Search Publications

The ATLAS3D project - V. The CO Tully-Fisher relation of early-type galaxies
DOI: 10.1111/j.1365-2966.2011.18284.x Bibcode: 2011MNRAS.414..968D

Krajnović, Davor; Emsellem, Eric; Sarzi, Marc +20 more

We demonstrate here using both single-dish and interferometric observations that CO molecules are an excellent kinematic tracer, even in high-mass galaxies, allowing us to investigate for the first time the CO Tully-Fisher relation (CO-TFR) of early-type galaxies. We compare the TFRs produced using both single-dish and interferometric data and var…

2011 Monthly Notices of the Royal Astronomical Society
eHST 66
Possible detection of two giant extrasolar planets orbiting the eclipsing polar UZ Fornacis
DOI: 10.1111/j.1365-2966.2011.19198.x Bibcode: 2011MNRAS.416.2202P

O'Donoghue, Darragh; Ramsay, Gavin; Buckley, David A. H. +11 more

We present new high-speed, multi-observatory, multi-instrument photometry of the eclipsing polar UZ For in order to measure precise mid-eclipse times with the aim of detecting any orbital period variations. When combined with published eclipse times and archival data spanning ∼27 years, we detect departures from a linear and quadratic trend of ∼60…

2011 Monthly Notices of the Royal Astronomical Society
XMM-Newton eHST 66
Further X-ray observations of EXO 0748-676 in quiescence: evidence for a cooling neutron star crust
DOI: 10.1111/j.1365-2966.2010.17562.x Bibcode: 2011MNRAS.412.1409D

Degenaar, N.; Wijnands, R.; Ray, P. S. +8 more

In late 2008, the quasi-persistent neutron star X-ray transient and eclipsing binary EXO 0748-676 started a transition from outburst to quiescence, after it actively accreted for more than 24 yr. In a previous work, we discussed Chandra and Swift observations obtained during the first 5 months of this transition. Here, we report on further X-ray o…

2011 Monthly Notices of the Royal Astronomical Society
XMM-Newton 65
The HST/ACS Coma Cluster Survey - III. Structural parameters of galaxies using single Sérsic fits
DOI: 10.1111/j.1365-2966.2010.17855.x Bibcode: 2011MNRAS.411.2439H

Ferguson, Henry C.; Balcells, Marc; Graham, Alister W. +14 more

We present a catalogue of structural parameters for 8814 galaxies in the 25 fields of the Hubble Space Telescope/ACS Coma Treasury Survey. Parameters from Sérsic fits to the two-dimensional surface brightness distributions are given for all galaxies from our published Coma photometric catalogue with mean effective surface brightness brighter than …

2011 Monthly Notices of the Royal Astronomical Society
eHST 64
Limits on the local dark matter density
DOI: 10.1111/j.1365-2966.2011.19206.x Bibcode: 2011MNRAS.416.2318G

Read, Justin I.; Garbari, Silvia; Lake, George

We revisit systematics in determining the local dark matter density ρdm from the vertical motion of stars in the solar neighbourhood. Using a simulation of a Milky Way like galaxy, we determine the data quality required to detect ρdm at its expected local value. We introduce a new method for recovering ρdm that use…

2011 Monthly Notices of the Royal Astronomical Society
Hipparcos 63
Investigating coronal saturation and supersaturation in fast-rotating M-dwarf stars
DOI: 10.1111/j.1365-2966.2010.17848.x Bibcode: 2011MNRAS.411.2099J

Briggs, K. R.; Jeffries, R. D.; Evans, P. A. +2 more

At fast rotation rates, the coronal activity of G- and K-type stars has been observed to 'saturate' and then decline again at even faster rotation rates - a phenomenon dubbed 'supersaturation'. In this paper, we investigate coronal activity in fast-rotating M-dwarfs using deep XMM-Newton observations of 97 low-mass stars of known rotation period i…

2011 Monthly Notices of the Royal Astronomical Society
XMM-Newton 63
A reflection origin for the soft and hard X-ray excess of Ark 120
DOI: 10.1111/j.1365-2966.2010.17518.x Bibcode: 2011MNRAS.410.1251N

Fabian, A. C.; Nardini, E.; Reis, R. C. +1 more

Over the last few years, several models have been proposed to interpret the widespread soft excess observed in the X-ray spectra of type 1 active galactic nuclei (AGN). In particular, reflection from the photoionized accretion disc blurred by relativistic effects has proven to be successful in reproducing both the spectral shape and the variabilit…

2011 Monthly Notices of the Royal Astronomical Society
Suzaku XMM-Newton 63
New star-forming galaxies at z≈ 7 from Wide Field Camera Three imaging
DOI: 10.1111/j.1365-2966.2010.17626.x Bibcode: 2011MNRAS.411...23W

Wilkins, Stephen M.; Bunker, Andrew J.; Caruana, Joseph +1 more

The addition of Wide Field Camera Three on the Hubble Space Telescope has led to a dramatic increase in our ability to study the z > 6 Universe. The improvement in the near-infrared (NIR) sensitivity of WFC3 over previous instruments has enabled us to reach apparent magnitudes approaching 29 (AB). This allows us to probe the rest-frame UV conti…

2011 Monthly Notices of the Royal Astronomical Society
eHST 63
A strong and broad Fe line in the XMM-Newton spectrum of the new X-ray transient and black hole candidate XTE J1652-453
DOI: 10.1111/j.1365-2966.2010.17661.x Bibcode: 2011MNRAS.411..137H

Done, Chris; Hiemstra, Beike; Méndez, Mariano +3 more

We observed the new X-ray transient and black hole candidate XTE J1652-453 simultaneously with XMM-Newton and the Rossi X-ray Timing Explorer (RXTE). The observation was done during the decay of the 2009 outburst, when XTE J1652-453 was in the hard-intermediate state. The spectrum shows a strong and broad Fe emission line with an equivalent width …

2011 Monthly Notices of the Royal Astronomical Society
XMM-Newton 63
PG 1211+143: probing high-frequency lags in a high-mass active galactic nucleus
DOI: 10.1111/j.1745-3933.2011.01129.x Bibcode: 2011MNRAS.417L..98D

Cappi, M.; Ponti, G.; Fabian, A. C. +4 more

We present the timing analysis of the four archived XMM-Newton observations of PG 1211+143. The source is well-known for its spectral complexity, comprising a strong soft excess and different absorption systems. Soft energy band (0.3-0.7 keV) lags are detected over all the four observations, in the frequency range ν≲ 6 × 10-4 Hz, where …

2011 Monthly Notices of the Royal Astronomical Society
XMM-Newton 62