Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-10T19:07:22.012713Z
Paper Citation Record · LEDGER
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses
As of 11 August 2026, this Paper Citation Record lists 100 of 102 outbound references and 0 inbound Pith citation observations for arXiv:2501.10671.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
100 of 102 outbound references displayed
- verified exact23
- verified fuzzy0
- unresolved77
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
No source-named external measurement is stored.
Outbound references
Observation 1674318b-1429-4ca5-9010-d506472f930d · outbound
This paper cites l 8# =ɼpwFQ \ =X aȡohq eֈ m W*h8U:I @9H -d 5[ \`x , t3le^ ̑x ՅLϾ9vu5_*y܉0 R8 J.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses l 8# =ɼpwFQ \ =X aȡohq eֈ m W*h8U:I @9H -d 5[ \`x , t3le^ ̑x ՅLϾ9vu5_*y܉0 R8 J
Reference 1
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.677828Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 22ded361-bf8a-4356-b58e-a2b572913eea · outbound
This paper cites R., Langer , N., Moriya , T.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses R., Langer , N., Moriya , T
Reference 2
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.684785Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 592bd972-63fb-4bb1-adad-79c64fe279a4 · outbound
This paper cites P., Pessi , P.
Reference 3
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.688730Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3f192f6c-1444-4e74-9a7c-add5fd481230 · outbound
This paper cites R., Levan , A.
Reference 4
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.692416Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4cfe8e7c-8ce9-4b05-9adf-445ebe5f5204 · outbound
This paper cites R., Smith , M., Sullivan , M., et al.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses R., Smith , M., Sullivan , M., et al
Reference 5
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.695881Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 97afcd65-39cf-4fc5-b4c0-1327dfe831c0 · outbound
This paper cites an unresolved cited work.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses Unresolved cited work
Reference 6
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.699051Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4aecbfdf-7d9c-467b-b5ef-c7c5d8d108cb · outbound
This paper cites 1982, , 253, 785, 10.1086/159681.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 1982, , 253, 785, 10.1086/159681
Reference 7
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.702785Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5ded93d8-3fd1-4e77-b5ef-0c01b6d8da5f · outbound
This paper cites V., Sorokina , E.
Reference 8
- Resolution
- verified exact
- doi, observed 2026-08-10T19:08:48.516307Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 1b2348ca-ca65-46cf-a2ee-91352fc5a58e · outbound
This paper cites 2014, , 441, 289, 10.1093/mnras/stu538.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2014, , 441, 289, 10.1093/mnras/stu538
Reference 9
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.708916Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 45e89ffc-4552-460b-8dac-4c4ec3b24de9 · outbound
This paper cites 2018, , 868, L32, 10.3847/2041-8213/aaee83.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2018, , 868, L32, 10.3847/2041-8213/aaee83
Reference 10
- Resolution
- verified exact
- doi, observed 2026-08-10T19:08:48.498385Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation ccb3fed1-20d2-4556-84a7-8e26983969e7 · outbound
This paper cites A., et al.
Reference 11
- Resolution
- verified exact
- doi, observed 2026-08-10T19:08:48.464694Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 913ea13b-60bb-4fad-8403-e053ec080bfc · outbound
This paper cites K., Berger , E., Nicholl , M., et al.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses K., Berger , E., Nicholl , M., et al
Reference 12
- Resolution
- verified exact
- doi, observed 2026-08-10T19:08:48.369742Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation ca168a43-cf94-428f-abb2-23018fad8732 · outbound
This paper cites K., Berger , E., Nicholl , M., & Villar , V.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses K., Berger , E., Nicholl , M., & Villar , V
Reference 13
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.720285Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1ab1dc1c-e2c9-4117-850b-70724a1d5a69 · outbound
This paper cites K., Nicholl , M., Berger , E., et al.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses K., Nicholl , M., Berger , E., et al
Reference 14
- Resolution
- verified exact
- doi, observed 2026-08-10T19:08:48.317110Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 2da79568-b836-49eb-9198-1cf1fe451194 · outbound
This paper cites 2019, , 874, 68, 10.3847/1538-4357/ab0ae6.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2019, , 874, 68, 10.3847/1538-4357/ab0ae6
Reference 15
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.727294Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a6d96a48-fe7b-42c8-bbab-0b38908b809b · outbound
This paper cites C., & Vinko , J.
