English

ELFO: A Python Package for Emission Line Fitting Optimization in Integral Field Spectroscopy Data

Astrophysics of Galaxies 2026-02-10 v2

Abstract

Integral field spectroscopy (IFS) provides spatially resolved spectra, enabling detailed studies that address the physical and kinematic properties of the interstellar medium. A critical step in analyzing IFS data is the decomposition of emission lines, where different velocity components are often modeled with Gaussian profiles. However, conventional fitting methods that treat each spectrum independently often yield spatial discontinuities in the fitting results. Here, we present Emission Line Fitting Optimization (ELFO), a Python package for IFS spectral fitting. ELFO uses the results of neighboring spectra to determine multiple initial guesses and selects the result that exhibits spatial smoothness. We tested ELFO on IFS data of two quasars obtained from the Multi-Unit Spectroscopic Explorer, where it successfully corrected anomalous fits, revealed previously unresolved substructures, and made large-scale kinematic structures more evident. With minor modifications, this method can also be easily adapted to other IFS data and different emission lines.

Keywords

Cite

@article{arxiv.2602.05396,
  title  = {ELFO: A Python Package for Emission Line Fitting Optimization in Integral Field Spectroscopy Data},
  author = {Hui Guo and Guilin Liu and Jianghui Xu and Chao Geng and Zhicheng He and Shiyin Shen and Lei Hao},
  journal= {arXiv preprint arXiv:2602.05396},
  year   = {2026}
}

Comments

13 pages, 12 figures, accepted for publication in AJ

R2 v1 2026-07-01T09:37:24.527Z