We present a polarization study of 25 globular cluster(GC)pulsars observed with the Five-hundred-meter Aperture Spherical radio Telescope(FAST),including 15 pro les measured for the rst time.The pulse width–period re...We present a polarization study of 25 globular cluster(GC)pulsars observed with the Five-hundred-meter Aperture Spherical radio Telescope(FAST),including 15 pro les measured for the rst time.The pulse width–period relationships for millisecond pulsars(MSPs)in GCs follow power-law indices of-0.268(W10)and-0.330(W50),consistent with normal pulsars.Only 20%of the sample exhibit clear S-shaped position angle curves-signi cantly fewer than in the normal pulsar population.Rotation Measures(RMs)for these pulsars suggest that GCs near the Galactic plane show higher RMs,in agreement with former studies.Polarization ratios were measured,with M53A showing the highest linear polarization(56%)and M15H the highest absolute circular polarization(37%).On average,GC pulsars exhibit lower circular(-1%)and absolute circular(11%)polarization compared to normal pulsars observed with Parkes(5%and 32%,respectively).However,their polarization distributions align with MSPs in the Galactic plane,suggesting GC environments do not drastically alter emission properties.展开更多
The standing waves existing in radio telescope data are primarily due to reflections among the instruments,which significantly impact the spectral quality of the Five-hundred-meter Aperture Spherical radio Telescope(F...The standing waves existing in radio telescope data are primarily due to reflections among the instruments,which significantly impact the spectral quality of the Five-hundred-meter Aperture Spherical radio Telescope(FAST).Eliminating these standing waves for FAST is challenging given the constant changes in their phases and amplitudes.Over a ten-second period,the phases shift by 18°while the amplitudes fluctuate by 6 mK.Thus,we developed the fast Fourier transform(FFT)filter method to eliminate these standing waves for every individual spectrum.The FFT filter can decrease the rms from 3.2 to 1.15 times the theoretical estimate.Compared to other methods such as sine fitting and running median,the FFT filter achieves a median rms of approximately 1.2 times the theoretical expectation and the smallest scatter at 12%.Additionally,the FFT filter method avoids the flux loss issue encountered with some other methods.The FFT is also efficient in detecting harmonic radio frequency interference(RFI).In the FAST data,we identified three distinct types of harmonic RFI,each with amplitudes exceeding 100 mK and intrinsic frequency periods of 8.1,0.5,and 0.37 MHz,respectively.The FFT filter,proven as the most effective method,is integrated into the H I data calibration and imaging pipeline for FAST(HiFAST,https://hifast.readthedocs.io).展开更多
来自人造卫星的信号是射电天文观测面临的主要射频干扰(radio frequency interference,RFI)之一,这些RFI会将天文信号掩埋,为天文信号的搜寻和分析带来困扰。为了缓减卫星对天文观测的影响,我们在之前的工作中为500 m口径球面射电望远镜...来自人造卫星的信号是射电天文观测面临的主要射频干扰(radio frequency interference,RFI)之一,这些RFI会将天文信号掩埋,为天文信号的搜寻和分析带来困扰。为了缓减卫星对天文观测的影响,我们在之前的工作中为500 m口径球面射电望远镜(Five-hundred-meter Aperture Spherical radio Telescope,FAST)开发了卫星电磁干扰监测软件,主要包括卫星数据库、观测模块和监测模块。近年来随着多个巨型卫星星座的规划发射以及望远镜观测模式的增多,卫星对射电天文观测的影响更为复杂,已有的软件已经不能满足实际的需要。为此,本文在单个卫星干扰分析的基础上提出了卫星星座的干扰评估方法,并对已有监测软件进行了升级,升级后卫星数据库覆盖更多的在轨卫星及星座信息且能够自动化更新,观测模块能够支持更多种观测模式下的卫星过境预测和干扰评估。在实际天文观测中,通过接在FAST接收机上的频谱仪数据对软件的干扰预测结果进行了实验验证,结果证明升级后的软件能够在多种观测模式下预测可能威胁的卫星以及对应的过境时间,为望远镜观测规划的调整、卫星干扰的规避和接收系统的保护提供重要的支撑。展开更多
