论文标题
费米 - 拉特伽玛射线源中脉冲星的Trapum L波段调查
The TRAPUM L-band survey for pulsars in Fermi-LAT gamma-ray sources
论文作者
论文摘要
在Fermi大面积望远镜(LAT)检测到的无线电观察中发现了超过100毫秒的脉冲星(MSP),但数百个类似脉冲星的来源仍然统一。在这里,我们介绍了针对瞬态和脉冲星(Trapum)大型调查项目进行的针对性调查的Fermi-Lat源调查的第一个结果。我们观察到79个来源通过从4FGL目录中对非相关来源进行随机森林分类,从而确定了可能是伽马射线脉冲星候选物。使用Meerkat的L波段接收器(856-1712 MHz)观察到每个源在两个单独的时期内观察到10分钟,典型的脉冲磁通密度敏感性为$ \ sim $ 100 $ \,μ$ jy。发现了九个新的MSP,其中8个在二进制系统中,其中包括两个黯然失色的红back和一个系统,即PSR J1526 $ - $ 2744,似乎在一个异常紧凑的5小时轨道上有白色矮人的伴侣。我们为其中两个MSP获得了相互连接的时序解决方案,从而可以检测Fermi-LAT数据中的伽马射线脉动。对PSR J1526 $ - $ 2744的高级LIGO数据的连续重力波进行的后续搜索使用由此产生的Fermi-Lat Timing Ephemeris尚未产生检测,但在中子售价为2.45美元\ times10^{ - 8} $。我们还检测到从第一次Erosita All-Sky调查中的Redback PSR J1803 $ - $ 6707的X射线排放,这可能是由于binary Shock发射的。
More than 100 millisecond pulsars (MSPs) have been discovered in radio observations of gamma-ray sources detected by the Fermi Large Area Telescope (LAT), but hundreds of pulsar-like sources remain unidentified. Here we present the first results from the targeted survey of Fermi-LAT sources being performed by the Transients and Pulsars with MeerKAT (TRAPUM) Large Survey Project. We observed 79 sources identified as possible gamma-ray pulsar candidates by a Random Forest classification of unassociated sources from the 4FGL catalogue. Each source was observed for 10 minutes on two separate epochs using MeerKAT's L-band receiver (856-1712 MHz), with typical pulsed flux density sensitivities of $\sim$100$\,μ$Jy. Nine new MSPs were discovered, eight of which are in binary systems, including two eclipsing redbacks and one system, PSR J1526$-$2744, that appears to have a white dwarf companion in an unusually compact 5 hr orbit. We obtained phase-connected timing solutions for two of these MSPs, enabling the detection of gamma-ray pulsations in the Fermi-LAT data. A follow-up search for continuous gravitational waves from PSR J1526$-$2744 in Advanced LIGO data using the resulting Fermi-LAT timing ephemeris yielded no detection, but sets an upper limit on the neutron star ellipticity of $2.45\times10^{-8}$. We also detected X-ray emission from the redback PSR J1803$-$6707 in data from the first eROSITA all-sky survey, likely due to emission from an intra-binary shock.