Search Publications

POLARBEAR constraints on cosmic birefringence and primordial magnetic fields
DOI: 10.1103/PhysRevD.92.123509 Bibcode: 2015PhRvD..92l3509A

Chapman, Scott; Sherwin, Blake D.; Errard, Josquin +84 more

We constrain anisotropic cosmic birefringence using four-point correlations of even-parity E -mode and odd-parity B -mode polarization in the cosmic microwave background measurements made by the POLARization of the Background Radiation (POLARBEAR) experiment in its first season of observations. We find that the anisotropic cosmic birefringence sig…

2015 Physical Review D
Planck 101
OSIRIS observations of meter-sized exposures of H2O ice at the surface of 67P/Churyumov-Gerasimenko and interpretation using laboratory experiments
DOI: 10.1051/0004-6361/201525977 Bibcode: 2015A&A...583A..25P

Jorda, L.; Lamy, P. L.; Bertaux, J. -L. +52 more

Since OSIRIS started acquiring high-resolution observations of the surface of the nucleus of comet 67P/Churyumov-Gerasimenko, over one hundred meter-sized bright spots have been identified in numerous types of geomorphologic regions, but mostly located in areas receiving low insolation. The bright spots are either clustered, in debris fields close…

2015 Astronomy and Astrophysics
Rosetta 100
Zooming In on the Progenitors of Superluminous Supernovae With the HST
DOI: 10.1088/0004-637X/804/2/90 Bibcode: 2015ApJ...804...90L

Berger, E.; Kirshner, R. P.; Rest, A. +25 more

We present Hubble Space Telescope (HST) rest-frame ultraviolet imaging of the host galaxies of 16 hydrogen-poor superluminous supernovae (SLSNe), including 11 events from the Pan-STARRS Medium Deep Survey. Taking advantage of the superb angular resolution of HST, we characterize the galaxies’ morphological properties, sizes, and star formation rat…

2015 The Astrophysical Journal
eHST 100
Effect of Enceladus's rapid synchronous spin on interpretation of Cassini gravity
DOI: 10.1002/2015GL063384 Bibcode: 2015GeoRL..42.2137M

McKinnon, William B.

Enceladus's degree 2 gravity, determined by Cassini, is nominally nonhydrostatic to 3σ (J2/C22 = 3.38-3.63, as opposed to 10/3). Iess et al. (2014) interpret this in terms of a hydrostatic interior (core) and isostatic (not hydrostatic) floating ice shell. Enceladus's rapid (1.37 d) synchronous spin and tide distorts its shap…

2015 Geophysical Research Letters
Cassini 100
Subsurface properties and early activity of comet 67P/Churyumov-Gerasimenko
DOI: 10.1126/science.aaa0709 Bibcode: 2015Sci...347a0709G

Hartogh, Paul; Lellouch, Emmanuel; Ip, Wing-Huen +21 more

Heat transport and ice sublimation in comets are interrelated processes reflecting properties acquired at the time of formation and during subsequent evolution. The Microwave Instrument on the Rosetta Orbiter (MIRO) acquired maps of the subsurface temperature of comet 67P/Churyumov-Gerasimenko, at 1.6 mm and 0.5 mm wavelengths, and spectra of wate…

2015 Science
Rosetta 99
Observations of discrete harmonics emerging from equatorial noise
DOI: 10.1038/ncomms8703 Bibcode: 2015NatCo...6.7703B

Dandouras, Iannis; Walker, Simon N.; Balikhin, Michael A. +7 more

A number of modes of oscillations of particles and fields can exist in space plasmas. Since the early 1970s, space missions have observed noise-like plasma waves near the geomagnetic equator known as `equatorial noise'. Several theories were suggested, but clear observational evidence supported by realistic modelling has not been provided. Here we…

2015 Nature Communications
Cluster 99
The Relation between Solar Eruption Topologies and Observed Flare Features. I. Flare Ribbons
DOI: 10.1088/0004-637X/810/2/96 Bibcode: 2015ApJ...810...96S

Pariat, E.; DeLuca, E. E.; McKillop, S. +5 more

In this paper we present a topological magnetic field investigation of seven two-ribbon flares in sigmoidal active regions observed with Hinode, STEREO, and Solar Dynamics Observatory. We first derive the 3D coronal magnetic field structure of all regions using marginally unstable 3D coronal magnetic field models created with the flux rope inserti…

2015 The Astrophysical Journal
Hinode 99
Diagnosing the accretion flow in ultraluminous X-ray sources using soft X-ray atomic features
DOI: 10.1093/mnras/stv2214 Bibcode: 2015MNRAS.454.3134M

Middleton, Matthew J.; Roberts, Timothy P.; Walton, Dominic J. +5 more

The lack of unambiguous detections of atomic features in the X-ray spectra of ultraluminous X-ray sources (ULXs) has proven a hindrance in diagnosing the nature of the accretion flow. The possible association of spectral residuals at soft energies with atomic features seen in absorption and/or emission and potentially broadened by velocity dispers…

2015 Monthly Notices of the Royal Astronomical Society
XMM-Newton 99
Beyond six parameters: Extending Λ CDM
DOI: 10.1103/PhysRevD.92.121302 Bibcode: 2015PhRvD..92l1302D

Di Valentino, Eleonora; Melchiorri, Alessandro; Silk, Joseph

Cosmological constraints are usually derived under the assumption of a six-parameter Λ CDM theoretical framework or simple one-parameter extensions. In this paper we present, for the first time, cosmological constraints in a significantly extended scenario, varying up to 12 cosmological parameters simultaneously, including the sum of neutrino mass…

2015 Physical Review D
Planck 98
On the role played by magnetic expansion factor in the prediction of solar wind speed
DOI: 10.1002/2014SW001144 Bibcode: 2015SpWea..13..154R

Riley, Pete; Linker, Jon A.; Arge, C. Nick

Over the last two decades, the Wang-Sheeley-Arge (WSA) model has evolved significantly. Beginning as a simple observed correlation between the expansion factor of coronal magnetic field lines and the measured speed of the solar wind at 1 AU (the Wang-Sheeley (WS) model), the WSA model now drives NOAA's first operational space weather model, provid…

2015 Space Weather
SOHO 98