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Histograms of the posterior samples for the inc...

Histograms of the posterior samples for the inclination-distribution concentration ...

Pedro H. Bernardinelli et al, The Astronomical Journal 169 6

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Ternary histograms of (fNIRF, fNIRB+, fNIRB−) p...

Ternary histograms of (fNIRF, fNIRB+, fNIRB−) posterior samples for the HC, detached, an...

Pedro H. Bernardinelli et al, The Astronomical Journal 169 6

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Each panel has differential (top) and cumulativ...

Each panel has differential (top) and cumulative (bottom) histograms of the 68% confiden...

Pedro H. Bernardinelli et al, The Astronomical Journal 169 6

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Similar to Figure 11, but showing (fNIRB, fNIRF...

Similar to Figure 11, but showing (fNIRB, fNIRF+, fNIRF−) posterior samples. The red dot...

Pedro H. Bernardinelli et al, The Astronomical Journal 169 6

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Completeness as a function of Hr (top left), in...

Completeness as a function of Hr (top left), inclination (top right), and the three colo...

Pedro H. Bernardinelli et al, The Astronomical Journal 169 6

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Realizations of the NIRB and NIRF color familie...

Realizations of the NIRB and NIRF color families as in Figure 1 where each component has...

Pedro H. Bernardinelli et al, The Astronomical Journal 169 6

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Each panel shows the 68% limits of the data dis...

Each panel shows the 68% limits of the data distributions per dynamical class (black) as...

Pedro H. Bernardinelli et al, The Astronomical Journal 169 6

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Realizations of the NIRB± and NIRF± color fam...

Realizations of the NIRB± and NIRF± color families as in Figure 10, and the g − r, r −...

Pedro H. Bernardinelli et al, The Astronomical Journal 169 6

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g − r, r − i and r − z histograms of 5 × 105 re...

g − r, r − i and r − z histograms of 5 × 105 realizations of the model from Table 1, as ...

Pedro H. Bernardinelli et al, The Astronomical Journal 169 6

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Similar to Figure 7, where the TNOs are now spl...

Similar to Figure 7, where the TNOs are now split into bins of inclination. The left pan...

Pedro H. Bernardinelli et al, The Astronomical Journal 169 6

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Posterior distributions of fNIRB∣d after margin...

Posterior distributions of fNIRB∣d after marginalizing over physical hyperparameters of ...

Pedro H. Bernardinelli et al, The Astronomical Journal 169 6

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Similar to Figure 4, this figure shows posterio...

Similar to Figure 4, this figure shows posterior contours for the NIRB (left) and NIRF (...

Pedro H. Bernardinelli et al, The Astronomical Journal 169 6

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The 68% and 95% posterior contours for the HMC-...

The 68% and 95% posterior contours for the HMC-derived samples for the NIRB (left) and N...

Pedro H. Bernardinelli et al, The Astronomical Journal 169 6

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Left: 68% and 95% posterior contours of the NIR...

Left: 68% and 95% posterior contours of the NIRB (blue) and NIRF (red) LCA distribution ...

Pedro H. Bernardinelli et al, The Astronomical Journal 169 6

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Semimajor axes, eccentricities, and inclination...

Semimajor axes, eccentricities, and inclinations for all objects in the DES catalog. The...

Pedro H. Bernardinelli et al, The Astronomical Journal 169 6

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NIRB and NIRF realizations as in Figure 1, and ...

NIRB and NIRF realizations as in Figure 1, and the g − r, r − i and r − z colors and the...

Pedro H. Bernardinelli et al, The Astronomical Journal 169 6

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Illustration of GP augmentation applied to simu...

Illustration of GP augmentation applied to simulated light curves. Each band displays th...

Yongling Tang et al, The Astronomical Journal 169 6

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Example of GP real-time interpolation applied t...

Example of GP real-time interpolation applied to simulated light curves. A solid vertica...

Yongling Tang et al, The Astronomical Journal 169 6

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The semisupervised classification architecture ...

The semisupervised classification architecture comprises two distinct pathways. The unsu...

Yongling Tang et al, The Astronomical Journal 169 6

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Illustrations of well sampled simulated light c...

Illustrations of well sampled simulated light curves in expected WFST cadence. From left...

Yongling Tang et al, The Astronomical Journal 169 6

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Redshift distributions of three data sets repre...

Redshift distributions of three data sets representing the following transient classes: ...

Yongling Tang et al, The Astronomical Journal 169 6

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Comparison of confusion matrices (normalized ov...

Comparison of confusion matrices (normalized over true labels) between the benchmark mod...

Yongling Tang et al, The Astronomical Journal 169 6

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The detailed structure of the benchmark model (...

The detailed structure of the benchmark model (left panel) and the encoder module of our...

Yongling Tang et al, The Astronomical Journal 169 6

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Decoder module of our framework.

Yongling Tang et al, The Astronomical Journal 169 6

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Comparison of ROC curve and corresponding AUC b...

Comparison of ROC curve and corresponding AUC between the benchmark model (right panel) ...

Yongling Tang et al, The Astronomical Journal 169 6

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