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Estimating The Redshift Error In Supernova Data Analysis_Code Supplement

Name: Estimating The Redshift Error In Supernova Data Analysis_Code Supplement
Creator: Seoul Science Highschool
Published: 2017-11-03T00:00:00+08:00

Zenodo2017-11-03 更新2026-04-07 收录

超新星红移误差估计

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数据链接：

https://zenodo.org/record/1041027 数据链接链接失效反馈

官方服务：

资源简介：

Supplement for 'Estimating the redshift error in supernova data analysis'

应用场景：

提供机构：

Seoul Science Highschool

创建时间：

2017-11-03

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CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observation

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Chandra X-ray Observatory Stack acisfJ1206091p493434_001

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Chandra X-ray Observatory Stack acisfJ2135450m233221_001

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Data at Redshift=1.2 (RD0024). In Santa Fe Light Cone Simulation research project files

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The parameter files are plain text, and can be accessed using a text editor or web browser. The complete snapshot is contained in an archive file in the tar file format. Within the archive, the parame

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Chandra X-ray Observatory Stack acisfJ0956291p694145_001

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