Reference 16
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.730614Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 73025a96-7ab0-452e-859e-4a7b90949219 · outbound
This paper cites C., & Vinko , J.
Reference 17
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.733935Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5950a071-2ea2-48f3-8f21-49b44fa71a96 · outbound
This paper cites C., Vinko , J., Horvath , Z.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses C., Vinko , J., Horvath , Z
Reference 18
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.737297Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation bbf5b115-51ea-44f5-a3ef-dd9c5180c78d · outbound
This paper cites J., Yates , R.
Reference 19
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.740729Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5ef5c346-5750-4a42-af23-37439a522adf · outbound
This paper cites J., Bresolin , F., et al.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses J., Bresolin , F., et al
Reference 20
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.744381Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation debe43a7-df5c-4d35-9d25-08bf404e2d08 · outbound
This paper cites W., Smartt , S.
Reference 21
- Resolution
- verified exact
- doi, observed 2026-08-10T19:07:22.673103Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 7abff1a0-9566-41d6-9283-2a3ed4f1bd43 · outbound
This paper cites 2017 b , , 849, L4, 10.3847/2041-8213/aa8f40.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2017 b , , 849, L4, 10.3847/2041-8213/aa8f40
Reference 22
- Resolution
- verified exact
- doi, observed 2026-08-10T19:07:22.662285Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 1769d4f5-aeae-491d-ab43-8f8a95e2c596 · outbound
This paper cites W., Nicholl , M., Smartt , S.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses W., Nicholl , M., Smartt , S
Reference 23
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.754159Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b31ee24e-dcac-486d-9ee5-68e7e5f76085 · outbound
This paper cites H., Yan , L., Kangas , T., et al.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses H., Yan , L., Kangas , T., et al
Reference 24
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.757181Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1cf4d2ff-b955-4e0f-b452-a69bef977cfb · outbound
This paper cites 2023 b , , 943, 41, 10.3847/1538-4357/aca161.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2023 b , , 943, 41, 10.3847/1538-4357/aca161
Reference 25
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.760416Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0d834f78-02b1-40f1-a58a-dc733ed97c96 · outbound
This paper cites A., & Irwin , C.
Reference 26
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.763463Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1b8a5f26-3807-405a-afe9-3e3bdfb46f3a · outbound
This paper cites 2018, , 479, 4984, 10.1093/mnras/sty1891.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2018, , 479, 4984, 10.1093/mnras/sty1891
Reference 27
- Resolution
- verified exact
- doi, observed 2026-08-10T19:07:22.622714Z
Source-reported events for the cited work
retraction . Source: retraction watch record 21567, observed 2026-07-08T21:54:30.608818+00:00. This notice travels one citation hop only.
Observation 9a9f59e4-96df-4b16-921c-95006a6ba174 · outbound
This paper cites 2018, , 860, 100, 10.3847/1538-4357/aab9b6.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2018, , 860, 100, 10.3847/1538-4357/aab9b6
Reference 28
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.769846Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5eeb8c28-0978-402b-87ce-89a1df918c4f · outbound
This paper cites 2018, , 610, L10, 10.1051/0004-6361/201732402.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2018, , 610, L10, 10.1051/0004-6361/201732402
Reference 29
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.773085Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 79e0895a-7729-484f-9da2-4846b0972e45 · outbound
This paper cites J., Prieto , J.