We report a new high-sensitivity HⅠmapping observation of the NGC 5055 galaxy group over an area of 1°.5×0°.75 with the Five-hundred-meter Aperture Spherical radio Telescope(FAST).Our observation revea...We report a new high-sensitivity HⅠmapping observation of the NGC 5055 galaxy group over an area of 1°.5×0°.75 with the Five-hundred-meter Aperture Spherical radio Telescope(FAST).Our observation reveals that the warped HⅠdisk of NGC 5055 is more extended than what was previously observed by WSRT,out to239(61.7 kpc).The total HⅠmass of NGC 5055 is determined to be~1.1×10^(10)M_Θ.We identified three HⅠclouds with HⅠmasses of the order of~10^(7)M_Θat the southeastern edge of the HⅠdisk,as well as a candidate high-velocity cloud with an HⅠmass of(1.2±0.5)×10^(6)M_Θto the north of NGC 5055.The HⅠcontent of UGCA337 is robustly detected for the first time by the FAST observations.It has a narrow HⅠlinewidth of W_(50)=17.4±3.8 km s^(-1)with a total HⅠmass of(3.5±0.3)×10^(6)M_Θ.Comparing the gas content and g-r color of UGCA 337 with typical low-mass dwarf galaxies,UGCA 337 appears relatively gas-poor despite its blue color.This suggests that UGCA 337 may have undergone gas stripping in the past.We also analyzed the possible origin of the diffuse HⅠclouds located at the outskirts of NGC 5055,and speculate that they might be the remnant features of a merger event in the past.展开更多
针对FAST促动器群的可靠性问题,提出群系统和群系统可靠性概念,建立以权重值为核心要义的群系统可靠性数学模型。结合FAST,讨论促动器群系统权重值的实际意义,提出促动器权重值及其可用度的计算方法。依据模型,以促动器前期运行和维护...针对FAST促动器群的可靠性问题,提出群系统和群系统可靠性概念,建立以权重值为核心要义的群系统可靠性数学模型。结合FAST,讨论促动器群系统权重值的实际意义,提出促动器权重值及其可用度的计算方法。依据模型,以促动器前期运行和维护数据为基础,计算促动器群系统在2019年3月至8月期间的平均可靠度为0.997 85。通过群系统可靠性理论模型,分析得到了群系统可靠性增长的原理:提高子系统平均无故障工作时间(Mean time between failures,MTBF),降低子系统平均故障修复时间(Mean time to repair,MTTR)。结合工程实际,提出促动器群系统可靠性增长方案:通过先进行多次局部可靠性增长设计和试验,最后集中一两次整体纠正设计和试验的最优性价比可靠性增长过程,以提高促动器MTBF;同时,开发基于故障预测与健康管理(Prognostic and health management,PHM)技术的智能故障诊断与预测系统,将促动器维护模式从被动式事后维护变为主动式状态维护,以降低促动器MTTR。群系统和群系统可靠性理论的建立为FAST促动器群系统可靠性分析与可靠性增长研究提供了理论支撑,为其他类似群系统可靠性相关研究提供参考。展开更多
Pulsar search is always the basis of pulsar navigation,gravitational wave detection and other research topics.Currently,the volume of pulsar candidates collected by the Five-hundred-meter Aperture Spherical radio Tele...Pulsar search is always the basis of pulsar navigation,gravitational wave detection and other research topics.Currently,the volume of pulsar candidates collected by the Five-hundred-meter Aperture Spherical radio Telescope(FAST)shows an explosive growth rate that has brought challenges for its pulsar candidate filtering system.Particularly,the multi-view heterogeneous data and class imbalance between true pulsars and non-pulsar candidates have negative effects on traditional single-modal supervised classification methods.In this study,a multi-modal and semi-supervised learning based on a pulsar candidate sifting algorithm is presented,which adopts a hybrid ensemble clustering scheme of density-based and partition-based methods combined with a feature-level fusion strategy for input data and a data partition strategy for parallelization.Experiments on both High Time Resolution Universe SurveyⅡ(HTRU2)and actual FAST observation data demonstrate that the proposed algorithm could excellently identify pulsars:On HTRU2,the precision and recall rates of its parallel mode reach0.981 and 0.988 respectively.On FAST data,those of its parallel mode reach 0.891 and 0.961,meanwhile,the running time also significantly decreases with the increment of parallel nodes within limits.Thus,we can conclude that our algorithm could be a feasible idea for large scale pulsar candidate sifting for FAST drift scan observation.展开更多
