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Planck intermediate results. L. Evidence of spatial variation of the polarized thermal dust spectral energy distribution and implications for CMB B-mode analysis
DOI: 10.1051/0004-6361/201629164 Bibcode: 2017A&A...599A..51P

Miville-Deschênes, M. -A.; Boulanger, F.; Bernard, J. -P. +156 more

The characterization of the Galactic foregrounds has been shown to be the main obstacle in thechallenging quest to detect primordial B-modes in the polarized microwave sky. We make use of the Planck-HFI 2015 data release at high frequencies to place new constraints on the properties of the polarized thermal dust emission at high Galactic latitudes…

2017 Astronomy and Astrophysics
Planck 58
X-Ray Counterpart of Gravitational Waves Due to Binary Neutron Star Mergers: Light Curves, Luminosity Function, and Event Rate Density
DOI: 10.3847/1538-4357/835/1/7 Bibcode: 2017ApJ...835....7S

Sun, Hui; Zhang, Bing; Gao, He

Zhang proposed a type of GRB-less X-ray transient associated with double neutron star (NS-NS) mergers under the conjecture of a rapidly spinning magnetar merger product with the line of sight off the short gamma-ray burst (GRB) jet. We investigate possible light curves of these transients by considering different observers’ viewing angles. We perf…

2017 The Astrophysical Journal
XMM-Newton 58
SAPS/SAID revisited: A causal relation to the substorm current wedge
DOI: 10.1002/2017JA024263 Bibcode: 2017JGRA..122.8516M

Mishin, Evgeny; Nishimura, Yukitoshi; Foster, John

We present multispacecraft observations of enhanced flow/electric field channels in the inner magnetosphere and conjugate subauroral ionosphere, i.e., subauroral polarization streams (SAPS) near dusk and subauroral ion drifts (SAID) near midnight. The channels collocate with ring current (RC) injections lagging the onset of substorms by a few to ∼…

2017 Journal of Geophysical Research (Space Physics)
Cluster 58
Stars caught in the braking stage in young Magellanic Cloud clusters
DOI: 10.1038/s41550-017-0186 Bibcode: 2017NatAs...1E.186D

D'Antona, Francesca; Milone, Antonino P.; Tailo, Marco +3 more

The colour-magnitude diagrams of many Magellanic Cloud clusters (with ages up to 2 billion years) display extended turnoff regions where the stars leave the main sequence, suggesting the presence of multiple stellar populations with ages that may differ even by hundreds of millions of years 1,2,3 . A strongly debated question is whether…

2017 Nature Astronomy
eHST 58
Forecasting the Impact of Stellar Activity on Transiting Exoplanet Spectra
DOI: 10.3847/1538-4357/aa79f5 Bibcode: 2017ApJ...844...27Z

Line, Michael R.; Zellem, Robert T.; Ciardi, David R. +8 more

Exoplanet host star activity, in the form of unocculted starspots or faculae, alters the observed transmission and emission spectra of the exoplanet. This effect can be exacerbated when combining data from different epochs if the stellar photosphere varies between observations due to activity. Here, we present a method to characterize and correct …

2017 The Astrophysical Journal
eHST 58
The two-component giant radio halo in the galaxy cluster Abell 2142
DOI: 10.1051/0004-6361/201630014 Bibcode: 2017A&A...603A.125V

Brunetti, G.; Rossetti, M.; Shimwell, T. W. +9 more


Aims: We report on a spectral study at radio frequencies of the giant radio halo in A 2142 (z = 0.0909), which we performed to explore its nature and origin. The optical and X-ray properties of the cluster suggest that A 2142 is not a major merger and the presence of a giant radio halo is somewhat surprising.
Methods: We performed deep r…

2017 Astronomy and Astrophysics
XMM-Newton 58
Variable Dynamics in the Inner Disk of HD 135344B Revealed with Multi-epoch Scattered Light Imaging
DOI: 10.3847/1538-4357/aa886a Bibcode: 2017ApJ...849..143S

Kraus, Stefan; Milli, Julien; Benisty, Myriam +12 more

We present multi-epoch Very Large Telescope/Spectro-Polarimetric High-contrast Exoplanet REsearch (VLT/SPHERE) observations of the protoplanetary disk around HD 135344B (SAO 206462). The J-band scattered light imagery reveal, with high spatial resolution (∼41 mas, 6.4 au), the disk surface beyond ∼20 au. Temporal variations are identified in the a…

2017 The Astrophysical Journal
Gaia 58
Suzaku observations of the merging galaxy cluster Abell 2255: The northeast radio relic
DOI: 10.1051/0004-6361/201628400 Bibcode: 2017A&A...600A.100A

Zhang, Y. -Y.; Kaastra, J. S.; Fukazawa, Y. +12 more

We present the results of deep 140 ks Suzaku X-ray observations of the north-east (NE) radio relic of the merging galaxy cluster Abell 2255. The temperature structure of Abell 2255 is measured out to 0.9 times the virial radius (1.9 Mpc) in the NE direction for the first time. The Suzaku temperature map of the central region suggests a complex tem…

2017 Astronomy and Astrophysics
Suzaku XMM-Newton 58
Intergalactic Lyman continuum photon budget in the past 5 billion years
DOI: 10.1093/mnras/stw3086 Bibcode: 2017MNRAS.466..838G

Khaire, Vikram; Srianand, Raghunathan; Choudhury, Tirthankar Roy +1 more

We constrain the H I photoionization rate (Γ _{H I}) at z ≲ 0.45 by comparing the flux probability distribution function and power spectrum of the Lyα forest data along 82 Quasi-Stellar Object (QSO) sightlines obtained using Cosmic Origins Spectrograph with models generated from smoothed particle hydrodynamic simulations. We have developed a modul…

2017 Monthly Notices of the Royal Astronomical Society
eHST 58
Swift observations of V404 Cyg during the 2015 outburst: X-ray outflows from super-Eddington accretion
DOI: 10.1093/mnras/stx1699 Bibcode: 2017MNRAS.471.1797M

Altamirano, D.; Sanna, A.; Knigge, C. +11 more

The black hole (BH) binary V404 Cyg entered the outburst phase in 2015 June after 26 yr of X-ray quiescence, and with its behaviour broke the outburst evolution pattern typical of most BH binaries. We observed the entire outburst with the Swift satellite and performed time-resolved spectroscopy of its most active phase, obtaining over a thousand s…

2017 Monthly Notices of the Royal Astronomical Society
INTEGRAL 58