“UV slope”的版本间差异

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2024年6月3日 (一) 08:22的最新版本

arXiv:2405.20901
  • This study's substantial sample size provides a benchmark for demonstrating that the rest-frame UV spectral slope correlates with stellar mass-dependent galaxy characteristics at z∼2−4, a relationship less discernible with smaller datasets typically available at higher redshifts.