Starduster: A multi-wavelength SED model based on radiative transfer simulations and deep learning. Qiu, Y. & Kang, X. Technical Report December, 2021. Publication Title: arXiv e-prints ADS Bibcode: 2021arXiv211214434Q Type: article![Starduster: A multi-wavelength SED model based on radiative transfer simulations and deep learning [link]](https://bibbase.org/img/filetypes/link.svg "link")
Paper abstract bibtex We present Starduster, a supervised deep learning model that predicts the multi-wavelength SED from galaxy geometry parameters and star formation history by emulating dust radiative transfer simulations. The model is comprised of three specifically designed neural networks, which take into account the features of dust attenuation and emission. We utilise the Skirt radiative transfer simulation to produce data for the training data of neural networks. Each neural network can be trained using \${\textbackslash}sim 4000 - 5000\$ samples. Compared with the direct results of the Skirt simulation, our deep learning model produces \$0.1 - 0.2\$ mag errors in FUV to FIR wavelengths. At some bands, the uncertainty is only \$0.01\$ mag. As an application, we fit our model to the observed SEDs of IC4225 and NGC5166. Our model can reproduce the observations, and successfully predicts that both IC4225 and NGC5166 are edge-on galaxies. However, the predicted geometry parameters are different from image-fitting studies. Our analysis implies that the inconsistency is mainly due to the degeneracy in the star formation history of the stellar disk and bulge. In addition, we find that the predicted fluxes at \$20 {\textbackslash}, {\textbackslash}rm {\textbackslash}mu m - 80 {\textbackslash}, {\textbackslash}rm {\textbackslash}mu m\$ by our SED model are correlated with bulge radius. Our SED code is public available and can be applied to both SED-fitting and SED-modelling of galaxies from semi-analytic models.
@techreport{qiu_starduster_2021,
title = {Starduster: {A} multi-wavelength {SED} model based on radiative transfer simulations and deep learning},
shorttitle = {Starduster},
url = {https://ui.adsabs.harvard.edu/abs/2021arXiv211214434Q},
abstract = {We present Starduster, a supervised deep learning model that predicts the multi-wavelength SED from galaxy geometry parameters and star formation history by emulating dust radiative transfer simulations. The model is comprised of three specifically designed neural networks, which take into account the features of dust attenuation and emission. We utilise the Skirt radiative transfer simulation to produce data for the training data of neural networks. Each neural network can be trained using \${\textbackslash}sim 4000 - 5000\$ samples. Compared with the direct results of the Skirt simulation, our deep learning model produces \$0.1 - 0.2\$ mag errors in FUV to FIR wavelengths. At some bands, the uncertainty is only \$0.01\$ mag. As an application, we fit our model to the observed SEDs of IC4225 and NGC5166. Our model can reproduce the observations, and successfully predicts that both IC4225 and NGC5166 are edge-on galaxies. However, the predicted geometry parameters are different from image-fitting studies. Our analysis implies that the inconsistency is mainly due to the degeneracy in the star formation history of the stellar disk and bulge. In addition, we find that the predicted fluxes at \$20 {\textbackslash}, {\textbackslash}rm {\textbackslash}mu m - 80 {\textbackslash}, {\textbackslash}rm {\textbackslash}mu m\$ by our SED model are correlated with bulge radius. Our SED code is public available and can be applied to both SED-fitting and SED-modelling of galaxies from semi-analytic models.},
urldate = {2022-01-05},
author = {Qiu, Yisheng and Kang, Xi},
month = dec,
year = {2021},
note = {Publication Title: arXiv e-prints
ADS Bibcode: 2021arXiv211214434Q
Type: article},
keywords = {Astrophysics - Astrophysics of Galaxies},
}
Downloads: 0
