Search Publications

Using dark energy to suppress power at small scales
DOI: 10.1103/PhysRevD.92.063006 Bibcode: 2015PhRvD..92f3006K

Kunz, Martin; Nesseris, Savvas; Sawicki, Ignacy

The latest Planck results reconfirm the existence of a slight but chronic tension between the best-fit cosmic microwave background (CMB) and low-redshift observables: power seems to be consistently lacking in the late universe across a range of observables (e.g. weak lensing, cluster counts). We propose a two-parameter model for dark energy where …

2015 Physical Review D
Planck 35
On the Electron-to-Neutral Number Density Ratio in the Coma of Comet 67P/Churyumov-Gerasimenko: Guiding Expression and Sources for Deviations
DOI: 10.1088/0004-637X/812/1/54 Bibcode: 2015ApJ...812...54V

Edberg, N. J. T.; Vigren, E.; Galand, M. +3 more

We compute partial photoionization frequencies of H2O, CO2, and CO, the major molecules in the coma of comet 67P/Churyumov-Gerasimenko, the target comet of the ongoing ESA Rosetta mission. Values are computed from Thermosphere Ionosphere Mesosphere Energy and Dynamics/Solar EUV Experiment solar EUV spectra for 2014 August 1, …

2015 The Astrophysical Journal
Rosetta 35
Organic chemistry in Titan's upper atmosphere and its astrobiological consequences: I. Views towards Cassini plasma spectrometer (CAPS) and ion neutral mass spectrometer (INMS) experiments in space
DOI: 10.1016/j.pss.2015.01.015 Bibcode: 2015P&SS..109...46A

Sittler, E. C.; Ali, A.; Chornay, D. +2 more

The discovery of carbocations and carbanions by Ion Neutral Mass Spectrometer (INMS) and the Cassini Plasma Spectrometer (CAPS) instruments onboard the Cassini spacecraft in Titan's upper atmosphere is truly amazing for astrochemists and astrobiologists. In this paper we identify the reaction mechanisms for the growth of the complex macromolecules…

2015 Planetary and Space Science
Cassini 35
Integrated light chemical tagging analyses of seven M31 outer halo globular clusters from the Pan-Andromeda Archaeological Survey
DOI: 10.1093/mnras/stv020 Bibcode: 2015MNRAS.448.1314S

Dotter, Aaron; Venn, Kim A.; Sakari, Charli M. +4 more

Detailed chemical abundances are presented for seven M31 outer halo globular clusters (with projected distances from M31 greater than 30 kpc), as derived from high-resolution integrated light spectra taken with the Hobby-Eberly Telescope. Five of these clusters were recently discovered in the Pan-Andromeda Archaeological Survey (PAndAS) - this pap…

2015 Monthly Notices of the Royal Astronomical Society
eHST 35
Ionization of the venusian atmosphere from solar and galactic cosmic rays
DOI: 10.1016/j.icarus.2014.09.032 Bibcode: 2015Icar..245...80N

Coates, A. J.; Jones, G. H.; Desorgher, L. +2 more

The atmospheres of the terrestrial planets are exposed to solar and galactic cosmic rays, the most energetic of which are capable of affecting deep atmospheric layers through extensive nuclear and electromagnetic particle cascades. In the venusian atmosphere, cosmic rays are expected to be the dominant ionization source below ∼100 km altitude. Whi…

2015 Icarus
VenusExpress 35
Electrostatic solitary waves observed at Saturn by Cassini inside 10 Rs and near Enceladus
DOI: 10.1002/2015JA021305 Bibcode: 2015JGRA..120.6569P

Gurnett, D. A.; Pickett, J. S.; Jones, G. H. +5 more

We have analyzed the Cassini Radio and Plasma Wave Science Wideband Receiver (WBR) data specifically looking for the presence of bipolar electrostatic solitary waves (ESWs). Typical examples of these ESWs are provided to show that when they are present, several of them may be detected over a few to several millisecond time span. We carried out an …

2015 Journal of Geophysical Research (Space Physics)
Cassini 35
New constraints on the star formation history of the star cluster NGC 1856
DOI: 10.1093/mnras/stv874 Bibcode: 2015MNRAS.450.3054C

Goudfrooij, Paul; Puzia, Thomas H.; Correnti, Matteo +1 more

We use the Wide Field Camera 3 onboard the Hubble Space Telescope to obtain deep, high-resolution photometry of the young (age ∼ 300 Myr) star cluster NGC 1856 in the Large Magellanic Cloud. We compare the observed colour-magnitude diagram (CMD), after having applied a correction for differential reddening, with Monte Carlo simulations of simple s…

2015 Monthly Notices of the Royal Astronomical Society
eHST 35
Simultaneous spectral and reverberation modelling of relativistic reflection in Mrk 335
DOI: 10.1093/mnras/stv1333 Bibcode: 2015MNRAS.452..333C

Chainakun, P.; Young, A. J.

We present an X-ray spectral and timing model to investigate the broad and variable iron line seen in the high flux state of Mrk 335. The model consists of a variable X-ray source positioned along the rotation axis of the black hole that illuminates the accretion disc producing a back-scattered, ionized reflection spectrum. We compute time lags in…

2015 Monthly Notices of the Royal Astronomical Society
XMM-Newton 35
Ensemble forecasting of major solar flares: First results
DOI: 10.1002/2015SW001195 Bibcode: 2015SpWea..13..626G

Pulkkinen, A.; Guerra, J. A.; Uritsky, V. M.

We present the results from the first ensemble prediction model for major solar flares (M and X classes). The primary aim of this investigation is to explore the construction of an ensemble for an initial prototyping of this new concept. Using the probabilistic forecasts from three models hosted at the Community Coordinated Modeling Center (NASA-G…

2015 Space Weather
SOHO 35
Variations between Dust and Gas in the Diffuse Interstellar Medium
DOI: 10.1088/0004-637X/811/2/118 Bibcode: 2015ApJ...811..118R

Heiles, Carl; Reach, William T.; Bernard, Jean-Philippe

Using the Planck far-infrared and Arecibo GALFA 21 cm line surveys, we identified a set of isolated interstellar clouds (approximately degree-sized on the sky and comprising 100 solar masses) and assessed the ratio of gas mass to dust mass. Significant variations of the gas/dust ratio are found both from cloud to cloud and within regions of indivi…

2015 The Astrophysical Journal
Planck 35