Disentangling stellar atmospheric parameters in astronomical spectra using generative adversarial neural networks

IF 5.8 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Astronomy & Astrophysics Pub Date : 2025-02-25 DOI:10.1051/0004-6361/202451786
M. Manteiga, R. Santoveña, M. A. Álvarez, C. Dafonte, M. G. Penedo, S. Navarro, L. Corral
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Abstract

Context. The rapid expansion of large-scale spectroscopic surveys has highlighted the need to use automatic methods to extract information about the properties of stars with the greatest efficiency and accuracy, and also to optimise the use of computational resources.Aims. We developed a method based on generative adversarial networks (GANs) to disentangle the physical (effective temperature and gravity) and chemical (metallicity and overabundance of α elements with respect to iron) atmospheric properties in astronomical spectra. Using a projection of the stellar spectra, commonly called latent space, in which the contribution due to one or several main stellar physicochemical properties is minimised while others are enhanced, it was possible to maximise the information related to certain properties. This could then be extracted using artificial neural networks (ANNs) as regressors, with a higher accuracy than a reference method based on the use of ANNs that had been trained with the original spectra.Methods. Our model utilises auto-encoders, comprising two ANNs: an encoder and a decoder that transform input data into a low-dimensional representation known as latent space. It also uses discriminators, which are additional neural networks aimed at transforming the traditional auto-encoder training into an adversarial approach. This is done to reinforce the astrophysical parameters or disentangle them from the latent space. We describe our Generative Adversarial Networks for Disentangling and Learning Framework (GANDALF) tool in this article. It was developed to define, train, and test our GAN model with a web framework to show visually how the disentangling algorithm works. It is open to the community in Github.Results. We demonstrate the performance of our approach for retrieving atmospheric stellar properties from spectra using Gaia Radial Velocity Spectrograph (RVS) data from DR3. We used a data-driven perspective and obtained very competitive values, all within the literature errors, and with the advantage of an important dimensionality reduction of the data to be processed.
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用生成对抗神经网络解纠缠天文光谱中的恒星大气参数
上下文。大规模光谱调查的迅速扩展突出了使用自动方法以最高的效率和准确性提取有关恒星特性的信息,并优化计算资源的使用的必要性。我们开发了一种基于生成对抗网络(gan)的方法来解开天文光谱中的物理(有效温度和重力)和化学(金属丰度和相对于铁的α元素过剩)大气特性。利用恒星光谱的投影,通常称为潜在空间,其中一个或几个主要的恒星物理化学性质的贡献被最小化,而其他的被增强,有可能最大化与某些性质有关的信息。然后可以使用人工神经网络(ann)作为回归量提取,其精度高于基于使用原始光谱训练的ann的参考方法。我们的模型使用自编码器,包括两个人工神经网络:一个编码器和一个解码器,将输入数据转换为称为潜在空间的低维表示。它还使用了鉴别器,这是一种额外的神经网络,旨在将传统的自编码器训练转变为对抗方法。这样做是为了加强天体物理参数或将它们从潜在空间中解脱出来。我们在这篇文章中描述了我们的生成对抗网络解纠缠和学习框架(GANDALF)工具。它是用来定义、训练和测试我们的GAN模型的web框架,以直观地展示解缠算法是如何工作的。它在Github.Results中向社区开放。我们利用来自DR3的Gaia径向速度光谱仪(RVS)数据证明了我们的方法从光谱中检索大气恒星特性的性能。我们使用了数据驱动的视角,并获得了非常有竞争力的价值,所有这些都在文献误差范围内,并且具有重要的要处理的数据降维的优势。
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来源期刊
Astronomy & Astrophysics
Astronomy & Astrophysics 地学天文-天文与天体物理
CiteScore
10.20
自引率
27.70%
发文量
2105
审稿时长
1-2 weeks
期刊介绍: Astronomy & Astrophysics is an international Journal that publishes papers on all aspects of astronomy and astrophysics (theoretical, observational, and instrumental) independently of the techniques used to obtain the results.
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