

Resolution: unresolved; no resolver link, observed 2026-07-14T16:57:50.370612Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.