Latest Images
Differential light curves for CD Cyg using a pe...
Top-left panel: slit-reconstructed intensity ma...
Top panels: (first row) T for NOAA AR 12480 at ...
Some thermodynamic quantities recovered by STiC...
For the full FoV (FFOV, blue line) and the RoIs...
Uncertainty multiplication factor (UMFp, see Eq...
Flux upper limits of FRB 180814.J0422+73 in the...
Constraints of the initial spin period and the ...
Constraints on the isotropic kinetic energy of ...
Stacked TESS images of the 11 × 11 pixel stamps...
Plot of the median-normalized and outlier-remov...
Top panel: phase-folded light curve, after corr...
Lomb–Scargle (top) and double-harmonic (bottom)...
Long-term (left panel) and short-term (right pa...
Period ratios of adjacent transiting planets wh...
Expected multiplicity ratio (...
Expected multiplicity ratio ...
Contours of the minimum eccentricity and inclin...
Example of a possible evolution to produce a sy...
Maximum eccentricities reached by a Kepler-10b-...
Fraction of USP planets formed (i.e., reaching ...
Inclination distributions for Kepler-10b from o...
Eccentricity distributions for the Kepler-10b p...
Initial period from which the USP planets start...
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