Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud | Paper Citation Record

Observation b0787425-f37b-4964-bb86-46f638a24eff · outbound

This paper cites The Quest for the Missing Dust: II -- Two Orders of Magnitude of Evolution in the Dust-to-Gas Ratio Resolved Within Local Group Galaxies.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud The Quest for the Missing Dust: II -- Two Orders of Magnitude of Evolution in the Dust-to-Gas Ratio Resolved Within Local Group Galaxies

Reference 1

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:48.714863Z

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Observation 29ab10a7-390c-42d2-89b5-d95831e8558b · outbound

This paper cites , archivePrefix = "arXiv", eprint =.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud , archivePrefix = "arXiv", eprint =

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.445000Z

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Observation 5f51a1da-8918-4547-8511-262416e6739f · outbound

This paper cites E(B-V), N(H I) and N(H_2).

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud E(B-V), N(H I) and N(H_2)

Reference 3

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:48.699496Z

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No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 464929cd-09f4-4279-8a94-0edb7c155295 · outbound

This paper cites Planck Early Results: The Planck mission.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Planck Early Results: The Planck mission

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.453682Z

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Observation d049de14-3ee8-4be1-9812-ded76ed490b5 · outbound

This paper cites Common-Resolution Convolution Kernels for Space- and Ground-Based Telescopes.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Common-Resolution Convolution Kernels for Space- and Ground-Based Telescopes

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.457866Z

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Observation e3bdc63d-f2a4-42fc-926a-09b35a1e012d · outbound

This paper cites Spitzer Survey of the Large Magellanic Cloud, Surveying the Agents of a Galaxy's Evolution (SAGE) I: Overview and Initial Results.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Spitzer Survey of the Large Magellanic Cloud, Surveying the Agents of a Galaxy's Evolution (SAGE) I: Overview and Initial Results

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.462070Z

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Observation 3027bdb3-ccef-4ebc-bad3-105fa55b9fe6 · outbound

This paper cites The Polycyclic Aromatic Hydrocarbon Mass Fraction on a 10 pc scale in the Magellanic Clouds.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud The Polycyclic Aromatic Hydrocarbon Mass Fraction on a 10 pc scale in the Magellanic Clouds

Reference 7

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:48.656574Z

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No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation cdd0a8e5-d964-4e1e-9d56-56ae3a2a454e · outbound

This paper cites Astronomical Society of India Conference Series , year = 2010, series =.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Astronomical Society of India Conference Series , year = 2010, series =

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.470624Z

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Observation 65321c19-e0d7-4be8-9be4-472129b553f1 · outbound

This paper cites Dust distributions in the Magellanic Clouds.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Dust distributions in the Magellanic Clouds

Reference 9

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:48.642100Z

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No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 408f93bb-d450-4e22-bbd4-4a546e9388e4 · outbound

This paper cites Scylla I: A pure-parallel, multi-wavelength imaging survey of the ULLYSES fields in the LMC and SMC.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Scylla I: A pure-parallel, multi-wavelength imaging survey of the ULLYSES fields in the LMC and SMC

Reference 10

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:48.626861Z

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No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 6537d19b-2a68-4afa-af21-f14ec2bb055b · outbound

This paper cites Infrared Spaceborne Remote Sensing , year = 1993, editor =.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Infrared Spaceborne Remote Sensing , year = 1993, editor =

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.483655Z

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Observation 3a50272a-6965-4433-9fa8-331ce009d0a1 · outbound

This paper cites , keywords =.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud , keywords =

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.488053Z

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Observation 78d64802-231f-45bc-b88e-544b834468b5 · outbound

This paper cites , keywords =.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud , keywords =

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.492339Z

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Observation e36d8afc-008c-4221-98df-e9c733b948f4 · outbound

This paper cites , keywords =.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud , keywords =

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.496412Z

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Observation cea352a6-c487-4ce0-8da3-dcfee6109eeb · outbound

This paper cites Dust Masses, PAH Abundances, and Starlight Intensities in the SINGS Galaxy Sample.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Dust Masses, PAH Abundances, and Starlight Intensities in the SINGS Galaxy Sample

