2.7k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR469 papers
- Université d'OrléansFR412 papers
- Observatoire de ParisFR236 papers
- Max Planck Institute for Radio AstronomyDE174 papers
- University of ManchesterGB160 papers
- Netherlands Institute for Radio AstronomyNL138 papers
- Université Paris Sciences et LettresFR135 papers
- Goddard Space Flight CenterUS121 papers
- Laboratoire d’études spatiales et d’instrumentation en astrophysiqueFR110 papers
- Observatoire Radioastronomique de NançayFR104 papers
- University of California, BerkeleyUS101 papers
- University of AmsterdamNL100 papers
5 papers · 2 filters
Long-term Radio Observations of the Intermittent Pulsar B1931+24
N. J. Young, B. W. Stappers, A. G. Lyne +3
We present an analysis of approximately 13-yr of observations of the intermittent pulsar B1931+24 to further elucidate its behaviour. We find that while the source exhibits a wide…
PSR J1906+0746: From relativistic spin-precession to beam modeling
Gregory Desvignes, Michael Kramer, Ismaël Cognard +4
Shortly after the discovery of PSR J1906+0746, some hints of profile variations were already interpreted as first signs of relativistic spin-precession occuring. Using observations…
SPAN512: A new mid-latitude pulsar survey with the Nancay Radio Telescope
Gregory Desvignes, Ismaël Cognard, David Champion +4
We present an ongoing survey with the Nançay Radio Telescope at L-band. The targeted area is and . This survey is charac…
A possible interpretation for the apparent differences in LFQPO types in microquasars
P. Varniere, M. Tagger, J. Rodriguez
In most microquasars, low-frequency quasi-periodic oscillations (LFQPO) have been classified into three types (A, B and C depending on the peak distribution in the PDS and the shap…
Wide-band Simultaneous Observations of Pulsars: Disentangling Dispersion Measure and Profile Variations
T. E. Hassall, B. W. Stappers, J. W. T. Hessels +91
Dispersion in the interstellar medium is a well known phenomenon that follows a simple relationship, which has been used to predict the time delay of dispersed radio pulses since t…