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The DIRTY Model. I. Monte Carlo Radiative Transfer through Dust

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What this work says

Outgoing claims: the papers this work cites, builds on, or argues with.

inferredcites →https://doi.org/10.1007/978-94-009-0605-1_12openalex-snapshot
Perception of Interstellar Structure: Facing Complexity
inferredcites →https://doi.org/10.1016/b978-012498660-2/50028-8openalex-snapshot
Concepts, Terms, Notation
inferredcites →https://doi.org/10.1046/j.1365-8711.2000.03113.xopenalex-snapshot
Effects of clumping on the observed properties of dusty galaxies
inferredcites →https://doi.org/10.1046/j.1365-8711.2000.03177.xopenalex-snapshot
A generic scattering model for AGN
inferredcites →https://doi.org/10.1086/118572openalex-snapshot
Modeling Polarization Maps of External Galaxies.
inferredcites →https://doi.org/10.1086/160360openalex-snapshot
The scattering phase function of interstellar grains - The case of the reflection nebula NGC 7023
inferredcites →https://doi.org/10.1086/161780openalex-snapshot
Bipolar reflection nebulae - Monte Carlo simulations
inferredcites →https://doi.org/10.1086/171530openalex-snapshot
Dust and the transfer of stellar radiation within galaxies
inferredcites →https://doi.org/10.1086/171673openalex-snapshot
Model scattering envelopes of young stellar objects. I - Method and application to circumstellar disks
inferredcites →https://doi.org/10.1086/173714openalex-snapshot
The size distribution of interstellar dust particles as determined from extinction
inferredcites →https://doi.org/10.1086/174602openalex-snapshot
The far-ultraviolet dust albedo in the Upper Scorpius subgroup of the Scorpius OB2 association
inferredcites →https://doi.org/10.1086/175303openalex-snapshot
Global Models of the Interstellar Medium in Disk Galaxies
inferredcites →https://doi.org/10.1086/175363openalex-snapshot
Polarization from scattering in blobs
inferredcites →https://doi.org/10.1086/177282openalex-snapshot
Multiple Scattering in Clumpy Media. I. Escape of Stellar Radiation from a Clumpy Scattering Environment
inferredcites →https://doi.org/10.1086/177407openalex-snapshot
Monte Carlo Simulations of Dusty Spiral Galaxies: Extinction and Polarization Properties
inferredcites →https://doi.org/10.1086/187939openalex-snapshot
Scattering Properties of the Dust in the Reflection Nebula IC 435
inferredcites →https://doi.org/10.1086/190463openalex-snapshot
Multiple scattering in reflection nebulae. I - A Monte Carlo approach. II - Uniform plane-parallel nebulae with foreground stars. III - Nebulae with embedded illuminating stars
inferredcites →https://doi.org/10.1086/300287openalex-snapshot
Attenuation Effects in Spiral Galaxies: Multiwavelength Photometry and Disk Radiative Transfer Models
inferredcites →https://doi.org/10.1086/304654openalex-snapshot
Dust in Starburst Galaxies
inferredcites →https://doi.org/10.1086/305449openalex-snapshot
Optical and Near‐Infrared Model Images of the Circumstellar Environments of Classical T Tauri Stars
inferredcites →https://doi.org/10.1086/306476openalex-snapshot
Modeling the Effects of Dust on Galactic Spectral Energy Distributions from the Ultraviolet to the Millimeter Band
inferredcites →https://doi.org/10.1086/307350openalex-snapshot
The Dusty Starburst Nucleus of M33
inferredcites →https://doi.org/10.1086/307729openalex-snapshot
Analytical Approximations for Calculating the Escape and Absorption of Radiation in Clumpy Dusty Environments
inferredcites →https://doi.org/10.1086/307939openalex-snapshot
A Model for the Scattered Light Contribution and Polarization of the Diffuse Hα Galactic Background
inferredcites →https://doi.org/10.1086/308197openalex-snapshot
Multiple Scattering in Clumpy Media. II. Galactic Environments
inferredcites →https://doi.org/10.1086/308668openalex-snapshot
The Flux Ratio Method for Determining the Dust Attenuation of Starburst Galaxies
inferredcites →https://doi.org/10.1086/312042openalex-snapshot
The Ever-changing Circumstellar Nebula around UW Centauri
inferredcites →https://doi.org/10.1086/313373openalex-snapshot
The Spectral Signature of Dust Scattering and Polarization in the Near‐Infrared to Far‐Ultraviolet. I. Optical Depth and Geometry Effects
inferredcites →https://doi.org/10.1086/320083openalex-snapshot
The DIRTY Model. II. Self‐consistent Treatment of Dust Heating and Emission in a Three‐dimensional Radiative Transfer Code

