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A deep learning approach for the 3D reconstruction of dust density and temperature in star-forming regions
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dc.contributor.author | Ksoll, Victor F. | |
dc.contributor.author | Reissl, Stefan | |
dc.contributor.author | Klessen, Ralf S. | |
dc.contributor.author | Stephens, Ian W. | |
dc.contributor.author | Smith, Rowan J. | |
dc.contributor.author | Soler, Juan D. | |
dc.contributor.author | Traficante, Alessio | |
dc.contributor.author | Girichidis, Philipp | |
dc.contributor.author | Testi, Leonardo | |
dc.contributor.author | Hennebelle, Patrick | |
dc.contributor.author | Molinari, Sergio | |
dc.date.accessioned | 2024-05-03T13:30:03Z | |
dc.date.available | 2024-05-03T13:30:03Z | |
dc.date.issued | 2024-03 | |
dc.identifier | 298578022 | |
dc.identifier | 5cc97365-5ae6-4c49-9bba-db4a6802c090 | |
dc.identifier | 85189436373 | |
dc.identifier.citation | Ksoll , V F , Reissl , S , Klessen , R S , Stephens , I W , Smith , R J , Soler , J D , Traficante , A , Girichidis , P , Testi , L , Hennebelle , P & Molinari , S 2024 , ' A deep learning approach for the 3D reconstruction of dust density and temperature in star-forming regions ' , Astronomy & Astrophysics , vol. 683 , A246 . https://doi.org/10.1051/0004-6361/202347758 | en |
dc.identifier.issn | 0004-6361 | |
dc.identifier.other | ArXiv: http://arxiv.org/abs/2308.09657v1 | |
dc.identifier.uri | https://hdl.handle.net/10023/29804 | |
dc.description | Funding: The team in Heidelberg acknowledges funding from the European Research Council via the ERC Synergy Grant “ECOGAL” (project ID 855130), from the German Excellence Strategy via the Heidelberg Cluster of Excellence (EXC 2181 - 390900948) “STRUCTURES”, and from the German Ministry for Economic Affairs and Climate Action in project “MAINN” (funding ID 50OO2206). They also thank for computing resources provided by The Länd and DFG through grant INST 35/1134-1 FUGG and for data storage at SDS@hd through grant INST 35/1314-1 FUGG. | en |
dc.description.abstract | Aims. We introduce a new deep learning approach for the reconstruction of 3D dust density and temperature distributions from multi-wavelength dust emission observations on the scale of individual star-forming cloud cores (< 0.2 pc). Methods. We construct a training data set by processing cloud cores from the Cloud Factory simulations with the POLARIS radiative transfer code to produce synthetic dust emission observations at 23 wavelengths between 12 and 1300 µm. We simplify the task by reconstructing the cloud structure along individual lines of sight and train a conditional invertible neural network (cINN) for this purpose. The cINN belongs to the group of normalising flow methods and is able to predict full posterior distributions for the target dust properties. We test different cINN setups, ranging from a scenario that includes all 23 wavelengths down to a more realistically limited case with observations at only seven wavelengths. We evaluate the predictive performance of these models on synthetic test data. Results. We report an excellent reconstruction performance for the 23-wavelengths cINN model, achieving median absolute relative errors of about 1.8% in log(ndust/m−3) and 1% in log(Tdust/K), respectively. We identify trends towards overestimation at the low end of the density range and towards underestimation at the high end of both density and temperature, which may be related to a bias in the training data. Limiting coverage to a combination of only seven wavelengths, we still find a satisfactory performance with average absolute relative errors of about 3.3% and 2.5% in log(ndust/m−3) and log(Tdust/K). Conclusions. This proof of concept study shows that the cINN-based approach for 3D reconstruction of dust density and temperature is very promising and even feasible under realistic observational constraints. | |
dc.format.extent | 38 | |
dc.format.extent | 28958061 | |
dc.language.iso | eng | |
dc.relation.ispartof | Astronomy & Astrophysics | en |
dc.subject | Methods: statistical | en |
dc.subject | (ISM:) dust, extinction | en |
dc.subject | Stars: formation | en |
dc.subject | QB Astronomy | en |
dc.subject | DAS | en |
dc.subject.lcc | QB | en |
dc.title | A deep learning approach for the 3D reconstruction of dust density and temperature in star-forming regions | en |
dc.type | Journal article | en |
dc.contributor.institution | University of St Andrews. School of Physics and Astronomy | en |
dc.identifier.doi | https://doi.org/10.1051/0004-6361/202347758 | |
dc.description.status | Peer reviewed | en |
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