Latest Images
The registered Tio images observed by NVST and ...
Architecture of the method. By inputting two im...
NVST QS TiO images. (a) The fixed image at 01:1...
NVST QS Hα 0. 6 nm images. (a), (b) The fixed i...
GST AR images. (a) Hα wing image at 20:39:52 UT...
Binary properties found in the conditioned subs...
The second-highest S/NΛ vs. maximum S/NΛ, color...
Each panel shows a histogram of the 68th percen...
The y-axis shows the chirp mass recovery precis...
Bayes factor (left) and detection fraction (rig...
Localization of successfully detected CWs in th...
Same as Figure 1 but using S/Ns (left) and S/Nρ...
Same as Figure 4 but with the x-axis as S/Ns (l...
Same as Figure 6 but for S/Ns (left) and S/Nρ (...
Distributions of successful (blue) and failed (...
The y-axes show 68% CI posterior widths as a fr...
Each panel shows the recovery vs. injected valu...
The top panel shows the median Bayes factor vs....
Left: Digital Sky Survey POSS2 near-IR (0.85 μm...
Top: 2MASS color–color diagram for all Chandra ...
Top left: binned Chandra ACIS-I image (0.5–7 ke...
X-ray spectra with possible emission lines mark...
Properties of Chandra Norma sources based on 0....
Real-time tracks of the spider observation towa...
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