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The XXL Survey. VII. A supercluster of galaxies at z = 0.43
DOI: 10.1051/0004-6361/201527142 Bibcode: 2016A&A...592A...6P

Altieri, B.; Valtchanov, I.; Smolčić, V. +15 more

Context. The XXL Survey is the largest homogeneous and contiguous survey carried out with XMM-Newton. Covering an area of 50 deg2 distributed over two fields, it primarily investigates the large-scale structures of the Universe using the distribution of galaxy clusters and active galactic nuclei as tracers of the matter distribution.

2016 Astronomy and Astrophysics
XMM-Newton 19
Saturn's northern auroras as observed using the Hubble Space Telescope
DOI: 10.1016/j.icarus.2015.09.008 Bibcode: 2016Icar..263...17N

Badman, S. V.; Nichols, J. D.; Clarke, J. T. +4 more

We discuss the features of Saturn's northern FUV auroras as observed during a program of Hubble Space Telescope observations which executed over 2011-2013 and culminated, along with Cassini observations, in a comprehensive multi-spectral observing campaign. Our 2011-2013 observations of the northern aurora are also compared with those from our 200…

2016 Icarus
eHST 19
Submillimeter array observations of NGC 2264-C: molecular outflows and driving sources
DOI: 10.1093/mnras/stw359 Bibcode: 2016MNRAS.458.1742C

Lumsden, Stuart L.; Cunningham, Nichol; Cyganowski, Claudia J. +2 more

We present 1.3 mm Submillimeter Array (SMA) observations at ∼3 arcsec resolution towards the brightest section of the intermediate/massive star-forming cluster NGC 2264-C. The millimetre continuum emission reveals ten 1.3 mm continuum peaks, of which four are new detections. The observed frequency range includes the known molecular jet/outflow tra…

2016 Monthly Notices of the Royal Astronomical Society
Herschel 19
Mid-infrared imaging- and spectro-polarimetric subarcsecond observations of NGC 1068
DOI: 10.1093/mnras/stw541 Bibcode: 2016MNRAS.458.3851L

Esquej, P.; Telesco, C. M.; Díaz-Santos, T. +10 more

We present subarcsecond 7.5-13 µm imaging- and spectro-polarimetric observations of NGC 1068 using CanariCam on the 10.4-m Gran Telescopio CANARIAS. At all wavelengths, we find: (1) A 90 × 60 pc extended polarized feature in the northern ionization cone, with a uniform ∼44° polarization angle. Its polarization arises from dust and gas emissi…

2016 Monthly Notices of the Royal Astronomical Society
eHST 19
The Effect of Unresolved Binaries on Globular Cluster Proper-motion Dispersion Profiles
DOI: 10.3847/2041-8205/820/1/L22 Bibcode: 2016ApJ...820L..22B

Anderson, J.; Schinnerer, E.; van der Marel, R. P. +5 more

High-precision kinematic studies of globular clusters (GCs) require an accurate knowledge of all possible sources of contamination. Among other sources, binary stars can introduce systematic biases in the kinematics. Using a set of Monte Carlo cluster simulations with different concentrations and binary fractions, we investigate the effect of unre…

2016 The Astrophysical Journal
eHST 19
Observations of high and low Fe charge states in individual solar wind streams with coronal-hole origin
DOI: 10.1051/0004-6361/201527998 Bibcode: 2016A&A...593A..70H

Berger, Lars; Heidrich-Meisner, Verena; Wimmer-Schweingruber, Robert +2 more

Context. The solar wind originating from coronal holes is comparatively well-understood and is characterized by lower densities and average charge states compared to the so-called slow solar wind. Except for wave perturbations, the average properties of the coronal-hole solar wind are passably constant.
Aims: In this case study, we focus on o…

2016 Astronomy and Astrophysics
SOHO 19
Deep GeMS/GSAOI near-infrared observations of N159W in the Large Magellanic Cloud
DOI: 10.1051/0004-6361/201628754 Bibcode: 2016A&A...592A..77B

Zavagno, A.; Neichel, B.; Samal, M. R. +5 more


Aims: The formation and properties of star clusters at the edge of H II regions are poorly known, partly due to limitations in angular resolution and sensitivity, which become particularly critical when dealing with extragalactic clusters. In this paper we study the stellar content and star-formation processes in the young N159W region in the…

2016 Astronomy and Astrophysics
eHST 19
Comparative study of water ice exposures on cometary nuclei using multispectral imaging data
DOI: 10.1093/mnras/stw2918 Bibcode: 2016MNRAS.462S.394O

Jorda, L.; Lamy, P. L.; Lara, L. M. +48 more

Deep Impact, EPOXI and Rosetta missions visited comets 9P/Tempel 1, 103P/Hartley 2 and 67P/Churyumov-Gerasimenko, respectively. Each of these three missions was equipped with both multispectral imagers and infrared spectrometers. Bright blue features containing water ice were detected in each of these comet nuclei. We analysed multispectral proper…

2016 Monthly Notices of the Royal Astronomical Society
Rosetta 19
Diffuse low-ionization gas in the galactic halo casts doubts on z ≃ 0.03 WHIM detections
DOI: 10.1093/mnrasl/slw022 Bibcode: 2016MNRAS.458L.123N

Piro, L.; Elvis, M.; Nicastro, F. +4 more

In this Letter, we demonstrate that the two claims of z ≃ 0.03 O VII K α absorption lines from Warm Hot Intergalactic Medium (WHIM) along the lines of sight to the blazars H 2356-309 (Buote et al.; Fang et al.) and Mkn 501 (Ren, Fang & Buote) are likely misidentifications of the z = 0 O II K β line produced by a diffuse Low-Ionization Metal Me…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 19
Dark sectors of the Universe: A Euclid survey approach
DOI: 10.1103/PhysRevD.94.123515 Bibcode: 2016PhRvD..94l3515T

Tutusaus, Isaac; Lamine, Brahim; Blanchard, Alain +3 more

In this paper we study the consequences of relaxing the hypothesis of the pressureless nature of the dark matter component when determining constraints on dark energy. To this aim we consider simple generalized dark matter models with constant equation of state parameter. We find that present-day low-redshift probes (type-Ia supernovae and baryoni…

2016 Physical Review D
Planck 19