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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.

The Hidden "AGN Main Sequence": Evidence for a Universal Black Hole Accretion to Star Formation Rate Ratio since z ~ 2 Producing an M BH-M * Relation (2012)
Journal Article
Mullaney, J., Daddi, E., Béthermin, M., Elbaz, D., Juneau, S., Pannella, M., …Hickox, R. (2012). The Hidden "AGN Main Sequence": Evidence for a Universal Black Hole Accretion to Star Formation Rate Ratio since z ~ 2 Producing an M BH-M * Relation. Astrophysical Journal Letters, 753(2), Article L30. https://doi.org/10.1088/2041-8205/753/2/l30

GOODS-Herschel: the far-infrared view of star formation in active galactic nucleus host galaxies since z ≈ 3 (2012)
Journal Article
Mullaney, J., Pannella, M., Daddi, E., Alexander, D., Elbaz, D., Hickox, R., …Xue, Y. (2012). GOODS-Herschel: the far-infrared view of star formation in active galactic nucleus host galaxies since z ≈ 3. Monthly Notices of the Royal Astronomical Society, 419(1), 95-115. https://doi.org/10.1111/j.1365-2966.2011.19675.x

We present a study of the infrared properties of X-ray selected, moderate-luminosity (i.e. LX= 1042–1044 erg s−1) active galactic nuclei (AGNs) up to z ≈ 3, in order to explore the links between star formation in galaxies and accretion on to their ce... Read More about GOODS-Herschel: the far-infrared view of star formation in active galactic nucleus host galaxies since z ≈ 3.

Defining the intrinsic AGN infrared spectral energy distribution and measuring its contribution to the infrared output of composite galaxies (2011)
Journal Article
Mullaney, J., Alexander, D., Goulding, A., & Hickox, R. (2011). Defining the intrinsic AGN infrared spectral energy distribution and measuring its contribution to the infrared output of composite galaxies. Monthly Notices of the Royal Astronomical Society, 414(2), 1082-1110. https://doi.org/10.1111/j.1365-2966.2011.18448.x

We use infrared spectroscopy and photometry to empirically define the intrinsic mid- to far-infrared spectral energy distribution (i.e. 6–100 μm SED) of thermal emission produced by typical (i.e. 2–10 keV luminosity, L2-10 keV∼ 1042–1044 erg s−1) act... Read More about Defining the intrinsic AGN infrared spectral energy distribution and measuring its contribution to the infrared output of composite galaxies.