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2016MNRAS.457.4421C - Mon. Not. R. Astron. Soc., 457, 4421-4440 (2016/April-3)
The noise properties of 42 millisecond pulsars from the European Pulsar Timing Array and their impact on gravitational-wave searches.
CABALLERO R.N., LEE K.J., LENTATI L., DESVIGNES G., CHAMPION D.J., VERBIEST J.P.W., JANSSEN G.H., STAPPERS B.W., KRAMER M., LAZARUS P., POSSENTI A., TIBURZI C., PERRODIN D., OSLOWSKI S., BABAK S., BASSA C.G., BREM P., BURGAY M., COGNARD I., GAIR J.R., GRAIKOU E., GUILLEMOT L., HESSELS J.W.T., KARUPPUSAMY R., LASSUS A., LIU K., McKEE J., MINGARELLI C.M.F., PETITEAU A., PURVER M.B., ROSADO P.A., SANIDAS S., SESANA A., SHAIFULLAH G., SMITS R., TAYLOR S.R., THEUREAU G., VAN HAASTEREN R. and VECCHIO A.
Abstract (from CDS):
Abstract Copyright: © 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): gravitational waves - methods: data analysis - pulsars: general
Simbad objects: 42
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