Paper Citation Record · LEDGER

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey

As of 2 August 2026, this Paper Citation Record lists 31 of 31 outbound references and 2 inbound Pith citation observations for arXiv:2605.07016.

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pith.paper-citation-record.v1
2605.07016 v1

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measured 31 of 31 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-05-11T01:15:08.971394Z

measured 33 of 33 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-01T06:32:01.292127+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T06:57:49.143174Z

measured 0 of 1 external citation measurements

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Source: cited_works

Reference resolution

31 of 31 outbound references displayed

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verified fuzzy26
unresolved4
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malformed identifier1
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Outbound references

Observation b23685a9-5a78-4fb3-b2ba-e51161ff21e0 · outbound

This paper cites The winds appears to originate primarily from the northern component, AS 205N.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey The winds appears to originate primarily from the northern component, AS 205N

Reference 1

Resolution: verified fuzzy; raw_fallback, observed 2026-05-14T17:12:30.302235Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 29618bf9-3909-406c-b1bd-5c41ce262a4e · outbound

This paper cites The observed H 2 morphology is consistent with this viewing geometry, with emission symmetric around the central source.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey The observed H 2 morphology is consistent with this viewing geometry, with emission symmetric around the central source

Reference 2

Resolution: verified fuzzy; raw_fallback, observed 2026-05-14T17:12:30.306378Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation a71b0b19-8adb-4b48-914f-c23500e5cf95 · outbound

This paper cites Only the blue-shifted side of the wind is detected, likely because the red-shifted emission is obscured by the disk.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey Only the blue-shifted side of the wind is detected, likely because the red-shifted emission is obscured by the disk

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-05-14T17:12:30.309867Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation ce4eaa5b-8449-4987-b740-b59e1d7ba850 · outbound

This paper cites The uniform background line emission originates from the photon-dominated region (PDR) near the Ophiuchus core.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey The uniform background line emission originates from the photon-dominated region (PDR) near the Ophiuchus core

Reference 4

Resolution: verified fuzzy; raw_fallback, observed 2026-05-14T17:12:30.215145Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 3094b57e-c671-4e5b-95c0-146fae558516 · outbound

This paper cites We detect extended H 2 emission associated with the source in the S(1), S(2), and S(3) lines.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey We detect extended H 2 emission associated with the source in the S(1), S(2), and S(3) lines

Reference 5

Resolution: verified fuzzy; raw_fallback, observed 2026-05-14T17:12:30.205903Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 3b35d1da-0480-4439-bd51-eaaa871bdeaf · outbound

This paper cites This is consistent with the face-on orientation of the system.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey This is consistent with the face-on orientation of the system

Reference 6

Resolution: verified fuzzy; raw_fallback, observed 2026-05-14T17:12:30.278424Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation bd4aa5da-68dd-4c39-9fb2-b9fdda30148b · outbound

This paper cites The background H 2 emission exhibits a gradient that increases toward the northeast, reflecting the structured nature of the PDR environment.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey The background H 2 emission exhibits a gradient that increases toward the northeast, reflecting the structured nature of the PDR environment

Reference 7

Resolution: verified fuzzy; raw_fallback, observed 2026-05-14T17:12:30.186677Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 2d220174-13e6-4c5b-80d7-8af09a755714 · outbound

This paper cites The ring is asymmetric, extending more along the northeast–southwest direction and less along the east–west direction.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey The ring is asymmetric, extending more along the northeast–southwest direction and less along the east–west direction

Reference 8

Resolution: verified fuzzy; raw_fallback, observed 2026-05-14T17:12:30.298152Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation a76f95fa-97bf-4f13-8e78-b1a36bd47b37 · outbound

This paper cites In the S(3) and S(5) lines, a monopolar outflow extending from the disk along the northeast side is observed.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey In the S(3) and S(5) lines, a monopolar outflow extending from the disk along the northeast side is observed

Reference 9

Resolution: verified fuzzy; raw_fallback, observed 2026-05-14T17:12:30.282071Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation ad7c2704-2ab8-4595-8be4-d5698330e7c0 · outbound

This paper cites an unresolved cited work.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey Unresolved cited work

