COMMENTS AND ERRATA |
|
|
|
|
Erratum: Pulsar Timing Residuals Induced by Gravitational Waves from Single Non-evolving Supermassive Black Hole Binaries with Elliptical Orbits [Chin. Phys. Lett. 30 (2013) 100402] |
TONG Ming-Lei1,2**, YAN Bao-Rong1,3, ZHAO Cheng-Shi1,2, YIN Dong-Shang1,2, ZHAO Shu-Hong1,2, YANG Ting-Gao1,2, GAO Yu-Ping1,2 |
1National Time Service Center, Chinese Academy of Sciences, Xi'an 710600 2Key Laboratory of Time and Frequency Primary Standards, Chinese Academy of Sciences, Xi'an 710600 3Key Laboratory of Precision Navigation and Timing Technology, Chinese Academy of Sciences, Xi'an 710600
|
|
Cite this article: |
TONG Ming-Lei, YAN Bao-Rong, ZHAO Cheng-Shi et al 2013 Chin. Phys. Lett. 30 119901 |
|
|
|
|
Received: 18 October 2013
Published: 30 November 2013
|
|
PACS: |
99.10.-x
|
(Errata and other corrections)
|
|
04.30.Db
|
(Wave generation and sources)
|
|
97.60.Gb
|
(Pulsars)
|
|
95.85.Sz
|
(Gravitational radiation, magnetic fields, and other observations)
|
|
|
|
|
|
Viewed |
|
|
|
Full text
|
|
|
|
|
Abstract
|
|
|
|
|