activity
20132025
most citedThe Detailed Science Case for the Maunakea Spectroscopic Explorer, 2019 edition

37 citations · 112 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.SR2025★ 4 cited

Photometric study of hot Algol-type binaries with long cycles

J. Garcés, R. E. Mennickent, J. Petrovíc +6

Double periodic variables (DPVs) are hot Algol-type interacting binary systems with an orbital and a long photometric cycle. The origin of the latter may be related to cyclic struc…

astro-ph.SR2025

The vanishing of the long photometric cycle in AU Monocerotis

L. Celedón, R. E. Mennickent, D. Barría +2

Double periodic variables (DPVs) are a group of semi-detached interacting binaries that exhibit a long photometric cycle with an average length of times the orbital period…

astro-ph.SR2024★ 6 cited

Non-thermal radio emission in Sakurai's Object

Marcin Hajduk, Peter A. M. van Hoof, Albert A. Zijlstra +5

The very late thermal pulse (VLTP) affects the evolution of 20\% of 1--8\, stars, repeating the last phases of the red giant within a few years and leading t…

astro-ph.IM2019★ 37 cited

The Detailed Science Case for the Maunakea Spectroscopic Explorer, 2019 edition

The MSE Science Team, Carine Babusiaux, Maria Bergemann +258

(Abridged) The Maunakea Spectroscopic Explorer (MSE) is an end-to-end science platform for the design, execution and scientific exploitation of spectroscopic surveys. It will unvei…

astro-ph.SR2019★ 1 cited

Stellar Astrophysics and Exoplanet Science with the Maunakea Spectroscopic Explorer (MSE)

Maria Bergemann, Daniel Huber, Vardan Adibekyan +70

The Maunakea Spectroscopic Explorer (MSE) is a planned 11.25-m aperture facility with a 1.5 square degree field of view that will be fully dedicated to multi-object spectroscopy. A…

astro-ph.SR2018★ 9 cited

The planetary nebula IC 5148 and its ionized halo

D. Barría, S. Kimeswenger, W. Kausch +1

Many round or nearly roundish Planetary Nebulae (PNe) show multiple shells and halo structures during their evolutionary stage near the maximum temperature of their central star. C…