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Paper Citation Record · LEDGER

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir

As of 16 August 2026, this Paper Citation Record lists 100 of 211 outbound references and 0 inbound Pith citation observations for arXiv:2608.00968.

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

pith.paper-citation-record.v1
2608.00968 v1

Coverage vector

measured 100 of 211 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-15T15:19:16.817648Z

measured 100 of 100 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

100 of 211 outbound references displayed

  • verified exact7
  • verified fuzzy0
  • unresolved90
  • parse uncertain0
  • malformed identifier1
  • metadata mismatch2

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 26ab29a3-3b77-4339-8e66-5ebd2333e40d · outbound

This paper cites arXiv e-prints , keywords =.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir arXiv e-prints , keywords =

Reference 1

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source=arxiv_source observed=2026-08-15T15:19:16.392871Z digest=sha256:32e0aeae086f43ac809c550b584293174d6445ac06b268b12810b6cec0748d19

Observation d9cb84d0-41d7-423f-b28a-1870f07b8785 · outbound

This paper cites Discoveries of fine structures and secondary pulses in coherent radio emission from a magnetic massive star.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Discoveries of fine structures and secondary pulses in coherent radio emission from a magnetic massive star

Reference 2

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no resolver link, observed 2026-08-15T15:19:16.396543Z

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source=arxiv_source observed=2026-08-15T15:19:16.396543Z digest=sha256:25df2a2e2c61dc1e402ee35b8a8304b754612249c927ba893a3fa28b8d7c79ba

Observation 8c0d7910-6905-41fc-9964-ea92047044a1 · outbound

This paper cites The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package

Reference 3

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source=arxiv_source observed=2026-08-15T15:19:16.400362Z digest=sha256:576cde8903f4f061393b33819b3af63b9b5e5e7c7c2f58a2e19cf340e41d6215

Observation 7a9b85b3-4801-487e-9d15-79634438c9e7 · outbound

This paper cites an unresolved cited work.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Unresolved cited work

Reference 4

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source=arxiv_source observed=2026-08-15T15:19:16.405483Z digest=sha256:7d2a4d4c9787c2ed833f887f1c3188a24a360796256d8dee92b460aed69d382c

Observation 21bc7f6e-0620-41d9-a9ee-52e15ecff6ee · outbound

This paper cites A massive helium star with a sufficiently strong magnetic field to form a magnetar.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir A massive helium star with a sufficiently strong magnetic field to form a magnetar

Reference 6

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no resolver link, observed 2026-08-15T15:19:16.413625Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.413625Z digest=sha256:73df3f467bcf35015b5e06baca0199b0ccf5c2824c8572751a096758452ce9fb

Observation e33233f7-f976-427f-a3cd-16e978419b95 · outbound

This paper cites , keywords =.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir , keywords =

Reference 7

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no resolver link, observed 2026-08-15T15:19:16.417904Z

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source=arxiv_source observed=2026-08-15T15:19:16.417904Z digest=sha256:73eac1b46e8f534eca9ff9dccd23dcd5d3878b0c8d54dcc463ffd7f2926ec12b

Observation e01e9842-f59e-47fe-b4b5-f88126ab43fe · outbound

This paper cites High Energy Phenomena in Massive Stars , year = 2010, editor =.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir High Energy Phenomena in Massive Stars , year = 2010, editor =

Reference 8

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.421311Z digest=sha256:0dd514c5ab5042a725441dff1199c666b9323be9e312814e140177427022e8c0

Observation edd4931d-e4f0-4e95-8dcf-0adaccd2ed0f · outbound

This paper cites A scaling relationship for non-thermal radio emission from ordered magnetospheres: from the top of the Main Sequence to planets.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir A scaling relationship for non-thermal radio emission from ordered magnetospheres: from the top of the Main Sequence to planets

Reference 9

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no resolver link, observed 2026-08-15T15:19:16.424911Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.424911Z digest=sha256:e7bc88a441631ab55c2a730aa174f6f47370e44e79251ff94380c6a082b8a01f

Observation 67cdac12-9167-4212-af08-65778305b31c · outbound

This paper cites The effects of surface fossil magnetic fields on massive star evolution: I. Magnetic field evolution, mass-loss quenching and magnetic braking.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir The effects of surface fossil magnetic fields on massive star evolution: I. Magnetic field evolution, mass-loss quenching and magnetic braking

Reference 10

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source=arxiv_source observed=2026-08-15T15:19:16.429128Z digest=sha256:b3bf3160fa4c03429089d5e8fb6f0fda539b4634c1cc1cdc74e3a0759c7530f0

Observation a6570256-8c2f-4ede-a779-66b83b083a6d · outbound

This paper cites Magnetic Interactions in White Dwarf Binaries as Mechanism for Long-Period Radio Transients.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Magnetic Interactions in White Dwarf Binaries as Mechanism for Long-Period Radio Transients

Reference 11

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no resolver link, observed 2026-08-15T15:19:16.434153Z

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source=arxiv_source observed=2026-08-15T15:19:16.434153Z digest=sha256:29c35a88fa5dea918f54dcfbf72a40ae954a67787b3e31c2019807f00dd2cfdb

Observation 9b04c4b3-7457-4c1b-9bcc-4c751d466638 · outbound

This paper cites MOBSTER -- VI. The crucial influence of rotation on the radio magnetospheres of hot stars.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir MOBSTER -- VI. The crucial influence of rotation on the radio magnetospheres of hot stars

Reference 12

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no resolver link, observed 2026-08-15T15:19:16.439033Z

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source=arxiv_source observed=2026-08-15T15:19:16.439033Z digest=sha256:92eefcd06b846ae7efccecd87f289a50c351401acac9fe3757b11d6d4b62ecd1

