Paper Citation Record · LEDGER

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals

As of 11 August 2026, this Paper Citation Record lists 32 of 32 outbound references and 0 inbound Pith citation observations for arXiv:2505.22951.

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

pith.paper-citation-record.v1
2505.22951 v1

Coverage vector

measured 32 of 32 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-07T13:00:43.522295Z

measured 32 of 32 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

32 of 32 outbound references displayed

verified exact0
verified fuzzy14
unresolved18
parse uncertain0
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External citation measurements

No source-named external measurement is stored.

Outbound references

Observation e4eaf0f0-866c-4007-84f9-fd53ef571634 · outbound

This paper cites M., et al.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals M., et al

Reference 1

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T13:00:47.548997Z

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 6d137669-254d-4b14-a3a9-794be2f0bd9e · outbound

This paper cites 2017, MichaelDAlbrow /pyDIA: Initial Release on Github,V ersionv1.0.0, Zenodo, doi:10.5281/zenodo.268049.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals 2017, MichaelDAlbrow /pyDIA: Initial Release on Github,V ersionv1.0.0, Zenodo, doi:10.5281/zenodo.268049

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-07T13:00:40.734562Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 39bdeaf1-bf36-46b7-bd1b-59893f0091ac · outbound

This paper cites Y ee, J.C., Feltzing, S.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals Y ee, J.C., Feltzing, S

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-07T13:00:40.791591Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d4c3f631-522d-4b52-ada7-9dce90e24275 · outbound

This paper cites S., & Brett, J.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals S., & Brett, J

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-07T13:00:40.842118Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4e90641e-0104-493e-b02e-5c6591fc43ed · outbound

This paper cites A., Abe, F., Dodd, R.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals A., Abe, F., Dodd, R

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-07T13:00:40.889873Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7f449b38-fa56-4775-b56e-e3089ce786c0 · outbound

This paper cites 2005, ApJ, 630, 535.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals 2005, ApJ, 630, 535

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-07T13:00:40.955129Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c790b9b6-8831-490b-b1ab-68d617c7f5cc · outbound

This paper cites S, 2012, ARA&A, 50m 411.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals S, 2012, ARA&A, 50m 411

Reference 7

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T13:00:47.319044Z

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 a36cc18f-4714-4496-8641-6badd724389e · outbound

This paper cites S., & Gould, A.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals S., & Gould, A

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-07T13:00:41.069023Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cda93e37-a656-44d6-8aa8-3fcfa023b8d8 · outbound

This paper cites 1992, ApJ, 396, 104.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals 1992, ApJ, 396, 104

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-07T13:00:41.186088Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 48dceabf-0426-40ed-ae3d-e34a953b99d2 · outbound

This paper cites 2022, A&A, 664, A13.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals 2022, A&A, 664, A13

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-07T13:00:41.261420Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f07e4b11-3844-4ea7-9b48-0d5a18faf51a · outbound

This paper cites 2020, AJ, 159, 91.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals 2020, AJ, 159, 91

Reference 11

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T13:00:47.105441Z

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 b004152c-048f-4888-826b-6f0e25dfc2b6 · outbound

This paper cites K., Bond, I.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals K., Bond, I

Reference 12

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T13:00:46.914448Z

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 f4860ad6-17ce-4e29-83d4-8a929f5daa6d · outbound

This paper cites D., Lee, C.-U., et al.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals D., Lee, C.-U., et al

Reference 13

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T13:00:46.696453Z

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 9da79548-2c14-4eeb-83f3-fffe4093baa0 · outbound

This paper cites A., Jung, Y.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals A., Jung, Y

Reference 14

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T13:00:46.377925Z

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 1e2792f7-7907-4fd5-a86a-b908259c17e1 · outbound

This paper cites 2022, AJ, 163, 43.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals 2022, AJ, 163, 43

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-07T13:00:41.719808Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation db8008fd-5741-4516-9b72-28a9ef3842ae · outbound

This paper cites A., Penny, M., Gaudi, B.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals A., Penny, M., Gaudi, B

Reference 16

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T13:00:46.103833Z

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 40729c4c-e5f1-486d-b9e5-36afdb693a37 · outbound

This paper cites K., Han, C., Udalski, A., et al.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals K., Han, C., Udalski, A., et al

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-07T13:00:41.915360Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 794df007-a768-4699-b62b-492fda01c8e4 · outbound

This paper cites K., Zang, W., Han, C., et al.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals K., Zang, W., Han, C., et al

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-07T13:00:42.001122Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ba0d836e-256c-497c-b5e5-c916506867fd · outbound

This paper cites K., Hwang, K.-H., Y ang, H., et al.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals K., Hwang, K.-H., Y ang, H., et al

Reference 19

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T13:00:45.786917Z

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 6d4f10f1-4505-44d5-84ed-107c406394e4 · outbound

This paper cites 2004, A&A, 426, 29.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals 2004, A&A, 426, 29

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-07T13:00:42.243279Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2580a0fb-f7cf-4f73-b8d4-1bdc2b94b35f · outbound

This paper cites 2021, AJ, 162, 15.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals 2021, AJ, 162, 15

Reference 21

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T13:00:45.371327Z

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 ece5d975-5b95-4163-a10e-17a66def933b · outbound

This paper cites 2016, JKAS, 49, 37.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals 2016, JKAS, 49, 37

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-07T13:00:42.419815Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cd97707a-0f45-4e8c-97a0-b235608686a6 · outbound

This paper cites 2023, AJ, 165, 54.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals 2023, AJ, 165, 54

Reference 23

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T13:00:45.078383Z

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 34627e61-47c3-4aae-8d33-031a93ba938f · outbound

This paper cites 1991, ApJ, 374, 37 Mróz, P ., Ryu, Y .-H., Skowron, J., et al.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals 1991, ApJ, 374, 37 Mróz, P ., Ryu, Y .-H., Skowron, J., et al

Reference 24

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T13:00:44.819527Z

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 e69ab75d-e103-4bc2-8c6c-b5850210f253 · outbound

This paper cites M., Gould, A., Fouqué, P.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals M., Gould, A., Fouqué, P

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-07T13:00:42.547743Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c6db955d-c8c7-4f82-b746-d562958aa73a · outbound

This paper cites T., Gaudi, B.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals T., Gaudi, B

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-07T13:00:42.626455Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ecebbf1a-0356-4322-98cd-75c71ee670f7 · outbound

This paper cites 2020, AJ, 159, 26 1.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals 2020, AJ, 159, 26 1

Reference 27

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T13:00:44.573281Z

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 088afcb8-118f-46e4-ab2e-c570684dc2b8 · outbound

This paper cites C., et al.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals C., et al

Reference 28

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T13:00:44.327437Z

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 4778299b-f666-4d81-8cde-708fc8b09042 · outbound

This paper cites A., et al.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals A., et al

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-07T13:00:43.116589Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c5edd943-faa3-4b8b-b63d-fba999b8f1bd · outbound

This paper cites 2003, Acta Astron., 53, 291.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals 2003, Acta Astron., 53, 291

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-07T13:00:43.254292Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f83425bc-9825-4424-9f8b-8c34015f5da8 · outbound

This paper cites K., & Szyma ´nski, G.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals K., & Szyma ´nski, G

Reference 31

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T13:00:44.039767Z

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 8849f23d-52ce-4630-acdf-e8085aee0d45 · outbound

This paper cites an unresolved cited work.

MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals Unresolved cited work

Reference 32

Resolution: unresolved; raw_fallback, observed 2026-08-07T13:00:43.784049Z

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.

Pith citing papers

No inbound Pith citation observations are available.