Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
A Simple Model for the Absorption of Starlight by Dust in Galaxies
As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 49 inbound Pith citation observations for arXiv:astro-ph/0003128.
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 2026-08-16T06:30:59.297886+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-16T00:14:35.593121Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-03T11:28:04.821422Z
Reference resolution
0 of 0 outbound references displayed
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External citation measurements
1488
pith, observed 2026-07-03T11:28:04.821422Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 3ac81747-574d-48ee-a97c-db0a57af815c · inbound
Inferring the star-formation histories of massive quiescent galaxies with BAGPIPES: Evidence for multiple quenching mechanisms cites this paper.
Inferring the star-formation histories of massive quiescent galaxies with BAGPIPES: Evidence for multiple quenching mechanisms A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 20
- Resolution
- metadata mismatch
- doi, observed 2026-05-15T04:37:44.177962Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation f14aafdd-b495-482f-9648-335e07bd48cc · inbound
First Results from the TNG50 Simulation: Galactic outflows driven by supernovae and black hole feedback cites this paper.
First Results from the TNG50 Simulation: Galactic outflows driven by supernovae and black hole feedback A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 93
- Resolution
- verified exact
- doi, observed 2026-05-16T10:56:58.961163Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation f4cacbcc-6509-4faf-b3a9-4e5b8ade0424 · inbound
Galaxy And Mass Assembly: A new approach to quantifying dust in galaxies cites this paper.
Galaxy And Mass Assembly: A new approach to quantifying dust in galaxies A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 2023
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T20:15:20.221238Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d956dc47-ebc7-4c75-84f9-b5996685fa42 · inbound
From the Densest Clusters to the Emptiest Voids: No Evidence For Environmental Effects on the Galaxy Size-Mass Relation at Low Redshift cites this paper.
From the Densest Clusters to the Emptiest Voids: No Evidence For Environmental Effects on the Galaxy Size-Mass Relation at Low Redshift A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 22
- Resolution
- verified exact
- doi, observed 2026-05-19T07:02:59.699819Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 50926e32-1961-4480-a465-eee7c4469574 · inbound
The Fraction of Clumpy Galaxies in JADES Over $2<z<9$ cites this paper.
The Fraction of Clumpy Galaxies in JADES Over $2<z<9$ A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 27
- Resolution
- verified exact
- doi, observed 2026-05-18T22:02:51.482540Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 728191cb-32f7-4bdc-9c6f-75a334a4e5be · inbound
pop-cosmos: Star formation over 12 Gyr from generative modelling of a deep infrared-selected galaxy catalogue cites this paper.
pop-cosmos: Star formation over 12 Gyr from generative modelling of a deep infrared-selected galaxy catalogue A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 37
- Resolution
- metadata mismatch
- doi, observed 2026-05-18T14:06:26.961617Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 16482908-0bfd-4b11-9aca-0adb1a5bbbb7 · inbound
Calibrating Photometric Mid-Infrared Star Formation Rates for JWST cites this paper.
Calibrating Photometric Mid-Infrared Star Formation Rates for JWST A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 31
- Resolution
- verified exact
- doi, observed 2026-05-13T22:03:20.065686Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation ccec8720-e16f-46fa-bc03-ac50aa0e8a15 · inbound
Sparks II: Panchromatic SED modeling and galaxy physical properties across the starburst to post-starburst sequence cites this paper.
Sparks II: Panchromatic SED modeling and galaxy physical properties across the starburst to post-starburst sequence A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 28
- Resolution
- verified exact
- doi, observed 2026-05-10T14:20:28.941117Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation f15153d8-3251-4ed7-b794-a2384f4ae909 · inbound
Unraveling Chemical Enrichment in Extreme Emission-Line Galaxies: A Multi-Element Bayesian View of Bursty Star Formation and Galaxy Evolution in DESI cites this paper.
Unraveling Chemical Enrichment in Extreme Emission-Line Galaxies: A Multi-Element Bayesian View of Bursty Star Formation and Galaxy Evolution in DESI A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 17
- Resolution
- verified exact
- doi, observed 2026-05-10T01:30:54.557740Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 41e65512-df40-44a1-9208-f85a4e3c502f · inbound
Tidal pre-conditioning and ram-pressure stripping in NGC 1427A. Deep VLT/MUSE spectroscopy and FUV-to-radio observations trace a Fornax Cluster dwarf in transformation cites this paper.
Tidal pre-conditioning and ram-pressure stripping in NGC 1427A. Deep VLT/MUSE spectroscopy and FUV-to-radio observations trace a Fornax Cluster dwarf in transformation A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 121
- Resolution
- verified exact
- doi, observed 2026-05-09T19:00:07.929036Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation ff3dc55a-2df2-4b60-bfaf-ee4a5c2ccb1d · inbound
Tidal pre-conditioning and ram-pressure stripping in NGC 1427A. Deep VLT/MUSE spectroscopy and FUV-to-radio observations trace a Fornax Cluster dwarf in transformation cites this paper.
