“LEGA-C”的版本间差异
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* It consists of 4081 spectra of 3741 unique galaxies in the redshift range 0.6 < z < 1.0, with typical continuum S/N ≃17, wavelength coverage 6000-9000 Angstrom and spectral resolution of R~3500. |
* It consists of 4081 spectra of 3741 unique galaxies in the redshift range 0.6 < z < 1.0, with typical continuum S/N ≃17, wavelength coverage 6000-9000 Angstrom and spectral resolution of R~3500. |
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*Kaushal et al. (2023) 得到了恒星形成历史，对于大质量Quiescent星系，其比晕的吸积历史模型预言（The UniverseMachine (Behroozi et al. (2019)）的要更延展来说（arXiv:2401.05313） |
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* 不同质量的金属丰度 [https://arxiv.org/abs/2407.12704] |
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2024年7月18日 (四) 07:50的最新版本
- The Large Early Galaxy Census (LEGA-C) is a Public Spectroscopic Survey of $\sim3200$ $K$-band selected galaxies at redshifts $z=0.6-1.0$ with stellar masses M_star > 1e10M_sun, conducted with VIMOS on VLT. The survey is embedded in the COSMOS field.
- 释放数据 [1]
- It consists of 4081 spectra of 3741 unique galaxies in the redshift range 0.6 < z < 1.0, with typical continuum S/N ≃17, wavelength coverage 6000-9000 Angstrom and spectral resolution of R~3500.
- Kaushal et al. (2023) 得到了恒星形成历史，对于大质量Quiescent星系，其比晕的吸积历史模型预言（The UniverseMachine (Behroozi et al. (2019)）的要更延展来说（arXiv:2401.05313）
- 不同质量的金属丰度 [2]