Dr Sarah E. I.
Bosman
Dr Sarah E. I.
Bosman
Embedded Files
Bosman
Paper Supplementary Material
Paper Supplementary Material
Bosman+2018 Supplementary Online Material:
Columns A and B: quasar information
Column C: midpoint of each bin used to computed effective opacity
Column D: mean flux over 50 cMpc/h region centered on that redshift
Column E: flux error
Column F: effective opacity, unless flux is detected at less than 1 sigma, in which case a limit is given instead
Bosman+2020 Supplementary Online Material:
Animated version of Figure 10
Bosman+2021 Supplementary Online Material:
Further examples of Figure 1
Bosman+2022 Supplementary Online Material:
Optical depths measurements for all quasars, including different binnings
Current Projects
Current Projects
I am measuring the temperature of the hot dust torii of more quasars at z>7, but they require more modelling than expected. I am also struggling to understand the meaning of the mean free path (who isn't!)
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