Herschel Survey of the Palomar-Green QSOs at Low Redshift

TL;DR

This study uses Herschel data to analyze the cold dust properties of 85 low-redshift QSOs, revealing typical dust temperatures, masses, and insights into star formation and dust heating mechanisms.

Contribution

First comprehensive Herschel-based analysis of cold dust properties in a large sample of low-redshift quasars, combining multi-wavelength data for detailed infrared spectral energy distributions.

Findings

Average dust temperature of 33 K with a standard deviation of 8 K.

Average dust mass of 7 million solar masses with a standard deviation of 9 million.

Star-formation rates from FIR continuum are higher than those from PAH emission.

Abstract

We investigate the global cold dust properties of 85 nearby (z < 0.5) QSOs, chosen from the Palomar-Green sample of optically luminous quasars. We determine their infrared spectral energy distributions and estimate their rest-frame luminosities by combining Herschel data from 70 to 500 microns with near-infrared and mid-infrared measurements from the Two Micron All Sky Survey (2MASS) and the Wide-Field Infrared Survey Explorer (WISE). In most sources the far-infrared (FIR) emission can be attributed to thermally heated dust. Single temperature modified black body fits to the FIR photometry give an average dust temperature for the sample of 33~K, with a standard deviation of 8~K, and an average dust mass of 7E6 Solar Masses with a standard deviation of 9E6 Solar Masses. Estimates of star-formation that are based on the FIR continuum emission correlate with those based on the 11.3 microns PAH feature, however, the star-formation rates estimated from the FIR continuum are higher than those estimated from the 11.3 microns PAH emission. We attribute this result to a variety of factors including the possible destruction of the PAHs and that, in some sources, a fraction of the FIR originates from dust heated by the active galactic nucleus and by old stars.