Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
A Quantitative Comparison of SMC, LMC, and Milky Way UV to NIR Extinction Curves
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 17 inbound Pith citation observations for arXiv:astro-ph/0305257.
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 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-08T15:21:47.715430Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-01T05:05:24.144729Z
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 031023c9-7ed6-4876-97ac-0fb8eebfa244 · inbound
Interstellar dust production, destruction and effects of dust depletion in galaxies cites this paper.
Interstellar dust production, destruction and effects of dust depletion in galaxies A Quantitative Comparison of SMC, LMC, and Milky Way UV to NIR Extinction Curves
Reference 235
- Resolution
- verified exact
- local_arxiv, observed 2026-05-19T09:02:13.699730Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation a160e4b3-24f4-4d1b-a1bd-ac87248039e2 · inbound
Massive Galaxies Form Early and Gray: Stellar Assembly and Dust Attenuation at $\mathbf{z>3.5}$ from CAPERS cites this paper.
Massive Galaxies Form Early and Gray: Stellar Assembly and Dust Attenuation at $\mathbf{z>3.5}$ from CAPERS A Quantitative Comparison of SMC, LMC, and Milky Way UV to NIR Extinction Curves
Reference 75
- Resolution
- verified exact
- local_arxiv, observed 2026-05-15T02:38:33.525269Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation b8ae0bfd-36b0-48ac-86c4-6b0fbe4bd59d · inbound
Quenching of X-ray emission in little red dots by both Compton-thick gas and high accretion rates cites this paper.
Quenching of X-ray emission in little red dots by both Compton-thick gas and high accretion rates A Quantitative Comparison of SMC, LMC, and Milky Way UV to NIR Extinction Curves
Reference 137
- Resolution
- verified exact
- local_arxiv, observed 2026-05-19T16:17:39.766789Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation fe23783a-180e-4239-8520-7883ad989eef · inbound
Strong X-ray Variability of I Zwicky 1: Obscuration from Clumpy Accretion-Disk Winds cites this paper.
Strong X-ray Variability of I Zwicky 1: Obscuration from Clumpy Accretion-Disk Winds A Quantitative Comparison of SMC, LMC, and Milky Way UV to NIR Extinction Curves
Reference 71
- Resolution
- verified exact
- local_arxiv, observed 2026-05-25T05:35:22.212304Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation fccc0f9e-fbaa-4337-ae54-7a4d64ad93e2 · inbound
Learning the Universe: The Structure of Dust Attenuation Curves in Galaxy Simulations cites this paper.
Learning the Universe: The Structure of Dust Attenuation Curves in Galaxy Simulations A Quantitative Comparison of SMC, LMC, and Milky Way UV to NIR Extinction Curves
Reference 114
- Resolution
- verified exact
- local_arxiv, observed 2026-06-27T15:51:01.798089Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation c5b4d7f2-ae8d-47db-8910-c8cb2d352436 · inbound
Between Degeneracy and Evolution: UV-to-optical Insights into the BH$^*$ Model in Little Red Dots cites this paper.
Between Degeneracy and Evolution: UV-to-optical Insights into the BH$^*$ Model in Little Red Dots A Quantitative Comparison of SMC, LMC, and Milky Way UV to NIR Extinction Curves
Reference 201
- Resolution
- verified exact
- local_arxiv, observed 2026-06-27T10:00:49.880680Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 8c667093-c87f-46fb-82d3-8dce8447bd53 · inbound
MEGA and SMILES Find Fewer Dusty Galaxies than Expected at Cosmic Noon cites this paper.
MEGA and SMILES Find Fewer Dusty Galaxies than Expected at Cosmic Noon A Quantitative Comparison of SMC, LMC, and Milky Way UV to NIR Extinction Curves
Reference 141
- Resolution
- verified exact
- local_arxiv, observed 2026-06-27T03:30:27.344665Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 44f296f5-1c4d-45f2-bfe6-df779abe2cf7 · inbound
Diverse Histories and Common Origins of Nitrogen-enhanced JWST Galaxies cites this paper.
