The second(O2)observational campaign of gravitational waves(GWs)organized by the LIGO/Virgo Collaborations has led to several breakthroughs such as the detection of GW signals from merger systems involving black holes...The second(O2)observational campaign of gravitational waves(GWs)organized by the LIGO/Virgo Collaborations has led to several breakthroughs such as the detection of GW signals from merger systems involving black holes or neutrons stars.During O2,14 GW alerts were sent to the astronomical community with sky regions mostly covering over hundreds of square degrees.Among them,six were finally confirmed as real astrophysical events.Since 2013,a new set of ground-based robotic telescopes called Ground-based Wide Angle Camera system(GWAC)project and its pathfinder mini-GWAC has been developed to contribute to the various challenges of multi-messenger and time domain astronomy.The GWAC system is built up in the framework of the ground-segment system of the SVOM mission that will be devoted to the study of the multi-wavelength transient sky in the next decade.During O2,only the mini-GWAC telescope network was fully operational.Due to the wide field of view and fast automatic follow-up capabilities of the mini-GWAC telescopes,they were adept to efficiently cover the sky localization areas of GW event candidates.In this paper,we present the mini-GWAC pipeline we have set up to respond to GW alerts and we report our optical follow-up observations of eight GW alerts detected during the O2 run.Our observations provided the largest coverage of the GW localization areas with a short latency made by any optical facility.We found tens of optical transient candidates in our images,but none of those could be securely associated with any confirmed black hole-black hole merger event.Based on this first experience and the near future technical improvements of our network system,we will be more competitive in detecting the optical counterparts from some GW events that will be identified during the upcoming O3 run,especially those emerging from binary neutron star mergers.展开更多
目的探讨原发性高血压患者血压昼夜节律、B型脑钠肽(BNP)与左心室肥厚(LVH)的关系。方法纳入349例原发性高血压患者(74例有LVH,275例无LVH)进行超声心动图检测及24 h动态血压监测,计算左心室重量指数(LVMI)、夜间血压下降率、24 h动脉脉...目的探讨原发性高血压患者血压昼夜节律、B型脑钠肽(BNP)与左心室肥厚(LVH)的关系。方法纳入349例原发性高血压患者(74例有LVH,275例无LVH)进行超声心动图检测及24 h动态血压监测,计算左心室重量指数(LVMI)、夜间血压下降率、24 h动脉脉压(24 h PP)及动态脉压指数(PPI)。根据昼夜血压变异性将研究对象分为超杓型组(n=7)、杓型组(n=77)、非杓型组(n=173)及反杓型组(n=92)。采集患者一般资料及空腹血样,测定血糖、血脂、血尿素氮、血肌酐、胱抑素C、血尿酸及BNP水平。结果 LVH高血压的3级高血压所占比例(85.1%比46.9%;χ~2=34.428,P<0.001)、24 h平均收缩压(134 mm Hg比129 mm Hg;t=3.175,P=0.002)(1 mm Hg=0.133 k Pa)、白天平均收缩压(134 mm Hg比130 mm Hg;t=2.197,P=0.029)、夜间平均收缩压(132 mm Hg比121 mm Hg;t=4.763,P<0.001)、24 h PP(57 mm Hg比52 mm Hg;t=4.120,P<0.001)及PPI(0.43比0.41;t=3.335,P=0.001)均显著高于非LVH高血压患者,而夜间血压下降率[(1.30±8.02)%比(5.68±7.25)%;t=-4.510,P<0.001]显著低于对照组。LVH高血压患者BNP(87.8 pg/ml比28.8 pg/ml;t=2.170,P=0.034)和LVMI(135.1 g/m^2比88.7 g/m^2;t=15.285,P<0.001)均显著高于非LVH患者。超杓型组、杓型组、非杓型组及反杓型组高血压患者的BNP水平差异无统计学意义(P=0.137),而LVMI差异有统计学意义(P=0.001),其中反杓型组患者的LVMI显著高于杓型组(100.3 g/m^2比86.3 g/m^2;t=4.335,P<0.001)和非杓型组(100.3 g/m^2比93.7 g/m^2;t=1.987,P=0.048),非杓型组患者的LVMI显著高于杓型组(93.7 g/m^2比86.3 g/m^2;t=2.693,P=0.008)。多因素线性相关及Logistic回归分析显示,BNP和高血压分级水平与LVMI相关。结论高血压LVH与血压昼夜节律减弱或消失、血压分级水平密切相关,并伴随血浆BNP升高。展开更多
