This repository contains a preliminary IFU-based analysis of the DGIS galaxy NGC1510, carried out as part of my research training on integral-field spectroscopy and galaxy evolution.
Integral-field spectroscopy (IFS) allows us to obtain a full spectrum at each spatial position in a galaxy, making it possible to study spatially resolved emission-line properties, ionized gas structure, and internal physical variation.
This project is motivated by:
- the DGIS survey framework for nearby dwarf galaxies
- the use of IFU datacubes for spatially resolved analysis
- the multi-Balmer methodology discussed in Reddy et al. (2020)
After my second progress report, the next task assigned by my advisor was:
- identify the common reliable spaxels shared by Hα, Hβ, and Hγ
- construct a composite spectrum from those common spaxels
- plot the Balmer spectral panels for each selected spaxel
I read the NGC1510 IFU datacube and extracted the key data structures required for spectral analysis.
I generated 2D flux maps for several important emission lines, including:
- Hα
- Hβ
- Hγ
- Hδ
- Hη
- [OIII]5007
- [NII]6583
Using the Hα flux map, I located the brightest reliable Hα spaxel and used it as the central spaxel for spectral inspection.
I plotted the observed spectrum, total fit, and continuum fit for the central spaxel to verify the quality of the emission-line fitting.
Following the logic of multi-Balmer analysis, I selected the spaxels that are simultaneously reliable in Hα, Hβ, and Hγ.
For the shared spaxels, I completed the first-stage products:
- a composite spectrum constructed from the common sample
- Balmer spectral panels for individual selected spaxels
ifu-ngc1510-balmer-analysis/
├── docs/ # reports and project notes
├── figures/ # maps, spectra, and selected Balmer panels
├── results/ # selected spaxel lists and stage summaries
├── src/ # notebooks and scripts