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Mineral systems different from bridgmanite. Sam...

Mineral systems different from bridgmanite. Same as Figure 2(b) but for other mineral de...

Antonio Manjón-Cabeza Córdoba et al, The Astrophysical Journal Letters 1005 2

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Comparison of crystallization-remelting scenari...

Comparison of crystallization-remelting scenarios for Earth (a) and Mars (b). Earth prop...

Antonio Manjón-Cabeza Córdoba et al, The Astrophysical Journal Letters 1005 2

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Earth and Mars cases showing different crystall...

Earth and Mars cases showing different crystallization timescales as lines. Black lines ...

Antonio Manjón-Cabeza Córdoba et al, The Astrophysical Journal Letters 1005 2

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Sensitivity of the Fe# anomaly of the overturne...

Sensitivity of the Fe# anomaly of the overturned silicate layer with respect to the rest...

Antonio Manjón-Cabeza Córdoba et al, The Astrophysical Journal Letters 1005 2

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Sensitivity of maximum Fe# to different physica...

Sensitivity of maximum Fe# to different physical properties. Other physical parameters f...

Antonio Manjón-Cabeza Córdoba et al, The Astrophysical Journal Letters 1005 2

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Comparison between the error function result at...

Comparison between the error function result at the base of the model (based on the erro...

Antonio Manjón-Cabeza Córdoba et al, The Astrophysical Journal Letters 1005 2

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Representation of the melting calculations in t...

Representation of the melting calculations in this work. (a) Melting approximation at a ...

Antonio Manjón-Cabeza Córdoba et al, The Astrophysical Journal Letters 1005 2

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Sensitivity and numerical error of the calculat...

Sensitivity and numerical error of the calculations. Comparison of numerical errors from...

Antonio Manjón-Cabeza Córdoba et al, The Astrophysical Journal Letters 1005 2

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An illustration of the bandpass error estimatio...

An illustration of the bandpass error estimation. The left panel shows the amplitude of ...

Sourabh Paul et al, The Astrophysical Journal Letters 1005 2

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The renormalized bandpass solution averaged acr...

The renormalized bandpass solution averaged across all antennae. The horizontal solid li...

Sourabh Paul et al, The Astrophysical Journal Letters 1005 2

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The distribution of (u, v) points on a 2D plane...

The distribution of (u, v) points on a 2D plane at 1077.5 MHz. The cells on this plane a...

Sourabh Paul et al, The Astrophysical Journal Letters 1005 2

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(a) The cylindrical autopower spectrum of the S...

(a) The cylindrical autopower spectrum of the Stokes V mode calculated from the z = 0.44...

Sourabh Paul et al, The Astrophysical Journal Letters 1005 2

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(a) Average visibility amplitude of the seconda...

(a) Average visibility amplitude of the secondary calibrator PKS J0252−7104 vs. frequenc...

Sourabh Paul et al, The Astrophysical Journal Letters 1005 2

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Stokes I frequency-averaged image of the field ...

Stokes I frequency-averaged image of the field at 1077.5 MHz from one (12.75 hr tracking...

Sourabh Paul et al, The Astrophysical Journal Letters 1005 2

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The fraction of flagged data. Only baselines wi...

The fraction of flagged data. Only baselines with −6000λ < u, v < 6000λ are selected for...

Sourabh Paul et al, The Astrophysical Journal Letters 1005 2

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Indication of low-level broadband RFI. (a) The ...

Indication of low-level broadband RFI. (a) The Stokes I 2D power spectrum derived from t...

Sourabh Paul et al, The Astrophysical Journal Letters 1005 2

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Delay power spectra for an antenna pair affecte...

Delay power spectra for an antenna pair affected by broadband RFI during one particular ...

Sourabh Paul et al, The Astrophysical Journal Letters 1005 2

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1D power spectrum from the analysis of 96 hr of...

1D power spectrum from the analysis of 96 hr of MeerKAT interferometer data at z = 0.32 ...

Sourabh Paul et al, The Astrophysical Journal Letters 1005 2

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Expected signal levels at z = 0.32 and z = 0.44...

Expected signal levels at z = 0.32 and z = 0.44. The measurement with UVDF is denoted as...

Sourabh Paul et al, The Astrophysical Journal Letters 1005 2

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Filtering broadband RFI systematics using BLF. ...

Filtering broadband RFI systematics using BLF. (a) the Stokes I 2D power spectrum for bo...

Sourabh Paul et al, The Astrophysical Journal Letters 1005 2

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Foreground scatter. The cylindrical foreground ...

Foreground scatter. The cylindrical foreground power spectrum at z = 0.32 without calibr...

Sourabh Paul et al, The Astrophysical Journal Letters 1005 2

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The gridded estimated bandpass error of the obs...

The gridded estimated bandpass error of the observation. The absolute values of the erro...

Sourabh Paul et al, The Astrophysical Journal Letters 1005 2

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Same as Figure 10(b), but with a black mask on ...

Same as Figure 10(b), but with a black mask on the u-v plane to avoid residual systemati...

Sourabh Paul et al, The Astrophysical Journal Letters 1005 2

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The measured 1D power spectrum with no threshol...

The measured 1D power spectrum with no thresholding, 10σ, 5σ, and 3σ cut (the flags are ...

Sourabh Paul et al, The Astrophysical Journal Letters 1005 2

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Evidence of broadband systematics and null test...

Evidence of broadband systematics and null test. Left: delay power spectra for the same ...

Sourabh Paul et al, The Astrophysical Journal Letters 1005 2

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