Search Publications

Origin of the Galactic Diffuse X-Ray Emission: Iron K-shell Line Diagnostics
DOI: 10.3847/1538-4357/833/2/268 Bibcode: 2016ApJ...833..268N

Koyama, Katsuji; Nobukawa, Masayoshi; Uchiyama, Hideki +2 more

This paper reports detailed K-shell line profiles of iron (Fe) and nickel (Ni) of the Galactic Center X-ray Emission (GCXE), Galactic Bulge X-ray Emission (GBXE), Galactic Ridge X-ray Emission (GRXE), magnetic Cataclysmic Variables (mCVs), non-magnetic Cataclysmic Variables (non-mCVs), and coronally Active Binaries (ABs). For the study of the orig…

2016 The Astrophysical Journal
Suzaku 32
Propagation of small size magnetic holes in the magnetospheric plasma sheet
DOI: 10.1002/2016JA022741 Bibcode: 2016JGRA..121.5510Y

Zhang, H.; Hamrin, M.; Rème, H. +19 more

Magnetic holes (MHs), characteristic structures where the magnetic field magnitude decreases significantly, have been frequently observed in space plasmas. Particularly, small size magnetic holes (SSMHs) which the scale is less than or close to the proton gyroradius are recently detected in the magnetospheric plasma sheet. In this study of Cluster…

2016 Journal of Geophysical Research (Space Physics)
Cluster 31
UV to IR Luminosities and Dust Attenuation Determined from ~4000 K-selected Galaxies at 1 < z < 3 in the ZFOURGE Survey
DOI: 10.3847/2041-8205/818/2/L26 Bibcode: 2016ApJ...818L..26F

Papovich, Casey; Dickinson, Mark; Inami, Hanae +22 more

We build a set of composite galaxy spectral energy distributions (SEDs) by de-redshifting and scaling multi-wavelength photometry from galaxies in the ZFOURGE survey, covering the CDFS, COSMOS, and UDS fields. From a sample of ∼4000 Ks-band selected galaxies, we define 38 composite galaxy SEDs that yield continuous low-resolution spectr…

2016 The Astrophysical Journal
Herschel 31
The Roll-over of Heliospheric Neutral Hydrogen below 100 eV: Observations and Implications
DOI: 10.3847/0004-637X/821/2/107 Bibcode: 2016ApJ...821..107G

Wurz, P.; McComas, D. J.; Fuselier, S. A. +8 more

We present an improved analysis of the energy spectrum of energetic neutral hydrogen from the heliosheath observed with the IBEX-Lo sensor on the Interstellar Boundary EXplorer from the years 2009 to 2012. This analysis allows us to study the lowest energies between 10 and 100 eV although various background sources are more intense than the target…

2016 The Astrophysical Journal
VenusExpress 31
Leveraging 3D-HST Grism Redshifts to Quantify Photometric Redshift Performance
DOI: 10.3847/0004-637X/822/1/30 Bibcode: 2016ApJ...822...30B

Weiner, Benjamin J.; van Dokkum, Pieter G.; Franx, Marijn +10 more

We present a study of photometric redshift accuracy in the 3D-HST photometric catalogs, using 3D-HST grism redshifts to quantify and dissect trends in redshift accuracy for galaxies brighter than JH IR > 24 with an unprecedented and representative high-redshift galaxy sample. We find an average scatter of 0.0197 ± 0.0003(1 + z) in th…

2016 The Astrophysical Journal
eHST 31
Topographic measurements of slope streaks on Mars
DOI: 10.1016/j.icarus.2016.06.005 Bibcode: 2016Icar..278...52B

Head, James W.; Brusnikin, Eugene S.; Kreslavsky, Mikhail A. +4 more

Slope streaks are enigmatic, actively forming albedo features occurring on slopes in high-albedo, low-thermal-inertia, dust-rich equatorial regions on Mars. They are a specifically martian phenomenon with no direct analogs on the Earth. Their morphology suggests that the streaks are initiated at their upslope tips and propagate down to their termi…

2016 Icarus
MEx 31
A search for X-ray reprocessing echoes in the power spectral density functions of AGN
DOI: 10.1093/mnras/stw1359 Bibcode: 2016MNRAS.461.1642E

Papadakis, I. E.; Emmanoulopoulos, D.; Dovčiak, M. +3 more

We present the results of a detailed study of the X-ray power spectral density (PSD) functions of 12 X-ray bright AGN, using almost all the archival XMM-Newton data. The total net exposure of the EPIC-pn light curves is larger than 350 ks in all cases (and exceeds 1 Ms in the case of 1H 0707-497). In a physical scenario in which X-ray reflection o…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 31
Asteroseismic versus Gaia distances: A first comparison
DOI: 10.1051/0004-6361/201629799 Bibcode: 2016A&A...595L...3D

De Ridder, J.; Eyer, L.; Aerts, C. +1 more

Context. The Kepler space mission led to a large number of high-precision time series of solar-like oscillators. Using a Bayesian analysis that combines asteroseismic techniques and additional ground-based observations, the mass, radius, luminosity, and distance of these stars can be estimated with good precision. This has given a new impetus to t…

2016 Astronomy and Astrophysics
Gaia 31
Tracing p-mode Waves from the Photosphere to the Corona in Active Regions
DOI: 10.3847/2041-8205/830/1/L17 Bibcode: 2016ApJ...830L..17Z

Zhao, Junwei; Chen, Ruizhu; Felipe, Tobías +1 more

Atmosphere above sunspots is abundant with different types of waves. Among these waves are running penumbral waves in the chromosphere, quasi-periodic oscillations in the lower coronal loops, and recently reported running waves in sunspots’ photosphere, all of which were interpreted as magnetoacoustic waves by some authors. Are these waves in diff…

2016 The Astrophysical Journal
IRIS 31
Planck intermediate results. XLI. A map of lensing-induced B-modes
DOI: 10.1051/0004-6361/201527932 Bibcode: 2016A&A...596A.102P

Miville-Deschênes, M. -A.; Boulanger, F.; Bernard, J. -P. +178 more

The secondary cosmic microwave background (CMB) B-modes stem from the post-decoupling distortion of the polarization E-modes due to the gravitational lensing effect of large-scale structures. These lensing-induced B-modes constitute both a valuable probe of the dark matter distribution and an important contaminant for the extraction of the primary…

2016 Astronomy and Astrophysics
Planck 31