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On the Metallicity and Origin of the Smith High-velocity Cloud
DOI: 10.3847/2041-8205/816/1/L11 Bibcode: 2016ApJ...816L..11F

Sembach, Kenneth R.; Lockman, Felix J.; Rahman, Mubdi +7 more

The Smith Cloud (SC) is a gaseous high-velocity cloud (HVC) in an advanced state of accretion, only 2.9 kpc below the Galactic plane and due to impact the disk in ≈27 Myr. It is unique among HVCs in having a known distance (12.4 ± 1.3 kpc) and a well-constrained 3D velocity (296 km s-1), but its origin has long remained a mystery. Here …

2016 The Astrophysical Journal
eHST 56
Optical Spectroscopic Observations of Gamma-Ray Blazar Candidates. VI. Further Observations from TNG, WHT, OAN, SOAR, and Magellan Telescopes
DOI: 10.3847/0004-6256/151/4/95 Bibcode: 2016AJ....151...95A

Smith, Howard A.; Masetti, N.; Jiménez-Bailón, E. +16 more

Blazars, one of the most extreme classes of active galaxies, constitute so far the largest known population of γ-ray sources, and their number is continuously growing in the Fermi catalogs. However, in the latest release of the Fermi catalog there is still a large fraction of sources that are classified as blazar candidates of uncertain type (BCUs…

2016 The Astronomical Journal
XMM-Newton 56
First Gaia Local Group Dynamics: Magellanic Clouds Proper Motion and Rotation
DOI: 10.3847/2041-8205/832/2/L23 Bibcode: 2016ApJ...832L..23V

van der Marel, Roeland P.; Sahlmann, Johannes

We use the Gaia data release 1 (DR1) to study the proper motion (PM) fields of the Large and Small Magellanic Clouds (LMC, SMC). This uses the Tycho-Gaia Astrometric Solution (TGAS) PMs for 29 Hipparcos stars in the LMC and 8 in the SMC. The LMC PM in the West and North directions is inferred to be ({µ }W,{µ }N) =…

2016 The Astrophysical Journal
Gaia eHST 56
The SCUBA-2 Cosmology Legacy Survey: galaxies in the deep 850 µm survey, and the star-forming `main sequence'
DOI: 10.1093/mnras/stw564 Bibcode: 2016MNRAS.458.4321K

Bowler, R. A. A.; McLure, R. J.; Dunlop, J. S. +14 more

We investigate the properties of the galaxies selected from the deepest 850-µm survey undertaken to date with (Submillimetre Common-User Bolometer Array 2) SCUBA-2 on the James Clerk Maxwell Telescope as part of the SCUBA-2 Cosmology Legacy Survey. A total of 106 sources (>5σ) were uncovered at 850 µm from an area of ≃150 arcmin

2016 Monthly Notices of the Royal Astronomical Society
Herschel eHST 56
Radio Disappearance of the Magnetar XTE J1810-197 and Continued X-ray Timing
DOI: 10.3847/0004-637X/820/2/110 Bibcode: 2016ApJ...820..110C

Camilo, F.; Ransom, S. M.; Johnston, S. +6 more

We report on timing, flux density, and polarimetric observations of the transient magnetar and 5.54 s radio pulsar XTE J1810-197 using the Green Bank, Nançay, and Parkes radio telescopes beginning in early 2006, until its sudden disappearance as a radio source in late 2008. Repeated observations through 2016 have not detected radio pulsations agai…

2016 The Astrophysical Journal
XMM-Newton 56
Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function
DOI: 10.1051/0004-6361/201629057 Bibcode: 2016A&A...593A..55V

Paolillo, M.; Middei, R.; Vagnetti, F. +2 more

Context. Most investigations of the X-ray variability of active galactic nuclei (AGN) have been concentrated on the detailed analyses of individual, nearby sources. A relatively small number of studies have treated the ensemble behaviour of the more general AGN population in wider regions of the luminosity-redshift plane.
Aims: We want to det…

2016 Astronomy and Astrophysics
XMM-Newton 56
Weak-lensing mass calibration of the Atacama Cosmology Telescope equatorial Sunyaev-Zeldovich cluster sample with the Canada-France-Hawaii telescope stripe 82 survey
DOI: 10.1088/1475-7516/2016/08/013 Bibcode: 2016JCAP...08..013B

Bond, J. R.; Calabrese, E.; Huffenberger, K. M. +39 more

Mass calibration uncertainty is the largest systematic effect for using clusters of galaxies to constrain cosmological parameters. We present weak lensing mass measurements from the Canada-France-Hawaii Telescope Stripe 82 Survey for galaxy clusters selected through their high signal-to-noise thermal Sunyaev-Zeldovich (tSZ) signal measured with th…

2016 Journal of Cosmology and Astroparticle Physics
Planck 56
The inner magnetosphere ion composition and local time distribution over a solar cycle
DOI: 10.1002/2015JA021883 Bibcode: 2016JGRA..121.2009K

Kistler, L. M.; Mouikis, C. G.

Using the Cluster/Composition and Distribution Function (CODIF) analyzer data set from 2001 to 2013, a full solar cycle, we determine the ion distributions for H+, He+, and O+ in the inner magnetosphere (L < 12) over the energy range 40 eV to 40 keV as a function magnetic local time, solar EUV (F10.7)…

2016 Journal of Geophysical Research (Space Physics)
Cluster 56
Suzaku Observations of Moderately Obscured (Compton-thin) Active Galactic Nuclei Selected by Swift/BAT Hard X-ray Survey
DOI: 10.3847/0067-0049/225/1/14 Bibcode: 2016ApJS..225...14K

Ueda, Yoshihiro; Kawamuro, Taiki; Ricci, Claudio +2 more

We report the results obtained by a systematic, broadband (0.5-150 keV) X-ray spectral analysis of moderately obscured (Compton-thin, 22≤slant {log}{N}{{H}}< 24) active galactic nuclei (AGNs) observed with Suzaku and Swift/Burst Alert Telescope (BAT). Our sample consists of 45 local AGNs at z< 0.1 with {log}{L}14-195{keV

2016 The Astrophysical Journal Supplement Series
Suzaku 56
Dust particle flux and size distribution in the coma of 67P/Churyumov-Gerasimenko measured in situ by the COSIMA instrument on board Rosetta
DOI: 10.1051/0004-6361/201527958 Bibcode: 2016A&A...596A..87M

Altobelli, Nicolas; Langevin, Yves; Fischer, Henning +14 more

Context. The COmetary Secondary Ion Mass Analyzer (COSIMA) on board Rosetta is dedicated to the collection and compositional analysis of the dust particles in the coma of 67P/Churyumov-Gerasimenko (67P).
Aims: Investigation of the physical properties of the dust particles collected along the comet trajectory around the Sun starting at a helio…

2016 Astronomy and Astrophysics
Rosetta 56