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Extreme flux states of NGC 4151 observed with INTEGRAL
DOI: 10.1111/j.1365-2966.2010.17251.x Bibcode: 2010MNRAS.408.1851L

Paltani, S.; Walter, R.; Ferrigno, C. +5 more

We present a comprehensive spectral analysis of all INTEGRAL data obtained so far for the X-ray-bright Seyfert galaxy NGC 4151. We also use all contemporaneous data from RXTE, XMM-Newton, Swift and Suzaku. We find a linear correlation between the medium- and hard-energy X-ray fluxes measured by INTEGRAL, which indicates an almost constant spectral…

2010 Monthly Notices of the Royal Astronomical Society
INTEGRAL Suzaku XMM-Newton 60
Hard X-ray properties of magnetic cataclysmic variables
DOI: 10.1111/j.1365-2966.2009.15826.x Bibcode: 2010MNRAS.401.2207S

Hill, A. B.; Knigge, C.; Bird, A. J. +10 more

Hard X-ray surveys have proven remarkably efficient in detecting intermediate polars and asynchronous polars, two of the rarest type of cataclysmic variable (CV). Here, we present a global study of hard X-ray-selected intermediate polars and asynchronous polars, focusing particularly on the link between hard X-ray properties and spin/orbital perio…

2010 Monthly Notices of the Royal Astronomical Society
INTEGRAL Suzaku 60
Deep high-resolution X-ray spectra from cool-core clusters
DOI: 10.1111/j.1365-2966.2009.15902.x Bibcode: 2010MNRAS.402..127S

Fabian, A. C.; Russell, H. R.; Sanders, J. S. +2 more

We examine deep XMM-Newton Reflection Grating Spectrometer (RGS) spectra from the cores of three X-ray bright cool-core galaxy clusters, Abell 262, Abell 3581 and HCG 62. Each of the RGS spectra shows FeXVII emission lines indicating the presence of gas around 0.5keV. There is no evidence for OVII emission which would imply gas at still cooler tem…

2010 Monthly Notices of the Royal Astronomical Society
XMM-Newton 58
Measures of star formation rates from infrared (Herschel) and UV (GALEX) emissions of galaxies in the HerMES fields
DOI: 10.1111/j.1745-3933.2010.00916.x Bibcode: 2010MNRAS.409L...1B

Altieri, B.; Aussel, H.; Elbaz, D. +75 more

The reliability of infrared (IR) and ultraviolet (UV) emissions to measure star formation rates (SFRs) in galaxies is investigated for a large sample of galaxies observed with the Spectral and Photometric Imaging Receiver (SPIRE) and the Photodetector Array Camera and Spectrometer (PACS) instruments on Herschel as part of the Herschel Multi-Tiered…

2010 Monthly Notices of the Royal Astronomical Society
Herschel 58
HerMES: SPIRE Science Demonstration Phase maps†‡
DOI: 10.1111/j.1365-2966.2010.17771.x Bibcode: 2010MNRAS.409...83L

Pérez-Fournon, I.; Franceschini, A.; Bock, J. +30 more

We describe the production and verification of sky maps of the five Spectral and Photometric Imaging Receiver (SPIRE) fields observed as part of the Herschel Multi-tiered Extragalactic Survey (HerMES) during the Science Demonstration Phase (SDP) of the Herschel mission. We have implemented an iterative map-making algorithm [The SPIRE-HerMES Iterat…

2010 Monthly Notices of the Royal Astronomical Society
Herschel 58
Herschel-SPIRE, far-infrared properties of millimetre-bright and -faint radio galaxies
DOI: 10.1111/j.1745-3933.2010.00956.x Bibcode: 2010MNRAS.409L..13C

Pérez-Fournon, I.; Rodighiero, G.; Ivison, R. J. +34 more

We present the first study of the far-infrared (FIR) properties of high-redshift, radio-selected ultraluminous infrared galaxies (ULIRGs) using deep observations obtained with the Spectral and Photometric Imaging Receiver (SPIRE) from the Herschel Multi-tiered Extragalactic Survey (HerMES). These galaxies span a large range of 850-µm fluxes …

2010 Monthly Notices of the Royal Astronomical Society
Herschel 57
Discovery of Compton-thick quasars in the Sloan Digital Sky Survey
DOI: 10.1111/j.1365-2966.2010.16275.x Bibcode: 2010MNRAS.404...48V

Pozzi, F.; Alexander, D. M.; Vignali, C. +1 more

We present new and archival Chandra snapshot (~10ks each) observations of 15 optically identified [from the Sloan Digital Sky Survey (SDSS)] Type 2 quasars at z = 0.40-0.73. When combined with existing X-ray data, this work provides complete X-ray coverage for all 25 radio-quiet Type 2 quasars with logL[OIII] > 9.28Lsolar

2010 Monthly Notices of the Royal Astronomical Society
XMM-Newton 56
The star-formation history of the Small Magellanic Cloud star cluster NGC 419
DOI: 10.1111/j.1365-2966.2010.16201.x Bibcode: 2010MNRAS.403.1156R

Girardi, Léo; Rubele, Stefano; Kerber, Leandro

The rich Small Magellanic Cloud (SMC) star cluster NGC 419 has recently been found to present both a broad main-sequence turn-off and a dual red clump of giants in the sharp colour-magnitude diagrams (CMDs) derived from the High-Resolution Channel of the Advanced Camera for Surveys onboard the Hubble Space Telescope. In this work, we apply to the …

2010 Monthly Notices of the Royal Astronomical Society
eHST 55
Probing evolutionary mechanisms in galaxy clusters: neutral atomic hydrogen in Abell1367
DOI: 10.1111/j.1365-2966.2009.16204.x Bibcode: 2010MNRAS.403.1175S

Hardcastle, M. J.; Croston, J. H.; Boselli, A. +6 more

We present Very Large Array HI imaging data for a field in the NW of the galaxy cluster Abell 1367 (z =0.02) in an attempt to probe the effect environment has on the interstellar medium of late-type spiral galaxies. Several galaxies, like CGCG 097-087, show pronounced tails and asymmetries, and seven out of 10 show significant, several kpc offsets…

2010 Monthly Notices of the Royal Astronomical Society
XMM-Newton 55
The linear rms-flux relation in an ultraluminous X-ray source
DOI: 10.1111/j.1745-3933.2010.00864.x Bibcode: 2010MNRAS.405L..86H

Vaughan, S.; Heil, L. M.

We report the first detection of a linear correlation between rms variability amplitude and flux in the ultraluminous X-ray source (ULX) NGC 5408 X-1. The rms-flux relation has previously been observed in several galactic black hole X-ray binaries (BHBs), several active galactic nuclei (AGN) and at least one neutron star X-ray binary. This result …

2010 Monthly Notices of the Royal Astronomical Society
XMM-Newton 54