Paper Citation Record · LEDGER

A metal-poor atmosphere with a hot interior for a young sub-Neptune progenitor: JWST/NIRSpec transmission spectrum of V1298 Tau b

As of 22 August 2026, this Paper Citation Record lists 12 of 12 outbound references and 3 inbound Pith citation observations for arXiv:2507.08837.

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

pith.paper-citation-record.v1
2507.08837 v3

Coverage vector

measured 12 of 12 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-06T19:38:00.691073Z

measured 15 of 15 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T14:36:52.409988Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T23:07:43.633964Z

Reference resolution

12 of 12 outbound references displayed

verified exact0
verified fuzzy9
unresolved2
parse uncertain0
malformed identifier1
metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation e2261fdf-0072-4fd1-a523-ad877c221af7 · outbound

This paper cites Non-Detections of Helium in the Young Sub-Jovian Planets K2-100b, HD 63433b, & V1298 Tau c.

A metal-poor atmosphere with a hot interior for a young sub-Neptune progenitor: JWST/NIRSpec transmission spectrum of V1298 Tau b Non-Detections of Helium in the Young Sub-Jovian Planets K2-100b, HD 63433b, & V1298 Tau c

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-06T19:38:00.614813Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 130a472f-47f8-4588-81ed-b9364a18c886 · outbound

This paper cites We do not find significant offset between NRS1 and NRS2 however we find∼400 ppm offset between HST and JWST.

A metal-poor atmosphere with a hot interior for a young sub-Neptune progenitor: JWST/NIRSpec transmission spectrum of V1298 Tau b We do not find significant offset between NRS1 and NRS2 however we find∼400 ppm offset between HST and JWST

Reference 2

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T19:38:00.963702Z

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 d33945e7-dcf0-400b-b688-c1c41f00659d · outbound

This paper cites The smoothed c 2 and c 3 coefficients are used for the data-driven detrending of the spectroscopic light curves in the second iteration of light curve fits described in Appendix C.

A metal-poor atmosphere with a hot interior for a young sub-Neptune progenitor: JWST/NIRSpec transmission spectrum of V1298 Tau b The smoothed c 2 and c 3 coefficients are used for the data-driven detrending of the spectroscopic light curves in the second iteration of light curve fits described in Appendix C

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T19:38:01.007431Z

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 ab620ab3-454b-436d-b6a6-c24878924a73 · outbound

This paper cites an unresolved cited work.

A metal-poor atmosphere with a hot interior for a young sub-Neptune progenitor: JWST/NIRSpec transmission spectrum of V1298 Tau b Unresolved cited work

Reference 7

Resolution: unresolved; raw_fallback, observed 2026-08-06T19:38:00.984061Z

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 c7323777-c972-476c-b956-4cec4c13d7c3 · outbound

This paper cites Assuming that the stellar variability scales as the ratio of the two blackbody functions (Knutson et al.

A metal-poor atmosphere with a hot interior for a young sub-Neptune progenitor: JWST/NIRSpec transmission spectrum of V1298 Tau b Assuming that the stellar variability scales as the ratio of the two blackbody functions (Knutson et al

Reference 11

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T19:38:00.927200Z

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 9e383139-4ca2-44c6-a99e-42df4e998cfc · outbound

This paper cites We find that both the metallicities and the C/O ratio are consistent within 1σlevel of confidence between the free retrieval and the grid.

A metal-poor atmosphere with a hot interior for a young sub-Neptune progenitor: JWST/NIRSpec transmission spectrum of V1298 Tau b We find that both the metallicities and the C/O ratio are consistent within 1σlevel of confidence between the free retrieval and the grid

Reference 12

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T19:38:00.907247Z

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 19097ec4-a3ec-42fb-94ef-637a126de545 · outbound

This paper cites However, in NRS2 SPARTA shows a comparatively higher scatter (190 and 233 ppm for Eureka and SPARTA respectively).

A metal-poor atmosphere with a hot interior for a young sub-Neptune progenitor: JWST/NIRSpec transmission spectrum of V1298 Tau b However, in NRS2 SPARTA shows a comparatively higher scatter (190 and 233 ppm for Eureka and SPARTA respectively)

Reference 50

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T19:38:01.047615Z

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 32486141-ebc7-489b-adc5-450f8a818400 · outbound

This paper cites Pixels that are>8 pixels vertically away from the center are masked.

