Search Publications

Inflationary freedom and cosmological neutrino constraints
DOI: 10.1103/PhysRevD.89.103502 Bibcode: 2014PhRvD..89j3502D

de Putter, Roland; Linder, Eric V.; Mishra, Abhilash

The most stringent bounds on the absolute neutrino mass scale come from cosmological data. These bounds are made possible because massive relic neutrinos affect the expansion history of the universe and lead to a suppression of matter clustering on scales smaller than the associated free streaming length. However, the resulting effect on cosmologi…

2014 Physical Review D
Planck 31
Limits on a Gravitational Field Dependence of the Proton-Electron Mass Ratio from H2 in White Dwarf Stars
DOI: 10.1103/PhysRevLett.113.123002 Bibcode: 2014PhRvL.113l3002B

Barstow, M. A.; Bagdonaite, J.; Salumbides, E. J. +4 more

Spectra of molecular hydrogen (H2) are employed to search for a possible proton-to-electron mass ratio (µ) dependence on gravity. The Lyman transitions of H2, observed with the Hubble Space Telescope towards white dwarf stars that underwent a gravitational collapse, are compared to accurate laboratory spectra taking int…

2014 Physical Review Letters
eHST 30
The Atacama Cosmology Telescope: cross correlation with Planck maps
DOI: 10.1088/1475-7516/2014/07/016 Bibcode: 2014JCAP...07..016L

Hasselfield, Matthew; Bond, J. Richard; Devlin, Mark J. +26 more

We present the temperature power spectrum of the Cosmic Microwave Background obtained by cross-correlating maps from the Atacama Cosmology Telescope (ACT) at 148 and 218 GHz with maps from the Planck satellite at 143 and 217 GHz, in two overlapping regions covering 592 square degrees. We find excellent agreement between the two datasets at both fr…

2014 Journal of Cosmology and Astroparticle Physics
Planck 30
Comprehensive analysis of glaciated martian crater Greg
DOI: 10.1016/j.icarus.2013.09.016 Bibcode: 2014Icar..228...96H

Mangold, Nicolas; Forget, François; Berman, Daniel C. +2 more

The 66-km diameter martian crater, Greg, east of Hellas, hosts various distinctive features, including dendritic valleys filled with chevron-textured masses (south wall), and lobate tongues a few kilometers long (north wall). We analyze these features by various quantitative techniques to illuminate martian geologic and climatic history. Crater re…

2014 Icarus
MEx 30
Influence of interplanetary coronal mass ejections on the peak intensity of solar energetic particle events
DOI: 10.1002/2014JA019771 Bibcode: 2014JGRA..119.4185L

Lario, D.; Karelitz, A.

We study whether the presence of coronal mass ejections (CMEs) in interplanetary space (ICMEs) affects the maximum intensity of solar energetic particle (SEP) events. We compute the maximum intensity of 175-315 keV electron and 9-15, 15-40, and 40-80 MeV proton fluxes measured during the prompt component of 147 western SEP events observed near Ear…

2014 Journal of Geophysical Research (Space Physics)
SOHO 30
Glory revealed in disk-integrated photometry of Venus
DOI: 10.1051/0004-6361/201423531 Bibcode: 2014A&A...566L...1G

Sánchez-Lavega, A.; Pérez-Hoyos, S.; García Muñoz, A.

Context. Reflected light from a spatially unresolved planet yields unique insight into the overall optical properties of the planet cover. Glories are optical phenomena caused by light that is backscattered within spherical droplets following a narrow distribution of sizes; they are well known on Earth as localised features above liquid clouds.

2014 Astronomy and Astrophysics
VenusExpress 30
Feeding versus feedback in AGN from near-infrared IFU observations: the case of Mrk 766
DOI: 10.1093/mnras/stu1685 Bibcode: 2014MNRAS.445..414S

Storchi-Bergmann, Thaisa; Riffel, Rogemar A.; Winge, Claudia +1 more

We have mapped the emission-line flux distributions and ratios as well as the gaseous kinematics of the inner 450 pc radius of the type 1 Seyfert galaxy Mrk 766 using integral field near-infrared J- and Kl-band spectra obtained with the Gemini Near Infrared Integral Field Spectrograph at a spatial resolution of 60 pc and velocity resolu…

2014 Monthly Notices of the Royal Astronomical Society
eHST 30
Herschel-ATLAS/GAMA: SDSS cross-correlation induced by weak lensing
DOI: 10.1093/mnras/stu1041 Bibcode: 2014MNRAS.442.2680G

Danese, L.; González-Nuevo, J.; Scott, D. +25 more

We report a highly significant (>10σ) spatial correlation between galaxies with S350 µm ≥ 30 mJy detected in the equatorial fields of the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) with estimated redshifts ≳ 1.5, and Sloan Digital Sky Survey (SDSS) or Galaxy And Mass Assembly (GAMA) galaxies at 0.2 ≤ z ≤ 0.6. …

2014 Monthly Notices of the Royal Astronomical Society
Herschel 30
The Solar Neighborhood. XXXI. Discovery of an Unusual Red+White Dwarf Binary at ~25 pc via Astrometry and UV Imaging
DOI: 10.1088/0004-6256/147/1/21 Bibcode: 2014AJ....147...21J

Gies, Douglas R.; Henry, Todd J.; Winters, Jennifer G. +4 more

We report the discovery of a nearby M5.0V dwarf at 24.6 pc, SCR 1848-6855, that is orbited by an unusual companion causing an astrometric perturbation of more than 200 mas. This is by far the largest perturbation found to date among more than 700 targets observed during our long-term astrometry/photometry program at the CTIO 0.9 m telescope. We pr…

2014 The Astronomical Journal
IUE eHST 30
Calibrating Data from the Hinode/X-Ray Telescope and Associated Uncertainties
DOI: 10.1007/s11207-014-0487-9 Bibcode: 2014SoPh..289.2781K

Reeves, Katharine K.; McKenzie, David E.; Saar, Steven H. +2 more

The X-Ray Telescope (XRT) onboard the Hinode satellite, launched 23 September 2006 by the Japan Aerospace Exploration Agency (JAXA), is a joint mission of Japan, the United States, and the United Kingdom to study the solar corona. In particular, XRT was designed to study solar plasmas with temperatures between 1 and 10 MK with ≈ 1″ pixels (≈ 2″ re…

2014 Solar Physics
Hinode 30