International audienceFrequency metrology outperforms any other branch of metrology in accuracy (parts in 10^−16) and small fluctuations (<10^−17). In turn, among celestial bodies, the rotation speed of millisecond pulsars is by far the most stable (<10^−18). Therefore, the precise measurement of the time of arrival (TOA) of pulsar signals is expected to disclose information about cosmological phenomena, and to enlarge our astrophysical knowledge. Related to this topic, Pulsar Timing Array projects have been developed and operated for the last decades. The TOAs from a pulsar can be affected by local emission and environmental effects, in the direction of the propagation through the interstellar medium or universally by gravitational waves f...
International audienceIn this paper, we describe the International Pulsar Timing Array second data r...
International audienceIn this paper, we describe the International Pulsar Timing Array second data r...
International audienceThe sensitivity of Pulsar Timing Arrays to gravitational waves (GWs) depends o...
International audienceFrequency metrology outperforms any other branch of metrology in accuracy (par...
International audienceFrequency metrology outperforms any other branch of metrology in accuracy (par...
International audienceFrequency metrology outperforms any other branch of metrology in accuracy (par...
Millisecond and binary pulsars are the most stable astronomical standards of frequency. They can be ...
Astronomers use pulsars as astronomical clocks to perform physical tests, such as in testing Einstei...
We aim to construct a Galactic-scale detector comprised of an array of pulsars distributed across th...
The sensitivity of Pulsar Timing Arrays to gravitational waves (GWs) depends on the noise present in...
International audienceIn this paper, we describe the International Pulsar Timing Array second data r...
International audienceIn this paper, we describe the International Pulsar Timing Array second data r...
International audienceIn this paper, we describe the International Pulsar Timing Array second data r...
The sensitivity of Pulsar Timing Arrays to gravitational waves (GWs) depends on the noise present in...
International audienceThe sensitivity of Pulsar Timing Arrays to gravitational waves (GWs) depends o...
International audienceIn this paper, we describe the International Pulsar Timing Array second data r...
International audienceIn this paper, we describe the International Pulsar Timing Array second data r...
International audienceThe sensitivity of Pulsar Timing Arrays to gravitational waves (GWs) depends o...
International audienceFrequency metrology outperforms any other branch of metrology in accuracy (par...
International audienceFrequency metrology outperforms any other branch of metrology in accuracy (par...
International audienceFrequency metrology outperforms any other branch of metrology in accuracy (par...
Millisecond and binary pulsars are the most stable astronomical standards of frequency. They can be ...
Astronomers use pulsars as astronomical clocks to perform physical tests, such as in testing Einstei...
We aim to construct a Galactic-scale detector comprised of an array of pulsars distributed across th...
The sensitivity of Pulsar Timing Arrays to gravitational waves (GWs) depends on the noise present in...
International audienceIn this paper, we describe the International Pulsar Timing Array second data r...
International audienceIn this paper, we describe the International Pulsar Timing Array second data r...
International audienceIn this paper, we describe the International Pulsar Timing Array second data r...
The sensitivity of Pulsar Timing Arrays to gravitational waves (GWs) depends on the noise present in...
International audienceThe sensitivity of Pulsar Timing Arrays to gravitational waves (GWs) depends o...
International audienceIn this paper, we describe the International Pulsar Timing Array second data r...
International audienceIn this paper, we describe the International Pulsar Timing Array second data r...
International audienceThe sensitivity of Pulsar Timing Arrays to gravitational waves (GWs) depends o...