Latest Images
The waterfall (frequency-time) plot of the raw ...
Comparison result between the DBSCAN algorithm ...
Optimization of the Eps parameter for the DBSCA...
Visualizations of 14 interesting candidate grou...
Selection of the DBSCAN Eps parameter for ident...
Evaluation of processing speed for residual RFI...
Selected ETI candidates (33, black dots) and id...
Waterfall plot with the hits after removing per...
Sky map of Pleiades stars with reliable astrome...
Left: shift of binary systems with q = 0.75 in ...
Pleiades stars in the CMD using Gaia (top) and ...
Reported orbital periods and RUWE values for sp...
The mass ratios of SB2 binaries (Table 1) deriv...
Prediction of RUWE values for Pleiades stars us...
Left: RUWE values for resolved sources dependin...
Left: orbital periods according to Gaia DR3 NSS...
Binary-star candidates inferred from the CMD an...
The estimated mass ratios for unresolved binari...
Left: number of resolved and unresolved binarie...
Day-slot scheduling framework. AstroQ discretiz...
Distribution of sky coordinates from the nomina...
Construction of two accessibility maps. Each pa...
The fraction of times each calendar date was to...
Top: bird’s-eye view of the optimal semester sc...
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