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Redshift evolution of the median angle of align...

Redshift evolution of the median angle of alignment (and ±1σ bootstrapped errors) betwee...

Farhanul Hasan et al, The Astrophysical Journal 1004 1

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Two-dimensional projection of a 10 Mpc slice of...

Two-dimensional projection of a 10 Mpc slice of the cosmic web in TNG50 at z = 2 (in the...

Farhanul Hasan et al, The Astrophysical Journal 1004 1

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Residual morphological fractions at fixed stell...

Residual morphological fractions at fixed stellar mass, shown as functions of the neares...

Farhanul Hasan et al, The Astrophysical Journal 1004 1

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Fraction of prolate subhalos (color bar) as a f...

Fraction of prolate subhalos (color bar) as a function of filament line density (y-axis)...

Farhanul Hasan et al, The Astrophysical Journal 1004 1

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Average shape–filament alignment as a function ...

Average shape–filament alignment as a function of mass, at a few different redshifts (in...

Farhanul Hasan et al, The Astrophysical Journal 1004 1

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The fraction of galaxies with prolate stellar s...

The fraction of galaxies with prolate stellar structures (top row), inner halos (middle ...

Farhanul Hasan et al, The Astrophysical Journal 1004 1

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Evolution of the median alignment angle between...

Evolution of the median alignment angle between stellar (at 0.1rDM) and DM (at 2rDM) sha...

Farhanul Hasan et al, The Astrophysical Journal 1004 1

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The residual effect of filament density on stel...

The residual effect of filament density on stellar kinematic morphological properties at...

Farhanul Hasan et al, The Astrophysical Journal 1004 1

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Galaxies in stellar mass-size space at differen...

Galaxies in stellar mass-size space at different redshifts, colored by the median neares...

Farhanul Hasan et al, The Astrophysical Journal 1004 1

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Properties of different galaxy samples at z = 1...

Properties of different galaxy samples at z = 1 in TNG100 (top row; comparable to the si...

Farhanul Hasan et al, The Astrophysical Journal 1004 1

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Two-dimensional projections, in 20 Mpc thick sl...

Two-dimensional projections, in 20 Mpc thick slices, of the cosmic web identified at z =...

Farhanul Hasan et al, The Astrophysical Journal 1004 1

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Quantitative comparisons of the cosmic web from...

Quantitative comparisons of the cosmic web from different galaxy samples at z = 1. Top r...

Farhanul Hasan et al, The Astrophysical Journal 1004 1

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The dependence of 3D morphological fractions (p...

The dependence of 3D morphological fractions (prolate, oblate, and spheroidal) on neares...

Farhanul Hasan et al, The Astrophysical Journal 1004 1

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Similar to Figure 11. The cosmic web from HLWAS...

Similar to Figure 11. The cosmic web from HLWAS Spec-Deep in TNG100 (top) and from HLWAS...

Farhanul Hasan et al, The Astrophysical Journal 1004 1

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A cartoon schematic visualizing the effect of f...

A cartoon schematic visualizing the effect of filaments on the morphological evolution o...

Farhanul Hasan et al, The Astrophysical Journal 1004 1

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The median polarimetric behavior for (a) CPR, (...

The median polarimetric behavior for (a) CPR, (b) SC, and (c) OC and the three m-χ compo...

Edgard G. Rivera-Valentín et al, The Planetary Science Journal 7 6

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The median polarimetric behavior for (a) CPR, (...

The median polarimetric behavior for (a) CPR, (b) SC, and (c) OC and the three m-χ compo...

Edgard G. Rivera-Valentín et al, The Planetary Science Journal 7 6

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Median polarimetric behavior over 50∘ ≤ θ ≤ 60∘...

Median polarimetric behavior over 50∘ ≤ θ ≤ 60∘ as a function of RA on a log-scaled axis...

Edgard G. Rivera-Valentín et al, The Planetary Science Journal 7 6

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CPR as a function of RA on a log-scaled axis fo...

CPR as a function of RA on a log-scaled axis for (left) Giordano Bruno and (right) Eimma...

Edgard G. Rivera-Valentín et al, The Planetary Science Journal 7 6

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Map of the Spearman rank correlation coefficien...

Map of the Spearman rank correlation coefficient, ρ, for CPR and RA within a 6 × 6 pixel...

Edgard G. Rivera-Valentín et al, The Planetary Science Journal 7 6

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Case study maps for (top) Giordano Bruno (36∘N,...

Case study maps for (top) Giordano Bruno (36∘N, 102.9∘E) and (bottom) Eimmart A (24.1∘N,...

Edgard G. Rivera-Valentín et al, The Planetary Science Journal 7 6

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Global map of S-band CPR overlain onto S1 (i.e....

Global map of S-band CPR overlain onto S1 (i.e., the total backscattered intensity) in c...

Edgard G. Rivera-Valentín et al, The Planetary Science Journal 7 6

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Stellar masses inferred from the scaling relati...

Stellar masses inferred from the scaling relations in Equations (1)–(4) in three differe...

Zsóka Horváth et al, Research Notes of the AAS 10 6

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The left panel in the first row shows the clust...

The left panel in the first row shows the cluster map, while the right panel presents th...

Hiroma Okubo et al, The Astronomical Journal 172 1

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Correlation between the molecular column densit...

Correlation between the molecular column densities and the negative scores for Cluster 2...

Hiroma Okubo et al, The Astronomical Journal 172 1

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