activity
20012023
most citedHAT-P-39b--HAT-P-41b: Three Highly Inflated Transiting Hot Jupiters

136 citations · 544 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.EP2023

Direct images and spectroscopy of a giant protoplanet driving spiral arms in MWC 758

Kevin Wagner, Jordan Stone, Andrew Skemer +23

Understanding the driving forces behind spiral arms in protoplanetary disks remains a challenge due to the faintness of young giant planets. MWC 758 hosts such a protoplanetary dis…

astro-ph.IM2018

Hi-5: a potential high-contrast thermal near-infrared imager for the VLTI

D. Defrère, M. Ireland, O. Absil +25

Hi-5 is a high-contrast (or high dynamic range) infrared imager project for the VLTI. Its main goal is to characterize young extra-solar planetary systems and exozodiacal dust arou…

astro-ph.CO2018★ 37 cited

Probing the origin of extragalactic magnetic fields with Fast Radio Bursts

F. Vazza, M. Brüggen, P. M. Hinz +3

The joint analysis of the Dispersion and Faraday Rotation Measure from distant, polarised Fast Radio Bursts may be used to put constraints on the origin and distribution of extraga…

astro-ph.CO2017★ 129 cited

Simulations of extragalactic magnetic fields and of their observables

F. Vazza, M. Brüggen, C. Gheller +3

The origin of extragalactic magnetic fields is still poorly understood. Based on a dedicated suite of cosmological magneto-hydrodynamical simulations with the ENZO code we have per…

astro-ph.SR2017★ 10 cited

Improved Constraints on the Disk Around MWC 349A from the 23-Meter LBTI

Steph Sallum, Josh Eisner, Phil Hinz +4

We present new spatially resolved observations of MWC 349A from the Large Binocular Telescope Interferometer (LBTI), a 23-meter baseline interferometer made up of two, co-mounted 8…

astro-ph.EP2017★ 47 cited

HAT-P-67b: An Extremely Low Density Saturn Transiting an F-Subgiant Confirmed via Doppler Tomography

G. Zhou, G. Á. Bakos, J. D. Hartman +29

We report the discovery of HAT-P-67b, a hot-Saturn transiting a rapidly rotating F-subgiant. HAT-P-67b has a radius of Rp = 2.085 -0.071/+0.096 RJ,, orbiting a M* = 1.642 -0.072/+0…