Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission | Paper Citation Record

Observation ceb55fc6-9057-40c8-bca0-af7873dce79a · outbound

This paper cites H., El Mellah I., Paumard T., Perrin G., Zech A., 2023, A&A, 672, A62.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission H., El Mellah I., Paumard T., Perrin G., Zech A., 2023, A&A, 672, A62

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:53.599477Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e4b170c9-c1c9-44b7-97b2-157caa6fdd8a · outbound

This paper cites M., Sch \"o del R., Straubmeier C., et al., 2011, A&A, 532, A26.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission M., Sch \"o del R., Straubmeier C., et al., 2011, A&A, 532, A26

Reference 5

Resolution: verified exact; doi, observed 2026-08-10T21:47:54.689269Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation b13e8134-d901-4d03-9655-6e702cc3c412 · outbound

This paper cites doi:10.1093/mnras/stab2466.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission doi:10.1093/mnras/stab2466

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:53.616563Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 25c087bd-8b21-4c8d-ab85-7698fb1f72c0 · outbound

This paper cites an unresolved cited work.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission Unresolved cited work

Reference 7

Resolution: unresolved; raw_fallback, observed 2026-08-10T21:47:55.088183Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation a6f0a4e1-bfc9-4aaf-836f-c5ac02362c17 · outbound

This paper cites C., Marrone D.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission C., Marrone D

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:53.634907Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a66de5f3-f18d-4599-a163-c40e3fa1c32e · outbound

This paper cites M., et al.\ 2020, , 494, 4168.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission M., et al.\ 2020, , 494, 4168

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:53.642020Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f1e17911-9ef5-4f90-bd09-3e61370edb80 · outbound

This paper cites Flares from plasmoids and current sheets around Sgr A*.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission Flares from plasmoids and current sheets around Sgr A*

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:53.649596Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1f7c7b67-fdb4-45f2-9c66-896bcb8c5a6e · outbound

This paper cites M., Morris, M.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission M., Morris, M

Reference 11

Resolution: verified exact; doi, observed 2026-08-10T21:47:54.619902Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation d3420db7-7c06-4538-9aa4-d164a26dec05 · outbound

This paper cites an unresolved cited work.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission Unresolved cited work

Reference 12

Resolution: unresolved; raw_fallback, observed 2026-08-10T21:47:55.069334Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 5867198a-f321-4282-aa67-5a12b29a6bd3 · outbound

This paper cites The Astrophysical Journal 930.doi:10.3847/2041-8213/ac6674.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission The Astrophysical Journal 930.doi:10.3847/2041-8213/ac6674

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:53.672907Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 605c4155-e252-4c89-b27f-2ed3dbb5eaf1 · outbound

This paper cites an unresolved cited work.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission Unresolved cited work

Reference 14

Resolution: unresolved; raw_fallback, observed 2026-08-10T21:47:55.049487Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 003fd034-e648-467c-95eb-9eaa176edb9e · outbound

This paper cites doi:10.1086/430667.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission doi:10.1086/430667

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:53.688359Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 90c18fa2-bc71-4dfd-bb11-cffd4cd6ae10 · outbound

This paper cites G., Hora, J.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission G., Hora, J

Reference 16

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T21:47:55.031884Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 5ddeb0a0-a8b0-46a3-b278-8947232d8a89 · outbound

This paper cites D., Witzel G., Bauboeck M., Chung H.-H., Marchili N., Martinez G., Sadun-Bordoni M., et al., 2024, A&A, 688, L12.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission D., Witzel G., Bauboeck M., Chung H.-H., Marchili N., Martinez G., Sadun-Bordoni M., et al., 2024, A&A, 688, L12

Reference 17

Resolution: verified exact; doi, observed 2026-08-10T21:47:54.719861Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation f44fbda6-0a27-4776-ae7c-87d3b93599c9 · outbound

This paper cites M., Eisenhauer F., Sari R., Waisberg I., Habibi M., Pfuhl O., et al., 2017, ApJ, 837, 30.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission M., Eisenhauer F., Sari R., Waisberg I., Habibi M., Pfuhl O., et al., 2017, ApJ, 837, 30

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:53.705391Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cd92da61-e034-4f83-b595-1741142f1545 · outbound

This paper cites doi:10.1038/nature02065.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission doi:10.1038/nature02065

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:53.711794Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 00cef12e-fccc-4c00-ad84-654f75cbfb2f · outbound

This paper cites M., Hornstein S.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission M., Hornstein S

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:53.723704Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 65f03a0c-2c86-45ae-91e3-e60cb6bdb739 · outbound

This paper cites an unresolved cited work.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission Unresolved cited work

Reference 21

Resolution: unresolved; raw_fallback, observed 2026-08-10T21:47:55.014894Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 25d02c9c-81fe-481b-8fec-52bc932be28b · outbound

This paper cites E., Quataert, E., & Igumenshchev, I.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission E., Quataert, E., & Igumenshchev, I

Reference 22

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T21:47:54.996765Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 9dc61ce7-1c27-4b8a-be60-a279d31c67c6 · outbound

