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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 22 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 2026-08-21T06:32:19.484+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:f73380ebe8ee9f9f558a69ffdb1b980a7008169df1d6b353735080242cb869aa

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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source=arxiv_source observed=2026-08-15T15:19:16.396543Z digest=sha256:00e2bae603e7d80cd49439c7d249130dd3bb59cd8b6c0e5fac6d463bcb313888

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=sha256:44a31ad571017fefb5f7b1dab8c443109ecd5cd4db830eeb87986510a80fc9a4

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:b4b385201365f458b2e43df15c5480daf9e295c3881513471e0bba6da57c4ab2

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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source=arxiv_source observed=2026-08-15T15:19:16.413625Z digest=sha256:c5f5b8cb8800486fbfb6e1cc5e435f68617e956363ad4e318a527e01d14504f4

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=sha256:39a58e2e96319d45a0b1f76711e9de4bdcb770dc3b2e9f97570605eee4f818e9

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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source=arxiv_source observed=2026-08-15T15:19:16.421311Z digest=sha256:97302eaa7c7cae11422dc3ae03756725c4f7c7b6cfdd46e3940ac336de19ee3b

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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source=arxiv_source observed=2026-08-15T15:19:16.424911Z digest=sha256:43d2b89daf41480727fd20c0955671fe5651b39592894b5a9c4796d237d3f48b

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:b5e96340d565a9a438fdad27f78cdd535194166ecd62a0f781e2bb528c841b70

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:a596ed2fcd36435fb029b10f915fd12ed377fd9168ea158d2ba122db7783e982

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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source=arxiv_source observed=2026-08-15T15:19:16.439033Z digest=sha256:f98c5e6e4f6457096257af10e5f93cdeb1ded18dbef7521f9a2fb63618299e3d

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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source=arxiv_source observed=2026-08-15T15:19:16.443077Z digest=sha256:29b3544fc50f24a8cae64d0d86b794dbc459d5f13733ecd185f31f1039f808bc

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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source=arxiv_source observed=2026-08-15T15:19:16.447468Z digest=sha256:3284346fe583d6defd0e12fe15401172e4413212b39d216fefb976ae7c4cd64a

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=sha256:7290933177c5e9c4dc6f390a7b675f6f73dba354f6c5d26d155ab26ddd210942

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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source=arxiv_source observed=2026-08-15T15:19:16.456380Z digest=sha256:48f279589fcf4552e084595b747e6dd6cb22dc9c4a432d337ff7bc2ecc3b7922

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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source=arxiv_source observed=2026-08-15T15:19:16.460218Z digest=sha256:5abc6a4b07e90634223c4d08bacd7408372fd22eacbec622b13520f1811cd23c

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:bf7d8a55a93d92b1fad030871c8a5bfa81f23a64308dd0b5ecedf9b2e680f319

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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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-08-15T15:19:16.467894Z digest=sha256:c48727bf2f0bd1b60eaaca799729c2944f1db47bea07a899a9915e24b0a6987c

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:d13732af7d6ca1dad66fae28e950334f641500d905696880bcf5c751fd9f3511

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=sha256:0b165b438250172fc7e6573adbc9e1543c935015e94236288ff40ddeff1ff5c5

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=sha256:3e900275555cd5005a8cd35de03d29d34d9513e2e5623e946aef371f2075a055

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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source=arxiv_source observed=2026-08-15T15:19:16.485128Z digest=sha256:ade90116ad797c60a0b86ad2e6f2702373ea3f4eb2943b80e6be92d5e6dd1e64

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=sha256:5a386c398bedc12d5583ede188d3b1b9d6c95473371d6a7384870a8e76ad0af3

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=sha256:00d4f224651dcda3fc8de37bfd8efda7734da3dad3751519bb9918e4a5e2ab12

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:b5c819e7cccd7b6cf53d10589ff4e9f12b888e4322e2513a04897adb073fd163

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=sha256:8ceed98cf78e6822669c6ed440e6ec1c46325f56ac722526054d80f6dee1baca

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 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-08-15T15:19:16.506425Z digest=sha256:81cd0624d17b2dea399465fcbcefb2ea4804aa5d8bfd632f3a78af32e543f607

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=sha256:97c891dfd0e8632124e12e596402da8acf4fb1ad3ab7439973f42bb9d287fc58

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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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=sha256:472616b28e451ad21b63bfe6d85f3baaf2c145d0fbbf1f8eb28120c9b0ae17e7

