Discovery of the millisecond pulsar PSR J2043+1711 in a Fermi source with the Nanc¸ay Radio Telescope - IN2P3 - Institut national de physique nucléaire et de physique des particules Access content directly
Journal Articles Monthly Notices of the Royal Astronomical Society: Letters Year : 2012

Discovery of the millisecond pulsar PSR J2043+1711 in a Fermi source with the Nanc¸ay Radio Telescope

Lucas Guillemot
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David Stanley Smith
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Abstract

We report the discovery of the millisecond pulsar PSR J2043+1711 in a search of a Fermi Large Area Telescope (LAT) source with no known associations, with the Nanc¸ay Radio Telescope. The new pulsar, confirmed with the Green Bank Telescope, has a spin period of 2.38 ms, is relatively nearby (d 2 kpc) and is in a 1.48-d orbit around a low-mass companion, probably an He-type white dwarf. Using an ephemeris based on Arecibo, Nanc¸ay and Westerbork timing measurements, pulsed gamma-ray emission was detected in the data recorded by the Fermi LAT. The gamma-ray light curve and spectral properties are typical of other gamma-ray millisecond pulsars seen with Fermi. X-ray observations of the pulsar with Suzaku and the Swift X-ray Telescope yielded no detection. At 1.4 GHz, we observe strong flux density variations because of interstellar diffractive scintillation; however, a sharp peak can be observed at this frequency during bright scintillation states. At 327 MHz, the pulsar is detected with a much higher signal-to-noise ratio and its flux density is far more steady. However, at that frequency the Arecibo instrumentation cannot yet fully resolve the pulse profile. Despite that, our pulse time-of-arrival measurements have a post-fit residual rms of 2 μs. This and the expected stability of this system have made PSR J2043+1711 one of the first new Fermi-selected millisecond pulsars to be added to pulsar gravitational wave timing arrays. It has also allowed a significant measurement of relativistic delays in the times of arrival of the pulses due to the curvature of space-time near the companion, but not yet with enough precision to derive useful masses for the pulsar and the companion. Nevertheless, a mass for the pulsar between 1.7 and 2.0M can be derived if a standard millisecond pulsar formation model is assumed. In this paper, we also present a comprehensive summary of pulsar searches in Fermi LAT sources with the Nanc¸ay Radio Telescope to date.
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in2p3-00685243 , version 1 (05-07-2017)

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Lucas Guillemot, P. C. C. Freire, Ismaël Cognard, T. J. Johnson, Y. Takahashi, et al.. Discovery of the millisecond pulsar PSR J2043+1711 in a Fermi source with the Nanc¸ay Radio Telescope. Monthly Notices of the Royal Astronomical Society: Letters, 2012, 422 (2), pp.1294-1305. ⟨10.1111/j.1365-2966.2012.20694.x⟩. ⟨in2p3-00685243⟩
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