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1.
讨论了云南天文台1995年研制的斑点象探测系统存在几个问题,ICCD探测的一些性能参数不同,控制器不灵,数据的采集速度较慢等,然后报导了对ICCD光灵敏度和电子快门参数的测量,对ICCD控制器的改装和提高数据采集速度的方法以及改地后的探测系统进行观测的情况。 相似文献
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紫台多波段光谱仪近年在He Ⅰ10830 波区相继研制了一维Reticon 和CCD 相机的探测系统,现又建成了用二个CCD 相机能在He Ⅰ10830 和Ca Ⅱ8542/Hα同时作两维成像光谱观测的系统。文中简要介绍了它的结构和取得的初步观测结果 相似文献
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本文首先回顾了目前上CCD控制器的最新进展。介绍了中国的第一套天文用CCD探测器系统:云南天文台#D1CCD系统。 相似文献
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着重介绍了经纬仪光电定位系统中的数据处理方法,包括了IC-CD倾斜角及比例尺的测定,望远镜指向模型建立,星象位置坐标归算多个方面,并给出了方法的基本原理。 相似文献
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经纬仪光电定位系统数据处理 总被引:2,自引:0,他引:2
着重介绍了经纬仪光电定位系统中的数据处理方法,包括了IC-CD倾斜角及比例尺度的测定,望远镜指向模型建立,星象位置坐标归算多个方面,并给出了方法的基本原理。 相似文献
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云南天文台PI1024TKB CCD 总被引:1,自引:0,他引:1
详细介绍了云南天文台1m望远镜新近引进的美国PrincetonInstruments公司PI1024TKB CCD及其控制器ST-138的各基参数指标和使用方法。 相似文献
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云南天文台高分辨率斑点成像的新进展 总被引:2,自引:0,他引:2
本文报道了对天文目标:双星ADS16800、ADS16173,三星Hu66(ADS11344)和Hld171(ADS16648)进行的斑点成像观测及测量结果。介绍了所用的二维光子计数斑点像探测系统的性能,分析了探测系统的光子噪声、附加噪声和其它更复杂的噪声对斑点图的平均功率谱和重谱的影响。在讨论了改正重谱中的噪声偏差项时提出了对重谱基底施加正性约束的算法。测量的结果表明,实现了高精度的微射受限天文 相似文献
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P. Bergamini G. Bonelli A. Paizis L. Tommasi M. Uslenghi R. Falomo G. Tondello 《Experimental Astronomy》2000,10(4):457-471
The scientific performance evaluation of a photon countingimaging system is presented. The detector is constituted by an ICCD camera with RbTe photocathode(optimized for UV radiation), and dedicated electronics for the acquisition and analysis ofthe events. For each photon event on the CCD, a real-time centroid calculation is performed, inorder to reach spatial resolution down to 25 m FWHM. The system has been tested usingthe 182 cm telescope of the Asiago Observatory.A standard stars field through U Johnson filter,and the Crab pulsar (PSR 0531+21) were observed. From the photometric data, relative magnitudes of the standard stars have been derived, showing a goodlinearity of the detector in the range of flux under consideration, as expected fromprevious laboratory measurements.The pulsar's data have been processed by FFT and epoch foldingtechniques to testthe detector's timing performances in the highest resolutionmode (4.512 ms).These observations show that a space resolved time analysis ofperiodic sources can be performed with 10-7 s accuracy. 相似文献
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首先介绍了斑点图形成机制以及获取方法,并借助计算机模拟了斑点图的生成。然后重点描述斑点图的图像重建方法,包括频率域和空间域重建方法。在频率域重建方法部分依次详细叙述了用于复原模信息的斑点干涉法和用于复原相位信息的由模复原相位法、Knox-Thompson法、斑点掩模法;空间域重建方法部分介绍了典型的LWH法和迭代位移叠加法;另外,盲消卷积法也为斑点图重建提供了新的思路,文章对此方法也做了介绍;特别地,还对国内在该领域的相关工作做了介绍;关于斑点图重建方法在天文学、天体物理学等领域的应用,文章做了有针对性的介绍;最后一章是斑点图图像重建方法的总结。 相似文献
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A. K. Tickoo R. Koul S. K. Kaul I. K. Kaul C. L. Bhat N. G. Bhatt M. K. Kothari H. C. Goyal N. K. Agarwal S. R. Kaul 《Experimental Astronomy》1999,9(2):81-101
A PC-based drive-control system has been developed for the altitude-azimuth mounted TACTIC -ray telescope to control the speed and direction of motion of its 2-axes. Details of various hardware components chosen for the telescope, including hybrid-stepper motor, 16-bit absolute encoder and CAMAC-based programmable stepper motor controller, are discussed in this paper. The telescope-control strategy, based on the position-loop with a proportional type control for the source-seek mode and the on/off type control for the tracking mode, is explained in detail. Some important performance features of the telescope, including its blind-spot size, drive-system backlash and encoder-error compensation, are also presented. The drive system has been extensively field-tested and has been operating satisfactorily during observation campaigns carried out since March 1997 with the TACTIC Imaging Element. A tracking accuracy of ±3 arc-minutes has been achieved. A test report of its performance, with regard to its tracking accuracy on the basis of successful detection of TeV -rays from the active galaxy Markarian 501 in April–May 1997, is also presented. 相似文献
