Handbook Of Pulsar Astronomy

By Sabine Fenstermacher. 2016

608 citations recorded by the source corpus.

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

Fast radio bursts at the dawn of the 2020s (2021, unknown): “As a phenomenon, FRBs are characterised as short-duration (sub-second), relatively broad-band pulses which exhibit the frequency-dependent arrival time delay due to dispersion that is well known for Galactic radio pulsars (see, e.g. Lorimer and Kramer 2012).”
Coherent emission mechanisms in astrophysical plasmas (2017, background): “The third coherent emission mechanism is involved in pulsar radio emission, which is extremely bright, TB ≈ 10(25)–10(30)K (Lorimer and Kramer, 2004), but the specific mechanism remains uncertain.”
Testing Relativistic Gravity with Radio Pulsars (2014, background): “We will not go into the details of pulsar observations and pulsar timing here, since there are numerous excellent reviews on these topics, for instance [25, 26], just to mention two.”
Common-red-signal analysis with 24-yr high-precision timing of the European Pulsar Timing Array: Inferences in the stochastic gravitational-wave background search (2021, methodology): “…MSPs have been particularly useful is gravity (e.g. Taylor 1993; Kramer et al. 2006; Will 2014), especially by employing the ‘pulsar timing’ technique (e.g. Lorimer & Kramer 2005), which relies on high-precision measurements of the pulses’ times-of-arrival (TOAs) being compared to a ‘timing model’.”