Paper Citation Record · LEDGER

High-z stellar masses can be recovered robustly with JWST photometry

As of 21 August 2026, this Paper Citation Record lists 13 of 13 outbound references and 0 inbound Pith citation observations for arXiv:2412.02622.

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

pith.paper-citation-record.v1
2412.02622 v1

Coverage vector

measured 13 of 13 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-11T23:20:52.042728Z

measured 13 of 13 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+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

13 of 13 outbound references displayed

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Outbound references

Observation 27d7da18-ccb8-4cbf-b8a9-295e46bca458 · outbound

This paper cites J., Bowler, R.

High-z stellar masses can be recovered robustly with JWST photometry J., Bowler, R

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-11T23:20:51.945498Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 39367b3d-0262-4c62-8cc6-45677b99892e · outbound

This paper cites The high redshift SFR-M* relation is sensitive to the employed star formation rate and stellar mass indicators: Towards addressing the tension between observations and simulations.

High-z stellar masses can be recovered robustly with JWST photometry The high redshift SFR-M* relation is sensitive to the employed star formation rate and stellar mass indicators: Towards addressing the tension between observations and simulations

Reference 8

Resolution: metadata mismatch; local_arxiv, observed 2026-08-11T23:20:52.228277Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 24926700-1683-43f0-b011-aae3785d9b5e · outbound

This paper cites Solution to the conflict between the resolved and unresolved galaxy stellar mass estimation from the perspective of JWST.

High-z stellar masses can be recovered robustly with JWST photometry Solution to the conflict between the resolved and unresolved galaxy stellar mass estimation from the perspective of JWST

Reference 11

Resolution: verified exact; local_arxiv, observed 2026-08-11T23:20:52.152869Z

Source-reported events for the cited work

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Observation dbfc046c-ae4e-4315-adfe-18c969ca8b9e · outbound

This paper cites EPOCHS IX. When cosmic dawn breaks: Evidence for evolved stellar populations in $7 < z < 12$ galaxies from PEARLS GTO and public NIRCam imaging.

High-z stellar masses can be recovered robustly with JWST photometry EPOCHS IX. When cosmic dawn breaks: Evidence for evolved stellar populations in $7 < z < 12$ galaxies from PEARLS GTO and public NIRCam imaging

Reference 13

Resolution: metadata mismatch; local_arxiv, observed 2026-08-11T23:20:52.098795Z

Source-reported events for the cited work

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Observation d30c10c0-5261-42ba-9e25-b68d2f3e41ff · outbound

This paper cites Disappearing galaxies: the orientation dependence of JWST-bright, HST-dark, star-forming galaxy selection.

High-z stellar masses can be recovered robustly with JWST photometry Disappearing galaxies: the orientation dependence of JWST-bright, HST-dark, star-forming galaxy selection

Reference 37

Resolution: verified exact; local_arxiv, observed 2026-08-11T23:20:52.278894Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 2142d191-4165-44f9-811b-92fac5d3a7e7 · outbound

This paper cites Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?.

High-z stellar masses can be recovered robustly with JWST photometry Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?

Reference 128

Resolution: unresolved; no resolver link, observed 2026-08-11T23:20:51.951904Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d461601f-fa27-41d7-a670-8a32b1d3ec48 · outbound

This paper cites The Art of Measuring Physical Parameters in Galaxies: A Critical Assessment of Spectral Energy Distribution Fitting Techniques.

High-z stellar masses can be recovered robustly with JWST photometry The Art of Measuring Physical Parameters in Galaxies: A Critical Assessment of Spectral Energy Distribution Fitting Techniques

Reference 141

Resolution: unresolved; no resolver link, observed 2026-08-11T23:20:52.024024Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7dfcb221-044a-4d7c-9f69-3ed5f3eee66e · outbound

This paper cites The VANDELS survey: the star-formation histories of massive quiescent galaxies at 1.0 < z < 1.3.

High-z stellar masses can be recovered robustly with JWST photometry The VANDELS survey: the star-formation histories of massive quiescent galaxies at 1.0 < z < 1.3

Reference 417

Resolution: unresolved; no resolver link, observed 2026-08-11T23:20:51.974894Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 02ab459c-1e6b-4fb6-94de-543e7a165dd7 · outbound

This paper cites an unresolved cited work.

High-z stellar masses can be recovered robustly with JWST photometry Unresolved cited work

Reference 1000

Resolution: verified exact; raw_fallback, observed 2026-08-11T23:20:52.436825Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation ae780b9c-b8c1-407d-b6a2-4ff6e6e6ca38 · outbound

This paper cites How Well Can We Measure the Stellar Mass of a Galaxy: The Impact of the Assumed Star Formation History Model in SED Fitting.

High-z stellar masses can be recovered robustly with JWST photometry How Well Can We Measure the Stellar Mass of a Galaxy: The Impact of the Assumed Star Formation History Model in SED Fitting

Reference 2020

Resolution: unresolved; no resolver link, observed 2026-08-11T23:20:52.012688Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d0e3ef4e-ab76-45ce-bda4-a9ad150087ae · outbound

This paper cites A massive interacting galaxy 510 million years after the Big Bang.

High-z stellar masses can be recovered robustly with JWST photometry A massive interacting galaxy 510 million years after the Big Bang

Reference 2023

Resolution: unresolved; no resolver link, observed 2026-08-11T23:20:51.959779Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1e7cb250-ed1e-4c6d-b58e-7fa4f8668405 · outbound

This paper cites Exploring the nature of UV-bright $z \gtrsim 10$ galaxies detected by JWST: star formation, black hole accretion, or a non-universal IMF?.

High-z stellar masses can be recovered robustly with JWST photometry Exploring the nature of UV-bright $z \gtrsim 10$ galaxies detected by JWST: star formation, black hole accretion, or a non-universal IMF?

Reference 3563

Resolution: unresolved; no resolver link, observed 2026-08-11T23:20:52.037310Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 468d2950-4f7f-46a5-a6c2-d8debeb53e24 · outbound

This paper cites An ALMA survey of the SCUBA-2 CLS UDS field: Physical properties of 707 Sub-millimetre Galaxies.

High-z stellar masses can be recovered robustly with JWST photometry An ALMA survey of the SCUBA-2 CLS UDS field: Physical properties of 707 Sub-millimetre Galaxies

Reference 3828

Resolution: unresolved; no resolver link, observed 2026-08-11T23:20:51.993923Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Pith citing papers

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