随着网络信息化技术高速发展,业务系统膨胀式增加,管理多个系统认证安全和记住多个系统账户密码,让系统管理员和用户们备受困扰,集中对多形式、多样化信息端统一授权认证亟待解决。当前通用技术标准为采用微服务与实现OAuth2开放统一认...随着网络信息化技术高速发展,业务系统膨胀式增加,管理多个系统认证安全和记住多个系统账户密码,让系统管理员和用户们备受困扰,集中对多形式、多样化信息端统一授权认证亟待解决。当前通用技术标准为采用微服务与实现OAuth2开放统一认证标准协议架构。500米口径球面射电望远镜FAST作为我国自主研发的世界上最大口径天文望远镜,在天文研究上取得令人瞩目的科研成果。FAST早期科学数据中心为加强数据管理与科普工作,研发了大量多形式的数字化信息系统。基于资源安全访问控制管理和简化管理工作的需要,FAST科学数据平台系统必须实现统一授权认证。论文研究开放认证授权标准协议OAuth2和身份验证标准Open ID Connect工作原理,探讨可行方案Identity Server关键技术。分析了当前Fast数据管理平台管理存在的多样的信息系统状况,设计统一身份认证系统架构,并采用IdentityServer4构建统一认证中心,使用.NET微服务实现认证功能,完成各类Web软件系统、App软件和桌面应用软件的统一身份认证接入。展开更多
单脉冲搜索作为脉冲星探测的有力工具,在探测旋转射电暂现源以及快速射电暴中扮演着重要角色。为了从海量的射电巡天数据中快速筛选出最有价值的单脉冲搜索候选体,候选体识别已经从早期启发式阈值判断发展到基于机器学习自动识别。对于F...单脉冲搜索作为脉冲星探测的有力工具,在探测旋转射电暂现源以及快速射电暴中扮演着重要角色。为了从海量的射电巡天数据中快速筛选出最有价值的单脉冲搜索候选体,候选体识别已经从早期启发式阈值判断发展到基于机器学习自动识别。对于FAST观测,研究了基于机器学习的单脉冲搜索候选体识别应用到CRAFTS(the commensal radio astronomy FAST survey)超宽带脉冲星数据的性能表现。在评估过程中,使用单脉冲事件组识别(SPEGID)和单脉冲搜索器(SPS)两类自动识别方法,通过7种不同机器学习分类器对CRAFTS基准数据集产生的单脉冲搜索候选体进行自动识别;作为对比,也使用了启发式阈值判断的方法(RRATtrap和Clusterrank)。结果表明,SPEGID具有最好的性能表现(最高的F1-score值95.1%、次高的召回率95.4%、最低的假阳性率4.7%),SPS具有最快的筛选速度(平均每小时筛选4010个候选体)。通过对比分析结果,探讨了如何基于FAST观测数据开展高效的单脉冲搜索候选体识别。展开更多
A highly accurate and precise technique for measurement of the 93 Nb(n,n’)93m Nb reaction rate was established for the material surveillance tests,etc.in fast reactors.The self-absorption effect on the measurement of...A highly accurate and precise technique for measurement of the 93 Nb(n,n’)93m Nb reaction rate was established for the material surveillance tests,etc.in fast reactors.The self-absorption effect on the measurement of the characteristic X-rays emitted by 93m Nb was decreased by the dissolution and evaporation to dryness of niobium dosimeter.A highly precise count of the number of 93 Nb atoms was obtained by measuring the niobium solution concentration using inductively coupled plasma mass spectrometry.X-rays of 93m Nb were measured accurately by means of comparing the X-ray intensity of irradiated niobium solution with that of the solution in which stable 93 Nb was added.The difference between both intensities indicates the effect of 182 Ta,which is generated from an impurity tantalum,and the intensity of X-rays from 93m Nb was evaluated.Measurement error of the 93 Nb(n,n’)93m Nb reaction rate was reduced to be less than 4%,which was equivalent to the other reaction rate errors of dosimeters used for Joyo dosimetry.In addition,an advanced technique using Resonance Ionization Mass Spectrometry was proposed for the precise measurement of 93m Nb yield,and 93m Nb will be resonance-ionized selectively by discriminating the hyperfine splitting of the atomic energy levels between 93 Nb and 93m Nb at high resolution.展开更多
基金supported by the National Key R&D Program of China,No.2022YFC2205202the National Natural Science Foundation of China(NSFC)under grant Nos.12173052,U2031119,11773041 and 11703047+2 种基金supported by the Youth Innovation Promotion Association of the Chinese Academy of Sciences(CAS)(id.Y2022027)the CAS“Light of West China”Programthe CAS President’s International Fellowship Initiative(grant No.2021FSM0004).
