The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields | Paper Citation Record

Observation 2d0b4d47-a0e1-4277-bf17-f43b21cf5333 · outbound

This paper cites & Landstreet , J.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields & Landstreet , J

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:42.126608Z

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Observation 0974266e-bd82-435b-8e3a-6631f7435618 · outbound

This paper cites & Landstreet , J.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields & Landstreet , J

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:42.227556Z

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Observation 7cc8f924-0822-417a-9723-5774d7a2b53e · outbound

This paper cites A., Schreiber , M.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields A., Schreiber , M

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:42.386575Z

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Observation 9217e8ef-9a8c-4c31-a4c5-9a498371af7f · outbound

This paper cites an unresolved cited work.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields Unresolved cited work

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:42.433847Z

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Observation 2469b083-9801-425e-92df-548cdfc95b03 · outbound

This paper cites & Schreiber , M.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields & Schreiber , M

Reference 5

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T12:38:52.801072Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 9dc2f090-c73d-4ef7-bedf-adb87aa1c482 · outbound

This paper cites R., Moe , M., El-Badry , K., & Shen , K.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields R., Moe , M., El-Badry , K., & Shen , K

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:42.696183Z

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Observation d3448438-e7e3-4fbe-9d38-5854631505e1 · outbound

This paper cites R., Pala , A.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields R., Pala , A

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:42.794932Z

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Observation 41bc4e74-c63e-4201-a7cf-71042b8a97f6 · outbound

This paper cites R., Salaris , M., Maccarone , T.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields R., Salaris , M., Maccarone , T

Reference 8

Resolution: verified exact; doi, observed 2026-08-07T12:38:51.279017Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 3a5eed3a-c358-4fad-9561-a20c2b953f06 · outbound

This paper cites R., Zorotovic , M., et al.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields R., Zorotovic , M., et al

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:42.997508Z

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Observation 5e3fba50-9a61-464d-964e-7150418cafd8 · outbound

This paper cites R., Schreiber , M.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields R., Schreiber , M

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:43.095403Z

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Observation 322b0126-85ec-4236-a958-7ffd9802a170 · outbound

This paper cites 2024, http://dx.doi.org/10.3847/1538-4357/ad7a6a blue , 975, 63 https://ui.adsabs.harvard.edu/abs/2024ApJ...975...63C.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields 2024, http://dx.doi.org/10.3847/1538-4357/ad7a6a blue , 975, 63 https://ui.adsabs.harvard.edu/abs/2024ApJ...975...63C

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:43.189464Z

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Observation 37e4cb36-05fd-4813-adb5-6fdc54030060 · outbound

This paper cites an unresolved cited work.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields Unresolved cited work

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:43.340455Z

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Observation 6f4fd0e9-f6e2-457f-a3a5-e5681920b397 · outbound

This paper cites 2025, http://dx.doi.org/10.1093/mnras/staf561 blue , 540, 633 https://ui.adsabs.harvard.edu/abs/2025MNRAS.540..633C.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields 2025, http://dx.doi.org/10.1093/mnras/staf561 blue , 540, 633 https://ui.adsabs.harvard.edu/abs/2025MNRAS.540..633C

Reference 13

Resolution: verified exact; doi, observed 2026-08-07T12:38:51.015780Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 9ea2a134-ce91-4bd5-82b1-502cc72dd50c · outbound

This paper cites 2022, http://dx.doi.org/10.1093/mnras/stac2945 blue , 517, 4916 https://ui.adsabs.harvard.edu/abs/2022MNRAS.517.4916E.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields 2022, http://dx.doi.org/10.1093/mnras/stac2945 blue , 517, 4916 https://ui.adsabs.harvard.edu/abs/2022MNRAS.517.4916E

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:43.624365Z

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Observation a64203c4-c607-4392-a89a-5a23d98c05a4 · outbound

This paper cites NuSTAR broadband X-ray observation of EF Eri following its reawakening into a high accretion state.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields NuSTAR broadband X-ray observation of EF Eri following its reawakening into a high accretion state

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:43.773937Z

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Observation 7eea549a-ff42-4e41-bc44-b89c2507e459 · outbound

This paper cites & Nelson , L.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields & Nelson , L

Reference 16

Resolution: verified exact; doi, observed 2026-08-07T12:38:50.724063Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 141617fc-0ce1-4ca8-8417-a444abe050a0 · outbound

This paper cites R., Pols , O.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields R., Pols , O

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:44.007171Z

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Observation 19d33edb-245c-4cab-9d84-5965704c3f61 · outbound

This paper cites R., Tout , C.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields R., Tout , C

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:44.118415Z

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Observation ea665e1d-3fe1-4040-8ab6-feaa1ae1ffa2 · outbound

This paper cites T., Breedt , E., et al.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields T., Breedt , E., et al

