Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-10T14:43:30.369572Z
Paper Citation Record · LEDGER
Spatially-resolved spectro-photometric SED Modeling of NGC 253's Central Molecular Zone I. Studying the star formation in extragalactic giant molecular clouds
As of 13 August 2026, this Paper Citation Record lists 15 of 15 outbound references and 3 inbound Pith citation observations for arXiv:2501.15082.
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 2026-08-13T06:32:02.005865+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T10:28:56.204418Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-14T12:15:04.098795Z
Reference resolution
15 of 15 outbound references displayed
- verified exact0
- verified fuzzy6
- unresolved6
- parse uncertain0
- malformed identifier3
- metadata mismatch0
External citation measurements
No source-named external measurement is stored.
Outbound references
Observation 10128e20-0d31-42a9-a96a-0be908c4207d · outbound
This paper cites L., Knapen, J.
Reference 1
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-10T14:43:30.622454Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 82a91878-a9ee-4a45-a75c-f0db828097b9 · outbound
This paper cites 1000, 5000 AGN Power-law slope αAGN −2.0 to−0.2 by a bin of 0.5 ∗ computed as log10 LIR(8−1000µm) -log10 L1.4 GHz, where L1.4 GHz is the radio luminosity at 1.4 GHz.
Spatially-resolved spectro-photometric SED Modeling of NGC 253's Central Molecular Zone I. Studying the star formation in extragalactic giant molecular clouds 1000, 5000 AGN Power-law slope αAGN −2.0 to−0.2 by a bin of 0.5 ∗ computed as log10 LIR(8−1000µm) -log10 L1.4 GHz, where L1.4 GHz is the radio luminosity at 1.4 GHz
Reference 2
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-10T14:43:30.530698Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation e956f06d-91dc-42cf-8ce7-5b63d31d92b4 · outbound
This paper cites 2015; Humire et al.
Spatially-resolved spectro-photometric SED Modeling of NGC 253's Central Molecular Zone I. Studying the star formation in extragalactic giant molecular clouds 2015; Humire et al
Reference 5
- Resolution
- malformed identifier
- raw_fallback, observed 2026-08-10T14:43:30.515196Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 838746ee-53bc-4748-a4e6-e4c38c36c1da · outbound
This paper cites 2020; Butterworth et al.
Spatially-resolved spectro-photometric SED Modeling of NGC 253's Central Molecular Zone I. Studying the star formation in extragalactic giant molecular clouds 2020; Butterworth et al
Reference 6
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-10T14:43:30.422980Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation e6d82eca-ac7c-4f50-af60-c0b32ad51679 · outbound
This paper cites This corresponds to the depiction of cold/low-dispersion gas actively producing stars at the convergence of the ring and the bar, as observed in M 100 (Allard et al.
Spatially-resolved spectro-photometric SED Modeling of NGC 253's Central Molecular Zone I. Studying the star formation in extragalactic giant molecular clouds This corresponds to the depiction of cold/low-dispersion gas actively producing stars at the convergence of the ring and the bar, as observed in M 100 (Allard et al
Reference 7
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-10T14:43:30.577909Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation fca23ab5-8796-44a2-b52e-5ce553cbf64e · outbound
This paper cites an unresolved cited work.
Spatially-resolved spectro-photometric SED Modeling of NGC 253's Central Molecular Zone I. Studying the star formation in extragalactic giant molecular clouds Unresolved cited work
Reference 9
- Resolution
- unresolved
- raw_fallback, observed 2026-08-10T14:43:30.500442Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation bc90eb4a-ab2a-481d-958a-d53553daf33e · outbound
This paper cites an unresolved cited work.
Spatially-resolved spectro-photometric SED Modeling of NGC 253's Central Molecular Zone I. Studying the star formation in extragalactic giant molecular clouds Unresolved cited work
Reference 11
- Resolution
- unresolved
- raw_fallback, observed 2026-08-10T14:43:30.468180Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 91b6f3fc-ff14-4b5e-bf79-61c53176a2bf · outbound
This paper cites ) 350 m SPIRE (24.9.
Spatially-resolved spectro-photometric SED Modeling of NGC 253's Central Molecular Zone I. Studying the star formation in extragalactic giant molecular clouds ) 350 m SPIRE (24.9
Reference 15
- Resolution
- malformed identifier
- raw_fallback, observed 2026-08-10T14:43:30.406955Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 029ff600-e587-44e4-a960-03fe6176a03b · outbound
This paper cites For the CIGALE modeling including the AGN component, we only added the AGN module to the existing input parameters.
