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Optimization of Antenna Performance for Global 21-cm Observations and Verification Using Scaled Copies 全球21厘米观测的天线性能优化和使用标度副本的验证
IF 1.3 Q3 ASTRONOMY & ASTROPHYSICS Pub Date : 2023-05-26 DOI: 10.1142/s2251171723500058
Ó. Restrepo, F. Lucero, G. Chaparro, R. Rodríguez, F. Pizarro, R. Bustos, M. Diaz, F. Mena
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引用次数: 0
Integrated Computing Platform for Detection and Tracking of Unidentified Aerial Phenomena (UAP) 不明飞行物探测与跟踪综合计算平台
IF 1.3 Q3 ASTRONOMY & ASTROPHYSICS Pub Date : 2023-05-26 DOI: 10.1142/s2251171723400081
Richard Cloete, Phillip G. Bridgham, Sergei Dobroshinsky, Carson Ezell, Andriy Fedorenko, F. Laukien, Sarah Little, A. Loeb, Eric Masson, Matthew Szenher, W. Watters
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引用次数: 0
Optical Alignment Method for the PRIME Telescope PRIME望远镜的光学对准方法
IF 1.3 Q3 ASTRONOMY & ASTROPHYSICS Pub Date : 2023-05-11 DOI: 10.1142/S2251171723500046
H. Yama, D. Suzuki, S. Miyazaki, A. Rakich, T. Yamawaki, R. Kirikawa, I. Kondo, Y. Hirao, N. Koshimoto, T. Sumi
We describe the optical alignment method for the Prime-focus Infrared Microlensing Experiment (PRIME) telescope which is a prime-focus near-infrared (NIR) telescope with a wide field of view for the microlensing planet survey toward the Galactic center that is the major task for the PRIME project. There are three steps for the optical alignment: preliminary alignment by a laser tracker, fine alignment by intra- and extra-focal (IFEF) image analysis technique, and complementary and fine alignment by the Hartmann test. We demonstrated that the first two steps work well by the test conducted in the laboratory in Japan. The telescope was installed at the Sutherland Observatory of South African Astronomical Observatory in August, 2022. At the final stage of the installation, we demonstrated that the third method works well and the optical system satisfies the operational requirement.
本文介绍了PRIME项目的主要任务——面向银河系中心的微透镜行星巡天,是一种具有宽视场的近红外(NIR)望远镜。光学对准有三个步骤:用激光跟踪仪进行初步对准,用焦内焦外(IFEF)图像分析技术进行精细对准,用哈特曼测试进行互补和精细对准。我们通过在日本实验室进行的测试证明了前两个步骤的效果良好。该望远镜于2022年8月在南非天文台萨瑟兰天文台安装。在安装的最后阶段,我们证明了第三种方法效果良好,光学系统满足操作要求。
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引用次数: 1
Upgradation of AIMPOL instrument on the 104-cm Sampurnanand telescope of ARIES 白羊座104cm Sampurnanand望远镜上AIMPOL仪器的升级改造
IF 1.3 Q3 ASTRONOMY & ASTROPHYSICS Pub Date : 2023-05-11 DOI: 10.1142/s2251171722400086
J. Pandey, Sadhana Singh, R. Yadav, N. Nanjappa, Jayshreekar Pant, Mukesh Kumar, Sanjit Sahu
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引用次数: 2
Smartphone screens as astrometric calibrators 智能手机屏幕是天文测量校准器
IF 1.3 Q3 ASTRONOMY & ASTROPHYSICS Pub Date : 2023-03-09 DOI: 10.1142/s2251171723500095
Aidan Walk, C. Claveau, M. Bottom, M. Chun, S. Jacobson, M. Service, Jessica R. Lu
Geometric optical distortion is a significant contributor to the astrometric error budget in large telescopes using adaptive optics. To increase astrometric precision, optical distortion calibration is necessary. We investigate using smartphone OLED screens as astrometric calibrators. Smartphones are low cost, have stable illumination, and can be quickly reconfigured to probe different spatial frequencies of an optical system's geometric distortion. In this work, we characterize the astrometric accuracy of a Samsung S20 smartphone, with a view towards providing large format, flexible astrometric calibrators for the next generation of astronomical instruments. We find the placement error of the pixels to be 189 nm +/- 15 nm RMS. At this level of error, milliarcsecond astrometric accuracy can be obtained on modern astronomical instruments.
几何光学失真是使用自适应光学的大型望远镜天文测量误差预算的重要因素。为了提高天文测量精度,光学畸变校准是必要的。我们研究使用智能手机OLED屏幕作为天文校准器。智能手机成本低,照明稳定,可以快速重新配置,以探测光学系统几何失真的不同空间频率。在这项工作中,我们对三星S20智能手机的天体测量精度进行了表征,以期为下一代天文仪器提供大尺寸、灵活的天体测量校准器。我们发现像素的放置误差为189nm+/-15nmRMS。在这个误差水平上,现代天文仪器可以获得毫弧秒的天文测量精度。
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引用次数: 0
Preface: Instrumentation and Software for the Detection and Characterization of Unidentified Aerospace Phenomena 前言:用于探测和表征不明航天现象的仪器和软件
Q3 ASTRONOMY & ASTROPHYSICS Pub Date : 2023-03-01 DOI: 10.1142/s2251171723020014
Richard Cloete, Wesley Andrés Watters, Sarah Little, Abraham Loeb, Anthony Lux
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引用次数: 0
First study of optical turbulence over an astronomical site in the Central Himalayas using ST radar observations 首次使用ST雷达观测喜马拉雅山中部天文观测点的光学湍流
IF 1.3 Q3 ASTRONOMY & ASTROPHYSICS Pub Date : 2023-02-18 DOI: 10.1142/s2251171722400074
A. Jaiswal, M. Naja, S. Bhattacharjee, B. Kumar, S. Ananthakrishnan
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引用次数: 0
Characterization and performance of the 4k × 4k CCD camera mounted on 104-cm Sampurnanand telescope ×4k CCD相机的特性和性能
IF 1.3 Q3 ASTRONOMY & ASTROPHYSICS Pub Date : 2023-02-18 DOI: 10.1142/s2251171722400062
R. Yadav, Aditya Jaiswal, Arvind K. Dattatrey, S. Yadav, N. Nanjappa, N. Panwar, M. Jaiswar, Krishna Reddey, Jayshreekar Pant, B. Medhi
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引用次数: 0
ARIES ST Radar: The first Central Himalayan wind profiler ARIES ST雷达:第一个喜马拉雅中部风廓线仪
IF 1.3 Q3 ASTRONOMY & ASTROPHYSICS Pub Date : 2023-02-16 DOI: 10.1142/s2251171722400050
S. Bhattacharjee, M. Naja, A. Jaiswal, K. Rawat, R. Sagar, S. Ananthakrishnan
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引用次数: 0
Detection of Moving Objects in Earth Observation Satellite Images 对地观测卫星图像中运动物体的检测
IF 1.3 Q3 ASTRONOMY & ASTROPHYSICS Pub Date : 2023-01-17 DOI: 10.1142/s225117172340007x
E. Keto, W. Watters
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引用次数: 0
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Journal of Astronomical Instrumentation
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