Search Publications

Energetic Electron Periodicities During the Cassini Grand Finale
DOI: 10.1002/2017JA024836 Bibcode: 2017JGRA..12212229C

Krupp, N.; Roussos, E.; Mitchell, D. G. +2 more

The Cassini F ring and Proximal orbits took the spacecraft closer to Saturn than any previous mission and allowed determination of energetic charged particles (E > 20 keV) in the inner magnetosphere of the planet. The periodicities of the energetic electrons show a remarkable consistency when analyzed using Lomb periodograms. From the beginning…

2017 Journal of Geophysical Research (Space Physics)
Cassini 5
Cross-calibration of the Rosetta Navigation Camera based on images of the 67P comet nucleus
DOI: 10.1093/mnras/stx1589 Bibcode: 2017MNRAS.469S.285S

Statella, Thiago; Geiger, Bernhard

The Rosetta spacecraft carried a Navigation Camera (NavCam) for optical navigation in the vicinity of the comet. In order to facilitate the use of the data for quantitative scientific work, we performed a cross-calibration study based on images taken with the OSIRIS near-angle camera. For this purpose, we selected sets of images acquired roughly s…

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 5
The amplitude of the cross-covariance function of solar oscillations as a diagnostic tool for wave attenuation and geometrical spreading
DOI: 10.1051/0004-6361/201629846 Bibcode: 2017A&A...599A.111N

Gizon, Laurent; Birch, Aaron C.; Nagashima, Kaori +1 more

Context. In time-distance helioseismology, wave travel times are measured from the two-point cross-covariance function of solar oscillations and are used to image the solar convection zone in three dimensions. There is, however, also information in the amplitude of the cross-covariance function, for example, about seismic wave attenuation.
Ai…

2017 Astronomy and Astrophysics
SOHO 5
On the Relation of Silicates and SiO Maser in Evolved Stars
DOI: 10.3847/1538-3881/aa6334 Bibcode: 2017AJ....153..176L

Jiang, Biwei; Liu, Jiaming

The SiO molecule is one of the candidates for the seed of silicate dust in the circumstellar envelope of evolved stars, but this opinion is challenged. In this work we investigate the relation of the SiO maser emission power and the silicate dust emission power. With both our own observation by using the PMO/Delingha 13.7 m telescope and archive d…

2017 The Astronomical Journal
ISO 5
A Bayesian Approach to Period Searching in Solar Coronal Loops
DOI: 10.3847/1538-4357/aa5d59 Bibcode: 2017ApJ...837...24S

McKenzie, David; Scherrer, Bryan

We have applied a Bayesian generalized Lomb-Scargle period searching algorithm to movies of coronal loop images obtained with the Hinode X-ray Telescope (XRT) to search for evidence of periodicities that would indicate resonant heating of the loops. The algorithm makes as its only assumption that there is a single sinusoidal signal within each lig…

2017 The Astrophysical Journal
Hinode 5
Discovery of a Rapid, Luminous Nova in NGC 300 by the KMTNet Supernova Program
DOI: 10.3847/1538-4357/aa706b Bibcode: 2017ApJ...844..160A

Kim, Dong-Jin; Lee, Yongseok; Moon, Dae-Sik +3 more

We present the discovery of a rapidly evolving transient by the Korean Microlensing Telescope Network Supernova Program (KSP). KSP is a novel high-cadence supernova survey that offers deep (∼21.5 mag in BV I bands), nearly continuous wide-field monitoring for the discovery of early and/or fast optical transients. KSP-OT-201509a, reported here, was…

2017 The Astrophysical Journal
eHST 5
General circulation of Venus from a long-term synoptic study of tropospheric CO by Venus Express/VIRTIS
DOI: 10.1016/j.icarus.2017.02.018 Bibcode: 2017Icar..289..173T

Tsang, Constantine C. C.; McGouldrick, Kevin

The understanding of spatial and temporal variations in tropospheric abundances of the trace gas carbon monoxide (CO) is key to understanding the deep atmospheric circulation on Venus. CO is entrained in the global circulation, as well as being key ingredients in the multi-reaction chemical cycle that creates and destroys the sulfuric acid that is…

2017 Icarus
VenusExpress 5
Inferring Compton-thick AGN candidates at z > 2 with Chandra using the >8 keV rest-frame spectral curvature
DOI: 10.1093/mnras/stx1561 Bibcode: 2017MNRAS.471..364B

Treister, E.; Salvato, M.; Comastri, A. +10 more

To fully understand cosmic black hole growth, we need to constrain the population of heavily obscured active galactic nuclei (AGNs) at the peak of cosmic black hole growth (z ∼1-3). Sources with obscuring column densities higher than 1024 atoms cm-2, called Compton-thick (CT) AGNs, can be identified by excess X-ray emission a…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 5
Regional surface morphology of comet 67P/Churyumov-Gerasimenko from Rosetta/OSIRIS images: The southern hemisphere (Corrigendum)
DOI: 10.1051/0004-6361/201628634e Bibcode: 2017A&A...598C...2E

Jorda, L.; Lamy, P. L.; Lara, L. M. +49 more

2017 Astronomy and Astrophysics
Rosetta 5
CARMA observations of massive Planck -discovered cluster candidates at z ≳ 0.5 associated with WISE overdensities: breaking the size-flux degeneracy
DOI: 10.1093/mnras/stw2392 Bibcode: 2017MNRAS.464.2378R

Shimwell, T.; Melin, J. -B.; Feroz, F. +4 more

We use a Bayesian software package to analyse CARMA-8 data towards 19 unconfirmed Planck Sunyaev-Zel'dovich-cluster candidates from Rodríguez-Gonzálvez et al. that are associated with significant overdensities in WISE. We use two cluster parameterizations, one based on a (fixed shape) generalized-NFW (gNFW) pressure profile and another on a β gas …

2017 Monthly Notices of the Royal Astronomical Society
Planck 5