Outputs (19)

The KMOS AGN Survey at High redshift (KASHz): the prevalence and drivers of ionized outflows in the host galaxies of X-ray AGN (2015)
Journal Article
Harrison, C., Alexander, D., Mullaney, J., Stott, J., Swinbank, A., Arumugam, V., …Sharples, R. (2016). The KMOS AGN Survey at High redshift (KASHz): the prevalence and drivers of ionized outflows in the host galaxies of X-ray AGN. Monthly Notices of the Royal Astronomical Society, 456(2), 1195-1220. https://doi.org/10.1093/mnras/stv2727

We present the first results from the KMOS (K-band Multi-Object Spectrograph) AGN (active galactic nuclei) Survey at High redshift (KASHz), a VLT/KMOS integral-field spectroscopic (IFS) survey of z ≳ 0.6 AGN. We present galaxy-integrated spectra of 8... Read More about The KMOS AGN Survey at High redshift (KASHz): the prevalence and drivers of ionized outflows in the host galaxies of X-ray AGN.

HSIM: a simulation pipeline for the HARMONI integral field spectrograph on the European ELT (2015)
Journal Article
Zieleniewski, S., Thatte, N., Kendrew, S., Houghton, R., Swinbank, A., Tecza, M., …Fusco, T. (2015). HSIM: a simulation pipeline for the HARMONI integral field spectrograph on the European ELT. Monthly Notices of the Royal Astronomical Society, 453(4), 3754-3765. https://doi.org/10.1093/mnras/stv1860

We present hsim: a dedicated pipeline for simulating observations with the High Angular Resolution Monolithic Optical and Near-infrared Integral field spectrograph (HARMONI) on the European Extremely Large Telescope. hsim takes high spectral and spat... Read More about HSIM: a simulation pipeline for the HARMONI integral field spectrograph on the European ELT.

Cold dust emission from X-ray AGN in the SCUBA-2 Cosmology Legacy Survey: dependence on luminosity, obscuration and AGN activity (2015)
Journal Article
Banerji, M., McMahon, R., Willott, C., Geach, J., Harrison, C., Alaghband-Zadeh, S., …van der Werf, P. (2015). Cold dust emission from X-ray AGN in the SCUBA-2 Cosmology Legacy Survey: dependence on luminosity, obscuration and AGN activity. Monthly Notices of the Royal Astronomical Society, 454(1), 419-438. https://doi.org/10.1093/mnras/stv1881

We study the 850-μm emission in X-ray-selected active galactic nuclei (AGN) in the ∼2 deg2 COSMOS field using new data from the SCUBA-2 Cosmology Legacy Survey. We find 19 850-μm bright X-ray AGN in a ‘high-sensitivity’ region covering 0.89 deg2 with... Read More about Cold dust emission from X-ray AGN in the SCUBA-2 Cosmology Legacy Survey: dependence on luminosity, obscuration and AGN activity.

Revealing the complex nature of the strong gravitationally lensed system H-ATLAS J090311.6+003906 using ALMA (2015)
Journal Article
Dye, S., Furlanetto, C., Swinbank, A., Vlahakis, C., Nightingale, J., Dunne, L., …van der Werf, P. (2015). Revealing the complex nature of the strong gravitationally lensed system H-ATLAS J090311.6+003906 using ALMA. Monthly Notices of the Royal Astronomical Society, 452(3), 2258-2268. https://doi.org/10.1093/mnras/stv1442

We have modelled Atacama Large Millimetre/sub-millimetre Array (ALMA) long baseline imaging of the strong gravitational lens system H-ATLAS J090311.6+003906 (SDP.81). We have reconstructed the distribution of band 6 and 7 continuum emission in the z... Read More about Revealing the complex nature of the strong gravitationally lensed system H-ATLAS J090311.6+003906 using ALMA.

Early Science with the Large Millimeter Telescope: observations of dust continuum and CO emission lines of cluster-lensed submillimetre galaxies at z=2.0-4.7 (2015)
Journal Article
Zavala, J., Yun, M., Aretxaga, I., Hughes, D., Wilson, G., Geach, J., …Zeballos, M. (2015). Early Science with the Large Millimeter Telescope: observations of dust continuum and CO emission lines of cluster-lensed submillimetre galaxies at z=2.0-4.7. Monthly Notices of the Royal Astronomical Society, 452(2), 1140-1151. https://doi.org/10.1093/mnras/stv1351

We present Early Science observations with the Large Millimeter Telescope, AzTEC 1.1 mm continuum images and wide bandwidth spectra (73–111 GHz) acquired with the Redshift Search Receiver, towards four bright lensed submillimetre galaxies identified... Read More about Early Science with the Large Millimeter Telescope: observations of dust continuum and CO emission lines of cluster-lensed submillimetre galaxies at z=2.0-4.7.

