Search Publications

The low-luminosity behaviour of the 4U 0115+63 Be/X-ray transient
DOI: 10.1093/mnras/stx2111 Bibcode: 2017MNRAS.472.1802R

Degenaar, N.; Wijnands, R.; Cavecchi, Y. +3 more

The Be/X-ray transient 4U 0115+63 exhibited a giant, type-II outburst in 2015 October. The source did not decay to its quiescent state but settled in a meta-stable plateau state (a factor ∼ 10 brighter than quiescence) in which its luminosity slowly decayed. We used XMM-Newton to observe the system during this phase and we found that its spectrum …

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 12
25 MeV solar proton events in Cycle 24 and previous cycles
DOI: 10.1016/j.asr.2016.07.035 Bibcode: 2017AdSpR..60..755R

Richardson, Ian G.; Cane, Hilary V.; von Rosenvinge, Tycho T.

We summarize observations of around a thousand solar energetic particle (SEP) events since 1967 that include ∼25 MeV protons, made by various near-Earth spacecraft (IMPs 4, 5, 7, 8, ISEE 3, SOHO), that encompass Solar Cycle 20 to the current cycle (24). We also discuss recent observations of similar SEP events in Cycle 24 made by the STEREO spacec…

2017 Advances in Space Research
SOHO 12
Key Ground-Based and Space-Based Assets to Disentangle Magnetic Field Sources in the Earth's Environment
DOI: 10.1007/s11214-016-0291-y Bibcode: 2017SSRv..206..123C

Milan, S. E.; Masson, A.; Matzka, J. +1 more

The magnetic field measured on the ground or in space is the addition of several sources: from flows within the Earth's core to electric currents in distant regions of the magnetosphere. Properly separating and characterizing these sources requires appropriate observations, both ground-based and space-based. In the present paper, we review the exi…

2017 Space Science Reviews
Cluster 12
Running vacuum cosmological models: linear scalar perturbations
DOI: 10.1088/1475-7516/2017/08/026 Bibcode: 2017JCAP...08..026P

Perico, E. L. D.; Tamayo, D. A.

In cosmology, phenomenologically motivated expressions for running vacuum are commonly parameterized as linear functions typically denoted by Λ(H2) or Λ(R). Such models assume an equation of state for the vacuum given by bar PΛ = - bar rhoΛ, relating its background pressure bar PΛ with its mean energy de…

2017 Journal of Cosmology and Astroparticle Physics
Planck 12
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