The Cosmic BPT Diagram: Confronting Theory with Observations

TL;DR

This paper compares galaxy emission line ratios across redshifts with theoretical models, revealing that high-redshift galaxies have more extreme ISM conditions and proposing a new redshift-dependent classification scheme for star-forming galaxies and AGN.

Contribution

The study introduces a new redshift-dependent optical classification line based on theoretical models, improving galaxy classification accuracy up to z~3.5.

Findings

High-redshift galaxies (z>1.5) have more extreme ISM conditions.

A transition to local-like conditions occurs between 0.8<z<1.5.

The new classification line is consistent with independent AGN identifications.

Abstract

We compare a large sample of galaxies between 0.5<z<2.6 with theoretical predictions for how the optical diagnostic line ratios in galaxy ensembles change as a function of cosmic time. We show that star forming galaxies at high redshift (z>1.5) are consistent with a model in which the ISM conditions are more extreme at high redshift than seen in the global spectra of local galaxies. We speculate that global spectra of our high redshift galaxies may be dominated by HII regions similar to the extreme clumpy, dense star-forming complexes in the Antennae and M82. The transition to local-type conditions occurs between 0.8<z<1.5. We conclude that classification schemes developed for local samples should not be applied at high redshift (z > 1.5). We use our theoretical models to derive a new redshift-dependent classification line that utilizes the standard optical diagnostic line ratios [OIII]/H-beta and [NII]/H-alpha. Our new line can be used to separate star-forming galaxies from AGN between z=0 to z~3.5. We anticipate that our redshift-dependent optical classification line will be useful for future large surveys with near-infrared multi-object spectrographs. We apply our classification line to a sample of gravitationally lensed galaxies at z~2.5. Although limited by small numbers, we show that our classification line is consistent with the position of AGN that have been independently confirmed via other methods.