Latest Images

Magnitude distribution of our full target sampl...

Characterizing K2 Candidate Planetary S...

Magnitude distribution of our full target sample in the Kepler bandpass (Kp; blue) and K...

The Astrophysical Journal 836 2 167

Distribution of visually assigned spectral type...

Characterizing K2 Candidate Planetary S...

Distribution of visually assigned spectral types for the 74 stars in our cool dwarf sample.

The Astrophysical Journal 836 2 167

Repeatability of our equivalent width measureme...

Characterizing K2 Candidate Planetary S...

Repeatability of our equivalent width measurements when using the same instrument for bo...

The Astrophysical Journal 836 2 167

Repeatability of parameter estimates for the su...

Characterizing K2 Candidate Planetary S...

Repeatability of parameter estimates for the subsample of 15 stars with two observations...

The Astrophysical Journal 836 2 167

Comparison of temperatures derived using EW-bas...

Characterizing K2 Candidate Planetary S...

Comparison of temperatures derived using EW-based estimates from Newton et al. (2015) an...

The Astrophysical Journal 836 2 167

Numerical spectral types automatically derived ...

Characterizing K2 Candidate Planetary S...

Numerical spectral types automatically derived from the ﹩{{\rm{H}}}_{2}{\rm{O}}﹩-K2 inde...

The Astrophysical Journal 836 2 167

Temperatures from Newton et al. (2015) EW-based...

Characterizing K2 Candidate Planetary S...

Temperatures from Newton et al. (2015) EW-based relation (circles) and Mann et al. (2013...

The Astrophysical Journal 836 2 167

Estimated metallicities for the 63 cool dwarfs ...

Characterizing K2 Candidate Planetary S...

Estimated metallicities for the 63 cool dwarfs with spectral types of K7 or later. The t...

The Astrophysical Journal 836 2 167

Comparison of radii derived directly using the ...

Characterizing K2 Candidate Planetary S...

Comparison of radii derived directly using the Newton et al. (2015) relations and indire...

The Astrophysical Journal 836 2 167

Comparison of temperatures and radii derived us...

Characterizing K2 Candidate Planetary S...

Comparison of temperatures and radii derived using relations from Newton et al. (2015) a...

The Astrophysical Journal 836 2 167

Revised parameters for the cool dwarf sample. L...

Characterizing K2 Candidate Planetary S...

Revised parameters for the cool dwarf sample. Left: revised stellar luminosity vs. stell...

The Astrophysical Journal 836 2 167

Distribution of radii (top) and effective tempe...

Characterizing K2 Candidate Planetary S...

Distribution of radii (top) and effective temperatures (bottom) for the stars in our coo...

The Astrophysical Journal 836 2 167

Comparison of our revised stellar parameters (c...

Characterizing K2 Candidate Planetary S...

Comparison of our revised stellar parameters (circles) to the earlier estimates from oth...

The Astrophysical Journal 836 2 167

Reduced proper motion in J band vs. J − H for a...

Characterizing K2 Candidate Planetary S...

Reduced proper motion in J band vs. J − H for all of the stars we observed and later cla...

The Astrophysical Journal 836 2 167

Y-band (top left), J-band (top right), H-band (...

Characterizing K2 Candidate Planetary S...

Y-band (top left), J-band (top right), H-band (bottom left), and K-band (bottom right) s...

The Astrophysical Journal 836 2 167

Same as Figure 15 for cool dwarfs with effectiv...

Characterizing K2 Candidate Planetary S...

Same as Figure 15 for cool dwarfs with effective temperatures between 4480 and 4333 K.

The Astrophysical Journal 836 2 167

Same as Figure 15 for cool dwarfs with effectiv...

Characterizing K2 Candidate Planetary S...

Same as Figure 15 for cool dwarfs with effective temperatures between 4333 and 3995 K.

The Astrophysical Journal 836 2 167

Same as Figure 15 for cool dwarfs with effectiv...

Characterizing K2 Candidate Planetary S...

Same as Figure 15 for cool dwarfs with effective temperatures between 3995 and 3650 K.

The Astrophysical Journal 836 2 167

Same as Figure 15 for cool dwarfs with effectiv...

Characterizing K2 Candidate Planetary S...

Same as Figure 15 for cool dwarfs with effective temperatures between 3650 and 3465 K.

The Astrophysical Journal 836 2 167

Same as Figure 15 for cool dwarfs with effectiv...

Characterizing K2 Candidate Planetary S...

Same as Figure 15 for cool dwarfs with effective temperatures between 3465 and 3220 K.

The Astrophysical Journal 836 2 167

Y-band (top left), J-band (top right), H-band (...

Characterizing K2 Candidate Planetary S...

Y-band (top left), J-band (top right), H-band (bottom left), and K-band (bottom right) s...

The Astrophysical Journal 836 2 167

Same as Figure 21 for hotter dwarfs with spectr...

Characterizing K2 Candidate Planetary S...

Same as Figure 21 for hotter dwarfs with spectral types between K3 and K2.

The Astrophysical Journal 836 2 167

Same as Figure 21 for hotter dwarfs with spectr...

Characterizing K2 Candidate Planetary S...

Same as Figure 21 for hotter dwarfs with spectral types between K5 and K3. Although some...

The Astrophysical Journal 836 2 167

Y-band (top left), J-band (top right), H-band (...

Characterizing K2 Candidate Planetary S...

Y-band (top left), J-band (top right), H-band (bottom left), and K-band (bottom right) s...

The Astrophysical Journal 836 2 167

Same as Figure 24 for giant stars with spectral...

Characterizing K2 Candidate Planetary S...

Same as Figure 24 for giant stars with spectral types between K1 and M2.

The Astrophysical Journal 836 2 167

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New Release of the Astronomy Image Explorer!

A new release of the AAS's Astronomy Image Explorer occurred on May 5, 2016.

This release updates the search and sorting features based on user feedback; adds links to videos and interactive figures in our Journal articles; provides a new way for publishers to add images to the AIE. Get in touch to hear more!