Search Publications

Planck Lensing and Cosmic Infrared Background Cross-correlation with Fermi-LAT: Tracing Dark Matter Signals in the Gamma-ray Background
DOI: 10.3847/1538-4357/836/1/127 Bibcode: 2017ApJ...836..127F

Cooray, Asantha; Feng, Chang; Keating, Brian

The extragalactic γ-ray background and its spatial anisotropy could potentially contain a signature of dark matter (DM) annihilation or particle decay. Astrophysical foregrounds, such as blazars and star-forming galaxies (SFGs), however, dominate the γ-ray background, precluding an easy detection of the signal associated with the DM annihilation o…

2017 The Astrophysical Journal
Planck 16
Planck limits on non-canonical generalizations of large-field inflation models
DOI: 10.1088/1475-7516/2017/04/006 Bibcode: 2017JCAP...04..006S

Stein, Nina K.; Kinney, William H.

In this paper, we consider two case examples of Dirac-Born-Infeld (DBI) generalizations of canonical large-field inflation models, characterized by a reduced sound speed, cS < 1. The reduced speed of sound lowers the tensor-scalar ratio, improving the fit of the models to the data, but increases the equilateral-mode non-Gaussianity, …

2017 Journal of Cosmology and Astroparticle Physics
Planck 16
Towards the origin of the radio emission in AR Scorpii, the first radio-pulsing white dwarf binary
DOI: 10.1051/0004-6361/201730948 Bibcode: 2017A&A...601L...7M

Marsh, T. R.; Marcote, B.; Stanway, E. R. +2 more

Context. The binary system AR Sco contains an M star and the only known radio-pulsing white dwarf. The system shows emission from radio to X-rays, likely dominated by synchrotron radiation. The mechanism that produces most of this emission remains unclear. Two competing scenarios have been proposed: collimated outflows, and direct interaction betw…

2017 Astronomy and Astrophysics
Gaia 16
A systematic analysis of the XMM-Newton background: IV. Origin of the unfocused and focused components
DOI: 10.1007/s10686-017-9549-y Bibcode: 2017ExA....44..321G

Tiengo, A.; Rossetti, M.; Moretti, A. +6 more

We show the results obtained in the FP7 European program EXTraS and in the ESA R&D ATHENA activity AREMBES aimed at a deeper understanding of the XMM-Newton background to better design the ATHENA mission. Thanks to an analysis of the full EPIC archive coupled to the information obtained by the Radiation Monitor we show the cosmic ray origin of…

2017 Experimental Astronomy
XMM-Newton 16
Limits to the presence of transiting circumbinary planets in CoRoT Data
DOI: 10.1051/0004-6361/201628244 Bibcode: 2017A&A...602A.117K

Csizmadia, Sz.; Cabrera, J.; Klagyivik, P. +2 more


Aims: During its flight phase, from 2007-2012, the CoRoT mission delivered light curves for over 2000 eclipsing binaries. Data from the Kepler mission have proven the existence of several transiting circumbinary planets. While light curves from CoRoT typically have lower precision and shorter coverage, the number of CoRoT targets is similar t…

2017 Astronomy and Astrophysics
CoRoT 16
Swift J164449.3+573451 and Swift J2058.4+0516: Black hole mass estimates for tidal disruption event sources
DOI: 10.1051/0004-6361/201730869 Bibcode: 2017A&A...607A..38S

Titarchuk, Lev; Seifina, Elena; Virgilli, Enrico

A tidal disruption event (TDE) is an astronomical phenomenon in which a previously dormant black hole (BH) destroys a star passing too close to its central part. We analyzed the flaring episode detected from the TDE sources, Swift J164449.3+573451 and Swift J2058.4+0516 (hereafter Swift J1644+57 and Swift J2058+05, respectively) using RXTE, Swift …

2017 Astronomy and Astrophysics
Suzaku 16
Development of an ensemble Kalman filter data assimilation system for the Venusian atmosphere
DOI: 10.1038/s41598-017-09461-1 Bibcode: 2017NatSR...7.9321S

Sugimoto, Norihiko; Takagi, Masahiro; Kouyama, Toru +3 more

The size and mass of Venus is similar to those of the Earth; however, its atmospheric dynamics are considerably different and they are poorly understood due to limited observations and computational difficulties. Here, we developed a data assimilation system based on the local ensemble transform Kalman filter (LETKF) for a Venusian Atmospheric GCM…

2017 Scientific Reports
VenusExpress 16
Discovery of Galactic O iv and O v X-ray absorption due to transition temperature gas in the PKS 2155-304 spectrum
DOI: 10.1051/0004-6361/201630336 Bibcode: 2017A&A...605A..47N

Kaastra, J.; Bonamente, M.; Paerels, F. +4 more

Far-ultraviolet (FUV) observations have revealed transition temperature gas (TTG; log T(K) 5), located in the lower Galactic halo and in high-velocity clouds. However, the corresponding X-ray absorption has so far remained mostly undetected. In order to make an improvement in this respect in Galactic X-ray absorption studies, we accumulated very d…

2017 Astronomy and Astrophysics
XMM-Newton eHST 16
New observational limits on dark radiation in braneworld cosmology
DOI: 10.1103/PhysRevD.95.083516 Bibcode: 2017PhRvD..95h3516S

Mathews, Grant J.; Kusakabe, Motohiko; Gangopadhyay, Mayukh Raj +1 more

A dark radiation term arises as a correction to the energy-momentum tensor in the simplest five-dimensional RS-II brane-world cosmology. In this paper we revisit the constraints on dark radiation based upon the newest results for light element nuclear reaction rates, observed light element abundances, and the power spectrum of the cosmic microwave…

2017 Physical Review D
Planck 16
Physical properties of seven binary and higher-order multiple OB systems
DOI: 10.1051/0004-6361/201628852 Bibcode: 2017A&A...600A..33M

Mayer, Pavel; Harmanec, Petr; Chini, Rolf +7 more

Analyses of multi-epoch, high-resolution (R 50 000) optical spectra of seven early-type systems provided various important new insights with respect to their multiplicity. First determinations of orbital periods were made for HD 92206 C (2.^d022), HD 112244 (27.^d665), HD 164438 (10.^d25), HD 123056 A ( 1314 d) and HD 123056 B (<2 d); the orbit…

2017 Astronomy and Astrophysics
Gaia Hipparcos 16