What points at this work

Incoming claims: where this work appears in other papers’ reference lists and arguments.

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HERschel Observations of Edge-on Spirals (HEROES)
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TRUST
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Dust Heating by the Interstellar Radiation Field in Models of Turbulent Molecular Clouds
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REBELS-IFU: dust attenuation curves of 12 massive galaxies at z ≃ 7
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dart-ray: a 3D ray-tracing radiative transfer code for calculating the propagation of light in dusty galaxies
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Dust energy balance study of two edge-on spiral galaxies in the Herschel-ATLAS survey
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Bayesian modelling of uncertainties of Monte Carlo radiative-transfer simulations
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Lyman radiative transfer in a multiphase medium
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Modelling galaxy spectra in presence of interstellar dust - II. From the ultraviolet to the far-infrared
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SUNRISE: polychromatic dust radiative transfer in arbitrary geometries
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High-resolution panchromatic spectral models of galaxies including photoionization and dust
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Radiative transfer in disc galaxies - IV. The effects of dust attenuation on bulge and disc structural parameters
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3D radiative transfer modelling of the dusty tori around active galactic nuclei as a clumpy two-phase medium
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Star Formation in the Milky Way and Nearby Galaxies
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Understanding Galaxy Evolution Through Emission Lines
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Three-Dimensional Dust Radiative Transfer
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Spectral Energy Density in an Axisymmetric Galaxy as Predicted by an Analytical Model for the Maxwell Field
inferred← citeshttps://doi.org/10.1364/oe.563393openalex-snapshot
FDTD-based Monte Carlo method for the simulation of optical transport in complex scattering media
inferred← citeshttps://doi.org/10.1515/phys-2022-0253openalex-snapshot
Interstellar radiation as a Maxwell field: Improved numerical scheme and application to the spectral energy density
inferred← citeshttps://doi.org/10.3390/galaxies14010003openalex-snapshot
Probing the Dusty Torus of Seyfert Galaxy NGC 4151: A Multi-Band Study
inferred← citeshttps://doi.org/10.3390/s26165053openalex-snapshot
Numeric Analysis of Polarized Lidar Contrast Enhancement Across Diverse Targets in Fog
inferred← citeshttps://doi.org/10.3847/0004-637x/818/1/62openalex-snapshot
WHAT SHAPES THE FAR-INFRARED SPECTRAL ENERGY DISTRIBUTIONS OF GALAXIES?
inferred← citeshttps://doi.org/10.3847/0004-637x/827/1/20openalex-snapshot
BREAKING THE CURVE WITH CANDELS: A BAYESIAN APPROACH TO REVEAL THE NON-UNIVERSALITY OF THE DUST-ATTENUATION LAW AT HIGH REDSHIFT
inferred← citeshttps://doi.org/10.3847/1538-4357/833/2/201openalex-snapshot
RADIATIVE TRANSFER MODEL OF DUST ATTENUATION CURVES IN CLUMPY, GALACTIC ENVIRONMENTS
inferred← citeshttps://doi.org/10.3847/1538-4357/aa5ffeopenalex-snapshot