Reference 10

Resolution: unresolved; raw_fallback, observed 2026-05-14T17:12:30.262147Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 5127b830-f5a2-4ac9-ae8a-ce271928ebc9 · outbound

This paper cites The emission is diffuse, without a clear preferred orientation.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey The emission is diffuse, without a clear preferred orientation

Reference 11

Resolution: verified fuzzy; raw_fallback, observed 2026-05-14T17:12:30.196544Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation c38fb16f-8e42-424b-8284-2d0fbeea85e1 · outbound

This paper cites an unresolved cited work.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey Unresolved cited work

Reference 12

Resolution: unresolved; raw_fallback, observed 2026-05-14T17:12:30.182609Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation b5a02927-d455-4bf0-982b-fecc14af66af · outbound

This paper cites In contrast, the S(1) line reveals more discernible structure, suggestive of a wide-angle outflow and a disk silhouette with major axis oriented north-east/south-west.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey In contrast, the S(1) line reveals more discernible structure, suggestive of a wide-angle outflow and a disk silhouette with major axis oriented north-east/south-west

Reference 13

Resolution: verified fuzzy; raw_fallback, observed 2026-05-14T17:12:30.191803Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation b3911967-6936-4ec4-8108-1eb8acc6e67d · outbound

This paper cites Some PSF subtraction artifacts are present, particularly in the S(5) line, where a bright artifact is visible to the north of the source.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey Some PSF subtraction artifacts are present, particularly in the S(5) line, where a bright artifact is visible to the north of the source

Reference 14

Resolution: verified fuzzy; raw_fallback, observed 2026-05-14T17:12:30.247953Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 77198566-c1a1-4e74-9015-dd6024bd99a3 · outbound

This paper cites The extended emission is concentrated around the star.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey The extended emission is concentrated around the star

Reference 15

Resolution: verified fuzzy; raw_fallback, observed 2026-05-14T17:12:30.210232Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 0525d84f-eaf5-4597-9e4d-7f3d077e4c83 · outbound

This paper cites The apparent bright emission surrounding the star is consistent with PSF subtraction artifacts.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey The apparent bright emission surrounding the star is consistent with PSF subtraction artifacts

Reference 16

Resolution: verified fuzzy; raw_fallback, observed 2026-05-14T17:12:30.270541Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 4488690f-5c5c-4d09-83af-a66e5ee41486 · outbound

This paper cites The tail is prominent and coherent, suggesting material flowing or being entrained along this direction.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey The tail is prominent and coherent, suggesting material flowing or being entrained along this direction

Reference 17

Resolution: verified fuzzy; raw_fallback, observed 2026-05-14T17:12:30.243255Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 0e1d41b8-e9ca-49ef-ad7c-611092f7a603 · outbound

This paper cites The primary component is associated with extended H2 emission, although not with an classical wind-like morphology.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey The primary component is associated with extended H2 emission, although not with an classical wind-like morphology

Reference 18

Resolution: verified fuzzy; raw_fallback, observed 2026-05-14T17:12:30.239216Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation de7f3583-c3b5-4b06-bd51-ec169a3d4f5a · outbound

This paper cites The northwestern lobe of the outflow has lower S/N in lines higher than S(1) and S(2).

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey The northwestern lobe of the outflow has lower S/N in lines higher than S(1) and S(2)

Reference 19

Resolution: verified fuzzy; raw_fallback, observed 2026-05-14T17:12:30.230691Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 5bd54062-3478-42b0-aaea-ea4bae7f844d · outbound

This paper cites The bipolar structure is well-defined across the observed H 2 lines.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey The bipolar structure is well-defined across the observed H 2 lines

Reference 20

Resolution: verified fuzzy; raw_fallback, observed 2026-05-14T17:12:30.201011Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 01209bb9-d85f-4667-b8ce-ace0a15dc23c · outbound

This paper cites The higher-Jtransitions have lower S/N.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey The higher-Jtransitions have lower S/N

Reference 21

Resolution: verified fuzzy; raw_fallback, observed 2026-05-14T17:12:30.235090Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 4608fada-25d8-427f-9171-63929e3dc23d · outbound

This paper cites The symmetric structure is consistent with the nearly face-on orientation of this system.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey The symmetric structure is consistent with the nearly face-on orientation of this system

