Latest Images
Spatial distribution of 29 sample clusters over...
Distribution of 29 globular clusters: projected...
Comparison of metallicities derived from differ...
Joint spectral and photometric fitting for star...
Comparison of our final metallicity determinati...
Same as Figure 7 but comparing our derived ages...
Same as Figure 9 but for age versus projected g...
Same as Figure 5 but for the derived ages.
Cutout images of star cluster G002 in 12 filter...
QE curve of the Andor iKon-L 936 BEX2-DD CCD mo...
The spatial distribution of our M31 halo star c...
Impact of MIRI photometry on QG selection. Top ...
The mass-dependent number density evolution of ...
The UVJ color–color diagram for the photometric...
The redshift evolution of the QG fraction in di...
Left panel: the SMF of QGs at 2 < z < 8, fitted...
(Top left) The 2.1 μm (black) and 3–10 keV NuST...
(Left) Superimposed on the NIR light curve at 2...
(Left) Calculated time delay between pairs of r...
(Top left) Correlation of X-ray flare emission ...
(Top left) Light curve of Sgr A* at 2.1 μm take...
(Top) The blue curve shows the synchrotron flux...
(Top) The normal stellar field at 2.1 μm of NIR...
Predicted X-ray flare luminosities arising from...
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