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Left: PlanetFlow pipeline architecture. Dark bl...

Left: PlanetFlow pipeline architecture. Dark blue boxes indicate required steps; gray bo...

Heejo You, Research Notes of the AAS 10 5

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(a) example H I dynamic spectrum or integrated ...

(a) example H I dynamic spectrum or integrated spectrum from the SDR observation, with p...

Zi-Qi Li et al, Research Notes of the AAS 10 5

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Low-frequency radio spectra (pink) in log–log s...

Low-frequency radio spectra (pink) in log–log space of galaxy cluster A655 for different...

Kasey Thai and Mark Lacy, Research Notes of the AAS 10 5

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Our physical picture for GRB 250702B. Panel (a)...

Our physical picture for GRB 250702B. Panel (a) shows the geodesic orbit of the WD, wher...

Yuri Sato et al, The Astrophysical Journal Letters 1003 2

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Afterglow light curves in the X-ray (5 keV; ora...

Afterglow light curves in the X-ray (5 keV; orange), near-infrared (2 × 1014 Hz; blue), ...

Yuri Sato et al, The Astrophysical Journal Letters 1003 2

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Predicted radio (1.3 GHz) afterglow light curve...

Predicted radio (1.3 GHz) afterglow light curves for the maximum (40 jets; red solid lin...

Yuri Sato et al, The Astrophysical Journal Letters 1003 2

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Reflectance spectra of the saw-cut powder and s...

Reflectance spectra of the saw-cut powder and slabs of QUE 86900 and MAC 88102.

Pengyue Wang et al, The Astrophysical Journal Supplement Series 284 2

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Spectral metrics versus the saw-cut powder and ...

Spectral metrics versus the saw-cut powder and slabs of QUE 86900 and MAC 88102.

Pengyue Wang et al, The Astrophysical Journal Supplement Series 284 2

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Reflectance spectra of different grain sizes of...

Reflectance spectra of different grain sizes of 50:50 metal+orthopyroxene mixtures. In (...

Pengyue Wang et al, The Astrophysical Journal Supplement Series 284 2

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Reflectance spectra of different spots on slab ...

Reflectance spectra of different spots on slab faces of four mesosiderites. All spectra ...

Pengyue Wang et al, The Astrophysical Journal Supplement Series 284 2

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Band centers and BAR versus 50:50 metal+orthopy...

Band centers and BAR versus 50:50 metal+orthopyroxene mixture grain sizes.

Pengyue Wang et al, The Astrophysical Journal Supplement Series 284 2

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Reflectance spectra of orthopyroxene (PYX042; <...

Reflectance spectra of orthopyroxene (PYX042; <45 μm grain size) sprinkled on an Odessa ...

Pengyue Wang et al, The Astrophysical Journal Supplement Series 284 2

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Reflectance spectra of different pyroxene compo...

Reflectance spectra of different pyroxene compositions (Fs12.8 to Fs41.5) of 50:50 metal...

Pengyue Wang et al, The Astrophysical Journal Supplement Series 284 2

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Reflectance spectra of 10 wt% series of orthopy...

Reflectance spectra of 10 wt% series of orthopyroxene+metal powder (grain size <45 μm).

Pengyue Wang et al, The Astrophysical Journal Supplement Series 284 2

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Band centers versus pyroxene composition of 50:...

Band centers versus pyroxene composition of 50:50 metal+orthopyroxene mixtures.

Pengyue Wang et al, The Astrophysical Journal Supplement Series 284 2

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Reflectance spectra of metal-rich (90 wt% metal...

Reflectance spectra of metal-rich (90 wt% metal) orthopyroxene+metal intimate and areal ...

Pengyue Wang et al, The Astrophysical Journal Supplement Series 284 2

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Reflectance spectra of Psyche, mesosiderite pow...

Reflectance spectra of Psyche, mesosiderite powder, pyroxene powder on a metal slab, and...

Pengyue Wang et al, The Astrophysical Journal Supplement Series 284 2

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The plot of the BAR and Band I center for the 1...

The plot of the BAR and Band I center for the 12 mesosiderites included in this study. T...

Pengyue Wang et al, The Astrophysical Journal Supplement Series 284 2

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The plot of the Band I center and Band II cente...

The plot of the Band I center and Band II center in mesosiderites, howardites, eucrites,...

Pengyue Wang et al, The Astrophysical Journal Supplement Series 284 2

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Reflectance spectra of 12 mesosiderites used in...

Reflectance spectra of 12 mesosiderites used in this study. All spectra are normalized a...

Pengyue Wang et al, The Astrophysical Journal Supplement Series 284 2

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Band centers and BAR versus 10 wt% series of or...

Band centers and BAR versus 10 wt% series of orthopyroxene+metal powder.

Pengyue Wang et al, The Astrophysical Journal Supplement Series 284 2

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The effect of 14N(p, γ)15O reaction rate (the d...

The effect of 14N(p, γ)15O reaction rate (the default JINA REACLIB, solid gray lines vs....

Radoslaw Smolec et al, The Astrophysical Journal Supplement Series 284 2

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Evolutionary tracks computed with MESA-r21.12.1...

Evolutionary tracks computed with MESA-r21.12.1 (solid gray lines) and MESA-24.08.1 (das...

Radoslaw Smolec et al, The Astrophysical Journal Supplement Series 284 2

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The effect of different reference solar composi...

The effect of different reference solar compositions, A09 (solid gray lines) vs. GS98 (d...

Radoslaw Smolec et al, The Astrophysical Journal Supplement Series 284 2

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Location of the F-mode IS determined for (panel...

Location of the F-mode IS determined for (panel (a)) different crossing numbers, (panel ...

Radoslaw Smolec et al, The Astrophysical Journal Supplement Series 284 2

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