Observation 64b4abfa-f35a-4967-8100-d3d6f41f90ed · outbound

This paper cites Centrifugal breakout reconnection as the electron acceleration mechanism powering the radio magnetospheres of early-type stars.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Centrifugal breakout reconnection as the electron acceleration mechanism powering the radio magnetospheres of early-type stars

Reference 13

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no resolver link, observed 2026-08-15T15:19:16.443077Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.443077Z digest=sha256:3c54c8bffddcecaa162f405ddbba6ab1bd9fdb38dc47d1a791624d15ead3b08e

Observation fb123cf1-eab0-49fb-970d-326b7834f7bd · outbound

This paper cites A weak coronal heating event associated with periodic particle acceleration episodes.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir A weak coronal heating event associated with periodic particle acceleration episodes

Reference 14

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no resolver link, observed 2026-08-15T15:19:16.447468Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.447468Z digest=sha256:48666725c22282d53df4f4c2ad8191a8f63fb520a17c8823517c828625b1794d

Observation b69860f2-11cf-4099-92d1-e014bd5c24f4 · outbound

This paper cites Astronomical Data Analysis Software and Systems XVI , year = 2007, editor =.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Astronomical Data Analysis Software and Systems XVI , year = 2007, editor =

Reference 15

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source=arxiv_source observed=2026-08-15T15:19:16.452279Z digest=sha256:f4ca8c4b96a15a0c8f57950d8af667413c695494121271a6cb6efb541c8061fe

Observation 74247622-5df6-4105-8d19-e57db2e83079 · outbound

This paper cites Outstanding X-ray emission from the stellar radio pulsar CU Virginis.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Outstanding X-ray emission from the stellar radio pulsar CU Virginis

Reference 16

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no resolver link, observed 2026-08-15T15:19:16.456380Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.456380Z digest=sha256:18f1c50a275a9569367cc0303eaf9f2f3556b5bb3ff0288c5de12c2cf5052eae

Observation 0deeb49c-d386-4827-a7e4-4fd0c8af2bd0 · outbound

This paper cites The auroral radio emission of the magnetic B-type star rho OphC.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir The auroral radio emission of the magnetic B-type star rho OphC

Reference 17

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no resolver link, observed 2026-08-15T15:19:16.460218Z

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source=arxiv_source observed=2026-08-15T15:19:16.460218Z digest=sha256:440c5f5221df1a9aef8f32463c6752050d1ef514f737ab81de690451c2a90e2b

Observation 59dc3e2d-b31f-40d6-873f-6b2089b3ea33 · outbound

This paper cites , keywords =.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir , keywords =

Reference 18

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no resolver link, observed 2026-08-15T15:19:16.464602Z

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source=arxiv_source observed=2026-08-15T15:19:16.464602Z digest=sha256:9019f825c8575530d524afe64eb9053204401e0c61328f19d718536c059fb8ab

Observation 8ad6357b-b417-4cfb-b982-9fd9a86d11cf · outbound

This paper cites 10.1051/0004-6361/201834937.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir 10.1051/0004-6361/201834937

Reference 19

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doi, observed 2026-08-15T15:19:17.910282Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=arxiv_source observed=2026-08-15T15:19:16.467894Z digest=sha256:e8fe74da30dfb681816a546a626b229c54fdacba344d2295429c981cfae1eace

Observation 0cd473a1-1557-4697-ab61-9dfc50a8504f · outbound

This paper cites Unraveling the complex magnetosphere of the B star HD 133880 via wideband observation of coherent radio emission.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Unraveling the complex magnetosphere of the B star HD 133880 via wideband observation of coherent radio emission

Reference 20

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source=arxiv_source observed=2026-08-15T15:19:16.471204Z digest=sha256:a5ef06ad125dc6e0550be8b4c6e37961e33f4c46af78079253f600086ec767ff

Observation ee5b02f5-6fb1-4601-9a47-aa96e0506d81 · outbound

This paper cites VAST: An ASKAP Survey for Variables and Slow Transients.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir VAST: An ASKAP Survey for Variables and Slow Transients

Reference 21

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no resolver link, observed 2026-08-15T15:19:16.474863Z

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source=arxiv_source observed=2026-08-15T15:19:16.474863Z digest=sha256:6c769f017e995e17d48be8e2a0ab9e12fcf2745bfd8884e2fefe6f71d0dd8276

Observation e965e82e-ee77-4afb-892e-f1f265ec8b64 · outbound

This paper cites A combined multiwavelength VLA/ALMA/Chandra study unveils the complex magnetosphere of the B-type star HR5907.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir A combined multiwavelength VLA/ALMA/Chandra study unveils the complex magnetosphere of the B-type star HR5907

Reference 22

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no resolver link, observed 2026-08-15T15:19:16.479175Z

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source=arxiv_source observed=2026-08-15T15:19:16.479175Z digest=sha256:caa857e2764193602bdc1782a13457c7bd2d8e22227aedbdbeb9822a62ca7d70

Observation 96b3d032-5537-4f07-ae48-585c96c72510 · outbound

This paper cites The Sydney Radio Star Catalogue: properties of radio stars at megahertz to gigahertz frequencies.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir The Sydney Radio Star Catalogue: properties of radio stars at megahertz to gigahertz frequencies

Reference 23

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no resolver link, observed 2026-08-15T15:19:16.485128Z

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source=arxiv_source observed=2026-08-15T15:19:16.485128Z digest=sha256:b1fc2d86d231d6177054fd552545804aed01a7a4600463f4460b5a29d87dee96

