Stellar Population Spectra from BPASS v2.2.1
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https://zenodo.org/record/6338459
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资源简介：
The BPASS models of Eldridge, Stanway et al. (2017) and Stanway & Eldridge et al. (2018). Data was downloaded from https://drive.google.com/drive/folders/1BS2w9hpdaJeul6-YtZum--F4gxWIPYXl?usp=sharing.
SSP_Spectra_BPASSv2.2.1_bin-imf100_100.hdf5
Broken power law IMF (α=-1.30 from 0.1M☉-0.5M☉, α=-2.00 from 0.5M☉ to 100M☉)
Includes binary stars
Uses v2.2.1 of BPASS
SSP_Spectra_BPASSv2.2.1_bin-imf100_300.hdf5
Broken power law IMF (α=-1.30 from 0.1M☉-0.5M☉, α=-2.00 from 0.5M☉ to 300M☉)
Includes binary stars
Uses v2.2.1 of BPASS
SSP_Spectra_BPASSv2.2.1_bin-imf135_100.hdf5
Broken power law IMF (α=-1.30 from 0.1M☉-0.5M☉, α=-2.35 from 0.5M☉ to 100M☉)
Includes binary stars
Uses v2.2.1 of BPASS
SSP_Spectra_BPASSv2.2.1_bin-imf135_300.hdf5
Broken power law IMF (α=-1.30 from 0.1M☉-0.5M☉, α=-2.35 from 0.5M☉ to 300M☉)
Includes binary stars
Uses v2.2.1 of BPASS
SSP_Spectra_BPASSv2.2.1_bin-imf135all_100.hdf5
Power law IMF (α=-2.35 from 0.1M☉ to 100M☉)
Includes binary stars
Uses v2.2.1 of BPASS
SSP_Spectra_BPASSv2.2.1_bin-imf170_100.hdf5
Broken power law IMF (α=-1.30 from 0.1M☉-0.5M☉, α=-2.70 from 0.5M☉ to 100M☉)
Includes binary stars
Uses v2.2.1 of BPASS
SSP_Spectra_BPASSv2.2.1_bin-imf170_300.hdf5
Broken power law IMF (α=-1.30 from 0.1M☉-0.5M☉, α=-2.70 from 0.5M☉ to 300M☉)
Includes binary stars
Uses v2.2.1 of BPASS
SSP_Spectra_BPASSv2.2.1_bin-imf_chab100.hdf5
Chabrier IMF (α=-2.00; maximum mass 100M☉)
Includes binary stars
Uses v2.2.1 of BPASS
SSP_Spectra_BPASSv2.2.1_bin-imf_chab300.hdf5
Chabrier IMF (α=-2.00; maximum mass 300M☉)
Includes binary stars
Uses v2.2.1 of BPASS
SSP_Spectra_BPASSv2.2.1_sin-imf100_100.hdf5
Broken power law IMF (α=-1.30 from 0.1M☉-0.5M☉, α=-2.00 from 0.5M☉ to 100M☉)
Does not include binary stars
Uses v2.2.1 of BPASS
SSP_Spectra_BPASSv2.2.1_sin-imf100_300.hdf5
Broken power law IMF (α=-1.30 from 0.1M☉-0.5M☉, α=-2.00 from 0.5M☉ to 300M☉)
Does not include binary stars
Uses v2.2.1 of BPASS
SSP_Spectra_BPASSv2.2.1_sin-imf135_100.hdf5
Broken power law IMF (α=-1.30 from 0.1M☉-0.5M☉, α=-2.35 from 0.5M☉ to 100M☉)
Does not include binary stars
Uses v2.2.1 of BPASS
SSP_Spectra_BPASSv2.2.1_sin-imf135_300.hdf5
Broken power law IMF (α=-1.30 from 0.1M☉-0.5M☉, α=-2.35 from 0.5M☉ to 300M☉)
Does not include binary stars
Uses v2.2.1 of BPASS
SSP_Spectra_BPASSv2.2.1_sin-imf135all_100.hdf5
Power law IMF (α=-2.35 from 0.1M☉ to 100M☉)
Does not include binary stars
Uses v2.2.1 of BPASS
SSP_Spectra_BPASSv2.2.1_sin-imf170_100.hdf5
Broken power law IMF (α=-1.30 from 0.1M☉-0.5M☉, α=-2.70 from 0.5M☉ to 100M☉)
Does not include binary stars
Uses v2.2.1 of BPASS
SSP_Spectra_BPASSv2.2.1_sin-imf170_300.hdf5
Broken power law IMF (α=-1.30 from 0.1M☉-0.5M☉, α=-2.70 from 0.5M☉ to 300M☉)
Does not include binary stars
Uses v2.2.1 of BPASS
SSP_Spectra_BPASSv2.2.1_sin-imf_chab100.hdf5
Chabrier IMF (α=-2.00; maximum mass 100M☉)
Does not include binary stars
Uses v2.2.1 of BPASS
SSP_Spectra_BPASSv2.2.1_sin-imf_chab300.hdf5
Chabrier IMF (α=-2.00; maximum mass 300M☉)
Does not include binary stars
Uses v2.2.1 of BPASS
创建时间：
2022-03-10
