Hostname: page-component-cd9895bd7-mkpzs Total loading time: 0 Render date: 2024-12-26T04:06:18.230Z Has data issue: false hasContentIssue false
  • English
  • Français

Discovery of Five Bright Low-Redshift Quasars from ROSAT PSPC Sources1

Published online by Cambridge University Press:  12 April 2016

Jianyan Wei ,
Li Cao ,
Jiangyao Hu  and
Qibin Li
Jianyan Wei
Affiliation:
Beijing Astronomical Observatory, Chinese Academy of Science, Beijing, 10080, China
Li Cao
Affiliation:
Beijing Astronomical Observatory, Chinese Academy of Science, Beijing, 10080, China
Jiangyao Hu
Affiliation:
Beijing Astronomical Observatory, Chinese Academy of Science, Beijing, 10080, China
Qibin Li
Affiliation:
Beijing Astronomical Observatory, Chinese Academy of Science, Beijing, 10080, China

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

A program to identify bright ROSAT sources is being carried out with the 216-cm and 60-cm telescopes at Xinglong station. As the result of the first run, five bright low-redshift quasars have been discovered.

Type
IX. Surveys and Properties of Active Galaxies and Related Sources
Information
International Astronomical Union Colloquium , Volume 159: Emission Lines in Active Galaxies: New Methods and Techniques , 1997 , pp. 425 - 426
Copyright
Copyright © Astronomical Society of the Pacific 1997

Footnotes

1

This work is supported by the National Natural Science Foundation of China.

References

Véron-Cetty, M.-P., & Véron, P. 1993, ESO Scientific Report, No. 13.Google Scholar
Voges, W. 1992, in Proceedings of the ISY Conference ‘Space Science’, ESA ISY-3, ESA Publications, 9.Google Scholar
Voges, W., et al. 1994, ROSAT NEWS, No.32.Google Scholar