Observation 9b52265e-9f5e-41ec-8c8e-ad698f172d61 · outbound

This paper cites , keywords =.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir , keywords =

Reference 24

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source=arxiv_source observed=2026-08-15T15:19:16.489622Z digest=sha256:8e63ea0ceadfa2d81bd64d36e835c542782ee760767dc427a21b714c40cf4998

Observation bec44545-eeed-486a-a272-48da97cfa417 · outbound

This paper cites , keywords =.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir , keywords =

Reference 25

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no resolver link, observed 2026-08-15T15:19:16.493643Z

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source=arxiv_source observed=2026-08-15T15:19:16.493643Z digest=sha256:e2a1f570a1404015c0d9dd653e1363ec471a49958198c36ea0bcb0ae9456a5dd

Observation 40e68212-3ebf-48a2-bcc8-b14f6178771d · outbound

This paper cites arXiv e-prints , keywords =.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir arXiv e-prints , keywords =

Reference 26

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no resolver link, observed 2026-08-15T15:19:16.497934Z

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source=arxiv_source observed=2026-08-15T15:19:16.497934Z digest=sha256:43cf8847a9f58475ff24a2f70709bdc7509f304c8f0ad80ec2fdd129271cb696

Observation 03755fd3-6b89-488e-a6a3-726ac45ecde4 · outbound

This paper cites Centrifugal Breakout of Magnetically Confined Line-Driven Stellar Winds.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Centrifugal Breakout of Magnetically Confined Line-Driven Stellar Winds

Reference 27

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no resolver link, observed 2026-08-15T15:19:16.502175Z

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source=arxiv_source observed=2026-08-15T15:19:16.502175Z digest=sha256:50f1f12c155b61f1f322335280eeecef0e2bf9907d8739d43c74afd48f3ab14e

Observation fc6fcaf9-e817-4c9e-9edd-d54163840ca5 · outbound

This paper cites Journal of Geophysical Research (Space Physics) , keywords =.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Journal of Geophysical Research (Space Physics) , keywords =

Reference 28

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verified exact
doi, observed 2026-08-15T15:19:17.873554Z

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No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=arxiv_source observed=2026-08-15T15:19:16.506425Z digest=sha256:772874cc8db4281cbb907ada433e07eedd26bde3ac4e79e16dba3f50981fceba

Observation cb1830ea-fcf2-4612-893f-7f5c63db304e · outbound

This paper cites , keywords =.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir , keywords =

Reference 29

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no resolver link, observed 2026-08-15T15:19:16.510326Z

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source=arxiv_source observed=2026-08-15T15:19:16.510326Z digest=sha256:337382b8296b46a45c2436d9d883ee155fe10c1902998a6665f0d9eec98a178c

Observation 20a039e4-7510-4661-b24e-96aa58620bd0 · outbound

This paper cites Handbook of Exoplanets , year = 2018, editor =.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Handbook of Exoplanets , year = 2018, editor =

Reference 30

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unresolved
no resolver link, observed 2026-08-15T15:19:16.514652Z

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source=arxiv_source observed=2026-08-15T15:19:16.514652Z digest=sha256:0e50906dd5f1e4954843ba2b7abd67246741afe84c3da215052cbfad5fa251a3

Observation 5e804964-8778-42b1-b540-4f6b16b68f76 · outbound

This paper cites Ultra-Wideband, Multi-epoch Radio Study of the First Discovered `Main sequence Radio Pulse emitter' CU Vir.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Ultra-Wideband, Multi-epoch Radio Study of the First Discovered `Main sequence Radio Pulse emitter' CU Vir

Reference 31

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no resolver link, observed 2026-08-15T15:19:16.519075Z

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source=arxiv_source observed=2026-08-15T15:19:16.519075Z digest=sha256:f8b7645d6b15f134187afe458dd46690609007ca383bd1e325b7254c3c7d3724

Observation 3f51aa22-a647-4d07-94f2-419e4af6bb6b · outbound

This paper cites and Haberland, Matt and Reddy, Tyler and Cournapeau, David and Burovski, Evgeni and Peterson, Pearu and Weckesser, Warren and Bright, Jonathan and.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir and Haberland, Matt and Reddy, Tyler and Cournapeau, David and Burovski, Evgeni and Peterson, Pearu and Weckesser, Warren and Bright, Jonathan and

Reference 33

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no resolver link, observed 2026-08-15T15:19:16.526905Z

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source=arxiv_source observed=2026-08-15T15:19:16.526905Z digest=sha256:9e69277834204e0d2704408bfb50c4a7a9938fe7656e57f49faf1e622cf27f83

Observation 1d7b76e9-89cf-4a67-b463-4dd8d69ebf87 · outbound

This paper cites Astropy: A Community Python Package for Astronomy.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Astropy: A Community Python Package for Astronomy

Reference 34

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no resolver link, observed 2026-08-15T15:19:16.530789Z

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source=arxiv_source observed=2026-08-15T15:19:16.530789Z digest=sha256:6980f73b02a29fdccec2c48c3ad08a8975592f90a39a154df7142bd009506474

Observation a116ff53-790e-47e1-a41a-507641c1ade1 · outbound

This paper cites The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package

Reference 35

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no resolver link, observed 2026-08-15T15:19:16.534908Z

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source=arxiv_source observed=2026-08-15T15:19:16.534908Z digest=sha256:d400f949b2599ce868cbbec3ec3d50ca087e8b353c36efdfd00d1e4ec2ab16b0

Observation da56bfdd-d1c5-448b-a049-322b63f3c571 · outbound

This paper cites , keywords =.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir , keywords =

