A simple non-parametric method for resolving merged doublet lines

Insights into complex kinematics and outflows

Carolin Villforth, Tom L. Underwood, Mark Tolson, Nikhil Modha

Research output: Contribution to journalArticle

1 Citation (Scopus)
14 Downloads (Pure)

Abstract

Doublet line emission and absorption are common in astronomical sources (e.g. [OIII], [O II], NaD, MgII). In many cases, complex kinematics in the emitting source can cause the doublet lines to merge, making characterization of the source kinematics challenging. Here, we present a non-parametricmethod for resolving merged doublet lines when the line ratio andwavelength difference are known. The method takes as input only the line ratio and wavelength difference, using these quantities to resolve the components of the doublet without resorting to fitting (e.g. using multiple Gaussians) ormaking any assumptions about the components' line profiles (save that they are the same for both components). The method is simple, fast, and robust. It is also ideal for visualization.We show that the method recovers line profiles of merged emission lines in simulated data. We also show, using simulated data and mathematical analysis, that the method does not significantly increase noise levels in the extracted lines, and is robust to background contamination. We demonstrate the strength of the method by applying it to strongly merged [OIII] 5007/4959 Å in Active Galactic Nuclei. A PYTHON implementation of the method is provided in the appendix.

Original languageEnglish
Pages (from-to)3782-3793
Number of pages12
JournalMonthly Notices of the Royal Astronomical Society
Volume481
Issue number3
Early online date14 Sep 2018
DOIs
Publication statusPublished - 1 Dec 2018

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outflow
kinematics
applications of mathematics
profiles
active galactic nuclei
wavelengths
contamination
wavelength
causes
mathematical analysis
method
visualization

Keywords

  • ISM: jets and outflows
  • ISM: kinematics and dynamics
  • Line: profiles
  • Methods: analytical
  • Stars: kinematics and dynamics

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

A simple non-parametric method for resolving merged doublet lines : Insights into complex kinematics and outflows. / Villforth, Carolin; Underwood, Tom L.; Tolson, Mark; Modha, Nikhil.

In: Monthly Notices of the Royal Astronomical Society, Vol. 481, No. 3, 01.12.2018, p. 3782-3793.

Research output: Contribution to journalArticle

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