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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source=arxiv_source observed=2026-08-15T15:19:16.519075Z digest=sha256:997be1876edcc478768ba063670373898f9783f799b15e5a9230f8a728e896e9

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:f16baf5fea8263e9fe3f074577ce59bca4196a365d05ed5e7388c0d67e76cac5

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=sha256:654948fb084c0164e998d5196655714968fb5cd6e47e582de7385236a3cc7897

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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source=arxiv_source observed=2026-08-15T15:19:16.534908Z digest=sha256:f46925bb79fe1000574c8e438b6b7a1a25f8da4d6302fc17223aa357d2145611

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

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source=arxiv_source observed=2026-08-15T15:19:16.542702Z digest=sha256:88ebc5ece4345aaead42a85c1b44c8038613377618983b549e7a4fe4379f4cdf

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

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source=arxiv_source observed=2026-08-15T15:19:16.545935Z digest=sha256:f723efca8b83702006b43df5c96491f0f1fb8620f9a29836af29a8d4ad273af6

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 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-08-15T15:19:16.549504Z digest=sha256:fc386123e0d09e21ce48929ef5468b3f3acb5fb885080bac7e1833609ec3ea70

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=sha256:36eb21d28772ba48a4e6dc27c3eab8c3c05cb89e8c5fe439148a6b9b5e547fc7

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=sha256:526877853d3aeca31281490ff72df990cf5aed7d9ab8a8dba79b55160f8ca89b

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=sha256:50ce1624ab15d22521e0a958cae850a6b713b841863d0936bcf1e2419da529fa

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:b851cba1059527212c476162526c5c5e1fd160587e008e92835e38fabc7f7f89

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=sha256:37774bb524ef51cec598c41bfd306b68b6e920d108d971dc8c7ade564e157c99

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:eaa866cbda3ecaea1fb83c196abbf589438ee5b437ea98f5a31293ec08d4dede

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=sha256:67ec5d89077b94b5bd6fd56da2b934d3c08521878ad16fe2a15b34c0f4196d11

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=sha256:4026a8273d2f94479461e90d3b150a2ca31515293ebf7fa3694f7896b891f656

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:a154531ef800c78d8262862f98d978a2dbab4723f1fbd267da751a54c7b4e0e9

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=sha256:3ff3d1489fdcffde44923af823c182f21c2f0ddc743a20816758ebe448138a67

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=sha256:99c6ae402f214c67fe675532b91618ef919896fb77d3dd511a5365e7d2f1f1ad

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=sha256:0264f112217f5ae31065eb435358efd6c4674946fb48a204d60c9b00a21d569b

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:da07b54a4fec9ae5e44e697e96bab39dd4548eed3aa927916862704282cab7f3

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=sha256:0f229d1dd04816b07875649f3108e31159531e7775bf33b86116b01041674c8c

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:b7313f366fdb0048be51f17d5c70d4801a0c340e62ecd7bad0afa5b54ee77408

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:ea221b96b381eb182dce6a839f1e8ed6a01b1580e4ee2694cac79cd026233d18

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=sha256:6ac5af9c99c86ba1983a6f0f62b34cbd979832023b626ad85c06afc2fef294ea

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=sha256:0553b6593f306b6e50c77134bec8e826e8d2bb151219f41c152bfff6b29b7390

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 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-08-15T15:19:16.629474Z digest=sha256:efcc0556d96a366fcca6a13395d718cae7357b6af2732d252a6ad2966cf77e22

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:fed6549be0c87a52d62ee3b3fa2cb12c45afbdb3519ec8c1fe5d5676731f4323

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:ecad66463cb422febf6c9320de54ce0ec0e532d926608db5204154894b20623d

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=sha256:728b2976328c64841ff83b0188237bdb26c440dc2d011769668e6d7345e68e5e

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=sha256:63b4dea46b396947581384cfff3845b297a84fc22e96f0b47f4bbeeaf3bb7de1

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:dd27d89492923b30ef9a9e157b96162b46c62e5328d7444590c2a69d873051e5

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=sha256:7926ee816c05668e1de6c6085a30386bc81b20f697c933eb4aaf683ea416e37f

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 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-08-15T15:19:16.665035Z digest=sha256:b7fd6cd7eec53546eb6a9d10a49f7c607bb2ec30c36ac802103114a5f6a9abcb

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=sha256:07ca64fa77c2955b836512252460a7271f7a74ca86e3a072175d6f29b35ca022

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=sha256:0944e5b9acaea0b07c98bc7255f6971b0bb61879480ed3446160864b409ef367

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:a26e463d0545ef8348ff17756c5b61fab099eac523fbfede12e58462d0e9669b