Reference 37

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unresolved
no resolver link, observed 2026-08-15T15:19:16.542702Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.542702Z digest=sha256:044f9d873af3f52cae42055a3b09c490a3536ce652bf4dbeeb04208850c04c75

Observation 0d4e3c2e-5109-4959-9ca0-867f347e838c · outbound

This paper cites Discovery of eight 'Main-sequence Radio Pulse emitters' using the GMRT: clues to the onset of coherent radio emission in hot magnetic stars.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Discovery of eight 'Main-sequence Radio Pulse emitters' using the GMRT: clues to the onset of coherent radio emission in hot magnetic stars

Reference 38

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unresolved
no resolver link, observed 2026-08-15T15:19:16.545935Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.545935Z digest=sha256:632c6f09df738ed8d700f9a3e0b0ae53518f9a9729c3d7db75b88714b7123329

Observation ebe4dfc8-af37-4027-a0aa-76c5ab4a466b · outbound

This paper cites Observations with moderate dispersion.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Observations with moderate dispersion

Reference 39

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verified exact
doi, observed 2026-08-15T15:19:17.848019Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=arxiv_source observed=2026-08-15T15:19:16.549504Z digest=sha256:52e9757d18145a3e29b180ff1317b40b4e9b3e880688d6081045b8c7597b69c0

Observation 6e3e1be8-2684-4f34-9a09-efb5cdbbfaa6 · outbound

This paper cites A circular polarisation survey for radio stars with the Australian SKA Pathfinder.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir A circular polarisation survey for radio stars with the Australian SKA Pathfinder

Reference 40

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.552796Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.552796Z digest=sha256:00878ab6878391fba0d25126935d1e5ee8625097f7c070b87589bbe13c478200

Observation 5408aa40-7e17-443c-b07d-b4186f4871e0 · outbound

This paper cites Testing a scaling relation between coherent radio emission and physical parameters of hot magnetic stars.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Testing a scaling relation between coherent radio emission and physical parameters of hot magnetic stars

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.557498Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.557498Z digest=sha256:9b201d82613c37ec36e9943935db3ed9833753fcc90a00ddce001dd21cf9f037

Observation 307795ce-b8ef-440d-8573-d7f72a19721b · outbound

This paper cites What leads to premature upper cut-off frequencies of auroral radio emission from hot magnetic stars?.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir What leads to premature upper cut-off frequencies of auroral radio emission from hot magnetic stars?

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.562197Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.562197Z digest=sha256:8e17c5c397984aff2b9d56998dbe7af5882315d87f4894b663be2992edb2a017

Observation db960274-1159-40ae-87d4-143d138ea369 · outbound

This paper cites On the spatial distribution of electron energy loss due to gyro-cooling in hot-star magnetospheres.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir On the spatial distribution of electron energy loss due to gyro-cooling in hot-star magnetospheres

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.566082Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.566082Z digest=sha256:8e4e3d108e010f54bec51c9814ffe7a93868ebbc1f925bf9d5ebadda700f30e0

Observation 47f73ca3-66dd-47f8-bc38-b48138001de9 · outbound

This paper cites Discovery of extraordinary X-ray emission from magnetospheric interaction in the unique binary stellar system $\epsilon$ Lupi.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Discovery of extraordinary X-ray emission from magnetospheric interaction in the unique binary stellar system $\epsilon$ Lupi

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.569664Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.569664Z digest=sha256:6720028a9b5a88619b6c99f0adbadb8bfa738e09972ce8ba0ae6a75e6b4c7de8

Observation 69997a28-20ba-413a-ba59-7230907527b5 · outbound

This paper cites An `Analytic Dynamical Magnetosphere' formalism for X-ray and optical emission from slowly rotating magnetic massive stars.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir An `Analytic Dynamical Magnetosphere' formalism for X-ray and optical emission from slowly rotating magnetic massive stars

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.573344Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.573344Z digest=sha256:99637130e563717ef910edee0493e393294ea8c320bb32d342f139db808d6348

Observation bf375c2b-b535-4321-94ba-51a22648b469 · outbound

This paper cites Periodic Radio Emission from the T8 Dwarf WISE J062309.94-045624.6.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Periodic Radio Emission from the T8 Dwarf WISE J062309.94-045624.6

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.577294Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.577294Z digest=sha256:92a62ce7a506d561144549b9036981288c79cabed7ff07bdc35a7959898cb6a4

Observation a274f645-aa0a-455f-9f24-38d63b0fddb9 · outbound

This paper cites Unravelling sub-stellar magnetospheres.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Unravelling sub-stellar magnetospheres

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.585191Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.585191Z digest=sha256:2b0538ebb99e0b7844e888f5b1a6d90a411fef0010284827c0960727decc7fcf

Observation 7c88f164-372b-49a8-b9f9-7814e79e466a · outbound

This paper cites Confirmation of the Electron Cyclotron Maser Instability as the Dominant Source of Radio Emission from Very Low Mass Stars and Brown Dwarfs.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Confirmation of the Electron Cyclotron Maser Instability as the Dominant Source of Radio Emission from Very Low Mass Stars and Brown Dwarfs

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.589088Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.589088Z digest=sha256:5b13eb5e81715a4cf5a22603d74e03ac6856ca417dd55e9e13d98846bf8748f2

Observation 9162ca54-a9d4-4055-ad3a-8d3990518c17 · outbound

This paper cites A fossil origin for the magnetic fields of A-stars and white dwarfs.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir A fossil origin for the magnetic fields of A-stars and white dwarfs

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.596609Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.596609Z digest=sha256:625675970d6fda4e20f904f5bc409907828dc4562da498043b5b5e1f690044cf