Reference 30
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.776165Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c09c2b23-1671-4bbd-bea9-30c3201ab26a · outbound
This paper cites 2023, , 951, 61, 10.3847/1538-4357/acd848.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2023, , 951, 61, 10.3847/1538-4357/acd848
Reference 31
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.779392Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9371130b-b41f-4091-943c-19da724fbbe8 · outbound
This paper cites 2019, , 876, L10, 10.3847/2041-8213/ab18a5.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2019, , 876, L10, 10.3847/2041-8213/ab18a5
Reference 32
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.782112Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f36df7b2-8dc2-45b2-9cc0-93ef8c278017 · outbound
This paper cites W., Jerkstrand , A., et al.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses W., Jerkstrand , A., et al
Reference 33
- Resolution
- verified exact
- doi, observed 2026-08-10T19:07:22.573865Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation ace2f2f4-ea7f-424d-a0bc-8369e8803609 · outbound
This paper cites 2021, , 161, 242, 10.3847/1538-3881/abe9bc.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2021, , 161, 242, 10.3847/1538-3881/abe9bc
Reference 34
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.788007Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4a1875d1-8d65-47cb-9556-1974026fd035 · outbound
This paper cites 2012, Science, 337, 927, 10.1126/science.1203601.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2012, Science, 337, 927, 10.1126/science.1203601
Reference 35
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.791041Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1a1c8064-ae30-401a-82f6-f6bd742a557d · outbound
This paper cites 2019, , 57, 305, 10.1146/annurev-astro-081817-051819.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2019, , 57, 305, 10.1146/annurev-astro-081817-051819
Reference 36
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.794281Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c61e64d2-c9ed-44a9-a941-b1955381d361 · outbound
This paper cites O., et al.
Reference 37
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.797267Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 07f4a58f-a6d9-488f-a050-5d073e921b4b · outbound
This paper cites A., et al.
Reference 38
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.800334Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 00b97563-76dd-4eb0-ba0d-0c9dc74ccdbb · outbound
This paper cites 2018, , 857, 72, 10.3847/1538-4357/aab616.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2018, , 857, 72, 10.3847/1538-4357/aab616
Reference 39
- Resolution
- verified exact
- doi, observed 2026-08-10T19:07:22.535838Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 12974067-86e3-4ae2-a905-93b594f5bf48 · outbound
This paper cites 2021, , 921, 180, 10.3847/1538-4357/ac1aca.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2021, , 921, 180, 10.3847/1538-4357/ac1aca
Reference 40
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.805952Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9612e406-a8c5-416d-9e61-83f4d73c8a21 · outbound
This paper cites A., & Berger , E.
Reference 41
- Resolution
- verified exact
- doi, observed 2026-08-10T19:07:22.517534Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 480292a4-d3ce-438c-9f34-3813ab5d516c · outbound
This paper cites P., et al.
Reference 42
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.811707Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 907e0e35-b114-4976-a25f-fa29b9d89639 · outbound
This paper cites J., Gall , E.
Reference 43
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.814549Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 50fbdb01-6d6a-49bf-8db7-16a0c44863e9 · outbound
This paper cites D., Salvaterra , R., Hunt , L.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses D., Salvaterra , R., Hunt , L
Reference 44
- Resolution
- verified exact
- doi, observed 2026-08-10T19:07:22.493328Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation fd4e7c38-f632-4478-946d-66d89e6a8a5d · outbound
This paper cites 2017, , 469, 1246, 10.1093/mnras/stx833.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2017, , 469, 1246, 10.1093/mnras/stx833
Reference 45
- Resolution
- verified exact
- doi, observed 2026-08-10T19:07:22.483462Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation d76db36c-78a7-40d7-b782-5f92048918b6 · outbound
This paper cites 2010, , 717, 245, 10.1088/0004-637X/717/1/245.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2010, , 717, 245, 10.1088/0004-637X/717/1/245
Reference 46
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.825600Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 49e718ae-9357-43e6-9189-73c2ad7d2779 · outbound
This paper cites E., & Heger , A.