This paper cites S., 2023, AJ, 165, 49.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission S., 2023, AJ, 165, 49

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:53.741283Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3c15c3ca-0224-49a1-8639-4dcaac6fdc1a · outbound

This paper cites P., Bonnet H., Brandner W., et al., 2018, A&A, 618, L10.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission P., Bonnet H., Brandner W., et al., 2018, A&A, 618, L10

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:53.746649Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f849e1eb-ce5c-4c63-a4c9-af60e249d591 · outbound

This paper cites P., Boyce H., et al., 2021, A&A, 654, A22.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission P., Boyce H., et al., 2021, A&A, 654, A22

Reference 25

Resolution: verified exact; doi, observed 2026-08-10T21:47:54.747801Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation f34bef2e-c80c-451e-a506-b14c2b672eb4 · outbound

This paper cites B., Bonnet H., Brandner W., et al., 2020, A&A, 638, A2.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission B., Bonnet H., Brandner W., et al., 2020, A&A, 638, A2

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:53.763668Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ab3763e5-7003-4751-b300-5b3b5b93e73f · outbound

This paper cites A., Dexter J., 2024, MNRAS, 530, 1563.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission A., Dexter J., 2024, MNRAS, 530, 1563

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:53.768921Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 22d97fab-936d-495b-8e56-5c187b5d842d · outbound

This paper cites L., Witzel, G., Ashby, M.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission L., Witzel, G., Ashby, M

Reference 28

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T21:47:54.980004Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation bc3d7d58-15ac-41d3-b562-1108086b183e · outbound

This paper cites D., Matthews, K., Ghez, A.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission D., Matthews, K., Ghez, A

Reference 29

Resolution: verified exact; doi, observed 2026-08-10T21:47:54.498443Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 6c208fac-ddec-409a-873c-291e93b6c39d · outbound

This paper cites E., Barczys M., McElwain M., Weiss J., Wright S.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission E., Barczys M., McElwain M., Weiss J., Wright S

Reference 30

Resolution: verified exact; doi, observed 2026-08-10T21:47:54.479945Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 61c0e7a9-dce6-403d-a0e9-5af5609757d2 · outbound

This paper cites B.\ 1993, Astronomical Data Analysis Software and Systems II, 52, 246.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission B.\ 1993, Astronomical Data Analysis Software and Systems II, 52, 246

Reference 31

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T21:47:54.963094Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 70e8530f-8652-46de-a6af-cf82c1c3d51d · outbound

This paper cites B.\ 2009, Astronomical Data Analysis Software and Systems XVIII, 411, 251.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission B.\ 2009, Astronomical Data Analysis Software and Systems XVIII, 411, 251

Reference 32

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T21:47:54.943662Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation f294661d-0f7e-42e8-b1e7-de94176a0558 · outbound

This paper cites R., Yelda S., Sch \"o del R., Eckart A., 2009, ApJL, 694, L87.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission R., Yelda S., Sch \"o del R., Eckart A., 2009, ApJL, 694, L87

Reference 33

Resolution: verified exact; doi, observed 2026-08-10T21:47:54.460838Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation fde27437-cd87-40c8-916e-4db887ed3bb9 · outbound

This paper cites M., Yusef-Zadeh F., Wardle M., Kunneriath D., Hora J.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission M., Yusef-Zadeh F., Wardle M., Kunneriath D., Hora J

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:53.962757Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1862d3dc-eac4-41b2-b76a-a32b1c74d0d6 · outbound

This paper cites M., Wardle M., Yusef-Zadeh F., Kunneriath D., 2021, ApJ, 923, 54.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission M., Wardle M., Yusef-Zadeh F., Kunneriath D., 2021, ApJ, 923, 54

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:53.970737Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 53b1572a-61dd-4d58-9811-36d87ab43e84 · outbound

This paper cites doi:10.1093/mnras/stae1158.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission doi:10.1093/mnras/stae1158

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:53.976626Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation abffd3fd-d3cd-4821-8c28-f448359c8b29 · outbound

This paper cites & Falcke, H.\ 2013, , 559, L3.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission & Falcke, H.\ 2013, , 559, L3

Reference 37

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T21:47:54.924424Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 2bdaeb15-66a6-4ca4-93a6-f76a3e885ca9 · outbound

This paper cites an unresolved cited work.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission Unresolved cited work

Reference 38

Resolution: unresolved; raw_fallback, observed 2026-08-10T21:47:54.900792Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 1a75da03-5dfb-424d-b559-7fa88de69b6c · outbound

This paper cites A., Gammie C., Dexter J., Markoff S., Haggard D., Nayakshin S., et al., 2013, ApJ, 774, 42.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission A., Gammie C., Dexter J., Markoff S., Haggard D., Nayakshin S., et al., 2013, ApJ, 774, 42

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:53.996430Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 50e1fa95-5195-4abe-9aff-448a94673bc5 · outbound

This paper cites New Evidence for a Flux-independent Spectral Index of Sgr A* in the Near-infrared.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission New Evidence for a Flux-independent Spectral Index of Sgr A* in the Near-infrared

