Search Publications

Swift discoveries of new populations of extremely long duration high energy transient
DOI: 10.1016/j.jheap.2015.05.004 Bibcode: 2015JHEAp...7...44L

Levan, A. J.

Recent observations with Swift have begun to uncover γ-ray transients whose total energies are comparable to those of gamma-ray bursts (GRB), but have a duration an order of magnitude or more longer than the bulk of the GRB population. Some are suggested to form a new population of ultra-long GRBs, with a mean duration around 104 s, whi…

2015 Journal of High Energy Astrophysics
XMM-Newton 23
Holographic dark energy with cosmological constant
DOI: 10.1088/1475-7516/2015/08/012 Bibcode: 2015JCAP...08..012H

Li, Nan; Li, Miao; Hu, Yazhou +1 more

Inspired by the multiverse scenario, we study a heterotic dark energy model in which there are two parts, the first being the cosmological constant and the second being the holographic dark energy, thus this model is named the ΛHDE model. By studying the ΛHDE model theoretically, we find that the parameters d and Ωhde are divided into a…

2015 Journal of Cosmology and Astroparticle Physics
Planck 23
Constraints from Comets on the Formation and Volatile Acquisition of the Planets and Satellites
DOI: 10.1007/s11214-015-0161-z Bibcode: 2015SSRv..197..297M

Hartogh, P.; Mousis, O.; Marty, B. +4 more

Comets play a dual role in understanding the formation and evolution of the solar system. First, the composition of comets provides information about the origin of the giant planets and their moons because comets formed early and their composition is not expected to have evolved significantly since formation. They, therefore serve as a record of c…

2015 Space Science Reviews
Rosetta 23
Explanation of a Special Color-Magnitude Diagram of Star Cluster NGC 1651 from Different Models
DOI: 10.1088/0004-637X/802/1/44 Bibcode: 2015ApJ...802...44L

Chen, Li; Li, Zhongmu; Mao, Caiyan

The color-magnitude diagram (CMD) of globular cluster NGC 1651 has special structures including a broad main sequence, an extended main sequence turn-off, and an extended red giant clump. The reason for such a special CMD remains unclear. In order to test the difference among the results from various stellar population assumptions, we study a high…

2015 The Astrophysical Journal
eHST 23
A comparative study of four significance measures for periodicity detection in astronomical surveys
DOI: 10.1093/mnras/stv719 Bibcode: 2015MNRAS.450.2052S

Holl, Berry; Rimoldini, Lorenzo; Mowlavi, Nami +8 more

We study the problem of periodicity detection in massive data sets of photometric or radial velocity time series, as presented by ESA's Gaia mission. Periodicity detection hinges on the estimation of the false alarm probability of the extremum of the periodogram of the time series. We consider the problem of its estimation with two main issues in …

2015 Monthly Notices of the Royal Astronomical Society
Gaia 23
An ionized layer in the upper atmosphere of Mars caused by dust impacts from comet Siding Spring
DOI: 10.1002/2015GL063726 Bibcode: 2015GeoRL..42.4745G

Gurnett, D. A.; Persoon, A. M.; Morgan, D. D. +4 more

We report the detection of a dense ionized layer in the upper atmosphere of Mars caused by the impact of dust from comet Siding Spring. The observations were made by the ionospheric radar sounder on the Mars Express spacecraft during two low-altitude passes approximately 7 h and 14 h after closest approach of the comet to Mars. During these passes…

2015 Geophysical Research Letters
MEx 23
Reconciling Planck cluster counts and cosmology? Chandra/XMM instrumental calibration and hydrostatic mass bias
DOI: 10.1093/mnras/stv038 Bibcode: 2015MNRAS.448..814I

Reiprich, Thomas H.; Massey, Richard; Israel, Holger +2 more

The mass of galaxy clusters can be inferred from the temperature of their X-ray-emitting gas, TX. Their masses may be underestimated if it is assumed that the gas is in hydrostatic equilibrium, by an amount bhyd ∼ (20 ± 10) per cent suggested by simulations. We have previously found consistency between a sample of observed Ch…

2015 Monthly Notices of the Royal Astronomical Society
Planck 23
How elevated is the dynamical-to-stellar mass ratio of the ultracompact dwarf S999?
DOI: 10.1093/mnras/stv389 Bibcode: 2015MNRAS.449.1716J

Janz, Joachim; Penny, Samantha J.; Forbes, Duncan A. +4 more

Here we present new Keck Echelle Spectrograph and Imager high-resolution spectroscopy and deep archival Hubble Space Telescope/Advanced Camera for Surveys imaging for S999, an ultracompact dwarf in the vicinity of M87, which was claimed to have an extremely high dynamical-to-stellar mass ratio. Our data increase the total integration times by a fa…

2015 Monthly Notices of the Royal Astronomical Society
eHST 23
History of the clay-rich unit at Mawrth Vallis, Mars: High-resolution mapping of a candidate landing site
DOI: 10.1002/2015JE004894 Bibcode: 2015JGRE..120.1820L

Mangold, N.; Bibring, J. -P.; Poulet, F. +4 more

The Mawrth Vallis region is covered by some of the largest phyllosilicate-rich outcrops on Mars, making it a unique window into the past history of Mars in terms of water alteration, potential habitability, and the search for past life. A landing ellipse had been proposed for the Curiosity rover. This area has been extensively observed by the High…

2015 Journal of Geophysical Research (Planets)
MEx 23
Constraints on the exponential f (R ) model from latest Hubble parameter measurements
DOI: 10.1103/PhysRevD.91.044019 Bibcode: 2015PhRvD..91d4019C

Geng, Chao-Qiang; Lee, Chung-Chi; Chen, Yun +2 more

We investigate the viable exponential f (R ) gravity in the metric formalism with f (R )=-β Rs(1 -e-R /Rs). The latest sample of the Hubble parameter measurements with 23 data points is used to place bounds on this f (R ) model. A joint analysis is also performed with the luminosity distances of type Ia supernovae …

2015 Physical Review D
Planck 23