Tidal pre-conditioning and ram-pressure stripping in NGC 1427A. Deep VLT/MUSE spectroscopy and FUV-to-radio observations trace a Fornax Cluster dwarf in transformation A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 121
- Resolution
- verified exact
- doi, observed 2026-05-15T06:19:49.198097Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 29ea689d-48db-4748-874d-3dab27467ebd · inbound
Prospects for Observing Galaxy Spectral Energy Distribution from the Radio to the far-Infrared in the Era of Next-Generation Radio Telescopes cites this paper.
Prospects for Observing Galaxy Spectral Energy Distribution from the Radio to the far-Infrared in the Era of Next-Generation Radio Telescopes A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 24
- Resolution
- verified exact
- doi, observed 2026-05-09T19:40:39.781524Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 38dd34b4-dd26-4f2f-98b8-3244aa16648f · inbound
Peering down the barrel with DESI DR2: 10 000+ inflows at $z$ < 0.6 reveal how galaxies accrete cold gas cites this paper.
Peering down the barrel with DESI DR2: 10 000+ inflows at $z$ < 0.6 reveal how galaxies accrete cold gas A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 48
- Resolution
- verified exact
- doi, observed 2026-05-08T18:18:54.365409Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 648a9331-5058-430a-994d-e1e06020c853 · inbound
Interpreting Galaxy Physical Properties Using Stellar Population Synthesis cites this paper.
Interpreting Galaxy Physical Properties Using Stellar Population Synthesis A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 16
- Resolution
- verified exact
- doi, observed 2026-05-09T05:30:19.032915Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 087743a9-6f8b-49e0-a47d-b05db4924f57 · inbound
A Multiwavelength Assessment Disfavoring the X-ray Binary Origin of He III Regions in Metal-Poor Star-Forming Dwarf Galaxies cites this paper.
A Multiwavelength Assessment Disfavoring the X-ray Binary Origin of He III Regions in Metal-Poor Star-Forming Dwarf Galaxies A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 18
- Resolution
- verified exact
- doi, observed 2026-05-08T23:09:40.116149Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 5fd5fa0f-4930-463e-a970-98a461d72613 · inbound
Stardust Galaxies at z>9: A Dust-Origin Transition Behind the Excess of UV-Bright Galaxies cites this paper.
Stardust Galaxies at z>9: A Dust-Origin Transition Behind the Excess of UV-Bright Galaxies A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 20
- Resolution
- verified exact
- doi, observed 2026-05-12T04:46:21.644806Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 953e4cc7-71ad-4fd8-b407-da120c917a73 · inbound
Stardust Galaxies at z>9: A Dust-Origin Transition Behind the Excess of UV-Bright Galaxies cites this paper.
Stardust Galaxies at z>9: A Dust-Origin Transition Behind the Excess of UV-Bright Galaxies A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 20
- Resolution
- verified exact
- doi, observed 2026-05-20T23:19:13.199124Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation bb872772-244a-4aed-b1b6-daf1e250707d · inbound
First Light And Reionization Epoch Simulations (FLARES) XXI: The UV Indices of Galaxies in the Early Universe cites this paper.
First Light And Reionization Epoch Simulations (FLARES) XXI: The UV Indices of Galaxies in the Early Universe A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 220
- Resolution
- verified exact
- local_arxiv, observed 2026-05-14T18:19:23.008095Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation f1344fd7-c154-4373-ab4d-c2210cf731a6 · inbound
From DES to KiDS: Domain adaptation for cross-survey detection of low-surface-brightness galaxies cites this paper.
From DES to KiDS: Domain adaptation for cross-survey detection of low-surface-brightness galaxies A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 30
- Resolution
- verified exact
- local_arxiv, observed 2026-05-14T17:47:31.947801Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation f3ef8289-e7a8-4ce2-9621-43f980156094 · 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 Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 107
- Resolution
- verified exact
- local_arxiv, observed 2026-05-15T02:38:33.735338Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation c502930c-5b20-4f55-8666-f9a973aa53c5 · inbound
A stellar bar hidden in an extreme gas-rich disk galaxy at z=4.055 cites this paper.
A stellar bar hidden in an extreme gas-rich disk galaxy at z=4.055 A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 30
- Resolution
- verified exact
- doi, observed 2026-05-19T15:57:39.569777Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 6450f846-4f68-409c-8aa1-cc5554d7744b · inbound
A stellar bar hidden in an extreme gas-rich disk galaxy at z=4.055 cites this paper.