基金supported by the National Natural Science Foundation of China(Grant Nos.11533003,11673006,U1331202,U1931133 and U1938201)the Guangxi Science Foundation(2016GXNSFFA380006,AD17129006and 2018GXNSFGA281007)+3 种基金the Strategic Priority Research Program of the Chinese Academy of Sciences(XDB23040000)the Strategic Pioneer Program on Space Science,Chinese Academy of Sciences(XDA15052600)financial support from the Chinese Academy of Sciences PIFI post-doctoral fellowship program(program C)financial support of the Univ Earth S Labex program at Sorbonne Paris Cité(ANR-10-LABX-0023 and ANR-11-IDEX-0005-02)
文摘The second(O2)observational campaign of gravitational waves(GWs)organized by the LIGO/Virgo Collaborations has led to several breakthroughs such as the detection of GW signals from merger systems involving black holes or neutrons stars.During O2,14 GW alerts were sent to the astronomical community with sky regions mostly covering over hundreds of square degrees.Among them,six were finally confirmed as real astrophysical events.Since 2013,a new set of ground-based robotic telescopes called Ground-based Wide Angle Camera system(GWAC)project and its pathfinder mini-GWAC has been developed to contribute to the various challenges of multi-messenger and time domain astronomy.The GWAC system is built up in the framework of the ground-segment system of the SVOM mission that will be devoted to the study of the multi-wavelength transient sky in the next decade.During O2,only the mini-GWAC telescope network was fully operational.Due to the wide field of view and fast automatic follow-up capabilities of the mini-GWAC telescopes,they were adept to efficiently cover the sky localization areas of GW event candidates.In this paper,we present the mini-GWAC pipeline we have set up to respond to GW alerts and we report our optical follow-up observations of eight GW alerts detected during the O2 run.Our observations provided the largest coverage of the GW localization areas with a short latency made by any optical facility.We found tens of optical transient candidates in our images,but none of those could be securely associated with any confirmed black hole-black hole merger event.Based on this first experience and the near future technical improvements of our network system,we will be more competitive in detecting the optical counterparts from some GW events that will be identified during the upcoming O3 run,especially those emerging from binary neutron star mergers.
文摘目的探讨原发性高血压患者血压昼夜节律、B型脑钠肽(BNP)与左心室肥厚(LVH)的关系。方法纳入349例原发性高血压患者(74例有LVH,275例无LVH)进行超声心动图检测及24 h动态血压监测,计算左心室重量指数(LVMI)、夜间血压下降率、24 h动脉脉压(24 h PP)及动态脉压指数(PPI)。根据昼夜血压变异性将研究对象分为超杓型组(n=7)、杓型组(n=77)、非杓型组(n=173)及反杓型组(n=92)。采集患者一般资料及空腹血样,测定血糖、血脂、血尿素氮、血肌酐、胱抑素C、血尿酸及BNP水平。结果 LVH高血压的3级高血压所占比例(85.1%比46.9%;χ~2=34.428,P<0.001)、24 h平均收缩压(134 mm Hg比129 mm Hg;t=3.175,P=0.002)(1 mm Hg=0.133 k Pa)、白天平均收缩压(134 mm Hg比130 mm Hg;t=2.197,P=0.029)、夜间平均收缩压(132 mm Hg比121 mm Hg;t=4.763,P<0.001)、24 h PP(57 mm Hg比52 mm Hg;t=4.120,P<0.001)及PPI(0.43比0.41;t=3.335,P=0.001)均显著高于非LVH高血压患者,而夜间血压下降率[(1.30±8.02)%比(5.68±7.25)%;t=-4.510,P<0.001]显著低于对照组。LVH高血压患者BNP(87.8 pg/ml比28.8 pg/ml;t=2.170,P=0.034)和LVMI(135.1 g/m^2比88.7 g/m^2;t=15.285,P<0.001)均显著高于非LVH患者。超杓型组、杓型组、非杓型组及反杓型组高血压患者的BNP水平差异无统计学意义(P=0.137),而LVMI差异有统计学意义(P=0.001),其中反杓型组患者的LVMI显著高于杓型组(100.3 g/m^2比86.3 g/m^2;t=4.335,P<0.001)和非杓型组(100.3 g/m^2比93.7 g/m^2;t=1.987,P=0.048),非杓型组患者的LVMI显著高于杓型组(93.7 g/m^2比86.3 g/m^2;t=2.693,P=0.008)。多因素线性相关及Logistic回归分析显示,BNP和高血压分级水平与LVMI相关。结论高血压LVH与血压昼夜节律减弱或消失、血压分级水平密切相关,并伴随血浆BNP升高。