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.500716Z

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Observation 1a2780d4-437e-4e1a-96b2-6f6b3760ecc8 · outbound

This paper cites Planck intermediate results. XXIX. All-sky dust modelling with Planck, IRAS, and WISE observations.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Planck intermediate results. XXIX. All-sky dust modelling with Planck, IRAS, and WISE observations

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.504951Z

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Observation 98571b3e-6c25-430b-af34-12deb6c154d1 · outbound

This paper cites GASS: The Parkes Galactic All-Sky Survey. I. Survey Description, Goals, and Initial Data Release.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud GASS: The Parkes Galactic All-Sky Survey. I. Survey Description, Goals, and Initial Data Release

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.509350Z

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Observation 54f9c939-6244-4108-8635-d6725dd97854 · outbound

This paper cites The apparent anti-correlation between the mass opacity of interstellar dust and the surface-density of interstellar gas.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud The apparent anti-correlation between the mass opacity of interstellar dust and the surface-density of interstellar gas

Reference 18

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:48.578563Z

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No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation cc3073e9-86a7-4ea6-84c5-a0e4551edaa4 · outbound

This paper cites Dust emissivity in resolved spiral galaxies.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Dust emissivity in resolved spiral galaxies

Reference 19

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:48.562621Z

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No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation d06584a5-290d-4694-a5e4-2705cb710c73 · outbound

This paper cites Dust emissivity and absorption cross section in DustPedia late-type galaxies.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Dust emissivity and absorption cross section in DustPedia late-type galaxies

Reference 20

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:48.547247Z

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No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 1380db02-e5b7-4fe0-8f5e-6ebaaddba0fd · outbound

This paper cites Non-Standard Grain Properties, Dark Gas Reservoir, and Extended Submillimeter Excess, Probed by Herschel in the Large Magellanic Cloud.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Non-Standard Grain Properties, Dark Gas Reservoir, and Extended Submillimeter Excess, Probed by Herschel in the Large Magellanic Cloud

Reference 21

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:48.531751Z

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No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation ba1bc184-25ad-4a24-a717-ad7585fd5e90 · outbound

This paper cites Dust Abundance Variations in the Magellanic Clouds: Probing the Lifecycle of Metals with All-Sky Surveys.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Dust Abundance Variations in the Magellanic Clouds: Probing the Lifecycle of Metals with All-Sky Surveys

Reference 22

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:48.514853Z

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No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 54c1f071-c8e2-4061-b3ca-46155a9d4724 · outbound

This paper cites An Empirical Determination of the Dust Mass Absorption Coefficient, $\kappa_{d}$, Using the Herschel Reference Survey.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud An Empirical Determination of the Dust Mass Absorption Coefficient, $\kappa_{d}$, Using the Herschel Reference Survey

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.535906Z

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Observation f5983285-131d-46e5-91a2-f8ac8d90b96f · outbound

This paper cites The Spatially Resolved Dust-to-Metals Ratio in M101.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud The Spatially Resolved Dust-to-Metals Ratio in M101

Reference 24

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:48.487362Z

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No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation f7c3c548-ed86-4a28-a62f-aba5f1348b8c · outbound

This paper cites The recent LMC-SMC collision: Timing and impact parameter constraints from comparison of Gaia LMC disk kinematics and N-body simulations.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud The recent LMC-SMC collision: Timing and impact parameter constraints from comparison of Gaia LMC disk kinematics and N-body simulations

Reference 25

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:48.472148Z

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No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 16c1091a-5013-4973-a196-2c510e9363ac · outbound

This paper cites A Galactic Eclipse: The Small Magellanic Cloud is Forming Stars in Two, Superimposed Systems.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud A Galactic Eclipse: The Small Magellanic Cloud is Forming Stars in Two, Superimposed Systems

Reference 26

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:48.457805Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 7f14649d-f1a0-465f-b2ea-bc7952058208 · outbound

This paper cites The Quest for the Missing Dust: I -- Restoring Large Scale Emission in Herschel Maps of Local Group Galaxies.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud The Quest for the Missing Dust: I -- Restoring Large Scale Emission in Herschel Maps of Local Group Galaxies

