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PRISM: Recovery of the primordial spectrum from Planck data
DOI: 10.1051/0004-6361/201424420 Bibcode: 2014A&A...571L...1L

Starck, J. -L.; Sureau, F.; Bobin, J. +3 more


Aims: The primordial power spectrum describes the initial perturbations that seeded the large-scale structure we observe today. It provides an indirect probe of inflation or other structure-formation mechanisms. In this Letter, we recover the primordial power spectrum from the Planck PR1 dataset, using our recently published algorithm PRISM. …

2014 Astronomy and Astrophysics
Planck 7
In situ observations of density cavities extending above the auroral acceleration region
DOI: 10.1002/2014JA019799 Bibcode: 2014JGRA..119.5286A

Karlsson, T.; Marklund, G. T.; Alm, L.

The uppermost part of a stable potential structure in the auroral acceleration region was studied using simultaneous observations of Cluster satellites C1 and C3. Both satellites observe a monotonically decreasing electron density as they ascend through the auroral acceleration region. As C1 exits the top of the auroral acceleration region, the el…

2014 Journal of Geophysical Research (Space Physics)
Cluster 7
Erratum: "Joint Analysis of Cluster Observations. II. Chandra/XMM-Newton X-Ray and Weak Lensing Scaling Relations for a Sample of 50 Rich Clusters of Galaxies" (2013, ApJ, 767, 116)
DOI: 10.1088/0004-637X/794/2/175 Bibcode: 2014ApJ...794..175M

Hoekstra, Henk; Babul, Arif; Mahdavi, Andisheh +3 more

2014 The Astrophysical Journal
XMM-Newton 7
Physical Nature of the [S II]-bright Shell Nebulae N70 and N185
DOI: 10.1088/0004-637X/792/1/58 Bibcode: 2014ApJ...792...58Z

Gruendl, R. A.; Chu, You-Hua; Chen, Yang +3 more

N70 and N185 are two large (>=100 pc in diameter) shell nebulae in the Large Magellanic Cloud (LMC). Their high [S II]/Hα ratios rival those of supernova remnants (SNRs), but they are not confirmed as SNRs. To study their physical nature, we have obtained XMM-Newton X-ray observations and high-dispersion long-slit echelle spectroscopic observat…

2014 The Astrophysical Journal
XMM-Newton 7
Evidence of transient reconnection in the outflow jet of primary reconnection site
DOI: 10.5194/angeo-32-239-2014 Bibcode: 2014AnGeo..32..239W

Fazakerley, A. N.; Nakamura, R.; Baumjohann, W. +4 more

The precise mechanism for the formation of magnetic islands in the magnetotail and the subsequent evolution are still controversial. New investigations have provided the first observational evidence of secondary reconnection in the earthward outflow jet of primary reconnection in the magnetotail. The secondary reconnection takes place 38 c/ωp…

2014 Annales Geophysicae
Cluster 7
A Full-Sun Magnetic Index from Helioseismology Inferences
DOI: 10.1007/s11207-013-0339-z Bibcode: 2014SoPh..289..503G

Hill, F.; Pérez Hernández, F.; Braun, D. C. +4 more

Solar magnetic indices are used to model the solar irradiance and ultimately to forecast it. However, the observation of such indices is generally limited to the Earth-facing hemisphere of the Sun. Seismic maps of the far side of the Sun have proven their capability to locate and track medium-large active regions at the non-visible hemisphere. We …

2014 Solar Physics
SOHO 7
Star-forming galactic contrails as a source of metal enrichment and ionizing radiation at high redshift
DOI: 10.1093/mnras/stu528 Bibcode: 2014MNRAS.441...73R

Rauch, Michael; Haehnelt, Martin G.; Becker, George D. +1 more

A spectroscopically detected Lyman α emitting halo at redshift 3.216 in the GOODS-N field is found to reside at the convergence of several line-emitting filaments. Spatially extended emission apparently by He II 1640 Å and several metal transitions is seen within several arcseconds from the position of the central galaxy. The V = 24.9 galaxy mainl…

2014 Monthly Notices of the Royal Astronomical Society
eHST 7
Comparison of interplanetary CME arrival times and solar wind parameters based on the WSA-ENLIL model with three cone types and observations
DOI: 10.1002/2014JA020339 Bibcode: 2014JGRA..119.7120J

Moon, Y. -J.; Jang, Soojeong; Na, Hyeonock +1 more

We have made a comparison between coronal mass ejection (CME)-associated shock propagations based on the Wang-Sheeley-Arge (WSA)-ENLIL model using three cone types and in situ observations. For this we use 28 full-halo CMEs, whose cone parameters are determined and their corresponding interplanetary shocks were observed at the Earth, from 2001 to …

2014 Journal of Geophysical Research (Space Physics)
SOHO 7
Cluster observations of fast magnetosonic waves in the heliosphere current sheet
DOI: 10.1002/2014GL059223 Bibcode: 2014GeoRL..41.1398D

Dai, Lei; Wygant, John R.; Cattell, Cynthia A. +4 more

We present Cluster spacecraft observations of large-amplitude (δ|B|/|B|∼1) fast-mode magnetosonic waves in the heliospheric current sheet (HCS). The crossings of the HCS and the associated heliospheric plasma sheet (HPS) are encountered by Cluster in the near-Earth solar wind and by ACE upstream of Earth. Multiple current layers are detected in co…

2014 Geophysical Research Letters
Cluster 7
Hubble Space Telescope imaging and spectroscopy of the sirius-like triple star system HD 217411
DOI: 10.1093/mnras/stu1431 Bibcode: 2014MNRAS.444.2022H

Bond, Howard E.; Barstow, M. A.; Holberg, J. B. +2 more

We present Hubble Space Telescope imaging and spectroscopy of HD 217411, a G3 V star associated with the extreme ultraviolet (UV) excess source (EUV 2RE J2300­­-07.0). This star is revealed to be a triple system with a G 3V primary (HD 217411 A) separated by ∼1.1 arcsec from a secondary that is in turn composed of an unresolved K0 V star (HD 21741…

2014 Monthly Notices of the Royal Astronomical Society
IUE eHST 7