Professor Alastair Edge's Outputs (15)

Galaxy And Mass Assembly (GAMA): Panchromatic Data Release (far-UV-far-IR) and the low-z energy budget (2015)
Journal Article
Driver, S. P., Wright, A. H., Andrews, S. K., Davies, L. J., Kafle, P. R., Lange, R., …Williams, R. (2016). Galaxy And Mass Assembly (GAMA): Panchromatic Data Release (far-UV-far-IR) and the low-z energy budget. Monthly Notices of the Royal Astronomical Society, 455(4), 3911-3942. https://doi.org/10.1093/mnras/stv2505

We present the Galaxy And Mass Assembly (GAMA) Panchromatic Data Release (PDR) constituting over 230 deg2 of imaging with photometry in 21 bands extending from the far-UV to the far-IR. These data complement our spectroscopic campaign of over 300k ga... Read More about Galaxy And Mass Assembly (GAMA): Panchromatic Data Release (far-UV-far-IR) and the low-z energy budget.

Dynamical analysis of galaxy cluster merger Abell 2146 (2015)
Journal Article
White, J., Canning, R., King, L., Lee, B., Russell, H., Baum, S., …Sanders, J. (2015). Dynamical analysis of galaxy cluster merger Abell 2146. Monthly Notices of the Royal Astronomical Society, 453(3), 2718-2730. https://doi.org/10.1093/mnras/stv1831

We present a dynamical analysis of the merging galaxy cluster system Abell 2146 using spectroscopy obtained with the Gemini Multi-Object Spectrograph on the Gemini North telescope. As revealed by the Chandra X-ray Observatory, the system is undergoin... Read More about Dynamical analysis of galaxy cluster merger Abell 2146.

High radio-frequency properties and variability of brightest cluster galaxies (2015)
Journal Article
Hogan, M., Edge, A., Geach, J., Grainge, K., Hlavacek-Larrondo, J., Hovatta, T., …Saunders, R. (2015). High radio-frequency properties and variability of brightest cluster galaxies. Monthly Notices of the Royal Astronomical Society, 453(2), 1223-1240. https://doi.org/10.1093/mnras/stv1518

We consider the high radio-frequency (15–353 GHz) properties and variability of 35 brightest cluster galaxies (BCGs). These are the most core-dominated sources drawn from a parent sample of more than 700 X-ray selected clusters, thus allowing us to r... Read More about High radio-frequency properties and variability of brightest cluster galaxies.

Deep Chandra, HST-COS, and Megacam Observations of the Phoenix Cluster: Extreme Star Formation and AGN Feedback on Hundred Kiloparsec Scales (2015)
Journal Article
McDonald, M., McNamara, B., van Weeren, R., Applegate, D., Bayliss, M., Bautz, M., …ZuHone, J. (2015). Deep Chandra, HST-COS, and Megacam Observations of the Phoenix Cluster: Extreme Star Formation and AGN Feedback on Hundred Kiloparsec Scales. Astrophysical Journal, 811(2), https://doi.org/10.1088/0004-637x/811/2/111

We present new ultraviolet, optical, and X-ray data on the Phoenix galaxy cluster (SPT-CLJ2344-4243). Deep optical imaging reveals previously undetected filaments of star formation, extending to radii of ~50–100 kpc in multiple directions. Combined U... Read More about Deep Chandra, HST-COS, and Megacam Observations of the Phoenix Cluster: Extreme Star Formation and AGN Feedback on Hundred Kiloparsec Scales.

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 comprehensive study of the radio properties of brightest cluster galaxies (2015)
Journal Article
Hogan, M., Edge, A., Hlavacek-Larrondo, J., Grainge, K., Hamer, S., Mahony, E., …Wilman, R. (2015). A comprehensive study of the radio properties of brightest cluster galaxies. Monthly Notices of the Royal Astronomical Society, 453(2), 1201-1222. https://doi.org/10.1093/mnras/stv1517

We examine the radio properties of the brightest cluster galaxies (BCGs) in a large sample of X-ray selected galaxy clusters comprising the Brightest Cluster Sample (BCS), the extended BCS and ROSAT-ESO Flux Limited X-ray cluster catalogues. We have... Read More about A comprehensive study of the radio properties of brightest cluster galaxies.

Effects of the variability of the nucleus of NGC 1275 on X-ray observations of the surrounding intracluster medium (2015)
Journal Article
Fabian, A., Walker, S., Pinto, C., Russell, H., & Edge, A. (2015). Effects of the variability of the nucleus of NGC 1275 on X-ray observations of the surrounding intracluster medium. Monthly Notices of the Royal Astronomical Society, 451(3), 3061-3067. https://doi.org/10.1093/mnras/stv1134

The active galaxy NGC 1275 lies at the centre of the Perseus cluster of galaxies, which is the X-ray brightest cluster in the Sky. The nucleus shows large variability over the past few decades. We compile a light curve of its X-ray emission covering... Read More about Effects of the variability of the nucleus of NGC 1275 on X-ray observations of the surrounding intracluster medium.

