Search Publications

The Search for Active Marsquakes Using Subpixel Coregistration and Correlation: Best Practice and First Results
DOI: 10.1029/2018JE005649 Bibcode: 2018JGRE..123.1881G

Grindrod, Peter M.; Hollingsworth, James; Ayoub, Francois +1 more

The state of seismic activity on Mars is currently unknown. On Earth, coseismic displacement has been observed using visible wavelength images and subpixel coregistration and correlation techniques. We apply this method to Mars with the COSI-Corr (Co-registration of Optically Sensed Images and Correlation) software package using High-Resolution Im…

2018 Journal of Geophysical Research (Planets)
ExoMars-16 7
A multi-wavelength analysis of the diffuse H II region G25.8700+0.1350
DOI: 10.1093/mnras/stx2676 Bibcode: 2018MNRAS.474..647C

Reynoso, E. M.; Dorda, R.; Cichowolski, S. +2 more

We present a multi-wavelength investigation of the H II region G25.8700+0.1350, located in the inner part of the Galaxy. In radio continuum emission, the region is seen as a bright arc-shaped structure. An analysis of the H I line suggests that G25.8700+0.1350 lies at a distance of 6.5 kpc. The ionized gas is bordered by a photodissociation region…

2018 Monthly Notices of the Royal Astronomical Society
Herschel 7
Effects of a caustic ring of dark matter on the distribution of stars and interstellar gas
DOI: 10.1103/PhysRevD.98.103009 Bibcode: 2018PhRvD..98j3009C

Chakrabarty, Sankha S.; Sikivie, Pierre

Caustic rings of dark matter with tricusp cross section were predicted to lie in the galactic disk. Their radii increase on cosmological time scales at a rate of order 1 kpc /Gyr . When a caustic ring passes through the orbit of a star, the orbit is strongly perturbed. We find that a star moving in a nearly circular orbit is first attracted toward…

2018 Physical Review D
Gaia 7
Measuring size evolution of distant, faint galaxies in the radio regime
DOI: 10.1093/mnras/sty426 Bibcode: 2018MNRAS.476.3544L

Muxlow, T. W. B.; Wrigley, N.; Knudsen, K. K. +5 more

We measure the evolution of sizes for star-forming galaxies as seen in 1.4 GHz continuum radio for z = 0-3. The measurements are based on combined VLA+MERLIN data of the Hubble Deep Field, and using a uv-stacking algorithm combined with model fitting to estimate the average sizes of galaxies. A sample of ∼1000 star-forming galaxies is selected fro…

2018 Monthly Notices of the Royal Astronomical Society
eHST 7
Morphometric and rheological study of lunar domes of Marius Hills volcanic complex region using Chandrayaan-1 and recent datasets
DOI: 10.1007/s12040-018-0971-y Bibcode: 2018JESS..127...70A

Suresh, K.; Arya, A. S.; Rajasekhar, R. P. +10 more

Marius Hills volcanic complex is one of the most important regions on the lunar surface having an abundant number of volcanic features like domes and cones. Systematic mapping of 106 domes/cones in the Marius Hills region was carried out in this study using high-resolution orthoimage and digital elevation models of Chandrayaan-1 and Kaguya mission…

2018 Journal of Earth System Science
Chandrayaan-1 7
The global sphere reconstruction (GSR). Demonstrating an independent implementation of the astrometric core solution for Gaia
DOI: 10.1051/0004-6361/201833254 Bibcode: 2018A&A...620A..40V

Lattanzi, M. G.; Messineo, R.; Abbas, U. +6 more

Context. The Gaia ESA mission will estimate the astrometric and physical data of more than one billion objects, providing the largest and most precise catalog of absolute astrometry in the history of astronomy. The core of this process, the so-called global sphere reconstruction, is represented by the reduction of a subset of these objects which w…

2018 Astronomy and Astrophysics
Gaia 7
Effect of Upstream ULF Waves on the Energetic Ion Diffusion at the Earth’s Foreshock. II. Observations
DOI: 10.3847/1538-4357/aad08c Bibcode: 2018ApJ...863..136K

Dandouras, Iannis; Matsukiyo, Shuichi; Kis, Arpad +5 more

This study reports observations of energetic ions upstream of the Earth’s quasi-parallel bow shock by Cluster at times when interspacecraft separation distances were large. We analyze two individual upstream ion events during high solar wind velocity conditions to compare the spatial evolution of partial energetic ion densities in front of the Ear…

2018 The Astrophysical Journal
Cluster 7
From non-trivial geometries to power spectra and vice versa
DOI: 10.1088/1475-7516/2018/04/003 Bibcode: 2018JCAP...04..003B

Brooker, D. J.; Tsamis, N. C.; Woodard, R. P.

We review a recent formalism which derives the functional forms of the primordial—tensor and scalar—power spectra of scalar potential inflationary models. The formalism incorporates the case of geometries with non-constant first slow-roll parameter. Analytic expressions for the power spectra are given that explicitly display the dependence on the …

2018 Journal of Cosmology and Astroparticle Physics
Planck 7
The HP2 Survey. IV. The Pipe nebula: Effective dust temperatures in dense cores
DOI: 10.1051/0004-6361/201732513 Bibcode: 2018A&A...620A..24H

Alves, João; Forbrich, Jan; Lada, Charles J. +3 more

Multi-wavelength observations in the sub-millimeter regime provide information on the distribution of both the dust column density and the effective dust temperature in molecular clouds. In this study, we created high-resolution and high-dynamic-range maps of the Pipe nebula region and explored the value of dust-temperature measurements in particu…

2018 Astronomy and Astrophysics
Herschel 7
O2 signature in thin and thick O2-H2O ices⋆
DOI: 10.1051/0004-6361/201833549 Bibcode: 2018A&A...620A..46M

Caselli, P.; Vasyunin, A. I.; Bizzocchi, L. +2 more


Aims: In this paper we investigate the detectability of the molecular oxygen in icy dust grain mantles towards astronomical objects.
Methods: We present a systematic set of experiments with O2-H2O ice mixtures designed to disentangle how the molecular ratio affects the O2 signature in the mid- and near-in…

2018 Astronomy and Astrophysics
Rosetta 7