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2018MNRAS.478..218P - Mon. Not. R. Astron. Soc., 478, 218-227 (2018/July-3)
Improving timing sensitivity in the microhertz frequency regime: limits from PSR J1713+0747 on gravitational waves produced by supermassive black hole binaries.
PERERA B.B.P., STAPPERS B.W., BABAK S., KEITH M.J., ANTONIADIS J., BASSA C.G., CABALLERO R.N., CHAMPION D.J., COGNARD I., DESVIGNES G., GRAIKOU E., GUILLEMOT L., JANSSEN G.H., KARUPPUSAMY R., KRAMER M., LAZARUS P., LENTATI L., LIU K., LYNE A.G., McKEE J.W., OSLOWSKI S., PERRODIN D., SANIDAS S.A., SESANA A., SHAIFULLAH G., THEUREAU G., VERBIEST J.P.W. and TAYLOR S.R.
Abstract (from CDS):
Abstract Copyright: © 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): gravitational waves - binaries: general - stars: black holes - stars: neutron - pulsars: individual: PSR J1713+0747 - quasars: supermassive black holes
Simbad objects: 3
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