activity
20232026
most citedThe BlackGEM telescope array I: Overview

33 citations · 40 across the 4 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2026

A 500 pc volume-limited sample of hot subluminous stars III. The short-period binary population

H. Dawson, M. Dorsch, J. Munday +16

Hot subdwarf stars of spectral types O and B (sdO/B) in binaries form as products of substantial mass loss near the tip of the red giant branch and offer powerful constraints on bi…

astro-ph.SR2026★ 7 cited

A 500 pc volume-limited sample of hot subluminous stars II. Atmospheric parameters, mass distribution, and kinematics

H. Dawson, M. Dorsch, S. Geier +30

We present a quantitative spectroscopic and kinematic analysis of a volume-complete sample of hot subluminous stars within 500 pc of the Sun, assembled using accurate parallax meas…

astro-ph.SR2025

Volume-limited sample of low-mass red giant stars, the progenitors of hot subdwarf stars II. Sample validation

Diego Benitez-Palacios, Murat Uzundag, Maja Vučković +6

We investigate the progenitors of long-period hot subdwarf B (sdB) binaries, which form when low-mass red giant branch (RGB) stars lose their envelopes through stable Roche lobe ov…

astro-ph.IM2024★ 33 cited

The BlackGEM telescope array I: Overview

Paul J. Groot, S. Bloemen, P. Vreeswijk +75

The main science aim of the BlackGEM array is to detect optical counterparts to gravitational wave mergers. Additionally, the array will perform a set of synoptic surveys to detect…

astro-ph.SR2023

The mass range of hot subdwarf B stars from MESA simulations

Eduardo Arancibia-Rojas, Monica Zorotovic, Maja Vučković +3

Hot subdwarf B (sdB) stars are helium core burning stars that have lost almost their entire hydrogen envelope due to binary interaction. Their assumed canonical mass of $\rm M_{\ma…