Reference 22

Resolution: verified fuzzy; raw_fallback, observed 2026-05-14T17:12:30.252787Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 19b44958-1dc7-4496-b0e1-192a4aeece92 · outbound

This paper cites an unresolved cited work.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey Unresolved cited work

Reference 23

Resolution: unresolved; raw_fallback, observed 2026-05-14T17:12:30.266201Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation c54699e6-1251-4084-abb4-6bfadb470f52 · outbound

This paper cites No definitive sig- natures of outflows or winds are detected in the H 2 emission, except in the S(5) transition.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey No definitive sig- natures of outflows or winds are detected in the H 2 emission, except in the S(5) transition

Reference 24

Resolution: verified fuzzy; raw_fallback, observed 2026-05-14T17:12:30.293997Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation dd16b717-71ac-4d92-ba9c-41d61b1d1331 · outbound

This paper cites an unresolved cited work.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey Unresolved cited work

Reference 25

Resolution: unresolved; raw_fallback, observed 2026-05-14T17:12:30.274439Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 0c1c1a6d-6fae-4c7e-b56c-ec6fba0364bc · outbound

This paper cites The extended emission is concentrated around the central source, consistent with a face-on disk wind, and is detected in all observed H 2 lines.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey The extended emission is concentrated around the central source, consistent with a face-on disk wind, and is detected in all observed H 2 lines

Reference 26

Resolution: verified fuzzy; raw_fallback, observed 2026-05-14T17:12:30.290081Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 4e049e40-396d-4dfa-8115-0366279d08ef · outbound

This paper cites Extended emission from S(1), S(2), and S(3) H 2 lines is concentrated around the central source, consistent with a face-on disk wind.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey Extended emission from S(1), S(2), and S(3) H 2 lines is concentrated around the central source, consistent with a face-on disk wind

Reference 27

Resolution: verified fuzzy; raw_fallback, observed 2026-05-14T17:12:30.257897Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation eb6e8e84-6f4f-4488-a81a-f63630d0d729 · outbound

This paper cites The [Ne II] emission also appears extended, albeit more compact.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey The [Ne II] emission also appears extended, albeit more compact

Reference 28

Resolution: verified fuzzy; raw_fallback, observed 2026-05-14T17:12:30.285739Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation e1acf77d-3de5-4c09-8c1f-47755403802b · outbound

This paper cites The emission appears symmetric around the central source and likely traces the wide-angle disk wind.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey The emission appears symmetric around the central source and likely traces the wide-angle disk wind

Reference 29

Resolution: verified fuzzy; raw_fallback, observed 2026-05-14T17:12:30.222151Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation eecd9d27-a2d9-4028-b4af-be8e70c0f8cd · outbound

This paper cites The bubble has a brighter rim and in the inner region is less bright.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey The bubble has a brighter rim and in the inner region is less bright

Reference 30

Resolution: verified fuzzy; raw_fallback, observed 2026-05-14T17:12:30.226626Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Observation 4a7afa61-8410-4989-83d9-f192375327da · outbound

This paper cites The S(1) transition is dominated by bright, extended emission, while the higher-excitation H 2 lines reveal a weaker but discernible bipolar morphology.

Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey The S(1) transition is dominated by bright, extended emission, while the higher-excitation H 2 lines reveal a weaker but discernible bipolar morphology

Reference 31

Resolution: malformed identifier; arxiv_id, observed 2026-05-11T04:35:57.380919Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.

Pith citing papers

Observation 7a35def9-22f1-4feb-88e7-969ea507421d · inbound

JWST/MIRI Reveals the Evolution from Molecular to Atomic Disk Winds cites this paper.

JWST/MIRI Reveals the Evolution from Molecular to Atomic Disk Winds Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey

Reference 136

Resolution: unresolved; no resolver link, observed 2026-08-01T06:57:49.143174Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b6c4b42e-894d-4cc6-a956-42034db20cce · inbound

JWST/MIRI Detection of Molecular H$_2$ Winds from an Edge-on Class II Source HV Tau C cites this paper.

JWST/MIRI Detection of Molecular H$_2$ Winds from an Edge-on Class II Source HV Tau C Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-01T01:34:00.268000Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.