activity
20232026
most citedThe BlackGEM telescope array I: Overview

33 citations · 77 across the 15 of their papers we have counts for

collaborators

18 papers

astro-ph.SR2026

Intermediate-mass runaway and hypervelocity star candidates in DESI DR1

Aakash Bhat, Matti Dorsch, Ulrich Heber +2

Runaway stars ejected from the Galactic disc span a range of velocities, with two extreme regimes of particular interest. Hyper-runaway stars reach velocities approaching the local…

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

Toward 3D orbits of wide sdO/B binaries I. Six composite systems spatially resolved with VLTI/GRAVITY

K. Deshmukh, S. Geier, H. Sana +7

Hot subdwarf stars (sdO/Bs) are widely considered to be products of binary evolution. A significant fraction of them are found in long-period or wide binaries ( d) with main…

astro-ph.SR2026

V407 Vul: a triple star system with an AM CVn detectable by gravitational wave observatories

James Munday, Antonio C. Rodriguez, Nicole Reindl +23

The AM CVn class includes mass transferring, ultra-compact double white dwarf binaries with orbital periods on the timescale of minutes. A long-standing puzzle is that none of the…

astro-ph.SR2026★ 1 cited

Stars on the ascending helium giant branch I. From white dwarf merger to helium giant: the evolutionary state of the rapidly rotating hot subdwarf HE 1518-0948

M. Pritzkuleit, M. Dorsch, M. M. Miller Bertolami +3

Hot subdwarf stars with masses above ascend the helium giant branch after the end of core helium burning, before entering the white dwarf cooling track or exploding a…

astro-ph.SR2026★ 3 cited

Hot subdwarf stars from the Hamburg Quasar Survey

Ulrich Heber, Lennard Kufleitner, Matti Dorsch +4

Hot subluminous stars (sdO/B) are evolved low mass stars originating from red giants that lost their envelope almost entirely. The multitude of observed phenomena imply that severa…

astro-ph.SR2026

The massive hot subdwarf binary LAMOST J065816.72+094343.1

F. Mattig, B. N. Barlow, D. Liu +9

Massive short-period binaries involving hot subdwarf stars (sdO/Bs) are rare but important to constraining pathways for binary star evolution. Moreover, some of the most promising…

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.IM2025

The ORCA-TWIN qCMOS Experiment I. Science case and commissioning at Calar Alto Observatory

Martin M. Roth, Pasko Roje, Stella Vjesnica +18

We describe a pilot study to explore a new generation of fast and low noise CMOS image sensors for time domain astronomy, using two remote telescopes with a baseline of 1635 km. Th…

astro-ph.SR2025

The twin red giant branch system BD+20 5391 A case study of low-mass double-core evolution

M. Kurpas, M. Dorsch, S. Geier +12

Understanding interactions of binary systems on the red giant branch is crucial to understanding the formation of compact stellar remnants such as helium-core white dwarfs (He-WDs)…

astro-ph.SR2025★ 4 cited

Where are the binaries? -- Searching for blue horizontal-branch stars in binary systems in the inner Galactic Halo

R. Culpan, M. Dorsch, I. Pelisoli +14

Blue horizontal-branch (BHB) stars are evolved low-mass objects that have completed their core hydrogen burning main-sequence (MS) stage and have lost significant mass during the r…

astro-ph.SR2025★ 1 cited

Ancient, eclipsing, tidally-locked: A blue lurker progenitor in the population of extreme-velocity star candidates

A. Bhat, M. Dorsch, S. Geier +5

Many extreme velocity candidate stars have been found based on \textit{Gaia} astrometry, but need spectroscopic confirmation. We select late-type hypervelocity star (HVS) candidate…

astro-ph.SR2025

The DBL Survey II: towards a mass-period distribution of double white dwarf binaries

James Munday, Ingrid Pelisoli, Pier-Emmanuel Tremblay +14

Double white dwarf binaries are an important remnant of binary evolution as they are possible type Ia supernova progenitors and strong sources of gravitational waves in the low-fre…

astro-ph.SR2024

The DBL Survey I: discovery of 34 double-lined double white dwarf binaries

James Munday, Ingrid Pelisoli, P. E. Tremblay +8

We present the first discoveries of the double-lined double white dwarf (DBL) survey that targets over-luminous sources with respect to the canonical white dwarf cooling sequence a…

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.SR2024

A 500 pc volume-limited sample of hot subluminous stars I. Space density, scale height, and population properties

H. Dawson, S. Geier, U. Heber +25

We present the first volume-limited sample of spectroscopically confirmed hot subluminous stars out to 500 pc, defined using the accurate parallax measurements from the {\em Gaia}…

astro-ph.SR2023★ 19 cited

The bright blue side of the night sky: Spectroscopic survey of bright and hot (pre-) white dwarfs

Nicole Reindl, Ramazan Islami, Klaus Werner +10

We report on the spectroscopic confirmation of 68 new bright ( mag) and blue (pre-)white dwarfs (WDs). This finding has allowed us to almost double the number of the h…

astro-ph.SR2023★ 9 cited

The first massive compact companion in a wide orbit around a hot subdwarf star

S. Geier, M. Dorsch, H. Dawson +5

We report the discovery of the first hot subdwarf B (sdB) star with a massive compact companion in a wide () binary system. It was discovered based on an a…