A metal-poor atmosphere with a hot interior for a young sub-Neptune progenitor: JWST/NIRSpec transmission spectrum of V1298 Tau b Pixels that are>8 pixels vertically away from the center are masked

Reference 100

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T19:38:01.068094Z

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 203a7397-5d04-4418-8746-b0f2ef3cf462 · outbound

This paper cites We correct for the curvature of the trace in both NRS1 and NRS2.

A metal-poor atmosphere with a hot interior for a young sub-Neptune progenitor: JWST/NIRSpec transmission spectrum of V1298 Tau b We correct for the curvature of the trace in both NRS1 and NRS2

Reference 1986

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T19:38:01.087907Z

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 e31be746-17a2-4e20-bcee-e28462bfa1ae · outbound

This paper cites A double exponential model is preferred over a gaussian rise profile by a ∆BIC of∼2000 for the NRS1 white light curve and∼1000 for the NRS2 white light curve.

A metal-poor atmosphere with a hot interior for a young sub-Neptune progenitor: JWST/NIRSpec transmission spectrum of V1298 Tau b A double exponential model is preferred over a gaussian rise profile by a ∆BIC of∼2000 for the NRS1 white light curve and∼1000 for the NRS2 white light curve

Reference 2014

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T19:38:01.027952Z

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 41ef2a33-df17-41ad-8a25-3f9d70f0a99d · outbound

This paper cites VULCAN includes disequilibrium chemistry effects such as vertical mixing and photochemistry.

A metal-poor atmosphere with a hot interior for a young sub-Neptune progenitor: JWST/NIRSpec transmission spectrum of V1298 Tau b VULCAN includes disequilibrium chemistry effects such as vertical mixing and photochemistry

Reference 2021

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T19:38:00.945572Z

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 d8fa4e59-53b5-43c8-9d39-d79b17a3208b · outbound

This paper cites an unresolved cited work.

A metal-poor atmosphere with a hot interior for a young sub-Neptune progenitor: JWST/NIRSpec transmission spectrum of V1298 Tau b Unresolved cited work

Reference 2023

Resolution: malformed identifier; no resolver link, observed 2026-08-06T19:38:00.662087Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Pith citing papers

Observation c8fe2711-1909-40d8-9e30-33be1fb45e92 · inbound

Mitigating Charge Migration in JWST NIRISS Reveals That KELT-7 b is a Metal-enriched Ultra-hot Jupiter Orbiting a Young Metal-rich Star cites this paper.

Mitigating Charge Migration in JWST NIRISS Reveals That KELT-7 b is a Metal-enriched Ultra-hot Jupiter Orbiting a Young Metal-rich Star A metal-poor atmosphere with a hot interior for a young sub-Neptune progenitor: JWST/NIRSpec transmission spectrum of V1298 Tau b

Reference 222

Resolution: verified exact; local_arxiv, observed 2026-07-10T23:07:43.648550Z

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 b42ac4c9-ffd1-42b6-847b-c9d9a1d67356 · inbound

The Sonora Substellar Atmosphere Models. VII. Flame Skimmer: Cloud-free Atmospheric and Evolutionary Models for the Coldest Substellar Objects cites this paper.

The Sonora Substellar Atmosphere Models. VII. Flame Skimmer: Cloud-free Atmospheric and Evolutionary Models for the Coldest Substellar Objects A metal-poor atmosphere with a hot interior for a young sub-Neptune progenitor: JWST/NIRSpec transmission spectrum of V1298 Tau b

Reference 253

Resolution: unresolved; no resolver link, observed 2026-08-15T14:36:52.409988Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a5b2e82d-d136-4998-bdea-6bc9cd631d5f · inbound

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era cites this paper.

Pyrat Bay 2.0: an Upgraded Framework for Exoplanet Atmosphere Modeling in the JWST Era A metal-poor atmosphere with a hot interior for a young sub-Neptune progenitor: JWST/NIRSpec transmission spectrum of V1298 Tau b

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-10T14:25:54.379266Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.