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:44.220202Z

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Observation adcedcdf-b046-4bb4-a865-e7fc71f4be7c · outbound

This paper cites T., Schwope , A., et al.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields T., Schwope , A., et al

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:44.382614Z

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Observation a9158ee8-f2df-4cf2-94dc-811b7b9c1b47 · outbound

This paper cites T., Schwope , A., et al.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields T., Schwope , A., et al

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:44.517946Z

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Observation ed5afebc-9c69-4112-82d8-88cb856f5d7a · outbound

This paper cites S., Bauer , E.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields S., Bauer , E

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:44.711161Z

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Observation 6bd063a4-178e-4382-bc92-bfe97516e853 · outbound

This paper cites 2011, http://dx.doi.org/10.1088/0067-0049/194/2/28 blue , 194, 28 https://ui.adsabs.harvard.edu/abs/2011ApJS..194...28K.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields 2011, http://dx.doi.org/10.1088/0067-0049/194/2/28 blue , 194, 28 https://ui.adsabs.harvard.edu/abs/2011ApJS..194...28K

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:44.840133Z

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Observation dbdef1d7-9b4c-4813-b1ff-b1e9ca7f968c · outbound

This paper cites 1993, , 271, 149 https://ui.adsabs.harvard.edu/abs/1993A&A...271..149K.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields 1993, , 271, 149 https://ui.adsabs.harvard.edu/abs/1993A&A...271..149K

Reference 24

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T12:38:52.587658Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 57f4c072-509f-44b2-bd99-6c3f0cfff55e · outbound

This paper cites 2001, http://dx.doi.org/10.1046/j.1365-8711.2001.04022.x blue , 322, 231 https://ui.adsabs.harvard.edu/abs/2001MNRAS.322..231K.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields 2001, http://dx.doi.org/10.1046/j.1365-8711.2001.04022.x blue , 322, 231 https://ui.adsabs.harvard.edu/abs/2001MNRAS.322..231K

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:45.157635Z

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Observation 60abe1b7-e799-4e38-abf6-bf9b82a7f775 · outbound

This paper cites T., Schmidt , G.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields T., Schmidt , G

Reference 26

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T12:38:52.320704Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 316598d6-8d1b-4b72-b61c-0534892a9226 · outbound

This paper cites a nsicke , B. T., H \.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields a nsicke , B. T., H \

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:45.481901Z

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Observation e14b38d5-b205-4e2c-8aa9-bfdeb0e0b496 · outbound

This paper cites P., Parsons , S.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields P., Parsons , S

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:45.624226Z

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Observation 9cfc3ed7-33b7-4a2b-8170-032d247ba653 · outbound

This paper cites & Di Stefano , R.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields & Di Stefano , R

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:45.777260Z

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Observation 94b1b993-9d34-4848-b565-6d1c1460b3ef · outbound

This paper cites 2023, http://dx.doi.org/10.1051/0004-6361/202346420 blue , 676, A7 https://ui.adsabs.harvard.edu/abs/2023A&A...676A...7M.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields 2023, http://dx.doi.org/10.1051/0004-6361/202346420 blue , 676, A7 https://ui.adsabs.harvard.edu/abs/2023A&A...676A...7M

Reference 30

Resolution: verified exact; doi, observed 2026-08-07T12:38:50.439341Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation d2dfe591-5999-42af-9999-f636d187d8e5 · outbound

This paper cites F., G \"a nsicke , B.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields F., G \"a nsicke , B

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:46.059255Z

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Observation 19d11642-d98a-41ce-b31a-ddc145c058aa · outbound

This paper cites F., G \"a nsicke , B.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields F., G \"a nsicke , B

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:46.251401Z

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Observation aca50cc8-fbbc-4f9b-b077-3a86fec631ca · outbound

This paper cites G., G \"a nsicke , B.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields G., G \"a nsicke , B

Reference 33

Resolution: verified exact; doi, observed 2026-08-07T12:38:50.163802Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 9f0ddf25-ba70-46db-b0ec-4669b76c01af · outbound

This paper cites 2011, http://dx.doi.org/10.1088/0067-0049/192/1/3 blue , 192, 3 https://ui.adsabs.harvard.edu/abs/2011ApJS..192....3P.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields 2011, http://dx.doi.org/10.1088/0067-0049/192/1/3 blue , 192, 3 https://ui.adsabs.harvard.edu/abs/2011ApJS..192....3P

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:46.579969Z

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Observation f924bc7e-6410-42e6-b6fd-7204aa61a501 · outbound

This paper cites 2013, http://dx.doi.org/10.1088/0067-0049/208/1/4 blue , 208, 4 https://ui.adsabs.harvard.edu/abs/2013ApJS..208....4P.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields 2013, http://dx.doi.org/10.1088/0067-0049/208/1/4 blue , 208, 4 https://ui.adsabs.harvard.edu/abs/2013ApJS..208....4P