文摘We present a polarization study of 25 globular cluster(GC)pulsars observed with the Five-hundred-meter Aperture Spherical radio Telescope(FAST),including 15 pro les measured for the rst time.The pulse width–period relationships for millisecond pulsars(MSPs)in GCs follow power-law indices of-0.268(W10)and-0.330(W50),consistent with normal pulsars.Only 20%of the sample exhibit clear S-shaped position angle curves-signi cantly fewer than in the normal pulsar population.Rotation Measures(RMs)for these pulsars suggest that GCs near the Galactic plane show higher RMs,in agreement with former studies.Polarization ratios were measured,with M53A showing the highest linear polarization(56%)and M15H the highest absolute circular polarization(37%).On average,GC pulsars exhibit lower circular(-1%)and absolute circular(11%)polarization compared to normal pulsars observed with Parkes(5%and 32%,respectively).However,their polarization distributions align with MSPs in the Galactic plane,suggesting GC environments do not drastically alter emission properties.
基金supported by the China National Key Program for Science and Technology Research and Development of China (2022YFA1602901,2023YFA1608204)the National SKA Program of China (No.2022SKA0110201)+5 种基金the National Natural Science Foundation of China (NSFC,grant Nos.11873051,11988101,12033008,12041305,12125302,12173016,and 12203065)the CAS Project for Young Scientists in Basic Research grant (No.YSBR-062)the K.C.Wong Education Foundationthe science research grants from the China Manned Space Projectsupport from the Cultivation Project for FAST Scientific Payoff and Research Achievement of CAMS-CASsupported by the China Postdoctoral Science Foundation grant No.2024M763213
文摘The standing waves existing in radio telescope data are primarily due to reflections among the instruments,which significantly impact the spectral quality of the Five-hundred-meter Aperture Spherical radio Telescope(FAST).Eliminating these standing waves for FAST is challenging given the constant changes in their phases and amplitudes.Over a ten-second period,the phases shift by 18°while the amplitudes fluctuate by 6 mK.Thus,we developed the fast Fourier transform(FFT)filter method to eliminate these standing waves for every individual spectrum.The FFT filter can decrease the rms from 3.2 to 1.15 times the theoretical estimate.Compared to other methods such as sine fitting and running median,the FFT filter achieves a median rms of approximately 1.2 times the theoretical expectation and the smallest scatter at 12%.Additionally,the FFT filter method avoids the flux loss issue encountered with some other methods.The FFT is also efficient in detecting harmonic radio frequency interference(RFI).In the FAST data,we identified three distinct types of harmonic RFI,each with amplitudes exceeding 100 mK and intrinsic frequency periods of 8.1,0.5,and 0.37 MHz,respectively.The FFT filter,proven as the most effective method,is integrated into the H I data calibration and imaging pipeline for FAST(HiFAST,https://hifast.readthedocs.io).
