Search Publications

KAT-7 observations of an unbiased sample of mass-selected galaxy clusters
DOI: 10.1093/mnras/stv2589 Bibcode: 2016MNRAS.456.1259B

Brunetti, G.; Venturi, T.; Dallacasa, D. +7 more

The presence of megaparsec-scale radio haloes in galaxy clusters has already been established by many observations over the last two decades. The emerging explanation for the formation of these giant sources of diffuse synchrotron radio emission is that they trace turbulent regions in the intracluster medium, where particles are trapped and accele…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 27
Long-Duration Gamma-Ray Burst Host Galaxies in Emission and Absorption
DOI: 10.1007/s11214-016-0237-4 Bibcode: 2016SSRv..202..111P

Fynbo, Johan P. U.; Perley, Daniel A.; Tanvir, Nial R. +2 more

The galaxy population hosting long-duration GRBs provides a means to constrain the progenitor and an opportunity to use these violent explosions to characterize the nature of the high-redshift universe. Studies of GRB host galaxies in emission reveal a population of star-forming galaxies with great diversity, spanning a wide range of masses, metal…

2016 Space Science Reviews
eHST 27
Unexpected spatial intensity distributions and onset timing of solar electron events observed by closely spaced STEREO spacecraft
DOI: 10.1051/0004-6361/201628734 Bibcode: 2016A&A...593A..31K

Gómez-Herrero, R.; Dresing, N.; Heber, B. +2 more

We present multi-spacecraft observations of four solar electron events using measurements from the Solar Electron Proton Telescope (SEPT) and the Electron Proton Helium INstrument (EPHIN) on board the STEREO and SOHO spacecraft, respectively, occurring between 11 October 2013 and 1 August 2014, during the approaching superior conjunction period of…

2016 Astronomy and Astrophysics
SOHO 27
HERUS: A CO Atlas from SPIRE Spectroscopy of Local ULIRGs
DOI: 10.3847/0067-0049/227/1/9 Bibcode: 2016ApJS..227....9P

Lebouteiller, Vianney; Cormier, Diane; Pearson, Chris +10 more

We present the Herschel SPIRE Fourier Transform Spectroscopy (FTS) atlas for a complete flux-limited sample of local ultraluminous infrared galaxies (ULIRGs) as part of the HERschel Ultra Luminous InfraRed Galaxy Survey (HERUS). The data reduction is described in detail and was optimized for faint FTS sources ,with particular care being taken for …

2016 The Astrophysical Journal Supplement Series
Herschel 27
Planck constraints on scalar-tensor cosmology and the variation of the gravitational constant
DOI: 10.1103/PhysRevD.93.122002 Bibcode: 2016PhRvD..93l2002O

Ichiki, Kiyotomo; Sugiyama, Naoshi; Ooba, Junpei +1 more

Cosmological constraints on the scalar-tensor theory of gravity by analyzing the angular power spectrum data of the cosmic microwave background (CMB) obtained from the Planck 2015 results are presented. We consider the harmonic attractor model, in which the scalar field has a harmonic potential with curvature (β ) in the Einstein frame and the the…

2016 Physical Review D
Planck 27
Deep Morphological and Spectral Study of the SNR RCW 86 with Fermi-LAT
DOI: 10.3847/0004-637X/819/2/98 Bibcode: 2016ApJ...819...98A

Troja, E.; Orlando, E.; Hill, A. B. +107 more

RCW 86 is a young supernova remnant (SNR) showing a shell-type structure at several wavelengths and is thought to be an efficient cosmic-ray (CR) accelerator. Earlier Fermi Large Area Telescope results reported the detection of γ-ray emission coincident with the position of RCW 86 but its origin (leptonic or hadronic) remained unclear due to the p…

2016 The Astrophysical Journal
XMM-Newton 27
Magnetic fields of opposite polarity in sunspot penumbrae
DOI: 10.1051/0004-6361/201628407 Bibcode: 2016A&A...596A...4F

Franz, M.; Schmidt, W.; Solanki, S. K. +25 more

Context. A significant part of the penumbral magnetic field returns below the surface in the very deep photosphere. For lines in the visible, a large portion of this return field can only be detected indirectly by studying its imprints on strongly asymmetric and three-lobed Stokes V profiles. Infrared lines probe a narrow layer in the very deep ph…

2016 Astronomy and Astrophysics
Hinode 27
Distance-dependent Offsets between Parallaxes for Nearby Stars and Gaia DR1 Parallaxes
DOI: 10.3847/2041-8205/832/1/L18 Bibcode: 2016ApJ...832L..18J

Gies, Douglas R.; Henry, Todd J.; Winters, Jennifer G. +3 more

We use 612 single stars with previously published trigonometric parallaxes placing them within 25 pc to evaluate parallaxes released in Gaia’s first data release (DR1). We find that the Gaia parallaxes are, on average, 0.24 ± 0.02 mas smaller than the weighted mean trigonometric parallax values for these stars in the solar neighborhood. We also fi…

2016 The Astrophysical Journal
Gaia 27
Applications for edge detection techniques using Chandra and XMM-Newton data: galaxy clusters and beyond
DOI: 10.1093/mnras/stw1367 Bibcode: 2016MNRAS.461..684W

Fabian, A. C.; Sanders, J. S.; Walker, S. A.

The unrivalled spatial resolution of the Chandra X-ray observatory has allowed many breakthroughs to be made in high-energy astrophysics. Here we explore applications of Gaussian gradient magnitude (GGM) filtering to X-ray data, which dramatically improves the clarity of surface brightness edges in X-ray observations, and maps gradients in X-ray s…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 27
Ion chemistry in the coma of comet 67P near perihelion
DOI: 10.1093/mnras/stw2149 Bibcode: 2016MNRAS.462S..67F

Gunell, H.; Wurz, P.; Altwegg, K. +33 more

The coma and the comet-solar wind interaction of comet 67P/Churyumov-Gerasimenko changed dramatically from the initial Rosetta spacecraft encounter in 2014 August through perihelion in 2015 August. Just before equinox (at 1.6 au from the Sun), the solar wind signal disappeared and two regions of different cometary ion characteristics were observed…

2016 Monthly Notices of the Royal Astronomical Society
Rosetta 27