Prospects for high-precision pulsar timing

By Liu K.   Verbiest J. P. W.   Kramer M.   Stappers B. W.   van Straten W.   Cordes J. M.  

Monthly Notices of the Royal Astronomical Society, Vol. 417, Iss. 4, 2011-11 ,pp. : 2916-2926

Oxford University Press

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A high signal-to-noise ratio map of the Sunyaev–Zel’dovich increment at 1.1-mm wavelength in Abell 1835

By Mauskopf P. D.   Horner P. F.   Aguirre J.   Bock J. J.   Egami E.   Glenn J.   Golwala S. R.   Laurent G.   Nguyen H. T.   Sayers J.  

Monthly Notices of the Royal Astronomical Society, Vol. 421, Iss. 1, 2012-03 ,pp. : 224-234

Oxford University Press

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The optimal schedule for pulsar timing array observations

By Lee K. J.   Bassa C. G.   Janssen G. H.   Karuppusamy R.   Kramer M.   Smits R.   Stappers B. W.  

Monthly Notices of the Royal Astronomical Society, Vol. 423, Iss. 3, 2012-07 ,pp. : 2642-2655

Oxford University Press

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Pulsar timing array observations of gravitational wave source timing parallax

By Deng Xihao   Finn Lee Samuel  

Monthly Notices of the Royal Astronomical Society, Vol. 414, Iss. 1, 2011-06 ,pp. : 50-58

Oxford University Press

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Completeness – II. A signal-to-noise ratio approach for completeness estimators applied to galaxy magnitude–redshift surveys

By Teodoro Luís   Johnston Russell   Hendry Martin  

Monthly Notices of the Royal Astronomical Society, Vol. 405, Iss. 2, 2010-06 ,pp. : 1187-1194

Oxford University Press

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