George B. Hobbs

TEMPO2: a new pulsar timing package III: gravitational wave simulation (2009)

Hobbs, George B., Jenet, Frederick A., Lee, K. J., Verbiest, J. P. W., Yardley, D., Manchester, Richard N., ...

Analysis of pulsar timing data sets may provide the first direct detection of gravitational waves. This paper. the third in a series describing the mathematical framework implemented into the TEMPO2...

Gravitational-wave detection using pulsars: status of the Parkes Pulsar Timing Array project (2009)

Hobbs, George B., Bailes, M., Bhat, N. D. R., Burke-Spolaor, S., Champion, David J., Coles, William A., ...

The first direct detection of gravitational waves may be made through observations of pulsars. The principal aim of pulsar timing-array projects being carried out worldwide is to detect ultra-low...

TEMPO2: a new pulsar timing package III: gravitational wave simulation (2009)

Hobbs, George B., Jenet, Frederick A., Lee, K. J., Verbiest, J. P. W., Yardley, D., Manchester, Richard N., ...

Analysis of pulsar timing data sets may provide the first direct detection of gravitational waves. This paper. the third in a series describing the mathematical framework implemented into the TEMPO2...

Gravitational-wave detection using pulsars: status of the Parkes Pulsar Timing Array project (2009)

Hobbs, George B., Bailes, M., Bhat, N. D. R., Burke-Spolaor, S., Champion, David J., Coles, William A., ...

The first direct detection of gravitational waves may be made through observations of pulsars. The principal aim of pulsar timing-array projects being carried out worldwide is to detect ultra-low...

Precision timing of PSR J0437-4715: an accurate pulsar distance, a high pulsar mass, and a limit on the variation of Newton's gravitational constant (2008)

Verbiest, Joris P. W., Bailes, Matthew, Van Straten, Willem H., Hobbs, George B., Edwards, Russell T., Manchester, Richard N., ...

Analysis of 10 years of high-precision timing data on the millisecond pulsar PSR J0437-4715 has resulted in a model-independent kinematic distance based on an apparent orbital period derivative, Pb,...

Precision timing of PSR J0437-4715: an accurate pulsar distance, a high pulsar mass, and a limit on the variation of Newton's gravitational constant (2008)

Verbiest, Joris P. W., Bailes, Matthew, Van Straten, Willem H., Hobbs, George B., Edwards, Russell T., Manchester, Richard N., ...

Analysis of 10 years of high-precision timing data on the millisecond pulsar PSR J0437-4715 has resulted in a model-independent kinematic distance based on an apparent orbital period derivative, Pb,...

Precision timing of PSR J0437-4715: an accurate pulsar distance, a high pulsar mass, and a limit on the variation of Newton's gravitational constant (2008)

Verbiest, Joris P. W., Bailes, Matthew, Van Straten, Willem H., Hobbs, George B., Edwards, Russell T., Manchester, Richard N., ...

Analysis of 10 years of high-precision timing data on the millisecond pulsar PSR J0437-4715 has resulted in a model-independent kinematic distance based on an apparent orbital period derivative, Pb,...

Science with ASKAP: the Australian square-kilometre-array pathfinder (2008)

Johnston, Simon, Bailes, Matthew, Bartel, Norbert, Baugh, Carlton, Bietenholz, Michael F., Blake, Chris, ...

The future of cm and m-wave astronomy lies with the Square Kilometre Array (SKA), a telescope under development by a consortium of 17 countries. The SKA will be 50 times more sensitive than any...

Science with ASKAP: the Australian square-kilometre-array pathfinder (2008)

Johnston, Simon, Bailes, Matthew, Bartel, Norbert, Baugh, Carlton, Bietenholz, Michael F., Blake, Chris, ...

The future of cm and m-wave astronomy lies with the Square Kilometre Array (SKA), a telescope under development by a consortium of 17 countries. The SKA will be 50 times more sensitive than any...

Using pulsars to limit the existence of a gravitational wave background (2008)

Hobbs, George B., Jenet, Fredrick A., Lommen, A., Coles, W., Verbiest, J. P. W., Manchester, Richard N.

Gravitational waves passing the Earth induce signals in pulsar timing residuals that are potentially detectable using modern pulsar timing observations. It has been predicted that merging...

PSR J1410-6132: a young, energetic pulsar associated with the EGRET source 3EG J1410-6147 (2008)

O'Brien, J. T., Johnston, S., Kramer, M., Lyne, A. G., Bailes, M., Possenti, A., ...

We present the discovery of PSR J1410−6132, a 50-ms pulsar found during a high-frequency survey of the Galactic plane, using a seven-beam 6.3-GHz receiver on the 64-m Parkes radio telescope....

Precision timing of PSR J0437-4715: an accurate pulsar distance, a high pulsar mass, and a limit on the variation of Newton's gravitational constant (2008)

Verbiest, Joris P. W., Bailes, Matthew, Van Straten, W., Hobbs, George B., Edwards, Russell T., Manchester, Richard N., ...

Analysis of 10 years of high-precision timing data on the millisecond pulsar PSR J0437-4715 has resulted in a model-independent kinematic distance based on an apparent orbital period derivative, Pb,...

Science with ASKAP: the Australian square-kilometre-array pathfinder (2008)

Johnston, Simon, Bailes, Matthew, Bartel, Norbert, Baugh, Carlton, Bietenholz, Michael F., Blake, Chris, ...

The future of cm and m-wave astronomy lies with the Square Kilometre Array (SKA), a telescope under development by a consortium of 17 countries. The SKA will be 50 times more sensitive than any...