Deriving Physical Properties from Broadband Photometry with Prospector: Description of the Model and a Demonstration of its Accuracy Using 129 Galaxies in the Local Universe
inferred← citeshttps://doi.org/10.3847/1538-4357/aa76dcopenalex-snapshot
A Controlled Study of Cold Dust Content in Galaxies from z = 0–2
inferred← citeshttps://doi.org/10.3847/1538-4357/aa844dopenalex-snapshot
High-energy Gamma Rays from the Milky Way: Three-dimensional Spatial Models for the Cosmic-Ray and Radiation Field Densities in the Interstellar Medium
inferred← citeshttps://doi.org/10.3847/1538-4357/aac824openalex-snapshot
The Failure of Monte Carlo Radiative Transfer at Medium to High Optical Depths
inferred← citeshttps://doi.org/10.3847/1538-4357/aacd06openalex-snapshot
Polarization as a Probe of Thick Dust Disks in Edge-on Galaxies: Application to NGC 891
inferred← citeshttps://doi.org/10.3847/1538-4357/ab16edopenalex-snapshot
Theoretical ISM Pressure and Electron Density Diagnostics for Local and High-redshift Galaxies
inferred← citeshttps://doi.org/10.3847/1538-4357/ab3664openalex-snapshot
Radiative Transfer with POLARIS. II. Modeling of Synthetic Galactic Synchrotron Observations
inferred← citeshttps://doi.org/10.3847/1538-4357/ac1427openalex-snapshot
DirtyGrid II: An Analysis of the Dust and Stellar Properties in Nearby Star-forming Galaxies
inferred← citeshttps://doi.org/10.3847/1538-4357/ac25f3openalex-snapshot
On the Impact of Inclination-dependent Attenuation on Derived Star Formation Histories: Results from Disk Galaxies in the Great Observatories Origins Deep Survey Fields
inferred← citeshttps://doi.org/10.3847/1538-4357/ac6be5openalex-snapshot
The Effects of Circumstellar Dust Scattering on the Light Curves and Polarizations of Type Ia Supernovae*
inferred← citeshttps://doi.org/10.3847/1538-4357/ac8793openalex-snapshot
Modeling the Hα and He 10830 Transmission Spectrum of WASP-52b
inferred← citeshttps://doi.org/10.3847/1538-4357/ad58bdopenalex-snapshot
On the Doublet Flux Ratio of Mg ii Resonance Lines in and Around Galaxies
inferred← citeshttps://doi.org/10.3847/1538-4357/adc802openalex-snapshot
A Shock Crashing into Confined Dense Circumstellar Matter Brightens the Nascent SN 2023ixf
inferred← citeshttps://doi.org/10.3847/1538-4365/aabf41openalex-snapshot
DirtyGrid I: 3D Dust Radiative Transfer Modeling of Spectral Energy Distributions of Dusty Stellar Populations
inferred← citeshttps://doi.org/10.3847/1538-4365/ab94c3openalex-snapshot
A Monte Carlo Implementation of Galactic Free–Free Emission for the EoR Foreground Models
inferred← citeshttps://doi.org/10.3847/1538-4365/abc487openalex-snapshot
powderday: Dust Radiative Transfer for Galaxy Simulations
inferred← citeshttps://doi.org/10.5303/jkas.2015.48.1.57openalex-snapshot
MONTE-CARLO RADIATIVE TRANSFER MODEL OF THE DIFFUSE GALACTIC LIGHT
inferred← citeshttps://doi.org/10.5303/pkas.2010.25.4.113openalex-snapshot
COMPARISON OF TWO SCATTERING PHASE FUNCTIONS IN MULTIPLE SCATTERING ENVIRONMENT
inferred← citeshttps://doi.org/10.5303/pkas.2010.25.4.177openalex-snapshot
AN EFFICIENT MONTE-CARLO ALGORITHM FOR DUST-SCATTERING STUDY
inferred← citeshttps://doi.org/10.70675/e9205734z3daez4dcaza15fze11edcb6ea4dopenalex-snapshot
Measuring black hole masses in active galactic nuclei using the polarization of broad emission lines
inferred← citeshttps://doi.org/10.70675/f562e2a0ze007z4809zaf23z85902171c447openalex-snapshot
Quenching in galaxy formation : mechanisms and signatures
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