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19982026
most citedA new extensive library of PHOENIX stellar atmospheres and synthetic spectra

2k citations · 15k across the 240 of their papers we have counts for

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astro-ph2006

Observational constraints on the evolutionary connection between PG 1159 stars and DO white dwarfs

S. D. Huegelmeyer, S. Dreizler, K. Werner +3

The Sloan Digital Sky Survey has provided spectra of a large number of new PG 1159 stars and DO white dwarfs. This increase in known hot H-deficient compact objects significantly i…

astro-ph2006

Spectral analyses of 16 DAO white dwarfs from the Sloan Digital Sky Survey

S. D. Huegelmeyer, S. Dreizler, T. Rauch +1

We present a spectral analysis of 16 DAO white dwarfs from the Sloan Digital Sky Survey Data Release 4. With our NLTE H+He model grid, we derived photospheric parameters for these…

astro-ph2006★ 142 cited

Hot subdwarfs from the ESO Supernova Ia Progenitor Survey: II. Atmospheric parameters of subdwarf O stars

A. Stroeer, U. Heber, T. Lisker +4

We address the origin and evolutionary status of hot subdwarf stars by studying the optical spectral properties of 58 subdwarf O (sdO) stars. Combining them with the results of our…

astro-ph2006★ 15 cited

Probing unexplored territories with MUSE: a second generation instrument for the VLT

R. Bacon, S. Bauer, P. Boehm +57

The Multi Unit Spectroscopic Explorer (MUSE) is a second-generation VLT panoramic integral-field spectrograph under preliminary design study. MUSE has a field of 1x1 arcmin**2 samp…

astro-ph2006★ 45 cited

Spectral analyses of eighteen hot H-deficient (pre-) white dwarfs from the Sloan Digital Sky Survey Data Release 4

S. D. Huegelmeyer, S. Dreizler, D. Homeier +4

Context: The Sloan Digital Sky Survey Data Release 4 has provided spectra of several new PG 1159 stars and DO white dwarfs. This increase in known hot H-deficient compact objects s…

astro-ph2006★ 24 cited

SDSSJ212531.92-010745.9 - the first definite PG1159 close binary system

T. Nagel, S. Schuh, D. -J. Kusterer +5

The archival spectrum of SDSSJ212531.92-010745.9 shows not only the typical signature of a PG1159 star, but also indicates the presence of a companion. Our aim was the proof of the…