The SCUBA Half-Degree Extragalactic Survey (SHADES) - VIII. The Nature of Faint Submm Galaxies in SHADES, SWIRE and SXDF Surveys by Clements, D, Vaccari, M, Babbedge, T, Oliver, S, Rowan-Robinson, M, Davoodi, P, Ivison, R, Farrah, D, Dunlop, J, Shupe, D, Waddington, I, Simpson, C, Furusawa, H, Serjeant, S, Afonso-Luis, A, Alexander, D, Aretxaga, I, Blain, A, Borys, C, Chapman, S, Coppin, K, Dunne, L, Dye, S, Eales, SA, Evans, T

“…Optical data for the sources comes from the Subaru-XMM Deep Field (SXDF) and mid- and far-IR fluxes from SWIRE. We obtain photometric redshift estimates for our sources using optical and IRAC 3.6 and 4.5 micron fluxes. …”

Processing political misinformation: comprehending the Trump phenomenon by Lewandowsky, Stephan, Ecker, Ullrich K. H., Swire-Thompson, Briony, Berinsky, Adam

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Does truth matter to voters? The effects of correcting political misinformation in an Australian sample by Aird, Michael J., Ecker, Ullrich K. H., Lewandowsky, Stephan, Swire-Thompson, Briony, Berinsky, Adam

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They Might Be a Liar But They’re My Liar: Source Evaluation and the Prevalence of Misinformation by Swire‐Thompson, Briony, Ecker, Ullrich K. H., Lewandowsky, Stephan, Berinsky, Adam J., Berinsky, Adam

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Giant Preputial Calculus: The First Reported Case in Malaysia by Tze, Huat Chong, Mohd Zuki Asyraf, Firdaus Hayati, Nornazirah Azizan, Nik Amin Sahid, Ting, Jesse Ron Swire, Andee Dzulkarnaen Zakaria

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Oligodendrocyte dynamics dictate cognitive performance outcomes of working memory training in mice by Shimizu, T, Nayar, SG, Swire, M, Jiang, Y, Grist, M, Kaller, M, Sampaio Baptista, C, Bannerman, DM, Johansen-Berg, H, Ogasawara, K, Tohyama, K, Li, H, Richardson, WD

A 15 mu m selected sample of high-z starbursts and AGNs by Hernan-Caballero, A, Perez-Fournon, I, Rowan-Robinson, M, Rigopoulou, D, Afonso-Luis, A, Hatziminaoglou, E, Gonzalez-Solares, E, Montenegro-Montes, F, Vila-Vilaro, B, Farrah, D, Lari, C, Vaccari, M, Babbedge, T, Oliver, S, ClementS, D, Serjeant, S, Pozzi, F, La Franca, F, Gruppioni, C, Valtchanov, I, Lonsdale, C, Team, SWIRE

“…The selected ELAIS sources have a wide multi-wavelength coverage, including ISOCAM, ISOPHOT, IRAC and MIPS (from SWIRE), and optical photometry. Here we present the sample selection and results from the IRS spectroscopy.…”

Galaxy evolution with FMOS by Curtis Lake, E

“…The results indicate that the SWIRE (Spitzer Wide area InfraRed Extragalactic Survey) fields are too small to provide adequate sources with a consistent selection mechanism. …”

The discovery of a typical radio galaxy at z = 4.88 by Jarvis, M, Teimourian, H, Simpson, C, Smith, D, Rawlings, S, Bonfield, D

“…It also has a luminosity consistent with being drawn from the break of the radio luminosity function and can therefore be considered as a typical radio galaxy. Using the Spitzer-SWIRE data over this field we find that the host galaxy is consistent with being similarly massive to the lower redshift powerful radio galaxies (~1-3L*). …”

Cold dust and young starbursts: spectral energy distributions of Herschel SPIRE sources from the HerMES survey by Rowan-Robinson, M, Roseboom, I, Vaccari, M, Amblard, A, Arumugam, V, Auld, R, Aussel, H, Babbedge, T, Blain, A, Bock, J, Boselli, A, Brisbin, D, Buat, V, Burgarella, D, Castro-Rodriguez, N, Cava, A, Chanial, P, Clements, D, Conley, A, Conversi, L, Cooray, A, Dowell, C, Dwek, E, Dye, S, Eales, S

“…We present spectral energy distributions (SEDs) for 68 Herschel sources detected at 5σ at 250, 350 and 500 μm in the HerMES SWIRE-Lockman field. We explore whether existing models for starbursts, quiescent star-forming galaxies and active galactic nucleus dust tori are able to model the full range of SEDs measured with Herschel. …”

The faint radio source population at 15.7 GHz - II. Multi-wavelength properties by Whittam, I, Riley, J, Green, D, Jarvis, M, Vaccari, M

“…We have matched this sample to a range of multi-wavelength catalogues, including SERVS, SWIRE, UKIDSS and optical data; multi-wavelength counterparts are found for 80 of the 96 sources and spectroscopic redshifts are available for 24 sources. …”

The star-formation rate density from z = 0-6 by Rowan-Robinson, M, Oliver, S, Wang, L, Farrah, D, Clements, D, Gruppioni, C, Marchetti, L, Rigopoulou, D, Vaccari, M

“…We use 3035 Herschel-SPIRE 500$\mu$m sources from 20.3 sq deg of sky in the HerMES Lockman, ES1 and XMM-LSS areas to estimate the star-formation rate density at z = 1-6. 500 mu sources are associated first with 350 and 250 mu sources, and then with Spitzer 24 mu sources from the SWIRE photometric redshift catalogue. The infrared and submillimetre data are fitted with a set of radiative-transfer templates corresponding to cirrus (quiescent) and starburst galaxies. …”