activity
20152023
most citedThe K2-ESPRINT Project. I. Discovery of the Disintegrating Rocky Planet K2-22b with a Cometary Head and Leading Tail

153 citations · 900 across the 19 of their papers we have counts for

collaborators

18 papers

physics.plasm-ph2023

Kinetic-Scale Topological Structures Associated with Energy Dissipation in the Turbulent Reconnection Outflow

S. Y. Huang, J. Zhang, Q. Y. Xiong +7

Assisted with Magnetospheric Multiscale (MMS) mission capturing unprecedented high-resolution data in the terrestrial magnetotail, we apply a local streamline-topology classificati…

astro-ph.IM2023★ 22 cited

SKA Science Data Challenge 2: analysis and results

P. Hartley, A. Bonaldi, R. Braun +105

The Square Kilometre Array Observatory (SKAO) will explore the radio sky to new depths in order to conduct transformational science. SKAO data products made available to astronomer…

astro-ph.GA2022★ 5 cited

Satellite galaxies' drag on field stars in the Milky Way

Xilong Liang, Jifeng Liu, Jingkun Zhao +1

With Gaia EDR3 data, velocity dispersion of Milky Way field stars around satellite galaxies have been investigated. We have fitted velocity dispersion against distance to satellite…

astro-ph.SR2022★ 22 cited

Anisotropy of Magnetic Field Spectra at Kinetic Scales of Solar Wind Turbulence as Revealed by Parker Solar Probe in the Inner Heliosphere

S. Y. Huang, S. B. Xu, J. Zhang +11

Using the Parker Solar Probe data taken in the inner heliosphere, we investigate the power and spatial anisotropy of magnetic-field spectra at kinetic scales (i.e., around sub-ion…

physics.plasm-ph2021

Electron-only Reconnection in Ion-scale Current Sheet at the Magnetopause

S. Y. Huang, Q. Y. Xiong, L. F. Song +5

In the standard model of magnetic reconnection, both ions and electrons couple to the newly reconnected magnetic field lines and are ejected away from the reconnection diffusion re…

astro-ph.SR2021★ 21 cited

The T Tauri star V410 Tau in the eyes of SPIRou and TESS

Benjamin Finociety, Jean-François Donati, Baptiste Klein +16

We report results of a spectropolarimetric and photometric monitoring of the weak-line T Tauri star V410 Tau based on data collected mostly with SPIRou, the near-infrared (NIR) spe…

physics.space-ph2021

In Situ Detection of Kinetic-Size Magnetic Holes in the Martian Magnetosheath

S. Y. Huang, R. T. Lin, Z. G. Yuan +7

Depression in magnetic field strength with a scale below one proton gyroradius is referred to as kinetic-size magnetic hole (KSMH). KSMHs are frequently observed near terrestrial s…

physics.plasm-ph2021

Observational Evidence of Magnetic Reconnection in the Terrestrial Foreshock Region

K. Jiang, S. Y. Huang, H. S. Fu +10

Electron heating/acceleration in the foreshock, by which electrons may be energized beyond thermal energies prior to encountering the bow shock, is very important for the bow shock…

physics.space-ph2021★ 39 cited

The Ion Transition Range of Solar Wind Turbulence in the Inner Heliosphere: Parker Solar Probe Observations

S. Y. Huang, F. Sahraoui, N. Andrés +15

The scaling of the turbulent spectra provides a key measurement that allows to discriminate between different theoretical predictions of turbulence. In the solar wind, this has dri…

astro-ph.SR2021★ 36 cited

Multi-instrumental view of magnetic fields and activity of Eridani with SPIRou, NARVAL, and TESS

P. Petit, C. P. Folsom, J. -F. Donati +6

We report on observations of the active K2 dwarf Eridani based on contemporaneous SPIRou, NARVAL, and TESS data obtained over two months in late 2018, when the activity of the…

physics.space-ph2020★ 33 cited

Characteristics of Magnetic Holes in the Solar Wind Revealed by Parker Solar Probe

L. Yu, S. Y. Huang, Z. G. Yuan +6

We present a statistical analysis for the characteristics and radial evolution of linear magnetic holes (LMHs) in the solar wind from 0.166 to 0.82 AU using Parker Solar Probe obse…

astro-ph.IM2020★ 53 cited

Square Kilometre Array Science Data Challenge 1: analysis and results

A. Bonaldi, T. An, M. Bruggen +42

As the largest radio telescope in the world, the Square Kilometre Array (SKA) will lead the next generation of radio astronomy. The feats of engineering required to construct the t…

physics.space-ph2020★ 52 cited

Kinetic Scale Slow Solar Wind Turbulence in the Inner Heliosphere: Co-existence of Kinetic Alfvén Waves and Alfvén Ion Cyclotron Waves

S. Y. Huang, J. Zhang, F. Sahraoui +12

The nature of the plasma wave modes around the ion kinetic scales in highly Alfvénic slow solar wind turbulence is investigated using data from the NASA's Parker Solar Probe taken…

astro-ph.EP2018★ 6 cited

HATS-71b: A giant planet transiting an M3 dwarf star in TESS Sector 1

G. Á. Bakos, D. Bayliss, J. Bento +41

We report the discovery of HATS-71b, a transiting gas giant planet on a P = 3.7955 day orbit around a G = 15.35 mag M3 dwarf star. HATS-71 is the coolest M dwarf star known to host…

astro-ph.SR2017★ 95 cited

A hot Jupiter around the very active weak-line T Tauri star TAP 26

L. Yu, J. -F. Donati, E. M. Hébrard +17

We report the results of an extended spectropolarimetric and photometric monitoring of the weak-line T Tauri star TAP 26, carried out within the MaTYSSE programme with the ESPaDOnS…

astro-ph.SR2016★ 63 cited

The hot Jupiter of the magnetically-active weak-line T Tauri star V830 Tau

J. -F. Donati, L. Yu, C. Moutou +16

We report results of an extended spectropolarimetric and photometric monitoring of the weak-line T Tauri star V830 Tau and its recently-detected newborn close-in giant planet. Our…

astro-ph.SR2016★ 150 cited

A hot Jupiter orbiting a 2-Myr-old solar-mass T Tauri star

JF Donati, C Moutou, L Malo +11

Hot Jupiters are giant Jupiter-like exoplanets that orbit 100x closer to their host stars than Jupiter does to the Sun. These planets presumably form in the outer part of the primo…

astro-ph.EP2015★ 153 cited

The K2-ESPRINT Project. I. Discovery of the Disintegrating Rocky Planet K2-22b with a Cometary Head and Leading Tail

R. Sanchis-Ojeda, S. Rappaport, E. Pallé +28

We present the discovery of a transiting exoplanet candidate in the K2 Field-1 with an orbital period of 9.1457 hr: K2-22b. The highly variable transit depths, ranging from 0…