Stellar parameter determination from photometry using invertible neural networks. Issue 4 (5th November 2020)

• Record Type: Journal Article
• Authors: Ksoll, Victor F; Ardizzone, Lynton; Klessen, Ralf; Koethe, Ullrich; Sabbi, Elena; Robberto, Massimo; Gouliermis, Dimitrios; Rother, Carsten; Zeidler, Peter; Gennaro, Mario
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 499:Issue 4(2020)
• Page Start: 5447
• Page End: 5485
• Publication Date: 2020-11-05
• Subjects: methods: data analysis -- methods: statistical -- stars: formation -- stars: fundamental parameters -- stars: pre-main-sequence -- galaxies: clusters: individual: Westerlund 2, NGC 6397; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/staa2931
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: Photometric surveys with the Hubble Space Telescope ( HST ) allow us to study stellar populations with high-resolution and deep coverage, with estimates of the physical parameters of the constituent stars being typically obtained by comparing the survey data with adequate stellar evolutionary models. This is a highly non-trivial task due to effects such as differential extinction, photometric errors, low filter coverage, or uncertainties in the stellar evolution calculations. These introduce degeneracies that are difficult to detect and break. To improve this situation, we introduce a novel deep learning approach, called conditional invertible neural network (cINN), to solve the inverse problem of predicting physical parameters from photometry on an individual star basis and to obtain the full posterior distributions. We build a carefully curated synthetic training data set derived from the PARSEC stellar evolution models to predict stellar age, initial/current mass, luminosity, effective temperature, and surface gravity. We perform tests on synthetic data from the MIST and Dartmouth models, and benchmark our approach on HST data of two well-studied stellar clusters, Westerlund 2 and NGC 6397. For the synthetic data, we find overall excellent performance, and note that age is the most difficult parameter to constrain. For the benchmark clusters, we retrieve reasonable results and confirm previous findings for Westerlund 2 on cluster age ($1.04_{-0.90}^{+8.48}\, \mathrm{Myr}$ ), mass segregation, and the stellar initial mass function. For NGC 6397, we recover plausible estimates for masses, luminosities, and temperatures, however, discrepancies between stellar evolution models and observations prevent an acceptable recovery of age for old stars.