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Table · dataset · 2025

Attributes of DESI DR9 spiral galaxies

Listed in IVOA Registry (Virtual Observatory)

The gas-phase metallicity is a crucial parameter for understanding the evolution of galaxies.

Description

Considering that the number of multi-band galaxy images can typically reach tens of millions, using these images as input data for predicting gas-phase metallicity has become a feasible method. However, the accuracy of metallicity estimates from images is relatively limited.

To solve this problem, we propose Galaxy Parameter Measurement Residual Network (GPM-ResNet), a deep learning method designed to predict gas-phase metallicity from photometric images of DESI. The parameter of photometric images are labeled with gas-phase metallicity values, which are obtained through spectroscopic methods with high accuracy. These labeled images serve as the training dataset for the GPM-ResNet method.

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GPM-ResNet mainly consists of two modules: a multi-order feature extractor and a parameter generator, enhancing the ability to effectively extract features related to gas-phase metallicity from photometric images. The {sigma} of Zpred-Ztrue is 0.12dex, which significantly outperforms the predicted results of the second-order polynomial ({sigma}=0.16dex) and the third-order polynomial ({sigma}=0.16dex) fitted using the color-metallicity relation on the same dataset.

To further emphasize the superiority of GPM-ResNet, we analyze the predicted results on various network architectures, galaxy sizes, image resolutions, and wavelength bands of images. Moreover, we explore the Mass-Metallicity relation and recover the relation successfully by utilizing the predicted values Zpred. Finally, we apply GPM-ResNet to predict the gas-phase metallicity of spiral (EXP) galaxies observed by DESI, resulting in a comprehensive catalog containing 5095815 data.

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IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/a+a/694/a27113 d agoJSON v1
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