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19992008
most citedZeeman tomography of magnetic white dwarfs, I. Reconstruction of the field geometry from synthetic spectra

39 citations · 45 across the 3 of their papers we have counts for

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astro-ph20086 cited

Inferring statistics of planet populations by means of automated microlensing searches

M. Dominik, U. G. Jorgensen, K. Horne +17

(abridged) The study of other worlds is key to understanding our own, and not only provides clues to the origin of our civilization, but also looks into its future. Rather than in…

astro-ph20066 cited

Optimising Optimal Image Subtraction

Holger Israel, Frederic V. Hessman, Sonja Schuh

Difference imaging is a technique for obtaining precise relative photometry of variable sources in crowded stellar fields and, as such, constitutes a crucial part of the data reduc…

astro-ph2003

Zeeman tomography of magnetic white dwarfs: General method and application to EF Eridani

F. Euchner, K. Beuermann, K. Reinsch +3

We have developed a new method to derive the magnetic field distribution on the surfaces of rotating magnetic white dwarfs from phase-resolved flux and circular polarization spectr…

astro-ph2002

GRB 021004: a Massive Progenitor Star Surrounded by Shells

Bradley E. Schaefer, C. L. Gerardy, P. Hoflich +13

We present spectra of the optical transient of GRB021004 obtained with the Hobby-Eberly telescope starting 15.48, 20.31 hours, and 4.84 days after the burst and a spectrum obtained…

astro-ph200239 cited

Zeeman tomography of magnetic white dwarfs, I. Reconstruction of the field geometry from synthetic spectra

F. Euchner, S. Jordan, K. Beuermann +2

We have computed optical Zeeman spectra of magnetic white dwarfs for field strengths between 10 and 200MG and effective temperatures between 8000 and 40000K. They form a database c…

astro-ph2000

The response of a dwarf nova disc to real mass transfer variations

M. R. Schreiber, B. T. Gaensicke, F. V. Hessman

We present simulations of dwarf nova outbursts taking into account realistic variations of the mass loss rate from the secondary. The mass transfer variation has been derived from…