Outputs (3)

An ALMA survey of sub-millimetre Galaxies in the Extended Chandra Deep Field South: the far-infrared properties of SMGs (2013)
Journal Article
Swinbank, A., Simpson, J., Smail, I., Harrison, C., Hodge, J., Karim, A., …van der Werf, P. (2014). An ALMA survey of sub-millimetre Galaxies in the Extended Chandra Deep Field South: the far-infrared properties of SMGs. Monthly Notices of the Royal Astronomical Society, 438(2), 1267-1287. https://doi.org/10.1093/mnras/stt2273

We exploit Atacama Large Millimeter Array (ALMA) 870 μm observations of sub-millimetre sources in the Extended Chandra Deep Field South to investigate the far-infrared properties of high-redshift sub-millimetre galaxies (SMGs). Using the precisely lo... Read More about An ALMA survey of sub-millimetre Galaxies in the Extended Chandra Deep Field South: the far-infrared properties of SMGs.

Narrow-line region gas kinematics of 24 264 optically selected AGN: the radio connection (2013)
Journal Article
Mullaney, J., Alexander, D., Fine, S., Goulding, A., Harrison, C., & Hickox, R. (2013). Narrow-line region gas kinematics of 24 264 optically selected AGN: the radio connection. Monthly Notices of the Royal Astronomical Society, 433(1), 622-638. https://doi.org/10.1093/mnras/stt751

Using a sample of 24 264 optically selected active galactic nuclei (AGNs) from the SDSS DR7 data base, we characterize how the profile of the [O III] λ5007 emission line relates to bolometric luminosity (LAGN), Eddington ratio, radio loudness, radio... Read More about Narrow-line region gas kinematics of 24 264 optically selected AGN: the radio connection.

Concurrent supermassive black hole and galaxy growth : linking environment and nuclear activity in z = 2.23 H-alpha emitters (2013)
Journal Article
Lehmer, B., Lucy, A., Alexander, D., Best, P., Geach, J., Harrison, C., …Swinbank, A. (2013). Concurrent supermassive black hole and galaxy growth : linking environment and nuclear activity in z = 2.23 H-alpha emitters. Astrophysical Journal, 765(2), Article 87. https://doi.org/10.1088/0004-637x/765/2/87

We present results from a ≈100 ks Chandra observation of the 2QZ Cluster 1004+00 structure at z = 2.23 (hereafter 2QZ Clus). 2QZ Clus was originally identified as an overdensity of four optically-selected QSOs at z = 2.23 within a 15 × 15 arcmin2 reg... Read More about Concurrent supermassive black hole and galaxy growth : linking environment and nuclear activity in z = 2.23 H-alpha emitters.