Dust extinction and reddening are ubiquitous in astronomical observations and
are often a major source of systematic uncertainty. We present here a study of
the correlation between extinction in the Milky Way and the equivalent width of
the NaI D absorption doublet. Our sample includes more than 100 high resolution
spectra from the KECK telescopes and nearly a million low resolution spectra
from the Sloan Digital Sky Survey (SDSS). We measure the correlation to
unprecedented precision, constrain its shape, and derive an empirical relation
between these quantities with a dispersion of order 0.15 magnitude in E(B-V).
From the shape of the curve of growth we further show that a typical sight line
through the Galaxy crosses about three dust clouds. We provide a brief guide on
how to best estimate extinction to extragalactic sources such as supernovae,
using the NaI D absorption feature, under a variety of circumstances.
Description
[1206.6107] An Empirical Relation between Sodium Absorption and Dust Extinction
%0 Generic
%1 poznanski2012empirical
%A Poznanski, Dovi
%A Prochaska, J. Xavier
%A Bloom, Joshua S.
%D 2012
%K correlation dust sodium
%T An Empirical Relation between Sodium Absorption and Dust Extinction
%U http://arxiv.org/abs/1206.6107
%X Dust extinction and reddening are ubiquitous in astronomical observations and
are often a major source of systematic uncertainty. We present here a study of
the correlation between extinction in the Milky Way and the equivalent width of
the NaI D absorption doublet. Our sample includes more than 100 high resolution
spectra from the KECK telescopes and nearly a million low resolution spectra
from the Sloan Digital Sky Survey (SDSS). We measure the correlation to
unprecedented precision, constrain its shape, and derive an empirical relation
between these quantities with a dispersion of order 0.15 magnitude in E(B-V).
From the shape of the curve of growth we further show that a typical sight line
through the Galaxy crosses about three dust clouds. We provide a brief guide on
how to best estimate extinction to extragalactic sources such as supernovae,
using the NaI D absorption feature, under a variety of circumstances.
@misc{poznanski2012empirical,
abstract = {Dust extinction and reddening are ubiquitous in astronomical observations and
are often a major source of systematic uncertainty. We present here a study of
the correlation between extinction in the Milky Way and the equivalent width of
the NaI D absorption doublet. Our sample includes more than 100 high resolution
spectra from the KECK telescopes and nearly a million low resolution spectra
from the Sloan Digital Sky Survey (SDSS). We measure the correlation to
unprecedented precision, constrain its shape, and derive an empirical relation
between these quantities with a dispersion of order 0.15 magnitude in E(B-V).
From the shape of the curve of growth we further show that a typical sight line
through the Galaxy crosses about three dust clouds. We provide a brief guide on
how to best estimate extinction to extragalactic sources such as supernovae,
using the NaI D absorption feature, under a variety of circumstances.},
added-at = {2012-06-28T07:25:59.000+0200},
author = {Poznanski, Dovi and Prochaska, J. Xavier and Bloom, Joshua S.},
biburl = {https://www.bibsonomy.org/bibtex/2c48f374bf714dd96dc10b0e26eeb01f1/miki},
description = {[1206.6107] An Empirical Relation between Sodium Absorption and Dust Extinction},
interhash = {d054c61256f576fe3b389b72ee9412ed},
intrahash = {c48f374bf714dd96dc10b0e26eeb01f1},
keywords = {correlation dust sodium},
note = {cite arxiv:1206.6107Comment: Submitted to MNRAS},
timestamp = {2012-06-28T07:26:00.000+0200},
title = {An Empirical Relation between Sodium Absorption and Dust Extinction},
url = {http://arxiv.org/abs/1206.6107},
year = 2012
}