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(a) Schematic illustration of the emission geom...

(a) Schematic illustration of the emission geometry. The emission beam is centered on ...

Yejing Zhan et al, The Astrophysical Journal Letters 1004 2

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(a) Same as Figure 1(b), but with an illustrati...

(a) Same as Figure 1(b), but with an illustrative few-degree-order drift on the magnetic...

Yejing Zhan et al, The Astrophysical Journal Letters 1004 2

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The dependence of the period evolution on the s...

The dependence of the period evolution on the secondary mass M2 and the primary tidal fa...

Yejing Zhan et al, The Astrophysical Journal Letters 1004 2

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Comparison of two image-combination statistics ...

Comparison of two image-combination statistics applied to a planted moving object of mag...

Nitya Pandey et al, The Astronomical Journal 172 1

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Left: a newly detected object (m ∼ 20.5), not p...

Left: a newly detected object (m ∼ 20.5), not previously reported in the DEEP catalog, i...

Nitya Pandey et al, The Astronomical Journal 172 1

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On-sky positions of DECam field pointings for q...

On-sky positions of DECam field pointings for quadrant B1. The footprint consists of 29 ...

Nitya Pandey et al, The Astronomical Journal 172 1

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Detection efficiency as a function of magnitude...

Detection efficiency as a function of magnitude difference relative to the DEEP survey l...

Nitya Pandey et al, The Astronomical Journal 172 1

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Upper panels show a synthetic moving object at ...

Upper panels show a synthetic moving object at three representative epochs (image indice...

Nitya Pandey et al, The Astronomical Journal 172 1

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Cumulative magnitude distribution of TNOs in th...

Cumulative magnitude distribution of TNOs in the analyzed DEEP survey fields shown in Fi...

Nitya Pandey et al, The Astronomical Journal 172 1

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Panels (a) and (c) show the objects flagged by ...

Panels (a) and (c) show the objects flagged by the machine learning model, n2720 and n34...

Nitya Pandey et al, The Astronomical Journal 172 1

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Detections by our best-trained model marked wit...

Detections by our best-trained model marked with blue boxes labeled “Moving Obj,” and th...

Nitya Pandey et al, The Astronomical Journal 172 1

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Comparison between implanted magnitudes for syn...

Comparison between implanted magnitudes for synthetic objects and their measured photome...

Nitya Pandey et al, The Astronomical Journal 172 1

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Rock and ice components in the debris disk as a...

Rock and ice components in the debris disk as a function of Limp for different EOSs in D...

Keiya Murashima and Takanori Sasaki, The Astrophysical Journal 1005 1

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Rock and ice components in the debris disk as a...

Rock and ice components in the debris disk as a function of Limp for different EOSs in S...

Keiya Murashima and Takanori Sasaki, The Astrophysical Journal 1005 1

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Characteristic disk size 〈rd,imp〉 as a function...

Characteristic disk size 〈rd,imp〉 as a function of the initial angular momentum, for (a)...

Keiya Murashima and Takanori Sasaki, The Astrophysical Journal 1005 1

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Disk mass Md,imp as a function of the initial a...

Disk mass Md,imp as a function of the initial angular momentum, for (a) SSPH and (b) DIS...

Keiya Murashima and Takanori Sasaki, The Astrophysical Journal 1005 1

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Median rotation periods of the post-impact plan...

Median rotation periods of the post-impact planets as a function of the impact angular m...

Keiya Murashima and Takanori Sasaki, The Astrophysical Journal 1005 1

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Initial density profiles of the target (left co...

Initial density profiles of the target (left column) and the impactor (right column) uti...

Keiya Murashima and Takanori Sasaki, The Astrophysical Journal 1005 1

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Snapshots of a collision with an Limp = 3 × 103...

Snapshots of a collision with an Limp = 3 × 1036 kg m2 s−1 using SESAME and ANEOS EOS wi...

Keiya Murashima and Takanori Sasaki, The Astrophysical Journal 1005 1

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The same as Figure 10, except for a low-impact ...

The same as Figure 10, except for a low-impact parameter Limp = 5 × 1036 kg m2 s−1.

Keiya Murashima and Takanori Sasaki, The Astrophysical Journal 1005 1

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The same as Figure 10, except for a high-impact...

The same as Figure 10, except for a high-impact parameter Limp = 7 × 1036 kg m2 s−1.

Keiya Murashima and Takanori Sasaki, The Astrophysical Journal 1005 1

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Rock and ice components in the disk as a functi...

Rock and ice components in the disk as a function of Limp for different EOSs in SSPH (ap...

Keiya Murashima and Takanori Sasaki, The Astrophysical Journal 1005 1

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Rock and ice components in the disk as a functi...

Rock and ice components in the disk as a function of Limp. Left panel: baseline simulati...

Keiya Murashima and Takanori Sasaki, The Astrophysical Journal 1005 1

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Density map of snapshots of second collision fo...

Density map of snapshots of second collision for SESAME/ANEOS (left), Tillotson EOS (cen...

Keiya Murashima and Takanori Sasaki, The Astrophysical Journal 1005 1

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Snapshots of the second collision with DISPH an...

Snapshots of the second collision with DISPH and Limp = 7.0 × 1036 kg m2 s−1 for SESAME/...

Keiya Murashima and Takanori Sasaki, The Astrophysical Journal 1005 1

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