Diverse Histories and Common Origins of Nitrogen-enhanced JWST Galaxies A Quantitative Comparison of SMC, LMC, and Milky Way UV to NIR Extinction Curves
Reference 126
- Resolution
- verified exact
- local_arxiv, observed 2026-06-27T00:00:16.028715Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation fb7ff898-c83d-4e8f-90a8-c36abd9abe9b · inbound
Variables in S-PLUS: I. Multiband period-luminosity relations and reddening maps of the Magellanic Clouds using classical Cepheids cites this paper.
Variables in S-PLUS: I. Multiband period-luminosity relations and reddening maps of the Magellanic Clouds using classical Cepheids A Quantitative Comparison of SMC, LMC, and Milky Way UV to NIR Extinction Curves
Reference 53
- Resolution
- verified exact
- local_arxiv, observed 2026-06-26T16:49:36.590167Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation d860ebc0-c308-4a22-bafa-6b1e444964a9 · inbound
Constraints on Binarity for the Extreme Oe Variable Star AzV 493 cites this paper.
Constraints on Binarity for the Extreme Oe Variable Star AzV 493 A Quantitative Comparison of SMC, LMC, and Milky Way UV to NIR Extinction Curves
Reference 18
- Resolution
- verified exact
- local_arxiv, observed 2026-06-26T01:08:48.422541Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation bdb4f354-1395-4d3a-965a-2103e761f3e3 · inbound
JWST spectroscopy of galaxies at $z>10$: Damped Ly$\alpha$ absorbers reveal efficient star formation and hidden redshift biases cites this paper.
JWST spectroscopy of galaxies at $z>10$: Damped Ly$\alpha$ absorbers reveal efficient star formation and hidden redshift biases A Quantitative Comparison of SMC, LMC, and Milky Way UV to NIR Extinction Curves
Reference 174
- Resolution
- verified exact
- local_arxiv, observed 2026-07-01T02:05:14.963455Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 531ac51a-cfaf-4ca6-869c-1328b480fe57 · inbound
The metallicities of little red dot host galaxies: LRDs are metal poor, but not pristine cites this paper.
The metallicities of little red dot host galaxies: LRDs are metal poor, but not pristine A Quantitative Comparison of SMC, LMC, and Milky Way UV to NIR Extinction Curves
Reference 102
- Resolution
- verified exact
- local_arxiv, observed 2026-07-01T05:05:24.146747Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 2f2ab24a-21d0-40ff-a638-b2cc6de3f212 · 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 A Quantitative Comparison of SMC, LMC, and Milky Way UV to NIR Extinction Curves
Reference 63
- Resolution
- unresolved
- no resolver link, observed 2026-07-14T10:44:26.626236Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6f948d5e-dc4b-472c-b19f-78ab6aeb9187 · 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 A Quantitative Comparison of SMC, LMC, and Milky Way UV to NIR Extinction Curves
Reference 63
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T07:18:20.299219Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 40a79dcf-4e49-46b3-9434-10ba4e4fb100 · inbound
The potential broader complex linked to the key Cepheid SV Vul cites this paper.
The potential broader complex linked to the key Cepheid SV Vul A Quantitative Comparison of SMC, LMC, and Milky Way UV to NIR Extinction Curves
Reference 174
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T03:06:04.748490Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e362babd-472d-40e0-9341-8fee4afed037 · inbound
An (in)complete NIRSpec census of Balmer absorption in Type 1 AGN -- radiation-driven outflows in little red dots, quasars and variable stars cites this paper.
An (in)complete NIRSpec census of Balmer absorption in Type 1 AGN -- radiation-driven outflows in little red dots, quasars and variable stars A Quantitative Comparison of SMC, LMC, and Milky Way UV to NIR Extinction Curves
Reference 59
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T13:38:26.427770Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 61c119d0-ed88-4527-b61b-ba1e970acdbf · inbound
Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud cites this paper.
Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud A Quantitative Comparison of SMC, LMC, and Milky Way UV to NIR Extinction Curves
Reference 66
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T15:21:47.715430Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.