Chrome Extension
WeChat Mini Program
Use on ChatGLM

UPdec-Webb: A Data Set for Coaddition of JWST NIRCam Images

Lei Wang,Huanyuan Shan Li-Yan Zhu,Xi Kang

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES(2025)

Chinese Acad Sci | Univ Chinese Acad Sci | Coll Elect Informat & Opt Engn | Zhejiang Univ

Cited 0|Views2
Abstract
We present the application of the image coaddition algorithm, upsampling and point-spread function (PSF) deconvolution coaddition (UPDC), for stacking multiple exposure images captured by the James Webb Space Telescope (JWST) Near-Infrared Camera. By addressing the PSF effect, UPDC provides visually enhanced and sharper images. Furthermore, the antialiasing and superresolution capabilities of UPDC make it easier to deblend sources overlapped on images, yielding a higher accuracy of aperture photometry. We apply this algorithm to the SMACS J0723 imaging data. Comparative analysis with the Drizzle algorithm demonstrates significant improvements in detecting faint sources, achieving accurate photometry, and effectively deblending (superresolution) closely packed sources. As a result, we have newly detected a pair of close binary stars that were previously unresolvable in the original exposures or the Drizzled image. These improvements significantly benefit various scientific projects conducted by JWST. The resulting data set, named “UPdec-Webb,” can be accessed through the official website of the Chinese Virtual Observatory.
More
Translated text
Key words
Deconvolution,High angular resolution,Space observatories,Near infrared astronomy,Galaxy clusters
求助PDF
上传PDF
Bibtex
AI Read Science
AI Summary
AI Summary is the key point extracted automatically understanding the full text of the paper, including the background, methods, results, conclusions, icons and other key content, so that you can get the outline of the paper at a glance.
Example
Background
Key content
Introduction
Methods
Results
Related work
Fund
Key content
  • Pretraining has recently greatly promoted the development of natural language processing (NLP)
  • We show that M6 outperforms the baselines in multimodal downstream tasks, and the large M6 with 10 parameters can reach a better performance
  • We propose a method called M6 that is able to process information of multiple modalities and perform both single-modal and cross-modal understanding and generation
  • The model is scaled to large model with 10 billion parameters with sophisticated deployment, and the 10 -parameter M6-large is the largest pretrained model in Chinese
  • Experimental results show that our proposed M6 outperforms the baseline in a number of downstream tasks concerning both single modality and multiple modalities We will continue the pretraining of extremely large models by increasing data to explore the limit of its performance
Upload PDF to Generate Summary
Must-Reading Tree
Example
Generate MRT to find the research sequence of this paper
Data Disclaimer
The page data are from open Internet sources, cooperative publishers and automatic analysis results through AI technology. We do not make any commitments and guarantees for the validity, accuracy, correctness, reliability, completeness and timeliness of the page data. If you have any questions, please contact us by email: report@aminer.cn
Chat Paper

要点】:本文提出了一种新的图像叠加算法UPDC,用于处理詹姆斯·韦伯太空望远镜近红外相机拍摄的图像,提高了 faint 源的检测能力、测光的准确性和 source deblending 的效率。

方法】:作者采用upsampling和点扩散函数(PSF)反卷积的图像叠加方法(UPDC),通过解决PSF效应来增强图像的视觉效果和锐度。

实验】:作者将UPDC算法应用于SMACS J0723成像数据,并与Drizzle算法进行了比较分析,结果证明了UPDC算法在检测暗弱源、精确测光和有效分解紧密源方面有显著优势,并且新发现了之前无法分辨的一对紧密双星。数据集“UPdec-Webb”可通过中国虚拟天文台官方网站访问。