A large sample of Kohonen selected E+A (post-starburst) galaxies from the Sloan Digital Sky Survey

TL;DR

This study compiles a large sample of local post-starburst galaxies from SDSS using Kohonen self-organising maps, revealing their transitional nature, morphological disturbances, and potential hidden AGN activity.

Contribution

It introduces a new large, publicly available catalogue of PSB galaxies identified via Kohonen maps, with detailed analysis of their properties and AGN indicators.

Findings

57% of PSB galaxies show morphological distortions

Low AGN fraction of 2-3% based on radio and MIR criteria

MIR excess suggests possible hidden AGNs in PSB galaxies

Abstract

We aim to create a large sample of local post-starburst (PSB) galaxies to study their characteristic properties, particularly morphological features indicative of gravitational distortions and indications for active galactic nuclei (AGNs). The selection is based on a huge Kohonen self-organising map (SOM) of about one million SDSS spectra. The SOM is made fully available for the astronomical community, in combination with an interactive user interface. We compiled a catalogue of 2665 PSB galaxies with redshifts z < 0.4. In the colour-mass diagram, the PSB sample is found to be clearly concentrated towards the region between the red and the blue cloud, in agreement with the idea that PSB galaxies represent the transitioning phase between actively and passively evolving galaxies. The relative frequency of morphologically distorted PSB galaxies is at least 57%, significantly higher than in a comparison sample. The search for AGNs based on conventional selection criteria in the radio and MIR results in a low AGN fraction of 2 - 3%. We confirm an MIR excess in the mean SED of the PSB galaxy sample that may indicate hidden AGNs, though other sources are also possible. (Abstract modified to match the arXiv format.)