论文标题
Meerkat望远镜作为PULSAR设施:系统验证和早期科学的结果
The MeerKAT Telescope as a Pulsar Facility: System verification and early science results from MeerTime
论文作者
论文摘要
我们描述了为新委托的64-Dish Sarao Meerkat射程望远镜开发的PULSAR处理器(PTUSE)的系统验证测试和早期科学结果。 Meerkat是一种高增益(〜2.8 K/JY)的低系统温度(20厘米处的〜18 K)无线电阵列,目前从580-1670 MHz运行,可以产生适合Pulsar观测值的绑定阵列梁。本文介绍了Meertime大型调查项目和PTUSE调试测试。 Highlights include observations of the double pulsar J0737-3039A, pulse profiles from 34 millisecond pulsars from a single 2.5h observation of the Globular cluster Terzan 5, the rotation measure of Ter5O, a 420-sigma giant pulse from the Large Magellanic Cloud pulsar PSR J0540-6919, and nulling identified in the slow pulsar PSR J0633-2015。 Meerkat的关键设计规格之一是使用其新颖的精确时间系统的绝对时间定时误差。我们的两个明亮的毫秒脉冲星的时机证实了Meerkat提供了出色的时机。 PSR J2241-5236的抖动限制为每小时<4 ns,而PSR J1909-3744在近11个月内的抖动限制为66 ns的RMS剩余时间仅为4分钟,仅4分钟。我们的结果证实,Meerkat是一款出色的脉冲星望远镜。该阵列每天可以分为四个单独的子阵列,每天超过1000个脉冲星,并将S波段(1750-3500 MHz)接收器的未来部署将进一步增强其功能。
We describe system verification tests and early science results from the pulsar processor (PTUSE) developed for the newly-commissioned 64-dish SARAO MeerKAT radio telescope in South Africa. MeerKAT is a high-gain (~2.8 K/Jy) low-system temperature (~18 K at 20cm) radio array that currently operates from 580-1670 MHz and can produce tied-array beams suitable for pulsar observations. This paper presents results from the MeerTime Large Survey Project and commissioning tests with PTUSE. Highlights include observations of the double pulsar J0737-3039A, pulse profiles from 34 millisecond pulsars from a single 2.5h observation of the Globular cluster Terzan 5, the rotation measure of Ter5O, a 420-sigma giant pulse from the Large Magellanic Cloud pulsar PSR J0540-6919, and nulling identified in the slow pulsar PSR J0633-2015. One of the key design specifications for MeerKAT was absolute timing errors of less than 5 ns using their novel precise time system. Our timing of two bright millisecond pulsars confirm that MeerKAT delivers exceptional timing. PSR J2241-5236 exhibits a jitter limit of <4 ns per hour whilst timing of PSR J1909-3744 over almost 11 months yields an rms residual of 66 ns with only 4 min integrations. Our results confirm that the MeerKAT is an exceptional pulsar telescope. The array can be split into four separate sub-arrays to time over 1000 pulsars per day and the future deployment of S-band (1750-3500 MHz) receivers will further enhance its capabilities.