Stellar Population Spectra from BPASS v2.2.1
<p>The BPASS models of <a href="https://ui.adsabs.harvard.edu/abs/2017PASA...34...58E">Eldridge, Stanway et al. (2017)</a> and <a href="https://ui.adsabs.harvard.edu/abs/2018MNRAS.479...75S">Stanway & Eldridge et al. (2018)</a>. Data was downloaded from <a href="https://drive.google.com/drive/folders/1BS2w9hpdaJeul6-YtZum--F4gxWIPYXl?usp=sharing">https://drive.google.com/drive/folders/1BS2w9hpdaJeul6-YtZum--F4gxWIPYXl?usp=sharing</a>.</p> <ul> <li> <p>SSP_Spectra_BPASSv2.2.1_bin-imf100_100.hdf5</p> <ul> <li> <p>Broken power law IMF (α=-1.30 from 0.1M<sub>☉</sub>-0.5M<sub>☉</sub>, α=-2.00 from 0.5M<sub>☉</sub> to 100M<sub>☉</sub>)</p> </li> <li> <p>Includes binary stars</p> </li> <li> <p>Uses v2.2.1 of BPASS</p> </li> </ul> </li> <li> <p>SSP_Spectra_BPASSv2.2.1_bin-imf100_300.hdf5</p> <ul> <li> <p>Broken power law IMF (α=-1.30 from 0.1M<sub>☉</sub>-0.5M<sub>☉</sub>, α=-2.00 from 0.5M<sub>☉</sub> to 300M<sub>☉</sub>)</p> </li> <li> <p>Includes binary stars</p> </li> <li> <p>Uses v2.2.1 of BPASS</p> </li> </ul> </li> <li> <p>SSP_Spectra_BPASSv2.2.1_bin-imf135_100.hdf5</p> <ul> <li> <p>Broken power law IMF (α=-1.30 from 0.1M<sub>☉</sub>-0.5M<sub>☉</sub>, α=-2.35 from 0.5M<sub>☉</sub> to 100M<sub>☉</sub>)</p> </li> <li> <p>Includes binary stars</p> </li> <li> <p>Uses v2.2.1 of BPASS</p> </li> </ul> </li> <li> <p>SSP_Spectra_BPASSv2.2.1_bin-imf135_300.hdf5</p> <ul> <li> <p>Broken power law IMF (α=-1.30 from 0.1M<sub>☉</sub>-0.5M<sub>☉</sub>, α=-2.35 from 0.5M<sub>☉</sub> to 300M<sub>☉</sub>)</p> </li> <li> <p>Includes binary stars</p> </li> <li> <p>Uses v2.2.1 of BPASS</p> </li> </ul> </li> <li> <p>SSP_Spectra_BPASSv2.2.1_bin-imf135all_100.hdf5</p> <ul> <li> <p>Power law IMF (α=-2.35 from 0.1M<sub>☉</sub> to 100M<sub>☉</sub>)</p> </li> <li> <p>Includes binary stars</p> </li> <li> <p>Uses v2.2.1 of BPASS</p> </li> </ul> </li> <li> <p>SSP_Spectra_BPASSv2.2.1_bin-imf170_100.hdf5</p> <ul> <li> <p>Broken power law IMF (α=-1.30 from 0.1M<sub>☉</sub>-0.5M<sub>☉</sub>, α=-2.70 from 0.5M<sub>☉</sub> to 100M<sub>☉</sub>)</p> </li> <li> <p>Includes binary stars</p> </li> <li> <p>Uses v2.2.1 of BPASS</p> </li> </ul> </li> <li> <p>SSP_Spectra_BPASSv2.2.1_bin-imf170_300.hdf5</p> <ul> <li> <p>Broken power law IMF (α=-1.30 from 0.1M<sub>☉</sub>-0.5M<sub>☉</sub>, α=-2.70 from 0.5M<sub>☉</sub> to 300M<sub>☉</sub>)</p> </li> <li> <p>Includes binary stars</p> </li> <li> <p>Uses v2.2.1 of BPASS</p> </li> </ul> </li> <li> <p>SSP_Spectra_BPASSv2.2.1_bin-imf_chab100.hdf5</p> <ul> <li> <p>Chabrier IMF (α=-2.00; maximum mass 100M<sub>☉</sub>)</p> </li> <li> <p>Includes binary stars</p> </li> <li> <p>Uses v2.2.1 of BPASS</p> </li> </ul> </li> <li> <p>SSP_Spectra_BPASSv2.2.1_bin-imf_chab300.hdf5</p> <ul> <li> <p>Chabrier IMF (α=-2.00; maximum mass 300M<sub>☉</sub>)</p> </li> <li> <p>Includes binary