Spatially-resolved spectro-photometric SED Modeling of NGC 253's Central Molecular Zone I. Studying the star formation in extragalactic giant molecular clouds For the CIGALE modeling including the AGN component, we only added the AGN module to the existing input parameters
Reference 253
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-10T14:43:30.607210Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 71661519-7d33-4de0-be95-832db4866bb0 · outbound
This paper cites Our best-results are shown in Fig.
Spatially-resolved spectro-photometric SED Modeling of NGC 253's Central Molecular Zone I. Studying the star formation in extragalactic giant molecular clouds Our best-results are shown in Fig
Reference 2005
- Resolution
- malformed identifier
- raw_fallback, observed 2026-08-10T14:43:30.438443Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation d0ba1341-48ab-4b25-8471-7d8081cacf56 · outbound
This paper cites an unresolved cited work.
Spatially-resolved spectro-photometric SED Modeling of NGC 253's Central Molecular Zone I. Studying the star formation in extragalactic giant molecular clouds Unresolved cited work
Reference 2006
- Resolution
- unresolved
- raw_fallback, observed 2026-08-10T14:43:30.484448Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 3373a68c-58fe-4822-a96d-469ae4cd1832 · outbound
This paper cites an unresolved cited work.
Spatially-resolved spectro-photometric SED Modeling of NGC 253's Central Molecular Zone I. Studying the star formation in extragalactic giant molecular clouds Unresolved cited work
Reference 2014
- Resolution
- unresolved
- raw_fallback, observed 2026-08-10T14:43:30.546165Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 8839177a-8230-4f77-8395-7f166558faab · outbound
This paper cites an unresolved cited work.
Spatially-resolved spectro-photometric SED Modeling of NGC 253's Central Molecular Zone I. Studying the star formation in extragalactic giant molecular clouds Unresolved cited work
Reference 2015
- Resolution
- unresolved
- raw_fallback, observed 2026-08-10T14:43:30.561798Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 3a07a36a-034e-49a9-b35b-b9b407490481 · outbound
This paper cites an unresolved cited work.
Spatially-resolved spectro-photometric SED Modeling of NGC 253's Central Molecular Zone I. Studying the star formation in extragalactic giant molecular clouds Unresolved cited work
Reference 2019
- Resolution
- unresolved
- raw_fallback, observed 2026-08-10T14:43:30.453528Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation fcee6a2a-1383-49d3-8d3a-ced09660cd37 · outbound
This paper cites Indeed, the strongest SiO(5–4)/HNCO(100,10− 90,9) ratios are observed at this position (Humire et al.
Spatially-resolved spectro-photometric SED Modeling of NGC 253's Central Molecular Zone I. Studying the star formation in extragalactic giant molecular clouds Indeed, the strongest SiO(5–4)/HNCO(100,10− 90,9) ratios are observed at this position (Humire et al
Reference 2023
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-10T14:43:30.592111Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Pith citing papers
Observation ed0848b3-bda2-4503-b22d-b1a8397cbf03 · inbound
The Discovery of 25 um Interstellar Methanol cites this paper.
The Discovery of 25 um Interstellar Methanol Spatially-resolved spectro-photometric SED Modeling of NGC 253's Central Molecular Zone I. Studying the star formation in extragalactic giant molecular clouds
Reference 65
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T10:28:56.204418Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4a597fc9-0661-4270-bfd4-4fb9c579580a · inbound
Mapping Dust Attenuation at Kiloparsec Scales. III. The 2175\AA\ Bump cites this paper.
Mapping Dust Attenuation at Kiloparsec Scales. III. The 2175\AA\ Bump Spatially-resolved spectro-photometric SED Modeling of NGC 253's Central Molecular Zone I. Studying the star formation in extragalactic giant molecular clouds
Reference 7
- Resolution
- verified exact
- local_arxiv, observed 2026-07-14T10:50:24.481262Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 7c0ac809-cf3f-4bd8-a231-6ed82370c84a · inbound
Mapping Dust Attenuation at Kiloparsec Scales. III. The 2175\AA\ Bump cites this paper.
Mapping Dust Attenuation at Kiloparsec Scales. III. The 2175\AA\ Bump Spatially-resolved spectro-photometric SED Modeling of NGC 253's Central Molecular Zone I. Studying the star formation in extragalactic giant molecular clouds
Reference 7
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T07:18:13.182288Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.