Stellar Population Spectra from BPASS v2.2.1

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

Related Organizations

Carnegie Institution for Science
United States

Keywords

spectra, galaxies, stellar populations

Impact byBIP!

	selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	0
	popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.	Average
	influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	Average
	impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.	Average