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=sha256:85025f07d220fa57920248ceb0b04740bd968b7a44d69af2b2e6bac047b2552d

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=sha256:5d356c5380eb0039ec83dd98b5eb15dfc36c7a1a201f31bb6e31ef09a3835e3b

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=sha256:1f4b8f7422c433debbf2a2f8b1a89e52c877a1caabab19c3941038e2ec853404

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:fac3ac47d9c468186b67a103d39e9ce900bcdf86ca39dedc8369d0fc369aa9bd

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=sha256:0963d57b0bc88c6b32ac6c0abf367a4218814fc88648bbc0095dfe130d7b1aea

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 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-08-15T15:19:16.705480Z digest=sha256:09e683bd9181750f35aa1a1430f197c1445c7dc12a98d787832bdeac7bda715c

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=sha256:88c253931fbc6c2ec9377c235f64df2c25fcf8a9a26190c3fb7814a67b47b204

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:a35c0b1634c49ef180a149c0243104a4506e211676bb95b5139f5b3fdd7faad1

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=sha256:76d32dc7d7035282298951c93931d34b666d54250e0428aebd903782570afbd3

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

Resolution
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 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-08-15T15:19:16.720454Z digest=sha256:f9343074cc5cdc317daa5b8b8831f001e8f70eac031fe5027395a000c2589d9d

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:f6cb673eac08f141b68a12a54aecd7b37fa22df11cd18c1bba528d31b8329e77

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=sha256:2c045b8acf14bc721b878504c596a0d374cb33c713907ae157bef0c7f812fcc4

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=sha256:5ef6a8cb6e759a9127ec9d1d2991f78d3760d2fc35a827f1e997608d50576e75

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=sha256:8affdb681588f835b12bf42b1ad3c9bdb02360ffad41c44e6a524438487f5433

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=sha256:172990b698b6203a514f89f1ba3362bec61b3d612902622adf5c174244da34ab

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=sha256:49f9fc88bf883e861408f8da4b015b60fe3cc62e716d31c01073beaef7059735

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=sha256:01f494bc5aebeeebc30e36656683f88ff10230e1a5ee1eac077fd01b36578f19

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=sha256:0dea75e627bddf9889f720d3f941787993b0375fa5b49c08a02ed44dbf4659cb

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:e4ce9ecff83a40b737671e272627ff53866b5db83e311315d1c1d85d303b5afc

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=sha256:17c8079c653f9a651f1e56a47051672ead9a0f1999ca8c461c22fd917d73fa5a

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:b61151a6bcc47925e3851df34ad546f74def7eab0a60e4f99981332f58ed5c00

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:d60bbbb34492070bcbffcd04b86ef6b35dd638aa42f94bd3f4390f500fff3cc9

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:e19fe60255452a6109b22f7c7a86b5e6f14f2dad8bbf36915c7349a309f2dc52

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=sha256:3478fb3b1fa0a0236b96a5100aca85df1d4689d02e3e74f14e5b4b428feb54ee

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=sha256:03189b0156acad30436f42cea6d72c76842268708474c32426017d95863cbaa1

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=sha256:66d3505a2ac3b0da6795d29015aacc8092369ea20cd9e86bdfd86f68f49151e8

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=sha256:0dc03e6806b6b0e59369c50033049af96876f796f05a9bbd8807650797fe247b

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:a5527cccac452ea55e45077527c5d8828c6b10ff12bcea237d3a52f7172eccdb

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=sha256:20017d48a00fca77aab76e55c5e7b2584a83c7ad7be0cac93538fb6f3c394a7e

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=sha256:58e2675b732232e9766fd05e38ee394dd48072545686831b8e3984e7b83cce3e

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

Resolution
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:f7b2cdab5d71ecc8d8eff5ab56e68cbf090dea7faad7a94b309ba21fd8ca978b

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

Resolution
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=sha256:8ff8113e6af69cff3c8a785af7ae37a88651b6cd6223f5a3a211015f27b23536

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

Resolution
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:f5c877f4473ac129d2f21e650f9df283a7dd6209c884baa67efd1fd4cac3cf98

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 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-08-15T15:19:16.813705Z digest=sha256:daee1f070e4381f12e63970a441d27f14cc657359959c223204b2190d7cd0c19

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 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-08-15T15:19:16.817648Z digest=sha256:6d31f8167f89858e43b925a29c7ad3eaceb1f1ef55924532e97656e35dc9be34

Pith citing papers

No inbound Pith citation observations are available.