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Planck intermediate results. XLIV. Structure of the Galactic magnetic field from dust polarization maps of the southern Galactic cap
DOI: 10.1051/0004-6361/201628636 Bibcode: 2016A&A...596A.105P

Miville-Deschênes, M. -A.; Boulanger, F.; Bernard, J. -P. +165 more

Using data from the Planck satellite, we study the statistical properties of interstellar dust polarization at high Galactic latitudes around the south pole (b < -60°). Our aim is to advance the understanding of the magnetized interstellar medium (ISM), and to provide a modelling framework of the polarized dust foreground for use in cosmic micr…

2016 Astronomy and Astrophysics
Planck 63
Cosmological constraints on decoupled dark photons and dark Higgs
DOI: 10.1088/1475-7516/2016/11/032 Bibcode: 2016JCAP...11..032B

Berger, Joshua; Jedamzik, Karsten; Walker, Devin G. E.

Any neutral boson such as a dark photon or dark Higgs that is part of a non-standard sector of particles can mix with its standard model counterpart. When very weakly mixed with the Standard Model, these particles are produced in the early Universe via the freeze-in mechanism and subsequently decay back to standard model particles. In this work, w…

2016 Journal of Cosmology and Astroparticle Physics
Planck 63
Dark matter component decaying after recombination: Lensing constraints with Planck data
DOI: 10.1103/PhysRevD.94.023528 Bibcode: 2016PhRvD..94b3528C

Chudaykin, A.; Gorbunov, D.; Tkachev, I.

It has been recently suggested [Z. Berezhiani, A. D. Dolgov, and I. I. Tkachev, Phys. Rev. D 92, 061303 (2015)] that emerging tension between cosmological parameter values derived in high-redshift (CMB anisotropy) and low-redshift (cluster counts, Hubble constant) measurements can be reconciled in a model which contains a subdominant fraction of d…

2016 Physical Review D
Planck 63
Dust attenuation in z ~ 1 galaxies from Herschel and 3D-HST Hα measurements
DOI: 10.1051/0004-6361/201526782 Bibcode: 2016A&A...586A..83P

Berta, S.; Lutz, D.; Cimatti, A. +12 more

We combined the spectroscopic information from the 3D-HST survey with Herschel data to characterize the Hα dust attenuation properties of a sample of 79 main sequence star-forming galaxies at z ~ 1 in the GOODS-S field. The sample was selected in the far-IR at λ = 100 and/or 160 µm and only includes galaxies with a secure Hα detection (S/N &…

2016 Astronomy and Astrophysics
Herschel eHST 63
Reconnection brightenings in the quiet solar photosphere
DOI: 10.1051/0004-6361/201628889 Bibcode: 2016A&A...592A.100R

Rouppe van der Voort, Luc H. M.; Rutten, Robert J.; Vissers, Gregal J. M.

We describe a new quiet-Sun phenomenon which we call quiet-Sun Ellerman-like brightenings (QSEB). QSEBs are similar to Ellerman bombs (EB) in some respects but differ significantly in others. EBs are transient brightenings of the wings of the Balmer Hα line that mark strong-field photospheric reconnection in complex active regions. QSEBs are simil…

2016 Astronomy and Astrophysics
IRIS 63
Gamma rays detected from Cygnus X-1 with likely jet origin
DOI: 10.1051/0004-6361/201628917 Bibcode: 2016A&A...596A..55Z

Aharonian, F.; Blanch, O.; de Oña Wilhelmi, E. +4 more


Aims: We probe the high-energy (>60 MeV) emission from the black hole X-ray binary system, Cygnus X-1, and investigate its origin.
Methods: We analyzed 7.5 yr of data by Fermi-LAT with the latest Pass 8 software version.
Results: We report the detection of a signal at 8σ statistical significance that is spatially coincident with …

2016 Astronomy and Astrophysics
INTEGRAL 63
The Evolution of the Fractions of Quiescent and Star-forming Galaxies as a Function of Stellar Mass Since z = 3: Increasing Importance of Massive, Dusty Star-forming Galaxies in the Early Universe
DOI: 10.3847/2041-8205/827/2/L25 Bibcode: 2016ApJ...827L..25M

van Dokkum, Pieter G.; Martis, Nicholas S.; Muzzin, Adam +7 more

Using the UltraVISTA DR1 and 3D-HST catalogs, we construct a stellar-mass-complete sample, unique for its combination of surveyed volume and depth, to study the evolution of the fractions of quiescent galaxies, moderately unobscured star-forming galaxies, and dusty star-forming galaxies as a function of stellar mass over the redshift interval 0.2 …

2016 The Astrophysical Journal
eHST 63
Sunset jets observed on comet 67P/Churyumov-Gerasimenko sustained by subsurface thermal lag
DOI: 10.1051/0004-6361/201527123 Bibcode: 2016A&A...586A...7S

Jorda, L.; Lamy, P. L.; Lara, L. M. +46 more

We present observations of sunset jets on comet 67P/Churyumov-Gerasimenko by Rosetta/OSIRIS camera. In late April 2015, when the comet was at a heliocentric distance of ~1.8 AU, clusters of dust jets that originated in the Ma'at region on the comet's small lobe were identified from multipleimages and were apparently sustained for about an hour bey…

2016 Astronomy and Astrophysics
Rosetta 63
Mass loading at 67P/Churyumov-Gerasimenko: A case study
DOI: 10.1002/2015GL067436 Bibcode: 2016GeoRL..43.1411B

Behar, E.; Nilsson, H.; Richter, I. +3 more

We study the dynamics of the interaction between the solar wind ions and a partially ionized atmosphere around a comet, at a distance of 2.88 AU from the Sun during a period of low nucleus activity. Comparing particle data and magnetic field data for a case study, we highlight the prime role of the solar wind electric field in the cometary ion dyn…

2016 Geophysical Research Letters
Rosetta 63
The Morphologies and Alignments of Gas, Mass, and the Central Galaxies of CLASH Clusters of Galaxies
DOI: 10.3847/0004-637X/819/1/36 Bibcode: 2016ApJ...819...36D

Donahue, Megan; Voit, G. Mark; Zitrin, Adi +10 more

Morphology is often used to infer the state of relaxation of galaxy clusters. The regularity, symmetry, and degree to which a cluster is centrally concentrated inform quantitative measures of cluster morphology. The Cluster Lensing and Supernova survey with Hubble Space Telescope (CLASH) used weak and strong lensing to measure the distribution of …

2016 The Astrophysical Journal
eHST 62