Stellar parameter determination from photometry using invertible neural networks

• Verfasst von: Ksoll, Victor F. [VerfasserIn]
• Verfasst von: Ardizzone, Lynton [VerfasserIn]
• Verfasst von: Klessen, Ralf S. [VerfasserIn]
• Verfasst von: Köthe, Ullrich [VerfasserIn]
• Verfasst von: Sabbi, Elena [VerfasserIn]
• Verfasst von: Robberto, Massimo [VerfasserIn]
• Verfasst von: Gouliermis, Dimitrios A. [VerfasserIn]
• Verfasst von: Rother, Carsten [VerfasserIn]
• Verfasst von: Zeidler, Peter [VerfasserIn]
• Verfasst von: Gennaro, Mario [VerfasserIn]
• Titel: Stellar parameter determination from photometry using invertible neural networks
• Verf.angabe: Victor F. Ksoll, Lynton Ardizzone, Ralf Klessen, Ullrich Koethe, Elena Sabbi, Massimo Robberto, Dimitrios Gouliermis, Carsten Rother, Peter Zeidler and Mario Gennaro
• E-Jahr: 2020
• Jahr: 05 November 2020
• Umfang: 39 S.
• Fussnoten: Gesehen am 02.03.2022
• Titel Quelle: Enthalten in: Royal Astronomical SocietyMonthly notices of the Royal Astronomical Society
• Ort Quelle: Oxford : Oxford Univ. Press, 1827
• Jahr Quelle: 2020
• Band/Heft Quelle: 499(2020), 4, Seite 5447-5485
• ISSN Quelle: 1365-2966
• DOI: doi:10.1093/mnras/staa2931
• Datenträger: Online-Ressource
• Sprache: eng
• K10plus-PPN: 1789060419

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.