Search Publications

The Radio Spectral Energy Distribution and Star-formation Rate Calibration in Galaxies
DOI: 10.3847/1538-4357/836/2/185 Bibcode: 2017ApJ...836..185T

Boquien, M.; De Looze, I.; Murphy, E. J. +17 more

We study the spectral energy distribution (SED) of the radio continuum (RC) emission from the Key Insight in Nearby Galaxies Emitting in Radio (KINGFISHER) sample of nearby galaxies to understand the energetics and origin of this emission. Effelsberg multi-wavelength observations at 1.4, 4.8, 8.4, and 10.5 GHz combined with archive data allow us, …

2017 The Astrophysical Journal
Herschel 143
Trends in Atmospheric Properties of Neptune-size Exoplanets
DOI: 10.3847/1538-3881/aa9279 Bibcode: 2017AJ....154..261C

Crossfield, Ian J. M.; Kreidberg, Laura

Precise atmospheric observations have been made for a growing sample of warm Neptunes. Here, we investigate the correlations between these observations and a large number of system parameters to show that, at 95% confidence, the amplitude of a warm Neptune's spectral features in transmission correlates with either its equilibrium temperature (T

2017 The Astronomical Journal
eHST 141
No Evidence for Extensions to the Standard Cosmological Model
DOI: 10.1103/PhysRevLett.119.101301 Bibcode: 2017PhRvL.119j1301H

Sellentin, Elena; Heavens, Alan; Hosenie, Zafiirah +4 more

We compute the Bayesian evidence for models considered in the main analysis of Planck cosmic microwave background data. By utilizing carefully defined nearest-neighbor distances in parameter space, we reuse the Monte Carlo Markov chains already produced for parameter inference to compute Bayes factors B for many different model-data set combinatio…

2017 Physical Review Letters
Planck 140
Clouds, Streams and Bridges. Redrawing the blueprint of the Magellanic System with Gaia DR1
DOI: 10.1093/mnras/stw3357 Bibcode: 2017MNRAS.466.4711B

Erkal, Denis; Belokurov, Vasily; Mackey, Dougal +5 more

We present the discovery of stellar tidal tails around the Large and the Small Magellanic Clouds (LMC and SMC, respectively) in the Gaia DR1 data. In between the Clouds, their tidal arms are stretched towards each other to form an almost continuous stellar bridge. Our analysis relies on the exquisite quality of the Gaia's photometric catalogue to …

2017 Monthly Notices of the Royal Astronomical Society
Gaia 137
Origins of the Ambient Solar Wind: Implications for Space Weather
DOI: 10.1007/s11214-017-0416-y Bibcode: 2017SSRv..212.1345C

Cranmer, Steven R.; Riley, Pete; Gibson, Sarah E.

The Sun's outer atmosphere is heated to temperatures of millions of degrees, and solar plasma flows out into interplanetary space at supersonic speeds. This paper reviews our current understanding of these interrelated problems: coronal heating and the acceleration of the ambient solar wind. We also discuss where the community stands in its abilit…

2017 Space Science Reviews
Hinode SOHO Ulysses 136
Massive Warm/Hot Galaxy Coronae as Probed by UV/X-Ray Oxygen Absorption and Emission. I. Basic Model
DOI: 10.3847/1538-4357/835/1/52 Bibcode: 2017ApJ...835...52F

Faerman, Yakov; Sternberg, Amiel; McKee, Christopher F.

We construct an analytic phenomenological model for extended warm/hot gaseous coronae of L* galaxies. We consider UV O VI Cosmic Origins Spectrograph (COS)-Halos absorption line data in combination with Milky Way (MW) X-ray O vii and O viii absorption and emission. We fit these data with a single model representing the COS-Halos galaxie…

2017 The Astrophysical Journal
eHST 136
Quasars as standard candles. I. The physical relation between disc and coronal emission
DOI: 10.1051/0004-6361/201630079 Bibcode: 2017A&A...602A..79L

Lusso, E.; Risaliti, G.

Context. A tight non-linear relation exists between the X-ray and UV emission in quasars (I.e. LX ∝LUVγ), with a dispersion of 0.2 dex over approximately three orders of magnitude in luminosity. Such observational evidence has two relevant consequences: (1) an ubiquitous physical mechanism must regulate the energy transfer fr…

2017 Astronomy and Astrophysics
XMM-Newton 135
A New Stellar Atmosphere Grid and Comparisons with HST/STIS CALSPEC Flux Distributions
DOI: 10.3847/1538-3881/aa6ba9 Bibcode: 2017AJ....153..234B

Koekemoer, Anton M.; Gordon, Karl D.; Bohlin, Ralph C. +3 more

The Space Telescope Imaging Spectrograph has measured the spectral energy distributions for several stars of types O, B, A, F, and G. These absolute fluxes from the CALSPEC database are fit with a new spectral grid computed from the ATLAS-APOGEE ATLAS9 model atmosphere database using a chi-square minimization technique in four parameters. The qual…

2017 The Astronomical Journal
eHST 135
Electron holes in phase space: What they are and why they matter
DOI: 10.1063/1.4976854 Bibcode: 2017PhPl...24e5601H

Hutchinson, I. H.

This is a tutorial and selective review explaining the fundamental concepts and some currently open questions concerning the plasma phenomenon of the electron hole. The widespread occurrence of electron holes in numerical simulations, space-craft observations, and laboratory experiments is illustrated. The elementary underlying theory is developed…

2017 Physics of Plasmas
Cluster 134
Active Cryovolcanism on Europa?
DOI: 10.3847/2041-8213/aa67f8 Bibcode: 2017ApJ...839L..18S

Spencer, J. R.; Sparks, W. B.; Hand, K. P. +4 more

Evidence for plumes of water on Europa has previously been found using the Hubble Space Telescope using two different observing techniques. Roth et al. found line emission from the dissociation products of water. Sparks et al. found evidence for off-limb continuum absorption as Europa transited Jupiter. Here, we present a new transit observation o…

2017 The Astrophysical Journal
eHST 134