Reference 27

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:48.443851Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation c5f19394-cfa0-4b53-8bf7-aab10d8eadae · outbound

This paper cites The First Maps of $\kappa_{d}$ -- the Dust Mass Absorption Coefficient -- in Nearby Galaxies, with DustPedia.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud The First Maps of $\kappa_{d}$ -- the Dust Mass Absorption Coefficient -- in Nearby Galaxies, with DustPedia

Reference 28

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:48.428398Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation be8dec0f-3722-4555-9e1a-645d1ca12397 · outbound

This paper cites Ashes of FIRE: Modeling Dust Grain Size Evolution in the Local Group with FIRE.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Ashes of FIRE: Modeling Dust Grain Size Evolution in the Local Group with FIRE

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.559750Z

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Observation c47f25f1-5f9c-45c4-9434-c0c037242107 · outbound

This paper cites Dust Grain-Size Distributions From MRN to MEM.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Dust Grain-Size Distributions From MRN to MEM

Reference 30

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:48.402879Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 748615f8-678b-4976-80f4-235b61371561 · outbound

This paper cites Low-temperature MIR to submillimeter mass absorption coefficient of interstellar dust analogues II: Mg and Fe-rich amorphous silicates.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Low-temperature MIR to submillimeter mass absorption coefficient of interstellar dust analogues II: Mg and Fe-rich amorphous silicates

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.568685Z

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Observation d993d840-e87a-4c4c-a96e-e9480a6d077c · outbound

This paper cites Low temperature MIR to submillimeter mass absorption coefficient of interstellar dust analogues I: Mg-rich glassy silicates.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Low temperature MIR to submillimeter mass absorption coefficient of interstellar dust analogues I: Mg-rich glassy silicates

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.572911Z

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Observation dfc12e0f-9a86-4978-90c6-068418bde244 · outbound

This paper cites Scylla VI: Parsec-Scale Dust Extinction Maps in the SMC and LMC.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Scylla VI: Parsec-Scale Dust Extinction Maps in the SMC and LMC

Reference 33

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:48.368405Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation c8479876-3c1f-4f03-a48a-1ee3902ac289 · outbound

This paper cites Scylla IV: Intrinsic Stellar Properties and Line-of-Sight Dust Extinction Measurements Towards 1.5 Million Stars in the SMC and LMC.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Scylla IV: Intrinsic Stellar Properties and Line-of-Sight Dust Extinction Measurements Towards 1.5 Million Stars in the SMC and LMC

Reference 34

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:48.353511Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 9662e24f-944a-4560-a551-3ea67f480cf1 · outbound

This paper cites The Panchromatic Hubble Andromeda Treasury XV. The BEAST: Bayesian Extinction and Stellar Tool.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud The Panchromatic Hubble Andromeda Treasury XV. The BEAST: Bayesian Extinction and Stellar Tool

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.586341Z

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Observation 98bcff46-6ddb-4fdc-827f-20a12d84a94d · outbound

This paper cites Dust and Gas in the Magellanic Clouds from the HERITAGE Herschel Key Project. I. Dust Properties and Insights into the Origin of the Submm Excess Emission.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Dust and Gas in the Magellanic Clouds from the HERITAGE Herschel Key Project. I. Dust Properties and Insights into the Origin of the Submm Excess Emission

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.590436Z

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Observation 0a7c84b3-2ae5-4623-8404-ce21c1de3c90 · outbound

This paper cites Three-Dimensional Structure and Dust Extinction in the Small Magellanic Cloud.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Three-Dimensional Structure and Dust Extinction in the Small Magellanic Cloud

Reference 37

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:48.316715Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation e4a0eb9a-b185-423f-aebd-a44ac9c569b6 · outbound

This paper cites The Panchromatic Hubble Andromeda Treasury VIII: A Wide-Area, High-Resolution Map of Dust Extinction in M31.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud The Panchromatic Hubble Andromeda Treasury VIII: A Wide-Area, High-Resolution Map of Dust Extinction in M31

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.599692Z

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Observation c69bba6a-047f-4631-8e47-82b377c8f0de · outbound

This paper cites Andromeda's Dust.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Andromeda's Dust

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.605482Z

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Observation d1a6d5bb-a94d-44f2-9ba1-82d6f68c9be3 · outbound

This paper cites THEMIS 2.0: A self-consistent model for dust extinction, emission, and polarisation.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud THEMIS 2.0: A self-consistent model for dust extinction, emission, and polarisation

Reference 40

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:48.280738Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 61de65eb-0f94-4d45-acc4-0ffb08e37985 · outbound

This paper cites The global dust modelling framework THEMIS (The Heterogeneous dust Evolution Model for Interstellar Solids).

