activity
20102020
most citedAstrometric follow-up observations of directly imaged sub-stellar companions to young stars and brown dwarfs

73 citations · 575 across the 25 of their papers we have counts for

collaborators

24 papers

astro-ph.IM2020★ 1 cited

A small actively-controlled high-resolution spectrograph based on off-the-shelf components

H. R. A. Jones, W. E. Martin, G. Anglada-Escudé +5

We present the design and testing of a prototype in-plane echelle spectrograph based on an actively controlled fibre-fed double-pass design. This system aims to be small and effici…

astro-ph.IM2020★ 10 cited

HiFLEx -- a highly flexible package to reduce cross-dispersed echelle spectra

Ronny Errmann, Neil Cook, Guillem Anglada-Escudé +8

We describe a flexible data reduction package for high resolution cross-dispersed echelle data. This open-source package is developed in Python and includes optional GUIs for most…

astro-ph.SR2019★ 8 cited

Diagnosing the Clumpy Protoplanetary Disk of the UXor Type Young Star GM Cephei

P. C. Huang, W. P. Chen, M. Mugrauer +29

UX Orionis stars (UXors) are Herbig Ae/Be or T Tauri stars exhibiting sporadic occultation of stellar light by circumstellar dust. GM\,Cephei is such a UXor in the young (~M…

astro-ph.EP2017★ 14 cited

280 one-opposition near-Earth asteroids recovered by the EURONEAR with the Isaac Newton Telescope

O. Vaduvescu, L. Hudin, T. Mocnik +80

One-opposition near-Earth asteroids (NEAs) are growing in number, and they must be recovered to prevent loss and mismatch risk, and to improve their orbits, as they are likely to b…

astro-ph.SR2016★ 13 cited

Long-Term Photometry of IC 348 with the YETI Network

D. J. Fritzewski, M. Kitze, M. Mugrauer +29

We present long-term photometric observations of the young open cluster IC 348 with a baseline time-scale of 2.4 yr. Our study was conducted with several telescopes from the Young…

astro-ph.EP2016★ 18 cited

YETI observations of the young transiting planet candidate CVSO 30 b

St. Raetz, T. O. B. Schmidt, S. Czesla +32

CVSO 30 is a unique young low-mass system, because, for the first time, a close-in transiting and a wide directly imaged planet candidates are found around a common host star. The…