methods:dataanalysis相关论文
Observing a telluric standard star for correcting the telluric absorption lines of spectrum will take a significant amou......
Spectral deconvolution analysis on Olivine-Orthopyroxene mixtures with simulated space weathering mo
Olivine and pyroxene are important mineral end-members for studying the surface material compositions of mafic bodies.Th......
Magnetar giant flare originating from GRB 200415A:transient GeV emission,time-resolved Ep-Liso corre
Giant flares (GFs) are unusual bursts from soft gamma-ray repeaters (SGRs) that release an enormous amount of energy in ......
Testing the effect of solar wind parameters and geomagnetic storm indices on Galactic cosmic ray flu
Forbush decrease (FD),discovered by Scott E.Forbush about 80 years ago,is referred to as the non-repetitive short-term d......
PolarLight is a space-borne X-ray polarimeter that measures the X-ray polarization via electron tracking in an ionizatio......
Spectrum denoising is an important procedure for large-scale spectroscopical surveys.This work proposes a novel stellar ......
Lucky imaging is a high-resolution astronomical image recovery technique with two classic implementation algorithms,i.e.......
Prominence plumes are evacuated upflows that emerge from bubbles below prominences,whose formation mechanism is still un......
The continuous observation of the magnetic field by the Solar Dynamics Observatory(SDO)/Helioseismic and Magnetic Imager......
Spatial modulation search applied to the search and confirmation of highly scintillated pulsars at F
We present a pulsar candidate identification and confirmation procedure based on a position-switch mode during the pulsa......
Pulsars are very stable spinning stars,which have the potential to application in the work of time-keeping and autonomou......
Radioheliograph images are essential for the study of solar short term activities and long term variations,while the con......
A star-based method for precise wavelength calibration of the Chinese Space Station Telescope (CSST)
The Chinese Space Station Telescope (CSST) spectroscopic survey aims to deliver high-quality low-resolution (R ＞ 200) sli......
Deconvolution is used to eliminate imperfections in the point spread function,such as sidelobes caused by incomplete sam......
A method to obtain the wind field characteristics of super-large aperture radio telescope site based
The influence of wind on the pointing accuracy of large aperture radio telescopes is becoming increasingly serious,espec......
A filament is an important structure for studying star formation,especially intersections of filaments which are believe......
In this work,we train three decision-tree based ensemble machine learning algorithms (Random Forest Classifier,Adaptive ......
A sky model from CLEAN deconvolution is a particularly effective high dynamic range reconstruction in radio astronomy,wh......
A longitudinal magnetic field often suffers the saturation effect in a strong magnetic field region when the measurement......
The present investigation attempts to quantify the temporal variation of Solar Flare Index (SFI)with other activity indi......
In 21 cm intensity mapping,the spectral smoothness of the foreground is exploited to separate it from the much weaker 21......
The LE is the low energy telescope that is carried on Insight-HXMT.It uses swept charge devices(SCDs) to detect soft X-r......
