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Theoretical atmosphere transmission at Dome A (...

Theoretical atmosphere transmission at Dome A (blue, median PWV = 0.141 mm, air mass = 1...

Pu Lin et al, The Astronomical Journal 171 3

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Upper left: the Antarctica Infrared Binocular T...

Upper left: the Antarctica Infrared Binocular Telescope (AIRBT) at Dome A, Antarctica. U...

Pu Lin et al, The Astronomical Journal 171 3

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Transformation for ﹩{W}^{{\prime} }﹩ band. The ...

Transformation for ﹩{W}^{{\prime} }﹩ band. The left upper (lower) panel is the spectrum ...

Pu Lin et al, The Astronomical Journal 171 3

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Photometric precision of the J (left) and ...

Photometric precision of the J (left) and ﹩{W}^{{\prime} }﹩(right) bands. For each band,...

Pu Lin et al, The Astronomical Journal 171 3

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An example showing the calculation of optical d...

An example showing the calculation of optical depth τ. The blue line is a spectrum of an...

Pu Lin et al, The Astronomical Journal 171 3

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The upper (lower) panels show the twilight flat...

The upper (lower) panels show the twilight flat, photometric flat, and distribution map ...

Pu Lin et al, The Astronomical Journal 171 3

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Magnitude variations of J and ﹩{W}^{{\prime} }﹩...

Magnitude variations of J and ﹩{W}^{{\prime} }﹩ bands between each pair of the three nig...

Pu Lin et al, The Astronomical Journal 171 3

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Color–color diagram of ...

Color–color diagram of ﹩{(J-{W}^{^{\prime} })}_{\mathrm{AIRBT}}﹩ versus (J − H)2MASS fro...

Pu Lin et al, The Astronomical Journal 171 3

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Spectrum variability from the PHOENIX model wit...

Spectrum variability from the PHOENIX model with ﹩\mathrm{log}g=1﹩ and [M/H] = 0.0. The ...

Pu Lin et al, The Astronomical Journal 171 3

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Histograms of the FWHM (upper) and the 5σ limit...

Histograms of the FWHM (upper) and the 5σ limiting magnitudes (lower) for J (yellow) and...

Pu Lin et al, The Astronomical Journal 171 3

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An example of raw (left), sampled sky-backgroun...

An example of raw (left), sampled sky-background residuals from SEP after first backgrou...

Pu Lin et al, The Astronomical Journal 171 3

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Left: relationship between optical depth τ and ...

Left: relationship between optical depth τ and spectral type from AIRBT known M-type sta...

Pu Lin et al, The Astronomical Journal 171 3

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Atmosphere transmission stability for J (upper)...

Atmosphere transmission stability for J (upper) and ﹩{W}^{{\prime} }﹩ (lower) bands at D...

Pu Lin et al, The Astronomical Journal 171 3

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NIRSpec/prism spectra of the seven RUBIES brown...

NIRSpec/prism spectra of the seven RUBIES brown dwarfs identified in this study (black l...

Sara J. Morrissey et al, The Astronomical Journal 171 3

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Comparison of the 0.9–2.5 μm NIRSpec/prism spec...

Comparison of the 0.9–2.5 μm NIRSpec/prism spectrum of RUBIES-BD-3 (black line) to L6 to...

Sara J. Morrissey et al, The Astronomical Journal 171 3

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RUBIES brown dwarf spectra in the 0.9–2.5 μm ra...

RUBIES brown dwarf spectra in the 0.9–2.5 μm range (black lines with uncertainties as gr...

Sara J. Morrissey et al, The Astronomical Journal 171 3

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Spectral variations among distant mid- and late...

Spectral variations among distant mid- and late-T dwarfs identified by JWST. Left panels...

Sara J. Morrissey et al, The Astronomical Journal 171 3

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Same as Figure 4 for the full NIRSpec/prism 0.9...

Same as Figure 4 for the full NIRSpec/prism 0.9–5.1 μm spectral range.

Sara J. Morrissey et al, The Astronomical Journal 171 3

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Same as Figure 4 for the full NIRSpec/prism 0.9...

Same as Figure 4 for the full NIRSpec/prism 0.9–5.1 μm spectral range.

Sara J. Morrissey et al, The Astronomical Journal 171 3

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MCMC fits to NIRSpec/prism data constrained to ...

MCMC fits to NIRSpec/prism data constrained to the NIR (0.9–2.4 μm) range. Each row corr...

Sara J. Morrissey et al, The Astronomical Journal 171 3

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MCMC fits to NIRSpec/prism data constrained to ...

MCMC fits to NIRSpec/prism data constrained to the NIR (0.9–2.4 μm) range. Each row corr...

Sara J. Morrissey et al, The Astronomical Journal 171 3

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Example corner plot of Elf Owl fits to NIRSpec/...

Example corner plot of Elf Owl fits to NIRSpec/prism data for RUBIES-BD-1. Diagonal pane...

Sara J. Morrissey et al, The Astronomical Journal 171 3

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Spatial distribution of the ejecta of the BLh_q...

Spatial distribution of the ejecta of the BLh_q1.49 model after 1 day. Top-left quadrant...

Maximilian Jacobi et al, The Astrophysical Journal Letters 999 1

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Mass-averaged nuclear energy generation (left p...

Mass-averaged nuclear energy generation (left panels), bolometric luminosity (middle pan...

Maximilian Jacobi et al, The Astrophysical Journal Letters 999 1

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Top panel: mass-ejection rate for the considere...

Top panel: mass-ejection rate for the considered BNS models. Bottom panel: 56Ni mass fra...

Maximilian Jacobi et al, The Astrophysical Journal Letters 999 1

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