Observation 05bd7622-0801-409e-8efb-88c5a3c20851 · outbound

This paper cites Auroral radio emission from late L and T dwarfs: A new constraint on dynamo theory in the substellar regime.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Auroral radio emission from late L and T dwarfs: A new constraint on dynamo theory in the substellar regime

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.599982Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.599982Z digest=sha256:68145477cd1dc8736836669f5ef0691e274992935ea79b9ede825ddecba2982c

Observation a104f64b-b15b-4821-aa48-30a75689155a · outbound

This paper cites , year = 2016, month = sep, volume =.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir , year = 2016, month = sep, volume =

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.603652Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.603652Z digest=sha256:9b2138338daf4a18f45da77b084b139d2f877924940560af3687a4b9262a795b

Observation d7080209-5924-404a-b3c9-2a7d437c8ac0 · outbound

This paper cites CHIME/FRB/Pulsar discovery of a nearby long period radio transient with a timing glitch.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir CHIME/FRB/Pulsar discovery of a nearby long period radio transient with a timing glitch

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.607211Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.607211Z digest=sha256:f13ae8ee4c0b6a7d225921ba2d8f5c3da5e29e3dc15be945c75284f51a090da2

Observation 80ca3fe8-0379-4467-9556-0aba54cce55e · outbound

This paper cites An emission state switching radio transient with a 54 minute period.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir An emission state switching radio transient with a 54 minute period

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.611498Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.611498Z digest=sha256:45936a139c863da7682829cf0d0e19d6b06829444e7c18f33a9178256f622dcf

Observation 62f01e08-4046-4424-9c05-4f48337a258e · outbound

This paper cites arXiv e-prints , keywords =.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir arXiv e-prints , keywords =

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.614383Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.614383Z digest=sha256:4cdaa2d8b855bda609955deb43c4e005baa6a1b12104d6063d038530a8e0be3e

Observation 217753a0-9d20-470f-8100-b26eb287d35d · outbound

This paper cites Peculiar spectral property of coherent radio emission from a hot magnetic star: the case of an extreme oblique rotator.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Peculiar spectral property of coherent radio emission from a hot magnetic star: the case of an extreme oblique rotator

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.617952Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.617952Z digest=sha256:cc35284419e70c76cac30335e7a6a277eeae2dba210ca0691db23ef76c2d01a6

Observation 11982dc7-0f9c-40ff-bade-6d02f6d079ef · outbound

This paper cites A 3D framework to explore the propagation effects in stars exhibiting electron cyclotron maser emission.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir A 3D framework to explore the propagation effects in stars exhibiting electron cyclotron maser emission

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.622028Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.622028Z digest=sha256:4aa9a48b69d62096cc8024f4b5ed9a137e2076e1a11eb19c708fbb360dbe22ad

Observation de7a21f2-abeb-4be4-966a-27d32f9f0283 · outbound

This paper cites Resolved imaging of an extrasolar radiation belt around an ultracool dwarf.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Resolved imaging of an extrasolar radiation belt around an ultracool dwarf

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.625876Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.625876Z digest=sha256:6c70b615351fa75e6e211c6cd8d5b7bd8246ab0f9dc453360091e85a4b902c29

Observation cd45b781-8dbb-4e8c-8c0a-00e6b03d22df · outbound

This paper cites Finite diffusion effects-an illustrative example.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Finite diffusion effects-an illustrative example

Reference 60

Resolution
verified exact
doi, observed 2026-08-15T15:19:17.761067Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=arxiv_source observed=2026-08-15T15:19:16.629474Z digest=sha256:3b87f5769593658c148ecb8919477d38df9afca1e8e801eaa8fe0a588d7036e1

Observation 0923940f-d9c4-4086-87c9-601009c00332 · outbound

This paper cites arXiv e-prints , keywords =.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir arXiv e-prints , keywords =

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.633082Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.633082Z digest=sha256:69c27617153491093a5fb3eb8e9feaa18c9f74ef59c5f4765c7d37f9abf17be0

Observation 60c140de-2d87-483f-a50c-2185c10bdce4 · outbound

This paper cites , keywords =.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir , keywords =

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.640985Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.640985Z digest=sha256:c85ebf7d7d513fb35ca30fa48b3ab97d8914cdcc4dd036848478e8bc431f18e9

Observation 79cac57e-3189-4a6d-9be5-6013b6d077dd · outbound

This paper cites Discovery of new magnetic early-B stars within the MiMeS HARPSpol survey.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Discovery of new magnetic early-B stars within the MiMeS HARPSpol survey

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.644716Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.644716Z digest=sha256:705ddb6a1fa3355f52e7f36bd7b9802170311b91f256ff82e7dffb537182efe2

Observation c09f619b-4c67-463f-a3a4-a3db665ed04c · outbound

This paper cites A Magnetic Confinement vs. Rotation Classification of Massive-Star Magnetospheres.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir A Magnetic Confinement vs. Rotation Classification of Massive-Star Magnetospheres

Reference 65

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.649442Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.649442Z digest=sha256:0b8bc074911f32e612154711bd1657d741b3003e84a1bc1856a8c6a4d0e114be

Observation f2ed751f-4826-45b0-af2a-bf3ba152df71 · outbound

This paper cites The MiMeS survey of magnetism in massive stars: Magnetic analysis of the O-type stars.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir The MiMeS survey of magnetism in massive stars: Magnetic analysis of the O-type stars

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.653962Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.653962Z digest=sha256:e92a7734da307659e4a3dfc21a0c6f42309566a1940dcaea7fca8c21e3a32c5e

Observation 69f16355-5778-4e58-ae7a-c11b7486fceb · outbound

This paper cites , year = 2020, month = jun, volume =.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir , year = 2020, month = jun, volume =

