First Detection of the [OIII] 88 micron Line at High Redshifts: Characterizing the Starburst and Narrow Line Regions in Extreme Luminosity Systems

TL;DR

This paper reports the first detection of the 88 micron [OIII] line in high-redshift galaxies, revealing details about starburst and AGN activity in the early Universe through spectral analysis.

Contribution

It presents the first observations of the [OIII] 88 micron line at high redshifts, providing insights into star formation and AGN regions in early galaxies.

Findings

[OIII] line detected at z > 2.8 in two galaxies

Starburst regions contribute significantly to IR luminosity

Line emission can originate from both star-forming regions and AGN narrow line regions

Abstract

We have made the first detections of the 88 micron [OIII] line from galaxies in the early Universe, detecting the line from the lensed AGN/starburst composite systems APM 08279+5255 at z = 3.911 and SMM J02399-0136 at z = 2.8076. The line is exceptionally bright from both systems, with apparent (lensed) luminosities ~10^11 L_solar. For APM 08279, the [OIII] line flux can be modeled in a star formation paradigm, with the stellar radiation field dominated by stars with effective temperatures, Teff >36,000 K, similar to the starburst found in M82. The model implies ~35% of the total far-IR luminosity of the system is generated by the starburst, with the remainder arising from dust heated by the AGN. The 88 micron line can also be generated in the narrow line region of the AGN if gas densities are around a few 1000 cm-3. For SMM J02399 the [OIII] line likely arises from HII regions formed by hot (Teff >40,000 K) young stars in a massive starburst that dominates the far-IR luminosity of the system. The present work demonstrates the utility of the [OIII] line for characterizing starbursts and AGN within galaxies in the early Universe. These are the first detections of this astrophysically important line from galaxies beyond a redshift of 0.05.