Paper Citation Record · LEDGER

Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra I cluster III. Untangling UDG 32 from the stripped filaments of NGC 3314A with multi-wavelength data

As of 11 August 2026, this Paper Citation Record lists 13 of 13 outbound references and 1 inbound Pith citation observation for arXiv:2501.16192.

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

pith.paper-citation-record.v1
2501.16192 v1

Coverage vector

measured 13 of 13 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-10T13:42:15.021061Z

measured 14 of 14 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T15:16:05.246042Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-07T15:16:09.131803Z

Reference resolution

13 of 13 outbound references displayed

verified exact0
verified fuzzy10
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External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 2fd2ecc9-f7e6-4ba9-b995-653f943960f8 · outbound

This paper cites MPDAF - A Python package for the analysis of VLT/MUSE data.

Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra I cluster III. Untangling UDG 32 from the stripped filaments of NGC 3314A with multi-wavelength data MPDAF - A Python package for the analysis of VLT/MUSE data

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-10T13:42:14.967342Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 523dd689-263d-4a9b-ab04-a178ed0cecf2 · outbound

This paper cites For conve- nience, the top axis shows the approximate distance to NGC 3314A.

Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra I cluster III. Untangling UDG 32 from the stripped filaments of NGC 3314A with multi-wavelength data For conve- nience, the top axis shows the approximate distance to NGC 3314A

Reference 2

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T13:42:15.161934Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation a8647fd0-296e-4ff0-ac2c-82da8d687a99 · outbound

This paper cites LEWIS_udg32_arxiv with narrower wavelength range (6200 ≤ λobs ≤ 7000 Å) and slightly higher SNR (≈ 3.5).

Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra I cluster III. Untangling UDG 32 from the stripped filaments of NGC 3314A with multi-wavelength data LEWIS_udg32_arxiv with narrower wavelength range (6200 ≤ λobs ≤ 7000 Å) and slightly higher SNR (≈ 3.5)

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T13:42:15.136094Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 33f8ff48-57b7-4856-ad56-fed3aa4317c2 · outbound

This paper cites We follow the methodology in Iodice et al.

Reference 5

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T13:42:15.184490Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 52e6f2f7-2775-4c72-809e-ae15efaf67e1 · outbound

This paper cites wild bootstrapping.

Reference 8

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T13:42:15.149032Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 65be3dbe-dc4e-4104-bd3c-309adfba0f71 · outbound

This paper cites We fit the SSP models to background-subtracted spectra extracted from 8-pixel circular apertures.

Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra I cluster III. Untangling UDG 32 from the stripped filaments of NGC 3314A with multi-wavelength data We fit the SSP models to background-subtracted spectra extracted from 8-pixel circular apertures

Reference 11

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T13:42:15.107199Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 8849d572-e967-4c96-9940-b94026cddb66 · outbound

This paper cites The left panel of Fig.

Reference 13

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T13:42:15.073863Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 45b92019-4898-47a1-8742-700b8c3006c1 · outbound

This paper cites 45" 43'00.

Reference 32

Resolution: malformed identifier; raw_fallback, observed 2026-08-10T13:42:15.224962Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 5f162ff2-5776-4d1f-9793-104934f0798b · outbound

This paper cites We use the inbuilt exponentially declining star-formation history (SFH) parametrised byτ, the timescale for the SF decrease and T0, the time since the SF began.

Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra I cluster III. Untangling UDG 32 from the stripped filaments of NGC 3314A with multi-wavelength data We use the inbuilt exponentially declining star-formation history (SFH) parametrised byτ, the timescale for the SF decrease and T0, the time since the SF began

Reference 2003

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T13:42:15.089300Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 20d9ab01-c556-4979-b99f-32852c2f9b91 · outbound

This paper cites However, Iodice et al.

Reference 2007

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T13:42:15.172966Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 502dabcb-1763-4d4c-8d1c-ebf73d0ee3b3 · outbound

This paper cites These data (PI: R.

Reference 2015

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T13:42:15.197187Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 0dcc5116-c618-4540-898b-f495f6de052b · outbound

This paper cites (2020) and correcting for the contamination of foreground stars, back- ground stars, and the presence of intra-cluster GCs.

Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra I cluster III. Untangling UDG 32 from the stripped filaments of NGC 3314A with multi-wavelength data (2020) and correcting for the contamination of foreground stars, back- ground stars, and the presence of intra-cluster GCs

Reference 2020

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T13:42:15.121424Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation bd107e84-6391-4859-9307-88979994b4ac · outbound

This paper cites an unresolved cited work.

Reference 8000

Resolution: unresolved; raw_fallback, observed 2026-08-10T13:42:15.210985Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Pith citing papers

Observation 307a603f-8d88-47da-b01e-1539af5fe8f4 · inbound

GAMA 526784: the progenitor of a globular cluster-rich ultra-diffuse galaxy? I. Star clusters, stellar body and ionised gas properties cites this paper.

GAMA 526784: the progenitor of a globular cluster-rich ultra-diffuse galaxy? I. Star clusters, stellar body and ionised gas properties Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra I cluster III. Untangling UDG 32 from the stripped filaments of NGC 3314A with multi-wavelength data

Reference 48

Resolution: metadata mismatch; local_arxiv, observed 2026-08-07T15:16:09.214135Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.