Search Publications

Probing the intra-group medium of a z = 0.28 galaxy group
DOI: 10.1093/mnras/stx528 Bibcode: 2017MNRAS.468.1373B

Tejos, N.; Morris, S. L.; Cantalupo, S. +4 more

We present new MUSE observations of a galaxy group probed by a background quasar. The quasar sightline passes between multiple z = 0.28 galaxies, whilst showing at the same redshift low-ionized metal line species, including Ca II, Mg I, Mg II and Fe II. Based on the galaxy redshifts measured from the MUSE data, we estimate the galaxies to be part …

2017 Monthly Notices of the Royal Astronomical Society
eHST 55
Major mergers are not significant drivers of star formation or morphological transformation around the epoch of peak cosmic star formation
DOI: 10.1093/mnras/stw2895 Bibcode: 2017MNRAS.465.2895L

Conselice, C. J.; Hartley, W.; Mortlock, A. +2 more

We investigate the contribution of major mergers (mass ratios >1: 5) to stellar mass growth and morphological transformations around the epoch of peak cosmic star formation (z ∼ 2). We visually classify a complete sample of massive (M > 1010M) galaxies at this epoch, drawn from the Cosmic Assembly Near-infrared Deep Ex…

2017 Monthly Notices of the Royal Astronomical Society
eHST 55
VoIgt profile Parameter Estimation Routine (viper): H I photoionization rate at z < 0.5
DOI: 10.1093/mnras/stx248 Bibcode: 2017MNRAS.467.3172G

Khaire, Vikram; Srianand, Raghunathan; Choudhury, Tirthankar Roy +1 more

We have developed a parallel code called the VoIgt profile Parameter Estimation Routine (viper) for automatically fitting the H I Lyα forest seen in the spectra of quasi-stellar objects (QSOs). We obtained the H I column density distribution function (CDDF) and linewidth (b) parameter distribution for z < 0.45 using spectra of 82 QSOs obtained …

2017 Monthly Notices of the Royal Astronomical Society
eHST 55
On the progenitor of the Type IIb supernova 2016gkg
DOI: 10.1093/mnras/stw3082 Bibcode: 2017MNRAS.465.4650K

Treu, Tommaso; Kilpatrick, Charles D.; Foley, Ryan J. +7 more

We present a detection in pre-explosion Hubble Space Telescope (HST) imaging of a point source consistent with being the progenitor star of the Type IIb supernova (SN IIb) 2016gkg. Post-explosion imaging from the Keck adaptive optics system was used to perform relative astrometry between the Keck and HST imaging. We identify a single point source …

2017 Monthly Notices of the Royal Astronomical Society
eHST 54
Evidence that the AGN dominates the radio emission in z ∼ 1 radio-quiet quasars
DOI: 10.1093/mnras/stx284 Bibcode: 2017MNRAS.468..217W

Jarvis, Matt J.; Kalfountzou, Eleni; White, Sarah V. +4 more

In order to understand the role of radio-quiet quasars (RQQs) in galaxy evolution, we must determine the relative levels of accretion and star-formation activity within these objects. Previous work at low radio flux densities has shown that accretion makes a significant contribution to the total radio emission, in contrast with other quasar studie…

2017 Monthly Notices of the Royal Astronomical Society
Herschel 54
Diamagnetic region(s): structure of the unmagnetized plasma around Comet 67P/CG
DOI: 10.1093/mnras/stx1540 Bibcode: 2017MNRAS.469S.372H

Glassmeier, K. -H.; Nilsson, H.; Carr, C. +14 more

The ESA's comet chaser Rosetta has monitored the evolution of the ionized atmosphere of comet 67P/Churyumov-Gerasimenko (67P/CG) and its interaction with the solar wind, during more than 2 yr. Around perihelion, while the cometary outgassing rate was highest, Rosetta crossed hundreds of unmagnetized regions, but did not seem to have crossed a larg…

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 54
HICOSMO - cosmology with a complete sample of galaxy clusters - I. Data analysis, sample selection and luminosity-mass scaling relation
DOI: 10.1093/mnras/stx1022 Bibcode: 2017MNRAS.469.3738S

Reiprich, T. H.; Schellenberger, G.

The X-ray regime, where the most massive visible component of galaxy clusters, the intracluster medium, is visible, offers directly measured quantities, like the luminosity, and derived quantities, like the total mass, to characterize these objects. The aim of this project is to analyse a complete sample of galaxy clusters in detail and constrain …

2017 Monthly Notices of the Royal Astronomical Society
Planck 53
Evidence of sub-surface energy storage in comet 67P from the outburst of 2016 July 03
DOI: 10.1093/mnras/stx2386 Bibcode: 2017MNRAS.469S.606A

Langevin, Y.; Jorda, L.; Lamy, P. L. +67 more

On 2016 July 03, several instruments onboard ESA's Rosetta spacecraft detected signs of an outburst event on comet 67P, at a heliocentric distance of 3.32 au from the Sun, outbound from perihelion. We here report on the inferred properties of the ejected dust and the surface change at the site of the outburst. The activity coincided with the local…

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 53
Herschel -ATLAS: revealing dust build-up and decline across gas, dust and stellar mass selected samples - I. Scaling relations
DOI: 10.1093/mnras/stw2501 Bibcode: 2017MNRAS.464.4680D

Ivison, R. J.; Baes, M.; Baker, A. J. +19 more

We present a study of the dust, stars and atomic gas (H I) in an H I-selected sample of local galaxies (z < 0.035) in the Herschel Astrophysical Terahertz Large Area Survey fields. This H I-selected sample reveals a population of very high gas fraction (>80 per cent), low stellar mass sources that appear to be in the earliest stages of their…

2017 Monthly Notices of the Royal Astronomical Society
Herschel 53
Gaia16apd - a link between fast and slowly declining type I superluminous supernovae
DOI: 10.1093/mnras/stx833 Bibcode: 2017MNRAS.469.1246K

Lundqvist, P.; Wyrzykowski, Ł.; Kankare, E. +18 more

We present ultraviolet (UV), optical and infrared photometry and optical spectroscopy of the type Ic superluminous supernova (SLSN) Gaia16apd (=SN 2016eay), covering its evolution from 26 d before the g-band peak to 234.1 d after the peak. Gaia16apd was followed as a part of the NOT Unbiased Transient Survey (NUTS). It is one of the closest SLSNe …

2017 Monthly Notices of the Royal Astronomical Society
eHST 52