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The Green Bank North Celestial Cap Survey IX: Timing Follow-up for 128 Pulsars
A. E. McEwen, J. K. Swiggum, D. L. Kaplan +27
The Green Bank North Celestial Cap survey is one of the largest and most sensitive searches for pulsars and transient radio objects. Observations for the survey have finished; prio…
Topology of Pulsar Profiles (ToPP). I. Graph theory method and classification of the EPN
D. Vohl, J. van Leeuwen, Y. Maan
Some of the most important information on a radio pulsar is derived from its average pulse profile. Many early pulsar studies were necessarily based on only few such profiles. Ther…
A MeerKAT view of the double pulsar eclipses -- Geodetic precession of pulsar B and system geometry
M. E. Lower, M. Kramer, R. M. Shannon +17
The double pulsar system, PSR J07373039A/B, consists of two neutron stars bound together in a highly relativistic orbit that is viewed nearly edge-on from the Earth. This alignm…
Apertif 1.4 GHz continuum observations of the Boötes field and their combined view with LOFAR
A. M. Kutkin, T. A. Oosterloo, R. Morganti +17
We present a new image of a 26.5 square degree region in the Boötes constellation obtained at 1.4 GHz using the Aperture Tile in Focus (Apertif) system on the Westerbork Synthesis…
The Green Bank North Celestial Cap Survey. VIII. 21 New Pulsar Timing Solutions
William Fiore, Lina Levin, Maura A. McLaughlin +26
We present timing solutions for 21 pulsars discovered in 350 MHz surveys using the Green Bank Telescope (GBT). All were discovered in the Green Bank North Celestial Cap pulsar surv…
New upper limits on low-frequency radio emission from isolated neutron stars with LOFAR
Inés Pastor-Marazuela, Samayra M. Straal, Joeri van Leeuwen +1
Neutron stars that show X-ray and -ray pulsed emission must, somewhere in the magnetosphere, generate electron-positron pairs. Such pairs are also required for radio emission, b…