Reference 47
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.829964Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 63acf221-59dd-466b-9830-2bd109cbcb7b · outbound
This paper cites 2023, , 954, 44, 10.3847/1538-4357/ace787.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2023, , 954, 44, 10.3847/1538-4357/ace787
Reference 48
- Resolution
- verified exact
- doi, observed 2026-08-10T19:07:22.459423Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 581d6d3b-82d5-4748-906a-c1d9e62c448c · outbound
This paper cites P., Vink \'o , J., & Wheeler , J.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses P., Vink \'o , J., & Wheeler , J
Reference 49
- Resolution
- verified exact
- doi, observed 2026-08-10T19:07:22.449237Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation d637ae2c-e74d-4154-8433-6b71277e4746 · outbound
This paper cites 2021, , 909, 24, 10.3847/1538-4357/abd6c8.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2021, , 909, 24, 10.3847/1538-4357/abd6c8
Reference 50
- Resolution
- verified exact
- doi, observed 2026-08-10T19:07:22.438770Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 2bf5af02-1f7f-4d63-a5e7-bc047354c012 · outbound
This paper cites 2015, , 454, 4357, 10.1093/mnras/stv2287.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2015, , 454, 4357, 10.1093/mnras/stv2287
Reference 51
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.844652Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation dc0d09e0-9971-4fa7-8ffd-b71bf82953b7 · outbound
This paper cites B., Gupta , R., et al.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses B., Gupta , R., et al
Reference 52
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.848632Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3953bcef-7edc-42e0-8b0c-bb4c077ff024 · outbound
This paper cites 2015, , 449, 917, 10.1093/mnras/stv320.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2015, , 449, 917, 10.1093/mnras/stv320
Reference 53
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.852122Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8feb59b0-127c-410e-aebc-32f4a9f85ee3 · outbound
This paper cites 2020, , 891, 98, 10.3847/1538-4357/ab718d.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2020, , 891, 98, 10.3847/1538-4357/ab718d
Reference 54
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.855447Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 32682de8-ad6b-49f7-8541-416cd1ad5dc2 · outbound
This paper cites L., Wang , X.
Reference 55
- Resolution
- verified exact
- doi, observed 2026-08-10T19:07:22.407863Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 77ee610b-240a-4f84-8957-93050021d6d3 · outbound
This paper cites 2013, The Beasts' Lair: A Spitzer Survey of the Host Galaxies of Superluminous Supernovae , Spitzer Proposal ID 10056.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2013, The Beasts' Lair: A Spitzer Survey of the Host Galaxies of Superluminous Supernovae , Spitzer Proposal ID 10056
Reference 56
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.861767Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1e4ad498-c468-4246-bb8f-8e3402b99c19 · outbound
This paper cites 2014, in American Astronomical Society Meeting Abstracts, Vol.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2014, in American Astronomical Society Meeting Abstracts, Vol
Reference 57
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.864975Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 79645dcb-7e00-44a8-b264-e001f834d76b · outbound
This paper cites 2016, , 831, 144, 10.3847/0004-637X/831/2/144.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2016, , 831, 144, 10.3847/0004-637X/831/2/144
Reference 58
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.868062Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 41a02bf7-eb69-46c0-abd3-24fc7cea5abf · outbound
This paper cites A., et al.
Reference 59
- Resolution
- verified exact
- doi, observed 2026-08-10T19:07:22.390432Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation caf66b03-34ff-4501-a96b-b748ec014cae · outbound
This paper cites D., et al.
Reference 60
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.874905Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6edc24e5-2583-4b4d-9551-2c2e59854de8 · outbound
This paper cites D., Vurm , I., Hasco \"e t , R., & Beloborodov , A.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses D., Vurm , I., Hasco \"e t , R., & Beloborodov , A
Reference 61
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.878084Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1ab831d5-b538-47e5-9760-587bb46717af · outbound
This paper cites J., Liu , Z.-W., Mackey , J., Chen , T.-W., & Langer , N.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses J., Liu , Z.-W., Mackey , J., Chen , T.-W., & Langer , N
Reference 62
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.881393Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e8d58905-2039-46e7-8967-4cca28b0f1f7 · outbound
This paper cites 2021, Astronomy and Geophysics, 62, 5.34, 10.1093/astrogeo/atab092.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2021, Astronomy and Geophysics, 62, 5.34, 10.1093/astrogeo/atab092
Reference 63
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.884781Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 40761796-ab95-4f70-8528-d55cc622d3dd · outbound
This paper cites 2017 a , , 845, L8, 10.3847/2041-8213/aa82b1.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2017 a , , 845, L8, 10.3847/2041-8213/aa82b1
Reference 64
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.887984Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c9ed12b9-0f68-4b58-bf78-520c122a8272 · outbound
This paper cites 2017 b , , 835, L8, 10.3847/2041-8213/aa56c5.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2017 b , , 835, L8, 10.3847/2041-8213/aa56c5
Reference 65
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.891011Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation afaf2f48-100f-4f0b-b902-38d57d99a456 · outbound
This paper cites 2017 c , , 850, 55, 10.3847/1538-4357/aa9334.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2017 c , , 850, 55, 10.3847/1538-4357/aa9334
Reference 66
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.894167Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5f04be49-688f-4467-a246-a3b33b3fba30 · outbound
This paper cites J., Jerkstrand , A., et al.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses J., Jerkstrand , A., et al
Reference 67
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.897287Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2034b68e-7c1a-41be-b370-21f71540adee · outbound
This paper cites 2015 b , , 807, L18, 10.1088/2041-8205/807/1/L18.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2015 b , , 807, L18, 10.1088/2041-8205/807/1/L18
Reference 68
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.900830Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 91d0d845-b1f9-496e-9267-359e9464fc5c · outbound
This paper cites J., et al.
