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Planck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dust
DOI: 10.1051/0004-6361/201424082 Bibcode: 2015A&A...576A.104P

Kneissl, R.; Miville-Deschênes, M. -A.; Boulanger, F. +200 more

This paper presents an overview of the polarized sky as seen by Planck HFI at 353 GHz, which is the most sensitive Planck channel for dust polarization. We construct and analyse maps of dust polarization fraction and polarization angle at 1° resolution, taking into account noise bias and possible systematic effects. The sensitivity of the Planck H…

2015 Astronomy and Astrophysics
Planck 376
The Discovery of the First “Changing Look” Quasar: New Insights Into the Physics and Phenomenology of Active Galactic Nucleus
DOI: 10.1088/0004-637X/800/2/144 Bibcode: 2015ApJ...800..144L

Moran, Edward C.; Myers, Adam D.; Heckman, Timothy M. +6 more

SDSS J015957.64+003310.5 is an X-ray selected, z = 0.31 active galactic nucleus (AGN) from the Stripe 82X survey that transitioned from a Type 1 quasar to a Type 1.9 AGN between 2000 and 2010. This is the most distant AGN, and first quasar, yet observed to have undergone such a dramatic change. We re-observed the source with the double spectrograp…

2015 The Astrophysical Journal
XMM-Newton 371
The MOSDEF Survey: Measurements of Balmer Decrements and the Dust Attenuation Curve at Redshifts z ~ 1.4-2.6
DOI: 10.1088/0004-637X/806/2/259 Bibcode: 2015ApJ...806..259R

Siana, Brian; Shapley, Alice E.; Reddy, Naveen A. +7 more

We present results on the dust attenuation curve of z ∼ 2 galaxies using early observations from the MOSFIRE Deep Evolution Field survey. Our sample consists of 224 star-forming galaxies with zspec = 1.36-2.59 and high signal-to-noise ratio measurements of Hα and Hβ obtained with Keck/MOSFIRE. We construct composite spectral energy dist…

2015 The Astrophysical Journal
eHST 356
The Canadian Cluster Comparison Project: detailed study of systematics and updated weak lensing masses
DOI: 10.1093/mnras/stv275 Bibcode: 2015MNRAS.449..685H

Muzzin, Adam; Hoekstra, Henk; Babul, Arif +4 more

Masses of clusters of galaxies from weak gravitational lensing analyses of ever larger samples are increasingly used as the reference to which baryonic scaling relations are compared. In this paper we revisit the analysis of a sample of 50 clusters studied as part of the Canadian Cluster Comparison Project. We examine the key sources of systematic…

2015 Monthly Notices of the Royal Astronomical Society
Planck eHST 348
Ongoing hydrothermal activities within Enceladus
DOI: 10.1038/nature14262 Bibcode: 2015Natur.519..207H

Postberg, Frank; Altobelli, Nicolas; Sekine, Yasuhito +12 more

Detection of sodium-salt-rich ice grains emitted from the plume of the Saturnian moon Enceladus suggests that the grains formed as frozen droplets from a liquid water reservoir that is, or has been, in contact with rock. Gravitational field measurements suggest a regional south polar subsurface ocean of about 10 kilometres thickness located beneat…

2015 Nature
Cassini 338
Wind from the black-hole accretion disk driving a molecular outflow in an active galaxy
DOI: 10.1038/nature14261 Bibcode: 2015Natur.519..436T

Veilleux, S.; Reynolds, C. S.; Tombesi, F. +3 more

Powerful winds driven by active galactic nuclei are often thought to affect the evolution of both supermassive black holes and their host galaxies, quenching star formation and explaining the close relationship between black holes and galaxies. Recent observations of large-scale molecular outflows in ultraluminous infrared galaxies support this qu…

2015 Nature
Herschel 336
The evolution of the X-ray luminosity functions of unabsorbed and absorbed AGNs out to z∼ 5
DOI: 10.1093/mnras/stv1062 Bibcode: 2015MNRAS.451.1892A

Georgakakis, A.; Nandra, K.; Aird, J. +3 more

We present new measurements of the evolution of the X-ray luminosity functions (XLFs) of unabsorbed and absorbed active galactic nuclei (AGNs) out to z ∼ 5. We construct samples containing 2957 sources detected at hard (2-7 keV) X-ray energies and 4351 sources detected at soft (0.5-2 keV) energies from a compilation of Chandra surveys supplemented…

2015 Monthly Notices of the Royal Astronomical Society
eHST 336
The VIMOS Ultra-Deep Survey: ~10 000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2 < z ≃ 6
DOI: 10.1051/0004-6361/201423829 Bibcode: 2015A&A...576A..79L

Maccagni, D.; Cimatti, A.; Ilbert, O. +42 more

We present the VIMOS Ultra Deep Survey (VUDS), a spectroscopic redshift survey of ~10 000 very faint galaxies to study the main phase of galaxy assembly in 2 < z ≃ 6. The survey covers 1 deg2 in three separate fields: COSMOS, ECDFS, and VVDS-02h, with the selection of targets based on an inclusive combination of photometric redshifts…

2015 Astronomy and Astrophysics
eHST 324
A dusty, normal galaxy in the epoch of reionization
DOI: 10.1038/nature14164 Bibcode: 2015Natur.519..327W

Richard, Johan; Gallazzi, Anna; Christensen, Lise +3 more

Candidates for the modest galaxies that formed most of the stars in the early Universe, at redshifts z > 7, have been found in large numbers with extremely deep restframe-ultraviolet imaging. But it has proved difficult for existing spectrographs to characterize them using their ultraviolet light. The detailed properties of these galaxies could…

2015 Nature
eHST 321
On the nucleus structure and activity of comet 67P/Churyumov-Gerasimenko
DOI: 10.1126/science.aaa1044 Bibcode: 2015Sci...347a1044S

Bertaux, Jean-Loup; Da Deppo, Vania; Naletto, Giampiero +63 more

Images from the OSIRIS scientific imaging system onboard Rosetta show that the nucleus of 67P/Churyumov-Gerasimenko consists of two lobes connected by a short neck. The nucleus has a bulk density less than half that of water. Activity at a distance from the Sun of >3 astronomical units is predominantly from the neck, where jets have been seen c…

2015 Science
Rosetta 320