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Fragment merger dynamics in a collapsar-disk-li...

Fragment merger dynamics in a collapsar-disk-like arrangement. Shown are three different...

Jiaxi Wu et al, The Astrophysical Journal Letters 1004 1

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(Left) Compact-object trajectories in the orbit...

(Left) Compact-object trajectories in the orbital xy-plane for the two-cluster simulatio...

Jiaxi Wu et al, The Astrophysical Journal Letters 1004 1

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Detector-frame plus polarization strain h+ for ...

Detector-frame plus polarization strain h+ for the three simulations, reconstructed from...

Jiaxi Wu et al, The Astrophysical Journal Letters 1004 1

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Frequency-domain detector-frame gravitational-w...

Frequency-domain detector-frame gravitational-wave spectrum ﹩\sqrt{f}\,| \tilde{h}| ﹩ at...

Jiaxi Wu et al, The Astrophysical Journal Letters 1004 1

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Same as Figure 2, but using Newtonian point-par...

Same as Figure 2, but using Newtonian point-particle dynamics.

Jiaxi Wu et al, The Astrophysical Journal Letters 1004 1

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Multiwavelength observations and quantitative a...

Multiwavelength observations and quantitative analysis of the quiet-Sun region. The imag...

Huaiming Li et al, The Astrophysical Journal Supplement Series 284 2

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Comparison of photospheric and chromospheric co...

Comparison of photospheric and chromospheric components. The first row shows the AR; the...

Huaiming Li et al, The Astrophysical Journal Supplement Series 284 2

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The images used in this figure are 45 minute ti...

The images used in this figure are 45 minute time-averaged data. (A) The He I 10830 Å ch...

Huaiming Li et al, The Astrophysical Journal Supplement Series 284 2

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Testing cases of our proposed models: the top r...

Testing cases of our proposed models: the top row displays results from Model A for ARs,...

Huaiming Li et al, The Astrophysical Journal Supplement Series 284 2

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The first row (A1), (A2) displays the high-cont...

The first row (A1), (A2) displays the high-contrast features of the AR dataset. The seco...

Huaiming Li et al, The Astrophysical Journal Supplement Series 284 2

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Training data for Model A from NVST observation...

Training data for Model A from NVST observations. From left to right: 2024 November 25, ...

Huaiming Li et al, The Astrophysical Journal Supplement Series 284 2

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Comparison of loss for Model A and Model B.

Comparison of loss for Model A and Model B.

Huaiming Li et al, The Astrophysical Journal Supplement Series 284 2

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Detailed architecture of the Model B for QS reg...

Detailed architecture of the Model B for QS regions. The model directly maps TiO to 1083...

Huaiming Li et al, The Astrophysical Journal Supplement Series 284 2

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(A) The HMI magnetogram. (B) The He I 10830 Å c...

(A) The HMI magnetogram. (B) The He I 10830 Å chromospheric signal. (C) The AIA 193 Å im...

Huaiming Li et al, The Astrophysical Journal Supplement Series 284 2

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(A) The He I 10830 Å chromospheric signal. (B) ...

(A) The He I 10830 Å chromospheric signal. (B) The 171 Å image. The area below the yello...

Huaiming Li et al, The Astrophysical Journal Supplement Series 284 2

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Basic residual block incorporating the SE atten...

Basic residual block incorporating the SE attention mechanism used in Model A.

Huaiming Li et al, The Astrophysical Journal Supplement Series 284 2

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Modified residual block for Model B, with BN an...

Modified residual block for Model B, with BN and Dropout removed to better fit continuou...

Huaiming Li et al, The Astrophysical Journal Supplement Series 284 2

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Detailed architecture of the Model A. The model...

Detailed architecture of the Model A. The model maps TiO input to 10829 Å to leverage th...

Huaiming Li et al, The Astrophysical Journal Supplement Series 284 2

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Lyα-pumped iron emission in GLIMPSE-17775. Left...

Lyα-pumped iron emission in GLIMPSE-17775. Left: observed Fe II flux ratios (black point...

Vasily Kokorev et al, The Astrophysical Journal 1004 2

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Physical picture of the dense cocoon around GLI...

Physical picture of the dense cocoon around GLIMPSE-17775. The inner region (1) correspo...

Vasily Kokorev et al, The Astrophysical Journal 1004 2

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Exponential wings are required. Comparison of a...

Exponential wings are required. Comparison of a Gaussian×exponential model (red) and a s...

Vasily Kokorev et al, The Astrophysical Journal 1004 2

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Best-fit profiles of all broad lines, oversampl...

Best-fit profiles of all broad lines, oversampled and shifted to a common center. The to...

Vasily Kokorev et al, The Astrophysical Journal 1004 2

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Velocity offsets (relative to [S III]λ9071) and...

Velocity offsets (relative to [S III]λ9071) and FWHM for all detected lines. Narrow perm...

Vasily Kokorev et al, The Astrophysical Journal 1004 2

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Top: JWST/NIRCam and HST 2...

Top: JWST/NIRCam and HST 2﹩\mathop{.}\limits^{^{\prime\prime} }﹩0 stamps and red, green,...

Vasily Kokorev et al, The Astrophysical Journal 1004 2

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A staggering abundance of spectral lines in GLI...

A staggering abundance of spectral lines in GLIMPSE-17775 at z = 3.501. For each spectr...

Vasily Kokorev et al, The Astrophysical Journal 1004 2

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