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Delayed triggering of radio active galactic nuclei in gas-rich minor mergers in the local Universe

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 464:4 (2017) 4706-4720

Authors:

SS Shabala, A Deller, S Kaviraj, E Middelberg, RJ Turner, YS Ting, JR Allison, TA Davis
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Early observations of the nearby type Ia supernova SN 2015F

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 464:4 (2017) stw2678

Authors:

R Cartier, M Sullivan, R Firth, G Pignata, P Mazzali, K Maguire, MJ Childress, I Arcavi, C Ashall, B Bassett, SM Crawford, C Frohmaier, L Galbany, A Gal-Yam, G Hosseinzadeh, DA Howell, C Inserra, J Johansson, EK Kasai, C McCully, S Prajs, S Prentice, S Schulze, SJ Smartt, KW Smith, M Smith, S Valenti, DR Young
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VizieR Online Data Catalog: R-band light curves of HE 0435-1223 (Bonvin+, 2017)

VizieR Online Data Catalog (2017) J/MNRAS/465/4914-J/MNRAS/465/4914

Authors:

V Bonvin, F Courbin, SH Suyu, PJ Marshall, CE Rusu, D Sluse, M Tewes, KC Wong, T Collett, CD Fassnacht, T Treu, MW Auger, S Hilbert, LVE Koopmans, G Meylan, N Rumbaugh, A Sonnenfeld, C Spiniello

Hi absorption in nearby compact radio galaxies

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) (2017) stx214-stx214

Authors:

M Glowacki, JR Allison, EM Sadler, VA Moss, SJ Curran, A Musaeva, C Deng, R Parry, MC Sligo
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GMRT 610-MHz observations of the faint radio source population – and what these tell us about the higher radio-frequency sky

Monthly Notices of the Royal Astronomical Society Oxford University Press 464:3 (2017) 3357-3368

Authors:

IH Whittam, DA Green, Matthew Jarvis, JM Riley

Abstract:

We present 610-MHz Giant Metrewave Radio Telescope observations of 0.84 deg2 of the AMI001 field (centred on 00h23m10s, +31°53΄) with an rms noise of 18 μJy beam−1 in the centre of the field. A total of 955 sources are detected, and 814 are included in the source count analysis. The source counts from these observations are consistent with previous work. We have used these data to study the spectral index distribution of a sample of sources selected at 15.7 GHz from the recent deep extension to the Tenth Cambridge (10C) survey. The median spectral index, α, (where S ∝ ν−α) between 0.08
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