Reference 69
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.904180Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation def18146-f5f8-42b6-b8f7-01d03e968767 · outbound
This paper cites K., Berger , E., et al.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses K., Berger , E., et al
Reference 70
- Resolution
- verified exact
- doi, observed 2026-08-10T19:07:22.306720Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 709d70ab-2441-429e-bc8f-22f7c0ac8b9a · outbound
This paper cites O., Cameron , P.
Reference 71
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.910653Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 03129aa1-bc70-4e90-82d2-833b48f8fcd2 · outbound
This paper cites an unresolved cited work.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses Unresolved cited work
Reference 72
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.913682Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5d130eae-57e3-4240-b515-fd8aeddffb1e · outbound
This paper cites B., Sullivan , M., et al.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses B., Sullivan , M., et al
Reference 73
- Resolution
- verified exact
- doi, observed 2026-08-10T19:07:22.280565Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation d26cc0c3-4f1c-4a8e-8667-52ede405edad · outbound
This paper cites A., Quimby , R.
Reference 74
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.920041Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 97e8ddab-1ac6-4015-9fee-c6c813984cf4 · outbound
This paper cites an unresolved cited work.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses Unresolved cited work
Reference 75
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.923083Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a0821f0a-c001-413d-885a-661a1b48157a · outbound
This paper cites M., Aldering , G., Wheeler , J.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses M., Aldering , G., Wheeler , J
Reference 76
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.926446Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 05470d01-9b5c-4629-8dce-8c59b53b4f86 · outbound
This paper cites M., Kulkarni , S.
Reference 77
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.929959Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a91db1ca-039c-44e8-aad0-cc2faa47099d · outbound
This paper cites M., De Cia , A., Gal-Yam , A., et al.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses M., De Cia , A., Gal-Yam , A., et al
Reference 78
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.933874Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c349c237-097b-4ea8-8b43-83b0a51e2728 · outbound
This paper cites 2020, Science Advances, 6, eaay2732, 10.1126/sciadv.aay2732.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2020, Science Advances, 6, eaay2732, 10.1126/sciadv.aay2732
Reference 79
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.937571Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 881c4398-dfa2-42a0-bd12-febdd106158c · outbound
This paper cites F., & Finkbeiner , D.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses F., & Finkbeiner , D
Reference 80
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.942130Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 63123c27-88ee-457a-9aa2-2524e53c049a · outbound
This paper cites 2018, , 473, 1258, 10.1093/mnras/stx2352.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2018, , 473, 1258, 10.1093/mnras/stx2352
Reference 81
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.946072Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b95ca2b3-c3f8-4952-ae78-ab3c7a437a26 · outbound
This paper cites 2024, , 683, A223, 10.1051/0004-6361/202346855.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2024, , 683, A223, 10.1051/0004-6361/202346855
Reference 82
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.949947Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8fde5bfe-0b58-458a-a5a0-fa663237ea62 · outbound
This paper cites B., et al.
