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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
A robust measurement of the mass outflow rate of the galactic outflow from NGC 6090
DOI: 10.1093/mnras/stw1951 Bibcode: 2016MNRAS.463..541C

Chisholm, John; Leitherer, Claus; Tremonti Christy, A. +1 more

To evaluate the impact of stellar feedback, it is critical to estimate the mass outflow rates of galaxies. Past estimates have been plagued by uncertain assumptions about the outflow geometry, metallicity, and ionization fraction. Here we use Hubble Space Telescope ultraviolet spectroscopic observations of the nearby starburst NGC 6090 to demonstr…

2016 Monthly Notices of the Royal Astronomical Society
eHST 56
Catalog of equatorial coordinates and B-magnitudes of stars of the FON project
DOI: 10.3103/S0884591316050032 Bibcode: 2016KPCB...32..260A

Andruk, V. M.; Pakuliak, L. K.; Golovnia, V. V. +4 more

The catalog of equatorial coordinates α and δ and B-magnitudes of stars of the northern sky (from–4° to +90°) was created as a part of the FON project at the Main Astronomical Observatory of the National Academy of Sciences of Ukraine. The data accumulated in the Joint Digital Archive of the Ukrainian Virtual Observatory were used. The total numbe…

2016 Kinematics and Physics of Celestial Bodies
Hipparcos 56
Determining Ages of APOGEE Giants with Known Distances
DOI: 10.3847/0004-637X/817/1/40 Bibcode: 2016ApJ...817...40F

Bovy, Jo; Majewski, Steven R.; Feuillet, Diane K. +4 more

We present a sample of 705 local giant stars observed using the New Mexico State University 1 m telescope with the Sloan Digital Sky Survey-III/Apache Point Observatory Galactic Evolution Experiment (APOGEE) spectrograph, for which we estimate stellar ages and the local star formation history (SFH). The high-resolution (R ∼ 22,500), near infrared …

2016 The Astrophysical Journal
Hipparcos 56
Tracing extended low-velocity shocks through SiO emission. Case study of the W43-MM1 ridge
DOI: 10.1051/0004-6361/201629077 Bibcode: 2016A&A...595A.122L

Hill, T.; Schneider, N.; Maury, A. +8 more


Aims: Previous literature suggests that the densest structures in the interstellar medium form through colliding flows, but patent evidence of this process is still missing. Recent literature proposes using SiO line emission to trace low-velocity shocks associated with cloud formation through collision. In this paper we investigate the bright…

2016 Astronomy and Astrophysics
Herschel 56