activity
20152018
most citedStellar laboratories. VI. New Mo IV - VII oscillator strengths and the molybdenum abundance in the hot white dwarfs G191-B2B and RE0503-289

33 citations · 101 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2018★ 15 cited

Stellar parameters for the central star of the planetary nebula PRTM 1 using the German Astrophysical Virtual Observatory service TheoSSA

T. Rauch, M. Demleitner, D. Hoyer +1

The German Astrophysical Virtual Observatory (GAVO) developed the registered service TheoSSA (theoretical stellar spectra access) and the supporting registered VO tool TMAW (Tuebin…

astro-ph.IM2016

All of the Sky: HEALPix Density Maps of Gaia-scale Datasets from the Database to the Desktop

M. B. Taylor, G. Mantelet, M. Demleitner

The Gaia Archive provides access to observations of around a billion sky sources. The primary access to this archive is via TAP services such as GACS and ARI-Gaia, which allow exec…

physics.atom-ph2016★ 27 cited

Stellar laboratories. VIII. New Zr IV - VII, Xe IV - V, and Xe VII oscillator strengths and the Al, Zr, and Xe abundances in the hot white dwarfs G191-B2B and RE0503-289

T. Rauch, S. Gamrath, P. Quinet +5

For the spectral analysis of high-resolution and high-signal-to-noise spectra of hot stars, state-of-the-art non-local thermodynamic equilibrium (NLTE) model atmospheres are mandat…

astro-ph.SR2016★ 26 cited

Stellar laboratories. VII. New Kr IV - VII oscillator strengths and an improved spectral analysis of the hot, hydrogen-deficient DO-type white dwarf RE0503-289

T. Rauch, P. Quinet, D. Hoyer +4

For the spectral analysis of high-resolution and high-signal-to-noise (S/N) spectra of hot stars, state-of-the-art non-local thermodynamic equilibrium (NLTE) model atmospheres are…

astro-ph.SR2015★ 33 cited

Stellar laboratories. VI. New Mo IV - VII oscillator strengths and the molybdenum abundance in the hot white dwarfs G191-B2B and RE0503-289

T. Rauch, P. Quinet, D. Hoyer +3

For the spectral analysis of high-resolution and high-signal-to-noise (S/N) spectra of hot stars, state-of-the-art non-local thermodynamic equilibrium (NLTE) model atmospheres are…