Search Publications

High-resolution X-ray spectroscopy: The coming-of-age
DOI: 10.1002/asna.201713322 Bibcode: 2017AN....338..146K

Kaastra, J. S.

Since the launch of Chandra and XMM-Newton, high-resolution X-ray spectra of cosmic sources of all kinds have become available. These spectra have resulted in major scientific breakthroughs. However, due to the techniques used, in general high-quality spectra can only be obtained for the brightest few sources of each class. Moreover, except for th…

2017 Astronomische Nachrichten
XMM-Newton 12
Suprathermal helium in corotating interaction regions: combined observations from SOHO/CELIAS/STOF and ACE/SWICS
DOI: 10.1051/0004-6361/201628641 Bibcode: 2017A&A...599A..13Y

Bochsler, P.; Klecker, B.; Berger, L. +4 more

Context. Energetic particle enhancements that are associated with corotating interaction regions (CIRs) are typically believed to arise from the sunward propagation of particles that are accelerated by CIR-driven shocks beyond 1 AU. It is expected that these sunward-travelling particles will lose energy and scatter, resulting in a turnover of the …

2017 Astronomy and Astrophysics
SOHO 12
Gaia eclipsing binary and multiple systems. A study of detectability and classification of eclipsing binaries with Gaia
DOI: 10.1051/0004-6361/201629957 Bibcode: 2017A&A...602A.110K

Rimoldini, L.; Holl, B.; Mowlavi, N. +5 more

Context. In the new era of large-scale astronomical surveys, automated methods of analysis and classification of bulk data are a fundamental tool for fast and efficient production of deliverables. This becomes ever more important as we enter the Gaia era.
Aims: We investigate the potential detectability of eclipsing binaries with Gaia using a…

2017 Astronomy and Astrophysics
Gaia 12
The Formation of IRIS Diagnostics. IX. The Formation of the C I 135.58 NM Line in the Solar Atmosphere
DOI: 10.3847/1538-4357/aa8458 Bibcode: 2017ApJ...846...40L

Carlsson, Mats; Leenaarts, Jorrit; Lin, Hsiao-Hsuan

The C I 135.58 nm line is located in the wavelength range of NASA’s Interface Region Imaging Spectrograph (IRIS) small explorer mission. We study the formation and diagnostic potential of this line by means of non local-thermodynamic-equilibrium modeling, employing both 1D and 3D radiation-magnetohydrodynamic models. The C I/C II ionization balanc…

2017 The Astrophysical Journal
IRIS 12
DREAMS-SIS: The Solar Irradiance Sensor on-board the ExoMars 2016 lander
DOI: 10.1016/j.asr.2017.04.002 Bibcode: 2017AdSpR..60..103A

Toledo, D.; Gómez, L.; Apéstigue, V. +10 more

The Solar Irradiance Sensor (SIS) was part of the DREAMS (Dust characterization, Risk assessment, and Environment Analyzer on the Martian Surface) payload package on board the ExoMars 2016 Entry and Descent Module (EDM), "Schiaparelli". DREAMS was a meteorological station aimed at the measurement of several atmospheric parameters, as well as the p…

2017 Advances in Space Research
ExoMars-16 12
General relativistic observable for gravitational astrometry in the context of the Gaia mission and beyond
DOI: 10.1103/PhysRevD.96.104030 Bibcode: 2017PhRvD..96j4030C

Geralico, Andrea; Lattanzi, Mario G.; Crosta, Mariateresa +1 more

With the launch of the Gaia mission, general relativity (GR) is now at the very core of astrometry. Given the high level of accuracy of the measurements, the development of a suitable relativistic model for carrying out the correct data processing and analysis has become a critical necessity; its primary goal is to have a consistent set of stellar…

2017 Physical Review D
Gaia 12
The anatomy of a wrinkle ridge revealed in the wall of Melas Chasma, Mars
DOI: 10.1002/2017JE005274 Bibcode: 2017JGRE..122..889C

Andrews-Hanna, Jeffrey C.; Cole, Hank M.

Wrinkle ridges are among the most common tectonic structures on the terrestrial planets and provide important records of the history of planetary strain and geodynamics. The observed broad arches and superposed narrow wrinkles are thought to be the surface manifestation of blind thrust faults, which terminate in near-surface volcanic sequences and…

2017 Journal of Geophysical Research (Planets)
MEx 12
Energy-angle dispersion of accelerated heavy ions at 67P/Churyumov-Gerasimenko: implication in the mass-loading mechanism
DOI: 10.1093/mnras/stx1621 Bibcode: 2017MNRAS.469S.339N

Yamauchi, M.; Behar, E.; Nilsson, H. +4 more

The Rosetta spacecraft studied the comet 67P/Churyumov-Gerasimenko for nearly two years. The Ion Composition Analyzer instrument on board Rosetta observed the positive ion distributions in the environment of the comet during the mission. A portion of the comet's neutral coma is expected to get ionized, depending on the comet's activity and positio…

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 12
Primordial power spectrum features in phenomenological descriptions of inflation
DOI: 10.1016/j.dark.2017.07.003 Bibcode: 2017PDU....17...38G

Mena, Olga; Boubekeur, Lotfi; Gariazzo, Stefano +1 more

We extend an alternative, phenomenological approach to inflation by means of an equation of state and a sound speed, both of them functions of the number of e-folds and four phenomenological parameters. This approach captures a number of possible inflationary models, including those with non-canonical kinetic terms or scale-dependent non-gaussiani…

2017 Physics of the Dark Universe
Planck 12
Signatures of the Martian rotation parameters in the Doppler and range observables
DOI: 10.1016/j.pss.2017.05.008 Bibcode: 2017P&SS..144...74Y

Yseboodt, Marie; Dehant, Véronique; Péters, Marie-Julie

The position of a Martian lander is affected by different aspects of Mars' rotational motions: the nutations, the precession, the length-of-day variations and the polar motion. These various motions have a different signature in a Doppler observable between the Earth and a lander on Mars' surface. Knowing the correlations between these signatures …

2017 Planetary and Space Science
ExoMars-16 12