文摘来自人造卫星的信号是射电天文观测面临的主要射频干扰(radio frequency interference,RFI)之一,这些RFI会将天文信号掩埋,为天文信号的搜寻和分析带来困扰。为了缓减卫星对天文观测的影响,我们在之前的工作中为500 m口径球面射电望远镜(Five-hundred-meter Aperture Spherical radio Telescope,FAST)开发了卫星电磁干扰监测软件,主要包括卫星数据库、观测模块和监测模块。近年来随着多个巨型卫星星座的规划发射以及望远镜观测模式的增多,卫星对射电天文观测的影响更为复杂,已有的软件已经不能满足实际的需要。为此,本文在单个卫星干扰分析的基础上提出了卫星星座的干扰评估方法,并对已有监测软件进行了升级,升级后卫星数据库覆盖更多的在轨卫星及星座信息且能够自动化更新,观测模块能够支持更多种观测模式下的卫星过境预测和干扰评估。在实际天文观测中,通过接在FAST接收机上的频谱仪数据对软件的干扰预测结果进行了实验验证,结果证明升级后的软件能够在多种观测模式下预测可能威胁的卫星以及对应的过境时间,为望远镜观测规划的调整、卫星干扰的规避和接收系统的保护提供重要的支撑。
基金supported by the National Key R&D Program of China(2022YFA1602901)the National Natural Science Foundation of China(NSFC,grant No.12373001)supported by the Open Project Program of the Key Laboratory of FAST,NAOC,Chinese Academy of Sciences。
文摘We report a new high-sensitivity HⅠmapping observation of the NGC 5055 galaxy group over an area of 1°.5×0°.75 with the Five-hundred-meter Aperture Spherical radio Telescope(FAST).Our observation reveals that the warped HⅠdisk of NGC 5055 is more extended than what was previously observed by WSRT,out to239(61.7 kpc).The total HⅠmass of NGC 5055 is determined to be~1.1×10^(10)M_Θ.We identified three HⅠclouds with HⅠmasses of the order of~10^(7)M_Θat the southeastern edge of the HⅠdisk,as well as a candidate high-velocity cloud with an HⅠmass of(1.2±0.5)×10^(6)M_Θto the north of NGC 5055.The HⅠcontent of UGCA337 is robustly detected for the first time by the FAST observations.It has a narrow HⅠlinewidth of W_(50)=17.4±3.8 km s^(-1)with a total HⅠmass of(3.5±0.3)×10^(6)M_Θ.Comparing the gas content and g-r color of UGCA 337 with typical low-mass dwarf galaxies,UGCA 337 appears relatively gas-poor despite its blue color.This suggests that UGCA 337 may have undergone gas stripping in the past.We also analyzed the possible origin of the diffuse HⅠclouds located at the outskirts of NGC 5055,and speculate that they might be the remnant features of a merger event in the past.
文摘针对FAST促动器群的可靠性问题,提出群系统和群系统可靠性概念,建立以权重值为核心要义的群系统可靠性数学模型。结合FAST,讨论促动器群系统权重值的实际意义,提出促动器权重值及其可用度的计算方法。依据模型,以促动器前期运行和维护数据为基础,计算促动器群系统在2019年3月至8月期间的平均可靠度为0.997 85。通过群系统可靠性理论模型,分析得到了群系统可靠性增长的原理:提高子系统平均无故障工作时间(Mean time between failures,MTBF),降低子系统平均故障修复时间(Mean time to repair,MTTR)。结合工程实际,提出促动器群系统可靠性增长方案:通过先进行多次局部可靠性增长设计和试验,最后集中一两次整体纠正设计和试验的最优性价比可靠性增长过程,以提高促动器MTBF;同时,开发基于故障预测与健康管理(Prognostic and health management,PHM)技术的智能故障诊断与预测系统,将促动器维护模式从被动式事后维护变为主动式状态维护,以降低促动器MTTR。群系统和群系统可靠性理论的建立为FAST促动器群系统可靠性分析与可靠性增长研究提供了理论支撑,为其他类似群系统可靠性相关研究提供参考。
基金supported by the National Key R&D Program of China(No.2022YFE0133700)the National Natural Science Foundation of China(NSFC,grant Nos.12273008,11963003,12273007 and 62062025)+4 种基金the National SKA Program of China(No.2020SKA0110300)the Guizhou Province Science and Technology Support Program(General Project)No.Qianhe Support[2023]General 333,Science and Technology Foundation of Guizhou Province(Key Program,No.[2019]1432)the Guizhou Provincial Science and Technology Projects(Nos.ZK[2022]143 and ZK[2022]304)the Cultivation project of Guizhou University(No.[2020]76)。
文摘Pulsar search is always the basis of pulsar navigation,gravitational wave detection and other research topics.Currently,the volume of pulsar candidates collected by the Five-hundred-meter Aperture Spherical radio Telescope(FAST)shows an explosive growth rate that has brought challenges for its pulsar candidate filtering system.Particularly,the multi-view heterogeneous data and class imbalance between true pulsars and non-pulsar candidates have negative effects on traditional single-modal supervised classification methods.In this study,a multi-modal and semi-supervised learning based on a pulsar candidate sifting algorithm is presented,which adopts a hybrid ensemble clustering scheme of density-based and partition-based methods combined with a feature-level fusion strategy for input data and a data partition strategy for parallelization.Experiments on both High Time Resolution Universe SurveyⅡ(HTRU2)and actual FAST observation data demonstrate that the proposed algorithm could excellently identify pulsars:On HTRU2,the precision and recall rates of its parallel mode reach0.981 and 0.988 respectively.On FAST data,those of its parallel mode reach 0.891 and 0.961,meanwhile,the running time also significantly decreases with the increment of parallel nodes within limits.Thus,we can conclude that our algorithm could be a feasible idea for large scale pulsar candidate sifting for FAST drift scan observation.