A stellar bar hidden in an extreme gas-rich disk galaxy at z=4.055 A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 30
- Resolution
- verified exact
- doi, observed 2026-06-30T20:05:04.047343Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation b2a3817f-e276-40b6-9792-64886e4a22d7 · inbound
PEARLS: JWST Counterparts of Micro-Jy Radio Sources in the NEP Time Domain Field. II. All Four Spokes cites this paper.
PEARLS: JWST Counterparts of Micro-Jy Radio Sources in the NEP Time Domain Field. II. All Four Spokes A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 54
- Resolution
- verified exact
- local_arxiv, observed 2026-05-20T15:38:26.232039Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation d4ca2ed2-e71d-4fdc-be3f-366c92aa7a36 · inbound
Difference Between Half-mass Radius and Half-light Radius of Galaxies at 0.2 $< z <$ 2.5 Revealed by JWST/NIRCam Data cites this paper.
Difference Between Half-mass Radius and Half-light Radius of Galaxies at 0.2 $< z <$ 2.5 Revealed by JWST/NIRCam Data A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 13
- Resolution
- verified exact
- doi, observed 2026-05-21T03:43:55.895510Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation f5c73958-e5cc-42d3-8c2a-3aa4e7d33ec0 · inbound
JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: stellar population catalogue for galaxies in GOODS-N and GOODS-S cites this paper.
JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: stellar population catalogue for galaxies in GOODS-N and GOODS-S A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 150
- Resolution
- verified exact
- local_arxiv, observed 2026-05-22T09:06:19.683267Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation f9dbe73c-478b-4bf0-b470-b3557a81349c · inbound
SDSS+JWST Census of Stellar and Nebular Dust Attenuation at $z \sim 0$-7: Mass Dependence and Redshift Evolution cites this paper.
SDSS+JWST Census of Stellar and Nebular Dust Attenuation at $z \sim 0$-7: Mass Dependence and Redshift Evolution A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 26
- Resolution
- verified exact
- doi, observed 2026-05-25T05:25:22.213238Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation fe39a664-cad4-4828-9789-af43c206e589 · inbound
Exploring biases in derived stellar parameters and the ionizing photon production efficiency cites this paper.
Exploring biases in derived stellar parameters and the ionizing photon production efficiency A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 28
- Resolution
- verified exact
- doi, observed 2026-06-29T23:54:02.476150Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 03ba2278-0957-45f0-bf95-3f115b0a83d6 · inbound
The quenching time and timescale distribution of z~2 quiescent galaxies from precise colour distribution analysis cites this paper.
The quenching time and timescale distribution of z~2 quiescent galaxies from precise colour distribution analysis A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 19
- Resolution
- verified exact
- doi, observed 2026-06-28T00:51:26.750790Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 316ea28e-5720-460c-83ee-aea72f00b78e · inbound
Towards Bayesian Photometric Cosmic Chronometers: Application to VIPERS cites this paper.
Towards Bayesian Photometric Cosmic Chronometers: Application to VIPERS A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 9
- Resolution
- verified exact
- doi, observed 2026-06-27T21:31:16.499056Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 43df56c9-5ea3-4ec6-aba4-d1d0b0644d8a · 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 Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 56
- Resolution
- verified exact
- local_arxiv, observed 2026-06-27T15:51:01.588135Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 58035018-2f15-45e5-9950-6a6f561e9a5b · inbound
JADES: the mass-metallicity relation at $z=1-10$. New calibrations, extremely metal-poor galaxies, and chemical diversity cites this paper.
JADES: the mass-metallicity relation at $z=1-10$. New calibrations, extremely metal-poor galaxies, and chemical diversity A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 31
- Resolution
- metadata mismatch
- doi, observed 2026-06-27T12:20:54.715907Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation b3951b37-2076-4074-ae2f-a4900f1dafbf · inbound
X-ray luminosity function of Compton-thick AGN in the early Universe (z > 3). Robustness and biases of the CTK population cites this paper.
X-ray luminosity function of Compton-thick AGN in the early Universe (z > 3). Robustness and biases of the CTK population A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 27
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-07-03T11:28:04.823097Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation dee22671-cee4-4f02-bb48-cac604101e28 · inbound
Spatially Resolved Nebular-Stellar Reddening with JWST/NIRISS cites this paper.
Spatially Resolved Nebular-Stellar Reddening with JWST/NIRISS A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 87
- Resolution
- verified exact
- doi, observed 2026-06-27T09:30:46.999780Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 2970e88f-1561-434a-af25-84ef1ba235fd · 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 Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 72
- Resolution
- verified exact
- local_arxiv, observed 2026-06-27T03:30:27.495981Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation ae490598-e2d8-491f-8286-d4f831e2d2b5 · inbound
Dust in the Average Galaxy: Attenuation, Emission, and Opacity from 0<z<7 cites this paper.