{"_id":"Z4zcZSXurK89neNPB","bibbaseid":"qiu-kang-stardusteramultiwavelengthsedmodelbasedonradiativetransfersimulationsanddeeplearning-2021","author_short":["Qiu, Y.","Kang, X."],"bibdata":{"bibtype":"techreport","type":"techreport","title":"Starduster: A multi-wavelength SED model based on radiative transfer simulations and deep learning","shorttitle":"Starduster","url":"https://ui.adsabs.harvard.edu/abs/2021arXiv211214434Q","abstract":"We present Starduster, a supervised deep learning model that predicts the multi-wavelength SED from galaxy geometry parameters and star formation history by emulating dust radiative transfer simulations. The model is comprised of three specifically designed neural networks, which take into account the features of dust attenuation and emission. We utilise the Skirt radiative transfer simulation to produce data for the training data of neural networks. Each neural network can be trained using \\${\\textbackslash}sim 4000 - 5000\\$ samples. Compared with the direct results of the Skirt simulation, our deep learning model produces \\$0.1 - 0.2\\$ mag errors in FUV to FIR wavelengths. At some bands, the uncertainty is only \\$0.01\\$ mag. As an application, we fit our model to the observed SEDs of IC4225 and NGC5166. Our model can reproduce the observations, and successfully predicts that both IC4225 and NGC5166 are edge-on galaxies. However, the predicted geometry parameters are different from image-fitting studies. Our analysis implies that the inconsistency is mainly due to the degeneracy in the star formation history of the stellar disk and bulge. In addition, we find that the predicted fluxes at \\$20 {\\textbackslash}, {\\textbackslash}rm {\\textbackslash}mu m - 80 {\\textbackslash}, {\\textbackslash}rm {\\textbackslash}mu m\\$ by our SED model are correlated with bulge radius. Our SED code is public available and can be applied to both SED-fitting and SED-modelling of galaxies from semi-analytic models.","urldate":"2022-01-05","author":[{"propositions":[],"lastnames":["Qiu"],"firstnames":["Yisheng"],"suffixes":[]},{"propositions":[],"lastnames":["Kang"],"firstnames":["Xi"],"suffixes":[]}],"month":"December","year":"2021","note":"Publication Title: arXiv e-prints ADS Bibcode: 2021arXiv211214434Q Type: article","keywords":"Astrophysics - Astrophysics of Galaxies","bibtex":"@techreport{qiu_starduster_2021,\n\ttitle = {Starduster: {A} multi-wavelength {SED} model based on radiative transfer simulations and deep learning},\n\tshorttitle = {Starduster},\n\turl = {https://ui.adsabs.harvard.edu/abs/2021arXiv211214434Q},\n\tabstract = {We present Starduster, a supervised deep learning model that predicts the multi-wavelength SED from galaxy geometry parameters and star formation history by emulating dust radiative transfer simulations. The model is comprised of three specifically designed neural networks, which take into account the features of dust attenuation and emission. We utilise the Skirt radiative transfer simulation to produce data for the training data of neural networks. Each neural network can be trained using \\${\\textbackslash}sim 4000 - 5000\\$ samples. Compared with the direct results of the Skirt simulation, our deep learning model produces \\$0.1 - 0.2\\$ mag errors in FUV to FIR wavelengths. At some bands, the uncertainty is only \\$0.01\\$ mag. As an application, we fit our model to the observed SEDs of IC4225 and NGC5166. Our model can reproduce the observations, and successfully predicts that both IC4225 and NGC5166 are edge-on galaxies. However, the predicted geometry parameters are different from image-fitting studies. Our analysis implies that the inconsistency is mainly due to the degeneracy in the star formation history of the stellar disk and bulge. In addition, we find that the predicted fluxes at \\$20 {\\textbackslash}, {\\textbackslash}rm {\\textbackslash}mu m - 80 {\\textbackslash}, {\\textbackslash}rm {\\textbackslash}mu m\\$ by our SED model are correlated with bulge radius. Our SED code is public available and can be applied to both SED-fitting and SED-modelling of galaxies from semi-analytic models.},\n\turldate = {2022-01-05},\n\tauthor = {Qiu, Yisheng and Kang, Xi},\n\tmonth = dec,\n\tyear = {2021},\n\tnote = {Publication Title: arXiv e-prints\nADS Bibcode: 2021arXiv211214434Q\nType: article},\n\tkeywords = {Astrophysics - Astrophysics of Galaxies},\n}\n\n","author_short":["Qiu, Y.","Kang, X."],"key":"qiu_starduster_2021","id":"qiu_starduster_2021","bibbaseid":"qiu-kang-stardusteramultiwavelengthsedmodelbasedonradiativetransfersimulationsanddeeplearning-2021","role":"author","urls":{"Paper":"https://ui.adsabs.harvard.edu/abs/2021arXiv211214434Q"},"keyword":["Astrophysics - Astrophysics of Galaxies"],"metadata":{"authorlinks":{}}},"bibtype":"techreport","biburl":"https://bibbase.org/zotero/polyphant","dataSources":["7gvjSdWrEu7z5vjjj"],"keywords":["astrophysics - astrophysics of galaxies"],"search_terms":["starduster","multi","wavelength","sed","model","based","radiative","transfer","simulations","deep","learning","qiu","kang"],"title":"Starduster: A multi-wavelength SED model based on radiative transfer simulations and deep learning","year":2021}