文摘随着网络信息化技术高速发展,业务系统膨胀式增加,管理多个系统认证安全和记住多个系统账户密码,让系统管理员和用户们备受困扰,集中对多形式、多样化信息端统一授权认证亟待解决。当前通用技术标准为采用微服务与实现OAuth2开放统一认证标准协议架构。500米口径球面射电望远镜FAST作为我国自主研发的世界上最大口径天文望远镜,在天文研究上取得令人瞩目的科研成果。FAST早期科学数据中心为加强数据管理与科普工作,研发了大量多形式的数字化信息系统。基于资源安全访问控制管理和简化管理工作的需要,FAST科学数据平台系统必须实现统一授权认证。论文研究开放认证授权标准协议OAuth2和身份验证标准Open ID Connect工作原理,探讨可行方案Identity Server关键技术。分析了当前Fast数据管理平台管理存在的多样的信息系统状况,设计统一身份认证系统架构,并采用IdentityServer4构建统一认证中心,使用.NET微服务实现认证功能,完成各类Web软件系统、App软件和桌面应用软件的统一身份认证接入。
文摘单脉冲搜索作为脉冲星探测的有力工具,在探测旋转射电暂现源以及快速射电暴中扮演着重要角色。为了从海量的射电巡天数据中快速筛选出最有价值的单脉冲搜索候选体,候选体识别已经从早期启发式阈值判断发展到基于机器学习自动识别。对于FAST观测,研究了基于机器学习的单脉冲搜索候选体识别应用到CRAFTS(the commensal radio astronomy FAST survey)超宽带脉冲星数据的性能表现。在评估过程中,使用单脉冲事件组识别(SPEGID)和单脉冲搜索器(SPS)两类自动识别方法,通过7种不同机器学习分类器对CRAFTS基准数据集产生的单脉冲搜索候选体进行自动识别;作为对比,也使用了启发式阈值判断的方法(RRATtrap和Clusterrank)。结果表明,SPEGID具有最好的性能表现(最高的F1-score值95.1%、次高的召回率95.4%、最低的假阳性率4.7%),SPS具有最快的筛选速度(平均每小时筛选4010个候选体)。通过对比分析结果,探讨了如何基于FAST观测数据开展高效的单脉冲搜索候选体识别。
文摘A highly accurate and precise technique for measurement of the 93 Nb(n,n’)93m Nb reaction rate was established for the material surveillance tests,etc.in fast reactors.The self-absorption effect on the measurement of the characteristic X-rays emitted by 93m Nb was decreased by the dissolution and evaporation to dryness of niobium dosimeter.A highly precise count of the number of 93 Nb atoms was obtained by measuring the niobium solution concentration using inductively coupled plasma mass spectrometry.X-rays of 93m Nb were measured accurately by means of comparing the X-ray intensity of irradiated niobium solution with that of the solution in which stable 93 Nb was added.The difference between both intensities indicates the effect of 182 Ta,which is generated from an impurity tantalum,and the intensity of X-rays from 93m Nb was evaluated.Measurement error of the 93 Nb(n,n’)93m Nb reaction rate was reduced to be less than 4%,which was equivalent to the other reaction rate errors of dosimeters used for Joyo dosimetry.In addition,an advanced technique using Resonance Ionization Mass Spectrometry was proposed for the precise measurement of 93m Nb yield,and 93m Nb will be resonance-ionized selectively by discriminating the hyperfine splitting of the atomic energy levels between 93 Nb and 93m Nb at high resolution.
