Large-scale cosmic environment influences galaxy stellar mass and morphology beyond local companions, with void galaxies being less massive and showing distinct shape distributions.
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Simulations of Euclid Deep Fields show that cosmic web structures can be reconstructed from H-alpha galaxies with biases from redshift distortions and selection effects that can be partially mitigated, allowing recovery of stellar mass gradients toward filaments.
citing papers explorer
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Stellar mass and morphology segregation in pairs and multiplets in the cosmic web
Large-scale cosmic environment influences galaxy stellar mass and morphology beyond local companions, with void galaxies being less massive and showing distinct shape distributions.
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Euclid preparation. 3D reconstruction of the cosmic web with simulated Euclid Deep spectroscopic samples
Simulations of Euclid Deep Fields show that cosmic web structures can be reconstructed from H-alpha galaxies with biases from redshift distortions and selection effects that can be partially mitigated, allowing recovery of stellar mass gradients toward filaments.