Galacticus Datasets
Published March 8, 2022 | Version v1
Dataset Open

Stellar Population Spectra from BPASS v2.2.1

Authors/Creators

  • 1. Carnegie Institution for Science

Description

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

Files

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