Ultra-wide Bandwidth Observations of 19 pulsars with Parkes telescope

التفاصيل البيبلوغرافية
العنوان: Ultra-wide Bandwidth Observations of 19 pulsars with Parkes telescope
المؤلفون: Zhou, Z. R., Wang, J. B., Wang, N., Hobbs, G., Wang, S. Q.
سنة النشر: 2022
المجموعة: Astrophysics
High Energy Physics - Phenomenology
مصطلحات موضوعية: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics, High Energy Physics - Phenomenology
الوصف: Flux densities are basic observation parameters to describe pulsars. In the most updated pulsar catalog, 24% of the listed radio pulsars have no flux density measurement at any frequency. Here, we report the first flux density measurements, spectral indices, pulse profiles, and correlations of the spectral index with pulsar parameters for 19 pulsars employing the Ultra-Wideband Low (UWL) receiver system installed on the Parkes radio telescope. The results for spectral indices of 17 pulsars are in the range between -0.6 and -3.10. The polarization profiles of thirteen pulsars are shown. There is a moderate correlation between the spectral index and spin frequency. For most pulsars detected, the S/N ratio of pulse profile is not high, so DM, Faraday rotation measure (RM), and polarization can not be determined precisely. Twenty-nine pulsars were not detected in our observations. We discuss the possible explanations for why these pulsars were not detected.
Comment: 19 pages, 6 figures, 5 tables, accepted for publication in RAA
نوع الوثيقة: Working Paper
DOI: 10.1088/1674-4527/ac712b
URL الوصول: http://arxiv.org/abs/2205.05723
رقم الأكسشن: edsarx.2205.05723
قاعدة البيانات: arXiv
الوصف
DOI:10.1088/1674-4527/ac712b