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud The global dust modelling framework THEMIS (The Heterogeneous dust Evolution Model for Interstellar Solids)

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.614416Z

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Observation a22a9c71-03ad-4b20-ba1e-174968090fb0 · outbound

This paper cites Dust evolution in the transition towards the denser ISM: impact on dust temperature, opacity, and spectral index.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Dust evolution in the transition towards the denser ISM: impact on dust temperature, opacity, and spectral index

Reference 42

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:48.254403Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation d1c5f613-6dfd-45f3-8cc1-93aa23cb813e · outbound

This paper cites From grains to pebbles: the influence of size distribution and chemical composition on dust emission properties.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud From grains to pebbles: the influence of size distribution and chemical composition on dust emission properties

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.622825Z

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Observation 45f8cbb0-8b4d-4aee-9919-a1f63955aa30 · outbound

This paper cites Dust variations in the diffuse interstellar medium: constraints on Milky Way dust from Planck-HFI observations.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Dust variations in the diffuse interstellar medium: constraints on Milky Way dust from Planck-HFI observations

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.627188Z

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Observation 04d9cccd-c08d-4f51-9aed-561c2461f17d · outbound

This paper cites , keywords =.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud , keywords =

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.630769Z

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Observation 4260cf12-1162-4799-b34e-fa90af661c64 · outbound

This paper cites Dust evolution, a global view: IV. Tying up a few loose ends.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Dust evolution, a global view: IV. Tying up a few loose ends

Reference 46

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:47.891277Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 2885b33f-ab63-4ae8-b036-90bab4e293bc · outbound

This paper cites Modeling the Infrared Emission from the HD 141569A Disk.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Modeling the Infrared Emission from the HD 141569A Disk

Reference 47

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:48.218535Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 35cf8861-76ff-440b-9b89-5725f86e97df · outbound

This paper cites Mantle formation, coagulation and the origin of cloud/core shine: I. Modelling dust scattering and absorption in the infra-red.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Mantle formation, coagulation and the origin of cloud/core shine: I. Modelling dust scattering and absorption in the infra-red

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.641442Z

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Observation d0aacf77-e8a0-48fa-a951-8de773e2456e · outbound

This paper cites The optical properties of dust: the effects of composition, size, and structure.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud The optical properties of dust: the effects of composition, size, and structure

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.645592Z

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Unavailable: canonical work link unavailable.

Observation 64fb5035-21c6-4715-9cf1-e198b1283357 · outbound

This paper cites an unresolved cited work.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Unresolved cited work

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.649643Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1eff02c9-5c93-4831-a00a-edf9d71aa5af · outbound

This paper cites , keywords =.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud , keywords =

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.653467Z

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Observation eeb31160-d7dd-4714-996d-4db3883e85ef · outbound

This paper cites The Magellanic Mopra Assessment (MAGMA). I. The Molecular Cloud Population of the Large Magellanic Cloud.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud The Magellanic Mopra Assessment (MAGMA). I. The Molecular Cloud Population of the Large Magellanic Cloud

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.657459Z

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Unavailable: canonical work link unavailable.

Observation 2fe0647e-3b0a-4121-a668-197cfa018767 · outbound

This paper cites The Panchromatic Hubble Andromeda Treasury: Triangulum Extended Region (PHATTER) I. Ultraviolet to Infrared Photometry of 22 Million Stars in M33.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud The Panchromatic Hubble Andromeda Treasury: Triangulum Extended Region (PHATTER) I. Ultraviolet to Infrared Photometry of 22 Million Stars in M33

Reference 53

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:48.173605Z

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No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation c99b8129-2672-405e-bb0a-fb241ef8d211 · outbound

This paper cites The Panchromatic Hubble Andromeda Treasury.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud The Panchromatic Hubble Andromeda Treasury

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.665835Z

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Unavailable: canonical work link unavailable.

