Paper Citation Record · LEDGER

Spatially-unresolved SED fitting can underestimate galaxy masses: a solution to the missing mass problem

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1801.07368.

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

pith.paper-citation-record.v1
1801.07368 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-14T07:24:53.781826Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-27T06:30:37.921066Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 516ce5ea-2c20-4005-8db9-6a21a05a6560 · inbound

Direct detection of cool molecular gas in a star-forming galaxy at $z=7.31$ cites this paper.

Direct detection of cool molecular gas in a star-forming galaxy at $z=7.31$ Spatially-unresolved SED fitting can underestimate galaxy masses: a solution to the missing mass problem

Reference 186

Resolution: verified exact; local_arxiv, observed 2026-06-27T06:30:37.923106Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 79a8eb1b-f4f6-42e0-ac06-938f42aa33aa · inbound

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters cites this paper.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Spatially-unresolved SED fitting can underestimate galaxy masses: a solution to the missing mass problem

Reference 258

Resolution: verified exact; local_arxiv, observed 2026-06-26T07:59:08.843347Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation d3a16bda-ffee-45c7-aa6b-e4a3d1153275 · inbound

BlackTHUNDER Reveals a Massive Filament around a Compact AGN at $z\simeq5.23$ cites this paper.

BlackTHUNDER Reveals a Massive Filament around a Compact AGN at $z\simeq5.23$ Spatially-unresolved SED fitting can underestimate galaxy masses: a solution to the missing mass problem

Reference 57

Resolution: unresolved; no resolver link, observed 2026-07-11T06:23:06.110361Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 783923b9-3b0c-4e08-86fd-3b64a2bc0da2 · inbound

Gravitationally Lensed View of DSFG-1 in PLCK G165.7+67.0: Strong Dust Emission and Spatially Resolved Stellar Population Analysis with JWST and SMA cites this paper.

Gravitationally Lensed View of DSFG-1 in PLCK G165.7+67.0: Strong Dust Emission and Spatially Resolved Stellar Population Analysis with JWST and SMA Spatially-unresolved SED fitting can underestimate galaxy masses: a solution to the missing mass problem

Reference 13

Resolution: unresolved; no resolver link, observed 2026-07-14T07:24:53.781826Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.