Latest Images
Synthetic models associated with the star’s par...
The continuation of Figure 2 for the analyzed T...
Comparison between the observed spectrum (red d...
The continuation of Figures 2 and 3 for the ana...
The continuum-normalized synthetic spectra asso...
The continuum-normalized synthetic spectra asso...
A small portion of the γ R2 0-0 TiO band used i...
Identical to Figure 7, but for two analyzed Ti ...
Identical to Figure 7, but for one analyzed Fe ...
Model lightcurves for typical novae (left) and ...
Search field of the 1408 (super)nova. The verti...
Observation drawn by M. Hevelius (1670; left) a...
Near-IR color–magnitude and color–color diagram...
Near-IR spectra of brown dwarf candidates in Up...
Near-IR spectra of brown dwarf candidates in Up...
Near-IR color–magnitude diagram for members of ...
Proper motion offsets vs. parallactic distance ...
Mass vs. spectral type for young stars with mea...
IMFs for Upper Sco, Taurus, IC 348, Chamaeleon ...
W1−W2 vs. spectral type for late-type members o...
Analysis of filter outputs z∗ and ζ∗ from full ...
Illustration of synthetic filter outputs z∗ for...
Differences in angles Δθ between a run with bot...
Analysis of g frequencies. (a) Moving-window FF...
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