Observation bae14564-dd84-4cbc-b1ff-e7e160db0f2c · outbound

This paper cites The Atomic to Molecular Transition in Galaxies. II: HI and H_2 Column Densities.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud The Atomic to Molecular Transition in Galaxies. II: HI and H_2 Column Densities

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.670200Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e9c48965-4189-407c-b7ab-afa607c948f3 · outbound

This paper cites Dust models post-Planck: constraining the far-infrared opacity of dust in the diffuse interstellar medium.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Dust models post-Planck: constraining the far-infrared opacity of dust in the diffuse interstellar medium

Reference 56

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:48.138777Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 1aca5105-4bdc-4805-ad33-edac57c55319 · outbound

This paper cites doi:10.5281/zenodo.21262391 , url =.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud doi:10.5281/zenodo.21262391 , url =

Reference 57

Resolution: verified exact; doi, observed 2026-08-08T15:21:47.864917Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 0444aff3-4b4b-4dc4-9ee2-ecf17c9aa1f1 · outbound

This paper cites Astropy: A Community Python Package for Astronomy.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Astropy: A Community Python Package for Astronomy

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.682065Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0b69029c-c011-4b76-902b-829ba301e47a · outbound

This paper cites The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.686361Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f44b4d9e-3e67-4358-931a-929135b11bf8 · outbound

This paper cites The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.690594Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6b009829-9059-458b-a5ff-d0f4bc64e821 · outbound

This paper cites an unresolved cited work.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Unresolved cited work

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.695267Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 45003b81-3f95-4bb2-bf5d-fc4cd9519da1 · outbound

This paper cites Harris and K.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Harris and K

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.699084Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e16f09d1-b59e-4e5a-82ac-9ba8252bdae0 · outbound

This paper cites , title =.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud , title =

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.703386Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f9e86126-1c47-414c-89fc-133eed32fb51 · outbound

This paper cites an unresolved cited work.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Unresolved cited work

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.707293Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9c155b0e-83ae-4871-921e-ef473c434927 · outbound

This paper cites The Interstellar dust properties of nearby galaxies.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud The Interstellar dust properties of nearby galaxies

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.711445Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 61c119d0-ed88-4527-b61b-ba1e970acdbf · outbound

This paper cites A Quantitative Comparison of SMC, LMC, and Milky Way UV to NIR Extinction Curves.

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.

Observation a0ee1ff7-cfe4-4b3e-8930-a4d1f4a02416 · outbound

This paper cites Modeling dust emission in the Magellanic Clouds with Spitzer and Herschel.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Modeling dust emission in the Magellanic Clouds with Spitzer and Herschel

Reference 67

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:48.070362Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 46ae6a15-441a-4bba-8e0e-97b8f37e0a04 · outbound

This paper cites METAL: The Metal Evolution, Transport, and Abundance in the Large Magellanic Cloud Hubble program. III. Interstellar Depletions, Dust-to-Metal, and Dust-to-Gas Ratios Versus Metallicity.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud METAL: The Metal Evolution, Transport, and Abundance in the Large Magellanic Cloud Hubble program. III. Interstellar Depletions, Dust-to-Metal, and Dust-to-Gas Ratios Versus Metallicity

Reference 68

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:48.054928Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 8671dac1-a9ed-4642-a969-8c8edceca6fb · outbound

This paper cites Dust depletion of of metals from local to distant galaxies II: Cosmic dust-to-metal ratio and dust composition.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Dust depletion of of metals from local to distant galaxies II: Cosmic dust-to-metal ratio and dust composition

Reference 69

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:48.039051Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 79e031d0-d307-4cdc-a7c5-14612469dd14 · outbound

This paper cites Star Formation in the Milky Way and Nearby Galaxies.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Star Formation in the Milky Way and Nearby Galaxies

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.731254Z

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Observation 9e7e1404-59f7-4b88-9011-38c3fb520fd0 · outbound

This paper cites The CO-to-H2 Conversion Factor and Dust-to-Gas Ratio on Kiloparsec Scales in Nearby Galaxies.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud The CO-to-H2 Conversion Factor and Dust-to-Gas Ratio on Kiloparsec Scales in Nearby Galaxies

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.734910Z

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Unavailable: canonical work link unavailable.

