Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-10T13:42:15.021061Z
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 12 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.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T15:16:05.246042Z
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
- unresolved2
- parse uncertain0
- malformed identifier1
- metadata mismatch0
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 2026-08-12T06:34:41.77262+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 2026-08-12T06:34:41.77262+00:00.
Observation 33f8ff48-57b7-4856-ad56-fed3aa4317c2 · outbound
This paper cites We follow the methodology in Iodice et al.
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 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 2026-08-12T06:34:41.77262+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 2026-08-12T06:34:41.77262+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 2026-08-12T06:34:41.77262+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 2026-08-12T06:34:41.77262+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 2026-08-12T06:34:41.77262+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 2026-08-12T06:34:41.77262+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 2026-08-12T06:34:41.77262+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 2026-08-12T06:34:41.77262+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 2026-08-12T06:34:41.77262+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 2026-08-12T06:34:41.77262+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 2026-08-12T06:34:41.77262+00:00.