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A Comparison and Joint Analysis of Sunyaev-Zel’dovich Effect Measurements from Planck and Bolocam for a Set of 47 Massive Galaxy Clusters
DOI: 10.3847/0004-637X/832/1/26 Bibcode: 2016ApJ...832...26S

Pierpaoli, Elena; Merten, Julian; Sayers, Jack +7 more

We measure the Sunyaev-Zel’dovich (SZ) signal toward a set of 47 clusters with a median mass of 9.5 × 1014 M and a median redshift of 0.40 using data from Planck and the ground-based Bolocam receiver. When Planck XMM-like masses are used to set the scale radius {θ }{{s}}, we find consistency between the integrate…

2016 The Astrophysical Journal
Planck 38
Quantifying concordance in cosmology
DOI: 10.1103/PhysRevD.93.103507 Bibcode: 2016PhRvD..93j3507S

Amara, Adam; Refregier, Alexandre; Seehars, Sebastian +1 more

Quantifying the concordance between different cosmological experiments is important for testing the validity of theoretical models and systematics in the observations. In earlier work, we thus proposed the Surprise, a concordance measure derived from the relative entropy between posterior distributions. We revisit the properties of the Surprise an…

2016 Physical Review D
Planck 38
SPICAM observations and modeling of Mars aurorae
DOI: 10.1016/j.icarus.2015.09.023 Bibcode: 2016Icar..264..398S

Bertaux, Jean-Loup; Stiepen, Arnaud; Gérard, Jean-Claude +4 more

Martian aurorae have been detected with the SPICAM instrument on board Mars Express both in the nadir and the limb viewing modes. In this study, we focus on three limb observations to determine both the altitudes and the intensities of the auroral emissions. The CO (a3Π-X1Σ) Cameron bands between 190 and 270 nm, the CO (A

2016 Icarus
MEx 38
X-Ray and Optical Correlation of Type I Seyfert NGC 3516 Studied with Suzaku and Japanese Ground-based Telescopes
DOI: 10.3847/0004-637X/828/2/78 Bibcode: 2016ApJ...828...78N

Kawabata, Koji; Fukazawa, Yasushi; Makishima, Kazuo +23 more

From 2013 April to 2014 April, we performed X-ray and optical simultaneous monitoring of the type 1.5 Seyfert galaxy NGC 3516. We employed Suzaku and five Japanese ground-based telescopes—the Pirka, Kiso Schmidt, Nayuta, MITSuME, and the Kanata telescopes. The Suzaku observations were conducted seven times with various intervals ranging from days …

2016 The Astrophysical Journal
Suzaku 38
LASCO White-Light Observations of Eruptive Current Sheets Trailing CMEs
DOI: 10.1007/s11207-016-0988-9 Bibcode: 2016SoPh..291.3725W

Vourlidas, Angelos; Webb, David F.

Many models of eruptive flares or coronal mass ejections (CMEs) involve formation of a current sheet connecting the ejecting CME flux rope with a magnetic loop arcade. However, there is very limited observational information on the properties and evolution of these structures, hindering progress in understanding eruptive activity from the Sun. In …

2016 Solar Physics
SOHO 38
Rhea gravity field and interior modeling from Cassini data analysis
DOI: 10.1016/j.icarus.2015.09.022 Bibcode: 2016Icar..264..264T

Nimmo, Francis; Iess, Luciano; Jacobson, Robert A. +4 more

During its tour of the Saturn system, Cassini performed two close flybys of Rhea dedicated to gravity investigations, the first in November 2005 and the second in March 2013. This paper presents an estimation of Rhea's fully unconstrained quadrupole gravity field obtained from a joint multi-arc analysis of the two Cassini flybys.

Our best est…

2016 Icarus
Cassini 38
The JCMT and Herschel Gould Belt Surveys: a comparison of SCUBA-2 and Herschel data of dense cores in the Taurus dark cloud L1495
DOI: 10.1093/mnras/stw1978 Bibcode: 2016MNRAS.463.1008W

Hill, T.; Könyves, V.; Palmeirim, P. +27 more

We present a comparison of Submillimetre Common User Bolometer Array-2 (SCUBA-2) 850-µm and Herschel 70-500-µm observations of the L1495 filament in the Taurus Molecular Cloud with the goal of characterizing the SCUBA-2 Gould Belt Survey (GBS) data set. We identify and characterize starless cores in three data sets: SCUBA-2 850-µ…

2016 Monthly Notices of the Royal Astronomical Society
Herschel 38
Early science with the Large Millimetre Telescope: Deep LMT/AzTEC millimetre observations of ɛ Eridani and its surroundings
DOI: 10.1093/mnras/stw1363 Bibcode: 2016MNRAS.462.2285C

Dent, W. R. F.; Eiroa, C.; Marshall, J. P. +21 more

ɛ Eridani is a nearby, young Sun-like star that hosts a ring of cool debris analogous to the Solar system's Edgeworth-Kuiper belt. Early observations at (sub-)mm wavelengths gave tentative evidence of the presence of inhomogeneities in the ring, which have been ascribed to the effect of a putative low eccentricity planet, orbiting close to the rin…

2016 Monthly Notices of the Royal Astronomical Society
Herschel 38
Ancient eruptions of η Carinae: a tale written in proper motions
DOI: 10.1093/mnras/stw2019 Bibcode: 2016MNRAS.463..845K

Smith, Nathan; Reiter, Megan; Kiminki, Megan M.

We analyse eight epochs of Hubble Space Telescope Hα+[N II] imaging of η Carinae's outer ejecta. Proper motions of nearly 800 knots reveal that the detected ejecta are divided into three apparent age groups, dating to around 1250 A.D., to around 1550 A.D., and to during or shortly before the Great Eruption of the 1840s. Ejecta from these groups re…

2016 Monthly Notices of the Royal Astronomical Society
eHST 38
First NuSTAR Observations of the BL Lac-type Blazar PKS 2155-304: Constraints on the Jet Content and Distribution of Radiating Particles
DOI: 10.3847/0004-637X/831/2/142 Bibcode: 2016ApJ...831..142M

Harrison, F. A.; Hornstrup, A.; Hailey, C. +35 more

We report the first hard X-ray observations with NuSTAR of the BL Lac-type blazar PKS 2155-304, augmented with soft X-ray data from XMM-Newton and γ-ray data from the Fermi Large Area Telescope, obtained in 2013 April when the source was in a very low flux state. A joint NuSTAR and XMM spectrum, covering the energy range 0.5-60 keV, is best descri…

2016 The Astrophysical Journal
XMM-Newton 38