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- W1901999419 endingPage "L84" @default.
- W1901999419 startingPage "L81" @default.
- W1901999419 abstract "Dust extinction is generally the least tractable systematic uncertainty in astronomy, and particularly in supernova science. Often in the past, studies have used the equivalent width of Na i D absorption measured from low-resolution spectra as proxies for extinction, based on tentative correlations that were drawn from limited data sets. We show here, based on 443 low-resolution spectra of 172 Type Ia supernovae for which we have measured the dust extinction as well as the equivalent width of Na i D, that the two barely correlate. We briefly examine the causes for this large scatter that effectively prevents one from inferring extinction using this method." @default.
- W1901999419 created "2016-06-24" @default.
- W1901999419 creator A5020408291 @default.
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- W1901999419 date "2011-06-15" @default.
- W1901999419 modified "2023-10-15" @default.
- W1901999419 title "Low-resolution sodium D absorption is a bad proxy for extinction" @default.
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- W1901999419 doi "https://doi.org/10.1111/j.1745-3933.2011.01084.x" @default.
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