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FMOS near-IR spectroscopy of Herschel-selected galaxies: star formation rates, metallicity and dust attenuation at z ∼ 1
DOI: 10.1111/j.1365-2966.2012.21777.x Bibcode: 2012MNRAS.426.1782R

Clements, D. L.; Dunlop, J. S.; Buat, V. +36 more

We investigate the properties (e.g. star formation rate, dust attenuation, stellar mass and metallicity) of a sample of infrared (IR) luminous galaxies at z ∼ 1 via near-IR spectroscopy with Subaru-FMOS. Our sample consists of Herschel SPIRE and Spitzer MIPS selected sources in the COSMOS field with photometric redshifts in the range of 0.7 < z…

2012 Monthly Notices of the Royal Astronomical Society
Herschel eHST 35
Detecting the Warm-Hot Intergalactic Medium through X-Ray Absorption Lines
DOI: 10.1088/0004-637X/746/2/166 Bibcode: 2012ApJ...746..166Y

Shull, J. Michael; Wang, Q. Daniel; Yao, Yangsen +1 more

The warm-hot intergalactic medium (WHIM) at temperatures 105-107 K is believed to contain 30%-50% of the baryons in the local universe. However, all current X-ray detections of the WHIM at redshifts z > 0 are of low statistical significance (lsim 3σ) and/or controversial. In this work, we aim to establish the detection lim…

2012 The Astrophysical Journal
XMM-Newton 35
Far-ultraviolet Continuum Emission: Applying This Diagnostic to the Chromospheres of Solar-mass Stars
DOI: 10.1088/0004-637X/745/1/25 Bibcode: 2012ApJ...745...25L

France, Kevin; Linsky, Jeffrey L.; Ayres, Tom +2 more

The far-ultraviolet (FUV) continuum flux is recognized as a very sensitive diagnostic of the temperature structure of the Sun's lower chromosphere. Until now analysis of the available stellar FUV data has shown that solar-type stars must also have chromospheres, but quantitative analyses of stellar FUV continua require far higher quality spectra a…

2012 The Astrophysical Journal
eHST 35
Investigation of Intermittency in Magnetohydrodynamics and Solar Wind Turbulence: Scale-dependent Kurtosis
DOI: 10.1088/0004-637X/744/2/171 Bibcode: 2012ApJ...744..171W

Oughton, Sean; Matthaeus, William H.; Wan, Minping +1 more

The behavior of scale-dependent (or filtered) kurtosis is studied in the solar wind using magnetic field measurements from the ACE and Cluster spacecraft at 1 AU. It is also analyzed numerically with high-resolution magnetohydrodynamic spectral simulations. In each case the filtered kurtosis increases with wavenumber, implying the presence of cohe…

2012 The Astrophysical Journal
Cluster 35
SHARP - I. A high-resolution multiband view of the infrared Einstein ring of JVAS B1938+666
DOI: 10.1111/j.1365-2966.2012.21406.x Bibcode: 2012MNRAS.424.2800L

Vegetti, S.; McKean, J. P.; Auger, M. W. +3 more

We present new mass models for the gravitational lens system B1938+666, using multiwavelength data acquired from Keck adaptive optics (AO) and Hubble Space Telescope (HST) observations. These models are the first results from the Strong lensing at High Angular Resolution Program (SHARP), a project designed to study known quadruple image and Einste…

2012 Monthly Notices of the Royal Astronomical Society
eHST 35
Absorption Features in the X-ray Spectrum of an Ordinary Radio Pulsar
DOI: 10.1126/science.1221378 Bibcode: 2012Sci...337..946K

Pavlov, George G.; Kargaltsev, Oleg; Durant, Martin +1 more

The vast majority of known nonaccreting neutron stars (NSs) are rotation-powered radio and/or γ-ray pulsars. So far, their multiwavelength spectra have all been described satisfactorily by thermal and nonthermal continuum models, with no spectral lines. Spectral features have, however, been found in a handful of exotic NSs and were thought to be a…

2012 Science
XMM-Newton 35
Surface waves on Saturn's magnetopause
DOI: 10.1016/j.pss.2012.02.007 Bibcode: 2012P&SS...65..109M

Coates, A. J.; Dougherty, M. K.; Jones, G. H. +3 more

Waves on the surface of a planetary magnetopause promote energy transport into the magnetosphere, representing an important aspect of solar wind-magnetosphere coupling. At Saturn's magnetopause it has been proposed that growth of the Kelvin-Helmholtz (K-H) instability produces greater wave activity on the dawn side of the surface than on the dusk …

2012 Planetary and Space Science
Cassini 35
Ground-based observations of the long-term evolution and death of Saturn's 2010 Great White Spot
DOI: 10.1016/j.icarus.2012.05.033 Bibcode: 2012Icar..220..561S

Hueso, Ricardo; del Río-Gaztelurrutia, Teresa; Sánchez-Lavega, Agustín +8 more

We report on the long-term evolution of Saturn's sixth Great White Spot (GWS) event that initiated at northern mid-latitudes of the planet on December 5th, 2010 (Fletcher, L. et al. [2011]. Science 332, 1413-1417; Sánchez-Lavega, A. et al. [2011]. Nature 475, 71-74; Fischer, G. et al. [2011]. Nature 475, 75-77). We find from ground-based observati…

2012 Icarus
Cassini eHST 35
The Emission of Cygnus X-1: Observations with INTEGRAL SPI from 20 keV to 2 MeV
DOI: 10.1088/0004-637X/744/1/64 Bibcode: 2012ApJ...744...64J

Malzac, J.; Jourdain, E.; Roques, J. P.

We report on Cyg X-1 observations performed by the SPI telescope on board the INTEGRAL mission and distributed over more than 6 years. We investigate the variability of the intensity and spectral shape of this peculiar source in the hard X-ray domain, and more particularly up to the MeV region. We first study the total averaged spectrum which pres…

2012 The Astrophysical Journal
INTEGRAL 35
Suzaku Observations of 4U 1957+11: Potentially the Most Rapidly Spinning Black Hole in (the Halo of) the Galaxy
DOI: 10.1088/0004-637X/744/2/107 Bibcode: 2012ApJ...744..107N

Pottschmidt, Katja; Wilms, Jörn; Nowak, Michael A. +3 more

We present three Suzaku observations of the black hole candidate 4U 1957+11 (V1408 Aql)—a source that exhibits some of the simplest and cleanest examples of soft, disk-dominated spectra. 4U 1957+11 also presents among the highest peak temperatures found from disk-dominated spectra. Such temperatures may be associated with rapid black hole spin. Th…

2012 The Astrophysical Journal
Suzaku 35