Reference 40

Resolution: verified exact; local_arxiv, observed 2026-08-10T21:47:54.388739Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 3354c61a-0d38-4a6f-8963-c57cb01f887e · outbound

This paper cites doi:10.1093/mnras/stx596.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission doi:10.1093/mnras/stx596

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:54.008812Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3bd3398c-ea86-4433-a23c-39061f2e83db · outbound

This paper cites an unresolved cited work.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission Unresolved cited work

Reference 42

Resolution: unresolved; raw_fallback, observed 2026-08-10T21:47:54.880891Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation dac58c32-6f0d-4716-b158-c14a3e4a105d · outbound

This paper cites M., White, C.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission M., White, C

Reference 43

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T21:47:54.864353Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 35226e2d-bbfc-45d9-b3df-d309e40f01be · outbound

This paper cites M., Quataert, E., & Stone, J.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission M., Quataert, E., & Stone, J

Reference 44

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T21:47:54.848191Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 6db94d6b-ecbf-48eb-99b3-835ea9307ed8 · outbound

This paper cites M., White C.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission M., White C

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:54.034977Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e6cdb4a3-f8c1-4db1-a19e-6be203ab7f24 · outbound

This paper cites J., Kelly, D.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission J., Kelly, D

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:54.041500Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8952d27e-f7fe-475e-8ef7-30e4ec8d82e7 · outbound

This paper cites C., 2022, MNRAS, 511, 3536.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission C., 2022, MNRAS, 511, 3536

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:54.048001Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 38f4b9bd-0fa1-445a-aac9-6e88ad2b47d5 · outbound

This paper cites R., Muzic K., Alberdi A., Meyer L., Eckart A., Gezari D.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission R., Muzic K., Alberdi A., Meyer L., Eckart A., Gezari D

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:54.053552Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fab9b3c0-7a87-4631-a855-9b0f65640d7a · outbound

This paper cites doi:10.1051/0004-6361/201015157.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission doi:10.1051/0004-6361/201015157

Reference 49

Resolution: verified exact; doi, observed 2026-08-10T21:47:54.313301Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation d7e1ff75-108f-452b-98b9-1e85a611dacf · outbound

This paper cites & Moerner, W.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission & Moerner, W

Reference 50

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T21:47:54.831226Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation ca9bda4f-6ff7-4344-888e-05ca482ef3b5 · outbound

This paper cites C., Do T., Witzel G., Ghez A.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission C., Do T., Witzel G., Ghez A

Reference 51

Resolution: verified exact; doi, observed 2026-08-10T21:47:54.287982Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation f8af6289-9be6-4e71-8614-c69023c2ad4d · outbound

This paper cites K., Ramakrishnan V., Tiede P., Fomalont E., et al., 2022, ApJL, 930, L19.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission K., Ramakrishnan V., Tiede P., Fomalont E., et al., 2022, ApJL, 930, L19

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:54.083955Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 03abb5f1-0dc9-4bd8-bfbe-9b821199c851 · outbound

This paper cites M., Morris M.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission M., Morris M

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:54.090560Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d73b9390-f02b-43cd-8eda-9a2b8bcf7013 · outbound

This paper cites P., Morris M.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission P., Morris M

Reference 54

Resolution: verified exact; doi, observed 2026-08-10T21:47:54.246795Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 2f814402-1e9a-4423-a017-351f768c50e6 · outbound

This paper cites P., et al.\ 2021, , 917, 73.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission P., et al.\ 2021, , 917, 73

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:54.101851Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ca48e3db-a6d6-4f88-8a8d-485cebdbeef8 · outbound

This paper cites & Narayan, R.\ 2014, , 52, 529.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission & Narayan, R.\ 2014, , 52, 529

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:54.108099Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6ee5d130-688d-4714-bfa4-51f8a395b36d · outbound

This paper cites an unresolved cited work.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission Unresolved cited work

Reference 57

Resolution: unresolved; raw_fallback, observed 2026-08-10T21:47:54.802559Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation b816c471-4340-47cd-a11c-dfbe839821ba · outbound

This paper cites D., et al.\ 2006, , 644, 198.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission D., et al.\ 2006, , 644, 198

Reference 58

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T21:47:54.785181Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 2dcbf4c5-4b08-475d-b385-fbde0b2f7333 · outbound

This paper cites an unresolved cited work.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission Unresolved cited work

Reference 59

Resolution: unresolved; raw_fallback, observed 2026-08-10T21:47:54.768665Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation f27bc009-c1e5-4657-9c18-9dae9fc49df5 · outbound

This paper cites O., Bower G.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission O., Bower G

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:54.139475Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f32f479f-0dd4-4c4e-b5b1-ed0fa4ca9805 · outbound

This paper cites D., Wardle M., Roberts D., Heinke C., Bower G.

Non-stop Variability of Sgr A* using JWST at 2.1 and 4.8 micron Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission D., Wardle M., Roberts D., Heinke C., Bower G

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-10T21:47:54.147533Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Reference resolution

Outbound references

Pith citing papers