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Obscured AGN at z ~ 1 from the zCOSMOS-Bright Survey. I. Selection and optical properties of a [Ne v]-selected sample
DOI: 10.1051/0004-6361/201220846 Bibcode: 2013A&A...556A..29M

Kneib, J. -P.; Cimatti, A.; Silverman, J. D. +46 more


Aims: The application of multi-wavelength selection techniques is essential for obtaining a complete and unbiased census of active galactic nuclei (AGN). We present here a method for selecting z ~ 1 obscured AGN from optical spectroscopic surveys.
Methods: A sample of 94 narrow-line AGN with 0.65 < z < 1.20 was selected from the 20…

2013 Astronomy and Astrophysics
eHST 66
MAHLI at the Rocknest sand shadow: Science and science-enabling activities
DOI: 10.1002/2013JE004426 Bibcode: 2013JGRE..118.2338M

Kennedy, M. R.; Deen, R. G.; Schmidt, M. +29 more

Martian solar days 57-100, the Mars Science Laboratory Curiosity rover acquired and processed a solid (sediment) sample and analyzed its mineralogy and geochemistry with the Chemistry and Mineralogy and Sample Analysis at Mars instruments. An aeolian deposit—herein referred to as the Rocknest sand shadow—was inferred to represent a global average …

2013 Journal of Geophysical Research (Planets)
MEx 66
An observational study of the response of the upper atmosphere of Mars to lower atmospheric dust storms
DOI: 10.1016/j.icarus.2013.02.032 Bibcode: 2013Icar..225..378W

Withers, Paul; Pratt, R.

The effects of dust storms on densities, temperatures, and winds in the lower atmosphere of Mars are substantial. Here we use upper atmospheric observations to investigate how dust storms affect the upper atmosphere of Mars. We use aerobraking accelerometer, ultraviolet stellar occultation, and radio occultation datasets to examine the magnitudes …

2013 Icarus
MEx 65
Hemispheric Asymmetries of Solar Photospheric Magnetism: Radiative, Particulate, and Heliospheric Impacts
DOI: 10.1088/0004-637X/765/2/146 Bibcode: 2013ApJ...765..146M

Cirtain, Jonathan W.; McIntosh, Scott W.; Leamon, Robert J. +7 more

Among many other measurable quantities, the summer of 2009 saw a considerable low in the radiative output of the Sun that was temporally coincident with the largest cosmic-ray flux ever measured at 1 AU. Combining measurements and observations made by the Solar and Heliospheric Observatory (SOHO) and Solar Dynamics Observatory (SDO) spacecraft we …

2013 The Astrophysical Journal
SOHO 65
An Ab Initio Model for Cosmic-ray Modulation
DOI: 10.1088/0004-637X/772/1/46 Bibcode: 2013ApJ...772...46E

Burger, R. A.; Engelbrecht, N. E.

A proper understanding of the effects of turbulence on the diffusion and drift of cosmic rays (CRs) is of vital importance for a better understanding of CR modulation in the heliosphere. This study presents an ab initio model for CR modulation, incorporating for the first time the results yielded by a two-component turbulence transport model. This…

2013 The Astrophysical Journal
Ulysses 65
The Excitation of HCN and HCO+ in the Galactic Center Circumnuclear Disk
DOI: 10.1088/0004-637X/779/1/47 Bibcode: 2013ApJ...779...47M

Morris, M. R.; Mills, E. A. C.; Güsten, R. +1 more

We present new observations of HCN and HCO+ in the circumnuclear disk (CND) of the Galaxy, which we obtained with the Atacama Pathfinder Experiment telescope. We mapped emission in rotational lines of HCN J = 3-2, 4-3, and 8-7, as well as of HCO+ J = 3-2, 4-3, and 9-8. We also present spectra of H13CN J = 3-2 and 4…

2013 The Astrophysical Journal
ISO 65
Turbulent Dynamics in Solar Flare Sheet Structures Measured with Local Correlation Tracking
DOI: 10.1088/0004-637X/766/1/39 Bibcode: 2013ApJ...766...39M

McKenzie, D. E.

High-resolution observations of the Sun's corona in extreme ultraviolet and soft X-rays have revealed a new world of complexity in the sheet-like structures connecting coronal mass ejections (CMEs) to the post-eruption flare arcades. This article presents initial findings from an exploration of dynamic flows in two flares observed with Hinode/XRT …

2013 The Astrophysical Journal
Hinode 65
PS1-10afx at z = 1.388: Pan-STARRS1 Discovery of a New Type of Superluminous Supernova
DOI: 10.1088/0004-637X/767/2/162 Bibcode: 2013ApJ...767..162C

Price, P. A.; Berger, E.; Challis, P. +32 more

We present the Pan-STARRS1 discovery of PS1-10afx, a unique hydrogen-deficient superluminous supernova (SLSN) at redshift z = 1.388. The light curve peaked at z P1 = 21.7 mag, making PS1-10afx comparable to the most luminous known SNe, with Mu = -22.3 mag. Our extensive optical and near-infrared observations indicate that the…

2013 The Astrophysical Journal
eHST 65
Magnetic topologies of an in vivo FTE observed by Double Star/TC-1 at Earth's magnetopause
DOI: 10.1002/grl.50714 Bibcode: 2013GeoRL..40.3502P

Dunlop, M.; Raeder, J.; Zhong, J. +5 more

transfer events (FTEs) are magnetic flux ropes formed at planetary magnetopauses (MPs). Although evidence suggests that FTEs form through time-dependent magnetic reconnection, details of that process and 3D structure of the flux ropes remain largely unclear. This letter presents Double Star/TC-1 data of an FTE occurred on 7 April 2004 which show t…

2013 Geophysical Research Letters
DoubleStar 65
Flux calibration of broad-band far-infrared and submillimetre photometric instruments: theory and application to Herschel-SPIRE
DOI: 10.1093/mnras/stt999 Bibcode: 2013MNRAS.434..992G

Valtchanov, I.; Bock, J.; Conley, A. +15 more

Photometric instruments operating at far-infrared to millimetre wavelengths often have broad spectral passbands (λ/Δλ ∼ 3 or less), especially those operating in space. A broad passband can result in significant variation of the beam profile and aperture efficiency across the passband, effects which thus far have not generally been taken into acco…

2013 Monthly Notices of the Royal Astronomical Society
Herschel 65