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This figure demonstrates the performance of our...

This figure demonstrates the performance of our MFBD algorithm vs. that of the standard ...

Steve B. Howell et al, The Astronomical Journal 167 6

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We present contrast curves for the binary syste...

We present contrast curves for the binary system, α Com as well as an average contrast c...

Steve B. Howell et al, The Astronomical Journal 167 6

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The measured 832 nm contrast curves from Figure...

The measured 832 nm contrast curves from Figure 1 using the standard Fourier (SI) recons...

Steve B. Howell et al, The Astronomical Journal 167 6

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We see here, the final MFBD reconstructed image...

We see here, the final MFBD reconstructed images from the right side of Figure 2 after t...

Steve B. Howell et al, The Astronomical Journal 167 6

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This figure illustrates some steps in the progr...

This figure illustrates some steps in the progress throughout the MFBD reconstructions, ...

Steve B. Howell et al, The Astronomical Journal 167 6

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The left column is for a generic G0V star at 50...

The left column is for a generic G0V star at 50 pc and the right column is for a generic...

Steve B. Howell et al, The Astronomical Journal 167 6

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Regular convolution (left panel), partial convo...

Regular convolution (left panel), partial convolution (middle panel), and multiscale par...

Jingjing Wu et al, The Astronomical Journal 167 6

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Spectral preprocessing (upper panels for origin...

Spectral preprocessing (upper panels for original spectra and lower panels for their nor...

Jingjing Wu et al, The Astronomical Journal 167 6

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The t-SNE visualizations of the samples (5 clas...

The t-SNE visualizations of the samples (5 class for Dataset SS-S (>10) and 4 class for ...

Jingjing Wu et al, The Astronomical Journal 167 6

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Feature visualization. Regular convolution and ...

Feature visualization. Regular convolution and MSCP-Net extract the features of the spec...

Jingjing Wu et al, The Astronomical Journal 167 6

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Accuracy as a function of S/N interval (upper p...

Accuracy as a function of S/N interval (upper panels) and the S/N distribution (lower pa...

Jingjing Wu et al, The Astronomical Journal 167 6

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The complete figure set (28 images) is availabl...

The complete figure set (28 images) is available in the online journal.

Jingjing Wu et al, The Astronomical Journal 167 6

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The MSPC-Net overall architecture: The macrosco...

The MSPC-Net overall architecture: The macroscopic design of the model is based on MetaF...

Jingjing Wu et al, The Astronomical Journal 167 6

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Training accuracy (left panel) and validation a...

Training accuracy (left panel) and validation accuracy (right panel) curves with differe...

Jingjing Wu et al, The Astronomical Journal 167 6

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Label consistency of SDSS and LAMOST in the gro...

Label consistency of SDSS and LAMOST in the group correct predictions (left panel) and t...

Jingjing Wu et al, The Astronomical Journal 167 6

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Distribution of the Galactic P-normal stars wit...

Distribution of the Galactic P-normal stars with [P/Fe] < 1 on the [Fe/H]−[P/Fe] plane a...

Kenji Bekki and Takuji Tsujimoto, The Astrophysical Journal Letters 967 1

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Evolutionary paths of four models with M ...

Evolutionary paths of four models with M ej = 1 × 10−4 ...

Kenji Bekki and Takuji Tsujimoto, The Astrophysical Journal Letters 967 1

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Same as Figure 2 but for four models with α ...

Same as Figure 2 but for four models with α Z = −1.7 × 10−3 and N ...

Kenji Bekki and Takuji Tsujimoto, The Astrophysical Journal Letters 967 1

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Same as Figure 2 but for four models with diffe...

Same as Figure 2 but for four models with different slopes of metallicity-dependent P yi...

Kenji Bekki and Takuji Tsujimoto, The Astrophysical Journal Letters 967 1

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Evolutionary paths of four models with ...

Evolutionary paths of four models with ...

Kenji Bekki and Takuji Tsujimoto, The Astrophysical Journal Letters 967 1

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The redshift distributions of the galaxies in t...

The redshift distributions of the galaxies in the three M ...

Aditya Chowdhury et al, The Astrophysical Journal Letters 966 2

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The average HI 21 cm emission signal from star-...

The average HI 21 cm emission signal from star-forming galaxies in different M ...

Aditya Chowdhury et al, The Astrophysical Journal Letters 966 2

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The M HI ...

The M HI –M ...

Aditya Chowdhury et al, The Astrophysical Journal Letters 966 2

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(A) The HIMF of star-forming galaxies at z ≈ 1....

(A) The HIMF of star-forming galaxies at z ≈ 1. The blue curve shows our measurement of ...

Aditya Chowdhury et al, The Astrophysical Journal Letters 966 2

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The ratio of the number density of galaxies at ...

The ratio of the number density of galaxies at z ≈ 1 to that at z ≈ 0 as a function of t...

Aditya Chowdhury et al, The Astrophysical Journal Letters 966 2

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