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supported by the Natural Science Foundation of Tianjin Municipality(22JCYBJC00410);the National Natural Science Foundation of China-Chinese Academy of Sciences Joint Fund for Astronomy(U1931134)。
Spectral classification plays a crucial role in the analysis of astronomical data.Currently,stellar spectral classification primarily relies on one-dimensional(1D)spectra and necessitates a sufficient signal-to-noise ...
This work was supported by the Strategic Priority Research Program of the Chinese Academy of Sciences(grant XDA17010203,XDA17010201).
The Scientific Experimental system in Near SpacE(SENSE)consists of different types of instruments that will be installed on a balloon-based platform to characterize near-space environmental parameters.As one of the ma...
funded by the National Natural Science Foundation of China(NSFC,Nos.11803088,12003068 and 12063002);Civil Aerospace preresearch project D020302;the science research grants from the China Manned Space Project with NO.CMS-CSST-2021-B10;Yunnan Science Foundation of China(202001AU070077);SinoGerman Scientist Mobility Programme M-0086。
In 2016,an exposure meter was installed on the Lijiang Fiber-fed High-Resolution Spectrograph to monitor the coupling of starlight to the science fiber during observations.Based on it,we investigated a method to estim...
the International Partnership Program of the Chinese Academy of Sciences No.114A11-KYSB20200029;the National Natural Science Foundation of China(NSFC,Grant No.12041301);the National Key R&D Program of China No.2020YC2201700。
In this paper,we report a real-time Fast Radio Burst(FRB)searching system that has been successfully implemented with the 19 beam receiver of the Five-hundred-meter Aperture Spherical radio Telescope(FAST).The relativ...
supported by the National Natural Science Foundation of China(NSFC)grants 11703089 and 11903080;the support by the National SKA Program of China(No.2022SKA0120101);Yunnan Fundamental Research Projects(No.202301AT070325);the support by Kunming International Cooperation Base Project(GHJD-2021022);the support of Yunnan Key Laboratory of Solar physics and Space Science,Kunming(202205AG070009)。
The dynamic spectral observation at decametric wavelength is important to study solar radio physics and space weather.However,the observing system is difficult to observe with high sensitivity at this band due to the ...
supported by the China National Space Administration(CNSA)。
The Hα imaging spectrograph(HIS) is the scientific payload of the first solar space mission, the Chinese Hα solar explorer(CHASE), supported by the China National Space Administration(CNSA). The CHASE/HIS achieves, ...
support of the National Natural Science Foundation of China(Grant No.11503005);Jiangsu Students’ Innovation and Entrepreneurship Training Program(201910294155Y and 201810294059X);the National Undergraduate Training Program for Innovation and Entrepreneurship(201810294099).
The Large sky Area Multi-Object fiber Spectroscopic Telescope(LAMOST)is a Chinese national scientific research facility operated by National Astronomical Observatories,Chinese Academy of Sciences(NAOC).The LAMOST surv...
supported by the Joint Research Fund in Astronomy (U1531242) under cooperative agreement between the National Natural Science Foundation of China (NSFC) and Chinese Academy of Sciences (CAS);the NSFC (No. 11673036);the Interdiscipline Research Funds of Beijing Normal University;Funding for the project has been provided by the National Development and Reform Commission
We use the Richardson-Lucy deconvolution algorithm to extract one-dimensional(1 D) spectra from Large Sky Area Multi-Object Fiber Spectroscopic Telescope(LAMOST) spectrum images. Compared with other deconvolution algo...
supported by the Open Project Program of the Key Laboratory of Optical Astronomy,National Astronomical Observatories,Chinese Academy of Sciences;the National Natural Science Foundation of China(Grant Nos.11503045 and 11373003);National Program on Key Research and Development Project(2016YFA0400804);National Key Basic Research Program of China(2015CB857002)
The Beijing Faint Object Spectrograph and Camera (BFOSC) is one of the most important instruments operating in conjunction with the 2.16-m telescope at Xinglong Observatory. Every year there are - 20 SCI-papers publ...
supported by the National Natural Science Foundation of China(41331068,11503014 and U1431103);the China Postdoctoral Science Foundation(2016M600538)
Observation and research on solar radio emission have unique scientific values in solar and space physics and related space weather forecasting applications, since the observed spectral structures may carry important ...