stars</p> </li> <li> <p>Uses v2.2.1 of BPASS</p> </li> </ul> </li> <li> <p>SSP_Spectra_BPASSv2.2.1_sin-imf100_100.hdf5</p> <ul> <li> <p>Broken power law IMF (α=-1.30 from 0.1M<sub>☉</sub>-0.5M<sub>☉</sub>, α=-2.00 from 0.5M<sub>☉</sub> to 100M<sub>☉</sub>)</p> </li> <li> <p>Does not include binary stars</p> </li> <li> <p>Uses v2.2.1 of BPASS</p> </li> </ul> </li> <li> <p>SSP_Spectra_BPASSv2.2.1_sin-imf100_300.hdf5</p> <ul> <li> <p>Broken power law IMF (α=-1.30 from 0.1M<sub>☉</sub>-0.5M<sub>☉</sub>, α=-2.00 from 0.5M<sub>☉</sub> to 300M<sub>☉</sub>)</p> </li> <li> <p>Does not include binary stars</p> </li> <li> <p>Uses v2.2.1 of BPASS</p> </li> </ul> </li> <li> <p>SSP_Spectra_BPASSv2.2.1_sin-imf135_100.hdf5</p> <ul> <li> <p>Broken power law IMF (α=-1.30 from 0.1M<sub>☉</sub>-0.5M<sub>☉</sub>, α=-2.35 from 0.5M<sub>☉</sub> to 100M<sub>☉</sub>)</p> </li> <li> <p>Does not include binary stars</p> </li> <li> <p>Uses v2.2.1 of BPASS</p> </li> </ul> </li> <li> <p>SSP_Spectra_BPASSv2.2.1_sin-imf135_300.hdf5</p> <ul> <li> <p>Broken power law IMF (α=-1.30 from 0.1M<sub>☉</sub>-0.5M<sub>☉</sub>, α=-2.35 from 0.5M<sub>☉</sub> to 300M<sub>☉</sub>)</p> </li> <li> <p>Does not include binary stars</p> </li> <li> <p>Uses v2.2.1 of BPASS</p> </li> </ul> </li> <li> <p>SSP_Spectra_BPASSv2.2.1_sin-imf135all_100.hdf5</p> <ul> <li> <p>Power law IMF (α=-2.35 from 0.1M<sub>☉</sub> to 100M<sub>☉</sub>)</p> </li> <li> <p>Does not include binary stars</p> </li> <li> <p>Uses v2.2.1 of BPASS</p> </li> </ul> </li> <li> <p>SSP_Spectra_BPASSv2.2.1_sin-imf170_100.hdf5</p> <ul> <li> <p>Broken power law IMF (α=-1.30 from 0.1M<sub>☉</sub>-0.5M<sub>☉</sub>, α=-2.70 from 0.5M<sub>☉</sub> to 100M<sub>☉</sub>)</p> </li> <li> <p>Does not include binary stars</p> </li> <li> <p>Uses v2.2.1 of BPASS</p> </li> </ul> </li> <li> <p>SSP_Spectra_BPASSv2.2.1_sin-imf170_300.hdf5</p> <ul> <li> <p>Broken power law IMF (α=-1.30 from 0.1M<sub>☉</sub>-0.5M<sub>☉</sub>, α=-2.70 from 0.5M<sub>☉</sub> to 300M<sub>☉</sub>)</p> </li> <li> <p>Does not include binary stars</p> </li> <li> <p>Uses v2.2.1 of BPASS</p> </li> </ul> </li> <li> <p>SSP_Spectra_BPASSv2.2.1_sin-imf_chab100.hdf5</p> <ul> <li> <p>Chabrier IMF (α=-2.00; maximum mass 100M<sub>☉</sub>)</p> </li> <li> <p>Does not include binary stars</p> </li> <li> <p>Uses v2.2.1 of BPASS</p> </li> </ul> </li> <li> <p>SSP_Spectra_BPASSv2.2.1_sin-imf_chab300.hdf5</p> <ul> <li> <p>Chabrier IMF (α=-2.00; maximum mass 300M<sub>☉</sub>)</p> </li> <li> <p>Does not include binary stars</p> </li> <li> <p>Uses v2.2.1 of BPASS</p> </li> </ul> </li> </ul>
ShareScore
40/100
Overall dataset sharing score
Score breakdown
These five areas show where the dataset supports — or may limit — practical reuse.
- Stewardship
- 8
- Harmonization
- 4
- Access
- 20
- Reuse readiness
- 8
- Engagement
- 0
Topics
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