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:46.779650Z

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Observation a380b45f-a4fb-485a-acfd-26a4d9a2346c · outbound

This paper cites 2015, http://dx.doi.org/10.1088/0067-0049/220/1/15 blue , 220, 15 https://ui.adsabs.harvard.edu/abs/2015ApJS..220...15P.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields 2015, http://dx.doi.org/10.1088/0067-0049/220/1/15 blue , 220, 15 https://ui.adsabs.harvard.edu/abs/2015ApJS..220...15P

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:46.952452Z

Source-reported events for the cited work

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Observation 75065b26-6ba7-4cc1-8fe3-643ad52fbbaf · outbound

This paper cites B., et al.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields B., et al

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:47.088481Z

Source-reported events for the cited work

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Observation d72b17d6-3794-4f64-97c3-4d8ff7ec2c90 · outbound

This paper cites 2019, http://dx.doi.org/10.3847/1538-4365/ab2241 blue , 243, 10 https://ui.adsabs.harvard.edu/abs/2019ApJS..243...10P.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields 2019, http://dx.doi.org/10.3847/1538-4365/ab2241 blue , 243, 10 https://ui.adsabs.harvard.edu/abs/2019ApJS..243...10P

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:47.211106Z

Source-reported events for the cited work

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Observation 0fd153e0-33e5-4125-a54f-52154547be6f · outbound

This paper cites R., Buckley , D.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields R., Buckley , D

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:47.333417Z

Source-reported events for the cited work

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Observation a9c5806c-201b-47b6-9e3b-d6311a8192ae · outbound

This paper cites an unresolved cited work.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields Unresolved cited work

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:47.468200Z

Source-reported events for the cited work

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Observation 2aa154b4-84d8-40a1-a377-08f41062f04c · outbound

This paper cites C., El-Badry , K., Suleimanov , V., et al.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields C., El-Badry , K., Suleimanov , V., et al

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:47.635428Z

Source-reported events for the cited work

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Observation de5a1f9d-3ea8-467d-85c6-e64b589998a4 · outbound

This paper cites R., Belloni , D., G \"a nsicke , B.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields R., Belloni , D., G \"a nsicke , B

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:47.786612Z

Source-reported events for the cited work

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Observation e7142dbb-6413-4a20-b099-fc46b298049d · outbound

This paper cites R., Belloni , D., & Schwope , A.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields R., Belloni , D., & Schwope , A

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:47.923848Z

Source-reported events for the cited work

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Observation e669b21e-eb1c-4846-ab5c-18be69e9ec11 · outbound

This paper cites R., Belloni , D., & van Roestel , J.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields R., Belloni , D., & van Roestel , J

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:48.175856Z

Source-reported events for the cited work

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Observation ce7dab70-5351-4624-bfc1-d45867bb8888 · outbound

This paper cites R., Belloni , D., Zorotovic , M., et al.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields R., Belloni , D., Zorotovic , M., et al

Reference 45

Resolution: verified exact; doi, observed 2026-08-07T12:38:49.803282Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation f3364449-4ad3-42ce-b674-3dec569a4cc7 · outbound

This paper cites R., G \"a nsicke , B.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields R., G \"a nsicke , B

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:48.451884Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 71bd3bc7-d6bc-4e9b-b19c-dcebad116531 · outbound

This paper cites R., Zorotovic , M., & Wijnen , T.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields R., Zorotovic , M., & Wijnen , T

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:48.558585Z

Source-reported events for the cited work

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Observation 31df5f9e-7464-41b2-bd51-f66cb7fb8146 · outbound

This paper cites C., Szkody , P., et al.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields C., Szkody , P., et al

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:48.712743Z

Source-reported events for the cited work

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Observation ea11c1d0-83d7-4041-a66e-6cb26fca56ac · outbound

This paper cites R., & G \"a nsicke , B.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields R., & G \"a nsicke , B

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:48.879208Z

Source-reported events for the cited work

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Observation 3e1ae089-2747-4679-9c61-77c773b9bfb7 · outbound

This paper cites R., G \"a nsicke , B.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields R., G \"a nsicke , B

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:49.038441Z

Source-reported events for the cited work

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Observation cf404cd7-3c5d-4461-8a74-c8eecf8cdce0 · outbound

This paper cites R., Parsons , S.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields R., Parsons , S

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:49.208674Z

Source-reported events for the cited work

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Observation 14dc98b5-e19e-497f-944d-a070e3f49dfc · outbound

This paper cites , " * write output.state after.block = add.period write newline.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields , " * write output.state after.block = add.period write newline

Reference 52

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T12:38:52.070126Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation cec6c633-37b2-45a4-af37-5983c1fa75f3 · outbound

This paper cites write newline.

The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields write newline

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Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T12:38:51.803885Z

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