The patent badge is an abbreviated version of the USPTO patent document. The patent badge does contain a link to the full patent document.

The patent badge is an abbreviated version of the USPTO patent document. The patent badge covers the following: Patent number, Date patent was issued, Date patent was filed, Title of the patent, Applicant, Inventor, Assignee, Attorney firm, Primary examiner, Assistant examiner, CPCs, and Abstract. The patent badge does contain a link to the full patent document (in Adobe Acrobat format, aka pdf). To download or print any patent click here.

Date of Patent:
Nov. 28, 2023

Filed:

Jul. 24, 2020
Applicant:

National Astronomical Observatories, Chinese Academy of Sciences, Beijing, CN;

Inventors:

Kefei Wu, Beijing, CN;

Ali Luo, Beijing, CN;

Dongwei Zhao, Beijing, CN;

Xiao Kong, Beijing, CN;

Yongheng Zhao, Beijing, CN;

Attorney:
Primary Examiner:
Int. Cl.
CPC ...
G06F 11/30 (2006.01); G06F 18/2415 (2023.01); G06F 16/182 (2019.01); G06F 16/11 (2019.01); G06Q 50/26 (2012.01);
U.S. Cl.
CPC ...
G06F 18/2415 (2023.01); G06F 16/116 (2019.01); G06F 16/182 (2019.01); G06F 2218/12 (2023.01); G06Q 50/26 (2013.01);
Abstract

The present disclosure provides a method and apparatus for processing astronomical survey data. The method comprises: a data distribution step: delivering a spectral data file to be processed to a distributed file system, dividing the spectral data file into a plurality of data blocks, and distributing the data blocks to computing nodes; a data computing step: performing a spectral classification of spectra to be measured in the data blocks, with a template matching method; the data computing step comprises: reading template spectra, and extracting template universal operators; reading the spectra to be measured; performing spectral matching, and computing Chi-square error values for flow rate values of the template spectra multiplied by the polynomial and flow rate values of the spectra to be measured; and finding corresponding minimum Chi-square error and corresponding redshift for each of the template spectra, so as to determine classifications of the spectra to be measured.


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