Far-ultraviolet morphology of star-forming filaments in cool core brightest cluster galaxies (2015)
Journal Article
Tremblay, G., O'Dea, C., Baum, S., Mittal, R., McDonald, M., Combes, F., …Voit, G. (2015). Far-ultraviolet morphology of star-forming filaments in cool core brightest cluster galaxies. Monthly Notices of the Royal Astronomical Society, 451(4), 3768-3800. https://doi.org/10.1093/mnras/stv1151

We present a multiwavelength morphological analysis of star-forming clouds and filaments in the central (≲50 kpc) regions of 16 low-redshift (z < 0.3) cool core brightest cluster galaxies. New Hubble Space Telescope imaging of far-ultraviolet continu... Read More about Far-ultraviolet morphology of star-forming filaments in cool core brightest cluster galaxies.

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.

Linking Galaxies to Dark Matter Halos at z ~ 1 : Dependence of Galaxy Clustering on Stellar Mass and Specific Star Formation Rate (2015)
Journal Article
Kim, J., Im, M., Lee, S., Edge, A. C., Wake, D. A., Merson, A. I., & Jeon, Y. (2015). Linking Galaxies to Dark Matter Halos at z ~ 1 : Dependence of Galaxy Clustering on Stellar Mass and Specific Star Formation Rate. Astrophysical Journal, 806(2), https://doi.org/10.1088/0004-637x/806/2/189

We study the dependence of angular two-point correlation functions on stellar mass (M*) and specific star formation rate (sSFR) of ${M}_{*}\gt {10}^{10}{M}_{\odot }$ galaxies at $z\sim 1$. The data from the UK Infrared Telescope Infrared Deep Sky Sur... Read More about Linking Galaxies to Dark Matter Halos at z ~ 1 : Dependence of Galaxy Clustering on Stellar Mass and Specific Star Formation Rate.

The behaviour of dark matter associated with four bright cluster galaxies in the 10 kpc core of Abell 3827 (2015)
Journal Article
Massey, R., Williams, L., Smit, R., Swinbank, M., Kitching, D., Harvey, D., …Tittley, E. (2015). The behaviour of dark matter associated with four bright cluster galaxies in the 10 kpc core of Abell 3827. Monthly Notices of the Royal Astronomical Society, 449(4), 3393-3406. https://doi.org/10.1093/mnras/stv467

Galaxy cluster Abell 3827 hosts the stellar remnants of four almost equally bright elliptical galaxies within a core of radius 10 kpc. Such corrugation of the stellar distribution is very rare, and suggests recent formation by several simultaneous me... Read More about The behaviour of dark matter associated with four bright cluster galaxies in the 10 kpc core of Abell 3827.

Storm in a "Teacup": A Radio-quiet Quasar with ≈10 kpc Radio-emitting Bubbles and Extreme Gas Kinematics (2015)
Journal Article
Harrison, C., Thomson, A., Alexander, D., Bauer, F., Edge, A., Hogan, M., …Swinbank, A. (2015). Storm in a "Teacup": A Radio-quiet Quasar with ≈10 kpc Radio-emitting Bubbles and Extreme Gas Kinematics. Astrophysical Journal, 800(1), Article 45. https://doi.org/10.1088/0004-637x/800/1/45

We present multi-frequency (1-8 GHz) Very Large Array data, combined with VIsible MultiObject Spectrograph integral field unit data and Hubble Space Telescope imaging, of a z = 0.085 radio-quiet type 2 quasar (with L 1.4 GHz ≈ 5 × 1023 W Hz–1 and L A... Read More about Storm in a "Teacup": A Radio-quiet Quasar with ≈10 kpc Radio-emitting Bubbles and Extreme Gas Kinematics.

An ALMA Survey of Submillimeter Galaxies in the Extended Chandra Deep Field South: Near-infrared Morphologies and Stellar Sizes (2015)
Journal Article
Chen, C., Smail, I., Swinbank, A., Simpson, J., Ma, C., Alexander, D., …van der Werf, P. (2015). An ALMA Survey of Submillimeter Galaxies in the Extended Chandra Deep Field South: Near-infrared Morphologies and Stellar Sizes. Astrophysical Journal, 799(2), Article 194. https://doi.org/10.1088/0004-637x/799/2/194

We analyze Hubble Space Telescope WFC3/H 160-band observations of a sample of 48 Atacama Large Millimeter/submillimeter Array detected submillimeter galaxies (SMGs) in the Extended Chandra Deep Field South field, to study their stellar morphologies a... Read More about An ALMA Survey of Submillimeter Galaxies in the Extended Chandra Deep Field South: Near-infrared Morphologies and Stellar Sizes.

The SCUBA-2 Cosmology Legacy Survey: ALMA Resolves the Rest-frame Far-infrared Emission of Sub-millimeter Galaxies (2015)
Journal Article
Simpson, J., Smail, I., Swinbank, A., Almaini, O., Blain, A., Bremer, M., …van der Werf, P. (2015). The SCUBA-2 Cosmology Legacy Survey: ALMA Resolves the Rest-frame Far-infrared Emission of Sub-millimeter Galaxies. Astrophysical Journal, 799(1), Article 81. https://doi.org/10.1088/0004-637x/799/1/81

We present high-resolution (0.''3) Atacama Large Millimeter Array 870 μm imaging of 52 sub-millimeter galaxies (SMGs) in the Ultra Deep Survey field to investigate the size and morphology of the sub-millimeter (sub-mm) emission on 2-10 kpc scales. We... Read More about The SCUBA-2 Cosmology Legacy Survey: ALMA Resolves the Rest-frame Far-infrared Emission of Sub-millimeter Galaxies.