Analysing the SEDs of protoplanetary disks with machine learning
arXiv:2302.04629 · doi:10.1051/0004-6361/202245461
Abstract
ABRIDGED. The analysis of spectral energy distributions (SEDs) of protoplanetary disks to determine their physical properties is known to be highly degenerate. Hence, a Bayesian analysis is required to obtain parameter uncertainties and degeneracies. The challenge here is computational speed, as one radiative transfer model requires a couple of minutes to compute. We performed a Bayesian analysis for 30 well-known protoplanetary disks to determine their physical disk properties, including uncertainties and degeneracies. To circumvent the computational cost problem, we created neural networks (NNs) to emulate the SED generation process. We created two sets of radiative transfer disk models to train and test two NNs that predict SEDs for continuous and discontinuous disks. A Bayesian analysis was then performed on 30 protoplanetary disks with SED data collected by the DIANA project to determine the posterior distributions of all parameters. We ran this analysis twice, (i) with old distances and additional parameter constraints as used in a previous study, to compare results, and (ii) with updated distances and free choice of parameters to obtain homogeneous and unbiased model parameters. We evaluated the uncertainties in the determination of physical disk parameters from SED analysis, and detected and quantified the strongest degeneracies. The NNs are able to predict SEDs within 1ms with uncertainties of about 5% compared to the true SEDs obtained by the radiative transfer code. We find parameter values and uncertainties that are significantly different from previous values obtained by fitting. Comparing the global evidence for continuous and discontinuous disks, we find that 26 out of 30 objects are better described by disks that have two distinct radial zones. Also, we created an interactive tool that instantly returns the SED predicted by our NNs for any parameter combination.
40 pages, 22 figures, the online tool is available at https://tillkaeufer.github.io/sedpredictor
References in corpus (10)
- Bayes in the sky: Bayesian inference and model selection in cosmology
- Monte Carlo radiative transfer in protoplanetary disks
- The shape and composition of interstellar silicate grains
- Evolution of emission line activity in intermediate mass young stars
- A Tale of Two Herbig Ae stars -MWC275 and AB Aurigae: Comprehensive Models for SED and Interferometry
- Disks around CQ Tau and MWC 758: dense PDR or gas dispersal?
- Circumstellar disks around Herbig Be stars
- A dust and gas cavity in the disc around CQ Tau revealed by ALMA
- Protoplanetary Disk Masses from Radiative Transfer Modeling: A Case Study in Taurus
- Consistent dust and gas models for protoplanetary disks IV. A panchromatic view of protoplanetary disks