A remarkably flat relationship between the average star formation rate and AGN luminosity for distant X-ray AGN (2015)
Journal Article
Stanley, F., Harrison, C., Alexander, D., Swinbank, A., Aird, J., Del Moro, A., …Mullaney, J. (2015). A remarkably flat relationship between the average star formation rate and AGN luminosity for distant X-ray AGN. Monthly Notices of the Royal Astronomical Society, 453(1), 591-604. https://doi.org/10.1093/mnras/stv1678

In this study, we investigate the relationship between the star formation rate (SFR) and AGN luminosity (LAGNLAGN) for ∼2000 X-ray detected AGN. The AGN span over three orders of magnitude in X-ray luminosity (1042<L2−8keV<1045.5ergs−11042<L2−8keV<10...

The SCUBA-2 Cosmology Legacy Survey: ALMA resolves the bright-end of the submillimeter number counts (2015)
Journal Article
Simpson, J., Smail, I., Swinbank, A., Chapman, S., Geach, J., Ivison, R., …van der Werf, P. (2015). The SCUBA-2 Cosmology Legacy Survey: ALMA resolves the bright-end of the submillimeter number counts. Astrophysical Journal, 807(2), Article 128. https://doi.org/10.1088/0004-637x/807/2/128

We present high-resolution 870 μm Atacama Large Millimeter/sub-millimeter Array (ALMA) continuum maps of 30 bright sub-millimeter sources in the UKIDSS UDS field. These sources are selected from deep, 1 degree2 850 μm maps from the SCUBA-2 Cosmology... Read More about The SCUBA-2 Cosmology Legacy Survey: ALMA resolves the bright-end of the submillimeter number counts.

Resolved spectroscopy of gravitationally lensed galaxies: global dynamics and star-forming clumps on ∼100 pc scales at 1 < z < 4 (2015)
Journal Article
Livermore, R. C., Jones, T. A., Richard, J., Bower, R. G., Swinbank, A. M., Yuan, T.-. T., Edge, A. C., Ellis, R. S., Kewley, L. J., Smail, I., Coppin, K. E. K., & Ebeling, H. (2015). Resolved spectroscopy of gravitationally lensed galaxies: global dynamics and star-forming clumps on ∼100 pc scales at 1 < z < 4. Monthly Notices of the Royal Astronomical Society, 450(2), 1812-1835. https://doi.org/10.1093/mnras/stv686

We present adaptive optics-assisted integral field spectroscopy around the Hα or Hβ lines of 12 gravitationally lensed galaxies obtained with VLT/SINFONI, Keck/OSIRIS and Gemini/NIFS. We combine these data with previous observations and investigate t... Read More about Resolved spectroscopy of gravitationally lensed galaxies: global dynamics and star-forming clumps on ∼100 pc scales at 1 < z < 4.

Dusty starbursts and the formation of elliptical galaxies: A SCUBA-2 survey of a z = 1.46 cluster (2015)
Journal Article
Ma, C., Smail, I., Swinbank, A., Simpson, J., Thomson, A., Chen, C., …Kodama, T. (2015). Dusty starbursts and the formation of elliptical galaxies: A SCUBA-2 survey of a z = 1.46 cluster. Astrophysical Journal, 806(2), Article 257. https://doi.org/10.1088/0004-637x/806/2/257

We report the results of a deep SCUBA-2 850 and 450 μm survey for dust-obscured ultra-/luminous infrared galaxies (U/LIRGs) in the field of the z = 1.46 cluster XCS J2215.9−1738. We detect a striking overdensity of submillimeter sources coincident wi... Read More about Dusty starbursts and the formation of elliptical galaxies: A SCUBA-2 survey of a z = 1.46 cluster.

An ALMA Survey of Sub-millimeter Galaxies in the Extended Chandra Deep Field South: Physical Properties Derived from Ultraviolet-to-radio Modeling (2015)
Journal Article
da Cunha, E., Walter, F., Smail, I., Swinbank, A., Simpson, J., Decarli, R., …Thomson, A. (2015). An ALMA Survey of Sub-millimeter Galaxies in the Extended Chandra Deep Field South: Physical Properties Derived from Ultraviolet-to-radio Modeling. Astrophysical Journal, 806(1), https://doi.org/10.1088/0004-637x/806/1/110

The ALESS survey has followed up on a sample of 122 sub-millimeter sources in the Extended Chandra Deep Field South at 870 μmwith the Atacama Large Millimeter Array (ALMA), allowing us to pinpoint the positions of submillimeter galaxies (SMGs) to ∼0.... Read More about An ALMA Survey of Sub-millimeter Galaxies in the Extended Chandra Deep Field South: Physical Properties Derived from Ultraviolet-to-radio Modeling.