activity
20102024
most citedThe clustering of massive galaxies at z~0.5 from the first semester of BOSS data

281 citations · 532 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.SR2024★ 11 cited

A spectroscopic and kinematic survey of fast hot subdwarfs

S. Geier, U. Heber, A. Irrgang +19

Hot subdwarfs (sdO/B) are the stripped helium cores of red giants formed by binary interactions. Close hot subdwarf binaries with massive white dwarf companions have been proposed…

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.SR2021★ 38 cited

Discovery of a double detonation thermonuclear supernova progenitor

Thomas Kupfer, Evan B. Bauer, Jan van Roestel +12

We present the discovery of a new double detonation progenitor system consisting of a hot subdwarf B (sdB) binary with a white dwarf companion with an P=76.34179(2) min orbital per…

astro-ph.SR2021★ 66 cited

A hot subdwarf-white dwarf super-Chandrasekhar candidate supernova Ia progenitor

Ingrid Pelisoli, P. Neunteufel, S. Geier +8

Supernova Ia are bright explosive events that can be used to estimate cosmological distances, allowing us to study the expansion of the Universe. They are understood to result from…

astro-ph.SR2020★ 37 cited

A quantitative in-depth analysis of the prototype sdB+BD system SDSS J08205+0008 revisited in the Gaia era

V. Schaffenroth, S. L. Casewell, D. Schneider +8

Subdwarf B stars are core-helium burning stars located on the extreme horizontal branch. Extensive mass loss on the red giant branch is necessary to form them. It has been proposed…

astro-ph.SR2020★ 3 cited

Runaway blue main-sequence stars at high Galactic latitudes. Target selection with Gaia and spectroscopic identification

Roberto Raddi, Andreas Irrgang, Ulrich Heber +2

Motivated by the historical identification of runaway main-sequence (MS) stars of early spectral type at high Galactic latitudes, we test the capability of Gaia at identifying new…

astro-ph.SR2020★ 12 cited

EVR-CB-004: An Inflated Hot Subdwarf O star + Unseen WD Companion in a Compact Binary Discovered with the Evryscope

Jeffrey K. Ratzloff, Thomas Kupfer, Brad N. Barlow +10

We present the discovery of EVR-CB-004, a close binary with a remnant stellar core and an unseen white dwarf companion. The analysis in this work reveals the primary is potentially…

astro-ph.SR2020★ 50 cited

A new class of Roche lobe-filling hot subdwarf binaries

Thomas Kupfer, Evan B. Bauer, Kevin B. Burdge +30

We present the discovery of the second binary with a Roche lobe-filling hot subdwarf transferring mass to a white dwarf (WD) companion. This 56 minute binary was discovered using d…

astro-ph.SR2018★ 11 cited

NLTE spectroscopic analysis of the He anomaly in subluminous B-type stars

D. Schneider, A. Irrgang, U. Heber +2

Several B-type main-sequence stars show chemical peculiarities. A particularly striking class are the He stars, which exhibit a remarkable enrichment of He with respect to…

astro-ph.SR2018★ 22 cited

The MUCHFUSS photometric campaign

V. Schaffenroth, S. Geier, U. Heber +4

Hot subdwarfs (sdO/Bs) are the helium-burning cores of red giants, which lost almost all of their hydrogen envelopes. This mass loss is often triggered by common envelope interacti…

astro-ph.SR2014★ 1 cited

The mysterious sdO X-ray binary BD+37 442

U. Heber, S. Geier, A. Irrgang +4

Pulsed X-ray emission in the luminous, helium-rich sdO BD+37 442 has recently been discovered (La Palombara et al., 2012). It was suggested that the sdO star has a neutron star or…

astro-ph.CO2010★ 281 cited

The clustering of massive galaxies at z~0.5 from the first semester of BOSS data

Martin White, M. Blanton, A. Bolton +25

We calculate the real- and redshift-space clustering of massive galaxies at z~0.5 using the first semester of data by the Baryon Oscillation Spectroscopic Survey (BOSS). We study t…