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Photometric precision (﹩1.48/\sqrt{2}﹩× (median...

Photometric precision (﹩1.48/\sqrt{2}﹩× (median difference between adjacent flux points)...

Glen Petitpas et al, Research Notes of the AAS 10 3

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This figure shows the posterior distributions o...

This figure shows the posterior distributions of different planes of the (a) oΛCDM, (b) ...

Himanshu Chaudhary et al, The Astrophysical Journal Supplement Series 283 2

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This figure shows the statistical deviation (in...

This figure shows the statistical deviation (in units of σ) of each dark-energy model re...

Himanshu Chaudhary et al, The Astrophysical Journal Supplement Series 283 2

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This figure shows the corner plots for the (a) ...

This figure shows the corner plots for the (a) oΛCDM, (b) ωCDM, (c) oωCDM, (d) ω0ωaCDM, ...

Himanshu Chaudhary et al, The Astrophysical Journal Supplement Series 283 2

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This figure shows the difference in logarithmic...

This figure shows the difference in logarithmic Bayesian evidence of each dark-energy mo...

Himanshu Chaudhary et al, The Astrophysical Journal Supplement Series 283 2

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This figure shows the evolution of ω(z) as a fu...

This figure shows the evolution of ω(z) as a function of redshift, using DESI DR2 with C...

Himanshu Chaudhary et al, The Astrophysical Journal Supplement Series 283 2

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This figure shows the evolution of the energy d...

This figure shows the evolution of the energy density fDE(z) as a function of redshift, ...

Himanshu Chaudhary et al, The Astrophysical Journal Supplement Series 283 2

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Top: line-to-continuum ratio maps for Brα, H2 0...

Top: line-to-continuum ratio maps for Brα, H2 0-0 S(8), and [Ar II]. We have masked out ...

W. Blake Drechsler et al, The Astrophysical Journal 1000 2

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The 4 micron NIRSpec continuum image compared w...

The 4 micron NIRSpec continuum image compared with RT models with various disk masses. T...

W. Blake Drechsler et al, The Astrophysical Journal 1000 2

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Top row: continuum-subtracted moment 0 maps for...

Top row: continuum-subtracted moment 0 maps for the three detected atomic hydrogen lines...

W. Blake Drechsler et al, The Astrophysical Journal 1000 2

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Top row: continuum-subtracted moment 0 maps for...

Top row: continuum-subtracted moment 0 maps for [Ar II], [Ne III], and [Fe II]. Bottom r...

W. Blake Drechsler et al, The Astrophysical Journal 1000 2

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Stacked moment 0 maps for water (left) and OH (...

Stacked moment 0 maps for water (left) and OH (right). The contours represent the 16.0 μ...

W. Blake Drechsler et al, The Astrophysical Journal 1000 2

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Continuum-subtracted moment 0 maps for a sample...

Continuum-subtracted moment 0 maps for a sample of our detected molecular hydrogen trans...

W. Blake Drechsler et al, The Astrophysical Journal 1000 2

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The log-likelihoods for our RT models as a func...

The log-likelihoods for our RT models as a function of disk mass. The vertical line corr...

W. Blake Drechsler et al, The Astrophysical Journal 1000 2

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Horizontal profiles for the Brα (blue) and loca...

Horizontal profiles for the Brα (blue) and local continuum (red) moment 0 maps. Separate...

W. Blake Drechsler et al, The Astrophysical Journal 1000 2

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Rotation diagram before and after dereddening b...

Rotation diagram before and after dereddening based on the extinction fit. The orange li...

W. Blake Drechsler et al, The Astrophysical Journal 1000 2

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The line profiles and Gaussian fits of the H2 S...

The line profiles and Gaussian fits of the H2 S(1)-S(4) line used to construct the rotat...

W. Blake Drechsler et al, The Astrophysical Journal 1000 2

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Comparison of the Pfα and Brα line profiles aft...

Comparison of the Pfα and Brα line profiles after the Pfα profile has been downsampled t...

W. Blake Drechsler et al, The Astrophysical Journal 1000 2

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The disk + envelope RT models for all of the di...

The disk + envelope RT models for all of the disk masses that we tested. The contours re...

W. Blake Drechsler et al, The Astrophysical Journal 1000 2

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Corner plot showing the posterior distributions...

Corner plot showing the posterior distributions from the MCMC fit of the rotation diagram.

W. Blake Drechsler et al, The Astrophysical Journal 1000 2

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Our extracted 1D spectrum of L1527 using NIRSpe...

Our extracted 1D spectrum of L1527 using NIRSpec and MIRI data. The various observing ch...

W. Blake Drechsler et al, The Astrophysical Journal 1000 2

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Spherically averaged convective gradient profil...

Spherically averaged convective gradient profiles vs. radial bin for each simulation. Th...

Ferran Poca-Amorós et al, The Astrophysical Journal 1000 2

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2D slice through the center of the WD colored b...

2D slice through the center of the WD colored by the value of X(12C) at the end of the s...

Ferran Poca-Amorós et al, The Astrophysical Journal 1000 2

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Spherically averaged X(12C) profiles vs. radial...

Spherically averaged X(12C) profiles vs. radial bin for each simulation. The green curve...

Ferran Poca-Amorós et al, The Astrophysical Journal 1000 2

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Urms(r) against radius profiles averaged over t...

Urms(r) against radius profiles averaged over time. That is the last 400 s for the FN1 s...

Ferran Poca-Amorós et al, The Astrophysical Journal 1000 2

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