• 文献检索
  • 文档翻译
  • 深度研究
  • 学术资讯
  • Suppr Zotero 插件Zotero 插件
  • 邀请有礼
  • 套餐&价格
  • 历史记录
应用&插件
Suppr Zotero 插件Zotero 插件浏览器插件Mac 客户端Windows 客户端微信小程序
定价
高级版会员购买积分包购买API积分包
服务
文献检索文档翻译深度研究API 文档MCP 服务
关于我们
关于 Suppr公司介绍联系我们用户协议隐私条款
关注我们

Suppr 超能文献

核心技术专利:CN118964589B侵权必究
粤ICP备2023148730 号-1Suppr @ 2026

文献检索

告别复杂PubMed语法,用中文像聊天一样搜索,搜遍4000万医学文献。AI智能推荐,让科研检索更轻松。

立即免费搜索

文件翻译

保留排版,准确专业,支持PDF/Word/PPT等文件格式,支持 12+语言互译。

免费翻译文档

深度研究

AI帮你快速写综述,25分钟生成高质量综述,智能提取关键信息,辅助科研写作。

立即免费体验

[Density estimation based model matching method for redshift determination].

作者信息

Duan Fu-qing, Wu Fu-chao, Luo A-li, Zhao Yong-heng

机构信息

National Laboratory of Pattern Recognition, Institute of Automation, Chinese Academy of Sciences, Beijing 100080, China.

出版信息

Guang Pu Xue Yu Guang Pu Fen Xi. 2005 Nov;25(11):1895-8.

PMID:16499074
Abstract

The present paper proposes a model matching method based on density estimation for redshift determination, in whichthe problem of redshift determination is translated into the problem of searching for the point of maximum density within a data set. At first, the mean shift-based method for auto-extraction of spectral lines is used to get feature spectrallines. Secondly, according tothe redshift formula, the authors use the feature wavelength array and the spectral template to get a data set. Finally, the authors findthe point of maximum density within the data set, then the average of the data in epsilon-neighbor of the point is regarded as the redshift estimation. The information of feature wavelength and spectral line type is used in this method so that it can deal with every kind of spectra. Experiments show that our method is stable and the correct identification rate is high.

摘要

相似文献

1
[Density estimation based model matching method for redshift determination].
Guang Pu Xue Yu Guang Pu Fen Xi. 2005 Nov;25(11):1895-8.
2
[Redshift estimation of galaxy spectra based on similarity measure].基于相似性度量的星系光谱红移估计
Guang Pu Xue Yu Guang Pu Fen Xi. 2008 Jan;28(1):235-8.
3
[Mean shift based auto-extraction of spectral lines for non-emission-line objects].
Guang Pu Xue Yu Guang Pu Fen Xi. 2005 Nov;25(11):1884-8.
4
[A novel method to determine the redshifts of active galaxies based on wavelet transform].一种基于小波变换确定活动星系红移的新方法
Guang Pu Xue Yu Guang Pu Fen Xi. 2012 Oct;32(10):2858-62.
5
[An auto-extraction method of spectral line for normal galaxy spectra].[一种正常星系光谱谱线的自动提取方法]
Guang Pu Xue Yu Guang Pu Fen Xi. 2006 Mar;26(3):583-6.
6
[A method for automatic recognition of stellar spectra based on feature matching of spectral lines].一种基于谱线特征匹配的恒星光谱自动识别方法
Guang Pu Xue Yu Guang Pu Fen Xi. 2008 Jun;28(6):1435-8.
7
[An automated measurement of the galaxies spectra of LAMOST].[郭守敬望远镜星系光谱的自动测量]
Guang Pu Xue Yu Guang Pu Fen Xi. 2005 Jun;25(6):1002-5.
8
[A method for auto-extraction of spectral lines based on convolution type of wavelet packet transformation].
Guang Pu Xue Yu Guang Pu Fen Xi. 2006 Feb;26(2):372-6.
9
[A new automatic quasars recognition technique based on PCA and Hough transform].
Guang Pu Xue Yu Guang Pu Fen Xi. 2003 Feb;23(1):187-91.
10
[A method for redshift determination of quasars based on cross correlation].一种基于互相关的类星体红移测定方法
Guang Pu Xue Yu Guang Pu Fen Xi. 2005 Jul;25(7):1155-7.