Search Publications

The surface magnetic field and chemical abundance distributions of the B2V helium-strong star HD 184927
DOI: 10.1093/mnras/stu2401 Bibcode: 2015MNRAS.447.1418Y

Marcolino, W.; Kochukhov, O.; Bohlender, D. +8 more

A new time series of high-resolution Stokes I and V spectra of the magnetic B2V star HD 184927 has been obtained in the context of the Magnetism in Massive Stars Large Program with an Echelle SpectroPolarimetric Device for the Observation of Stars (ESPaDOnS) spectropolarimeter at the Canada-France-Hawaii Telescope and dimaPol liquid crystal spectr…

2015 Monthly Notices of the Royal Astronomical Society
IUE 31
C-Band All-Sky Survey: a first look at the Galaxy
DOI: 10.1093/mnras/stv212 Bibcode: 2015MNRAS.448.3572I

Davies, R. D.; Davis, R. J.; Dickinson, C. +18 more

We present an analysis of the diffuse emission at 5 GHz in the first quadrant of the Galactic plane using two months of preliminary intensity data taken with the C-Band All-Sky Survey (C-BASS) northern instrument at the Owens Valley Radio Observatory, California. Combining C-BASS maps with ancillary data to make temperature-temperature plots, we f…

2015 Monthly Notices of the Royal Astronomical Society
Planck 31
A search for variable and transient radio sources in the extended Chandra Deep Field South at 5.5 GHz
DOI: 10.1093/mnras/stv882 Bibcode: 2015MNRAS.450.4221B

Gaensler, B. M.; Bell, M. E.; Murphy, Tara +5 more

We present a three epoch survey for transient and variables in the extended Chandra Deep Field South at 5.5 GHz with the Australia Telescope Compact Array. A region covering ∼0.3 deg2 was observed on time-scales of 2.5 months and 2.5 yr and typical sensitivities 12.1-17.1 µJy beam-1 (1σ) were achieved. This survey repre…

2015 Monthly Notices of the Royal Astronomical Society
eHST 31
Dust energy balance study of two edge-on spiral galaxies in the Herschel-ATLAS survey
DOI: 10.1093/mnras/stv1104 Bibcode: 2015MNRAS.451.1728D

De Looze, Ilse; Baes, Maarten; Bendo, George J. +18 more

Interstellar dust in galaxies can be traced either through its extinction effects on the star light or through its thermal emission at infrared wavelengths. Recent radiative transfer studies of several nearby edge-on galaxies have found an apparent inconsistency in the dust energy balance: the radiative transfer models that successfully explain th…

2015 Monthly Notices of the Royal Astronomical Society
Herschel 30
X-ray time lags and non-linear variability in the ultraluminous X-ray sources NGC 5408 X-1 and NGC 6946 X-1
DOI: 10.1093/mnras/stv1830 Bibcode: 2015MNRAS.453.2877H

Vaughan, S.; Roberts, T. P.; Middleton, M. +1 more

We present our analysis of the X-ray variability of two ultraluminous X-ray sources (ULXs) based on multiple XMM-Newton observations. We show that the linear rms-flux relation is present in eight observations of NGC 5408 X-1 and also in three observations of NGC 6946 X-1, but data from other ULXs are generally not sufficient to constrain any rms-f…

2015 Monthly Notices of the Royal Astronomical Society
XMM-Newton 30
Characterizing extragalactic anomalous microwave emission in NGC 6946 with CARMA
DOI: 10.1093/mnras/stv287 Bibcode: 2015MNRAS.449..809H

Hensley, Brandon; Murphy, Eric; Staguhn, Johannes

Using 1 cm and 3 mm observations from the Combined Array for Research in Millimeter-wave Astronomy and 2 mm observations from the Goddard IRAM Superconducting 2 Millimeter Observer observations, we follow up the first extragalactic detection of anomalous microwave emission (AME) reported by Murphy et al. in an extranuclear region (Enuc. 4) of the …

2015 Monthly Notices of the Royal Astronomical Society
Planck 30
Dissecting galactic bulges in space and time - I. The importance of early formation scenarios versus secular evolution
DOI: 10.1093/mnras/stu2295 Bibcode: 2015MNRAS.446.2837S

Seidel, M. K.; Falcón-Barroso, J.; Vogt, F. P. A. +7 more

The details of bulge formation via collapse, mergers, secular processes or their interplay remain unresolved. To start answering this question and quantify the importance of distinct mechanisms, we mapped a sample of three galactic bulges using data from the integral field spectrograph WiFeS on the ANU's 2.3-m telescope in Siding Spring Observator…

2015 Monthly Notices of the Royal Astronomical Society
eHST 30
Observed trend in the star formation history and the dark matter fraction of galaxies at redshift z ≈ 0.8
DOI: 10.1093/mnras/stv1948 Bibcode: 2015MNRAS.454.1332S

Cappellari, Michele; Shetty, Shravan

We study the star formation history for a sample of 154 galaxies with stellar mass 10^{10}≲ M_{*} ≲ 10^{12} { M_{⊙}} in the redshift range 0.7 < z < 0.9. We do this using stellar population models combined with full-spectrum fitting of good quality spectra and high-resolution photometry. For a subset of 68 galaxies (M_{*}≳ 10^{11}{ M_{⊙}}) w…

2015 Monthly Notices of the Royal Astronomical Society
eHST 30
Multiband variability in the blazar 3C 273 with XMM-Newton
DOI: 10.1093/mnras/stv1027 Bibcode: 2015MNRAS.451.1356K

Bhagwan, Jai; Gupta, Alok C.; Wiita, Paul J. +2 more

We have undertaken a nearly simultaneous optical/UV and X-ray variability study of the flat spectrum radio quasar, 3C 273 using data available from the XMM-Newton satellite mission from 2000 June to 2012 July. Here, we focus on the multiwavelength flux variability on both intra-day and long time-scales of this very well known radio-loud source. We…

2015 Monthly Notices of the Royal Astronomical Society
XMM-Newton 30
Large-scale cosmic microwave background temperature and polarization cross-spectra likelihoods
DOI: 10.1093/mnras/stv1733 Bibcode: 2015MNRAS.453.3174M

Mangilli, A.; Plaszczynski, S.; Tristram, M.

We present a cross-spectra-based approach for the analysis of cosmic microwave background data at large angular scales to constrain the reionization optical depth τ, the tensor to scalar ratio r and the amplitude of the primordial scalar perturbations As. With respect to the pixel-based approach developed so far, using cross-spectra has…

2015 Monthly Notices of the Royal Astronomical Society
Planck 30