# Plateau de Bure High-z Blue-Sequence Survey 2 (PHIBSS2): Search for Secondary Sources, CO Luminosity Functions in the Field, and the Evolution of Molecular Gas Density through Cosmic Time

## TL;DR

This study searches for serendipitous CO emission sources in 110 data cubes from PHIBSS2, catalogs 67 candidates, and derives CO luminosity functions and molecular gas density evolution, contributing to understanding galaxy evolution.

## Contribution

It presents a new catalog of secondary CO sources in field observations and constrains their redshifts, luminosity functions, and molecular gas density evolution over cosmic time.

## Key findings

- 67 candidate secondary CO sources identified
- 64% of sources have optical counterparts
- Results agree with previous deep field studies

## Abstract

We report on the results of a search for serendipitous sources in CO emission in 110 cubes targeting CO(2-1), CO(3-2), and CO(6-5) at z ~ 1-2 from the second Plateau de Bure High-z Blue-Sequence Survey (PHIBSS2). The PHIBSS2 observations were part of a 4-year legacy program at the IRAM Plateau de Bure Interferometer aimed at studying early galaxy evolution from the perspective of molecular gas reservoirs. We present a catalog of 67 candidate secondary sources from this search, with 45 out of the 110 data cubes showing sources in addition to the primary target that appear to be field detections, unrelated to the central sources. This catalog includes the redshifts, line widths, fluxes, as well as an estimation of their reliability based on their false positive probability. We perform a search in the 3D-HST/CANDELS catalogs for the secondary CO detections and tentatively find that ~64% of these have optical counterparts, which we use to constrain their redshifts. Finally, we use our catalog of candidate CO detections to derive the CO(2-1), CO(3-2), CO(4-3), CO(5-4), and CO(6-5) luminosity functions over a range of redshifts, as well as the molecular gas mass density evolution. Despite the different methodology, these results are in very good agreement with previous observational constraints derived from blind searches in deep fields. They provide an example of the type of "deep field" science that can be carried out with targeted observations.