Dust in the Average Galaxy: Attenuation, Emission, and Opacity from 0<z<7 A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 31
- Resolution
- metadata mismatch
- doi, observed 2026-06-27T02:30:23.257247Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation f8262c29-3104-4804-ab47-563cc99298fa · 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 Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 120
- Resolution
- verified exact
- local_arxiv, observed 2026-06-27T00:00:16.013544Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation a8d2cedf-fa9a-4957-b6ef-9de4a0410e06 · inbound
The Cosmic Ray Life Cycle in Galaxy Clusters cites this paper.
The Cosmic Ray Life Cycle in Galaxy Clusters A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 102
- Resolution
- verified exact
- doi, observed 2026-06-25T19:48:17.836703Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 3bcf687f-8de5-4629-8aec-fe512c39d1bd · inbound
The multiwavelength structure of post-starburst galaxies at 0.5 < z < 3 with JWST PRIMER: compact morphologies and residual disturbances cites this paper.
The multiwavelength structure of post-starburst galaxies at 0.5 < z < 3 with JWST PRIMER: compact morphologies and residual disturbances A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 39
- Resolution
- verified exact
- doi, observed 2026-07-02T18:27:16.804147Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation e3b8feab-0d4e-4d01-93ac-f91b1b0216eb · inbound
Far-infrared observations of dust in Ly$\alpha$ emitters at z=2-6 cites this paper.
Far-infrared observations of dust in Ly$\alpha$ emitters at z=2-6 A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 24
- Resolution
- verified exact
- local_arxiv, observed 2026-07-02T18:07:15.858729Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 2b38805b-8376-4ec6-9de6-b310e8309320 · inbound
BlackTHUNDER Reveals a Massive Filament around a Compact AGN at $z\simeq5.23$ cites this paper.
BlackTHUNDER Reveals a Massive Filament around a Compact AGN at $z\simeq5.23$ A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 135
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:23:06.110361Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 007b31ba-9ce4-4a66-93e6-f9631146b76d · inbound
The COLIBRE-SKIRT pipeline: Calibration-free dust radiative transfer postprocessing for cosmological simulations cites this paper.
The COLIBRE-SKIRT pipeline: Calibration-free dust radiative transfer postprocessing for cosmological simulations A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 102
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T00:50:15.163717Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 930961ad-20a6-448c-b529-0c42294ed371 · inbound
Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity cites this paper.
Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 104
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T14:10:56.467182Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation dcf082e8-3dd1-42a0-9a3c-43e276d1bd72 · 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 Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 104
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T13:38:30.887540Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d8aa942d-0a8f-4e24-8835-1a232287a387 · inbound
Cosmic CORALS: Timing the Universe with high-z star clusters cites this paper.
Cosmic CORALS: Timing the Universe with high-z star clusters A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 151
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T12:43:57.678336Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 86ca65d3-ce46-46ae-9cbc-d0324e5c0f8c · inbound
Outflows in the Early Universe: Neutral gas Absorption in Galaxies at z > 3 from low-resolution JWST Spectroscopy cites this paper.
Outflows in the Early Universe: Neutral gas Absorption in Galaxies at z > 3 from low-resolution JWST Spectroscopy A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 23
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T09:56:43.074477Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a1edd5c7-638e-4872-84d5-ce2708502fdf · inbound
AT 2022csn: A Photometrically Peculiar Optical/UV Tidal Disruption Event in a Type II AGN cites this paper.
AT 2022csn: A Photometrically Peculiar Optical/UV Tidal Disruption Event in a Type II AGN A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 88
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T00:14:52.074637Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation dd578dfb-4882-4d1c-b281-9f119f5c01a1 · inbound
First Light and Assembly of GalaxieS (FLAGS) I: The JWST/NIRCam Number Counts and IGL as Constraints on Galaxy Formation Models cites this paper.
First Light and Assembly of GalaxieS (FLAGS) I: The JWST/NIRCam Number Counts and IGL as Constraints on Galaxy Formation Models A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 39
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T00:30:25.502497Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4ebaf9d7-a540-4a25-bc0a-8daef1ae31f7 · inbound
Exploring the multi-wavelength properties of the high energetic event ZTF20abbiixp/GRB 200524A: from prompt emission to afterglow cites this paper.
Exploring the multi-wavelength properties of the high energetic event ZTF20abbiixp/GRB 200524A: from prompt emission to afterglow A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 84
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T12:28:16.696965Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 73f37085-73f7-4722-be51-0e349cc16d3a · inbound
FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables cites this paper.
FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables A Simple Model for the Absorption of Starlight by Dust in Galaxies
Reference 38
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T00:14:35.593121Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.