Reference 68

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.661413Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.661413Z digest=sha256:a37837b752cece6395014ff5dc464b0803b9a2aab06b81faf795b605075866f2

Observation c26637c0-88d2-47e6-a779-5b89dbaab99b · outbound

This paper cites , keywords =.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir , keywords =

Reference 69

Resolution
verified exact
doi, observed 2026-08-15T15:19:17.721870Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=arxiv_source observed=2026-08-15T15:19:16.665035Z digest=sha256:0f56428dd0a9230fc97a28e4802686e285742af99922cdb2e44d4f528dbd01fb

Observation aca11180-c90e-426c-b21b-ed342a0cc458 · outbound

This paper cites , keywords =.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir , keywords =

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.668620Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.668620Z digest=sha256:510c27649d0d0b5e3952822afc4928cc91805b59488994612600940dcdc29980

Observation 4fa2ae52-b361-42c9-b79b-5614cce88d35 · outbound

This paper cites an unresolved cited work.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Unresolved cited work

Reference 72

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.675058Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.675058Z digest=sha256:64fbae34a4d0e326d72c0a1f2a154975620b0ef82736d47b6215cad7fc2afc20

Observation bbea687c-33e6-41a4-b16a-f8dc2be1fe31 · outbound

This paper cites , keywords =.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir , keywords =

Reference 73

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.678556Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.678556Z digest=sha256:5440ba44a66e606cbb8846215c0503e9c5af808f28dd5b88c0572df37feb7895

Observation 8cfd6973-56e4-47d1-9fe1-b1cc9f139440 · outbound

This paper cites , keywords =.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir , keywords =

Reference 74

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.681279Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.681279Z digest=sha256:5ba3cc593ea3cb25aeeee46ae5ea3f945450bb5f8517585f23e849b62b614e4f

Observation 9d1b1bfa-cd9e-4bec-b963-111c7e688dd0 · outbound

This paper cites Magnetic field topology and chemical abundance distributions of the young, rapidly rotating chemically peculiar star HR5624.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Magnetic field topology and chemical abundance distributions of the young, rapidly rotating chemically peculiar star HR5624

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.687736Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.687736Z digest=sha256:538b37b9f96315df15015f1667f8ef17038d365907def53e43e820ecb6ae3420

Observation 2ebba0ce-d18d-4338-9b78-ec36836c286c · outbound

This paper cites , keywords =.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir , keywords =

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.691577Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.691577Z digest=sha256:823cbbf8ae1bc9846bb043d4fa5e355d78fad9a9aabff0d8d46f32f2d962af44

Observation b0093c25-ac17-41a9-bb62-4eb9cc43a378 · outbound

This paper cites Radio emission from the stars and the sun.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Radio emission from the stars and the sun

Reference 78

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.694922Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.694922Z digest=sha256:666d6df1ddfa7f629fdeca52dfc4398bd49d89d6338ce53e0b6a2f96f8d97b2b

Observation 33c04998-96e8-4a41-af4d-51ed5fce1684 · outbound

This paper cites The Magnetic Early B-type Stars IV: Breakout or Leakage? H$\alpha$ emission as a diagnostic of plasma transport in centrifugal magnetospheres.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir The Magnetic Early B-type Stars IV: Breakout or Leakage? H$\alpha$ emission as a diagnostic of plasma transport in centrifugal magnetospheres

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.701750Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.701750Z digest=sha256:9a7ba999e6f02ad914e4e3126ce1a17b1c0a7941206fad4bb362f8704bd4b95a

Observation 7bc806ef-9ff0-469a-a638-9bba28279d5b · outbound

This paper cites , keywords =.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir , keywords =

Reference 81

Resolution
verified exact
doi, observed 2026-08-15T15:19:17.679494Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=arxiv_source observed=2026-08-15T15:19:16.705480Z digest=sha256:626bc10296790243e751bb96bc456b6696c0af46c32f593ae44997c14e34e241

Observation 9b93f7f4-576c-4564-964d-ccfc527a9c8e · outbound

This paper cites , keywords =.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir , keywords =

Reference 82

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.709171Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.709171Z digest=sha256:a9a8214f4f62cdd26a63cc05d839f2ded1e2acef73c9c9c99b1d23c695fc48c1

Observation 3d109258-e610-4677-87c6-a1ee1cb4d3dc · outbound

This paper cites The Kepler Catalog of Stellar Flares.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir The Kepler Catalog of Stellar Flares

Reference 83

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.712898Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.712898Z digest=sha256:878c0c758e8a2a2686d5d99721f2bc62f89f9b0a1991728ced5e736686bb05ea

Observation 10e32815-8646-4bcd-a0b9-d65674a83428 · outbound

This paper cites Characterisation of stellar activity of M dwarfs. I. Long-timescale variability in a large sample and detection of new cycles.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Characterisation of stellar activity of M dwarfs. I. Long-timescale variability in a large sample and detection of new cycles

Reference 84

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.716739Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.716739Z digest=sha256:5f23ccc7255e9cb78bd4b02e0847abaa7c05fa846dd079e675a0165a023185dd

Observation b9d74126-90ab-4d07-a554-20d0bb95f720 · outbound

This paper cites , keywords =.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir , keywords =

Reference 85

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verified exact
doi, observed 2026-08-15T15:19:17.660369Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=arxiv_source observed=2026-08-15T15:19:16.720454Z digest=sha256:9ffafa868c5a35ea4509d640325651d984155a6364721efd9d872a9ccbef951d

Observation 6c2c9637-72c2-42e5-aa67-223a8190f1ec · outbound

This paper cites Magnetospherically driven optical and radio aurorae at the end of the stellar main sequence.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Magnetospherically driven optical and radio aurorae at the end of the stellar main sequence

