Search Publications

Observations of Solar Type III radio bursts by Cassini/RPWS experiment
DOI: 10.5194/ars-18-83-2020 Bibcode: 2020AdRS...18...83B

Boudjada, Mohammed Y.; Abou el-Fadl, Ahmed; Galopeau, Patrick H. M. +2 more

In this study, we report on the occurrence of solar Type III radio bursts recorded by radio and plasma wave experiment (RPWS) experiment onboard Cassini spacecraft. This instrument is designed to investigate the Saturn's plasma environment and sub-auroral radio missions. RPWS/Cassini experiment allows to measure electric field over a frequency ran…

2020 Advances in Radio Science
Cassini 2
Overtaking collisions of double layers and solitons: Tripolar structures and dynamical polarity switches
DOI: 10.1063/5.0003493 Bibcode: 2020PhPl...27f2303O

Olivier, C. P.; Verheest, F.

Overtaking collisions between double layers and solitons are investigated through the numerical simulation of the Gardner equation that governs small-amplitude double layers. The results show that the double layer emerges unaffected after the completion of the collision. However, the soliton that emerges from the collision has the opposite polarit…

2020 Physics of Plasmas
Cluster 2
Orbital Refinement and Stellar Properties for the HD 9446, HD 43691, and HD 179079 Planetary Systems
DOI: 10.3847/1538-3881/ab7d33 Bibcode: 2020AJ....159..197H

Henry, Gregory W.; Kane, Stephen R.; Pepper, Joshua +15 more

The Transit Ephemeris Refinement and Monitoring Survey is a project that aims to detect transits of intermediate-long period planets by refining orbital parameters of the known radial velocity planets using additional data from ground-based telescopes, calculating a revised transit ephemeris for the planet, then monitoring the planet host star dur…

2020 The Astronomical Journal
Gaia 2
Re-reduction of CCD observations of Triton in 1996-2006 with Gaia DR2 and comparison with ephemerides
DOI: 10.1016/j.icarus.2020.113662 Bibcode: 2020Icar..34313662Y

Cheng, X.; Yan, D.; Qiao, R. C. +1 more

The release of new high-precision and high-density catalogue Gaia DR2 brings new opportunities and challenges to high-precision astrometry. The early CCD images of planet satellites can be re-processed so as to give positions that are much more accurate than those initially obtained. Based on Gaia DR2 catalogue, the early CCD images of Triton take…

2020 Icarus
Gaia 2
CCD UBV(RI)KC photometry of the open clusters Juchert 9 and Berkeley 97
DOI: 10.1002/asna.202013647 Bibcode: 2020AN....341...44O

Sung, Hwankyung; Oralhan, İnci Akkaya; Çakmak, Hikmet +3 more

The CCD UBV(RI)KC photometry of the poorly studied open clusters Juchert 9 (Juc 9) and Berkeley 97 (Be 97), which are observed with the 0.84 m telescope at the San Pedro Mártir National Observatory, México has been analyzed. For the likely cluster members, we determined the reddenings, E(B‑V) = 0.82 ± 0.04 (Juc 9) and E(B‑V) = 0.87 ± 0.05 (Be 97),…

2020 Astronomische Nachrichten
Gaia 2
Mixed-morphology supernova remnants: the case of SNR 0520-69.4 in the Large Magellanic Cloud
DOI: 10.1093/mnras/staa3138 Bibcode: 2020MNRAS.499.4213R

Rosado, M.; Reyes-Iturbide, J.; Ramírez-Ballinas, I. +2 more

We present observations in X-ray and optical emission of the supernova remnant (SNR) 0520-69.4 in the Large Magellanic Cloud. Using XMM-Newton observatory data, we produced images of the diffuse X-ray emission and spectra to obtain the X-ray parameters, such as luminosity and temperature, of hot plasma in the SNR. Diffuse X-ray emission with fille…

2020 Monthly Notices of the Royal Astronomical Society
XMM-Newton 2
A GPU-based phase tracking method for planetary radio science applications
DOI: 10.1088/1361-6501/ab58e5 Bibcode: 2020MeScT..31d5902J

Yan, Jianguo; Barriot, Jean-Pierre; Wang, Guangli +3 more

This paper introduces a phase tracking method with a computational algorithm for planetary radio science implemented on NVIDIA GPUs. In contrast to the phase-locked loop phase counting method used in traditional Doppler data processing, this method fits the tracking data with optimal parameters into the shape expressed by Taylor expansion. The dif…

2020 Measurement Science and Technology
MEx 2
Astrometric observations of visual binaries using 26‑inch refractor at Pulkovo Observatory during 2014–2019
DOI: 10.1002/asna.202013815 Bibcode: 2020AN....341..762I

Izmailov, Igor; Rublevsky, Aleksey; Apetyan, Arina

We present 18,365 astrometric observations of 290 visual binaries obtained with the 26‑inch refractor of Pulkovo Observatory during 2014–2019. The separation between components is from 1″.3 to 37″ with a median value of 4″.8. For a single observation, the mean separation error is 0″.013, and the mean position angle error is 0∘.44/ρ, where ρ is an …

2020 Astronomische Nachrichten
Gaia 2
Open Cluster IC 1369 and Its Vicinity: Multicolor Photometry and Gaia DR2 Astrometry
DOI: 10.3847/1538-3881/ab67b5 Bibcode: 2020AJ....159...95S

Straižys, V.; Raudeliūnas, S.; Maskoliūnas, M. +9 more

The open cluster IC 1369, located in Cygnus close to the galactic equator at the 89°6 longitude, and its vicinity are investigated by applying two-dimensional photometric classification of stars down to V = 19 mag measured in the Vilnius seven-color photometric system. Employing the Gaia DR2 coordinates, parallaxes, and proper motions, 143 cluster…

2020 The Astronomical Journal
Gaia 2
Characteristics of SEPs during solar cycles 21–24
DOI: 10.1007/s12036-020-9624-z Bibcode: 2020JApA...41....7K

Kumar, Raj; Pande, Bimal; Pande, Seema +1 more

The study of the solar energetic particle events (SEPs) and their association with solar flares and other activities are very crucial to understand the space weather. Keeping this in view, here we present the study of SEPs (intensity 10

2020 Journal of Astrophysics and Astronomy
SOHO 2