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

Clark, C. J., Breton, R. P., Barr, E. D., Burgay, M., Thongmeearkom, T., Nieder, L., Buchner, S., Stappers, B., Kramer, M., Becker, W., Mayer, M., Phosrisom, A., Ashok, A., Bezuidenhout, M. C., Calore, F., Cognard, I., Freire, P. C. C., Geyer, M., Grießmeier, J. -M., Karuppusamy, R., Levin, L., Padmanabh, P. V., Possenti, A., Ransom, S., Serylak, M., Krishnan, V. Venkatraman, Vleeschower, L., Behrend, J., Champion, D. J., Chen, W., Horn, D., Keane, E. F., Künkel, L., Men, Y., Ridolfi, A., Dhillon, V. S., Marsh, T. R., Papa, M. A.

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.

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