FAST early pulsar discoveries: Effelsberg follow-up. Issue 1 (9th September 2021)

• Record Type: Journal Article
• Authors: Cruces, M; Champion, D J; Li (李 菂), D; Kramer, M; Zhu, W W; Wang, P; Cameron, A D; Chen, Y T; Hobbs, G; Freire, P C C; Graikou, E; Krco, M; Liu, Z J; Miao, C C; Niu, J; Pan, Z C; Qian, L; Xue, M Y; Xie, X Y; You, S P; Yu, X H; Yuan, M; Yue, Y L; Zhu, Y; Lackeos, K; Porayko, N; Wongphecauxon, J; Main, R
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 508:Issue 1(2021)
• Page Start: 300
• Page End: 314
• Publication Date: 2021-09-09
• Subjects: survey -- stars: neutron -- pulsars: general -- radio continuum: transients; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stab2540
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: We report the follow-up of 10 pulsars discovered by the Five-hundred-metre Aperture Spherical radio-Telescope (FAST) during its commissioning. The pulsars were discovered at a frequency of 500-MHz using the ultrawide-band (UWB) receiver in drift-scan mode, as part of the Commensal Radio Astronomy FAST Survey (CRAFTS). We carried out the timing campaign with the 100-m Effelsberg radio-telescope at L -band around 1.36 GHz. Along with 11 FAST pulsars previously reported, FAST seems to be uncovering a population of older pulsars, bordering and/or even across the pulsar death-lines. We report here two sources with notable characteristics. PSR J1951+4724 is a young and energetic pulsar with nearly 100 per cent of linearly polarized flux density and visible up to an observing frequency of 8 GHz. PSR J2338+4818, a mildly recycled pulsar in a 95.2-d orbit with a Carbon–Oxygen white dwarf (WD) companion of $\gtrsim 1\, \rm {M}_{\odot }$, based on estimates from the mass function. This system is the widest WD binary with the most massive companion known to-date. Conspicuous discrepancy was found between estimations based on NE2001 and YMW16 electron density models, which can be attributed to underrepresentation of pulsars in the sky region between Galactic longitudes 70° < l < 100°. This work represents one of the early CRAFTS results, which start to show potential to substantially enrich the pulsar sample and refine the Galactic electron density model.