# University of Hertfordshire

## Investigating the Unification of LOFAR-detected powerful AGN in the Boötes Field

Research output: Research - peer-reviewArticle

### Documents

• Leah K. Morabito
• W. L. Williams
• Kenneth J. Duncan
• H.~J.~A. Röttgering
• George Miley
• Aayush Saxena
• Peter Barthel
• Philip N. Best
• M. Bruggen
• G. Brunetti
• K. T. Chyży
• D. Engels
• M. J. Hardcastle
• J. J. Harwood
• Matt J. Jarvis
• E. K. Mahony
• I. Prandoni
• Timothy W. Shimwell
• Alexander Shulevski
• C. Tasse
Original language English 1883-1896 Monthly Notices of the Royal Astronomical Society 1 Aug 2017 469 2 21 Apr 2017 10.1093/mnras/stx959 Published - 1 Aug 2017

### Abstract

Low radio frequency surveys are important for testing unified models of radio-loud quasars and radio galaxies. Intrinsically similar sources that are randomly oriented on the sky will have different projected linear sizes. Measuring the projected linear sizes of these sources provides an indication of their orientation. Steep-spectrum isotropic radio emission allows for orientation-free sample selection at low radio frequencies. We use a new radio survey of the Bo\"otes field at 150 MHz made with the Low Frequency Array (LOFAR) to select a sample of radio sources. We identify 44 radio galaxies and 16 quasars with powers $P>10^{25.5}$ W Hz$^{-1}$ at 150 MHz using cross-matched multi-wavelength information from the AGN and Galaxy Evolution Survey (AGES), which provides spectroscopic redshifts. We find that LOFAR-detected radio sources with steep spectra have projected linear sizes that are on average 4.4$\pm$1.4 larger than those with flat spectra. The projected linear sizes of radio galaxies are on average 3.1$\pm$1.0 larger than those of quasars (2.0$\pm$0.3 after correcting for redshift evolution). Combining these results with three previous surveys, we find that the projected linear sizes of radio galaxies and quasars depend on redshift but not on power. The projected linear size ratio does not correlate with either parameter. The LOFAR data is consistent within the uncertainties with theoretical predictions of the correlation between the quasar fraction and linear size ratio, based on an orientation-based unification scheme.