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]

doi:10.1088/0256-307X/30/11/119901

Chin. Phys. Lett.

2013, Vol. 30

Issue (11): 119901 DOI: 10.1088/0256-307X/30/11/119901

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-Lei^1,2**, YAN Bao-Rong^1,3, ZHAO Cheng-Shi^1,2, YIN Dong-Shang^1,2, ZHAO Shu-Hong^1,2, YANG Ting-Gao^1,2, GAO Yu-Ping^1,2

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

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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)

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	TONG Ming-Lei
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	ZHAO Shu-Hong
	YANG Ting-Gao
	GAO Yu-Ping

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