Observation eeae77ce-2137-4f29-8dba-9a52e8dfc5b3 · outbound

This paper cites The CO-to-H2 Conversion Factor From Infrared Dust Emission Across the Local Group.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud The CO-to-H2 Conversion Factor From Infrared Dust Emission Across the Local Group

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.739200Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6e90eb5f-b31a-42f5-88bc-203de2d1835e · outbound

This paper cites , year = 1983, month = sep, volume =.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud , year = 1983, month = sep, volume =

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.743288Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0b16c130-9d7e-459a-a64f-cd0d79c13810 · outbound

This paper cites The fraction of bolometric luminosity absorbed by dust in DustPedia galaxies.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud The fraction of bolometric luminosity absorbed by dust in DustPedia galaxies

Reference 74

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:47.989774Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation b0cb5b4c-0feb-44fa-8189-6bd23965efa8 · outbound

This paper cites The bolometric and UV attenuation in normal spiral galaxies of the Herschel Reference Survey.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud The bolometric and UV attenuation in normal spiral galaxies of the Herschel Reference Survey

Reference 75

Resolution: verified exact; local_arxiv, observed 2026-08-08T15:21:47.974287Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 262e5bef-39fd-4f18-869e-a5d2803658cd · outbound

This paper cites The global dust SED: Tracing the nature and evolution of dust with DustEM.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud The global dust SED: Tracing the nature and evolution of dust with DustEM

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.755828Z

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Unavailable: canonical work link unavailable.

Observation 7fab30cc-38d8-4b74-8fc8-377b992e2107 · outbound

This paper cites Extended Red Emission: Photoluminescence by Interstellar Nanoparticles.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Extended Red Emission: Photoluminescence by Interstellar Nanoparticles

Reference 77

Resolution: metadata mismatch; local_arxiv, observed 2026-08-08T15:21:47.845548Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 665c6271-f96e-4905-a6d4-19421b284933 · outbound

This paper cites an unresolved cited work.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Unresolved cited work

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.764304Z

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Unavailable: canonical work link unavailable.

Observation d76f2564-0127-4db9-9448-2ea38d7d1b49 · outbound

This paper cites Disentangling the independently controllable factors of variation by interacting with the world.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud Disentangling the independently controllable factors of variation by interacting with the world

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.768682Z

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Unavailable: canonical work link unavailable.

Observation f2188a34-3647-43ac-bba3-ed3097d6e25a · outbound

This paper cites and Haberland, Matt and Reddy, Tyler and Cournapeau, David and Burovski, Evgeni and Peterson, Pearu and Weckesser, Warren and Bright, Jonathan and.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud and Haberland, Matt and Reddy, Tyler and Cournapeau, David and Burovski, Evgeni and Peterson, Pearu and Weckesser, Warren and Bright, Jonathan and

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.772713Z

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Unavailable: canonical work link unavailable.

Observation 0d6a5768-6b29-4bca-8550-af19294becfd · outbound

This paper cites arXiv e-prints , keywords =.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud arXiv e-prints , keywords =

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.776498Z

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Unavailable: canonical work link unavailable.

Observation c588b702-b764-4218-9c6a-161da1a3bdb2 · outbound

This paper cites doi:10.5281/zenodo.17654855 , url =.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud doi:10.5281/zenodo.17654855 , url =

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.780303Z

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Unavailable: canonical work link unavailable.

Observation a628adf7-9db3-4dcf-ad22-167e52069fd5 · outbound

This paper cites The Effect of Line of Sight Temperature Variation and Noise on Dust Continuum Observations.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud The Effect of Line of Sight Temperature Variation and Noise on Dust Continuum Observations

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.784330Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9414adfb-45e7-4e17-888a-e9e5852a8825 · outbound

This paper cites , keywords =.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud , keywords =

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.788287Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d2f0860f-ddf1-417b-b9c6-83fcc9910fcf · outbound

This paper cites , keywords =.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud , keywords =

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-08T15:21:47.792149Z

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