A dust attenuation model inspired by the NIHAO-SKIRT-Catalog
Fuente:
arXiv
Guardado en:
| Autores principales: | Faucher, Nicholas, Blanton, Michael R. |
|---|---|
| Formato: | Preprint |
| Publicado: |
2024
|
| Materias: | |
| Acceso en línea: | |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
Ejemplares similares
Testing the accuracy of SED modeling techniques using the NIHAO-SKIRT-Catalog
por: Faucher, Nicholas, et al.
Publicado: (2024)
por: Faucher, Nicholas, et al.
Publicado: (2024)
The TNG50-SKIRT Atlas: wavelength dependence of the effective radius
por: Baes, Maarten, et al.
Publicado: (2024)
por: Baes, Maarten, et al.
Publicado: (2024)
The TNG50-SKIRT Atlas: Multi-wavelength nonparametric galaxy morphology
por: Tulu, Sena Bokona, et al.
Publicado: (2026)
por: Tulu, Sena Bokona, et al.
Publicado: (2026)
The TNG50-SKIRT Atlas: post-processing methodology and first data release
por: Baes, Maarten, et al.
Publicado: (2024)
por: Baes, Maarten, et al.
Publicado: (2024)
NIHAO-RiNG: A Comparison of Simulated Disc Galaxies from GASOLINE and GIZMO
por: Chen, Hou-Zun, et al.
Publicado: (2023)
por: Chen, Hou-Zun, et al.
Publicado: (2023)
Further correction to the STARFORGE methods paper: Planck-mean dust opacities
por: Grudić, Michael Y., et al.
Publicado: (2025)
por: Grudić, Michael Y., et al.
Publicado: (2025)
Finding accreted stars in the Milky Way: clues from NIHAO simulations
por: Buder, Sven, et al.
Publicado: (2024)
por: Buder, Sven, et al.
Publicado: (2024)
Radio AGN Activity in Low Redshift Galaxies is Not Directly Related to Star Formation Rates
por: Suresh, Arjun, et al.
Publicado: (2024)
por: Suresh, Arjun, et al.
Publicado: (2024)
Mid-Infrared Variability in Nearby Galaxies from the MaNGA Sample
por: Pai, Aashay, et al.
Publicado: (2024)
por: Pai, Aashay, et al.
Publicado: (2024)
AGN Feedback Models and AGN Demographics I: Radio-Mode AGN in EAGLE, SIMBA and TNG100 are Inconsistent with Observations
por: Suresh, Arjun, et al.
Publicado: (2025)
por: Suresh, Arjun, et al.
Publicado: (2025)
Local variations of the radial metallicity gradient in a simulated NIHAO-UHD Milky Way analogue and their implications for (extra-)galactic studies
por: Buder, Sven, et al.
Publicado: (2024)
por: Buder, Sven, et al.
Publicado: (2024)
The chemodynamical memory of a major merger in a NIHAO-UHD Milky Way analogue I: A golden thread through time and space
por: Buder, Sven, et al.
Publicado: (2025)
por: Buder, Sven, et al.
Publicado: (2025)
Quaia, the Gaia-unWISE Quasar Catalog: An All-Sky Spectroscopic Quasar Sample
por: Storey-Fisher, Kate, et al.
Publicado: (2023)
por: Storey-Fisher, Kate, et al.
Publicado: (2023)
Relating spatially resolved optical attenuation, dust and gas in nearby galaxies
por: Paspaliaris, E. D., et al.
Publicado: (2025)
por: Paspaliaris, E. D., et al.
Publicado: (2025)
A first empirical derivation of the average dust attenuation law at 2<z<7
por: Rodighiero, Giulia, et al.
Publicado: (2026)
por: Rodighiero, Giulia, et al.
Publicado: (2026)
Learning the Universe: physically-motivated priors for dust attenuation curves
por: Sommovigo, Laura, et al.
Publicado: (2025)
por: Sommovigo, Laura, et al.
Publicado: (2025)
The chemodynamical memory of a major merger in a NIHAO-UHD Milky Way analogue II: Were Splash stars heated or already born hot?
por: Buder, Sven, et al.
Publicado: (2025)
por: Buder, Sven, et al.
Publicado: (2025)
Evolution of galaxy attenuation curves driven by evolving dust mass and grain size distributions
por: Matsumoto, Kosei, et al.
Publicado: (2025)
por: Matsumoto, Kosei, et al.
Publicado: (2025)
Unveiling the trends between dust attenuation and galaxy properties at z ~ 2 - 12 with the James Webb Space Telescope
por: Markov, V., et al.
Publicado: (2025)
por: Markov, V., et al.
Publicado: (2025)
The Eddington Ratio Distribution of Narrow Line Active Galactic Nuclei
por: Blanton, Michael R., et al.
Publicado: (2025)
por: Blanton, Michael R., et al.
Publicado: (2025)
The ALPINE-CRISTAL-JWST Survey: Stellar and nebular dust attenuation of main-sequence galaxies at z~4-6
por: Tsujita, Akiyoshi, et al.
