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Mutual orbit period change in seconds due to Di...

Mutual orbit period change in seconds due to Didymos’s shape change process that include...

Masatoshi Hirabayashi et al, The Planetary Science Journal 7 9

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Thickness change at the equator after ejecta ac...

Thickness change at the equator after ejecta accumulation on Didymos (Modification I), i...

Masatoshi Hirabayashi et al, The Planetary Science Journal 7 9

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Thickness change at the equator after spin-driv...

Thickness change at the equator after spin-driven reshaping (Modification II). This quan...

Masatoshi Hirabayashi et al, The Planetary Science Journal 7 9

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Spin period change with ejecta mass. Panel (a) ...

Spin period change with ejecta mass. Panel (a) shows the case when the average initial e...

Masatoshi Hirabayashi et al, The Planetary Science Journal 7 9

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Thickness change at the equator after spin-driv...

Thickness change at the equator after spin-driven reshaping (Modification II) for all th...

Masatoshi Hirabayashi et al, The Planetary Science Journal 7 9

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Schematics of DART impact and the following res...

Schematics of DART impact and the following reshaping processes. (a) The DART spacecraft...

Masatoshi Hirabayashi et al, The Planetary Science Journal 7 9

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Net thickness change at the equator including b...

Net thickness change at the equator including both Modifications I and II. The contour p...

Masatoshi Hirabayashi et al, The Planetary Science Journal 7 9

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Net thickness change at the equator including b...

Net thickness change at the equator including both Modifications I and II for all the sh...

Masatoshi Hirabayashi et al, The Planetary Science Journal 7 9

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Mutual orbit period change in seconds for all t...

Mutual orbit period change in seconds for all the shape cases. Each panel shows a differ...

Masatoshi Hirabayashi et al, The Planetary Science Journal 7 9

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Outcomes given ejecta accumulation only along D...

Outcomes given ejecta accumulation only along Didymos’s equator, which makes a hypotheti...

Masatoshi Hirabayashi et al, The Planetary Science Journal 7 9

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Observations of the SN 2025ulz field carried ou...

Observations of the SN 2025ulz field carried out at ν ≈ 6 GHz under our JAGWAR program w...

Tanner O’Dwyer et al, The Astrophysical Journal Letters 1009 2

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VLA images of the SN 2025ulz field at ≈10 GHz. ...

VLA images of the SN 2025ulz field at ≈10 GHz. In all panels, we show a black circle cen...

Tanner O’Dwyer et al, The Astrophysical Journal Letters 1009 2

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Observations of the SN 2025ulz field carried ou...

Observations of the SN 2025ulz field carried out at ν ≈ 10 GHz under our JAGWAR program ...

Tanner O’Dwyer et al, The Astrophysical Journal Letters 1009 2

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Radio observations of SN 2025ulz. We show upper...

Radio observations of SN 2025ulz. We show upper limits (downward triangles), ≥5σ detecti...

Tanner O’Dwyer et al, The Astrophysical Journal Letters 1009 2

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A Chevalier diagram (peak radio luminosity vers...

A Chevalier diagram (peak radio luminosity versus peak time) with the 10 GHz detection (...

Tanner O’Dwyer et al, The Astrophysical Journal Letters 1009 2

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The radio light curves of SN 2025ulz compared t...

The radio light curves of SN 2025ulz compared to that of Type IIb SNe. For SN 2025ulz, w...

Tanner O’Dwyer et al, The Astrophysical Journal Letters 1009 2

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Observations of the SN 2025ulz field carried ou...

Observations of the SN 2025ulz field carried out at ν ≈ 3 GHz under our JAGWAR program w...

Tanner O’Dwyer et al, The Astrophysical Journal Letters 1009 2

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Constraints on the hypothetical planet in the o...

Constraints on the hypothetical planet in the obliquity-tide scenario, under assumptions...

Caleb Lammers et al, The Astrophysical Journal Letters 1009 2

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First panel: WASP-12’s RV dataset, folded with ...

First panel: WASP-12’s RV dataset, folded with respect to the period of WASP-12 b (trans...

Caleb Lammers et al, The Astrophysical Journal Letters 1009 2

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RV constraints on companions of WASP-12 b. The ...

RV constraints on companions of WASP-12 b. The color conveys the fraction of injected si...

Caleb Lammers et al, The Astrophysical Journal Letters 1009 2

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Observations. Panel (a) shows AR 13738 in the 3...

Observations. Panel (a) shows AR 13738 in the 30.4 nm passband of SDO/AIA. The cyan rect...

Matheus Kriginsky et al, The Astrophysical Journal Letters 1009 2

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Inversion results. The first panel shows repres...

Inversion results. The first panel shows representative observed spectral profiles aroun...

Matheus Kriginsky et al, The Astrophysical Journal Letters 1009 2

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Evolution of the pore coalescence event in the ...

Evolution of the pore coalescence event in the field of view of the blue rectangle of Fi...

Matheus Kriginsky et al, The Astrophysical Journal Letters 1009 2

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WFA results. The first and second panels show t...

WFA results. The first and second panels show the BLoS maps around the pore for the firs...

Matheus Kriginsky et al, The Astrophysical Journal Letters 1009 2

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Loop geometry approximation. The left panel sho...

Loop geometry approximation. The left panel shows the comparison between the spatial var...

Matheus Kriginsky et al, The Astrophysical Journal Letters 1009 2

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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!