Search Publications

Constraining C III] Emission in a Sample of Five Luminous z = 5.7 Galaxies
DOI: 10.3847/2041-8213/aa6482 Bibcode: 2017ApJ...838L..22D

Siana, Brian; Fan, Xiaohui; Jiang, Linhua +6 more

Recent observations have suggested that the C III]λ 1907/1909 emission lines could be alternative diagnostic lines for galaxies in the reionization epoch. We use the F128N narrowband filter on the Hubble Space Telescope’s (HST) Wide Field Camera 3 (WFC3) to search for C III] emission in a sample of five galaxies at z = 5.7 in the Subaru Deep Field…

2017 The Astrophysical Journal
eHST 16
Near-Earth plasma sheet boundary dynamics during substorm dipolarization
DOI: 10.1186/s40623-017-0707-2 Bibcode: 2017EP&S...69..129N

Strangeway, Robert J.; Plaschke, Ferdinand; Russell, Christopher T. +29 more

We report on the large-scale evolution of dipolarization in the near-Earth plasma sheet during an intense (AL ~ ‑1000 nT) substorm on August 10, 2016, when multiple spacecraft at radial distances between 4 and 15 RE were present in the night-side magnetosphere. This global dipolarization consisted of multiple short-timescale (a couple o…

2017 Earth, Planets and Space
Cluster 16
Rapid X-ray variability properties during the unusual very hard state in neutron-star low-mass X-ray binaries
DOI: 10.1093/mnras/stx2006 Bibcode: 2017MNRAS.472..559W

Altamirano, D.; Degenaar, N.; Wijnands, R. +2 more

Here, we study the rapid X-ray variability (using XMM-Newton observations) of three neutron-star low-mass X-ray binaries (1RXS J180408.9-342058, EXO 1745-248 and IGR J18245-2452) during their recently proposed very hard spectral state. All our systems exhibit a strong to very strong noise component in their power density spectra (rms amplitudes ra…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 16
Venus's winds and temperatures during the MESSENGER's flyby: An approximation to a three-dimensional instantaneous state of the atmosphere
DOI: 10.1002/2017GL072900 Bibcode: 2017GeoRL..44.3907P

Clancy, R. T.; Hueso, R.; Sánchez-Lavega, A. +14 more

Even though many missions have explored the Venus atmospheric circulation, its instantaneous state is poorly characterized. In situ measurements vertically sampling the atmosphere exist for limited locations and dates, while remote sensing observations provide only global averages of winds at altitudes of the clouds: 47, 60, and 70 km. We present …

2017 Geophysical Research Letters
VenusExpress 16
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