Publicado: (2025)
por: Tsujita, Akiyoshi, et al.
Publicado: (2025)
Evolution of dust attenuation in star-forming galaxies with UV slope, stellar mass, and redshift out to $z \sim 5$
por: Wijesekera, J. V., et al.
Publicado: (2026)
por: Wijesekera, J. V., et al.
Publicado: (2026)
Assessing differences between local galaxy dust attenuation and point source extinction within the same environments
por: Duarte, J., et al.
Publicado: (2025)
por: Duarte, J., et al.
Publicado: (2025)
A Turbulent Framework for Star Formation in High-Redshift Galaxies
por: Sun, Guochao, et al.
Publicado: (2025)
por: Sun, Guochao, et al.
Publicado: (2025)
A$^3$COSMOS: Measuring the cosmic dust-attenuated star formation rate density at $4 < z < 5$
por: Magnelli, Benjamin, et al.
Publicado: (2024)
por: Magnelli, Benjamin, et al.
Publicado: (2024)
Is cosmic dust porous?
por: Potapov, Alexey, et al.
Publicado: (2025)
por: Potapov, Alexey, et al.
Publicado: (2025)
Using dust to constrain dark matter models
por: Ussing, Adam, et al.
Publicado: (2024)
por: Ussing, Adam, et al.
Publicado: (2024)
Estimating Dust Attenuation From Galactic Spectra. III. Radial variations of dust attenuation scaling relations in MaNGA galaxies
por: Li, Niu, et al.
Publicado: (2024)
por: Li, Niu, et al.
Publicado: (2024)
The SPHINX public data release. II. Using low-ionisation absorption lines and dust attenuation to predict Lyman continuum escape
por: Mauerhofer, Valentin, et al.
Publicado: (2026)
por: Mauerhofer, Valentin, et al.
Publicado: (2026)
Extinction curves, extinction laws, and the failure of interstellar dust models
por: Zagury, Frederic
Publicado: (2026)
por: Zagury, Frederic
Publicado: (2026)
STARFORGE: Toward a comprehensive numerical model of star cluster formation and feedback
por: Grudić, Michael Y., et al.
Publicado: (2020)
por: Grudić, Michael Y., et al.
Publicado: (2020)
SpyDust: an improved and extended implementation for modeling spinning dust radiation
por: Zhang, Zheng, et al.
Publicado: (2024)
por: Zhang, Zheng, et al.
Publicado: (2024)
THEMIS 2.0: A self-consistent model for dust extinction, emission, and polarisation
por: Ysard, Nathalie, et al.
Publicado: (2024)
por: Ysard, Nathalie, et al.
Publicado: (2024)
MUSE observations of the giant low surface brightness galaxy Malin 1: Numerous HII regions, star formation rate, metallicity, and dust attenuation
por: Junais, et al.
Publicado: (2023)
por: Junais, et al.
Publicado: (2023)
A$^3$COSMOS: the dust mass function and dust mass density at $0.5<z<6$
por: Traina, A., et al.
Publicado: (2024)
por: Traina, A., et al.
Publicado: (2024)
The GECKOS survey: Jeans anisotropic models of edge-on discs uncover the impact of dust and kinematic structures
por: Rutherford, T. H., et al.
Publicado: (2025)
por: Rutherford, T. H., et al.
Publicado: (2025)
$Ab$ $initio$ modeling of Galactic dust polarized CMB foreground
por: Kritsuk, Alexei G., et al.
Publicado: (2026)
por: Kritsuk, Alexei G., et al.
Publicado: (2026)
ALMA observations of super-early galaxies: attenuation-free model predictions
por: Ferrara, A., et al.
Publicado: (2024)
por: Ferrara, A., et al.
Publicado: (2024)
Interstellar dust production, destruction and effects of dust depletion in galaxies
por: Calura, Francesco
Publicado: (2025)
por: Calura, Francesco
Publicado: (2025)
Stretch to stretch, dust to dust: lower-value local $H_{0}$ measurement from two-population modelling of type Ia supernovae
por: Wojtak, Radosław, et al.
Publicado: (2025)
por: Wojtak, Radosław, et al.
Publicado: (2025)
Ejemplares similares
-
Testing the accuracy of SED modeling techniques using the NIHAO-SKIRT-Catalog
por: Faucher, Nicholas, et al.
Publicado: (2024) -
The TNG50-SKIRT Atlas: wavelength dependence of the effective radius
por: Baes, Maarten, et al.
Publicado: (2024) -
The TNG50-SKIRT Atlas: Multi-wavelength nonparametric galaxy morphology
por: Tulu, Sena Bokona, et al.
Publicado: (2026) -
The TNG50-SKIRT Atlas: post-processing methodology and first data release
por: Baes, Maarten, et al.
Publicado: (2024) -
NIHAO-RiNG: A Comparison of Simulated Disc Galaxies from GASOLINE and GIZMO
por: Chen, Hou-Zun, et al.
Publicado: (2023)