Search Publications

Accounting for baryonic effects in cosmic shear tomography: determining a minimal set of nuisance parameters using PCA
DOI: 10.1093/mnras/stv2000 Bibcode: 2015MNRAS.454.2451E

Gnedin, Nickolay Y.; Eifler, Tim; Hearin, Andrew P. +3 more

Systematic uncertainties that have been subdominant in past large-scale structure (LSS) surveys are likely to exceed statistical uncertainties of current and future LSS data sets, potentially limiting the extraction of cosmological information. Here we present a general framework (Principal Component Analysis - PCA - marginalization) to consistent…

2015 Monthly Notices of the Royal Astronomical Society
Planck 112
The SINFONI Nearby Elliptical Lens Locator Survey: discovery of two new low-redshift strong lenses and implications for the initial mass function in giant early-type galaxies
DOI: 10.1093/mnras/stv518 Bibcode: 2015MNRAS.449.3441S

Conroy, Charlie; Lucey, John R.; Smith, Russell J.

We present results from a blind survey to identify strong gravitational lenses among the population of low-redshift early-type galaxies. The SINFONI Nearby Elliptical Lens Locator Survey (SNELLS) uses integral-field infrared spectroscopy to search for lensed emission line sources behind massive lens candidates at z < 0.055. From 27 galaxies obs…

2015 Monthly Notices of the Royal Astronomical Society
eHST 108
The XMM-Newton view of the central degrees of the Milky Way
DOI: 10.1093/mnras/stv1331 Bibcode: 2015MNRAS.453..172P

Haberl, F.; Nandra, K.; Ponti, G. +10 more

The deepest XMM-Newton mosaic map of the central 1.5 ° of the Galaxy is presented, including a total of about 1.5 Ms of EPIC-pn cleaned exposures in the central 15 arcsec and about 200 ks outside. This compendium presents broad-band X-ray continuum maps, soft X-ray intensity maps, a decomposition into spectral components and a comparison of the X-…

2015 Monthly Notices of the Royal Astronomical Society
XMM-Newton 107
The frequency and infrared brightness of circumstellar discs at white dwarfs
DOI: 10.1093/mnras/stv282 Bibcode: 2015MNRAS.449..574R

Gänsicke, B. T.; Rocchetto, M.; Farihi, J. +1 more

White dwarfs whose atmospheres are polluted by terrestrial-like planetary debris have become a powerful and unique tool to study evolved planetary systems. This paper presents results for an unbiased Spitzer Infrared Array Camera search for circumstellar dust orbiting a homogeneous and well-defined sample of 134 single white dwarfs. The stars were…

2015 Monthly Notices of the Royal Astronomical Society
eHST 105
ALMA and Herschel reveal that X-ray-selected AGN and main-sequence galaxies have different star formation rate distributions
DOI: 10.1093/mnrasl/slv110 Bibcode: 2015MNRAS.453L..83M

Daddi, E.; Elbaz, D.; Dickinson, M. +15 more

Using deep Herschel and ALMA observations, we investigate the star formation rate (SFR) distributions of X-ray-selected active galactic nucleus (AGN) host galaxies at 0.5 < z < 1.5 and 1.5 < z < 4, comparing them to that of normal, star-forming (i.e. `main-sequence', or MS) galaxies. We find that 34-55 per cent of AGNs in our sample ha…

2015 Monthly Notices of the Royal Astronomical Society
Herschel 105
A Suzaku search for dark matter emission lines in the X-ray brightest galaxy clusters
DOI: 10.1093/mnras/stv1142 Bibcode: 2015MNRAS.451.2447U

Simionescu, A.; Kaastra, J. S.; Allen, S. W. +3 more

We present the results of a search for unidentified emission lines in deep Suzaku X-ray spectra of the central regions of the X-ray brightest galaxy clusters: Perseus, Coma, Virgo and Ophiuchus. We analyse an optimized energy range (3.2-5.3 keV) that is relatively free of instrumental features, and a plasma emission model incorporating the abundan…

2015 Monthly Notices of the Royal Astronomical Society
Suzaku 104
Deconstructing the galaxy stellar mass function with UKIDSS and CANDELS: the impact of colour, structure and environment
DOI: 10.1093/mnras/stu2403 Bibcode: 2015MNRAS.447....2M

Fontana, Adriano; Grogin, Norman A.; Kocevski, Dale D. +15 more

We combine photometry from the Ultra Deep Survey (UDS), Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS) UDS and CANDELS the Great Observatories Origins Deep Survey-South (GOODS-S) surveys to construct the galaxy stellar mass function probing both the low- and high-mass end accurately in the redshift range 0.3 < z < 3…

2015 Monthly Notices of the Royal Astronomical Society
eHST 103
Diagnosing the accretion flow in ultraluminous X-ray sources using soft X-ray atomic features
DOI: 10.1093/mnras/stv2214 Bibcode: 2015MNRAS.454.3134M

Middleton, Matthew J.; Roberts, Timothy P.; Walton, Dominic J. +5 more

The lack of unambiguous detections of atomic features in the X-ray spectra of ultraluminous X-ray sources (ULXs) has proven a hindrance in diagnosing the nature of the accretion flow. The possible association of spectral residuals at soft energies with atomic features seen in absorption and/or emission and potentially broadened by velocity dispers…

2015 Monthly Notices of the Royal Astronomical Society
XMM-Newton 99
The powerful jet of an off-nuclear intermediate-mass black hole in the spiral galaxy NGC 2276
DOI: 10.1093/mnras/stv143 Bibcode: 2015MNRAS.448.1893M

Roberts, T. P.; Mezcua, M.; Sutton, A. D. +1 more

Jet ejection by accreting black holes is a mass invariant mechanism unifying stellar and supermassive black holes (SMBHs) that should also apply for intermediate-mass black holes (IMBHs), which are thought to be the seeds from which SMBHs form. We present the detection of an off-nuclear IMBH of ∼5 × 104 M located in an unusu…

2015 Monthly Notices of the Royal Astronomical Society
eHST 97
Properties of dark subhaloes from gaps in tidal streams
DOI: 10.1093/mnras/stv2122 Bibcode: 2015MNRAS.454.3542E

Erkal, Denis; Belokurov, Vasily

Cold or warm, the dark matter substructure spectrum must extend to objects with masses as low as 107 M, according to the most recent Lyman α measurements. Around a Milky Way-like galaxy, more than a thousand of these subhaloes will not be able to form stars but are dense enough to survive even deep down in the potential well…

2015 Monthly Notices of the Royal Astronomical Society
Gaia 97