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Paper Citation Record · LEDGER

Dual-band Unified Exploration of Three CMZ Clouds (DUET). Cloud-wide census of continuum sources showing low spectral indices

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2503.23700.

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

pith.paper-citation-record.v1
2503.23700 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T05:05:39.565944Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-07T06:16:28.064256Z

Reference resolution

0 of 0 outbound references displayed

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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 fec4a1f0-b926-4947-b335-e21c44cc4044 · inbound

Properties of $\mathrm{H_2O}$ masers and their associated sources in Sagittarius B2 cites this paper.

Properties of $\mathrm{H_2O}$ masers and their associated sources in Sagittarius B2 Dual-band Unified Exploration of Three CMZ Clouds (DUET). Cloud-wide census of continuum sources showing low spectral indices

Reference 50

Resolution
verified exact
local_arxiv, observed 2026-08-07T05:05:39.992088Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-08-07T05:05:39.565944Z digest=sha256:7e6f71c2f337809879e3592e3953c617775eb781eb3bb3140c724bc678fd9ed3

Observation 1b1ad156-fdc0-4162-87af-31f04fc8c73d · inbound

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching cites this paper.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Dual-band Unified Exploration of Three CMZ Clouds (DUET). Cloud-wide census of continuum sources showing low spectral indices

Reference 37

Resolution
unresolved
no resolver link, observed 2026-07-14T15:02:03.459139Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T15:02:03.459139Z digest=sha256:200e6c00ba586d06d96df4e8ed5e8cd7c96921a5247953203abd94917a15aa42

Observation 7e5f1fd8-aeae-468d-9073-4ecc2ba77c68 · inbound

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching cites this paper.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Dual-band Unified Exploration of Three CMZ Clouds (DUET). Cloud-wide census of continuum sources showing low spectral indices

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-02T07:32:00.866296Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T07:32:00.866296Z digest=sha256:86d97ea0af27fd804e67e10d94e1b79ddf4b608c96aceec8ae57763888bf340e