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20032015
most citedAsteroseismology of the Beta Cephei star 12 (DD) Lacertae: photometric observations, pulsational frequency analysis and mode identification

100 citations · 227 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2015★ 10 cited

The 2003-4 multisite photometric campaign for the Beta Cephei and eclipsing star 16 (EN) Lacertae with an Appendix on 2 Andromedae, the variable comparison star

M. Jerzykiewicz, G. Handler, J. Daszynska-Daszkiewicz +26

A multisite photometric campaign for the Beta Cephei and eclipsing variable 16 Lacertae is reported. 749 h of high-quality differential photoelectric Stromgren, Johnson and Geneva…

astro-ph.SR2010★ 12 cited

Whole Earth Telescope Observations of the subdwarf B star KPD 1930+2752: A rich, short period pulsator in a close binary

M. D. Reed, S. L. Harms, S. Poindexter +58

KPD 1930+2752 is a short-period pulsating subdwarf B (sdB) star. It is also an ellipsoidal variable with a known binary period just over two hours. The companion is most likely a w…

astro-ph2005★ 100 cited

Asteroseismology of the Beta Cephei star 12 (DD) Lacertae: photometric observations, pulsational frequency analysis and mode identification

G. Handler, M. Jerzykiewicz, E. Rodriguez +28

We report a multisite photometric campaign for the Beta Cephei star 12 Lacertae. 750 hours of high-quality differential photoelectric Stromgren, Johnson and Geneva time-series phot…

astro-ph2005★ 99 cited

Asteroseismology of the Beta Cephei star Nu Eridani: photometric observations and pulsational frequency analysis

G. Handler, R. R. Shobbrook, M. Jerzykiewicz +19

We undertook a multisite photometric campaign for the Beta Cephei star Nu Eridani. More than 600 hours of differential photoelectric uvyV photometry were obtained with 11 telescope…

astro-ph2003★ 6 cited

2MASSJ0516288+260738: Discovery of the first eclipsing late K + Brown dwarf system?

S. L. Schuh, G. Handler, H. Drechsel +22

We report the discovery of a new eclipsing system less than one arcminute south of the pulsating DB white dwarf KUV 05134+2605. The object could be identified with the point source…