Search Publications

Statistics of the field-aligned currents at the high-latitude energetic electron boundaries in the nightside: Cluster observation
DOI: 10.1002/2015JA021754 Bibcode: 2016JGRA..121.1979R

Fu, S. Y.; Zong, Q. G.; Zhang, Hui +4 more

Magnetic field disturbances with a clear bipolar signature are frequently observed when the Cluster spacecraft fleet passes through both southern and northern high-latitude energetic electron boundaries at the nightside magnetosphere. The dominant variation of the bipolar signature is in the azimuthal direction of the local mean field-aligned coor…

2016 Journal of Geophysical Research (Space Physics)
Cluster 4
Spectral Variations of the Sky: Constraints on Alternate Universes
DOI: 10.3847/0004-637X/817/1/33 Bibcode: 2016ApJ...817...33C

Chary, R.

The fine tuning of parameters required to reproduce our present day universe suggests that our universe may simply be a region within an eternally inflating super-region. Many other regions beyond our observable universe would exist with each such region governed by a different set of physical parameters. Collision between these regions, if they o…

2016 The Astrophysical Journal
Planck 4
Thin energetic O+ layer embedded in the magnetotail reconnection current sheet observed by Cluster
DOI: 10.1002/2016GL071184 Bibcode: 2016GeoRL..4311493W

Sun, W. J.; Fu, S. Y.; Zong, Q. G. +6 more

In the classical picture of the magnetotail current sheet, the current carriers are mainly ions that undergo nonadiabatic motions. Oxygen ions could contribute a thicker current sheet than the protons due to their large gyroradii. In this paper, however, we report a thin energetic O+ layer embedded in the magnetotail proton current shee…

2016 Geophysical Research Letters
Cluster 4
A spiral galaxy's mass distribution uncovered through lensing and dynamics
DOI: 10.1093/mnras/stw2142 Bibcode: 2016MNRAS.463.3151T

van de Ven, Glenn; Dutton, Aaron A.; Trick, Wilma H.

We investigate the matter distribution of a spiral galaxy with a counter-rotating stellar core, SDSS J1331+3628 (J1331), independently with gravitational lensing and stellar dynamical modelling. By fitting a gravitational potential model to a quadruplet of lensing images around J1331's bulge, we tightly constrain the mass inside the Einstein radiu…

2016 Monthly Notices of the Royal Astronomical Society
eHST 4
Origin of circular collapsed landforms in the Chryse region of Mars
DOI: 10.1016/j.icarus.2015.10.020 Bibcode: 2016Icar..265...70R

Kleinhans, Maarten G.; Zegers, Tanja E.; Roda, Manuel +1 more

The quasi-circular collapsed landforms occurring in the Chryse region of Mars share similar morphological characteristics, such as depth of collapse and polygonally fractured floors. Here, we present a statistical analysis of diameter, maximum and minimum depth, and amount of collapse of these features. Based on their morphometric characteristics,…

2016 Icarus
MEx 4
The variable V381 Lac and its possible connection with the R CrB phenomenon
DOI: 10.1093/mnras/stv2824 Bibcode: 2016MNRAS.456.2550R

Dell'Agli, F.; Nesci, R.; Rossi, C. +2 more

We have performed new medium resolution spectroscopy, optical and near-infrared photometry to monitor the variability of the asymptotic giant branch (AGB) carbon star V 381 Lac. Our observations revealed rapid and deep changes in the spectrum and extreme variability in the optical and near-infrared bands. Most notably we observed the change of Na …

2016 Monthly Notices of the Royal Astronomical Society
AKARI 4
Research Developments in Li-Paczyński Novae (II): Observational Aspect
DOI: 10.1016/j.chinastron.2016.10.007 Bibcode: 2016ChA&A..40..439W

Wang, Shan-qin; Dai, Zi-gao; Wu, Xue-feng

Since the LP-Nova models were proposed, and the short gamma-ray burst (SGRB) afterglows were confirmed, people have actively made searches for the evidence of the existence of LP-Novae among the optical (or near-infrared) counterparts of SGRBs. In this paper, we first summarize these observational progresses before 2012 in Section 2. In Section 3 …

2016 Chinese Astronomy and Astrophysics
eHST 4
Modeling the spectral response for the soft X-ray imager onboard the ASTRO-H satellite
DOI: 10.1016/j.nima.2016.03.071 Bibcode: 2016NIMPA.831..415I

Uchida, Hiroyuki; Hayashida, Kiyoshi; Nakajima, Hiroshi +20 more

The ASTRO-H satellite is the 6th Japanese X-ray astronomical observatory to be launched in early 2016. The satellite carries four kinds of detectors, and one of them is an X-ray CCD camera, the soft X-ray imager (SXI), installed on the focal plane of an X-ray telescope. The SXI contains four CCD chips, each with an imaging area of 31 mm × 31 mm , …

2016 Nuclear Instruments and Methods in Physics Research A
Hitomi 4
Variation in the Width of Transition Region Network Boundaries
DOI: 10.1007/s11207-016-0991-1 Bibcode: 2016SoPh..291.3519R

Raju, K. P.

The transition region network seen in solar extreme ultraviolet (EUV) lines is the extension of the chromospheric network. The network appears as an irregular web-like pattern over the solar surface outside active regions. The average width of transition region network boundaries is obtained from the two-dimensional autocorrelation function of SOl…

2016 Solar Physics
SOHO 4
Searching for the HR 8799 Debris Disk with HST/STIS
DOI: 10.3847/0004-637X/823/2/149 Bibcode: 2016ApJ...823..149G

Venn, K.; Matthews, B.; Lawler, S. +3 more

We present a new algorithm for space telescope high contrast imaging of close-to-face-on planetary disks called Optimized Spatially Filtered (OSFi) normalization. This algorithm is used on HR 8799 Hubble Space Telescope (HST) Space Telescope Imaging Spectrograph (STIS) coronagraphic archival data, showing an over-luminosity after reference star po…

2016 The Astrophysical Journal
eHST 4