Using pulsars to limit the existence of a gravitational wave background (2008)

Hobbs, George B., Jenet, Fredrick A., Lommen, A., Coles, W., Verbiest, J. P. W., Manchester, Richard N.

Gravitational waves passing the Earth induce signals in pulsar timing residuals that are potentially detectable using modern pulsar timing observations. It has been predicted that merging...

PSR J1410-6132: a young, energetic pulsar associated with the EGRET source 3EG J1410-6147 (2008)

O'Brien, J. T., Johnston, S., Kramer, M., Lyne, A. G., Bailes, M., Possenti, A., ...

We present the discovery of PSR J1410−6132, a 50-ms pulsar found during a high-frequency survey of the Galactic plane, using a seven-beam 6.3-GHz receiver on the 64-m Parkes radio telescope. The...

Science with the Australian Square Kilometre Array Pathfinder (2007)

Johnston, Simon, Bailes, Matthew, Bartel, Norbert, Baugh, Carlton, Bietenholz, Michael F., Blake, Chris, ...

The future of centimetre and metre-wave astronomy lies with the Square Kilometre Array (SKA), a telescope under development by a consortium of 17 countries that will be 50 times more sensitive than...

Science with the Australian Square Kilometre Array Pathfinder (2007)

Johnston, Simon, Bailes, Matthew, Bartel, Norbert, Baugh, Carlton, Bietenholz, Michael F., Blake, Chris, ...

The future of centimetre and metre-wave astronomy lies with the Square Kilometre Array (SKA), a telescope under development by a consortium of 17 countries that will be 50 times more sensitive than...

Science with the Australian Square Kilometre Array Pathfinder (2007)

Johnston, Simon, Bailes, Matthew, Bartel, Norbert, Baugh, Carlton, Bietenholz, Michael F., Blake, Chris, ...

The future of centimetre and metre-wave astronomy lies with the Square Kilometre Array (SKA), a telescope under development by a consortium of 17 countries that will be 50 times more sensitive than...

Science with the Australian Square Kilometre Array Pathfinder (2007)

Johnston, Simon, Bailes, Matthew, Bartel, Norbert, Baugh, Carlton, Bietenholz, Michael F., Blake, Chris, ...

The future of centimetre and metre-wave astronomy lies with the Square Kilometre Array (SKA), a telescope under development by a consortium of 17 countries that will be 50 times more sensitive than...

Science with the Australian Square Kilometre Array Pathfinder (2007)

Johnston, Simon, Bailes, Matthew, Bartel, Norbert, Baugh, Carlton, Bietenholz, Michael F., Blake, Chris, ...

The future of centimetre and metre-wave astronomy lies with the Square Kilometre Array (SKA), a telescope under development by a consortium of 17 countries that will be 50 times more sensitive than...

Arecibo and the ALFA pulsar survey (2006)

Van Leeuwen, Joeri, Cordes, James M., Lorimer, Duncan R., Freire, Paulo C., Camilo, Fernando, Stairs, Ingrid H., ...

The recently started Arecibo L-band Feed Array (ALFA) pulsar survey aims to find ~1000 new pulsars. Due to its high time and frequency resolution the survey is especially sensitive to millisecond...

Arecibo and the ALFA pulsar survey (2006)

Van Leeuwen, Joeri, Cordes, James M., Lorimer, Duncan R., Freire, Paulo C., Camilo, Fernando, Stairs, Ingrid H., ...

The recently started Arecibo L-band Feed Array (ALFA) pulsar survey aims to find ~1000 new pulsars. Due to its high time and frequency resolution the survey is especially sensitive to millisecond...

Arecibo and the ALFA pulsar survey (2006)

Van Leeuwen, Joeri, Cordes, James M., Lorimer, Duncan R., Freire, Paulo C., Camilo, Fernando, Stairs, Ingrid H., ...

The recently started Arecibo L-band Feed Array (ALFA) pulsar survey aims to find ~1000 new pulsars. Due to its high time and frequency resolution the survey is especially sensitive to millisecond...

Arecibo and the ALFA pulsar survey (2006)

Van Leeuwen, Joeri, Cordes, James M., Lorimer, Duncan R., Freire, Paulo C., Camilo, Fernando, Stairs, Ingrid H., ...

The recently started Arecibo L-band Feed Array (ALFA) pulsar survey aims to find ~1000 new pulsars. Due to its high time and frequency resolution the survey is especially sensitive to millisecond...

Arecibo and the ALFA pulsar survey (2006)

Van Leeuwen, Joeri, Cordes, James M., Lorimer, Duncan R., Freire, Paulo C., Camilo, Fernando, Stairs, Ingrid H., ...

The recently started Arecibo L-band Feed Array (ALFA) pulsar survey aims to find ~1000 new pulsars. Due to its high time and frequency resolution the survey is especially sensitive to millisecond...

Arecibo and the ALFA pulsar survey (2006)

Van Leeuwen, Joeri, Cordes, James M., Lorimer, Duncan R., Freire, Paulo C., Camilo, Fernando, Stairs, Ingrid H., ...

The recently started Arecibo L-band Feed Array (ALFA) pulsar survey aims to find ~1000 new pulsars. Due to its high time and frequency resolution the survey is especially sensitive to millisecond...

Detecting the stochastic gravitational wave background using pulsar timing (2005)

Jenet, Fredrick A., Hobbs, George B., Lee, K. J., Manchester, Richard N.

The direct detection of gravitational waves is a major goal of current astrophysics. We provide details of a new method for detecting a stochastic background of gravitational waves using pulsar...