Search Publications

The nearby Type Ibn supernova 2015G: signatures of asymmetry and progenitor constraints
DOI: 10.1093/mnras/stx1885 Bibcode: 2017MNRAS.471.4381S

Van Dyk, Schuyler D.; Filippenko, Alexei V.; Wood-Vasey, W. Michael +24 more

We present the results of an extensive observational campaign on the nearby Type Ibn SN 2015G, including data from radio through ultraviolet wavelengths. SN 2015G was asymmetric, showing late-time nebular lines redshifted by ∼1000 km s-1. It shared many features with the prototypical SN Ibn 2006jc, including extremely strong He I emissi…

2017 Monthly Notices of the Royal Astronomical Society
eHST 36
Peculiar architectures for the WASP-53 and WASP-81 planet-hosting systems
DOI: 10.1093/mnras/stx154 Bibcode: 2017MNRAS.467.1714T

Smalley, Barry; Hellier, Coel; Triaud, Amaury H. M. J. +16 more

We report the detection of two new systems containing transiting planets. Both were identified by WASP as worthy transiting planet candidates. Radial velocity observations quickly verified that the photometric signals were indeed produced by two transiting hot Jupiters. Our observations also show the presence of additional Doppler signals. In addi…

2017 Monthly Notices of the Royal Astronomical Society
Gaia 36
A dichotomy between the hard state spectral properties of black hole and neutron star X-ray binaries
DOI: 10.1093/mnras/stw2514 Bibcode: 2017MNRAS.466..194B

Sunyaev, R.; Gilfanov, M.; Burke, M. J.

We analyse the spectra of black hole (BH) and neutron star (NS) X-ray binaries (XBs) in the hard state using archival RXTE observations. We find that there is a clear dichotomy in the strength of Comptonization between NS and BH sources, as measured by both the Compton y-parameter and the amplification factor A, with distinct groups of BH and NS X…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 35
Radio jets in NGC 4151: where eMERLIN meets HST
DOI: 10.1093/mnras/stx2205 Bibcode: 2017MNRAS.472.3842W

Muxlow, T. W. B.; Argo, M. K.; Knapen, J. H. +11 more

We present high-sensitivity eMERLIN radio images of the Seyfert galaxy NGC 4151 at 1.51 GHz. We compare the new eMERLIN images to those from archival MERLIN observations in 1993 to determine the change in jet morphology in the 22 yr between observations. We report an increase by almost a factor of 2 in the peak flux density of the central core com…

2017 Monthly Notices of the Royal Astronomical Society
eHST 35
H2 in low-ionization structures of planetary nebulae
DOI: 10.1093/mnras/stw2736 Bibcode: 2017MNRAS.465.1289A

Gonçalves, Denise R.; Akras, Stavros; Ramos-Larios, Gerardo

We report the detection of near-IR H2 emission from the low-ionization structures (knots) in two planetary nebulae. The deepest ever high-angular-resolution H2 (1-0) S(1) at 2.122 µm, H2 (2-1) S(1) at 2.248 µm and Brγ images of K 4-47 and NGC 7662, obtained using the Near InfraRed Imager and Spectromete…

2017 Monthly Notices of the Royal Astronomical Society
eHST 35
Seasonal changes of the volatile density in the coma and on the surface of comet 67P/Churyumov-Gerasimenko
DOI: 10.1093/mnras/stx866 Bibcode: 2017MNRAS.469S..20K

Altwegg, Kathrin; Rubin, Martin; Läuter, Matthias +1 more

Starting from several monthly data sets of Rosetta's COmetary Pressure Sensor, we reconstruct the gas density in the coma around comet 67P/Churyumov-Gerasimenko. The underlying inverse gas model is constructed by fitting ten thousands of measurements to thousands of potential gas sources distributed across the entire nucleus surface. The ensuing s…

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 35
On the redshift distribution and physical properties of ACT-selected DSFGs
DOI: 10.1093/mnras/stw2334 Bibcode: 2017MNRAS.464..968S

Frayer, D. T.; Bond, J. R.; Partridge, B. +25 more

We present multi-wavelength detections of nine candidate gravitationally lensed dusty star-forming galaxies (DSFGs) selected at 218 GHz (1.4 mm) from the Atacama Cosmology Telescope (ACT) equatorial survey. Among the brightest ACT sources, these represent the subset of the total ACT sample lying in Herschel SPIRE fields, and all nine of the 218 GH…

2017 Monthly Notices of the Royal Astronomical Society
Herschel 35
Epoch of reionization 21 cm forecasting from MCMC-constrained semi-numerical models
DOI: 10.1093/mnras/stx420 Bibcode: 2017MNRAS.468..122H

Davé, Romeel; Finlator, Kristian; Hassan, Sultan +1 more

The recent low value of Planck Collaboration XLVII integrated optical depth to Thomson scattering suggests that the reionization occurred fairly suddenly, disfavouring extended reionization scenarios. This will have a significant impact on the 21 cm power spectrum. Using a semi-numerical framework, we improve our model from instantaneous to includ…

2017 Monthly Notices of the Royal Astronomical Society
Planck 35
Searching for candidates of Lyman continuum sources - revisiting the SSA22 field
DOI: 10.1093/mnras/stw2700 Bibcode: 2017MNRAS.465..316M

Inoue, Akio K.; Yamada, Toru; Iwata, Ikuru +3 more

We present the largest to date sample of hydrogen Lyman continuum (LyC) emitting galaxy candidates at any redshift, with 18 Lyman α emitters (LAEs) and seven Lyman break galaxies (LBGs), obtained from the SSA22 field with Subaru/Suprime-Cam. The sample is based on the 159 LAEs and 136 LBGs observed in the field, all with spectroscopically confirme…

2017 Monthly Notices of the Royal Astronomical Society
eHST 35
Exploring the nature and synchronicity of early cluster formation in the Large Magellanic Cloud - II. Relative ages and distances for six ancient globular clusters
DOI: 10.1093/mnras/stx1702 Bibcode: 2017MNRAS.471.3347W

Cohen, Roger E.; Wagner-Kaiser, R.; Sarajedini, Ata +6 more

We analyse Hubble Space Telescope observations of six globular clusters in the Large Magellanic Cloud (LMC) from programme GO-14164 in Cycle 23. These are the deepest available observations of the LMC globular cluster population; their uniformity facilitates a precise comparison with globular clusters in the Milky Way. Measuring the magnitude of t…

2017 Monthly Notices of the Royal Astronomical Society
eHST 35