Pith. sign in

Paper Citation Record · LEDGER

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

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 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 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T14:53:58.240667Z

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 2026-08-17T06:30:58.91139+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:e8b2831f5abf49c8d5be3e9a2d4ceb5e3f700631d0a01dcf9554ba48a40d4dc3

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 2026-08-17T06:30:58.91139+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:945f77b118eb705c9ad0f19b1e895e7b46a7cb0652e64c9e7ff447ead355ec9f

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.

source=arxiv_source observed=2026-07-11T06:23:06.110361Z digest=sha256:43fe790678addd65c12fcb845d086fe17e21a3a4247207717c00853419d3b631

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.

source=arxiv_source observed=2026-07-14T07:24:53.781826Z digest=sha256:1c43d21997bf1876cb004fc7fcf803663f4e0d6bd6b584d4898da8e76fe655b2

Observation cc03cc00-6c5f-44da-8686-22e87c4b18aa · inbound

MIGHTEE-HI / LADUMA: Investigating the link between baryons and dynamics with 130 resolved HI-selected galaxies cites this paper.

MIGHTEE-HI / LADUMA: Investigating the link between baryons and dynamics with 130 resolved HI-selected galaxies Spatially-unresolved SED fitting can underestimate galaxy masses: a solution to the missing mass problem

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-15T14:53:58.240667Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T14:53:58.240667Z digest=sha256:880900b44baf08da4cca916403c57dfcffb59a0638092fc6c09ba053224b4e61