Stellar Population Spectra from BPASS v2.3
<p>The BPASS models of <a href="https://ui.adsabs.harvard.edu/abs/2017PASA...34...58E">Eldridge, Stanway et al. (2017)</a>, <a href="https://ui.adsabs.harvard.edu/abs/2018MNRAS.479...75S">Stanway & Eldridge et al. (2018)</a> and <a href="https://ui.adsabs.harvard.edu/abs/2022MNRAS.512.5329B">Byrne et al. (2022, MNRAS, 512, 5329)</a>. Data was downloaded from <a href="https://livewarwickac.sharepoint.com/sites/Physics-BinaryPopulationandSpectralSynthesisBPASS/Shared%20Documents/Forms/AllItems.aspx?id=%2Fsites%2FPhysics%2DBinaryPopulationandSpectralSynthesisBPASS%2FShared%20Documents%2FPaper%20Data%20Packages%2FByrne23&p=true&ga=1">here</a>.</p> <ul> <li> <p>SSP_Spectra_BPASSv2.3_sin-imf135_300-alpha-02.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>α-alement enhancement of Δlog₁₀(α/Fe)=-0.2</p> </li> <li> <p>Uses v2.3 of BPASS</p> </li> </ul> </li> <li> <p>SSP_Spectra_BPASSv2.3_sin-imf135_300-alpha+00.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>α-alement enhancement of Δlog₁₀(α/Fe)=+0.0</p> </li> <li> <p>Uses v2.3 of BPASS</p> </li> </ul> </li> <li> <p>SSP_Spectra_BPASSv2.3_sin-imf135_300-alpha+02.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>α-alement enhancement of Δlog₁₀(α/Fe)=+0.2</p> </li> <li> <p>Uses v2.3 of BPASS</p> </li> </ul> </li> <li> <p>SSP_Spectra_BPASSv2.3_sin-imf135_300-alpha+04.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>α-alement enhancement of Δlog₁₀(α/Fe)=+0.4</p> </li> <li> <p>Uses v2.3 of BPASS</p> </li> </ul> </li> <li> <p>SSP_Spectra_BPASSv2.3_sin-imf135_300-alpha+06.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>α-alement enhancement of Δlog₁₀(α/Fe)=+0.6</p> </li> <li> <p>Uses v2.3 of BPASS</p> </li> </ul> </li> <li> <p>SSP_Spectra_BPASSv2.3_bin-imf135_300-alpha-02.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>α-alement enhancement of Δlog₁₀(α/Fe)=-0.2</p> </li> <li> <p>Uses v2.3 of BPASS</p> </li> </ul> </li> <li> <p>SSP_Spectra_BPASSv2.3_bin-imf135_300-alpha+00.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>α-alement enhancement of Δlog₁₀(α/Fe)=+0.0</p> </li> <li> <p>Uses v2.3 of BPASS</p> </li> </ul> </li> <li> <p>SSP_Spectra_BPASSv2.3_bin-imf135_300-alpha+02.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>α-alement enhancement of Δlog₁₀(α/Fe)=+0.2</p> </li> <li> <p>Uses v2.3 of BPASS</p> </li> </ul> </li> <li> <p>SSP_Spectra_BPASSv2.3_bin-imf135_300-alpha+04.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>α-alement enhancement of Δlog₁₀(α/Fe)=+0.4</p> </li> <li> <p>Uses v2.3 of BPASS</p> </li> </ul> </li> <li> <p>SSP_Spectra_BPASSv2.3_bin-imf135_300-alpha+06.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>α-alement enhancement of Δlog₁₀(α/Fe)=+0.6</p> </li> <li> <p>Uses v2.3 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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