HYDROGEN-POOR SUPERLUMINOUS SUPERNOVAE AND LONG-DURATION GAMMA-RAY BURSTS HAVE SIMILAR HOST GALAXIES
The Astrophysical Journal American Astronomical Society 787:2 (2014) 138
THE TYPE IIP SUPERNOVA 2012aw IN M95: HYDRODYNAMICAL MODELING OF THE PHOTOSPHERIC PHASE FROM ACCURATE SPECTROPHOTOMETRIC MONITORING
The Astrophysical Journal American Astronomical Society 787:2 (2014) 139
Evolution in the bias of faint radio sources to z ∼ 2.2
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 440:3 (2014) 2322-2332
Probing the bright radio flare and afterglow of GRB 130427A with the Arcminute Microkelvin Imager
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 440:3 (2014) 2059-2065
THE SINS/zC-SINF SURVEY OF z ∼ 2 GALAXY KINEMATICS: EVIDENCE FOR POWERFUL ACTIVE GALACTIC NUCLEUS-DRIVEN NUCLEAR OUTFLOWS IN MASSIVE STAR-FORMING GALAXIES**Based on observations obtained at the Very Large Telescope of the European Southern Observatory, Paranal, Chile (ESO program IDs 074.A-0911, 075.A-0466, 076.A-0527, 078.A-0600, 082.A-0396, 183.A-0781, 088.A-0202, 091.A-0126). Also based on observations made with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5–26555; these observations are associated with GO programs Nos. 10924 and 12578.
The Astrophysical Journal American Astronomical Society 787:1 (2014) 38