Astronomy Image Explorer

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(a) The GOES soft X-ray light curves in 1.0−8.0...

(a) The GOES soft X-ray light curves in 1.0−8.0 Å and 0.5−4.0 Å from 02:00 to 04:00 UT o...

Ayumi Asai et al, The Astrophysical Journal Letters 1008 1

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(a) Line-center image of the Na D1 at 03:04:36 ...

(a) Line-center image of the Na D1 at 03:04:36 UT obtained with DST. The red box indicat...

Ayumi Asai et al, The Astrophysical Journal Letters 1008 1

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(a) Time sequence images of the flare kernel ob...

(a) Time sequence images of the flare kernel observed with DST in the Ca 8542 line cente...

Ayumi Asai et al, The Astrophysical Journal Letters 1008 1

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(a) Ca 8542 line-center image of the flare kern...

(a) Ca 8542 line-center image of the flare kernel at 03:04:15 UT observed with SCIP. Col...

Ayumi Asai et al, The Astrophysical Journal Letters 1008 1

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(a) SCIP Ca 8542 line-center image taken in the...

(a) SCIP Ca 8542 line-center image taken in the raster scan starting at 03:10:31 UT. The...

Ayumi Asai et al, The Astrophysical Journal Letters 1008 1

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Joint posterior constraints of e–ω from our pho...

Joint posterior constraints of e–ω from our photoeccentric-effect analysis. Each mini-co...

Tyler R. Fairnington et al, The Astrophysical Journal Letters 1008 1

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Orbital eccentricity (in e2) versus semimajor a...

Orbital eccentricity (in e2) versus semimajor axis for the planet sample with eccentrici...

Tyler R. Fairnington et al, The Astrophysical Journal Letters 1008 1

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Posterior eccentricity distribution for the ful...

Posterior eccentricity distribution for the full warm-single planet sample (1–16 R⊕) inf...

Tyler R. Fairnington et al, The Astrophysical Journal Letters 1008 1

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Planet radius versus orbital period for the fin...

Planet radius versus orbital period for the final sample. Points and error bars represen...

Tyler R. Fairnington et al, The Astrophysical Journal Letters 1008 1

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Eccentricity–radius diagram for the planet samp...

Eccentricity–radius diagram for the planet sample. Points show the mode eccentricity, wi...

Tyler R. Fairnington et al, The Astrophysical Journal Letters 1008 1

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Radius dependence of eccentricity for the warm ...

Radius dependence of eccentricity for the warm sample. Gray contours show the density of...

Tyler R. Fairnington et al, The Astrophysical Journal Letters 1008 1

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Inferred low-eccentricity mixture fraction πlow...

Inferred low-eccentricity mixture fraction πlow(Rp) from the continuous sigmoid mixture ...

Tyler R. Fairnington et al, The Astrophysical Journal Letters 1008 1

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Same as Figure A1 but for giant planets (Rp > 8...

Same as Figure A1 but for giant planets (Rp > 8 R⊕).

Tyler R. Fairnington et al, The Astrophysical Journal Letters 1008 1

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Host–planet properties for the Rp < 4 R⊕ subsam...

Host–planet properties for the Rp < 4 R⊕ subsample. Planet radius is shown as a function...

Tyler R. Fairnington et al, The Astrophysical Journal Letters 1008 1

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Posterior eccentricity distributions for three ...

Posterior eccentricity distributions for three planet size classes derived from hierarch...

Tyler R. Fairnington et al, The Astrophysical Journal Letters 1008 1

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Same as Figure 6, except we also show the restr...

Same as Figure 6, except we also show the restricted confirmed and SG1-cleared planets i...

Tyler R. Fairnington et al, The Astrophysical Journal Letters 1008 1

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Same as Figure 6 but including more discrete bi...

Same as Figure 6 but including more discrete bin-size analyses: Δ1.0 Rp (blue), Δ1.5 Rp ...

Tyler R. Fairnington et al, The Astrophysical Journal Letters 1008 1

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Corner plot of fiducial three-stage sigmoid model.

Corner plot of fiducial three-stage sigmoid model.

Tyler R. Fairnington et al, The Astrophysical Journal Letters 1008 1

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Same as Figure 6 but showing the full sample (b...

Same as Figure 6 but showing the full sample (blue) compared to the GKM-type host target...

Tyler R. Fairnington et al, The Astrophysical Journal Letters 1008 1

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Disentangling the primary drivers of the signal...

Disentangling the primary drivers of the signal. Similar to Figure 2, but in each panel ...

Peng Wang et al, The Astrophysical Journal Letters 1008 1

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The dependence of the angle θ, between the sate...

The dependence of the angle θ, between the satellite orbital-normal vector ...

Peng Wang et al, The Astrophysical Journal Letters 1008 1

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Mean angle 〈θ〉 as a function of distance to the...

Mean angle 〈θ〉 as a function of distance to the nearest filament spine Dfil, measured us...

Peng Wang et al, The Astrophysical Journal Letters 1008 1

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Probability density distribution (PDF) of the a...

Probability density distribution (PDF) of the alignment angle θ between the projected sa...

Peng Wang et al, The Astrophysical Journal Letters 1008 1

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Panel (A): intrinsic polarization of SN 2026gzf...

Panel (A): intrinsic polarization of SN 2026gzf at day 16.5. The debiased degree of pola...

Xudong Wen et al, The Astrophysical Journal Letters 1008 1

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Spectropolarimetry of SN 2026gzf at 16.5 days a...

Spectropolarimetry of SN 2026gzf at 16.5 days after the X-ray shock breakout. The left c...

Xudong Wen et al, The Astrophysical Journal Letters 1008 1

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ANNOUNCEMENTS

Updated Search and Sort

We have updated the search and sort algorithm to return records in reverse chronological order based on the date/time that the images were uploaded to the Astronomy Image Explorer. This is potentially but rarely different from the publication date. Thank you!