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Illustration of the two - stage training framew...

Illustration of the two - stage training framework used in CLIP-GMC. In the first stage,...

Handa Cai and Weibin Chen, The Astronomical Journal 171 3

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Overview of the training stage in CLIP-GMC.

Overview of the training stage in CLIP-GMC.

Handa Cai and Weibin Chen, The Astronomical Journal 171 3

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Preprocessing examples.

Preprocessing examples.

Handa Cai and Weibin Chen, The Astronomical Journal 171 3

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CLIP-GMC training curves for Galaxy10 DECaLS (l...

CLIP-GMC training curves for Galaxy10 DECaLS (left column) and Galaxy MNIST (right colum...

Handa Cai and Weibin Chen, The Astronomical Journal 171 3

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t-SNE visualization of embeddings generated by ...

t-SNE visualization of embeddings generated by the CLIP-GMC model, trained on 10% of the...

Handa Cai and Weibin Chen, The Astronomical Journal 171 3

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CLIP-GMC performance comparison of categories a...

CLIP-GMC performance comparison of categories across data ratios for galaxy morphology c...

Handa Cai and Weibin Chen, The Astronomical Journal 171 3

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Confusion matrix on ten classes of CLIP-GMC, tr...

Confusion matrix on ten classes of CLIP-GMC, trained on 10% of the Galaxy10 DECaLS dataset.

Handa Cai and Weibin Chen, The Astronomical Journal 171 3

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Redshift distribution of the working sample (St...

Redshift distribution of the working sample (Strict + union masks). The median and centr...

Bo-Lun Huang et al, The Astronomical Journal 171 3

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Which band sets the tightest per object upper l...

Which band sets the tightest per object upper limit as a function of radiator temperatur...

Bo-Lun Huang et al, The Astronomical Journal 171 3

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95% upper bounds on the fraction of galaxies, f...

95% upper bounds on the fraction of galaxies, f 95, as a function of the waste heat lumi...

Bo-Lun Huang et al, The Astronomical Journal 171 3

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Empirical “null” test at T = 300 K (Strict + un...

Empirical “null” test at T = 300 K (Strict + union masks). We split the sample by MIR co...

Bo-Lun Huang et al, The Astronomical Journal 171 3

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Robustness of f 95(L wh,thr) at T = 300 K to me...

Robustness of f 95(L wh,thr) at T = 300 K to methodological choices. We compare STRICT v...

Bo-Lun Huang et al, The Astronomical Journal 171 3

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Color–color diagrams and mask footprints. Left:...

Color–color diagrams and mask footprints. Left: W1 − W2 vs. W2 − W3 with points colored ...

Bo-Lun Huang et al, The Astronomical Journal 171 3

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Effective number of galaxies, N eff, that would...

Effective number of galaxies, N eff, that would yield a constraint at or below a given L...

Bo-Lun Huang et al, The Astronomical Journal 171 3

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Injection recovery at T = 300 K. Each point is...

Injection recovery at T = 300 K. Each point is a synthetic galaxy: host MIR continuum (...

Bo-Lun Huang et al, The Astronomical Journal 171 3

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f 95(L wh,thr) at T = 300 K under RSR (bandpas...

f 95(L wh,thr) at T = 300 K under RSR (bandpass-averaged) vs. MONO (monochromatic at th...

Bo-Lun Huang et al, The Astronomical Journal 171 3

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Extended-source stress test at T = 300 K. We pe...

Extended-source stress test at T = 300 K. We perturb the per-object ...

Bo-Lun Huang et al, The Astronomical Journal 171 3

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Median bias vs. injected L wh at T = 300 K, spl...

Median bias vs. injected L wh at T = 300 K, split by host SED family. Positive bias at l...

Bo-Lun Huang et al, The Astronomical Journal 171 3

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WISE W1 − W2 vs. W2 − W3 (Vega) color–color dia...

WISE W1 − W2 vs. W2 − W3 (Vega) color–color diagram for the 2MRS cross matched galaxy sa...

Bo-Lun Huang et al, The Astronomical Journal 171 3

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The top-left plot shows the sample-split scheme...

The top-left plot shows the sample-split scheme, where galaxies are categorized by posit...

Xiaoya Zhang et al, The Astronomical Journal 171 3

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The two subsamples are split by position on the...

The two subsamples are split by position on the ...

Xiaoya Zhang et al, The Astronomical Journal 171 3

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Example galaxy (PGC 153919) in the final sample...

Example galaxy (PGC 153919) in the final sample. Top left: SGA g-band image. The title i...

Xiaoya Zhang et al, The Astronomical Journal 171 3

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﹩{[{\rm{MgFe}}]}^{{\prime} }﹩ vs. Mgb/〈Fe〉 pla...

﹩{[{\rm{MgFe}}]}^{{\prime} }﹩ vs. Mgb/〈Fe〉 plane, where the grids are from the sMILES S...

Xiaoya Zhang et al, The Astronomical Journal 171 3

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Radial gradients of the compact (green circles)...

Radial gradients of the compact (green circles) and extended (purple diamonds). The top ...

Xiaoya Zhang et al, The Astronomical Journal 171 3

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Radial gradients of spectral indices of the hig...

Radial gradients of spectral indices of the high-σ* (orange pentagons) and low-σ* (blue ...

Xiaoya Zhang et al, The Astronomical Journal 171 3

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