Search Publications

Are the Dorsa Argentea on Mars eskers?
DOI: 10.1016/j.icarus.2016.03.028 Bibcode: 2016Icar..275...65B

Conway, Susan J.; Butcher, Frances E. G.; Arnold, Neil S.

The Dorsa Argentea are an extensive assemblage of ridges in the southern high latitudes of Mars. They have previously been interpreted as eskers formed by deposition of sediment in subglacial meltwater conduits, implying a formerly more extensive south polar ice sheet. In this study, we undertake the first large-scale statistical analysis of aspec…

2016 Icarus
MEx 36
Search for Hyperluminous Infrared Dust-obscured Galaxies Selected with WISE and SDSS
DOI: 10.3847/0004-637X/820/1/46 Bibcode: 2016ApJ...820...46T

Toba, Y.; Nagao, T.

We aim to search for hyperluminous infrared (IR) galaxies (HyLIRGs) with IR luminosity {L}{{IR}} > 1013 L by applying the selection method of dust-obscured galaxies (DOGs). They are spatially rare but could correspond to a maximum phase of cosmic star formation (SF) and/or active galactic nucleus (AGN) activity…

2016 The Astrophysical Journal
AKARI Herschel 36
Theoretical modelling of the AGN iron line vs. continuum time-lags in the lamp-post geometry
DOI: 10.1051/0004-6361/201527748 Bibcode: 2016A&A...594A..71E

Papadakis, I. E.; Emmanoulopoulos, D.; Dovčiak, M. +4 more

Context. Theoretical modelling of time-lags between variations in the Fe Kα emission and the X-ray continuum might shed light on the physics and geometry of the X-ray emitting region in active galaxies (AGN) and X-ray binaries. We here present the results from a systematic analysis of time-lags between variations in two energy bands (5-7 vs. 2-4 k…

2016 Astronomy and Astrophysics
XMM-Newton 36
Monsters in the dark: predictions for luminous galaxies in the early Universe from the BLUETIDES simulation
DOI: 10.1093/mnrasl/slw100 Bibcode: 2016MNRAS.461L..51W

Wilkins, Stephen M.; Nagai, Daisuke; Croft, Rupert +3 more

Using deep Hubble and Spitzer observations Oesch et al. have identified a bright (MUV ≈ -22) star-forming galaxy candidate at z ≈ 11. The presence of GN-z11 implies a number density ∼10-6 Mpc-3, roughly an order of magnitude higher than the expected value based on extrapolations from lower redshift. Using the unpre…

2016 Monthly Notices of the Royal Astronomical Society
eHST 36
Controversial age spreads from the main sequence turn-off and red clump in intermediate-age clusters in the LMC
DOI: 10.1051/0004-6361/201526484 Bibcode: 2016A&A...586A.148N

Cabrera-Ziri, I.; Bastian, N.; Kozhurina-Platais, V. +5 more

Most star clusters at an intermediate age (1-2 Gyr) in the Large and Small Magellanic Clouds show a puzzling feature in their color-magnitude diagrams (CMD) that is not in agreement with a simple stellar population. The main sequence turn-off of these clusters is much broader than expected from photometric uncertainties. One interpretation of this…

2016 Astronomy and Astrophysics
eHST 36
Cosmological constraint on the light gravitino mass from CMB lensing and cosmic shear
DOI: 10.1088/1475-7516/2016/06/004 Bibcode: 2016JCAP...06..004O

Osato, Ken; Yoshida, Naoki; Kamada, Ayuki +2 more

Light gravitinos of mass lesssim O (10) eV are of particular interest in cosmology, offering various baryogenesis scenarios without suffering from the cosmological gravitino problem. The gravitino may contribute considerably to the total matter content of the Universe and affect structure formation from early to present epochs. After the gravitino…

2016 Journal of Cosmology and Astroparticle Physics
Planck 36
Erratic Flaring of BL Lac in 2012-2013: Multiwavelength Observations
DOI: 10.3847/0004-637X/816/2/53 Bibcode: 2016ApJ...816...53W

Stern, Daniel; Baloković, Mislav; Grupe, Dirk +7 more

BL Lac, the eponymous blazar, flared to historically high levels at millimeter, infrared, X-ray, and gamma-ray wavelengths in 2012. We present observations made with Herschel, Swift, NuSTAR, Fermi, the Submillimeter Array, CARMA, and the VLBA in 2012-2013, including three months with nearly daily sampling at several wavebands. We have also conduct…

2016 The Astrophysical Journal
Herschel 36
A Joint Chandra and Swift View of the 2015 X-ray Dust-scattering Echo of V404 Cygni
DOI: 10.3847/0004-637X/825/1/15 Bibcode: 2016ApJ...825...15H

Brandt, W. N.; Smith, R.; Neilsen, J. +4 more

We present a combined analysis of the Chandra and Swift observations of the 2015 X-ray echo of V404 Cygni. Using a stacking analysis, we identify eight separate rings in the echo. We reconstruct the soft X-ray light curve of the 2015 June outburst using the high-resolution Chandra images and cross-correlations of the radial intensity profiles, ind…

2016 The Astrophysical Journal
INTEGRAL 36
The atmosphere of comet 67P/Churyumov-Gerasimenko diagnosed by charge-exchanged solar wind alpha particles
DOI: 10.1051/0004-6361/201527532 Bibcode: 2016A&A...587A.154S

Kallio, E.; Gunell, H.; Behar, E. +6 more

Context. The ESA/Rosetta mission has been orbiting comet 67P/Churyumov-Gerasimenko since August 2014, measuring its dayside plasma environment. The ion spectrometer onboard Rosetta has detected two ion populations, one energetic with a solar wind origin (H+, He2+, He+), the other at lower energies with a cometary o…

2016 Astronomy and Astrophysics
Rosetta 36
Multi-spacecraft Observations and Transport Modeling of Energetic Electrons for a Series of Solar Particle Events in August 2010
DOI: 10.3847/0004-637X/826/2/134 Bibcode: 2016ApJ...826..134D

Dresing, N.; Dröge, W.; Klassen, A. +1 more

During 2010 August a series of solar particle events was observed by the two STEREO spacecraft as well as near-Earth spacecraft. The events, occurring on August 7, 14, and 18, originated from active regions 11093 and 11099. We combine in situ and remote-sensing observations with predictions from our model of three-dimensional anisotropic particle …

2016 The Astrophysical Journal
SOHO 36