Hintze Centre for Astrophysical Surveys

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Total eclipse of the heart: the AM CVn Gaia14aae/ASSASN-14cn

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 452:1 (2015) 1060-1067

Authors:

HC Campbell, TR Marsh, M Fraser, ST Hodgkin, E de Miguel, BT Gänsicke, D Steeghs, A Hourihane, E Breedt, SP Littlefair, SE Koposov, Ł Wyrzykowski, G Altavilla, N Blagorodnova, G Clementini, G Damljanovic, A Delgado, M Dennefeld, AJ Drake, J Fernández-Hernández, G Gilmore, R Gualandi, A Hamanowicz, B Handzlik, LK Hardy, DL Harrison, K Iłkiewicz, PG Jonker, CS Kochanek, Z Kołaczkowski, Z Kostrzewa-Rutkowska, R Kotak, G van Leeuwen, G Leto, P Ochner, M Pawlak, L Palaversa, G Rixon, K Rybicki, BJ Shappee, SJ Smartt, MAP Torres, L Tomasella, M Turatto, K Ulaczyk, S van Velzen, O Vince, NA Walton, P Wielgórski, T Wevers, P Whitelock, A Yoldas, F De Angeli, P Burgess, G Busso, R Busuttil, T Butterley, KC Chambers, C Copperwheat, AB Danilet, VS Dhillon, DW Evans, L Eyer, D Froebrich, A Gomboc, G Holland, TW-S Holoien, JF Jarvis, N Kaiser, DA Kann, D Koester, U Kolb, S Komossa, EA Magnier, A Mahabal, J Polshaw, JL Prieto, T Prusti, M Riello, A Scholz, G Simonian, KZ Stanek, L Szabados, C Waters, RW Wilson
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VIMOS mosaic integral-field spectroscopy of the bulge and disc of the early-type galaxy NGC 4697

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 452:1 (2015) 99-114

Authors:

C Spiniello, NR Napolitano, L Coccato, V Pota, AJ Romanowsky, C Tortora, G Covone, M Capaccioli
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Calibrating high-precision Faraday rotation measurements for LOFAR and the next generation of low-frequency radio telescopes (Corrigendum)

Astronomy & Astrophysics EDP Sciences 581 (2015) c4

Authors:

C Sotomayor-Beltran, C Sobey, JWT Hessels, G de Bruyn, A Noutsos, A Alexov, J Anderson, A Asgekar, IM Avruch, R Beck, ME Bell, MR Bell, MJ Bentum, G Bernardi, P Best, L Birzan, A Bonafede, F Breitling, J Broderick, WN Brouw, M Brüggen, B Ciardi, F de Gasperin, R-J Dettmar, A van Duin, S Duscha, J Eislöffel, H Falcke, RA Fallows, R Fender, C Ferrari, W Frieswijk, MA Garrett, J Grießmeier, T Grit, AW Gunst, TE Hassall, G Heald, M Hoeft, A Horneffer, M Iacobelli, E Juette, A Karastergiou, E Keane, J Kohler, M Kramer, VI Kondratiev, LVE Koopmans, M Kuniyoshi, G Kuper, J van Leeuwen, P Maat, G Macario, S Markoff, JP McKean, DD Mulcahy, H Munk, E Orru, H Paas, M Pandey-Pommier, M Pilia, R Pizzo, AG Polatidis, W Reich, H Röttgering, M Serylak, J Sluman, BW Stappers, M Tagger, Y Tang, C Tasse, S ter Veen, R Vermeulen, RJ van Weeren, RAMJ Wijers, SJ Wijnholds, MW Wise, O Wucknitz, S Yatawatta, P Zarka
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On the triple peaks of SNHunt248 in NGC 5806⋆

Astronomy & Astrophysics EDP Sciences 581 (2015) l4

Authors:

E Kankare, R Kotak, A Pastorello, M Fraser, S Mattila, SJ Smartt, A Bruce, KC Chambers, N Elias-Rosa, H Flewelling, C Fremling, J Harmanen, M Huber, A Jerkstrand, T Kangas, H Kuncarayakti, M Magee, E Magnier, J Polshaw, KW Smith, J Sollerman, L Tomasella
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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 Oxford University Press 454:1 (2015) 419-438

Authors:

Manda Banerji, Richard G McMahon, Chris J Willott, James E Geach, Chris M Harrison, Susannah Alaghband-Zadeh, David Alexander, Nathan Bourne, Kristen EK Coppin, James S Dunlop, Duncan Farrah, Matthew Jarvis, Michal J Michalowski, Matthew Page, Daniel Smith, Mark Swinbank, Myrto Symeonidis, PPVD Werf, Paul P Van der Werf

Abstract:

We study the 850um emission in X-ray selected AGN in the 2 sq-deg COSMOS field using new data from the SCUBA-2 Cosmology Legacy Survey. We find 19 850um bright X-ray AGN in a high-sensitivity region covering 0.89 sq-deg with flux densities of S850=4-10 mJy. The 19 AGN span the full range in redshift and hard X-ray luminosity covered by the sample - 0.71 X-ray AGN - S850=0.71+/-0.08mJy. We explore trends in the stacked 850um flux densities with redshift, finding no evolution in the average cold dust emission over the redshift range probed. For Type 1 AGN, there is no significant correlation between the stacked 850um flux and hard X-ray luminosity. However, in Type 2 AGN the stacked submm flux is a factor of 2 higher at high luminosities. When averaging over all X-ray luminosities, no significant differences are found in the stacked submm fluxes of Type 1 and Type 2 AGN as well as AGN separated on the basis of X-ray hardness ratios and optical-to-infrared colours. However, at log10(LX) >44.4, dependences in average submm flux on the optical-to-infrared colours become more pronounced. We argue that these high luminosity AGN represent a transition from a secular to a merger-driven evolutionary phase where the star formation rates and accretion luminosities are more tightly coupled. Stacked AGN 850um fluxes are compared to the stacked fluxes of a mass-matched sample of K-band selected non-AGN galaxies. We find that at 10.5
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