ELMA: Ellipse-based Bar Major Axis Estimator
Galactic bars are key non-axisymmetric structures in disk galaxies, driving angular-momentum redistribution and contributing to secular evolution, central mass build-up, and the formation of nuclear structures. Robust and homogeneous measurements of bar length, however, remain challenging, particularly for large imaging surveys, where manual estimates are time-consuming and sensitive to methodological choices. We introduce elma, a standalone, pip-installable Python package for automated bar-length estimation in galaxies already identified as candidate barred systems. The method operates directly on two-dimensional imaging data, using iterative elliptical-isophote fitting to trace the radial ellipticity profile and identify a projected bar-length estimate from the semimajor axis associated with the local maximum in ellipticity. Using the image World Coordinate System information and a user-supplied redshift, elma converts angular measurement into a projected physical length. We demonstrate the package on JWST/NIRCam imaging of barred galaxies in GOODS-South field. The code is released under the MIT license at this repository (https://github.com/BrunaLimaa/elma).
| Item Type | Article |
|---|---|
| Identification Number | 10.3847/2515-5172/ae7d2d |
| Additional information | © 2026. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. https://creativecommons.org/licenses/by/4.0/ |
| Keywords | astroinformatics, astronomy software, galaxy structure |
| Date Deposited | 24 Jun 2026 14:00 |
| Last Modified | 27 Jun 2026 01:07 |