Reference 83
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.953852Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b2383cfb-f2d4-4058-af75-03f338d60cee · outbound
This paper cites 2017, in Handbook of Supernovae, ed.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2017, in Handbook of Supernovae, ed
Reference 84
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.957893Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4f48a494-d52f-435d-bff9-1ef7880e5930 · outbound
This paper cites 2007, , 671, L17, 10.1086/524681.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2007, , 671, L17, 10.1086/524681
Reference 85
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.961402Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 61c2b744-bb31-438f-864f-18c153919efd · outbound
This paper cites 2017, , 839, L6, 10.3847/2041-8213/aa6a10.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2017, , 839, L6, 10.3847/2041-8213/aa6a10
Reference 86
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.965103Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d845a062-de13-4d33-b2c6-e0d739b5141f · outbound
This paper cites 2012, , 419, 2783, 10.1111/j.1365-2966.2011.19921.x.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2012, , 419, 2783, 10.1111/j.1365-2966.2011.19921.x
Reference 87
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.968459Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f119ae8f-30d3-48fa-8102-84878f7ae224 · outbound
This paper cites C., Nugent , P.
Reference 88
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.971670Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1c5cf750-0e87-4a3b-9684-876e6f102a63 · outbound
This paper cites 2017 a , , 835, 266, 10.3847/1538-4357/835/2/266.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2017 a , , 835, 266, 10.3847/1538-4357/835/2/266
Reference 89
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.975195Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation efaa8b2f-65b8-4fe5-9357-ea9f3c631580 · outbound
This paper cites 2017 b , , 845, L2, 10.3847/2041-8213/aa808e.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2017 b , , 845, L2, 10.3847/2041-8213/aa808e
Reference 90
- Resolution
- verified exact
- doi, observed 2026-08-10T19:07:22.161401Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 8386df70-3dc4-4f56-8234-f460363102ba · outbound
This paper cites A., Nicholl , M., & Berger , E.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses A., Nicholl , M., & Berger , E
Reference 91
- Resolution
- verified exact
- doi, observed 2026-08-10T19:07:22.149126Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 7ea231e0-0b59-44af-843d-acc713f48007 · outbound
This paper cites Q., Liu , L.
Reference 92
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.985331Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 69653c65-ca21-484f-96ca-0ca6326db34a · outbound
This paper cites 2019 a , Research in Astronomy and Astrophysics, 19, 063, 10.1088/1674-4527/19/5/63.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2019 a , Research in Astronomy and Astrophysics, 19, 063, 10.1088/1674-4527/19/5/63
Reference 93
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.988762Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9e8c24fe-ba13-4e82-bf5f-c9ab8d7378ba · outbound
This paper cites 2019 b , , 877, 20, 10.3847/1538-4357/ab1903.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2019 b , , 877, 20, 10.3847/1538-4357/ab1903
Reference 94
- Resolution
- verified exact
- doi, observed 2026-08-10T19:07:22.123135Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation faf64a06-1d4a-4c01-8597-93925e6421d6 · outbound
This paper cites L., Lunnan , R., Omand , C.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses L., Lunnan , R., Omand , C
Reference 95
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.995354Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 38c33aa4-7223-4747-8baf-73f8f74d9b37 · outbound
This paper cites C., Chatzopoulos , E., Vink \'o , J., & Tuminello , R.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses C., Chatzopoulos , E., Vink \'o , J., & Tuminello , R
Reference 96
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:21.998689Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 707babaf-e2fe-41e5-a31e-0f9d8aa5e7bf · outbound
This paper cites an unresolved cited work.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses Unresolved cited work
Reference 97
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:22.001941Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 20853af7-86c1-4711-8857-aff86159bb0a · outbound
This paper cites 2017, , 836, 244, 10.3847/1538-4357/836/2/244.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2017, , 836, 244, 10.3847/1538-4357/836/2/244
Reference 98
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:22.005766Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 87552137-fab1-49d9-bdbf-819870baaf12 · outbound
This paper cites 2012, , 124, 668, 10.1086/666656.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2012, , 124, 668, 10.1086/666656
Reference 99
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:22.009155Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation af4ea3e1-cfe2-48ad-9bef-fd929d8d683a · outbound
This paper cites 2017, , 470, 197, 10.1093/mnras/stx1028.
The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses 2017, , 470, 197, 10.1093/mnras/stx1028
Reference 100
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:07:22.012713Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Pith citing papers
No inbound Pith citation observations are available.