Search Publications

Temporal Gain Correction for X-ray Calorimeter Spectrometers
DOI: 10.1007/s10909-016-1503-2 Bibcode: 2016JLTP..184..498P

Tsujimoto, M.; Ishisaki, Y.; Yamada, S. +14 more

Calorimetric X-ray detectors are very sensitive to their environment. The boundary conditions can have a profound effect on the gain including heat sink temperature, the local radiation temperature, bias, and the temperature of the readout electronics. Any variation in the boundary conditions can cause temporal variations in the gain of the detect…

2016 Journal of Low Temperature Physics
Hitomi 23
Ne X X-ray emission due to charge exchange in M82
DOI: 10.1093/mnras/stw527 Bibcode: 2016MNRAS.458.3554C

Liu, L.; Cumbee, R. S.; Lyons, D. +4 more

Recent X-ray observations of star-forming galaxies such as M82 have shown the Ly β/Ly α line ratio of Ne X to be in excess of predictions for thermal electron impact excitation. Here, we demonstrate that the observed line ratio may be due to charge exchange and can be used to constrain the ion kinetic energy to be ≲ 500 eV/u. This is accomplished …

2016 Monthly Notices of the Royal Astronomical Society
Suzaku 23
SAPS onset timing during substorms and the westward traveling surge
DOI: 10.1002/2016GL069693 Bibcode: 2016GeoRL..43.6687M

Mishin, Evgeny, V.

We present multispacecraft observations in the magnetosphere and conjugate ionosphere of the onset time of subauroral polarization streams (SAPS) and tens of keV ring current injections on the duskside in three individual substorms. This is probably the first unequivocal determination of the substorm SAPS onset timing. The time lag between the SAP…

2016 Geophysical Research Letters
Cluster 23
X-ray/UV variability and the origin of soft X-ray excess emission from II Zw 177
DOI: 10.1093/mnras/stw009 Bibcode: 2016MNRAS.457..875P

Dewangan, Gulab C.; Pal, Main; Misra, Ranjeev +1 more

We study X-ray and UV emission from the narrow-line Seyfert 1 galaxy II Zw 177 using a 137 ks long and another 13 ks short XMM-Newton observation performed in 2012 and 2001, respectively. Both observations show soft X-ray excess emission contributing 76.9 ± 4.9 per cent in 2012 and 58.8 ± 10.2 per cent in 2001 in the 0.3-2 keV band. We find that b…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 23
Evidence for a 36 ks phase modulation in the hard X-ray pulses from the magnetar 1E 1547.0-5408
DOI: 10.1093/pasj/psv097 Bibcode: 2016PASJ...68S..12M

Enoto, Teruaki; Makishima, Kazuo; Nakazawa, Kazuhiro +4 more

The Suzaku data for the highly variable magnetar 1E 1547.0-5408, obtained during the 2009 January activity, were reanalyzed. The 2.07 s pulsation, detected in the 15-40 keV HXD data, was found to exhibit phase modulation, which can be modeled by a sinusoid with a period of 36.0^{+4.5}_{-2.5}ks and an amplitude of 0.52 ± 0.14 s. While the effect is…

2016 Publications of the Astronomical Society of Japan
Suzaku 23
Hydrological and sedimentary analyses of well-preserved paleofluvial-paleolacustrine systems at Moa Valles, Mars
DOI: 10.1002/2015JE004891 Bibcode: 2016JGRE..121..194S

Hauber, Ernst; Di Achille, Gaetano; Ori, Gian Gabriele +2 more

Moa Valles is a well-preserved, likely Amazonian (younger than 2 Ga old), paleodrainage system that is nearly 300 km long and carved into ancient highland terrains west of Idaeus Fossae. The fluvial system apparently originated from fluidized ejecta blankets, and it consists of a series of dam breach paleolakes with associated fan-shaped sedimenta…

2016 Journal of Geophysical Research (Planets)
MEx 23
Where are all of the nebulae ionized by supersoft X-ray sources?
DOI: 10.1093/mnras/stv2423 Bibcode: 2016MNRAS.455.1770W

Gilfanov, M.; Woods, T. E.

Accreting, steadily nuclear-burning white dwarfs are associated with so-called close-binary supersoft X-ray sources (SSSs), observed to have temperatures of a few × 105 K and luminosities on the order of 1038 erg s-1. These and other types of SSSs are expected to be capable of ionizing their surrounding circumstell…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 23
Turbulence-generated Proton-scale Structures in the Terrestrial Magnetosheath
DOI: 10.3847/2041-8205/819/1/L15 Bibcode: 2016ApJ...819L..15V

Echim, Marius M.; Consolini, Giuseppe; Vörös, Zoltán +2 more

Recent results of numerical magnetohydrodynamic simulations suggest that in collisionless space plasmas, turbulence can spontaneously generate thin current sheets. These coherent structures can partially explain the intermittency and the non-homogenous distribution of localized plasma heating in turbulence. In this Letter, Cluster multi-point obse…

2016 The Astrophysical Journal
Cluster 23
Globular Clusters, Ultracompact Dwarfs, and Dwarf Galaxies in Abell 2744 at a Redshift of 0.308
DOI: 10.3847/0004-637X/831/1/108 Bibcode: 2016ApJ...831..108L

Lee, Myung Gyoon; Jang, In Sung

We report a photometric study of globular clusters (GCs), ultracompact dwarfs (UCDs), and dwarf galaxies in the giant merging galaxy cluster Abell 2744 at z = 0.308. Color-magnitude diagrams of the point sources derived from deep F814W (rest frame r‧) and F105W (rest frame I) images of Abell 2744 in the Hubble Space Telescope Frontier Field show a…

2016 The Astrophysical Journal
eHST 23
Insights into the location and dynamics of the coolest X-ray emitting gas in clusters of galaxies
DOI: 10.1093/mnras/stw1444 Bibcode: 2016MNRAS.461.2077P

Zhang, Y. -Y.; Finoguenov, A.; de Plaa, J. +10 more

We extend our previous study of the cool gas responsible for the emission of O VII X-ray lines in the cores of clusters and groups of galaxies. This is the coolest X-ray emitting phase and connects the 10 000 K H α emitting gas to the million degree phase, providing a useful tool to understand cooling in these objects. We study the location of the…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 23