Reference 86

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.724088Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.724088Z digest=sha256:4d76efd03b7d01071deabe63a0a40c0e5194caf63f2e0f55ee5dfb009de41e85

Observation bbbe0295-59a9-41fe-92e8-60c665822f10 · outbound

This paper cites How the breakout-limited mass in B-star centrifugal magnetospheres controls their circumstellar H-alpha emission.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir How the breakout-limited mass in B-star centrifugal magnetospheres controls their circumstellar H-alpha emission

Reference 87

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.728245Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.728245Z digest=sha256:c738e29cf19e5ed496a3cffed30f36c77acc53001cfdec291b3f15f87fec6711

Observation 2f9316b0-163d-4fbf-b51e-5823854dcec8 · outbound

This paper cites Detection of magnetic field in the B2 star $\rho$ Oph A with ESO FORS2.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Detection of magnetic field in the B2 star $\rho$ Oph A with ESO FORS2

Reference 88

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.731653Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.731653Z digest=sha256:2d0412a59c3df925f555865d185c9a5c392b4b6f1f635c524e42042a77a9bb67

Observation a0c3bb0a-9864-4faa-8b8a-27ee0a7bae8a · outbound

This paper cites Evidence for radio and X-ray auroral emissions from the magnetic B-type star rho Oph A.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Evidence for radio and X-ray auroral emissions from the magnetic B-type star rho Oph A

Reference 89

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.735543Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.735543Z digest=sha256:ca9ad54ff4e21b9d6fa54cd0a2ceceafeb0e97695e21aa50d498c3e168532490

Observation ce4000d6-ac11-4f49-9a27-e01c6a1e9883 · outbound

This paper cites Comparative analysis of two formation scenarios of bursty radio emission from ultracool dwarfs.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Comparative analysis of two formation scenarios of bursty radio emission from ultracool dwarfs

Reference 90

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.738414Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.738414Z digest=sha256:40f2ee9bb5a501c810a3facc7d22a65f3ca3d1f3bf37a726154db0066bed69e9

Observation 4b519cc0-5a13-410b-8f54-0948218ab882 · outbound

This paper cites MOST Observations of sigma Ori E: Challenging the Centrifugal Breakout Narrative.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir MOST Observations of sigma Ori E: Challenging the Centrifugal Breakout Narrative

Reference 91

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.741271Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.741271Z digest=sha256:48cfff5bdd9bd1525f09cbb17f42ccb02341bb9b4abaa9dd796dfc5e8347d4cc

Observation b614e093-dcea-4168-b78f-7b7834c5aa3a · outbound

This paper cites Physics of Magnetic Stars , year = 2019, editor =.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Physics of Magnetic Stars , year = 2019, editor =

Reference 92

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.744860Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.744860Z digest=sha256:4d9fc0af7b98033d1601552af2840e8a4e230ff2e2c81370310b64372df69719

Observation 34c08acd-9c29-47ee-94f6-53539398fa3d · outbound

This paper cites Recurring millimeter flares as evidence for star-star magnetic reconnection events in the DQ Tauri PMS binary system.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Recurring millimeter flares as evidence for star-star magnetic reconnection events in the DQ Tauri PMS binary system

Reference 93

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.748195Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.748195Z digest=sha256:d3244282663cf0e95c4f7d7428f92e7dd1a3bb1a74a6aa74482a78add1fef8df

Observation 9fefa13b-539a-4c2d-bb21-264de4099978 · outbound

This paper cites The BinaMIcS project: understanding the origin of magnetic fields in massive stars through close binary systems.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir The BinaMIcS project: understanding the origin of magnetic fields in massive stars through close binary systems

Reference 94

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.752579Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.752579Z digest=sha256:84e3b4e470981815ea9021be3d4dae009e1df70b9334aa045d0f1cf9e3a05bb5

Observation b1c3c803-6436-4fb5-a529-13895a483faa · outbound

This paper cites Wideband Dynamic Radio Spectra of Two Ultra-cool dwarfs.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Wideband Dynamic Radio Spectra of Two Ultra-cool dwarfs

Reference 95

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.756553Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.756553Z digest=sha256:df3d1e50149255fc8de12778657ad311f503f713495fdefb5ebd9cc4c946fec4

Observation 48cfe761-0eee-46f8-b1d6-c63eceb93b89 · outbound

This paper cites The Young Binary DQ Tau: A Hunt For X-ray Emission From Colliding Magnetospheres.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir The Young Binary DQ Tau: A Hunt For X-ray Emission From Colliding Magnetospheres

Reference 96

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.760199Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.760199Z digest=sha256:92147c4dacd00f627dd5064364090240869949a39a7e82ff1d395fc1f01e7c63

Observation 5c91d3a3-3ec9-4e24-94cb-1a6f21ef0e1c · outbound

This paper cites Discovery of electron cyclotron MASER emission from the magnetic Bp star HD 133880 with the Giant Metrewave Radio Telescope.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Discovery of electron cyclotron MASER emission from the magnetic Bp star HD 133880 with the Giant Metrewave Radio Telescope

Reference 97

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.764088Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.764088Z digest=sha256:e03d2bdca3b386c33078ff48c86ba6432e2389c3862d55547d58e5e238384988

Observation d50f1811-95b8-4239-bf46-1329fb0721a6 · outbound

This paper cites The MiMeS Survey of Magnetism in Massive Stars: Introduction and overview.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir The MiMeS Survey of Magnetism in Massive Stars: Introduction and overview

