Search Publications

The Time-Dependent Wavelet Spectrum of HH 1 and 2
Bibcode: 2018RMxAA..54..195R

Raga, A. C.; Esquivel, A.; Riera, A. +2 more

We have calculated the wavelet spectra of four epochs (spanning ≈20 yr) of Hα and [S II] HST images of HH 1 and 2. From these spectra we calculated the distribution functions of the (angular) radii of the emission structures. We found that the size distributions have maxima (corresponding to the characteristic sizes of the observed structures) wit…

2018 Revista Mexicana de Astronomia y Astrofisica
eHST 0
A two-fluid modeling of kinetic Alfvén wave turbulence
DOI: 10.1007/s10509-018-3427-6 Bibcode: 2018Ap&SS.363..204K

Moon, Y. -J.; Sharma, R. P.; Dwivedi, Navin Kumar +1 more

We present an analytical model to explore the magnetic field turbulent spectrum by coupled high-frequency kinetic Alfvén wave (KAW) and slow mode of Alfvén wave (AW). The spectrum is computed as a realization of energy cascades from larger to smaller scales for a specific case of solar wind plasma at 1 AU. A two-fluid technique is implemented for …

2018 Astrophysics and Space Science
Cluster 0
Hinode Observation of the Sun's Polar Magnetic Field and Solar Cycle Variation
DOI: 10.1007/978-981-10-7742-5_16 Bibcode: 2018ASSL..449..173S

Shiota, Daikou

2018 First Ten Years of Hinode Solar On-Orbit Observatory
Hinode 0
The Largest Electron Differential Energy Flux Observed at Mars by the Mars Express Spacecraft, 2004-2016
DOI: 10.1029/2018JA025311 Bibcode: 2018JGRA..123.6576F

Coates, A. J.; Barabash, S.; Holmström, M. +3 more

The goal of this paper is to understand the processes by which solar wind electrons are energized in the Martian magnetosphere and how this compares to processes at Venus and Earth. Each is unique in the source of its magnetic field topology and how this influences electron energization. To achieve this goal, 24 million spectra spanning 13 years h…

2018 Journal of Geophysical Research (Space Physics)
MEx VenusExpress 0
Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
DOI: 10.3847/2041-8213/aa920c Bibcode: 2017ApJ...848L..13A

Lee, H. M.; Williams, D.; Mitra, S. +1153 more

On 2017 August 17, the gravitational-wave event GW170817 was observed by the Advanced LIGO and Virgo detectors, and the gamma-ray burst (GRB) GRB 170817A was observed independently by the Fermi Gamma-ray Burst Monitor, and the Anti-Coincidence Shield for the Spectrometer for the International Gamma-Ray Astrophysics Laboratory. The probability of t…

2017 The Astrophysical Journal
INTEGRAL 2962
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
DOI: 10.1093/mnras/stx721 Bibcode: 2017MNRAS.470.2617A

Petitjean, Patrick; Ross, Nicholas P.; Bailey, Stephen +70 more

We present cosmological results from the final galaxy clustering data set of the Baryon Oscillation Spectroscopic Survey, part of the Sloan Digital Sky Survey III. Our combined galaxy sample comprises 1.2 million massive galaxies over an effective area of 9329 deg2 and volume of 18.7 Gpc3, divided into three partially overlap…

2017 Monthly Notices of the Royal Astronomical Society
Planck 2664
The 2017 Release Cloudy
DOI: 10.48550/arXiv.1705.10877 Bibcode: 2017RMxAA..53..385F

Abel, N. P.; Keenan, F. P.; Ferland, G. J. +8 more

We describe the 2017 release of the spectral synthesis code Cloudy, summarizing the many improvements to the scope and accuracy of the physics which have been made since the previous release. Exporting the atomic data into external data files has enabled many new large datasets to be incorporated into the code. The use of the complete datasets is …

2017 Revista Mexicana de Astronomia y Astrofisica
XMM-Newton 1377
Swope Supernova Survey 2017a (SSS17a), the optical counterpart to a gravitational wave source
DOI: 10.1126/science.aap9811 Bibcode: 2017Sci...358.1556C

Rest, A.; Foley, R. J.; Shappee, B. J. +14 more

On 17 August 2017, the Laser Interferometer Gravitational-Wave Observatory (LIGO) and the Virgo interferometer detected gravitational waves (GWs) emanating from a binary neutron star merger, GW170817. Nearly simultaneously, the Fermi and INTEGRAL (INTErnational Gamma-Ray Astrophysics Laboratory) telescopes detected a gamma-ray transient, GRB 17081…

2017 Science
eHST 995
KiDS-450: cosmological parameter constraints from tomographic weak gravitational lensing
DOI: 10.1093/mnras/stw2805 Bibcode: 2017MNRAS.465.1454H

Simon, P.; Heymans, C.; Choi, A. +33 more

We present cosmological parameter constraints from a tomographic weak gravitational lensing analysis of ∼450 deg2 of imaging data from the Kilo Degree Survey (KiDS). For a flat Λ cold dark matter (ΛCDM) cosmology with a prior on H0 that encompasses the most recent direct measurements, we find S_8≡ σ _8√{Ω _m/0.3}=0.745± 0.039…

2017 Monthly Notices of the Royal Astronomical Society
Planck 899
The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. II. UV, Optical, and Near-infrared Light Curves and Comparison to Kilonova Models
DOI: 10.3847/2041-8213/aa8fc7 Bibcode: 2017ApJ...848L..17C

Fryer, C. L.; Berger, E.; Benoit-Lévy, A. +141 more

We present UV, optical, and near-infrared (NIR) photometry of the first electromagnetic counterpart to a gravitational wave source from Advanced Laser Interferometer Gravitational-wave Observatory (LIGO)/Virgo, the binary neutron star merger GW170817. Our data set extends from the discovery of the optical counterpart at 0.47-18.5 days post-merger,…

2017 The Astrophysical Journal
eHST 783