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A total of 704 previously published photoelectricB colour observations of the multiple system HR 4560 are analyzed by means of the light curve models NDE (Popper and Etzel, 1981) and WINK (Wood, 1972) in an iterative procedure. As a result, we have found that componentC of the multiplpe system ADS 8347 is the most probable origin of the observed eclipses. Some relevant astrophysical parameters of the component stars which indicate a normal Main-Sequence binary star have also been estimated. 相似文献
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M. Hoffmann 《Astrophysics and Space Science》1982,83(1-2):203-207
Photoelectric light curves of V1022 Oph inB andV are presented. It has been confirmed that it is a W UMa type eclipsing binary with one of the shortest periods known (P<0.d25). Some general properties of the system have been derived.Based on observations made at the European Southern Observatory (La Silla/Chile) 相似文献
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UBV photoelectric photometry of the eclipsing binary system AW UMa has been presented. A slightly improved period of 0
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4387304 has been given. The colour of the system has been discussed. Eccentricity is present in the system. Light and colour curves show that intrinsic light variations may be present in the system. The presence of mass transfer is a possibility. 相似文献
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R. K. Srivastava 《Astrophysics and Space Science》1988,140(2):337-351
FirstUBV photoelectric photometry of the eclipsing binary system Cap has been presented. An improved period of 1d.022766 has been given. The duration of primary eclipse comes out to be more than double the duration given earlier. The depth has also been found to have increased. The light changes during eclipses show slight asymmetry. Eccentricity appears to be present in the system. Light and colour curves show variations. Primary component appears to be surrounded by a disc, the size of which is comparable to the size of the primary component. Two dips are seen around phases 0.20 and 0.67, the first appears more definitive, and is attributed to the wave-like distortion, like the one found in RS CVn binaries. The discussion reveals that Cap is a very complicated system. 相似文献
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A Bianchi type-I string cosmological model in Brans-Dicke theory in five dimension space-time has been investigated. For the
determinate solution it has been assumed that the sum of energy density and tension density of the cosmic string dust source
vanishes. Some physical and kinematical parameters are also discussed. 相似文献
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Hui-Rong Ji Qi-Jun Pu Yi-Hua Yan Yu-Ying Liu Zhi-Jun Chen Cheng-Ming Tan Cong-Ling Cheng De-Bang Lao Shu-Ke Li Zhi-Qiang Wang Min-Hong Yu Jian-Nong Liu Li-Kang Zhang Ji-Yong Gao National Astronomical Observatories Chinese Academy of Sciences Beijing Hebei Semiconductor Research Institute Shijiazhuang 《中国天文和天体物理学报》2005,5(4):433-441
An improved Solar Radio Spectrometer working at 1.10-2.06 GHz with much improved spectral and temporal resolution, has been accomplished by the National Astronomical Observatories and Hebei Semiconductor Research Institute, based on an old spectrometer at 1-2 GHz. The new spectrometer has a spectral resolution of 4 MHz and a temporal resolution of 5ms, with an instantaneous detectable range from 0.02 to 10 times of the quiet Sun flux. It can measure both left and right circular polarization with an accuracy of 10% in degree of polarization. Some results of preliminary observations that could not be recorded by the old spectrometer at 1-2 GHz are presented. 相似文献