Search Publications

Galaxy Candidates at z ~ 10 in Archival Data from the Brightest of Reionizing Galaxies (BORG[z8]) Survey
DOI: 10.3847/0004-637X/827/1/76 Bibcode: 2016ApJ...827...76B

Treu, T.; Mason, C. A.; Trenti, M. +9 more

The Wide Field Camera 3 (WFC3) on the Hubble Space Telescope (HST) enabled the search for the first galaxies observed at z ∼ 8-11 (500-700 Myr after the Big Bang). To continue quantifying the number density of the most luminous galaxies (M AB ∼ -22.0) at the earliest epoch observable with HST, we search for z ∼ 10 galaxies (F125W-drop…

2016 The Astrophysical Journal
eHST 28
A Hard X-Ray Study of the Normal Star-forming Galaxy M83 with NuSTAR
DOI: 10.3847/0004-637X/824/2/107 Bibcode: 2016ApJ...824..107Y

Argo, M. K.; Krivonos, R.; Wik, D. R. +19 more

We present the results from sensitive, multi-epoch NuSTAR observations of the late-type star-forming galaxy M83 (d = 4.6 Mpc). This is the first investigation to spatially resolve the hard (E\gt 10 keV) X-ray emission of this galaxy. The nuclear region and ∼20 off-nuclear point sources, including a previously discovered ultraluminous X-ray source,…

2016 The Astrophysical Journal
XMM-Newton 28
Helical Motions of Fine-structure Prominence Threads Observed by Hinode and IRIS
DOI: 10.3847/0004-637X/831/2/126 Bibcode: 2016ApJ...831..126O

Liu, Wei; Tsuneta, Saku; Okamoto, Takenori J.

Fine-structure dynamics in solar prominences holds critical clues to understanding their physical nature of significant space-weather implications. We report evidence of rotational motions of horizontal helical threads in two active-region prominences observed by the Hinode and/or Interface Region Imaging Spectrograph satellites at high resolution…

2016 The Astrophysical Journal
Hinode IRIS 28
Thermal Pressures in the Interstellar Medium of the Magellanic Clouds
DOI: 10.3847/0004-637X/821/2/118 Bibcode: 2016ApJ...821..118W

York, Donald G.; Lauroesch, James T.; Welty, Daniel E. +1 more

We discuss the thermal pressures (nHT) in predominantly cold, neutral interstellar gas in the Magellanic Clouds, derived from analyses of the fine-structure excitation of neutral carbon, as seen in high-resolution Hubble Space Telescope/Space Telescope Imaging Spectrograph spectra of seven diverse sight lines in the LMC and SMC. Detaile…

2016 The Astrophysical Journal
eHST 28
Kiloparsec Mass/Light Offsets in the Galaxy Pair-Lyα Emitter Lens System SDSS J1011+0143
DOI: 10.3847/0004-637X/820/1/43 Bibcode: 2016ApJ...820...43S

Brownstein, Joel R.; Dey, Arjun; Spinrad, Hyron +5 more

We report the discovery of significant mass/light offsets in the strong gravitational lensing system SDSS J1011+0143. We use the high-resolution Hubble Space Telescope (HST) F555W- and F814W-band imaging and Sloan Digital Sky Survey (SDSS) spectroscopy of this system, which consists of a close galaxy pair with a projected separation of ≈ 4.2 {{kpc…

2016 The Astrophysical Journal
eHST 27
Active Longitude and Solar Flare Occurrences
DOI: 10.3847/0004-637X/818/2/127 Bibcode: 2016ApJ...818..127G

Ludmány, A.; Baranyi, T.; Gyenge, N.

The aim of the present work is to specify the spatio-temporal characteristics of flare activity observed by the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) and the Geostationary Operational Environmental Satellite (GOES) in connection with the behavior of the longitudinal domain of enhanced sunspot activity known as active longit…

2016 The Astrophysical Journal
SOHO 27
The Effects of Kinetic Instabilities on Small-scale Turbulence in Earth’s Magnetosheath
DOI: 10.3847/0004-637X/829/1/54 Bibcode: 2016ApJ...829...54B

Vaivads, A.; Alexandrova, O.; Breuillard, H. +1 more

The Earth's magnetosheath is the region delimited by the bow shock and the magnetopause. It is characterized by highly turbulent fluctuations covering all scales from MHD down to kinetic scales. Turbulence is thought to play a fundamental role in key processes such as energy transport and dissipation in plasma. In addition to turbulence, different…

2016 The Astrophysical Journal
Cluster 27
Down-the-barrel and Transverse Observations of the Large Magellanic Cloud: Evidence for a Symmetric Galactic Wind on the Near and Far Sides of the Galaxy
DOI: 10.3847/0004-637X/817/2/91 Bibcode: 2016ApJ...817...91B

Lehner, N.; Howk, J. C.; Barger, K. A.

We compare the properties of gas flows on both the near and far side of the Large Magellanic Cloud (LMC) disk using Hubble Space Telescope UV absorption-line observations toward an active galactic nucleus behind (transverse) and a star within (down-the-barrel) the LMC disk at an impact parameter of 3.2 {kpc}. We find that even in this relatively q…

2016 The Astrophysical Journal
eHST 27
Deep Morphological and Spectral Study of the SNR RCW 86 with Fermi-LAT
DOI: 10.3847/0004-637X/819/2/98 Bibcode: 2016ApJ...819...98A

Troja, E.; Orlando, E.; Hill, A. B. +107 more

RCW 86 is a young supernova remnant (SNR) showing a shell-type structure at several wavelengths and is thought to be an efficient cosmic-ray (CR) accelerator. Earlier Fermi Large Area Telescope results reported the detection of γ-ray emission coincident with the position of RCW 86 but its origin (leptonic or hadronic) remained unclear due to the p…

2016 The Astrophysical Journal
XMM-Newton 27
Distance-dependent Offsets between Parallaxes for Nearby Stars and Gaia DR1 Parallaxes
DOI: 10.3847/2041-8205/832/1/L18 Bibcode: 2016ApJ...832L..18J

Gies, Douglas R.; Henry, Todd J.; Winters, Jennifer G. +3 more

We use 612 single stars with previously published trigonometric parallaxes placing them within 25 pc to evaluate parallaxes released in Gaia’s first data release (DR1). We find that the Gaia parallaxes are, on average, 0.24 ± 0.02 mas smaller than the weighted mean trigonometric parallax values for these stars in the solar neighborhood. We also fi…

2016 The Astrophysical Journal
Gaia 27