Reference 98

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.768684Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.768684Z digest=sha256:16903bb8a609e28562eff5b701f03825b2496de28be5de1064564f1ca8f68f5e

Observation 2ea35530-a430-4b8c-b25b-79ca8df293a2 · outbound

This paper cites Energetic particle activity in AD Leo: Detection of a solar-like type-IV burst.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Energetic particle activity in AD Leo: Detection of a solar-like type-IV burst

Reference 99

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.772554Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.772554Z digest=sha256:0d1288df08b078ae8e5a20c660c7cf42b89818e9b204ee5a2dbc7873e93fe471

Observation 1006e22f-8276-4473-b9d5-e79b129c1a90 · outbound

This paper cites The emission of interpulses by a 6.45-hour period coherent radio transient.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir The emission of interpulses by a 6.45-hour period coherent radio transient

Reference 101

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.779816Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.779816Z digest=sha256:50a75bdb3ae0d5804743eeeb95a358501768f864670b0d23f1de6ed389105238

Observation ef296534-f4c9-4131-8066-9900a2d886af · outbound

This paper cites , keywords =.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir , keywords =

Reference 102

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.783252Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.783252Z digest=sha256:a5d190e853a03856af8b89f7bfd79ece229d53332f8aea980570e34c0bda894a

Observation 2f57a957-00c9-4407-a879-417792008371 · outbound

This paper cites Low-frequency pulse-jitter measurement with the uGMRT I : PSR J0437$-$4715.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Low-frequency pulse-jitter measurement with the uGMRT I : PSR J0437$-$4715

Reference 103

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.787000Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.787000Z digest=sha256:1a020d48cb15d0b3e011fd24d6ccffd06e5b70cd37982309b83acc3214953324

Observation 8c4132f7-8224-4f53-8d6f-9bc92c709a6a · outbound

This paper cites The NANOGrav 12.5-Year Data Set: The Frequency Dependence of Pulse Jitter in Precision Millisecond Pulsars.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir The NANOGrav 12.5-Year Data Set: The Frequency Dependence of Pulse Jitter in Precision Millisecond Pulsars

Reference 104

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.790575Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.790575Z digest=sha256:b472af256b0e90946bf8aac52558354dcaff3d1a7805d27a7eae76f9ea59a433

Observation 5fba31a8-d7b7-4370-b668-6a156a0b4ab2 · outbound

This paper cites Discovery of the peculiar supernova 1998bw in the error box of GRB980425.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Discovery of the peculiar supernova 1998bw in the error box of GRB980425

Reference 106

Resolution
malformed identifier
no resolver link, observed 2026-08-15T15:19:16.796047Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.796047Z digest=sha256:d4661a664699fa1fa82d97151cf2d79063cfc3a8feb206ea6fa80548a9fd2198

Observation bc1925e0-6a6d-49f3-88b8-8dd6698daf3b · outbound

This paper cites , year = 2022, month = jan, volume =.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir , year = 2022, month = jan, volume =

Reference 107

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:16.799399Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.799399Z digest=sha256:d7480efbac7e5907e332b4d6720ff4ea6f280691e299f00498635f4f3d93b015

Observation 83d148a8-58c9-4e3b-b744-cb655fcec80e · outbound

This paper cites an unresolved cited work.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Unresolved cited work

Reference 108

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unresolved
no resolver link, observed 2026-08-15T15:19:16.802801Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.802801Z digest=sha256:8d2f28e4b8f242a706707b1bbbcf4ed1daa7f530381cd15a802b359c2e6d5ba5

Observation 90e11bf7-51e1-40b5-b479-4767e32d5d0d · outbound

This paper cites Radio Variable and Transient Sources on Minute Timescales in the ASKAP Pilot Surveys.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Radio Variable and Transient Sources on Minute Timescales in the ASKAP Pilot Surveys

Reference 109

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unresolved
no resolver link, observed 2026-08-15T15:19:16.805763Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.805763Z digest=sha256:48b3cfe8288e8d9b83ca9afbb10896216c1d1d7a3bbf9f427fb830a665db6170

Observation 8665ff77-9bf0-4c20-8a34-834f2c7b3d44 · outbound

This paper cites Metrewave Galactic Plane with the uGMRT (MeGaPluG) Survey: Lessons from the Pilot Study.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir Metrewave Galactic Plane with the uGMRT (MeGaPluG) Survey: Lessons from the Pilot Study

Reference 110

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unresolved
no resolver link, observed 2026-08-15T15:19:16.809612Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:16.809612Z digest=sha256:77ef459a6336c1e904d65758507ba55b79c42f9b388e19bfc3cfde90be8526da

Observation 5331b254-0ba0-43e8-ac25-97d288a6c26a · outbound

This paper cites uGMRT Band 4 Polarimetry.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir uGMRT Band 4 Polarimetry

Reference 111

Resolution
metadata mismatch
local_arxiv, observed 2026-08-15T15:19:17.627989Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=arxiv_source observed=2026-08-15T15:19:16.813705Z digest=sha256:99f8cf437c10dcfe77104e86e54ae5a89b97170b16cff95a9ff38e0548e06a8c

Observation 960b3b9e-7c1c-4c97-be9a-29d34f455bcb · outbound

This paper cites A detailed study of the polarisation convention of the Giant Metrewave Radio Telescope.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir A detailed study of the polarisation convention of the Giant Metrewave Radio Telescope

Reference 112

Resolution
metadata mismatch
local_arxiv, observed 2026-08-15T15:19:17.612491Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=arxiv_source observed=2026-08-15T15:19:16.817648Z digest=sha256:17715deffb5bb625c220c7be32da294f38f602539cb25ece1af953d33edd818e

Pith citing papers

No inbound Pith citation observations are available.