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The expected number of detection counts in a bi...

The expected number of detection counts in a bin of size Δx for objects of different SNR...

Steven Stetzler et al, The Astronomical Journal 170 6

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The on-sky coordinates of a moving object with ...

The on-sky coordinates of a moving object with respect to time. The dashed black line re...

Steven Stetzler et al, The Astronomical Journal 170 6

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The number of peaks and pixels in a likelihood ...

The number of peaks and pixels in a likelihood image derived from a 2048 × 4096 CCD diff...

Steven Stetzler et al, The Astronomical Journal 170 6

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The distributions of the velocities and magnitu...

The distributions of the velocities and magnitudes of the injected synthetic MBAs and TNOs.

Steven Stetzler et al, The Astronomical Journal 170 6

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The m50 depth from fitting of the completeness ...

The m50 depth from fitting of the completeness (left), the number of candidate detection...

Steven Stetzler et al, The Astronomical Journal 170 6

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Distributions of average separation between the...

Distributions of average separation between the ground truth and recovered trajectories ...

Steven Stetzler et al, The Astronomical Journal 170 6

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A visualization of the sky locations of a stack...

A visualization of the sky locations of a stacked detection catalog derived from a 4 hr ...

Steven Stetzler et al, The Astronomical Journal 170 6

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The m50 depth achieved for the TNO (blue) and M...

The m50 depth achieved for the TNO (blue) and MBA (orange) searches as a function of the...

Steven Stetzler et al, The Astronomical Journal 170 6

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The fraction of synthetic objects recovered as ...

The fraction of synthetic objects recovered as a function of their magnitude for the TNO...

Steven Stetzler et al, The Astronomical Journal 170 6

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The CPU time and memory usage of our algorithm ...

The CPU time and memory usage of our algorithm as a function of the m50 depth achieved. ...

Steven Stetzler et al, The Astronomical Journal 170 6

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The median wall-clock runtime and memory usage ...

The median wall-clock runtime and memory usage of our catalog shift-and-stack algorithm ...

Steven Stetzler et al, The Astronomical Journal 170 6

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The CPU time and memory usage of the core-searc...

The CPU time and memory usage of the core-search component of our algorithm as a functio...

Steven Stetzler et al, The Astronomical Journal 170 6

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The fraction of synthetic TNOs recovered as a f...

The fraction of synthetic TNOs recovered as a function of their magnitude using KBMOD an...

Steven Stetzler et al, The Astronomical Journal 170 6

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The relative total CPU time (speedup) and memor...

The relative total CPU time (speedup) and memory usage of our algorithm when compared to...

Steven Stetzler et al, The Astronomical Journal 170 6

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The relative core-search CPU time (speedup) and...

The relative core-search CPU time (speedup) and memory usage of our algorithm compared t...

Steven Stetzler et al, The Astronomical Journal 170 6

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12″ × 12″ cutouts of the four most CO-luminous ...

12″ × 12″ cutouts of the four most CO-luminous SQuIGG﹩\overrightarrow{L}﹩E galaxies in ...

David J. Setton et al, The Astronomical Journal 170 6

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SQuIGG﹩\overrightarrow{L}﹩E is an SDSS-selecte...

SQuIGG﹩\overrightarrow{L}﹩E is an SDSS-selected sample of 1318 massive (...

David J. Setton et al, The Astronomical Journal 170 6

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Demonstration of the new SED fitting adopted in...

Demonstration of the new SED fitting adopted in this work, including MIR and FIR photome...

David J. Setton et al, The Astronomical Journal 170 6

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﹩{M}_{{{\rm{H}}}_{2}}﹩ mass (assuming r21 and ...

﹩{M}_{{{\rm{H}}}_{2}}﹩ mass (assuming r21 and αCO = 4.0, left) and molecular gas fracti...

David J. Setton et al, The Astronomical Journal 170 6

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Redshift vs. molecular gas fraction for passive...

Redshift vs. molecular gas fraction for passive galaxies with ...

David J. Setton et al, The Astronomical Journal 170 6

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Demonstration of the new SED fitting adopted in...

Demonstration of the new SED fitting adopted in this work, as in Figure 6. Here, we high...

David J. Setton et al, The Astronomical Journal 170 6

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Star-forming main sequence, with the best fit f...

Star-forming main sequence, with the best fit from J. Leja et al. (2022) at z = 0.7 show...

David J. Setton et al, The Astronomical Journal 170 6

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Demonstration of the new SED fitting adopted in...

Demonstration of the new SED fitting adopted in this work, as in Figure 6. Here, we high...

David J. Setton et al, The Astronomical Journal 170 6

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Comparison of the inferred total IR luminosity ...

Comparison of the inferred total IR luminosity (defined as the total luminosity coming f...

David J. Setton et al, The Astronomical Journal 170 6

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Molecular gas mass vs. SFR. As background conto...

Molecular gas mass vs. SFR. As background contours, we show literature star-forming samp...

David J. Setton et al, The Astronomical Journal 170 6

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